WorldWideScience

Sample records for survey mesur pathfinder

  1. CRED REA Fish Team Stationary Point Count Surveys at Pathfinder Reef, Marianas Archipelago, 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Stationary Point Counts at 4 stations at each survey site were surveyed as part of Rapid Ecological Assessments (REA) conducted at 2 sites around Pathfinder Reef in...

  2. CRED REA Fish Team Belt Transect Survey at Pathfinder Reef, Marianas Archipelago, 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Belt transects along 3 consecutively-placed, 25m transect lines were surveyed as part of Rapid Ecological Assessments conducted at 2 sites at Pathfinder Reef in the...

  3. The Joint Milli-Arcsecond Pathfinder Survey (JMAPS): Mission Overview and Attitude Sensing Applications

    CERN Document Server

    Dorland, Bryan N; Dugan, Zachary; nessy, Gregory S Hen-

    2009-01-01

    The Joint Milliarcsecond Pathfinder Survey (JMAPS) is a Department of Navy bright star astrometric all-sky survey scheduled for launch in the 2012 timeframe. Mission objectives include a complete update of star positions for the 2015 epoch to accuracy levels of 1 milliarcsecond (5 nano-radians) for bright stars, as well as demonstration of 10 milliarcsecond attitude determination capability and 50 milli-arcsecond attitude control on-orbit. In the following paper, we describe the general instrument design and expected performance. We also discuss the new mission capabilities enabled by the unprecedented attitude determination accuracy of such an instrument, and focus specifically on the application to long distance (50,000-100,00 km) formation flying and solar system navigation.

  4. The JCMT 12CO(3-2) Survey of the Cygnus X Region: I. A Pathfinder

    CERN Document Server

    Gottschalk, M; Matthews, H E; Landecker, T L; Dent, W R F

    2012-01-01

    Cygnus X is one of the most complex areas in the sky. This complicates interpretation, but also creates the opportunity to investigate accretion into molecular clouds and many subsequent stages of star formation, all within one small field of view. Understanding large complexes like Cygnus X is the key to understanding the dominant role that massive star complexes play in galaxies across the Universe. The main goal of this study is to establish feasibility of a high-resolution CO survey of the entire Cygnus X region by observing part of it as a Pathfinder, and to evaluate the survey as a tool for investigating the star-formation process. A 2x4 degree area of the Cygnus X region has been mapped in the 12CO(3-2) line at an angular resolution of 15" and a velocity resolution of ~0.4km/s using HARP-B and ACSIS on the James Clerk Maxwell Telescope. The star formation process is heavily connected to the life-cycle of the molecular material in the interstellar medium. The high critical density of the 12CO(3-2) trans...

  5. Oral health related behaviors among adult Tanzanians: a national pathfinder survey

    Directory of Open Access Journals (Sweden)

    Senkoro Ahadieli R

    2009-09-01

    Full Text Available Abstract Background The oral health education programs which have been organised and delivered in Tanzania were not based on a thorough understanding of behaviours which influence oral health. Therefore, evaluation of these programs became difficult. This study aimed at investigating the oral health related behaviours and their determinants among Tanzanian adults. Methods A national pathfinder cross sectional survey was conducted in 2006 involving 1759 respondents from the six geographic zones of mainland Tanzania. Frequency distributions, Chi square and multiple logistic regression analyses were performed using SPSS version 13.0. Results The rates of abstinence from alcohol for the past 30 days and life time smoking were 61.6% and 16.7% respectively, with males being more likely to smoke (OR 9.2, CI 6.3 -12.9, p Conclusion The findings of this study demonstrated social demographic disparities in relation to oral health related behaviors, while dental pain was associated with low consumption of sugar and high likelihood to take alcohol.

  6. CRED Towed-Diver Fish Biomass Surveys at Pathfinder Bank, Marianas Archipelago in 2003

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Towed-diver surveys (aka. Towboard surveys) are conducted by the Coral Reef Ecosystem Division (CRED) of the NOAA Pacific Islands Fisheries Science Center (PIFSC)...

  7. Pathfinder Program

    Science.gov (United States)

    London, John R., III; Rogacki, Row (Technical Monitor)

    2000-01-01

    The topics in this viewgraph include: 1) High visibility Flight Projects; 2) Pathfinder Flight Experiments; 3) X-37 Configuration Modification Options; 4) Flight Testing for a Multistage Reusable System; 5) X-34 Vehicle Description; 6) X-34 Expanded View; 7) Vehicle Size Comparison; 8) X-34 Experiment Status; 9) Government Participation; 10) Government and Industry Participants; 11) X-34 Project Status; 12) X-34 Captive Carry Fight; 13) Little Joe III; 14) Fastpac; and 15) Islunar Tug.

  8. CRED Towed-Diver Benthic Characterization Surveys at Pathfinder Bank, Marianas Archipelago in 2003

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — To support NOAA Coral Reef Conservation Program (CRCP) long-term goals for sustainable management and conservation of coral reef ecosystems, towed-diver surveys...

  9. CRED Towed-Diver Benthic Characterization Surveys at Pathfinder Bank, Marianas Archipelago in 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — To support NOAA Coral Reef Conservation Program (CRCP) long-term goals for sustainable management and conservation of coral reef ecosystems, towed-diver surveys...

  10. School libraries Pathfinders

    Directory of Open Access Journals (Sweden)

    Shideh Taleban

    2009-01-01

    Full Text Available School library represents one of the important locations suited for offering reference services. The skill set necessary in order to use information resources, is called information literacy. When discussing information literacy and means of enhancing it, the first thing that comes to mind is the classroom for it is in schools that the foundation for learning skills is laid. Pathfinders have been used by libraries and librarians for guiding patrons to the required sources and answering their research questions since 1970’s. It is far different from a bibliography in as much as it does not necessarily include a complete list of available resources on a given topic. Nevertheless it provides sufficient basic resources for research for the patrons. Nowadays pathfinders are prepared by teacher-librarian or with the help of teachers at school so as to assist students in searching their prescribed assignments. The present paper offers definition of pathfinder, creation of pathfinders in schools, type of pathfinders, pathfinders characteristics, pathfinder elements as well as how to design pathfinders for children and teenagers.

  11. La mesure du danger

    CERN Document Server

    Manceron, Vanessa; Revet, Sandrine

    2014-01-01

    La mesure du danger permet d’explorer des dangers de nature aussi diverse que la délinquance, la pollution, l’écueil maritime, la maladie ou l’attaque sorcellaire, l’extinction d’espèces animales ou végétales, voire de la Planète tout entière. Au croisement de la sociologie, de l’anthropologie et de l’histoire, les différents articles analysent les pratiques concrètes de mesure pour tenter de comprendre ce qui se produit au cours de l’opération d’évaluation du danger sans préjuger de la nature de celui-ci. L’anthropologie a contribué à la réflexion sur l’infortune en s’intéressant aux temporalités de l’après : maladies, catastrophes, pandémies, etc. et en cherchant à rendre compte de l’expérience des victimes, de leur vie ordinaire bouleversée, de la recomposition du quotidien. Elle s’intéresse aussi aux autres types de mesures, les savoirs incorporés, qui reposent sur l’odorat, la vue ou le toucher et ceux qui ressortent d’une épistémologie « non ...

  12. The LISA Pathfinder mission

    Science.gov (United States)

    Antonucci, F.; Armano, M.; Audley, H.; Auger, G.; Benedetti, M.; Binetruy, P.; Bogenstahl, J.; Bortoluzzi, D.; Bosetti, P.; Brandt, N.; Caleno, M.; Cañizares, P.; Cavalleri, A.; Cesa, M.; Chmeissani, M.; Conchillo, A.; Congedo, G.; Cristofolini, I.; Cruise, M.; Danzmann, K.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Dunbar, N.; Fauste, J.; Ferraioli, L.; Ferrone, V.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marin, A.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gilbert, F.; Giardini, D.; Grimani, C.; Grynagier, A.; Guillaume, B.; Guzmán, F.; Harrison, I.; Heinzel, G.; Hernández, V.; Hewitson, M.; Hollington, D.; Hough, J.; Hoyland, D.; Hueller, M.; Huesler, J.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mitchell, E.; Monsky, A.; Nicolini, D.; Nicolodi, D.; Nofrarias, M.; Pedersen, F.; Perreur-Lloyd, M.; Plagnol, E.; Prat, P.; Racca, G. D.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Sanjuan, J.; Schleicher, A.; Schulte, M.; Shaul, D.; Stagnaro, L.; Strandmoe, S.; Steier, F.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tu, H.-B.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Weber, W. J.; Ziegler, T.; Zweifel, P.

    2012-06-01

    In this paper, we describe the current status of the LISA Pathfinder mission, a precursor mission aimed at demonstrating key technologies for future space-based gravitational wave detectors, like LISA. Since much of the flight hardware has already been constructed and tested, we will show that performance measurements and analysis of these flight components lead to an expected performance of the LISA Pathfinder which is a significant improvement over the mission requirements, and which actually reaches the LISA requirements over the entire LISA Pathfinder measurement band.

  13. Pathfinder Innovation Projects

    Science.gov (United States)

    The Pathfinder program supports high-risk, high-reward research ideas with funding and staff time. The goal is to feed a culture of innovation in the Agency and integrate innovative ideas in EPA research programs.

  14. Pathfinder Climate Data

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The NOAA/NASA Pathfinder climate data CD-ROM contains seven data sets: Advanced Very High Resolution Radiometer (AVHRR)Land and Ocean, TIROS Operational Vertical...

  15. UKIRT microlensing surveys as a pathfinder for $WFIRST$: The detection of five highly extinguished low-$|b|$ events

    CERN Document Server

    Shvartzvald, Y; Gould, A; Henderson, C B; Howell, S B; Beichman, C

    2016-01-01

    Optical microlensing surveys are restricted from detecting events near the Galactic plane and center, where the event rate is thought to be the highest, due to the high optical extinction of these fields. In the near-infrared (NIR), however, the lower extinction leads to a corresponding increase in event detections and is a primary driver for the wavelength coverage of the $WFIRST$ microlensing survey. During the 2015 and 2016 bulge observing seasons we conducted NIR microlensing surveys with UKIRT in conjunction with and in support of the $Spitzer$ and $Kepler$ microlensing campaigns. Here we report on five highly extinguished ($A_H=0.81-1.97$), low-Galactic latitude ($-0.98\\le b\\le -0.36$) microlensing events discovered from our 2016 survey. Four of them were monitored with an hourly cadence by optical surveys but were not reported as discoveries, likely due to the high extinction. Our UKIRT surveys and suggested future NIR surveys enable the first measurement of the microlensing event rate in the NIR. This...

  16. The LISA Pathfinder Mission

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; Gallegos, J.; García Marirrodriga, C.; Gerndt, R.; Gesa, L. I.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martín, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mendes, L.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vetrugno, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    LISA Pathfinder (LPF), the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology validation mission for future spaceborne gravitational wave detectors, such as the proposed eLISA mission. LISA Pathfinder, and its scientific payload - the LISA Technology Package - will test, in flight, the critical technologies required for low frequency gravitational wave detection: it will put two test masses in a near-perfect gravitational free-fall and control and measure their motion with unprecedented accuracy. This is achieved through technology comprising inertial sensors, high precision laser metrology, drag-free control and an ultra-precise micro-Newton propulsion system. LISA Pathfinder is due to be launched in mid-2015, with first results on the performance of the system being available 6 months thereafter. The paper introduces the LISA Pathfinder mission, followed by an explanation of the physical principles of measurement concept and associated hardware. We then provide a detailed discussion of the LISA Technology Package, including both the inertial sensor and interferometric readout. As we approach the launch of the LISA Pathfinder, the focus of the development is shifting towards the science operations and data analysis - this is described in the final section of the paper

  17. JWST Pathfinder Telescope Integration

    Science.gov (United States)

    Matthews, Gary W.; Kennard, Scott H.; Broccolo, Ronald T.; Ellis, James M.; Daly, Elizabeth A.; Hahn, Walter G.; Amon, John N.; Mt. Pleasant, Stephen M.; Texter, Scott; Atkinson, Charles B.; McKay, Andrew; Levi, Joshua; Keski-Kuha, Ritva; Feinberg, Lee

    2015-01-01

    The James Webb Space Telescope (JWST) is a 6.5m, segmented, IR telescope that will explore the first light of the universe after the big bang. In 2014, a major risk reduction effort related to the Alignment, Integration, and Test (AI&T) of the segmented telescope was completed. The Pathfinder telescope includes two Primary Mirror Segment Assemblies (PMSA's) and the Secondary Mirror Assembly (SMA) onto a flight-like composite telescope backplane. This pathfinder allowed the JWST team to assess the alignment process and to better understand the various error sources that need to be accommodated in the flight build. The successful completion of the Pathfinder Telescope provides a final integration roadmap for the flight operations that will start in August 2015.

  18. Pilot pathfinder survey of oral hygiene and periodontal conditions in the rural population of The Gambia (West Africa).

    Science.gov (United States)

    Jordan, R A; Lucaciu, A; Fotouhi, K; Markovic, L; Gaengler, P; Zimmer, S

    2011-02-01

    To document oral hygiene and periodontal conditions in the rural population of The Gambia. Cross-sectional study according to the recommendations of the WHO for oral health surveys. Examination by two calibrated investigators in the health centres of rural communities after a public radio call. Patients were randomly allocated to the investigators.   162 patients (20-54 years old; 52.5% female, 47.5% male). Patients were interviewed for personal information and examined in a full-mouth recording. Oral Hygiene Index (OHI), Gingival Index (GI), Community Periodontal Index (CPI), and the Gingivitis-Periodontitis-Missing/Teeth Index (GPM/T). Statistical analysis was performed using the Wilcoxon-rank-sum test and Kruskal-Wallis test with statistical significance at P Africa). © 2009 John Wiley & Sons A/S.

  19. Instruments de mesure en acoustique

    DEFF Research Database (Denmark)

    Tarnov, Viggo; Jacobsen, Finn

    2008-01-01

    La mesure en acoustique fait appel à des instruments qui mesurent, d'une part la pression, d'autre part l'intensité du signal. Ce dossier présentera, notamment, deux appareils spécialisés : les sonomètres et les microphones. Il abordera l'ensemble des informations majeures à connaître sur les...

  20. The LISA Pathfinder Mission

    Science.gov (United States)

    McNamara, Paul

    2013-04-01

    LISA Pathfinder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology validation mission for future interferometric spaceborne gravitational wave observatories, for example the proposed eLISA mission. The technologies required for eLISA are many and extremely challenging. This coupled with the fact that some flight hardware cannot be fully tested on ground due to Earth-induced noise, led to the implementation of the LISA Pathfinder mission to test the critical eLISA technologies in a flight environment. LISA Pathfinder essentially mimics one arm of the eLISA constellation by shrinking the 1 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology: the distance between the two test masses is measured using a laser interferometric technique similar to one aspect of the eLISA interferometry system. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. Here I will present an overview of the mission, focusing on scientific and technical goals, followed by the current status of the project.

  1. VR for Mars Pathfinder

    Science.gov (United States)

    Blackmon, Theodore

    1998-01-01

    Virtual reality (VR) technology has played an integral role for Mars Pathfinder mission, operations Using an automated machine vision algorithm, the 3d topography of the Martian surface was rapidly recovered fro -a the stereo images captured. by the Tender camera to produce photo-realistic 3d models, An advanced, interface was developed for visualization and interaction with. the virtual environment of the Pathfinder landing site for mission scientists at the Space Flight Operations Facility of the Jet Propulsion Laboratory. The VR aspect of the display allowed mission scientists to navigate on Mars in Bud while remaining here on Earth, thus improving their spatial awareness of the rock field that surrounds the lenders Measurements of positions, distances and angles could be easily extracted from the topographic models, providing valuable information for science analysis and mission. planning. Moreover, the VR map of Mars has also been used to assist with the archiving and planning of activities for the Sojourner rover.

  2. The Mars Pathfinder Mission

    Science.gov (United States)

    Golombek, M. P.

    1996-09-01

    The Mars Pathfinder mission is a Discovery class mission that will place a small lander and rover on the surface of Mars on July 4, 1997. The Pathfinder flight system is a single small lander, packaged within an aeroshell and back cover with a back-pack-style cruise stage. The vehicle will be launched, fly independently to Mars, and enter the atmosphere directly on approach behind the aeroshell. The vehicle is slowed by a parachute and 3 small solid rockets before landing on inflated airbags. Petals of a small tetrahedron shaped lander open up, to right the vehicle. The lander is solar powered with batteries and will operate on the surface for up to a year, downlinking data on a high-gain antenna. Pathfinder will be the first mission to use a rover, with 3 imagers and an alpha proton X-ray spectrometer, to characterize the rocks and soils in a landing area over hundreds of square meters on Mars, which will provide a calibration point or "ground truth" for orbital remote sensing observations. The rover (includes a series of technology experiments), the instruments (including a stereo multispectral surface imager on a pop up mast and an atmospheric structure instrument-surface meteorology package) and the telemetry system will allow investigations of: the surface morphology and geology at meter scale, the petrology and geochemistry of rocks and soils, the magnetic properties of dust, soil mechanics and properties, a variety of atmospheric investigations and the rotational and orbital dynamics of Mars. Landing downstream from the mouth of a giant catastrophic outflow channel, Ares Vallis, offers the potential of identifying and analyzing a wide variety of crustal materials, from the ancient heavily cratered terrain, intermediate-aged ridged plains and reworked channel deposits, thus allowing first-order scientific investigations of the early differentiation and evolution of the crust, the development of weathering products and early environments and conditions on Mars.

  3. Pathfinder - flight preparation on lakebed

    Science.gov (United States)

    1995-01-01

    AeroVironment, Inc., crew members prepare the Pathfinder solar-powered aircraft for its first flight on Rogers Dry Lake at NASA's Dryden Flight Research Center, Edwards, California, after its configuration was shanged from 8 electric motors to 6. Bob Curtin of AeroVironment is in the foreground of the photo. Pathfinder was a lightweight, solar-powered, remotely piloted flying wing aircraft used to demonstrate the use of solar power for long-duration, high-altitude flight. Its name denotes its mission as the 'Pathfinder' or first in a series of solar-powered aircraft that will be able to remain airborne for weeks or months on scientific sampling and imaging missions. Solar arrays covered most of the upper wing surface of the Pathfinder aircraft. These arrays provided up to 8,000 watts of power at high noon on a clear summer day. That power fed the aircraft's six electric motors as well as its avionics, communications, and other electrical systems. Pathfinder also had a backup battery system that could provide power for two to five hours, allowing for limited-duration flight after dark. Pathfinder flew at airspeeds of only 15 to 20 mph. Pitch control was maintained by using tiny elevators on the trailing edge of the wing while turns and yaw control were accomplished by slowing down or speeding up the motors on the outboard sections of the wing. On September 11, 1995, Pathfinder set a new altitude record for solar-powered aircraft of 50,567 feet above Edwards Air Force Base, California, on a 12-hour flight. On July 7, 1997, it set another, unofficial record of 71,500 feet at the Pacific Missile Range Facility, Kauai, Hawaii. In 1998, Pathfinder was modified into the longer-winged Pathfinder Plus configuration. (See the Pathfinder Plus photos and project description.)

  4. LISA Pathfinder: mission and status

    Science.gov (United States)

    Antonucci, F.; Armano, M.; Audley, H.; Auger, G.; Benedetti, M.; Binetruy, P.; Boatella, C.; Bogenstahl, J.; Bortoluzzi, D.; Bosetti, P.; Caleno, M.; Cavalleri, A.; Cesa, M.; Chmeissani, M.; Ciani, G.; Conchillo, A.; Congedo, G.; Cristofolini, I.; Cruise, M.; Danzmann, K.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Dunbar, N.; Fauste, J.; Ferraioli, L.; Fertin, D.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marin, A.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gilbert, F.; Giardini, D.; Grimani, C.; Grynagier, A.; Guillaume, B.; Guzmán, F.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hough, J.; Hoyland, D.; Hueller, M.; Huesler, J.; Jeannin, O.; Jennrich, O.; Jetzer, P.; Johlander, B.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mitchell, E.; Monsky, A.; Nicolini, D.; Nicolodi, D.; Nofrarias, M.; Pedersen, F.; Perreur-Lloyd, M.; Perreca, A.; Plagnol, E.; Prat, P.; Racca, G. D.; Rais, B.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Sanjuan, J.; Schleicher, A.; Schulte, M.; Shaul, D.; Stagnaro, L.; Strandmoe, S.; Steier, F.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tombolato, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Weber, W. J.; Zweifel, P.

    2011-05-01

    LISA Pathfinder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology demonstrator for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission. The technologies required for LISA are many and extremely challenging. This coupled with the fact that some flight hardware cannot be fully tested on ground due to Earth-induced noise led to the implementation of the LISA Pathfinder mission to test the critical LISA technologies in a flight environment. LISA Pathfinder essentially mimics one arm of the LISA constellation by shrinking the 5 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology: the distance between the two test masses is measured using a laser interferometric technique similar to one aspect of the LISA interferometry system. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. LISA Pathfinder is due to be launched in 2013 on-board a dedicated small launch vehicle (VEGA). After a series of apogee raising manoeuvres using an expendable propulsion module, LISA Pathfinder will enter a transfer orbit towards the first Sun-Earth Lagrange point (L1). After separation from the propulsion module, the LPF spacecraft will be stabilized using the micro-Newton thrusters, entering a 500 000 km by 800 000 km Lissajous orbit around L1. Science results will be available approximately 2 months after launch.

  5. LISA Pathfinder data analysis

    Science.gov (United States)

    Antonucci, F.; Armano, M.; Audley, H.; Auger, G.; Benedetti, M.; Binetruy, P.; Boatella, C.; Bogenstahl, J.; Bortoluzzi, D.; Bosetti, P.; Caleno, M.; Cavalleri, A.; Cesa, M.; Chmeissani, M.; Ciani, G.; Conchillo, A.; Congedo, G.; Cristofolini, I.; Cruise, M.; Danzmann, K.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Fauste, J.; Ferraioli, L.; Fertin, D.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marin, A.; García Marirrodriga, C.; Gesa, L.; Giardini, D.; Grimani, C.; Grynagier, A.; Guillaume, B.; Guzmán, F.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hough, J.; Hoyland, D.; Hueller, M.; Huesler, J.; Jeannin, O.; Jennrich, O.; Jetzer, P.; Johlander, B.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mitchell, E.; Monsky, A.; Nicolini, D.; Nicolodi, D.; Nofrarias, M.; Pedersen, F.; Perreur-Lloyd, M.; Perreca, A.; Plagnol, E.; Prat, P.; Racca, G. D.; Rais, B.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Sanjuan, J.; Schulte, M.; Shaul, D.; Stagnaro, L.; Strandmoe, S.; Steier, F.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tombolato, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Weber, W. J.; Zweifel, P.

    2011-05-01

    As the launch of LISA Pathfinder (LPF) draws near, more and more effort is being put in to the preparation of the data analysis activities that will be carried out during the mission operations. The operations phase of the mission will be composed of a series of experiments that will be carried out on the satellite. These experiments will be directed and analysed by the data analysis team, which is part of the operations team. The operations phase will last about 90 days, during which time the data analysis team aims to fully characterize the LPF, and in particular, its core instrument the LISA Technology Package. By analysing the various couplings present in the system, the different noise sources that will disturb the system, and through the identification of the key physical parameters of the system, a detailed noise budget of the instrument will be constructed that will allow the performance of the different subsystems to be assessed and projected towards LISA. This paper describes the various aspects of the full data analysis chain that are needed to successfully characterize the LPF and build up the noise budget during mission operations.

  6. LISA Pathfinder data analysis

    Energy Technology Data Exchange (ETDEWEB)

    Antonucci, F; Cavalleri, A; Congedo, G [Dipartimento di Fisica, Universita di Trento and INFN, Gruppo Collegato di Trento, 38123 Povo, Trento (Italy); Armano, M [European Space Astronomy Centre, European Space Agency, Villanueva de la Canada, 28692 Madrid (Spain); Audley, H; Bogenstahl, J; Danzmann, K [Albert-Einstein-Institut, Max-Planck-Institut fuer Gravitationsphysik und Universitaet Hannover, 30167 Hannover (Germany); Auger, G; Binetruy, P [APC UMR7164, Universite Paris Diderot, Paris (France); Benedetti, M [Dipartimento di Ingegneria dei Materiali e Tecnologie Industriali, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Boatella, C [CNES, DCT/AQ/EC, 18 Avenue Edouard Belin, 31401 Toulouse, Cedex9 (France); Bortoluzzi, D; Bosetti, P; Cristofolini, I [Dipartimento di Ingegneria Meccanica e Strutturale, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Caleno, M; Cesa, M [European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk (Netherlands); Chmeissani, M [IFAE, Universitat Autonoma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Ciani, G [Department of Physics, University of Florida, Gainesville, FL 32611-8440 (United States); Conchillo, A [ICE-CSIC/IEEC, Facultat de Ciencies, E-08193 Bellaterra (Barcelona) (Spain); Cruise, M, E-mail: martin.hewitson@aei.mpg.de [Department of Physics and Astronomy, University of Birmingham, Birmingham (United Kingdom)

    2011-05-07

    As the launch of LISA Pathfinder (LPF) draws near, more and more effort is being put in to the preparation of the data analysis activities that will be carried out during the mission operations. The operations phase of the mission will be composed of a series of experiments that will be carried out on the satellite. These experiments will be directed and analysed by the data analysis team, which is part of the operations team. The operations phase will last about 90 days, during which time the data analysis team aims to fully characterize the LPF, and in particular, its core instrument the LISA Technology Package. By analysing the various couplings present in the system, the different noise sources that will disturb the system, and through the identification of the key physical parameters of the system, a detailed noise budget of the instrument will be constructed that will allow the performance of the different subsystems to be assessed and projected towards LISA. This paper describes the various aspects of the full data analysis chain that are needed to successfully characterize the LPF and build up the noise budget during mission operations.

  7. Holographic Beam Mapping of the CHIME Pathfinder Array

    CERN Document Server

    Berger, Philippe; Amiri, Mandana; Bandura, Kevin; Cliche, Jean-Francois; Connor, Liam; Deng, Meiling; Denman, Nolan; Dobbs, Matt; Fandino, Mateus; Gilbert, Adam J; Good, Deborah; Halpern, Mark; Hanna, David; Hincks, Adam D; Hinshaw, Gary; Hofer, Carolin; Johnson, Andre M; Landecker, Tom L; Masui, Kiyoshi W; Parra, Juan Mena; Oppermann, Niels; Pen, Ue-Li; Peterson, Jeffrey B; Recnik, Andre; Robishaw, Timothy; Shaw, J Richard; Siegel, Seth; Sigurdson, Kris; Smith, Kendrick; Storer, Emilie; Tretyakov, Ian; Van Gassen, Kwinten; Vanderlinde, Keith; Wiebe, Donald

    2016-01-01

    The Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder radio telescope is currently surveying the northern hemisphere between 400 and 800 MHz. By mapping the large scale structure of neutral hydrogen through its redshifted 21 cm line emission between $z \\sim 0.8-2.5$ CHIME will contribute to our understanding of Dark Energy. Bright astrophysical foregrounds must be separated from the neutral hydrogen signal, a task which requires precise characterization of the polarized telescope beams. Using the DRAO John A. Galt 26 m telescope, we have developed a holography instrument and technique for mapping the CHIME Pathfinder beams. We report the status of the instrument and initial results of this effort.

  8. The LISA Pathfinder Radiation Monitor

    Science.gov (United States)

    Wass, P. J.; Araújo, H.; Boatella, C.; Chmeissani, M.; Hajdas, W.; Lobo, A.; Puigdengoles, C.; Sumner, T.

    2006-11-01

    We present the concept, design and testing of the radiation monitor for LISA Pathfinder. Galactic cosmic rays (GCRs) and solar energetic particles (SEPs) will cause charging of the LISA Pathfinder test masses producing unwanted disturbances which could be significant during a large solar eruption. A radiation monitor on board LISA Pathfinder, using silicon PIN diodes as particle detectors, will measure the particle flux responsible for charging. It will also be able to record spectral information to identify solar energetic particle events. The design of the monitor was supported by Monte Carlo simulations which allow detailed predictions of the radiation monitor performance. We present these predictions as well as the results of high-energy proton tests carried out at the Paul Scherrer Institute, Switzerland. The tests show good agreement with our simulations and confirm the capability of the radiation monitor to perform well in the space environment, meeting all science requirements.

  9. LISA Pathfinder: mission and status

    Energy Technology Data Exchange (ETDEWEB)

    Antonucci, F; Cavalleri, A; Congedo, G [Dipartimento di Fisica, Universita di Trento and INFN, Gruppo Collegato di Trento, 38050 Povo, Trento (Italy); Armano, M [European Space Astronomy Centre, European Space Agency, Villanueva de la Canada, 28692 Madrid (Spain); Audley, H; Bogenstahl, J; Danzmann, K [Albert-Einstein-Institut, Max-Planck-Institut fuer Gravitationsphysik und Universitaet Hannover, 30167 Hannover (Germany); Auger, G; Binetruy, P [APC UMR7164, Universite Paris Diderot, Paris (France); Benedetti, M [Dipartimento di Ingegneria dei Materiali e Tecnologie Industriali, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Boatella, C [CNES, DCT/AQ/EC, 18 Avenue Edouard Belin, 31401 Toulouse, Cedex 9 (France); Bortoluzzi, D; Bosetti, P; Cristofolini, I [Dipartimento di Ingegneria Meccanica e Strutturale, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Caleno, M; Cesa, M [European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk (Netherlands); Chmeissani, M [IFAE, Universitat Autonoma de Barcelona, E-08193 Bellaterra, Barcelona (Spain); Ciani, G [Department of Physics, University of Florida, Gainesville, FL 32611-8440 (United States); Conchillo, A [ICE-CSIC/IEEC, Facultat de Ciencies, E-08193 Bellaterra, Barcelona (Spain); Cruise, M, E-mail: Paul.McNamara@esa.int [Department of Physics and Astronomy, University of Birmingham, Birmingham (United Kingdom)

    2011-05-07

    LISA Pathfinder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology demonstrator for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission. The technologies required for LISA are many and extremely challenging. This coupled with the fact that some flight hardware cannot be fully tested on ground due to Earth-induced noise led to the implementation of the LISA Pathfinder mission to test the critical LISA technologies in a flight environment. LISA Pathfinder essentially mimics one arm of the LISA constellation by shrinking the 5 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology: the distance between the two test masses is measured using a laser interferometric technique similar to one aspect of the LISA interferometry system. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. LISA Pathfinder is due to be launched in 2013 on-board a dedicated small launch vehicle (VEGA). After a series of apogee raising manoeuvres using an expendable propulsion module, LISA Pathfinder will enter a transfer orbit towards the first Sun-Earth Lagrange point (L1). After separation from the propulsion module, the LPF spacecraft will be stabilized using the micro-Newton thrusters, entering a 500 000 km by 800 000 km Lissajous orbit around L1. Science results will be available approximately 2 months after launch.

  10. MESURE DE LA PERFORMANCE GLOBALE DES ENTREPRISES

    OpenAIRE

    Renaud, Angèle; Berland, Nicolas

    2007-01-01

    International audience; L'engagement des entreprises dans le développement durable consiste à conjuguer performance et responsabilité. La performance financière ne suffit plus à apprécier la performance d'une entreprise. Dès lors, les entreprises doivent mesurer leurs progrès à partir d'une performance plus globale incluant, en dehors de la dimension économique, des dimensions sociale et environnementale. A présent, comment mesurer cette performance globale ? Existe-il des outils de mesure gl...

  11. Long Memory of Pathfinding Aesthetics

    Directory of Open Access Journals (Sweden)

    Ron Coleman

    2009-01-01

    Full Text Available This paper investigates a new dynamic (i.e., space-time model to measure aesthetic values in pathfinding for videogames. The results we report are important firstly because the artificial intelligence literature has given relatively little attention to aesthetic considerations in pathfinding. Secondly, those investigators who have studied aesthetics in pathfinding have relied largely on anecdotal arguments rather than metrics. Finally, in those cases where metrics have been used in the past, they show only that aesthetic paths are different. They provide no quantitative means to classify aesthetic outcomes. The model we develop here overcomes these deficiencies using rescaled range (R/S analysis to estimate the Hurst exponent, . It measures long-range dependence (i.e., long memory in stochastic processes and provides a novel well-defined mathematical classification for pathfinding. Indeed, the data indicates that aesthetic and control paths have statistically significantly distinct signatures. Aesthetic paths furthermore have more long memory than controls with an effect size that is large, more than three times that of an alternative approach. These conclusions will be of interest to researchers investigating games as well as other forms of entertainment, simulation, and in general nonshortest path motion planning.

  12. Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder

    CERN Document Server

    Bandura, Kevin; Amiri, Mandana; Bond, J Richard; Campbell-Wilson, Duncan; Connor, Liam; Cliche, Jean-Francois; Davis, Greg; Deng, Meiling; Denman, Nolan; Dobbs, Matt; Fandino, Mateus; Gibbs, Kenneth; Gilbert, Adam; Halpern, Mark; Hanna, David; Hincks, Adam D; Hinshaw, Gary; Hofer, Carolin; Klages, Peter; Landecker, Tom L; Masui, Kiyoshi; Mena, Juan; Newburgh, Laura B; Pen, Ue-Li; Peterson, Jeffrey B; Recnik, Andre; Shaw, J Richard; Sigurdson, Kris; Sitwell, Michael; Smecher, Graeme; Smegal, Rick; Vanderlinde, Keith; Wiebe, Don

    2014-01-01

    A pathfinder version of CHIME (the Canadian Hydrogen Intensity Mapping Experiment) is currently being commissioned at the Dominion Radio Astrophysical Observatory (DRAO) in Penticton, BC. The instrument is a hybrid cylindrical interferometer designed to measure the large scale neutral hydrogen power spectrum across the redshift range 0.8 to 2.5. The power spectrum will be used to measure the baryon acoustic oscillation (BAO) scale across this poorly probed redshift range where dark energy becomes a significant contributor to the evolution of the Universe. The instrument revives the cylinder design in radio astronomy with a wide field survey as a primary goal. Modern low-noise amplifiers and digital processing remove the necessity for the analog beamforming that characterized previous designs. The Pathfinder consists of two cylinders 37\\,m long by 20\\,m wide oriented north-south for a total collecting area of 1,500 square meters. The cylinders are stationary with no moving parts, and form a transit instrument ...

  13. Desert Pathfinder at Work

    Science.gov (United States)

    2005-09-01

    The Atacama Pathfinder Experiment (APEX) project celebrates the inauguration of its outstanding 12-m telescope, located on the 5100m high Chajnantor plateau in the Atacama Desert (Chile). The APEX telescope, designed to work at sub-millimetre wavelengths, in the 0.2 to 1.5 mm range, passed successfully its Science Verification phase in July, and since then is performing regular science observations. This new front-line facility provides access to the "Cold Universe" with unprecedented sensitivity and image quality. After months of careful efforts to set up the telescope to work at the best possible technical level, those involved in the project are looking with satisfaction at the fruit of their labour: APEX is not only fully operational, it has already provided important scientific results. "The superb sensitivity of our detectors together with the excellence of the site allow fantastic observations that would not be possible with any other telescope in the world," said Karl Menten, Director of the group for Millimeter and Sub-Millimeter Astronomy at the Max-Planck-Institute for Radio Astronomy (MPIfR) and Principal Investigator of the APEX project. ESO PR Photo 30/05 ESO PR Photo 30/05 Sub-Millimetre Image of a Stellar Cradle [Preview - JPEG: 400 x 627 pix - 200k] [Normal - JPEG: 800 x 1254 pix - 503k] [Full Res - JPEG: 1539 x 2413 pix - 1.3M] Caption: ESO PR Photo 30/05 is an image of the giant molecular cloud G327 taken with APEX. More than 5000 spectra were taken in the J=3-2 line of the carbon monoxide molecule (CO), one of the best tracers of molecular clouds, in which star formation takes place. The bright peak in the north of the cloud is an evolved star forming region, where the gas is heated by a cluster of new stars. The most interesting region in the image is totally inconspicuous in CO: the G327 hot core, as seen in methanol contours. It is a truly exceptional source, and is one of the richest sources of emission from complex organic molecules in the

  14. A Comprehensive Study on Pathfinding Techniques for Robotics and Video Games

    Directory of Open Access Journals (Sweden)

    Zeyad Abd Algfoor

    2015-01-01

    Full Text Available This survey provides an overview of popular pathfinding algorithms and techniques based on graph generation problems. We focus on recent developments and improvements in existing techniques and examine their impact on robotics and the video games industry. We have categorized pathfinding algorithms based on a 2D/3D environment search. The aim of this paper is to provide researchers with a thorough background on the progress made in the last 10 years in this field, summarize the principal techniques, and describe their results. We also give our expectations for future trends in this field and discuss the possibility of using pathfinding techniques in more extensive areas.

  15. PAPPA: Primordial Anisotropy Polarization Pathfinder Array

    CERN Document Server

    Kogut, A; Fixsen, D; Hinshaw, G F; Limon, M; Moseley, S H; Phillips, N; Sharp, E; Wollack, E J; U-Yen, K; Cao, N; Stevenson, T; Hsieh, W; Devlin, M; Dicker, S; Semisch, C; Irwin, K

    2006-01-01

    The Primordial Anisotropy Polarization Pathfinder Array (PAPPA) is a balloon-based instrument to measure the polarization of the cosmic microwave background and search for the signal from gravity waves excited during an inflationary epoch in the early universe. PAPPA will survey a 20 x 20 deg patch at the North Celestial Pole using 32 pixels in 3 passbands centered at 89, 212, and 302 GHz. Each pixel uses MEMS switches in a superconducting microstrip transmission line to combine the phase modulation techniques used in radio astronomy with the sensitivity of transition-edge superconducting bolometers. Each switched circuit modulates the incident polarization on a single detector, allowing nearly instantaneous characterization of the Stokes I, Q, and U parameters. We describe the instrument design and status.

  16. Mission design for LISA Pathfinder

    CERN Document Server

    Landgraf, M; Kemble, S

    2004-01-01

    Here we describe the mission design for SMART-2/LISA Pathfinder. The best trade-off between the requirements of a low-disturbance environment and communications distance is found to be a free-insertion Lissajous orbit around the first co-linear Lagrange point of the Sun-Earth system L1, 1.5x 10^6 km from Earth. In order to transfer SMART-2/LISA Pathfinder from a low Earth orbit, where it will be placed by a small launcher, the spacecraft carries out a number of apogee-raise manoeuvres, which ultimatively place it to a parabolic escape trajectory towards L1. The challenges of the design of a small mission are met, fulfilling the very demanding technology demonstration requirements without creating excessive requirements on the launch system or the ground segment.

  17. Strategic Team AI Path Plans: Probabilistic Pathfinding

    Directory of Open Access Journals (Sweden)

    Tng C. H. John

    2008-01-01

    Full Text Available This paper proposes a novel method to generate strategic team AI pathfinding plans for computer games and simulations using probabilistic pathfinding. This method is inspired by genetic algorithms (Russell and Norvig, 2002, in that, a fitness function is used to test the quality of the path plans. The method generates high-quality path plans by eliminating the low-quality ones. The path plans are generated by probabilistic pathfinding, and the elimination is done by a fitness test of the path plans. This path plan generation method has the ability to generate variation or different high-quality paths, which is desired for games to increase replay values. This work is an extension of our earlier work on team AI: probabilistic pathfinding (John et al., 2006. We explore ways to combine probabilistic pathfinding and genetic algorithm to create a new method to generate strategic team AI pathfinding plans.

  18. Electrostatic disturbances aboard LISA Pathfinder

    Science.gov (United States)

    Ferroni, Valerio

    Test mass charging and stray electrostatic fields are a potentially important source of force noise for the LISA Pathfinder mission. During the flight we plan to measure the relevant stray electrostatic fields on the surfaces of both the test mass and the electrode housing and compensate them with DC electrode bias voltages. In addition we monitor the charge and reduce it to near zero by UV illumination. We describe the analysis techniques used during the mission and explain the importance of periodic charging/discharging and of long-term charge measurements to limit the force noise at low frequency, which is particularly relevant for the eLISA mission.

  19. LISA Pathfinder: OPD loop characterisation

    Science.gov (United States)

    Born, Michael; LPF Collaboration

    2017-05-01

    The optical metrology system (OMS) of the LISA Pathfinder mission is measuring the distance between two free-floating test masses with unprecedented precision. One of the four OMS heterodyne interferometers reads out the phase difference between the reference and the measurement laser beam. This phase from the reference interferometer is common to all other longitudinal interferometer read outs and therefore subtracted. In addition, the phase is fed back via the digital optical pathlength difference (OPD) control loop to keep it close to zero. Here, we analyse the loop parameters and compare them to on-ground measurement results.

  20. Symbolic PathFinder v7

    DEFF Research Database (Denmark)

    Luckow, Kasper Søe; Păsăreanu, Corina

    2014-01-01

    We describe Symbolic PathFinder v7 in terms of its updated design addressing the changes of Java PathFinder v7 and of its new optimization when computing path conditions. Furthermore, we describe the Symbolic Execution Tree Extension; a newly added feature that allows for outputting the symbolic ...

  1. MESUR: metrics from scholarly usage of resources

    CERN Document Server

    CERN. Geneva

    2007-01-01

    The MESUR project is constructing a large-scale semantic model of the scholarly community that seamlessly integrates a wide range of bibliographic, citation and usage data. Functioning as a reference data set, this model is analyzed to characterize the intricate networks of typed relationships that exist in the scholarly community. The resulting ...

  2. Pathfinder - flight preparation on lakebed at sunrise

    Science.gov (United States)

    1995-01-01

    Crew members prepare the Pathfinder solar-powered aircraft for its first flight on Rogers Dry Lake at NASA's Dryden Flight Research Center, Edwards, California, after its configuration was changed from 8 motors to 6. Pathfinder was a lightweight, solar-powered, remotely piloted flying wing aircraft used to demonstrate the use of solar power for long-duration, high-altitude flight. Its name denotes its mission as the 'Pathfinder' or first in a series of solar-powered aircraft that will be able to remain airborne for weeks or months on scientific sampling and imaging missions. Solar arrays covered most of the upper wing surface of the Pathfinder aircraft. These arrays provided up to 8,000 watts of power at high noon on a clear summer day. That power fed the aircraft's six electric motors as well as its avionics, communications, and other electrical systems. Pathfinder also had a backup battery system that could provide power for two to five hours, allowing for limited-duration flight after dark. Pathfinder flew at airspeeds of only 15 to 20 mph. Pitch control was maintained by using tiny elevators on the trailing edge of the wing while turns and yaw control were accomplished by slowing down or speeding up the motors on the outboard sections of the wing. On September 11, 1995, Pathfinder set a new altitude record for solar-powered aircraft of 50,567 feet above Edwards Air Force Base, California, on a 12-hour flight. On July 7, 1997, it set another, unofficial record of 71,500 feet at the Pacific Missile Range Facility, Kauai, Hawaii. In 1998, Pathfinder was modified into the longer-winged Pathfinder Plus configuration. (See the Pathfinder Plus photos and project description.)

  3. Pathfinder on lakebed preparing for test flight

    Science.gov (United States)

    1995-01-01

    Support crew prepare the Pathfinder solar-powered aircraft for a research flight on Rogers Dry Lake at NASA's Dryden Flight Research Center, Edwards, California. Pathfinder was a lightweight, solar-powered, remotely piloted flying wing aircraft used to demonstrate the use of solar power for long-duration, high-altitude flight. Its name denotes its mission as the 'Pathfinder' or first in a series of solar-powered aircraft that will be able to remain airborne for weeks or months on scientific sampling and imaging missions. Solar arrays covered most of the upper wing surface of the Pathfinder aircraft. These arrays provided up to 8,000 watts of power at high noon on a clear summer day. That power fed the aircraft's six electric motors as well as its avionics, communications, and other electrical systems. Pathfinder also had a backup battery system that could provide power for two to five hours, allowing for limited-duration flight after dark. Pathfinder flew at airspeeds of only 15 to 20 mph. Pitch control was maintained by using tiny elevators on the trailing edge of the wing while turns and yaw control were accomplished by slowing down or speeding up the motors on the outboard sections of the wing. On September 11, 1995, Pathfinder set a new altitude record for solar-powered aircraft of 50,567 feet above Edwards Air Force Base, California, on a 12-hour flight. On July 7, 1997, it set another, unofficial record of 71,500 feet at the Pacific Missile Range Facility, Kauai, Hawaii. In 1998, Pathfinder was modified into the longer-winged Pathfinder Plus configuration. (See the Pathfinder Plus photos and project description.)

  4. Spacetime Metrology with LISA Pathfinder

    CERN Document Server

    Congedo, Giuseppe

    2012-01-01

    LISA is the proposed ESA-NASA gravitational wave detector in the 0.1 mHz - 0.1 Hz band. LISA Pathfinder is the down-scaled version of a single LISA arm. The arm -- named Doppler link -- can be treated as a differential accelerometer, measuring the relative acceleration between test masses. LISA Pathfinder -- the in-flight test of the LISA instrumentation -- is currently in the final implementation and planned to be launched in 2014. It will set stringent constraints on the ability to put test masses in geodesic motion to within the required differential acceleration of 3\\times10^{-14} m s^{-2} Hz^{-1/2} and track their relative motion to within the required differential displacement measurement noise of 9\\times10^{-12} m Hz^{-1/2}, around 1 mHz. Given the scientific objectives, it will carry out -- for the first time with such high accuracy required for gravitational wave detection -- the science of spacetime metrology, in which the Doppler link between two free-falling test masses measures the curvature. Thi...

  5. MESUR metrics from scholarly usage of resources

    CERN Document Server

    CERN. Geneva; Van de Sompel, Herbert

    2007-01-01

    Usage data is increasingly regarded as a valuable resource in the assessment of scholarly communication items. However, the development of quantitative, usage-based indicators of scholarly impact is still in its infancy. The Digital Library Research & Prototyping Team at the Los Alamos National Laboratory's Research library has therefore started a program to expand the set of usage-based tools for the assessment of scholarly communication items. The two-year MESUR project, funded by the Andrew W. Mellon Foundation, aims to define and validate a range of usage-based impact metrics, and issue guidelines with regards to their characteristics and proper application. The MESUR project is constructing a large-scale semantic model of the scholarly community that seamlessly integrates a wide range of bibliographic, citation and usage data. Functioning as a reference data set, this model is analyzed to characterize the intricate networks of typed relationships that exist in the scholarly community. The resulting c...

  6. Comprehensive Conservation Plan: Pathfinder National Wildlife Refuge

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This Comprehensive Conservation Plan (CCP) was written to guide management on Pathfinder NWR for the next 15 years. This plan outlines the Refuge vision and purpose...

  7. Using Map Decomposition to Improve Pathfinding

    OpenAIRE

    Kári Halldórsson 1979

    2015-01-01

    Artificial intelligence in games performs computationally expensive searches in large state spaces, i.e. for pathfinding and strategic decisions. Breaking the state space down into regions, with clear connections, can greatly benefit these algorithms, allowing decision making on a higher level and guiding searches in a more focused way through the search space. We present an improved heuristic for pathfinding search that takes advantage of such decompositions, as well as a fully automated m...

  8. Periodontal status among adolescents in Georgia. A pathfinder study

    Directory of Open Access Journals (Sweden)

    Liran Levin

    2013-09-01

    Full Text Available Objectives. The aim of the present pathfinder study was to screen and map the periodontal status of Georgian population in accordance with the guidelines of the World Health Organization for population based surveys. Methods. During 2012, a pathfinder study was conducted to collect this data. For the periodontal portion of the study, 15-year-old school children were examined in the capital city of Tbilisi as well as in two other large cities and 4 smaller villages. All participants were examined by a trained dental team in a classroom using a dental mirror and a periodontal probe. Periodontal examination included plaque scores, calculus scores, probing depth measurements and bleeding on probing. These measurements were recorded for the Ramfjord index teeth. Results. A total of 397 15-year-old participants were examined in this pathfinder study. There were 240 females (60.45% and 157 males (39.55%. Of the total participants 196 (49.37% were urban adolescents while 201 (50.63% were from rural communities. Mean probing depth was 3.34 ± 0.57 mm with a range of 1 to 10 mm; a relatively high proportion (34.26% of these subjects presented with at least one site with pockets of 5 mm or deeper. Males presented with greater plaque, calculus and probing depths than females. When urban and rural populations were compared, urban participants presented with more plaque, probing depths and bleeding on probing. Greater pocket depths were found to be related to the presence of plaque calculus and bleeding on probing. Conclusions. Overall, rather high incidences of periodontal pockets ≥ 5 mm were detected in this population. This data should serve to prepare further more detailed epidemiological studies that will serve to plan and implement prevent and treat strategies for periodontal diseases in Georgia and also help make manpower decisions.

  9. Free-flight experiments in LISA Pathfinder

    CERN Document Server

    Armano, M; Auger, G; Baird, J; Binetruy, P; Born, M; Bortoluzzi, D; Brandt, N; Bursi, A; Caleno, M; Cavalleri, A; Cesarini, A; Cruise, M; Cutler, C; Danzmann, K; Diepholz, I; Dolesi, R; Dunbar, N; Ferraioli, L; Ferroni, V; Fitzsimons, E; Freschi, M; Gallegos, J; Marirrodriga, C Garcia; Gerndt, R; Gesa, LI; Gibert, F; Giardini, D; Giusteri, R; Grimani, C; Harrison, I; Heinzel, G; Hewitson, M; Hollington, D; Hueller, M; Huesler, J; Inchauspe, H; Jennrich, O; Jetzer, P; Johlander, B; Karnesis, N; Kaune, B; Korsakova, N; Killow, C; Lloro, I; Maarschalkerweerd, R; Madden, S; Maghami, P; Mance, D; Martin, V; Martin-Porqueras, F; Mateos, I; McNamara, P; Mendes, J; Mendes, L; Moroni, A; Nofrarias, M; Paczkowski, S; Perreur-Lloyd, M; Petiteau, A; Pivato, P; Plagnol, E; Prat, P; Ragnit, U; Ramos-Castro, J; Reiche, J; Perez, J A Romera; Robertson, D; Rozemeijer, H; Russano, G; Sarra, P; Schleicher, A; Slutsky, J; Sopuerta, C F; Sumner, T; Texier, D; Thorpe, J; Trenkel, C; Tu, H B; Vetrugno, D; Vitale, S; Wanner, G; Ward, H; Waschke, S; Wass, P; Wealthy, D; Wen, S; Weber, W; Wittchen, A; Zanoni, C; Ziegler, T; Zweifel, P

    2014-01-01

    The LISA Pathfinder mission will demonstrate the technology of drag-free test masses for use as inertial references in future space-based gravitational wave detectors. To accomplish this, the Pathfinder spacecraft will perform drag-free flight about a test mass while measuring the acceleration of this primary test mass relative to a second reference test mass. Because the reference test mass is contained within the same spacecraft, it is necessary to apply forces on it to maintain its position and attitude relative to the spacecraft. These forces are a potential source of acceleration noise in the LISA Pathfinder system that are not present in the full LISA configuration. While LISA Pathfinder has been designed to meet it's primary mission requirements in the presence of this noise, recent estimates suggest that the on-orbit performance may be limited by this `suspension noise'. The drift-mode or free-flight experiments provide an opportunity to mitigate this noise source and further characterize the underlyi...

  10. Free-flight experiments in LISA Pathfinder

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Cutler, C.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; Gallegos, J.; García Marirrodriga, C.; Gerndt, R.; Gesa, LI; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Maghami, P.; Mance, D.; Martín, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mendes, L.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vetrugno, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    The LISA Pathfinder mission will demonstrate the technology of drag-free test masses for use as inertial references in future space-based gravitational wave detectors. To accomplish this, the Pathfinder spacecraft will perform drag-free flight about a test mass while measuring the acceleration of this primary test mass relative to a second reference test mass. Because the reference test mass is contained within the same spacecraft, it is necessary to apply forces on it to maintain its position and attitude relative to the spacecraft. These forces are a potential source of acceleration noise in the LISA Pathfinder system that are not present in the full LISA configuration. While LISA Pathfinder has been designed to meet it's primary mission requirements in the presence of this noise, recent estimates suggest that the on-orbit performance may be limited by this ‘suspension noise’. The drift-mode or free-flight experiments provide an opportunity to mitigate this noise source and further characterize the underlying disturbances that are of interest to the designers of LISA-like instruments. This article provides a high-level overview of these experiments and the methods under development to analyze the resulting data.

  11. Mechanical design of the Mars Pathfinder mission

    Science.gov (United States)

    Eisen, Howard Jay; Buck, Carl W.; Gillis-Smith, Greg R.; Umland, Jeffrey W.

    1997-01-01

    The Mars Pathfinder mission and the Sojourner rover is reported on, with emphasis on the various mission steps and the performance of the technologies involved. The mechanical design of mission hardware was critical to the success of the entry sequence and the landing operations. The various mechanisms employed are considered.

  12. Parameter estimation in LISA Pathfinder operational exercises

    CERN Document Server

    Nofrarias, Miquel; Congedo, Giuseppe; Hueller, Mauro; Armano, M; Diaz-Aguilo, M; Grynagier, A; Hewitson, M

    2011-01-01

    The LISA Pathfinder data analysis team has been developing in the last years the infrastructure and methods required to run the mission during flight operations. These are gathered in the LTPDA toolbox, an object oriented MATLAB toolbox that allows all the data analysis functionalities for the mission, while storing the history of all operations performed to the data, thus easing traceability and reproducibility of the analysis. The parameter estimation methods in the toolbox have been applied recently to data sets generated with the OSE (Off-line Simulations Environment), a detailed LISA Pathfinder non-linear simulator that will serve as a reference simulator during mission operations. These operational exercises aim at testing the on-orbit experiments in a realistic environment in terms of software and time constraints. These simulations, so called operational exercises, are the last verification step before translating these experiments into tele-command sequences for the spacecraft, producing therefore ve...

  13. Direction Oriented Pathfinding In Video Games

    Directory of Open Access Journals (Sweden)

    Xiao Cui

    2011-11-01

    Full Text Available Pathfinding has been one of major research areas in video games for many years. It is a key problem that most video games are confronted with. Search algorithm such as Dijkstra’s algorithm and A* algorithm are representing only half of the picture. The underlying map representations such as regular grid, visibility graph and navigation mesh also have significant impact on the performance. This paper reviews the current widely used solutions for pathfinding and proposes a new method which is expected to generate a higher quality path using less time and memory than other existing solutions. The deployment of methodology and techniques is described in detail. The aim and significance of the proposed method in future video games is addressed and the conclusion is given at the end.

  14. Testing MOND/TEVES with LISA Pathfinder

    CERN Document Server

    Trenkel, Christian; Bevis, Neil; Magueijo, Joao

    2010-01-01

    We suggest that LISA Pathfinder could be used to subject TEVES, and in particular the non-relativistic MOND phenomenology it incorporates, to a direct, controlled experimental test, in just a few years' time. The basic concept is to fly LISA Pathfinder through the region around the Sun-Earth saddle point, following its nominal mission, in order to look for anomalous gravity gradients. We examine various strategies to reach the saddle point, and conclude that the preferred strategy, resulting in relatively short transfer times of order one year, probably involves a lunar fly-by. We present robust estimates of the MOND gravity gradients that LISA Pathfinder should be exposed to, and conclude that if the gradiometer on-board the spacecraft achieves its nominal performance, these gradients will not just be detected, but measured and characterised in some detail, should they exist. Conversely, given the large predicted signal based on standard assumptions, a null result would most likely spell the end of TEVES/MON...

  15. The LISA Pathfinder DMU and Radiation Monitor

    Science.gov (United States)

    Canizares, P.; Chmeissani, M.; Conchillo, A.; Diaz–Aguiló, M.; García-Berro, E.; Gesa, L.; Gibert, F.; Grimani, C.; Lloro, I.; Lobo, A.; Mateos, I.; Nofrarias, M.; Ramos-Castro, J.; Sanjuán, J.; Sopuerta, Carlos F.; Araújo, H. M.; Wass, P.

    2011-05-01

    The LISA Pathfinder DMU (Data Management Unit) flight model was formally accepted by ESA and ASD on 11 February 2010, after all hardware and software tests had been successfully completed. The diagnostics items are scheduled to be delivered by the end of 2010. In this paper, we review the requirements and performance of this instrumentation, specially focusing on the Radiation Monitor and the DMU, as well as the status of their programmed use during mission operations, on which work is ongoing at the time of writing.

  16. The LISA Pathfinder DMU and Radiation Monitor

    Energy Technology Data Exchange (ETDEWEB)

    Canizares, P; Conchillo, A; Gesa, L; Lloro, I; Lobo, A; Mateos, I; Sopuerta, Carlos F [Institut de Ciencies de l' Espai, CSIC, Facultat de Ciencies, Torre C5 parell, 08193 Bellaterra (Spain); Chmeissani, M [Institut de Fisica d' Altes Energies (IFAE), Edifici CN, UAB Campus, 08193 Bellaterra (Spain); Diaz-Aguilo, M; GarcIa-Berro, E; Gibert, F [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Grimani, C [Universita degli Studi di Urbino, MFI Department, Via Santa Chiara 27, 61029 Urbino, and INFN Florence (Italy); Nofrarias, M [Max-Planck-Institut fuer Gravitationsphysik (Albert-Einstein-Institut), Callinstrasse 38, D-30167 Hannover (Germany); Ramos-Castro, J [Departament d' Enginyeria Electronica, UPC, Campus Nord, Edifici C4, Jordi Girona 1-3, 08034 Barcelona (Spain); Sanjuan, J [Department of Physics, University of Florida, NPB-22258 PO Box 118 440, Gainesville, FL 32611-8440 (United States); Araujo, H M; Wass, P, E-mail: lobo@ieec.fcr.es [High Energy Physics Blackett Laboratory, Prince Consort Road, Imperial College London, London SW7 2BW (United Kingdom)

    2011-05-07

    The LISA Pathfinder DMU (Data Management Unit) flight model was formally accepted by ESA and ASD on 11 February 2010, after all hardware and software tests had been successfully completed. The diagnostics items are scheduled to be delivered by the end of 2010. In this paper, we review the requirements and performance of this instrumentation, specially focusing on the Radiation Monitor and the DMU, as well as the status of their programmed use during mission operations, on which work is ongoing at the time of writing.

  17. Scientific results of the Mars Pathfinder mission.

    Science.gov (United States)

    Golombek, M. P.

    1999-02-01

    The author, project scientist of the Mars Pathfinder mision, presents a summary of the most important scientific results from the space probe, which descended to the Martian surface on July 4, 1997. These results include the strong evidence for catastrophic water floods in the history of the planet; close-up studies of the morphology and mineralogy of Martian rocks; the characteristics, chemistry, and origin of the magnetic dust particles deposited on the Martian surface; and meteorological measurements of temperature fluctuations, pressure variations, and wind velocities.

  18. Pathfinder aircraft prepared for flight at dawn on lakebed

    Science.gov (United States)

    1996-01-01

    The Pathfinder solar-powered research aircraft is silhouetted by the morning sun on the bed of Rogers Dry Lake as technicians prepare it for flight. The unique remotely piloted flying wing flew for two hours under control of a ground-based pilot on Nov. 19, 1996, at NASA's Dryden Flight Research Center, Edwards, California, while engineers checked out various aircraft systems. Pathfinder was a lightweight, solar-powered, remotely piloted flying wing aircraft used to demonstrate the use of solar power for long-duration, high-altitude flight. Its name denotes its mission as the 'Pathfinder' or first in a series of solar-powered aircraft that will be able to remain airborne for weeks or months on scientific sampling and imaging missions. Solar arrays covered most of the upper wing surface of the Pathfinder aircraft. These arrays provided up to 8,000 watts of power at high noon on a clear summer day. That power fed the aircraft's six electric motors as well as its avionics, communications, and other electrical systems. Pathfinder also had a backup battery system that could provide power for two to five hours, allowing for limited-duration flight after dark. Pathfinder flew at airspeeds of only 15 to 20 mph. Pitch control was maintained by using tiny elevators on the trailing edge of the wing while turns and yaw control were accomplished by slowing down or speeding up the motors on the outboard sections of the wing. On September 11, 1995, Pathfinder set a new altitude record for solar-powered aircraft of 50,567 feet above Edwards Air Force Base, California, on a 12-hour flight. On July 7, 1997, it set another, unofficial record of 71,500 feet at the Pacific Missile Range Facility, Kauai, Hawaii. In 1998, Pathfinder was modified into the longer-winged Pathfinder Plus configuration. (See the Pathfinder Plus photos and project description.)

  19. In-flight Diagnostics in LISA Pathfinder

    Science.gov (United States)

    Lobo, A.; Nofrarias, M.; Ramos-Castro, J.; Sanjuan, J.; Conchillo, A.; Ortega, J. A.; Xirgu, X.; Araujo, H.; Boatella, C.; Chmeissani, M.; Grimani, C.; Puigdengoles, C.; Wass, P.; García-Berro, E.; García, S.; Martínez, L. M.; Montero, G.

    2006-11-01

    LISA PathFinder (LPF) will be flown with the objective to test in space key technologies for LISA. However its sensitivity goals are, for good reason, one order of magnitude less than those which LISA will have to meet, both in drag-free and optical metrology requirements, and in the observation frequency band. While the expected success of LPF will of course be of itself a major step forward to LISA, one might not forget that a further improvement by an order of magnitude in performance will still be needed. Clues for the last leap are to be derived from proper disentanglement of the various sources of noise which contribute to the total noise, as measured in flight during the PathFinder mission. This paper describes the principles, workings and requirements of one of the key tools to serve the above objective: the diagnostics subsystem. This consists in sets of temperature, magnetic field, and particle counter sensors, together with generators of controlled thermal and magnetic perturbations. At least during the commissioning phase, the latter will be used to identify feed-through coefficients between diagnostics sensor readings and associated actual noise contributions. A brief progress report of the current state of development of the diagnostics subsystem will be given as well.

  20. In-flight Diagnostics in LISA Pathfinder

    CERN Document Server

    Lobo, A; Ramos-Castro, J; Sanjuan, J; Conchillo, A; Ortega, J A; Xirgu, X; Araujo, H; Boatella, C; Chmeissani, M; Grimani, C; Puigdengoles, C; Wass, P; García-Berro, E; García, S; Martínez, L; Montero, G; Lobo, Alberto; Nofrarias, Miquel; Ramos-Castro, Juan; Sanjuan, Josep; Conchillo, Aleix; Ortega, Jose Antonio; Xirgu, Xevi; Araujo, Henrique; Boatella, Cesar; Chmeissani, Mokhtar; Grimani, Catia; Puigdengoles, Carles; Wass, Peter; Garcia-Berro, Enrique; Garcia, Sergi; Martinez, Lluis; Montero, Gustau

    2007-01-01

    LISA PathFinder (LPF) will be flown with the objective to test in space key technologies for LISA. However its sensitivity goals are, for good reason, one order of magnitude less than those which LISA will have to meet, both in drag-free and optical metrology requirements, and in the observation frequency band. While the expected success of LPF will of course be of itself a major step forward to LISA, one might not forget that a further improvement by an order of magnitude in performance will still be needed. Clues for the last leap are to be derived from proper disentanglement of the various sources of noise which contribute to the total noise, as measured in flight during the PathFinder mission. This paper describes the principles, workings and requirements of one of the key tools to serve the above objective: the diagnostics subsystem. This consists in sets of temperature, magnetic field, and particle counter sensors, together with generators of controlled thermal and magnetic perturbations. At least durin...

  1. Detection of Micrometeoroids with LISA Pathfinder

    Science.gov (United States)

    Thorpe, Ira; Littenberg, Tyson; Janchez, Diego; Baker, John; The LISA Pathfinder Team Team

    2017-01-01

    The LISA Pathfinder mission (LPF), a joint ESA/NASA technology demonstration mission currently operating at the Sun-Earth L1 point, contains the most precise accelerometry system ever flown. Analysis suggests that LPF should have sufficient sensitivity to detect impacts of small micrometeoroids and dust through their transfer of momentum to the spacecraft. Moreover, LPF's ability to fully resolve both the linear and angular momentum transfer in three dimensions allows a magnitude, direction, and location to be estimated for each impact. We present preliminary results from a systematic search of the LISA Pathfinder data for such impacts and discuss the prospects for using these and future results to inform models of the formation and evolution of dust populations in the inner solar system. These models have wide applicability to both pure and applied space science, ranging from the physics of planet formation and dynamics of minor Solar System bodies to estimates of the micrometeorite hazard for future spacecraft. 2017 NASA Science Innovation Fund.

  2. Les mesures de métrologie pour le CLIC

    CERN Document Server

    Cherif, A

    2008-01-01

    Le projet CLIC est en tout point un défi technique majeur ; c?est le cas également pour la mesure dimensionnelle. Quels sont les équipements et les méthodes qui permettent de caractériser les pièces avec une incertitude de mesure aussi réduite que possible, vu les tolérances micrométriques imposées ? Afin de répondre à cette question, une veille technologique a été maintenue sur une longue période. Les acteurs relevants ont été contactés pour bénéficier d?une ouverture sur les dernières avancées dans le domaine. Différentes techniques ont été étudiées et comparées telles que la digitalisation, la tomographie X, la mesure tridimensionnelle. L'assemblage de haute précision des composants est aussi primordial. Sa mise en ?uvre sous un microscope optique ou à l'aide d'une machine tridimensionnelle est en cours d?étude. L'exposé traitera aussi de la mesure de rugosité, un domaine où nous disposons de moyens adaptés aux exigences spécifiques du projet.

  3. Pathfinder landing sites at candidate SNC impact ejection sites

    Science.gov (United States)

    Golombek, Matthew P.

    1994-01-01

    If Mars Pathfinder were able to land at a site on Mars from which the SNC meteorites were ejected by impact, the Pathfinder mission would essentially represent a very inexpensive sample return mission. Geologic units that contain four potential impact craters from which SNC meteorites could have been ejected from Mars are accessible to the Mars Pathfinder lander. Determining that SNC meteorites came from a particular spot on Mars raises the intriguing possibility of using Pathfinder as a sample return mission and providing a radiometric age for the considerably uncertain martian crater-age timescale. Pathfinder instruments are capable of determining if the rock type at the landing site is similar to that of one or more of the SNC meteorites, which would strengthen the hypothesis that the SNC meteorites did, in fact, come from Mars. Unfortunately, instrument observations from Pathfinder are probably not capable of determining if the geologic unit sampled by the lander is definitively the unit from which a SNC meteorite came from as opposed to Mars in general or perhaps a particular region on Mars. This abstract evaluates the possibility of landing at potential SNC ejection sites and the ability of Pathfinder to identify the landing site as the place from which an SNC meteorite came.

  4. APECS - The Atacama Pathfinder Experiment Control System

    CERN Document Server

    Muders, D; Hafok, H; Hatchell, J; Koenig, C; Polehampton, E; Schaaf, R; Schuller, F; Tak, F; Wyrowski, F

    2006-01-01

    APECS is the distributed control system of the new Atacama Pathfinder EXperiment (APEX) telescope located on the Llano de Chajnantor at an altitude of 5107 m in the Atacama desert in northern Chile. APECS is based on Atacama Large Millimeter Array (ALMA) software and employs a modern, object-oriented design using the Common Object Request Broker Architecture (CORBA) as the middleware. New generic device interfaces simplify adding instruments to the control system. The Python based observer command scripting language allows using many existing software libraries and facilitates creating more complex observing modes. A new self-descriptive raw data format (Multi-Beam FITS or MBFITS) has been defined to store the multi-beam, multi-frequency data. APECS provides an online pipeline for initial calibration, observer feedback and a quick-look display. APECS is being used for regular science observations in local and remote mode since August 2005.

  5. Model Checking JAVA Programs Using Java Pathfinder

    Science.gov (United States)

    Havelund, Klaus; Pressburger, Thomas

    2000-01-01

    This paper describes a translator called JAVA PATHFINDER from JAVA to PROMELA, the "programming language" of the SPIN model checker. The purpose is to establish a framework for verification and debugging of JAVA programs based on model checking. This work should be seen in a broader attempt to make formal methods applicable "in the loop" of programming within NASA's areas such as space, aviation, and robotics. Our main goal is to create automated formal methods such that programmers themselves can apply these in their daily work (in the loop) without the need for specialists to manually reformulate a program into a different notation in order to analyze the program. This work is a continuation of an effort to formally verify, using SPIN, a multi-threaded operating system programmed in Lisp for the Deep-Space 1 spacecraft, and of previous work in applying existing model checkers and theorem provers to real applications.

  6. Modal analysis of PATHFINDER unmanned air vehicle

    Energy Technology Data Exchange (ETDEWEB)

    Woehrle, T.G.; Costerus, B.W.; Lee, C.L.

    1994-10-19

    An experimental modal analysis was performed on PATHFINDER, a 450-lb, 100-ft wing span, flying-wing-design aircraft powered by solar/electric motors. The aircraft was softly suspended and then excited using random input from a long-stroke shaker. Modal data was taken from 92 measurement locations on the aircraft using newly designed, lightweight, tri-axial accelerometers. A conventional PC-based data acquisition system provided data handling. Modal parameters were calculated, and animated mode shapes were produced using SMS STARStruct{trademark} Modal Analysis System software. The modal parameters will be used for validation of finite element models, optimum placement of onboard accelerometers during flight testing, and vibration isolation design of sensor platforms.

  7. Java PathFinder User Guide

    Science.gov (United States)

    Havelund, Klaus

    1999-01-01

    The JAVA PATHFINDER, JPF, is a translator from a subset of JAVA 1.0 to PROMELA, the programming language of the SPIN model checker. The purpose of JPF is to establish a framework for verification and debugging of JAVA programming based on model checking. The main goal is to automate program verification such that a programmer can apply it in the daily work without the need for a specialist to manually reformulate a program into a different notation in order to analyze the program. The system is especially suited for analyzing multi-threaded JAVA applications, where normal testing usually falls short. The system can find deadlocks and violations of boolean assertions stated by the programmer in a special assertion language. This document explains how to Use JPF.

  8. Imager for Mars Pathfinder (IMP) image calibration

    Science.gov (United States)

    Reid, R.J.; Smith, P.H.; Lemmon, M.; Tanner, R.; Burkland, M.; Wegryn, E.; Weinberg, J.; Marcialis, R.; Britt, D.T.; Thomas, N.; Kramm, R.; Dummel, A.; Crowe, D.; Bos, B.J.; Bell, J.F.; Rueffer, P.; Gliem, F.; Johnson, J. R.; Maki, J.N.; Herkenhoff, K. E.; Singer, Robert B.

    1999-01-01

    The Imager for Mars Pathfinder returned over 16,000 high-quality images from the surface of Mars. The camera was well-calibrated in the laboratory, with <5% radiometric uncertainty. The photometric properties of two radiometric targets were also measured with 3% uncertainty. Several data sets acquired during the cruise and on Mars confirm that the system operated nominally throughout the course of the mission. Image calibration algorithms were developed for landed operations to correct instrumental sources of noise and to calibrate images relative to observations of the radiometric targets. The uncertainties associated with these algorithms as well as current improvements to image calibration are discussed. Copyright 1999 by the American Geophysical Union.

  9. Birdseye View of Pathfinder Landing Site

    Science.gov (United States)

    1997-01-01

    This image is one frame of an animation that was created by using two mosaics: a color image of the Gallery Pan and an image which indicates the distance to the nearest object at each pixel location, referred to as a range image. The range data set is treated as a displacement map with respect to a sphere's surface, and the color image mosaic is draped onto the inside of the sphere. The position of the camera is fixed at the sphere's center, while its viewing direction is in this case looking at the south pole of the sphere. The mosaics were projected onto a continuous cylindrical/perspective coordinate system spanning 360 degrees of azimuth. The distortion visible near the edges of this image is due to the large field of view, as well as the limitation introduced by using cylindrically-projected images on the sphere - the effects of which are less apparent when smaller fields of view are used.The image has been rotated so that the main points of interest, which are the 'Rock Garden,' the rover Sojourner and the rock 'Yogi,' are easily seen arching across the upper hemisphere. In fixed Mars Surface coordinates, the top of the image looks out towards a point a few degrees north of West. Color has been enhanced to improve contrast in features, and is derived from IMP spectral filters 5, 9 and 0.Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology (Caltech).

  10. Lithium-Thionyl Chloride Batteries for the Mars Pathfinder Microrover

    Energy Technology Data Exchange (ETDEWEB)

    Deligiannis, F.; Frank, H.; Staniewicz, R.J.; Willson, J. [SAFT America, Inc., Cockeysville, MD (United States)

    1996-02-01

    A discussion of the power requirements for the Mars Pathfinder Mission is given. Topics include: battery requirements; cell design; battery design; test descriptions and results. A summary of the results is also included.

  11. Lithium-Thionyl Chloride Batteries for the Mars Pathfinder Microrover

    Science.gov (United States)

    Deligiannis, Frank; Frank, Harvey; Staniewicz, R. J.; Willson, John

    1996-01-01

    A discussion of the power requirements for the Mars Pathfinder Mission is given. Topics include: battery requirements; cell design; battery design; test descriptions and results. A summary of the results is also included.

  12. CRED REA Algal Assessment, Pathfinder Bank 2003 (NODC Accession 0010352)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Random collections of algae were made at 2 sites at Pathfinder Bank in the Commonwealth of the Northern Mariana Islands in August and September, 2003 from the NOAA...

  13. Narrative report Pathfinder National Wildlife Refuge: January through December, 1967

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1967 calendar year. The report begins by summarizing...

  14. Narrative report Pathfinder National Wildlife Refuge: January through December, 1969

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1969 calendar year. The report begins by summarizing...

  15. Narrative report Pathfinder National Wildlife Refuge: January through December, 1970

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1970 calendar year. The report begins by summarizing...

  16. Narrative report Pathfinder National Wildlife Refuge: January through December, 1964

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1964 calendar year. The report begins by summarizing...

  17. Narrative report: Pathfinder National Wildlife Refuge: January through December 1972

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1972 calendar year. The report begins by summarizing...

  18. Narrative report Pathfinder National Wildlife Refuge: January through December, 1966

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1966 calendar year. The report begins by summarizing...

  19. Narrative report Pathfinder National Wildlife Refuge: January through December, 1971

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1971 calendar year. The report begins by summarizing...

  20. Narrative report Pathfinder National Wildlife Refuge: January through December, 1968

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments during the 1968 calendar year. The report begins by summarizing...

  1. Bayesian Model Selection for LISA Pathfinder

    CERN Document Server

    Karnesis, Nikolaos; Sopuerta, Carlos F; Gibert, Ferran; Armano, Michele; Audley, Heather; Congedo, Giuseppe; Diepholz, Ingo; Ferraioli, Luigi; Hewitson, Martin; Hueller, Mauro; Korsakova, Natalia; Plagnol, Eric; Vitale, and Stefano

    2013-01-01

    The main goal of the LISA Pathfinder (LPF) mission is to fully characterize the acceleration noise models and to test key technologies for future space-based gravitational-wave observatories similar to the LISA/eLISA concept. The Data Analysis (DA) team has developed complex three-dimensional models of the LISA Technology Package (LTP) experiment on-board LPF. These models are used for simulations, but more importantly, they will be used for parameter estimation purposes during flight operations. One of the tasks of the DA team is to identify the physical effects that contribute significantly to the properties of the instrument noise. A way of approaching to this problem is to recover the essential parameters of the LTP which describe the data. Thus, we want to define the simplest model that efficiently explains the observations. To do so, adopting a Bayesian framework, one has to estimate the so-called Bayes Factor between two competing models. In our analysis, we use three main different methods to estimate...

  2. The Mars Pathfinder Mission and Science Results

    Science.gov (United States)

    Golombek, M. P.

    1999-01-01

    Mars Pathfinder, the first low-cost, quick Discovery class mission to be completed, successfully landed on the surface of Mars on July 4, 1997, deployed and navigated a small rover, and collected data from 3 science instruments and 10 technology experiments. The mission operated on Mars for 3 months and returned 2.3 Gbits of new data, including over 16,500 lander and 550 rover images, 16 chemical analyses of rocks and soil, and 8.5 million individual temperature, pressure and wind measurements. The rover traversed 100 m clockwise around the lander, exploring about 200 square meters of the surface. The mission captured the imagination of the public, and garnered front page headlines during the first week. A total of about 566 million internet "hits" were registered during the first month of the mission, with 47 million "hits" on July 8th alone, making the Pathfinder landing by far the largest internet event in history at the time. Pathfinder was the first mission to deploy a rover on Mars. It carried a chemical analysis instrument, to characterize the rocks and soils in a landing area over hundreds of square meters on Mars, which provided a calibration point or "ground truth" for orbital remote sensing observations. The combination of spectral imaging of the landing area by the lander camera, chemical analyses aboard the rover, and close-up imaging of colors, textures and fabrics with the rover cameras offered the potential of identifying rocks (petrology and mineralogy). With this payload, a landing site in Ares Vallis was selected because it appeared acceptably safe and offered the prospect of analyzing a variety of rock types expected to be deposited by catastrophic floods, which enabled addressing first-order scientific questions such as differentiation of the crust, the development of weathering products, and the nature of the early Martian environment and its subsequent evolution. The 3 instruments and rover allowed seven areas of scientific investigation: the

  3. Data Acquisition System for the UFFO Pathfinder

    CERN Document Server

    Na, G W; Choi, H S; Choi, Y J; Grossan, B; Hermann, I; Jeong, S; Jung, A; Kim, J E; Kim, S -W; Kim, Y W; Lee, J; Lim, H; Linder, E V; Min, K W; Nam, J W; Nam, K H; Panayuk, M I; Park, I H; Smoot, G F; Suh, Y D; Svelitov, S; Vedenken, N; Yashin, I; Zhao, M H

    2011-01-01

    The Ultra-Fast Flash Observatory (UFFO) Pathfinder is a payload on the Russian Lomonosov satellite, scheduled to be launched in November 2011. The Observatory is designed to detect early UV/Optical photons from Gamma-Ray Bursts (GRBs). There are two telescopes and one main data acquisition system: the UFFO Burst Alert & Trigger Telescope (UBAT), the Slewing Mirror Telescope (SMT), and the UFFO Data Acquisition (UDAQ) system. The UDAQ controls and manages the operation and communication of each telescope, and is also in charge of the interface with the satellite. It will write the data taken by each telescope to the NOR flash memory and sends them to the satellite via the Bus-Interface system (BI). It also receives data from the satellite including the coordinates and time of an external trigger from another payload, and distributes them to two telescopes. These functions are implemented in field programmable gates arrays (FPGA) for low power consumption and fast processing without a microprocessor. The UD...

  4. Rectangle expansion A∗ pathfinding for grid maps

    Directory of Open Access Journals (Sweden)

    Zhang An

    2016-10-01

    Full Text Available Search speed, quality of resulting paths and the cost of pre-processing are the principle evaluation metrics of a pathfinding algorithm. In this paper, a new algorithm for grid-based maps, rectangle expansion A∗ (REA∗, is presented that improves the performance of A∗ significantly. REA∗ explores maps in units of unblocked rectangles. All unnecessary points inside the rectangles are pruned and boundaries of the rectangles (instead of individual points within those boundaries are used as search nodes. This makes the algorithm plot fewer points and have a much shorter open list than A∗. REA∗ returns jump and grid-optimal path points, but since the line of sight between jump points is protected by the unblocked rectangles, the resulting path of REA∗ is usually better than grid-optimal. The algorithm is entirely online and requires no offline pre-processing. Experimental results for typical benchmark problem sets show that REA∗ can speed up a highly optimized A∗ by an order of magnitude and more while preserving completeness and optimality. This new algorithm is competitive with other highly successful variants of A∗.

  5. CBM a Pathfinder of Petroleum System?

    Directory of Open Access Journals (Sweden)

    Swapan Kumar Bhattacharya

    2014-04-01

    Full Text Available The present study aims to understand if there is any relation of commercial methane in CBM producers with oil producing kerogen. This is necessary because methane in coal, by default, is assigned to be sourced by bacterial/thermal actions on biomass during coalification process but critical analysis suggests it cannot be commercial because coal bears a ratio of molar concentrations of Hydrogen to Carbon (H/C around 0.8 whereas methane require H/C = 4.0. A simple calculation reveals 1Tcf of methane generation may come from around 25 trillion tonnes of coal, suggesting commercial methane cannot be sourced only from coal. Generation of methane can be biogenic or thermogenic, either from coal or related organic biomass or from oil generating kerogen. Technically, we can distinguish biogenic methane from thermogenic but we cannot distinguish same methane either from coal or from oil generating kerogen unless it is evident that one is distinctly biogenic and the other is thermogenic. Further, a review of successful major CBM projects also reveals that most of them are geologically associated with some producing petroliferous basin. This suggests that a close genetic relationship between the occurrence of coal bed methane and petroliferous basin probably exists whereby adsorbed methane in coal bed is possibly sourced from the same oil generating kerogen in the basin. Therefore, discovery of commercial coal bed methane may suggest possible existence of mature source rock in the basin and may act as pathfinder of possible new petroleum system attached to it.

  6. SST, Pathfinder Ver 5.0, Night, 4.4 km, Global, Science Quality

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — AVHRR Pathfinder Oceans Project seeks to create a long-term, continuous sea surface temperature data series for use in climate research. The Pathfinder SST data...

  7. SST, Pathfinder Ver 5.0, Day, 4.4 km, Global, Science Quality

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — AVHRR Pathfinder Oceans Project seeks to create a long-term, continuous sea surface temperature data series for use in climate research. The Pathfinder SST data...

  8. SST, Pathfinder Ver 5.0, Day and Night, 4.4 km, Global, Science Quality

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — AVHRR Pathfinder Oceans Project seeks to create a long-term, continuous sea surface temperature data series for use in climate research. The Pathfinder SST data...

  9. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

    Science.gov (United States)

    Antonucci, F.; Armano, M.; Audley, H.; Auger, G.; Benedetti, M.; Binetruy, P.; Boatella, C.; Bogenstahl, J.; Bortoluzzi, D.; Bosetti, P.; Brandt, N.; Caleno, M.; Cavalleri, A.; Cesa, M.; Chmeissani, M.; Ciani, G.; Conchillo, A.; Congedo, G.; Cristofolini, I.; Cruise, M.; Danzmann, K.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Dunbar, N.; Fauste, J.; Ferraioli, L.; Fertin, D.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marin, A.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Giardini, D.; Gibert, F.; Grimani, C.; Grynagier, A.; Guillaume, B.; Guzmán, F.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hough, J.; Hoyland, D.; Hueller, M.; Huesler, J.; Jeannin, O.; Jennrich, O.; Jetzer, P.; Johlander, B.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mitchell, E.; Monsky, A.; Nicolini, D.; Nicolodi, D.; Nofrarias, M.; Pedersen, F.; Perreur-Lloyd, M.; Perreca, A.; Plagnol, E.; Prat, P.; Racca, G. D.; Rais, B.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Sanjuan, J.; Schleicher, A.; Schulte, M.; Shaul, D.; Stagnaro, L.; Strandmoe, S.; Steier, F.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tombolato, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Weber, W. J.; Zweifel, P.

    2011-05-01

    This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware, flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor 2 of the LISA requirement at 1 mHz and within a factor 6 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement that will guarantee the LISA performance.

  10. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

    Energy Technology Data Exchange (ETDEWEB)

    Antonucci, F; Cavalleri, A; Congedo, G [Dipartimento di Fisica, Universita di Trento and INFN, Gruppo Collegato di Trento, 38050 Povo, Trento (Italy); Armano, M [European Space Astronomy Centre, European Space Agency, Villanueva de la Canada, 28692 Madrid (Spain); Audley, H; Bogenstahl, J [Albert-Einstein-Institut, Max-Planck-Institut fuer Gravitationsphysik und Universitaet Hannover, 30167 Hannover (Germany); Auger, G; Binetruy, P [APC UMR7164, Universite Paris Diderot, Paris (France); Benedetti, M [Dipartimento di Ingegneria dei Materiali e Tecnologie Industriali, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Boatella, C [CNES, DCT/AQ/EC, 18 Avenue Edouard Belin, 31401 Toulouse, Cedex 9 (France); Bortoluzzi, D; Bosetti, P; Cristofolini, I [Dipartimento di Ingegneria Meccanica e Strutturale, Universita di Trento and INFN, Gruppo Collegato di Trento, Mesiano, Trento (Italy); Brandt, N [Astrium GmbH Claude-Dornier-Strasse, 88090 Immenstaad (Germany); Caleno, M; Cesa, M [European Space Technology Centre, European Space Agency, Keplerlaan 1, 2200 AG Noordwijk (Netherlands); Chmeissani, M [IFAE, Universitat Autonoma de Barcelona, E-08193 Bellaterra, Barcelona (Spain); Ciani, G [Department of Physics, University of Florida, Gainesville, FL 32611-8440 (United States); Conchillo, A [ICE-CSIC/IEEC, Facultat de Ciencies, E-08193 Bellaterra, Barcelona (Spain); Cruise, M, E-mail: Stefano.Vitale@unitn.it [Department of Physics and Astronomy, University of Birmingham, Birmingham (United Kingdom)

    2011-05-07

    This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware, flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor 2 of the LISA requirement at 1 mHz and within a factor 6 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement that will guarantee the LISA performance.

  11. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

    CERN Document Server

    Antonucci, F; Audley, H; Auger, G; Benedetti, M; Binetruy, P; Boatella, C; Bogenstahl, J; Bortoluzzi, D; Bosetti, P; Brandt, N; Caleno, M; Cavalleri, A; Cesa, M; Chmeissani, M; Ciani, G; Conchillo, A; Congedo, G; Cristofolini, I; Cruise, M; Danzmann, K; De Marchi, F; Diaz-Aguilo, M; Diepholz, I; Dixon, G; Dolesi, R; Dunbar, N; Fauste, J; Ferraioli, L; Fertin, D; Fichter, W; Fitzsimons, E; Freschi, M; Marin, A García; Marirrodriga, C García; Gerndt, R; Gesa, L; Giardini, D; Gibert, F; Grimani, C; Grynagier, A; Guillaume, B; Guzmán, F; Harrison, I; Heinzel, G; Hewitson, M; Hollington, D; Hough, J; Hoyland, D; Hueller, M; Huesler, J; Jeannin, O; Jennrich, O; Jetzer, P; Johlander, B; Killow, C; Llamas, X; Lloro, I; Lobo, A; Maarschalkerweerd, R; Madden, S; Mance, D; Mateos, I; McNamara, P W; Mendestì, J; Mitchell, E; Monsky, A; Nicolini, D; Nicolodi, D; Nofrarias, M; Pedersen, F; Perreur-Lloyd, M; Perreca, A; Plagnol, E; Prat, P; Racca, G D; Rais, B; Ramos-Castro, J; Reiche, J; Perez, J A Romera; Robertson, D; Rozemeijer, H; Sanjuan, J; Schleicher, A; Schulte, M; Shaul, D; Stagnaro, L; Strandmoe, S; Steier, F; Sumner, T J; Taylor, A; Texier, D; Trenkel, C; Tombolato, D; Vitale, S; Wanner, G; Ward, H; Waschke, S; Wass, P; Weber, W J; Zweifel, P

    2010-01-01

    This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware and flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor two of the LISA requirement at 1 mHz and within a factor 10 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement, that will guarantee the LISA performance.

  12. Design Overview of the DM Radio Pathfinder Experiment

    CERN Document Server

    Silva-Feaver, Maximiliano; Cho, Hsiao-Mei; Dawson, Carl; Graham, Peter; Irwin, Kent; Kuenstner, Stephen; Li, Dale; Mardon, Jeremy; Moseley, Harvey; Mule, Richard; Phipps, Arran; Rajendran, Surjeet; Steffen, Zach; Young, Betty

    2016-01-01

    We introduce the DM Radio, a dual search for axion and hidden photon dark matter using a tunable superconducting lumped-element resonator. We discuss the prototype DM Radio Pathfinder experiment, which will probe hidden photons in the 500 peV (100 kHz)-50 neV (10 MHz) mass range. We detail the design of the various components: the LC resonant detector, the resonant frequency tuning procedure, the differential SQUID readout circuit, the shielding, and the cryogenic mounting structure. We present the current status of the pathfinder experiment and illustrate its potential science reach in the context of the larger experimental program.

  13. Lincoln Pathfinder: Internet Resources on Studying and Teaching Abraham Lincoln

    Directory of Open Access Journals (Sweden)

    Andreas Hübner

    2009-09-01

    Full Text Available Apart from encouraging an innumerable quantity of scholarly works and projects, the subject matter of Lincoln’s Legacy has also produced an increasing amount of online ventures and digital resource collections. The Lincoln Pathfinder aims to provide a quick guide to these Web sites and to initiate a controversial debate, likely to take place in the EFL classroom. Divided into five categories—general, primary, secondary, visual, and teaching resources—the Lincoln Pathfinder may function as a helpful research tool and a basis of discussion.

  14. Implementasi Algoritma A* Berbasis Pathfinding Dalam Pengembangan Game Menanam Pohon

    OpenAIRE

    Pohan, Rahmat Irfan

    2016-01-01

    Anyone would take the path that they consider to be the shortest path when they travel from one place to another. But it would be difficult for such a person to choose which path is the shortest, because it could be the chosen path is not the shortest path. The method for determining the shortest path is pathfinding. Pathfinding is widely used in various fields of Computer Science, one of them on the field of video game development. In this research, the authors will design and analyze the pa...

  15. Martian Mixed Layer during Pathfinder Mission

    Science.gov (United States)

    Martinez, G. M.; Valero, F.; Vazquez, L.

    2008-09-01

    In situ measurements of the Martian Planetary Boundary Layer (MPBL) encompass only the sur- face layer. Therefore, in order to fully address the MPBL, it becomes necessary to simulate somehow the behaviour of the martian mixed layer. The small-scale processes that happen in the MPBL cause GCM's ([1], [2]) to describe only partially the turbulent statistics, height, convective scales, etc, of the surface layer and the mixed layer. For this reason, 2D and 3D martian mesoscale models ([4], [5]), and large eddy simulations ([4], [6], [7], [8]) have been designed in the last years. Although they are expected to simulate more accurately the MPBL, they take an extremely expensive compu- tational time. Alternatively, we have derived the main turbu- lent characteristics of the martian mixed layer by using surface layer and mixed layer similarity ([9], [10]). From in situ temperature and wind speed measurements, together with quality-tested simu- lated ground temperature [11], we have character- ized the martian mixed layer during the convective hours of Pathfinder mission Sol 25. Mean mixed layer turbulent statistics like tem- perature variance , horizontal wind speed variance , vertical wind speed variance , viscous dissipation rate , and turbu- lent kinetic energy have been calculated, as well as the mixed layer height zi, and the convective scales of wind w? and temperature θ?. Our values, obtained with negligible time cost, match quite well with some previously obtained results via LES's ([4] and [8]). A comparisson between the above obtained mar- tian values and the typical Earth values are shown in Table 1. Convective velocity scale w doubles its counterpart terrestrial typical value, as it does the mean wind speed variances and . On the other hand, the temperature scale θ? and the mean temperature variance are virtually around one order higher on Mars. The limitations of these results concern the va- lidity of the convective mixed layer similarity. This theory

  16. La mesure du travail dans la famille : création, définition et mesure du travail parental

    OpenAIRE

    Marie-Agnès Barrère-Maurisson

    2012-01-01

    Comment les transformations de la famille, mais aussi celles de l'emploi, ont-elles conduit à de nouvelles pratiques, spécifiques et distinctes du travail domestique à proprement parler, autour de la prise en charge des enfants par la famille ? Commant ce travail particulier, le parental, a-t-il pu être isolé et défini ? Comment a-t-il été évalué, en référence à quelle mesure étalon, et pourquoi ?.

  17. MESUR: USAGE-BASED METRICS OF SCHOLARLY IMPACT

    Energy Technology Data Exchange (ETDEWEB)

    BOLLEN, JOHAN [Los Alamos National Laboratory; RODRIGUEZ, MARKO A. [Los Alamos National Laboratory; VAN DE SOMPEL, HERBERT [Los Alamos National Laboratory

    2007-01-30

    The evaluation of scholarly communication items is now largely a matter of expert opinion or metrics derived from citation data. Both approaches can fail to take into account the myriad of factors that shape scholarly impact. Usage data has emerged as a promising complement to existing methods o fassessment but the formal groundwork to reliably and validly apply usage-based metrics of schlolarly impact is lacking. The Andrew W. Mellon Foundation funded MESUR project constitutes a systematic effort to define, validate and cross-validate a range of usage-based metrics of schlolarly impact by creating a semantic model of the scholarly communication process. The constructed model will serve as the basis of a creating a large-scale semantic network that seamlessly relates citation, bibliographic and usage data from a variety of sources. A subsequent program that uses the established semantic network as a reference data set will determine the characteristics and semantics of a variety of usage-based metrics of schlolarly impact. This paper outlines the architecture and methodology adopted by the MESUR project and its future direction.

  18. Update on The Ultra-Fast Flash Observatory (UFFO) Pathfinder

    DEFF Research Database (Denmark)

    Grossan, B.; Brandt, Søren; Budtz-Jørgensen, Carl

    2011-01-01

    , the Slewing Mirror Telescope (SMT), is planned to use an array of micro-electromechanical (MEMS) mirrors, with negligible moments of inertia, to steer its beam rapidly and accurately. The UFFO Pathfinder is scheduled to be launched into orbit by 2012 January. In this presentation, we give the current design...

  19. A Pathfinder for Animal Research and Animal Rights.

    Science.gov (United States)

    Anderson, David C.

    1992-01-01

    This pathfinder was originally prepared for "Biomedical Research and Animal Rights," a session sponsored by the Veterinary Medical Libraries and Research Libraries Sections of the Medical Library Association. Current resources are described, from bibliographies to electronic bulletin boards, which relate to the issue of laboratory animal welfare…

  20. A Pathfinder for Animal Research and Animal Rights.

    Science.gov (United States)

    Anderson, David C.

    1992-01-01

    This pathfinder was originally prepared for "Biomedical Research and Animal Rights," a session sponsored by the Veterinary Medical Libraries and Research Libraries Sections of the Medical Library Association. Current resources are described, from bibliographies to electronic bulletin boards, which relate to the issue of laboratory animal…

  1. A review of Australian experience in the evaluation of helium as a pathfinder in exploration

    Science.gov (United States)

    Butt, C. R. M.; Gole, M. J.; Hart, M. K. W.

    1987-11-01

    Orientation surveys were conducted to test the potential of using 4He as a pathfinder in mineral and hydrocarbon exploration. Groundwaters were sampled from drill holes and stock wells. Overburden gas samples were collected via fixed tubes emplaced at 6 m depth in backfilled drill holes. While He concentrations in groundwaters associated with most U mineralization were far in excess of the atmospheric equilibrium value of 0.044 μL/L, equivalent, or higher, concentrations were found in groundwaters from unmineralized areas around the deposits. These latter concentrations appear to be due to accumulation of He in groundwaters with long residence times and by leakage from deep sources, particularly granitoid basement. Only at the Koongarra U deposit, where groundwaters are annually recharged, did anomalous He concentrations appear to indicate the presence of the deposit. No credible He anomaly was detected in overburden gas over any U deposit. However, a marked overburden gas He anomaly was detected over the Gingin gas field, although normalization to constant 20Ne suggested much of this to be a relative enrichment due to near-surface biological activity related to the leakage of hydrocarbons altering the major gas composition, particularly the CO2/O2 ratio of the soil atmosphere. It is concluded that He, when used in conjunction with other gases, may be useful in near-surface geochemical exploration for hydrocarbons but that it does not appear to be an effective pathfinder for U deposits.

  2. ``Astrophysique sur Mesure'', E-learning in Astronomy and Astrophysics

    Science.gov (United States)

    Mosser, Benoît; Delsanti, Audrey; Guillaume, Damien; Balança, Christian; Balkowski, Chantal

    2011-06-01

    ``Astrophysique sur Mesure'' (astrophysics made-to-measure) is a set of e-learning programmes started 4 years ago at the Paris Observatory. In order to deliver attractive and efficient programmes, we have added many multimedia tools to usual lectures: animations, Java applets. The programmes are presented on two different platforms. The first one offers the content of all the lectures in free access. A second platform with restricted access is provided to registered students taking part in the e-learning program and benefiting from the help of tutors. The development of these programs helps to increase the sphere of influence of astronomy taught at the Paris Observatory, hence to increase the presence of astronomy in various degree courses. Instead of teaching classical astronomy lectures to a happy few, we can bring astronomy and astrophysics to a wider audience.

  3. Limits on the Ultra-bright Fast Radio Burst Population from the CHIME Pathfinder

    Science.gov (United States)

    Amiri, M.; Bandura, K.; Berger, P.; Bond, J. R.; Cliche, J. F.; Connor, L.; Deng, M.; Denman, N.; Dobbs, M.; Domagalski, R. S.; Fandino, M.; Gilbert, A. J.; Good, D. C.; Halpern, M.; Hanna, D.; Hincks, A. D.; Hinshaw, G.; Höfer, C.; Hsyu, G.; Klages, P.; Landecker, T. L.; Masui, K.; Mena-Parra, J.; Newburgh, L. B.; Oppermann, N.; Pen, U. L.; Peterson, J. B.; Pinsonneault-Marotte, T.; Renard, A.; Shaw, J. R.; Siegel, S. R.; Sigurdson, K.; Smith, K.; Storer, E.; Tretyakov, I.; Vanderlinde, K.; Wiebe, D. V.; Scientific Collaboration20, CHIME

    2017-08-01

    We present results from a new incoherent-beam fast radio burst (FRB) search on the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder. Its large instantaneous field of view (FoV) and relative thermal insensitivity allow us to probe the ultra-bright tail of the FRB distribution, and to test a recent claim that this distribution’s slope, α \\equiv -\\tfrac{\\partial {log}N}{\\partial {log}S}, is quite small. A 256-input incoherent beamformer was deployed on the CHIME Pathfinder for this purpose. If the FRB distribution were described by a single power law with α = 0.7, we would expect an FRB detection every few days, making this the fastest survey on the sky at present. We collected 1268 hr of data, amounting to one of the largest exposures of any FRB survey, with over 2.4 × 105 deg2 hr. Having seen no bursts, we have constrained the rate of extremely bright events to <13 sky-1 day-1 above ˜ 220\\sqrt{(τ /{ms})} {Jy} {ms} for τ between 1.3 and 100 ms, at 400-800 MHz. The non-detection also allows us to rule out α ≲ 0.9 with 95% confidence, after marginalizing over uncertainties in the GBT rate at 700-900 MHz, though we show that for a cosmological population and a large dynamic range in flux density, α is brightness dependent. Since FRBs now extend to large enough distances that non-Euclidean effects are significant, there is still expected to be a dearth of faint events and relative excess of bright events. Nevertheless we have constrained the allowed number of ultra-intense FRBs. While this does not have significant implications for deeper, large-FoV surveys like full CHIME and APERTIF, it does have important consequences for other wide-field, small dish experiments.

  4. The Australian Square Kilometre Array Pathfinder: System Architecture and Specifications of the Boolardy Engineering Test Array

    CERN Document Server

    Hotan, A W; Harvey-Smith, L; Humphreys, B; Jeffs, B D; Shimwell, T; Tuthill, J; Voronkov, M; Allen, G; Amy, S; Ardern, K; Axtens, P; Ball, L; Bannister, K; Barker, S; Bateman, T; Beresford, R; Bock, D; Bolton, R; Bowen, M; Boyle, B; Braun, R; Broadhurst, S; Brodrick, D; Brooks, K; Brothers, M; Brown, A; Cantrall, C; Carrad, G; Chapman, J; Cheng, W; Chippendale, A; Chung, Y; Cooray, F; Cornwell, T; Davis, E; de Souza, L; DeBoer, D; Diamond, P; Edwards, P; Ekers, R; Feain, I; Ferris, D; Forsyth, R; Gough, R; Grancea, A; Gupta, N; Guzman, JC; Hampson, G; Haskins, C; Hay, S; Hayman, D; Hoyle, S; Jacka, C; Jackson, C; Jackson, S; Jeganathan, K; Johnston, S; Joseph, J; Kendall, R; Kesteven, M; Kiraly, D; Koribalski, B; Leach, M; Lenc, E; Lensson, E; Li, L; Mackay, S; Macleod, A; Maher, T; Marquarding, M; McClure-Griffiths, N; McConnell, D; Mickle, S; Mirtschin, P; Norris, R; Neuhold, S; Ng, A; O'Sullivan, J; Pathikulangara, J; Pearce, S; Phillips, C; Qiao, RY; Reynolds, J E; Rispler, A; Roberts, P; Roxby, D; Schinckel, A; Shaw, R; Shields, M; Storey, M; Sweetnam, T; Troup, E; Turner, B; Tzioumis, A; Westmeier, T; Whiting, M; Wilson, C; Wilson, T; Wormnes, K; Wu, X

    2014-01-01

    This paper describes the system architecture of a newly constructed radio telescope - the Boolardy Engineering Test Array, which is a prototype of the Australian Square Kilometre Array Pathfinder telescope. Phased array feed technology is used to form multiple simultaneous beams per antenna, providing astronomers with unprecedented survey speed. The test array described here is a 6-antenna interferometer, fitted with prototype signal processing hardware capable of forming at least 9 dual-polarisation beams simultaneously, allowing several square degrees to be imaged in a single pointed observation. The main purpose of the test array is to develop beamforming and wide-field calibration methods for use with the full telescope, but it will also be capable of limited early science demonstrations.

  5. Interface Generation and Compositional Verification in JavaPathfinder

    Science.gov (United States)

    Giannakopoulou, Dimitra; Pasareanu, Corina

    2009-01-01

    We present a novel algorithm for interface generation of software components. Given a component, our algorithm uses learning techniques to compute a permissive interface representing legal usage of the component. Unlike our previous work, this algorithm does not require knowledge about the component s environment. Furthermore, in contrast to other related approaches, our algorithm computes permissive interfaces even in the presence of non-determinism in the component. Our algorithm is implemented in the JavaPathfinder model checking framework for UML statechart components. We have also added support for automated assume-guarantee style compositional verification in JavaPathfinder, using component interfaces. We report on the application of the presented approach to the generation of interfaces for flight software components.

  6. First light of the LINC-NIRVANA Pathfinder experiment

    Science.gov (United States)

    Bergomi, M.; Viotto, V.; Arcidiacono, C.; Marafatto, L.; Farinato, J.; Baumeister, H.; Bertram, T.; Berwein, J.; Briegel, F.; Conrad, A.; Kittman, F.; Kopon, D.; Hofferbert, R.; Magrin, D.; Radhakrishnan Santhakumari, K. K.; Puglisi, A.; Xompero, M.; Briguglio, R.; Quiros-Pacheco, F.; Herbst, T. M.; Ragazzoni, R.

    2014-07-01

    The LINC-NIRVANA Pathfinder experiment is a test-bed to verify a very complex sub-system: the Ground-layer Wavefront Sensor, or GWS. Pathfinder will test the GWS in its final working environment and demonstrate on-sky the performance achievable with a multiple natural guide star, ground-layer adaptive optics system with a very wide FoV. The GWS uses up to 12 natural guide stars within a 2.8'-6' annular field of view and drives the LBT adaptive secondary mirror to correct the lower layers of atmospheric turbulence. This paper will trace the path of the instrument on its way to First Light on-sky in November 2013, from its installation on the telescope to the calibrations to its final operation, focusing in particular on opto-mechanical and software aspects and how they lead to the main achieved results.

  7. True Color of Mars - Pathfinder Sol 39 Sunrise

    Science.gov (United States)

    1999-01-01

    Sunrise, sol 39. This true color, pre-sunrise image (approximately 0530LST) is composed of six images extending 30 o in azimuth and 45 o in elevation and shows the brownish gray predawn sky. A description of the techniques used to generate this color image from IMP data can be found in Maki et al., 1999. Note: a calibrated output device is required accurately reproduce the correct colors.Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is an operating division of the California Institute of Technology (Caltech). The IMP was developed by the University of Arizona Lunar and Planetary Laboratory under contract to JPL. Peter Smith is the Principal investigator.

  8. Design of the magnetic diagnostics unit onboard LISA Pathfinder

    CERN Document Server

    Diaz-Aguiló, Marc; Ramos-Castro, Juan; Lobo, Alberto; García-Berro, Enrique

    2012-01-01

    LISA (Laser Interferometer Space Antenna) is a joint mission of ESA and NASA which aims to be the first space-borne gravita- tional wave observatory. Due to the high complexity and technological challenges that LISA will face, ESA decided to launch a technological demonstrator, LISA Pathfinder. The payload of LISA Pathfinder is the so-called LISA Technology Package, and will be the highest sensitivity geodesic explorer flown to date. The LISA Technology Package is designed to measure relative accelerations between two test masses in nominal free fall (geodesic motion). The magnetic, thermal and radiation disturbances affecting the payload are monitored and dealt by the diagnostics subsystem. The diagnostics subsystem consists of several modules, and one of these is the magnetic diagnostics unit. Its main function is the assessment of differential acceleration noise between test masses due to the magnetic effects. To do so, it has to determine the magnetic characteristics of the test masses, namely their magne...

  9. Algoritma Pathfinding A* Pada Game RPG Tanaman Higienis

    Directory of Open Access Journals (Sweden)

    Andy Pramono

    2015-11-01

    Full Text Available Penggunaan pestisida kimia pada produkpertanian berakibat buruk terhadap kesehatan manusiadan menimbulkan pencemaran lingkungan. Salah satusolusinya adalah dengan cara membuat media sosialisasipengenalan pertanian higienis kepada masyarakat.Penelitian ini bertujuan untuk menghasilkan sebuahproduk game tiga dimensi sebagai upaya untukmenyampaikan informasi mengenai konsep pertanianhigienis. Dalam game RPG diperlukan suatu penerapansuatu algoritma pathfinding sebagai implementasipenghalang pada game tanaman higienis.Model perancangan yang digunakan adalah modelprosedural, merupakan model penelitian yang bersifatdeskriptif, yang menggariskan langkah-langkah yangharus di ikuti untuk menghasilkan sebuah produk.Pengumpulan data dilakukan dengan cara studi literaturmengenai algoritma pathfinding A* dan game komputer,serta identifikasi target audiens dan produk kompetitor.Tahap ujicoba pada penerapan algoritma A* inidilakukan dengan 2 pola yaitu uji coba internal dan ujicoba eksternal.Berdasarkan hasil ujicoba yang telah dilakukanterhadap algoritma A* dalam game higienis dapatdisimpulkan algoritma A* dapat diimplementasikandengan perancangan game tanaman organis terutamapada pergerakan penghalang. Kata Kunci: perancangan, algoritma A*, game

  10. Inflight magnetic characterization of the test masses onboard LISA Pathfinder

    CERN Document Server

    Diaz-Aguiló, Marc; Lobo, Alberto

    2012-01-01

    LISA Pathfinder is a science and technology demonstrator of the European Space Agency within the framework of its LISA mission, the latter aiming to be the first space-borne gravitational wave observatory. The payload of LISA Pathfinder is the so-called LISA Technology Package, which is designed to measure relative accelerations between two test masses in nominal free fall. The diagnostics subsystem consists of several modules, one of which is the magnetic diagnostics unit. Its main function is the assessment of the differential acceleration noise between the test masses due to magnetic effects. This subsystem is composed of two onboard coils intended to produce controlled magnetic fields at the location of the test masses. These magnetic fields couple with the remanent magnetic moment and susceptibility and produce forces and torques on the test masses. These, in turn, produce kinematic excursions of the test masses which are sensed by the onboard interferometer. We prove that adequately processing these exc...

  11. RPP Game Edukasi Pathfinding Adventures - Materi Sistem Koordinat - Kelas 8

    OpenAIRE

    Hidayatullah, Aulia Muslim

    2016-01-01

    Pathfinding Adventures bertujuan untuk membantu pemain dalam memahami konsep matematika kelas 8 mengenai sistem koordinat. Pada game ini pemain dapat berpetualang di area khusus untuk mencari dan menggambar peta dari hasil perjalanan dalam melaksanakan misi di setiap tingkatan permainan. Pemain diberikan akses kontrol pada game dalam format “Third Person” atau dari sudut pandang luar karakter pada permainan. Menyelesaikan tantangan-tantangan yang diberikan di setiap tingkatan ...

  12. Analysis of pathfinder SST algorithm for global and regional conditions

    Indian Academy of Sciences (India)

    Ajoy Kumar; P Minnett; G Podesta; R Evans; K Kilpatrick

    2000-12-01

    As part of the Pathfinder program developed jointly by National Aeronautics and Space Administration (NASA) and National Oceanic and Atmospheric Administration (NOAA) a large database of in situ sea surface temperature (SST) measurements coincident with satellite data is now available to the user community. The Pathfinder Matchup Database (PMDB) is a multi-year, multi-satellite collection of coincident measurements from the Advanced Very High Resolution Radiometer (AVHRR) and broadly distributed buoy data (matchups). This database allows the user community to test and validate new SST algorithms to improve the present accuracy of surface temperature measurements from satellites. In this paper we investigate the performance of a global Pathfinder algorithm to specific regional conditions. It is shown that for zenith angles less than 45°, the best-expected statistical discrepancy between satellite and buoy data is about ∼0.5 K. In general, the bias of the residuals (satellite - buoy) is negative in most regions, except in the North Atlantic and adjacent seas, where the residuals are always positive. A seasonal signal in SST residuals is observed in all regions and is strongest in the Indian Ocean. The channel-difference term used as a proxy for atmospheric water vapor correction is observed to be unresponsive for columnar water vapor values greater than 45 mm and high zenith angles. This unresponsiveness of the channels leads to underestimation of sea surface temperature from satellites in these conditions.

  13. LISA Pathfinder: First steps to observing gravitational waves from space

    Science.gov (United States)

    McNamara, Paul; LISA Pathfinder Collaboration

    2017-01-01

    With the first direct detection of gravitational waves a little over a year ago, the gravitational window to the Universe has been opened. The gravitational wave spectrum spans many orders of magnitude in frequency, with several of the most interesting astronomical sources emitting gravitational waves at frequencies only observable from space The European Space Agency (ESA) has been active in the field of space-borne gravitational wave detection for many years, and in 2013 selected the Gravitational Universe as the science theme for the third large class mission in the Cosmic Vision science programme. In addition, ESA took the step of developing the LISA Pathfinder mission to demonstrate the critical technologies required for a future mission. The goal of the LISA Pathfinder mission is to place a test body in free fall such that any external forces (acceleration) are reduced to levels lower than those expected from the passage of a gravitational wave LISA Pathfinder was launched on the 3rd December 2015 from the European Spaceport in Kourou, French Guiana. After a series of 6 apogee raising manoeuvres, the satellite left earth orbit, and travelled to its final science orbit around the first Sun-Earth Lagrange point (L1). Following a relatively short commissioning phase, science operations began on 1st March 2016. In the following 3 months over 100 experiments and over 1500hours of noise measurements have been performed, demonstrating that the observation of gravitational waves from space can be realised.

  14. Le temps mesurable, réversible, insaisissable ?

    CERN Document Server

    Fink, Martin; Leduc , Michèle

    2016-01-01

    Depuis l'Antiquité, la nature du temps a fasciné nombre de grands penseurs. Cet ouvrage expose ce que la physique est capable de dire aujourd'hui sur le sujet. La mesure du temps, ou plus exactement celle d'une durée, se fait grâce à des horloges atomiques dont l'exactitude peut atteindre une seconde sur plusieurs milliards d'années. Nous décrivons la façon dont s'effectue le transfert du temps qui permet la synchronisation d'horloges en différents points de la Terre ou de l'espace au milliardième de seconde près, ou même mieux. Les relativités, restreinte et générale, ont bouleversé notre conception du temps et ont un impact considérable sur certains problèmes de la vie quotidienne comme l'utilisation du GPS. On abandonne l'idée d'un temps absolu, le temps devient multiple et insaisissable, et peut-être même une illusion. Enfin la flèche du temps, ou l'irréversibilité, implique que les phénomènes physiques se déroulent toujours dans un sens déterminé, en relation avec la croissan...

  15. NASA Ocean Altimeter Pathfinder Project. Report 1; Data Processing Handbook

    Science.gov (United States)

    Koblinsky, C. J.; Beckley, Brian D.; Ray, Richard D.; Wang, Yan-Ming; Tsaoussi, Lucia; Brenner, Anita; Williamson, Ron

    1998-01-01

    The NOAA/NASA Pathfinder program was created by the Earth Observing System (EOS) Program Office to determine how satellite-based data sets can be processed and used to study global change. The data sets are designed to be long time-sedes data processed with stable calibration and community consensus algorithms to better assist the research community. The Ocean Altimeter Pathfinder Project involves the reprocessing of all altimeter observations with a consistent set of improved algorithms, based on the results from TOPEX/POSEIDON (T/P), into easy-to-use data sets for the oceanographic community for climate research. This report describes the processing schemes used to produce a consistent data set and two of the products derived f rom these data. Other reports have been produced that: a) describe the validation of these data sets against tide gauge measurements and b) evaluate the statistical properties of the data that are relevant to climate change. The use of satellite altimetry for earth observations was proposed in the early 1960s. The first successful space based radar altimeter experiment was flown on SkyLab in 1974. The first successful satellite radar altimeter was flown aboard the Geos-3 spacecraft between 1975 and 1978. While a useful data set was collected from this mission for geophysical studies, the noise in the radar measured and incomplete global coverage precluded ft from inclusion in the Ocean Altimeter Pathfinder program. This program initiated its analysis with the Seasat mission, which was the first satellite radar altimeter flown for oceanography.

  16. Symbolic PathFinder: Symbolic Execution of Java Bytecode

    Science.gov (United States)

    Pasareanu, Corina S.; Rungta, Neha

    2010-01-01

    Symbolic Pathfinder (SPF) combines symbolic execution with model checking and constraint solving for automated test case generation and error detection in Java programs with unspecified inputs. In this tool, programs are executed on symbolic inputs representing multiple concrete inputs. Values of variables are represented as constraints generated from the analysis of Java bytecode. The constraints are solved using off-the shelf solvers to generate test inputs guaranteed to achieve complex coverage criteria. SPF has been used successfully at NASA, in academia, and in industry.

  17. The LISA PathFinder DMU and Radiation Monitor

    CERN Document Server

    Canizares, Priscilla; Diaz--Aguilo, Marc; Garcia-Berro, Enrique; Gesa, Lluis; Gibert, Ferran; Grimani, Catia; Lloro, Ivan; Lobo, Alberto; Mateos, Ignacio; Nofrarias, Miquel; Ramos-Castro, Juan; Sanjuan, Josep; Sopuerta, Carlos F

    2010-01-01

    The LISA PathFinder DMU (Data Management Unit) flight model was formally accepted by ESA and ASD on 11 February 2010, after all hardware and software tests had been successfully completed. The diagnostics items are scheduled to be delivered by the end of 2010. In this paper we review the requirements and performance of this instrumentation, specially focusing on the Radiation Monitor and the DMU, as well as the status of their programmed use during mission operations, on which work is ongoing at the time of writing.

  18. Design Overview of the DM Radio Pathfinder Experiment

    OpenAIRE

    Silva-Feaver, Maximiliano; Chaudhuri, Saptarshi; Cho, Hsiao-Mei; Dawson, Carl; Graham, Peter; Irwin, Kent; Kuenstner, Stephen; Li, Dale; Mardon, Jeremy; Moseley, Harvey; Mule, Richard; Phipps, Arran; Rajendran, Surjeet; Steffen, Zach; Young, Betty

    2016-01-01

    We introduce the DM Radio, a dual search for axion and hidden photon dark matter using a tunable superconducting lumped-element resonator. We discuss the prototype DM Radio Pathfinder experiment, which will probe hidden photons in the 500 peV (100 kHz)-50 neV (10 MHz) mass range. We detail the design of the various components: the LC resonant detector, the resonant frequency tuning procedure, the differential SQUID readout circuit, the shielding, and the cryogenic mounting structure. We prese...

  19. Closed loop simulations of the thermal experiments in LISA Pathfinder

    CERN Document Server

    Gibert, Ferran; Karnesis, Nikolaos; Díaz-Aguiló, Marc; Mateos, Ignacio; Lobo, Alberto; Gesa, Lluís; Martín, Víctor; Lloro, Ivan

    2013-01-01

    The thermal experiments to be carried out onboard LISA Pathfinder (LPF) will provide essential information of the dependences of the instrument with respect to temperature variations. These thermal experiments must be modelled and simulated both to be validated for mission operations purposes and also to develop a data analysis tool able to characterise the temperature noise contribution to the instrument performance. Here we will present the models developed and the simulated signals for some of the experiments together with the corresponding interferometer readouts, the latter being computed by combining the thermal models with the global LTP (LISA Technology Package) simulator of the LTP Data Analysis team.

  20. Dynamic real-time hierarchical heuristic search for pathfinding.

    OpenAIRE

    Naveed, Munir; Kitchin, Diane E.; Crampton, Andrew

    2009-01-01

    Movement of Units in Real-Time Strategy (RTS) Games is a non-trivial and challenging task mainly due to three factors which are constraints on CPU and memory usage, dynamicity of the game world, and concurrency. In this paper, we are focusing on finding a novel solution for solving the pathfinding problem in RTS Games for the units which are controlled by the computer. The novel solution combines two AI Planning approaches: Hierarchical Task Network (HTN) and Real-Time Heuristic Search (RHS)....

  1. 77 FR 6554 - Zephyr Power Transmission, LLC; Pathfinder Power Transmission, LLC; Duke-American Transmission...

    Science.gov (United States)

    2012-02-08

    ... Energy Regulatory Commission Zephyr Power Transmission, LLC; Pathfinder Power Transmission, LLC; Duke... (Commission), 18 CFR 381.302, Zephyr Power Transmission, LLC (Zephyr), Pathfinder Power Transmission, LLC (PPT... to exercise its negotiated rate authority for Zephyr Power Transmission Project; (2) that...

  2. Mars Pathfinder. (Latest citations from the EI Compendex*Plus database)

    Science.gov (United States)

    1996-11-01

    The bibliography contains citations concerning the Mars pathfinder mission launch. Topics discuss instrumentation, altimetry, and previous Mars Observer mission data. Concepts and goals of the Mars pathfinder program are examined. (Contains 50-250 citations and includes a subject term index and title list.)

  3. Portable Tester Friction (PFT). Mesures du coefficient de frottement dynamique de revêtements de sol

    OpenAIRE

    Marchal, P.; Jacques, M.

    2014-01-01

    Le Portable Tester Friction (PFT) est un appareil destiné à mesurer le coefficient de frottement dynamique d’un revêtement de sol en laboratoire et sur site. Ce document décrit le protocole de mesure avec le PFT et les résultats de mesures effectuées sur un panel de quinze revêtements de sol de caractéristiques différentes (matériaux, états de surface) réalisées en présence de deux polluants (huile et solution d’eau). Le PFT présente une très bonne sensibilité et une très bonne répétabilité. ...

  4. Mesure optimale de tilt et déplacement d'un faisceau gaussien

    Science.gov (United States)

    Delaubert, V.; Treps, N.; Fabre, C.; Harb, C.; Lam, P. K.; Bachor, H.

    2006-10-01

    Nous réalisons une expérience de mesure optimale de petits déplacements d'un faisceau gaussien TEM{00}, basée sur une détection homodyne employant un oscillateur local TEM{10}. Nous montrons une amélioration de 56% du signal détecté par rapport à une détection à deux zones. Ce nouveau dispositif permet également de mesurer de façon optimale de petites valeurs de tilt, la quantité conjuguée du déplacement. Enfin, nous montrons que la compression du mode TEM{10} du faisceau incident permet une mesure de déplacement au delà de la limite quantique standard.

  5. Disentangling the magnetic force noise contribution in LISA Pathfinder

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; Gallegos, J.; García Marirrodriga, C.; Gerndt, R.; Gesa, L. I.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martín, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mendes, L.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    Magnetically-induced forces on the inertial masses on-board LISA Pathfinder are expected to be one of the dominant contributions to the mission noise budget, accounting for up to 40%. The origin of this disturbance is the coupling of the residual magnetization and susceptibility of the test masses with the environmental magnetic field. In order to fully understand this important part of the noise model, a set of coils and magnetometers are integrated as a part of the diagnostics subsystem. During operations a sequence of magnetic excitations will be applied to precisely determine the coupling of the magnetic environment to the test mass displacement using the on-board magnetometers. Since no direct measurement of the magnetic field in the test mass position will be available, an extrapolation of the magnetic measurements to the test mass position will be carried out as a part of the data analysis activities. In this paper we show the first results on the magnetic experiments during an end- to-end LISA Pathfinder simulation, and we describe the methods under development to map the magnetic field on-board.

  6. Processing TOVS Polar Pathfinder data using the distributed batch controller

    Science.gov (United States)

    Duff, James; Salem, Kenneth M.; Schweiger, Axel; Livny, Miron

    1997-09-01

    The distributed batch controller (DBC) supports scientific batch data processing. Batch jobs are distributed by the DBC over a collection of computing resources. Since these resources may be widely scattered the DBC is well suited for collaborative research efforts whose resources may not be centrally located. The DBC provides its users with centralized monitoring and control of distributed batch jobs. Version 1 of the DBC is currently being used by the TOVS Polar Pathfinder project to generate Arctic atmospheric temperature and humidity profiles. Profile generating jobs are distributed and executed by the DBC on workstation clusters located at several sites across the US. This paper describes the data processing requirements of the TOVS Polar Pathfinder project, and how the DBC is being used to meet them. It also describes Version 2 of the DBC. DBC V2 is implemented in Java, and utilizes a number of advanced Java features such as threads and remote method invocation. It incorporates a number of functional enhancements. These include a flexible mechanism supporting interoperation of the DBC with a wider variety of execution resources and an improved user interface.

  7. MESURE DE LA QUALITE DE LA DIVULGATION SOCIETALE DES ENTREPRISES FRANCAISES

    OpenAIRE

    Ben Rhouma, Amel

    2006-01-01

    International audience; Le propos de ce papier est de présenter quelques résultats empiriques concernant la mesure du niveau et de la qualité de la divulgation sociétale. Notre outil de mesure est une grille de codage similaire à celle de Wiseman (1982) et Cormier et Magnan (1999 et 2003) et adaptée au contexte légal et réglementaire français, les résultats montrent qu'il y a une progression dans le niveau et la qualité de divulgation sociétale des entreprises françaises.

  8. Qualification de l’instrumentation pour des mesures nanométriques

    CERN Document Server

    Bernard, E

    2009-01-01

    Prise en main de l’instrumentation dédiée aux mesures de vibrations dans le domaine du nanomètre et mise en service de nouveaux capteurs. Développement de l’acquisition des données sous Labview, et analyse des signaux dans le domaine fréquentiel sous Matlab.

  9. The LISA Pathfinder interferometry—hardware and system testing

    Science.gov (United States)

    Audley, H.; Danzmann, K.; García Marín, A.; Heinzel, G.; Monsky, A.; Nofrarias, M.; Steier, F.; Gerardi, D.; Gerndt, R.; Hechenblaikner, G.; Johann, U.; Luetzow-Wentzky, P.; Wand, V.; Antonucci, F.; Armano, M.; Auger, G.; Benedetti, M.; Binetruy, P.; Boatella, C.; Bogenstahl, J.; Bortoluzzi, D.; Bosetti, P.; Caleno, M.; Cavalleri, A.; Cesa, M.; Chmeissani, M.; Ciani, G.; Conchillo, A.; Congedo, G.; Cristofolini, I.; Cruise, M.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Fauste, J.; Ferraioli, L.; Fertin, D.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marirrodriga, C.; Gesa, L.; Gibert, F.; Giardini, D.; Grimani, C.; Grynagier, A.; Guillaume, B.; Guzmán, F.; Harrison, I.; Hewitson, M.; Hollington, D.; Hough, J.; Hoyland, D.; Hueller, M.; Huesler, J.; Jeannin, O.; Jennrich, O.; Jetzer, P.; Johlander, B.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mitchell, E.; Nicolini, D.; Nicolodi, D.; Pedersen, F.; Perreur-Lloyd, M.; Perreca, A.; Plagnol, E.; Prat, P.; Racca, G. D.; Rais, B.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Sanjuan, J.; Schulte, M.; Shaul, D.; Stagnaro, L.; Strandmoe, S.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tombolato, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Weber, W. J.; Zweifel, P.

    2011-05-01

    Preparations for the LISA Pathfinder mission have reached an exciting stage. Tests of the engineering model (EM) of the optical metrology system have recently been completed at the Albert Einstein Institute, Hannover, and flight model tests are now underway. Significantly, they represent the first complete integration and testing of the space-qualified hardware and are the first tests on an optical system level. The results and test procedures of these campaigns will be utilized directly in the ground-based flight hardware tests, and subsequently during in-flight operations. In addition, they allow valuable testing of the data analysis methods using the MATLAB-based LTP data analysis toolbox. This paper presents an overview of the results from the EM test campaign that was successfully completed in December 2009.

  10. Source-finding for the Australian Square Kilometre Array Pathfinder

    CERN Document Server

    Whiting, Matthew

    2012-01-01

    The Australian Square Kilometre Array Pathfinder (ASKAP) presents a number of challenges in the area of source finding and cataloguing. The data rates and image sizes are very large, and require automated processing in a high-performance computing environment. This requires development of new tools, that are able to operate in such an environment and can reliably handle large datasets. These tools must also be able to accommodate the different types of observations ASKAP will make: continuum imaging, spectral-line imaging, transient imaging. The ASKAP project has developed a source-finder known as Selavy, built upon the Duchamp source-finder (Whiting 2012). Selavy incorporates a number of new features, which we describe here. Since distributed processing of large images and cubes will be essential, we describe the algorithms used to distribute the data, find an appropriate threshold and search to that threshold and form the final source catalogue. We describe the algorithm used to define a varying threshold t...

  11. Bayesian statistics for the calibration of the LISA Pathfinder experiment

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martin, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mitchell, E.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    The main goal of LISA Pathfinder (LPF) mission is to estimate the acceleration noise models of the overall LISA Technology Package (LTP) experiment on-board. This will be of crucial importance for the future space-based Gravitational-Wave (GW) detectors, like eLISA. Here, we present the Bayesian analysis framework to process the planned system identification experiments designed for that purpose. In particular, we focus on the analysis strategies to predict the accuracy of the parameters that describe the system in all degrees of freedom. The data sets were generated during the latest operational simulations organised by the data analysis team and this work is part of the LTPDA Matlab toolbox.

  12. Acquiring multiple stars with the LINC-NIRVANA Pathfinder

    Science.gov (United States)

    Conrad, Albert R.; Arcidiacono, Carmelo; Baumeister, Harald; Bergomi, Maria; Bertram, Thomas; Berwein, Jürgen; Briegel, Florian; Farinato, Jacopo; Herbst, Tom; Hofferbert, Ralph; Kittmann, Frank; Kürster, Martin; Kopon, Derek; Marafatto, Luca; Norris, Mark; Ragazzoni, Roberto; Viotto, Valentina

    2014-08-01

    The LINC-NIRVANA Pathfinder1 (LN-PF), a ground-layer adaptive optics (AO) system recently commissioned at the Large Binocular Telescope (LBT), is one of 4 sensors that provide AO corrected images to the full LINC-NIRVANA instrument. With first light having taken place on November 17, 2013,2, 3 the core goals for the LN-PF have been accomplished. In this report, we look forward to one of the LN-PF extended goals. In particular, we review the acquisition mechanism required to place each of several star probes on its corresponding star in the target asterism. For emerging AO systems in general, co-addition of light from multiple stars stands as one of several methods being pursued to boost sky coverage. With 12 probes patrolling a large field of view (an annulus 6-arcminutes in diameter), the LN-PF will provide a valuable testbed to verify this method.

  13. The case for testing MOND using LISA Pathfinder

    CERN Document Server

    Magueijo, Joao

    2011-01-01

    We quantify the potential for testing MOdified Newtonian Dynamics (MOND) with LISA Pathfinder (LPF), should a saddle point flyby be incorporated into the mission. We forecast the expected signal to noise ratio (SNR) for a variety of instrument noise models and trajectories past the saddle. For standard theoretical parameters the SNR reaches middle to high double figures even with modest assumptions about instrument performance and saddle approach. Obvious concerns, like systematics arising from LPF self-gravity, or the Newtonian background, are examined and shown not to be a problem. We also investigate the impact of a negative observational result upon the free-function determining the theory. We demonstrate that, if Newton's gravitational constant is constrained not be re-normalized by more than a few percent, only very contrived MONDian free-functions would survive a negative result. Finally we scan the structure of all proposed relativistic MONDian theories. We conclude that only the Einstein-Aether formu...

  14. Prediction and Validation of Mars Pathfinder Hypersonic Aerodynamic Data Base

    Science.gov (United States)

    Gnoffo, Peter A.; Braun, Robert D.; Weilmuenster, K. James; Mitcheltree, Robert A.; Engelund, Walter C.; Powell, Richard W.

    1998-01-01

    Postflight analysis of the Mars Pathfinder hypersonic, continuum aerodynamic data base is presented. Measured data include accelerations along the body axis and axis normal directions. Comparisons of preflight simulation and measurements show good agreement. The prediction of two static instabilities associated with movement of the sonic line from the shoulder to the nose and back was confirmed by measured normal accelerations. Reconstruction of atmospheric density during entry has an uncertainty directly proportional to the uncertainty in the predicted axial coefficient. The sensitivity of the moment coefficient to freestream density, kinetic models and center-of-gravity location are examined to provide additional consistency checks of the simulation with flight data. The atmospheric density as derived from axial coefficient and measured axial accelerations falls within the range required for sonic line shift and static stability transition as independently determined from normal accelerations.

  15. LISA Pathfinder: First steps to observing gravitational waves from space

    Science.gov (United States)

    LISA Pathfinder Collaboration

    2017-05-01

    LISA Pathfinder, the European Space Agency’s technology demonstrator mission for future spaceborne gravitational wave observatories, was launched on 3 December 2015, from the European space port of Kourou, French Guiana. After a short duration transfer to the final science orbit, the mission has been gathering science data since. This data has allowed the science community to validate the critical technologies and measurement principle for low frequency gravitational wave detection and thereby confirming the readiness to start the next generation gravitational wave observatories, such as LISA. This paper will briefly describe the mission, followed by a description of the science operations highlighting the performance achieved. Details of the various experiments performed during the nominal science operations phase can be found in accompanying papers in this volume.

  16. Exploring MEDLINE space with random indexing and pathfinder networks.

    Science.gov (United States)

    Cohen, Trevor

    2008-11-06

    The integration of disparate research domains is a prerequisite for the success of the translational science initiative. MEDLINE abstracts contain content from a broad range of disciplines, presenting an opportunity for the development of methods able to integrate the knowledge they contain. Latent Semantic Analysis (LSA) and related methods learn human-like associations between terms from unannotated text. However, their computational and memory demands limits their ability to address a corpus of this size. Furthermore, visualization methods previously used in conjunction with LSA have limited ability to define the local structure of the associative networks LSA learns. This paper explores these issues by (1) processing the entire MEDLINE corpus using Random Indexing, a variant of LSA, and (2) exploring learned associations using Pathfinder Networks. Meaningful associations are inferred from MEDLINE, including a drug-disease association undetected by PUBMED search.

  17. State Space Modelling and Data Analysis Exercises in LISA Pathfinder

    Science.gov (United States)

    Nofrarias, M.; Antonucci, F.; Armano, M.; Audley, H.; Auger, G.; Benedetti, M.; Binetruy, P.; Bogenstahl, J.; Bortoluzzi, D.; Brandt, N.; Caleno, M.; Cavalleri, A.; Congedo, G.; Cruise, M.; Danzmann, K.; De Marchi, F.; Diaz-Aguilo, M.; Diepholz, I.; Dixon, G.; Dolesi, R.; Dunbar, N.; Fauste, J.; Ferraioli, L.; Ferroni, V.; Fichter, W.; Fitzsimons, E.; Freschi, M.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gibert, F.; Giardini, D.; Grimani, C.; Grynagier, A.; Guzmán, F.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hoyland, D.; Hueller, M.; Huesler, J.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Korsakova, N.; Killow, C.; Llamas, X.; Lloro, I.; Lobo, A.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martin, V.; Mateos, I.; McNamara, P.; Mendes, J.; Mitchell, E.; Nicolodi, D.; Perreur-Lloyd, M.; Plagnol, E.; Prat, P.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Schleicher, A.; Shaul, D.; Sopuerta, C. F.; Sumner, T. J.; Taylor, A.; Texier, D.; Trenkel, C.; Tu, H. B.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Ziegler, T.; Zweifel, P.

    2013-01-01

    LISA Pathfinder is a mission planned by the European Space Agency (ESA) to test the key technologies that will allow the detection of gravitational waves in space. The instrument on-board, the LISA Technology package, will undergo an exhaustive campaign of calibrations and noise characterisation campaigns in order to fully describe the noise model. Data analysis plays an important role in the mission and for that reason the data analysis team has been developing a toolbox which contains all the functionality required during operations. In this contribution we give an overview of recent activities, focusing on the improvements in the modelling of the instrument and in the data analysis campaigns performed both with real and simulated data.

  18. State space modelling and data analysis exercises in LISA Pathfinder

    CERN Document Server

    Nofrarias, M; Armano, M; Audley, H; Auger, G; Benedetti, M; Binetruy, P; Bogenstahl, J; Bortoluzzi, D; Bosetti, P; Brandt, N; Caleno, M; Cañizares, P; Cavalleri, A; Cesa, M; Chmeissani, M; Conchillo, A; Congedo, G; Cristofolin, I; Cruise, M; Danzmann, K; De Marchi, F; Diaz-Aguilo, M; Diepholz, I; Dixon, G; Dolesi, R; Dunbar, N; Fauste, J; Ferraioli, L; Fichter, V Ferroni W; Fitzsimons, E; Freschi, M; Marin, A García; Marirrodriga, C García; Gesa, R Gerndt L; Gibert, F; Giardini, D; Grimani, C; Grynagier, A; Guillaume, B; Guzmán, F; Harrison, I; Heinzel, G; Hernández, V; Hewitson, M; Hollington, D; Hough, J; Hoyland, D; Hueller, M; Huesler, J; Jennrich, O; Jetzer, P; Johlander, B; Killow, C; Llamas, X; Lloro, I; Lobo, A; Maarschalkerweerd, R; Madden, S; Mance, D; Mateos, I; McNamara, P W; Mendes, J; Mitchell, E; Monsky, A; Nicolini, D; Nicolodi, D; Pedersen, F; Perreur-Lloyd, M; Plagnol, E; Prat, P; Racca, G D; Ramos-Castro, J; Reiche, J; Perez, J A Romera; Robertson, D; Rozemeijer, H; Sanjuan, J; Schleicher, A; Schulte, M; Shaul, D; Stagnaro, L; Strandmoe, S; Steier, F; Sumner, T J; Taylor, A; Texier, D; Trenkel, C; Vitale, H-B Tu S; Wanner, G; Ward, H; Waschke, S; Wass, P; Weber, W J; Ziegler, T; Zweifel, P

    2013-01-01

    LISA Pathfinder is a mission planned by the European Space Agency to test the key technologies that will allow the detection of gravitational waves in space. The instrument on-board, the LISA Technology package, will undergo an exhaustive campaign of calibrations and noise characterisation campaigns in order to fully describe the noise model. Data analysis plays an important role in the mission and for that reason the data analysis team has been developing a toolbox which contains all the functionalities required during operations. In this contribution we give an overview of recent activities, focusing on the improvements in the modelling of the instrument and in the data analysis campaigns performed both with real and simulated data.

  19. The Australian SKA Pathfinder: operations management and user engagement

    Science.gov (United States)

    Harvey-Smith, Lisa

    2016-07-01

    This paper describes the science operations model for the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. ASKAP is a radio interferometer currently being commissioned in Western Australia. It will be operated by a dedicated team of observatory staff with the support of telescope monitoring, control and scheduling software. These tools, as well as the proposal tools and data archive will enable the telescope to operate with little direct input from the astronomy user. The paper also discusses how close engagement with the telescope user community has been maintained throughout the ASKAP construction and commissioning phase, leading to positive outcomes including early input into the design of telescope systems and a vibrant early science program.

  20. Drill/borescope System for the Mars Polar Pathfinder

    Science.gov (United States)

    Paige, D. A.; Wood, S. E.; Vasavada, A. R.

    1993-01-01

    The primary goals of the Mars Polar Pathfinder (MPP) Discovery Mission are to characterize the composition and structure of Mars' north polar ice cap, and to determine whether a climate record may be preserved in layers of ice and dust. The MPP would land as close as possible to the geographic north pole of Mars and use a set of instruments similar to those used by glaciologists to study polar ice caps on Earth: a radar sounder, a drill/borescope system, and a thermal probe. The drill/borescope system will drill approximately 50 cm into the surface and image the sides of the hole at 10 micron resolution for compositional and stratigraphic analysis. Several uncertainties have guided the development of this instrument, and they are discussed.

  1. Discrete derivative estimation in LISA Pathfinder data reduction

    CERN Document Server

    Ferraioli, Luigi; Vitale, Stefano

    2009-01-01

    Data analysis for the LISA Technology package (LTP) experiment to be flown aboard the LISA Pathfinder mission requires the solution of the system dynamics for the calculation of the force acting on the test masses (TMs) starting from interferometer position data. The need for a solution to this problem has prompted us to implement a discrete time domain derivative estimator suited for the LTP experiment requirements. We first report on the mathematical procedures for the definition of two methods; the first based on a parabolic fit approximation and the second based on a Taylor series expansion. These two methods are then generalized and incorporated in a more general class of five point discrete derivative estimators. The same procedure employed for the second derivative can be applied to the estimation of the first derivative and of a data smoother allowing defining a class of simple five points estimators for both. The performances of three particular realization of the five point second derivative estimat...

  2. Differential measurement of the earth's magnetic field by nuclear magnetic resonance; Mesure differentielle du champ magnetique terrestre par resonance magnetique nucleaire

    Energy Technology Data Exchange (ETDEWEB)

    Robach, F. [Commissariat a l' Energie Atomique, 38 - Grenoble (France). Centre d' Etudes Nucleaires

    1967-07-01

    MNR transducers using proton dynamic polarisation allows to convert into a phase measurement any variation of the earth magnetic field. There exist several versions of the instrument corresponding to various models of MNR transducers, which the author analyses in detail, devoting an important place to influence of their alignment with respect to the earth's magnetic field. The sensibility obtained is of one hundredth of a gamma over a bandwidth of (0-0,1 Hz). - This instrument is designed for measuring field gradients in airborne magnetic surveying, for detecting nearly magnetic anomalies, and for distinguishing between nearly and distant magnetic phenomena. (author) [French] L'emploi de capteurs, bases sur la resonance magnetique nucleaire des protons en presence de polarisation dynamique, permet de traduire une difference de champ magnetique terrestre en une mesure de phase. L'appareil existe sous plusieurs versions avec des capteurs de modeles differents dont l'auteur fait une analyse detaillee en accordant une part importante a l'influence de l'orientation des capteurs par rapport au champ magnetique terrestre. La sensibilite est de 1/100 {gamma} pour une bande passante de (0 - 0,1 Hz). Cet appareil s'applique a la mesure du gradient en prospection magnetique aeroportee, a la detection d'anomalies magnetiques proches, a la differentiation d'effets magnetiques proches et lointains. (auteur)

  3. NOAA Climate Data Record (CDR) of AVHRR Polar Pathfinder (APP) Cryosphere

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This NOAA Climate Data Record (CDR) contains the AVHRR Polar Pathfinder (APP) product. APP is a fundamental CDR comprised of calibrated and navigated AVHRR channel...

  4. CRED REA Algal Assessments at Pathfinder Reef, Marianas Archipelago in 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — As part of Rapid Ecological Assessments (REA), Twelve quadrats were sampled along 2 consecutively-placed, 25m transect lines, conducted at 2 sites at Pathfinder Reef...

  5. Narrative report Pathfinder National Wildlife Refuge: September, October, November, December, 1963

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1963. The report begins by...

  6. Pathfinder National Wildlife Refuge, Narrative report: September, October, November, December, 1956

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1956. The report begins by...

  7. NOAA Climate Data Record (CDR) of AVHRR Polar Pathfinder Extended (APP-X) Cryosphere

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — NOAA Climate Data Record (CDR) of the extended AVHRR Polar Pathfinder (APP-x) cryosphere contains 19 geophysical variables over the Arctic and Antarctic for the...

  8. Narrative report Pathfinder National Wildlife Refuge: September, October, November, December, 1961

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1961. The report begins by...

  9. Narrative report Pathfinder National Wildlife Refuge: September, October, November, December, 1962

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1962. The report begins by...

  10. Narrative report Pathfinder National Wildlife Refuge: May, June, July, August, 1963

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1963. The report begins by summarizing the...

  11. Narrative report Pathfinder National Wildlife Refuge: January, February, March, April, 1961

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1961. The report begins by summarizing...

  12. Narrative report Pathfinder National Wildlife Refuge: May, June, July, August, 1962

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1962. The report begins by summarizing the...

  13. Pathfinder National Wildlife Refuge Narrative report: January, February, March, April, 1958

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1958. The report begins by summarizing...

  14. Pathfinder National Wildlife Refuge, Narrative report: May, June, July, August, 1958

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1958. The report begins by summarizing the...

  15. Pathfinder National Wildlife Refuge Narrative report: January, February, March, April, 1959

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1959. The report begins by summarizing...

  16. Pathfinder National Wildlife Refuge Narrative report: January, February, March, April, 1960

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1960. The report begins by summarizing...

  17. Narrative report Pathfinder National Wildlife Refuge: May, June, July, August, 1961

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1961. The report begins by summarizing the...

  18. Pathfinder National Wildlife Refuge, Narrative report: May, June, July, August, 1960

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1960. The report begins by summarizing the...

  19. Pathfinder National Wildlife Refuge, Narrative report: September, October, November, December, 1957

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1957. The report begins by...

  20. Pathfinder National Wildlife Refuge, Narrative report: May, June, July, August, 1959

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1959. The report begins by summarizing the...

  1. Pathfinder National Wildlife Refuge Narrative report: September, October, November, December, 1959

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1959. The report begins by...

  2. Pathfinder National Wildlife Refuge, Narrative report: January, February, March, April, 1957

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1957. The report begins by summarizing...

  3. Narrative report Pathfinder National Wildlife Refuge: January, February, March, April, 1962

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1962. The report begins by summarizing...

  4. Pathfinder National Wildlife Refuge, Narrative report: May, June, July, August, 1957

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1957. The report begins by summarizing the...

  5. Pathfinder National Wildlife Refuge Narrative report: September, October, November, December, 1960

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1960. The report begins by...

  6. Pathfinder National Wildlife Refuge, Narrative report: May, June, July, August, 1956

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from May through August of 1956. The report begins by summarizing the...

  7. Narrative report Pathfinder National Wildlife Refuge: January, February, March, April, 1963

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from January through April of 1963. The report begins by summarizing...

  8. Pathfinder National Wildlife Refuge Narrative report: September, October, November, December, 1958

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This narrative report for Pathfinder National Wildlife Refuge outlines Refuge accomplishments from September through December of 1958. The report begins by...

  9. [Bamforth, Hutton Lake and Pathfinder National Wildlife Refuges background and operating statement

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This document is a background on Bamforth, Hutton Lake and Pathfinder National Wildlife Refuges in northwestern Colorado. Part I is solely background information...

  10. HI Observations of two New Dwarf Galaxies: Pisces A & B with the SKA Pathfinder KAT-7

    CERN Document Server

    Carignan, C; Lucero, D M; Randriamampandry, T H; Jarrett, T H; Oosterloo, T A; Tollerud, E J

    2016-01-01

    Context. Pisces A & Pisces B are the only two galaxies found via optical imaging and spectroscopy out of 22 HI clouds identified in the GALFAHI survey as dwarf galaxy candidates. Aims. Derive the HI content and kinematics of Pisces A & B. Methods. Aperture synthesis HI observations using the seven dish Karoo Array Telescope (KAT-7), which is a pathfinder instrument for MeerKAT, the South African precursor to the mid-frequency Square Kilometre Array (SKA-MID). Results. The small rotation velocities detected of ~5 km/sec and ~10 km/sec in Pisces A & B respectively, and their HI content show that they are really dwarf irregular galaxies (dIrr). Despite that small rotation component, it is more the random motions ~9-11 km/sec that provide most of the gravitational support, especially in the outer parts. The study of their kinematics, especially the strong gradients of random motions, suggest that those two dwarf galaxies are not yet in equilibrium. Conclusions. These HI rich galaxies may be indicative...

  11. Motoneuron axon pathfinding errors in zebrafish: Differential effects related to concentration and timing of nicotine exposure

    Energy Technology Data Exchange (ETDEWEB)

    Menelaou, Evdokia; Paul, Latoya T. [Department of Biological Sciences, Louisiana State University, Baton Rouge, LA 70803 (United States); Perera, Surangi N. [Joseph J. Zilber School of Public Health, University of Wisconsin — Milwaukee, Milwaukee, WI 53205 (United States); Svoboda, Kurt R., E-mail: svobodak@uwm.edu [Department of Biological Sciences, Louisiana State University, Baton Rouge, LA 70803 (United States); Joseph J. Zilber School of Public Health, University of Wisconsin — Milwaukee, Milwaukee, WI 53205 (United States)

    2015-04-01

    Nicotine exposure during embryonic stages of development can affect many neurodevelopmental processes. In the developing zebrafish, exposure to nicotine was reported to cause axonal pathfinding errors in the later born secondary motoneurons (SMNs). These alterations in SMN axon morphology coincided with muscle degeneration at high nicotine concentrations (15–30 μM). Previous work showed that the paralytic mutant zebrafish known as sofa potato exhibited nicotine-induced effects onto SMN axons at these high concentrations but in the absence of any muscle deficits, indicating that pathfinding errors could occur independent of muscle effects. In this study, we used varying concentrations of nicotine at different developmental windows of exposure to specifically isolate its effects onto subpopulations of motoneuron axons. We found that nicotine exposure can affect SMN axon morphology in a dose-dependent manner. At low concentrations of nicotine, SMN axons exhibited pathfinding errors, in the absence of any nicotine-induced muscle abnormalities. Moreover, the nicotine exposure paradigms used affected the 3 subpopulations of SMN axons differently, but the dorsal projecting SMN axons were primarily affected. We then identified morphologically distinct pathfinding errors that best described the nicotine-induced effects on dorsal projecting SMN axons. To test whether SMN pathfinding was potentially influenced by alterations in the early born primary motoneuron (PMN), we performed dual labeling studies, where both PMN and SMN axons were simultaneously labeled with antibodies. We show that only a subset of the SMN axon pathfinding errors coincided with abnormal PMN axonal targeting in nicotine-exposed zebrafish. We conclude that nicotine exposure can exert differential effects depending on the levels of nicotine and developmental exposure window. - Highlights: • Embryonic nicotine exposure can specifically affect secondary motoneuron axons in a dose-dependent manner.

  12. Pathfinding with Hard Constraints : Mobile Systems and Real Time Strategy Games Combined

    OpenAIRE

    Erdtman, Samuel; Fylling, Johan

    2008-01-01

    There is an abundance of pathfinding solutions, but are any of those solutions suitable for usage in a real time strategy (RTS) game designed for mobile systems with limited processing and storage capabilities (such as the Nintendo DS, PSP, cellular phones, etc.)? The RTS domain puts great requirements on the pathfinding mechanics used in the game; in the form of de- mands on responsiveness and path optimality. Furthermore, the Nintendo DS, and its portable, distant relatives, bring hard con-...

  13. Mesure et retroaction sur un qubit multi-niveaux en electrodynamique quantique en circuit non lineair

    Science.gov (United States)

    Boissonneault, Maxime

    L'electrodynamique quantique en circuit est une architecture prometteuse pour le calcul quantique ainsi que pour etudier l'optique quantique. Dans cette architecture, on couple un ou plusieurs qubits supraconducteurs jouant le role d'atomes a un ou plusieurs resonateurs jouant le role de cavites optiques. Dans cette these, j'etudie l'interaction entre un seul qubit supraconducteur et un seul resonateur, en permettant cependant au qubit d'avoir plus de deux niveaux et au resonateur d'avoir une non-linearite Kerr. Je m'interesse particulierement a la lecture de l'etat du qubit et a son amelioration, a la retroaction du processus de mesure sur le qubit de meme qu'a l'etude des proprietes quantiques du resonateur a l'aide du qubit. J'utilise pour ce faire un modele analytique reduit que je developpe a partir de la description complete du systeme en utilisant principalement des transfprmations unitaires et une elimination adiabatique. J'utilise aussi une librairie de calcul numerique maison permettant de simuler efficacement l'evolution du systeme complet. Je compare les predictions du modele analytique reduit et les resultats de simulations numeriques a des resultats experimentaux obtenus par l'equipe de quantronique du CEASaclay. Ces resultats sont ceux d'une spectroscopie d'un qubit supraconducteur couple a un resonateur non lineaire excite. Dans un regime de faible puissance de spectroscopie le modele reduit predit correctement la position et la largeur de la raie. La position de la raie subit les decalages de Lamb et de Stark, et sa largeur est dominee par un dephasage induit par le processus de mesure. Je montre que, pour les parametres typiques de l'electrodynamique quantique en circuit, un accord quantitatif requiert un modele en reponse non lineaire du champ intra-resonateur, tel que celui developpe. Dans un regime de forte puissance de spectroscopie, des bandes laterales apparaissent et sont causees par les fluctuations quantiques du champ electromagnetique

  14. The semantic pathfinder: using an authoring metaphor for generic multimedia indexing.

    Science.gov (United States)

    Snoek, Cees G M; Worring, Marcel; Geusebroek, Jan-Mark; Koelma, Dennis C; Seinstra, Frank J; Smeulders, Arnold W M

    2006-10-01

    This paper presents the semantic pathfinder architecture for generic indexing of multimedia archives. The semantic pathfinder extracts semantic concepts from video by exploring different paths through three consecutive analysis steps, which we derive from the observation that produced video is the result of an authoring-driven process. We exploit this authoring metaphor for machine-driven understanding. The pathfinder starts with the content analysis step. In this analysis step, we follow a data-driven approach of indexing semantics. The style analysis step is the second analysis step. Here, we tackle the indexing problem by viewing a video from the perspective of production. Finally, in the context analysis step, we view semantics in context. The virtue of the semantic pathfinder is its ability to learn the best path of analysis steps on a per-concept basis. To show the generality of this novel indexing approach, we develop detectors for a lexicon of 32 concepts and we evaluate the semantic pathfinder against the 2004 NIST TRECVID video retrieval benchmark, using a news archive of 64 hours. Top ranking performance in the semantic concept detection task indicates the merit of the semantic pathfinder for generic indexing of multimedia archives.

  15. Dispositif de mesure calorimétrique des pertes dans les condensateurs de puissance

    Science.gov (United States)

    Seguin, B.; Gosse, J. P.

    1997-02-01

    A calorimetric technique is used to measure the power losses in capacitors. The power dissipated in the component is measured as the difference between the heat powers delivered by a temperature regulation when the capacitor is energetized or not. The original feature of the apparatus lies in the use of the isothermal calorimetry and in the measurement of an electrical power, in condradistinction with previous and dissatisfacting attempts based on the measurement of a temperature increase. The result is an improvement of the accuracy and sensibility of the apparatus which can be used to determine the equivalent series resistance of capacitors having very low losses. Measurements realized on a polypropylene capacitor and a sinusoidal applied voltage have allowed us to separate the ohmic losses from the dielectric ones and to study their variations with temperature. Une technique de calorimétrie isotherme est appliquée à la mesure des pertes électriques dans les condensateurs. La puissance calorifique dissipée par le composant est mesurée comme la différence des puissances de chauffe délivrées par une régulation de température quand le condensateur est hors tension ou sous tension. L'originalité du dispositif réside dans l'utilisation du principe de calorimétrie isotherme et dans la nature de la grandeur physique mesurée qui est une puissance électrique alors que les tentatives antérieures de mesures calorimétriques reposaient sur la mesure d'une élévation de température. Il en résulte une amélioration de la précision et de la sensibilité de ce type d'appareillage qui peut être employé pour caractériser la résistance série équivalente des condensateurs à très faibles pertes. Une série de mesures, réalisée sur un condensateur au polypropylène soumis à une tension sinusoïdale, a permis de séparer les pertes ohmiques des pertes diélectriques et d'étudier leurs variations avec la température.

  16. Une methode simple pour la mesure de l'evapotranspiration reelle a l'echelle de la parcelle

    OpenAIRE

    1981-01-01

    Après avoir passé en revue les différentes méthodes de mesure de l’évapotranspiration réelle, qu’il s’agisse des méthodes directes telles que la pesée ou la mesure du stock en eau du sol ou des méthodes indirectes telles que la méthode du rapport de Bowen et la méthode aérodynamique combinée, on développe une méthode de mesure simple cherchant à allier les avantages de la méthode du rapport de Bowen (deux niveaux de mesure dans l’air seulement) et ceux de la méthode aérodynamique combinée...

  17. Souci du social et action publique sur mesure

    Directory of Open Access Journals (Sweden)

    Bertrand Ravon

    2008-10-01

    Full Text Available L’engagement dans la lutte contre les problèmes sociaux s’est transformé. Avec l’individualisation et la territorialisation du traitement public des problèmes sociaux, se pose de plus en plus nettement la question d’une action publique de proximité, intersubjective. Mais plutôt que de renvoyer immédiatement les raisons de cette action publique sur mesure à une critique de la psychologisation des rapports sociaux ou du déclin des institutions, il s’agit de l’analyser comme une expérience publique, avec son lot d’actions et d’affects, de convictions et d’inquiétudes, de ressources et de préoccupations. La notion de souci s’impose alors pour tenir ce double mouvement de l’engagement, entre agir et subir, des épreuves qui nous conduisent dans l’action aux attentes qui nous y maintiennent. À partir de plusieurs exemples de formation de problèmes sociaux, l’article décline alors le souci des acteurs dans deux directions. D’une part, le souci de soi est analysé comme un engagement public au sens d’un travail d’orientation de soi dans un monde incertain via la reprise d’expériences sociales négatives. D’autre part, le souci commun est envisagé comme une « communauté de charge », c’est-à-dire comme un collectif d’action publique fondé non pas à partir de propriétés communes mais à partir d’affects partagés.“Concern” in the social sphere and public action adapted to the client: singular and critical public experience of social problemsCommitment in the struggle against social problems has changed. Along with the individualisation and territorial decentralisation of the public treatment of social problems, the question of very local and intersubjective public action has come more and more into focus. But rather than immediately relegating the reasons for this tailor-made version of social action to a critique of the increasing influence of psychological methods in social relations

  18. Comment mesurer correctement la PA chez les patients hémodialysés?

    OpenAIRE

    VANDERWECKENE, Pauline; Saint-Remy, Annie; Krzesinski, Jean-Marie

    2016-01-01

    Objectifs : Le contrôle de la pression artérielle (PA) chez le patient hémodialysé (HD) est un enjeu majeur en raison des résultats controversés sur les risques cardiovasculaires qui y sont associés. Cependant, la mesure de la PA dans cette population est difficile à appréhender au vu de sa grande variabilité. L’exactitude des mesures péridialytiques (enregistrées dans l’unité d’HD pendant la séance) est souvent remise en question. L’objectif de notre étude est d’établir la contribution et l...

  19. La mesure de la pression artérielle : écueils et chausse-trapes

    OpenAIRE

    Rorive, Georges; Dubois, Bernard; Saint-Remy, Annie

    2002-01-01

    La mesure de la pression artérielle est probablement l'acte médical le plus souvent réalisé et certainement un des moins fiables. L'introduction de la mesure ambulatoire de la pression artérielle a permis d'identifier l'importance de l'effet consultatio et, par là, de définir l'hypertension de "la blouse blanche". Celle-ci se définit comme une pression artérielle pathologique à la consultation et strictement normale en dehors. Si on la définit de cette manière, cette pathologie ne s'accompagn...

  20. Rectangle expansion A*pathfinding for grid maps

    Institute of Scientific and Technical Information of China (English)

    Zhang An; Li Chong; Bi Wenhao

    2016-01-01

    Search speed, quality of resulting paths and the cost of pre-processing are the principle evaluation metrics of a pathfinding algorithm. In this paper, a new algorithm for grid-based maps, rectangle expansion A* (REA*), is presented that improves the performance of A* significantly. REA*explores maps in units of unblocked rectangles. All unnecessary points inside the rectangles are pruned and boundaries of the rectangles (instead of individual points within those boundaries) are used as search nodes. This makes the algorithm plot fewer points and have a much shorter open list than A*. REA*returns jump and grid-optimal path points, but since the line of sight between jump points is protected by the unblocked rectangles, the resulting path of REA*is usually better than grid-optimal. The algorithm is entirely online and requires no offline pre-processing. Experi-mental results for typical benchmark problem sets show that REA*can speed up a highly optimized A* by an order of magnitude and more while preserving completeness and optimality. This new algorithm is competitive with other highly successful variants of A*.

  1. Detection and Characterization of Micrometeoroids with LISA Pathfinder

    CERN Document Server

    Thorpe, James Ira; Trigo-Rodriguez, Josep

    2015-01-01

    The Solar System contains a population of dust and small particles originating from asteroids, comets, and other bodies. These particles have been studied using a number of techniques ranging from in-situ satellite detectors to analysis of lunar microcraters to ground-based observations of zodiacal light. In this paper, we describe an approach for using the LISA Pathfinder (LPF) mission as an instrument to detect and characterize the dynamics of dust particles in the vicinity of Earth-Sun L1. Launching in late 2015, LPF is a dedicated technology demonstrator mission that will validate several key technologies for a future space-based gravitational-wave observatory. The primary science instrument aboard LPF is a precision accelerometer which we show will be capable of sensing discrete momentum impulses as small as $4\\times 10^{-8}\\,\\textrm{N}\\cdot\\textrm{s}$. We then estimate the rate of such impulses resulting from impacts of micrometeoroids based on standard models of the micrometeoroid environment in the in...

  2. Model Checking Real Time Java Using Java PathFinder

    Science.gov (United States)

    Lindstrom, Gary; Mehlitz, Peter C.; Visser, Willem

    2005-01-01

    The Real Time Specification for Java (RTSJ) is an augmentation of Java for real time applications of various degrees of hardness. The central features of RTSJ are real time threads; user defined schedulers; asynchronous events, handlers, and control transfers; a priority inheritance based default scheduler; non-heap memory areas such as immortal and scoped, and non-heap real time threads whose execution is not impeded by garbage collection. The Robust Software Systems group at NASA Ames Research Center has JAVA PATHFINDER (JPF) under development, a Java model checker. JPF at its core is a state exploring JVM which can examine alternative paths in a Java program (e.g., via backtracking) by trying all nondeterministic choices, including thread scheduling order. This paper describes our implementation of an RTSJ profile (subset) in JPF, including requirements, design decisions, and current implementation status. Two examples are analyzed: jobs on a multiprogramming operating system, and a complex resource contention example involving autonomous vehicles crossing an intersection. The utility of JPF in finding logic and timing errors is illustrated, and the remaining challenges in supporting all of RTSJ are assessed.

  3. Slope Morphology of Twin Peaks, Mars Pathfinder Landing Site

    Science.gov (United States)

    Hobbs, Steven; Paine, Colin; Clarke, Jon; Caprarelli, Graziella

    2010-05-01

    Development of slope form over time has long been a concern of geomorphologists, although recently this concern has been moved to slope processes rather than form. There are two basic approaches. The first is theoretical, involving modeling of different types and rates of processes, and calculation of results in terms of slope evolution over time. Comparisons with real-life slopes can follow this approach [1], [2]. The second, inductive, approach involves field measurements to test ideas about slope evolution starting from the assumption that observed slopes represent different stages of an essentially similar evolution [3]. Space is substituted for time, and a number of slopes, assumed to be of increasing age, are measured and placed in an evolutionary sequence (e.g. [4], [5], [6]). [5] showed that slope angles are modally distributed, with the modal angles controlled by the materials (regolith) of which the slopes are formed, and by the processes operating on them. Data can be obtained directly from field work or from digital elevation models (DEM) derived from remote sensing investigations [7]. DEMs are particularly useful to study inaccessible planets, such as Mars, where on site observations are restricted to only a few landing sites. Here we present a study of slopes on the Twin Peaks, two small hills located 780 m north and 910 m south of the Mars Pathfinder landing site at the mouth of the Ares and Tiu flood channels. The presence of streamlined hills, jumbled surfaces and conglomerates suggested the region was modified by massive flooding 1.8 - 3.5 billion years ago [8], [9]. The streamlined forms and terraces of the Twin Peaks were taken to indicate catastrophic flood conditions that were believed to be prevalent in the area [8]. It was also suggested that the northernmost peak was topped by floodwater, causing its flatter appearance. Other researchers postulated alternative geomorphological origins for the features observed at the Pathfinder landing site

  4. MONDian three-body predictions for LISA Pathfinder

    Energy Technology Data Exchange (ETDEWEB)

    Bevis, Neil; Magueijo, Joao [Theoretical Physics, Blackett Laboratory, Imperial College, London, SW7 2BZ (United Kingdom); Trenkel, Christian; Kemble, Steve, E-mail: n.bevis@imperial.ac.u, E-mail: magueijo@ic.ac.u, E-mail: Christian.Trenkel@astrium.eads.ne [Astrium Ltd, Gunnels Wood Road, Stevenage SG1 2AS (United Kingdom)

    2010-11-07

    In previous work it was shown that modified Newtonian dynamics (MOND) theories predict anomalously strong tidal stresses near the saddle points of the Newtonian gravitational potential. An analytical examination of the saddle between two bodies revealed a linear and a nonlinear solution, valid for the outer and inner regions. Here we present a numerical algorithm for solving the MOND equations. We check the code against the two-body analytical solutions and explore the region transitioning between them. We then develop a realistic model for the MONDian effects on the saddles of the Sun-Earth-Moon system (including further sources is straightforward). For the Sun-Earth saddle we find that the two-body results are almost unchanged, with corrections increasing from full to new Moon. In contrast, the Moon saddle is an intrinsically three-body problem, but we numerically find a recipe for adapting the two-body solution to this case, by means of a suitable rescaling and axis reorientation. We explore possible experimental scenarios for LISA Pathfinder and the prospect of a visit to the saddle(s) at the end of the mission. Given the chaotic nature of the orbits, awareness of the full range of the possibilities is crucial for a realistic prediction. We conclude that even with very conservative assumptions on the impact parameter, the accelerometers are abundantly sensitive to vindicate or rule out the theory.

  5. Optical Performances of Slewing Mirror Telescope for UFFO-Pathfinder

    CERN Document Server

    Jeong, S; Nam, J W; Park, I H; Kim, S -W; Choi, H S; Grossan, B; Hermann, I; Jung, A; Kim, Y W; Kim, J E; Linder, E V; Lee, J; Lim, H; Min, K W; Na, G W; Nam, K H; Panasyuk, M I; Smoot, G F; Svelitov, S; Suh, Y D; Vedenken, N; Yashin, I; Zhao, M H

    2011-01-01

    The Ultra-Fast Flash Observatory-Pathfinder (UFFO-P) is to be launched onboard Lomonosov spacecraft in November 2011. It is to measure early UV/Optical photons from Gamma Ray Bursts (GRBs). Slewing Mirror Telescope (SMT) is one of two instruments designed for detection of UV/Optical images of the GRBs. SMT is a Ritchey-Chr\\'etien telescope of 100 mm in diameter with a motorized slewing mirror at the entrance providing 17\\times17 arcmin2 in Field of View (FOV) and 4 arcsec in pixel resolution. Its sky coverage can be further expanded up to 35 degrees in FOV by tilting a motorized slewing mirror. All mirrors were fabricated to about RMS 0.02 waves in wave front error (WFE) and 84.7% (in average reflectivity) over 200nm~650nm range. SMT was aligned to RMS 0.05 waves in WFE (test wavelength 632.8nm). From the static gravity test result, SMT optics system is expected to survive during launch. The technical details of SMT assembly and laboratory performance test results are reported.

  6. Polar Geophysics Products Derived from AVHRR: The "AVHRR Polar Pathfinder

    Science.gov (United States)

    Maslanik, James; Fowler, Charles; Scambos, Theodore

    1999-01-01

    This NOAA/NASA Pathfinder effort was established to locate, acquire, and process Advanced Very High Resolution Radiometer (AVHRR) imagery into geo-located and calibrated radiances, cloud masks, surface clear-sky broadband albedo, clear-sky skin temperatures, satellite viewing times, and viewing and solar geometry for the, high-latitude portions of the northern and southern hemispheres (all area north of 48N and south of 53S). AVHRR GAC data for August 1981 - July 1998 were acquired, with some gaps remaining, and processed into twice-daily 5-km grids, with some products also provided at 25-km resolution. AVHRR LAC data for 3.5 years of coverage in the northern hemisphere and 2.75 years of coverage in the southern hemisphere were processed into 1.25-km grids for the same suite of products. The resulting data sets are presently being transferred to the National Snow and Ice Data Center (NSIDC) for archiving and distribution. Using these data, researchers now have at their disposal an extensive AVHRR data set for investigations of high-latitude processes. In addition, the data lend themselves to development and testing of algorithms. The products are particularly relevant for climate research and algorithm development as applied to relatively long time periods and large areas.

  7. Antenna Deployment for a Pathfinder Lunar Radio Observatory

    Science.gov (United States)

    MacDowall, Robert J.; Minetto, F. A.; Lazio, T. W.; Jones, D. L.; Kasper, J. C.; Burns, J. O.; Stewart, K. P.; Weiler, K. W.

    2012-01-01

    A first step in the development of a large radio observatory on the moon for cosmological or other astrophysical and planetary goals is to deploy a few antennas as a pathfinder mission. In this presentation, we describe a mechanism being developed to deploy such antennas from a small craft, such as a Google Lunar X-prize lander. The antenna concept is to deposit antennas and leads on a polyimide film, such as Kapton, and to unroll the film on the lunar surface. The deployment technique utilized is to launch an anchor which pulls a double line from a reel at the spacecraft. Subsequently, the anchor is set by catching on the surface or collecting sufficient regolith. A motor then pulls in one end of the line, pulling the film off of its roller onto the lunar surface. Detection of a low frequency cutoff of the galactic radio background or of solar radio bursts by such a system would determine the maximum lunar ionospheric density at the time of measurement. The current design and testing, including videos of the deployment, will be presented. These activities are funded in part by the NASA Lunar Science Institute as an activity of the Lunar University Network for Astrophysical Research (LUNAR) consortium. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

  8. SURVEY

    DEFF Research Database (Denmark)

    SURVEY er en udbredt metode og benyttes inden for bl.a. samfundsvidenskab, humaniora, psykologi og sundhedsforskning. Også uden for forskningsverdenen er der mange organisationer som f.eks. konsulentfirmaer og offentlige institutioner samt marketingsafdelinger i private virksomheder, der arbejder...... med surveys. Denne bog gennemgår alle surveyarbejdets faser og giver en praktisk indføring i: • design af undersøgelsen og udvælgelse af stikprøver, • formulering af spørgeskemaer samt indsamling og kodning af data, • metoder til at analysere resultaterne...

  9. Mesures magnétiques du dipôle BHN 45 pour le projet AD

    CERN Document Server

    Cornuet, D; CERN. Geneva. SPS and LEP Division

    1999-01-01

    La machine AC (Antiproton Collector) transformée en machine de décélérationd'antiprotons est appelée AD (Antiproton Decelerator). Pour vérifierle comportement de la machine à basse énergie et pendant la décélération, des mesures magnétiques ont été entreprises sur l'un des dipôles, le BHN 45.

  10. Experimental and numerical study of the mars pathfinder vehicle; Etude experimentale et numerique sur le mars pathfinder

    Energy Technology Data Exchange (ETDEWEB)

    Bur, R.; Benay, R.; Chanetz, B.; Galli, A.; Pot, T. [Office National d' Etudes et de Recherches Aerospatiales (ONERA), Dept. Fundamental and Experimental Aerodynamics, 92 - Chatillon (France); Hollis, B.; Moss, J. [Aerothermodynamics Branch, NASA Langley Research Center Hampton, Virginia (United States)

    2002-07-01

    An experimental and numerical study on the Mars Pathfinder aero-shell vehicle has been carried out in the framework of an agreement between ONERA and NASA. The experimental work was performed in the ONERA R5Ch hypersonic wind tunnel. Flow-field visualizations and heat-flux measurements along the model have been obtained. Numerical simulations have been performed at ONERA with the RANS solver NASCA and at NASA with a DSMC code. The flow-field structure is correctly reproduced by both computations. The location of the bow shock is well predicted, as well as the expansion waves emanating from the end of the fore-body cone. Both computations also predict the same extension of the separation bubble in the base flow region of the model. Measured and calculated heat-flux distributions along the model have been compared. Both computations give similar results, excepted on the prediction of the heat-flux level on the after-body cone. But computations over-predict the measured heat-flux values on the fore-body and the sting of the model: the value of the stagnation point is overestimated of 28% and the averaged sting level of 35%. (authors)

  11. The Pathfinder Testbed: Exploring Techniques for Achieving Precision Radial Velocities in the Near-Infrared

    CERN Document Server

    Ramsey, Larry; Redman, Stephen; Bender, Chad; Roy, Arpita; Zonak, Stephanie; Sigurdsson, Steinn; Wolszczan, Alex

    2010-01-01

    The Penn State Pathfinder is a prototype warm fiber-fed Echelle spectrograph with a Hawaii-1 NIR detector that has already demonstrated 7-10 m/s radial velocity precision on integrated sunlight. The Pathfinder testbed was initially setup for the Gemini PRVS design study to enable a systematic exploration of the challenges of achieving high radial velocity precision in the near-infrared, as well as to test possible solutions to these calibration challenges. The current version of the Pathfinder has an R3 echelle grating, and delivers a resolution of R~50,000 in the Y, J or H bands of the spectrum. We will discuss the on sky-performance of the Pathfinder during an engineering test run at the Hobby Eberly Telescope as well the results of velocity observations of M dwarfs. We will also discuss the unique calibration techniques we have explored, like Uranium-Neon hollow cathode lamps, notch filter, and modal noise mitigation to enable high precision radial velocity observation in the NIR. The Pathfinder is a proto...

  12. LISA and LISA PathFinder, the endeavour to detect low frequency GWs

    CERN Document Server

    Araujo, H; Chmeissani, M; Conchillo, A; García-Berro, E; Grimani, C; Hajdas, W; Lobo, A; Martínez, L; Nofrarias, M; Ortega, J A; Puigdengoles, C; Ramos-Castro, J; Sanjuan, J; Wass, P; Xirgu, X; Araujo, Henrique; Boatella, Cesar; Chmeissani, Mokhtar; Conchillo, Aleix; Garcia-Berro, Enrique; Grimani, Catia; Hajdas, Wojtek; Lobo, Alberto; Martinez, Lluis; Nofrarias, Miquel; Ortega, Jose Antonio; Puigdengoles, Carles; Ramos-Castro, Juan; Sanjuan, Josep; Wass, Peter; Xirgu, Xevi

    2006-01-01

    This is a review about LISA and its technology demonstrator, LISA PathFinder. We first describe the conceptual problems which need to be overcome in order to set up a working interferometric detector of low frequency Gravitational Waves (GW), then summarise the solutions to them as currently conceived by the LISA mission team. This will show that some of these solutions require new technological abilities which are still under development, and which need proper test before being fully implemented. LISA PathFinder (LPF) is the the testbed for such technologies. The final part of the paper will address the ideas and concepts behind the PathFinder as well as their impact on LISA.

  13. Preliminary Findings of the Photovoltaic Cell Calibration Experiment on Pathfinder Flight 95-3

    Science.gov (United States)

    Vargas-Aburto, Carlos

    1997-01-01

    The objective of the photovoltaic (PV) cell calibration experiment for Pathfinder was to develop an experiment compatible with an ultralight UAV to predict the performance of PV cells at AM0, the solar spectrum in space, using the Langley plot technique. The Langley plot is a valuable technique for this purpose and requires accurate measurements of air mass (pressure), cell temperature, solar irradiance, and current-voltage(IV) characteristics with the cells directed normal to the direct ray of the sun. Pathfinder's mission objective (95-3) of 65,000 ft. maximum altitude, is ideal for performing the Langley plot measurements. Miniaturization of electronic data acquisition equipment enabled the design and construction of an accurate and light weight measurement system that meets Pathfinder's low payload weight requirements.

  14. Apc1-mediated antagonism of Wnt/beta-catenin signaling is required for retino-tectal pathfinding in the zebrafish.

    NARCIS (Netherlands)

    Paridaen, J.T.M.; Danesin, C.; Elas, A.T.; van de Water, S.G.P.; Houart, C.; Zivkovic, D.

    2009-01-01

    The tumor suppressor Apc1 is an intracellular antagonist of the Wnt/beta-catenin pathway. We examined the effects of an Apc1 loss-of-function mutation on retino-tectal axon pathfinding in zebrafish. In apc mutants, the retina is disorganized and optic nerves portray pathfinding defects at the optic

  15. Apc1-mediated antagonism of Wnt/beta-catenin signaling is required for retino-tectal pathfinding in the zebrafish.

    NARCIS (Netherlands)

    Paridaen, J.T.M.; Danesin, C.; Elas, A.T.; van de Water, S.G.P.; Houart, C.; Zivkovic, D.

    2009-01-01

    The tumor suppressor Apc1 is an intracellular antagonist of the Wnt/beta-catenin pathway. We examined the effects of an Apc1 loss-of-function mutation on retino-tectal axon pathfinding in zebrafish. In apc mutants, the retina is disorganized and optic nerves portray pathfinding defects at the optic

  16. LabINRS. Mesures en laboratoire du coefficient de frottement dynamique de revêtements de sol

    OpenAIRE

    Marchal, P.; Jacques, M.

    2014-01-01

    Le LabINRS est un banc d’essai de laboratoire destiné à mesurer le coefficient de frottement dynamique d’un revêtement de sol. Ce document décrit le protocole de mesures avec le LabINRS et les résultats de mesures effectuées sur un panel de quinze revêtements de sol de caractéristiques différentes (matériaux, états de surface) réalisées en présence de deux polluants (huile et solution d’eau). Le LabINRS présente une sensibilité élevée et une très bonne répétabilité. Ces résultats ont été comp...

  17. Réduction de bruit quantique spatiale et mesures de petits déplacements en optique

    Science.gov (United States)

    Treps, N.; Maître, A.; Fabre, C.; Andersen, U.; Buchler, B.; Lame, P. K.; Bachor, H. A.

    2002-06-01

    L'étude des images optiques au niveau quantique nécessite de prendre en compte la structure multimode transverse de la lumière. Dans le cas particulier d'une mesure de position d'un faisceau lumineux effectuée par un détecteur à deux zone, on montre qu'il est nécessaire, si on veut améliorer la précision des mesures en réduisant le bruit quantique de la lumière, d'utiliser deux modes transverses. Nous présentons la première réalisation expérimentale d'une réduction de bruit spatiale, ce qui nous permet ensuite d'effectuer des mesures de petits déplacements sous la limite quantique standard.

  18. La mesure en éducation, un outil au service du politique

    OpenAIRE

    Agulhon, Catherine

    2009-01-01

    La statistique scolaire prétend rendre compte des processus complexes qui travaillent les institutions. Les organismes internationaux incitent les États à produire ces éléments de mesure, de comparaison et de mise en concurrence des systèmes scolaires, plus encore ces quinze dernières années. Chaque État a cependant construit un système d’information qui correspond aux formes d’évaluation qu’il veut donner à son projet éducatif. En France, ce système centralisé et très productif vise le suivi...

  19. Quelle mesure des effets du travail sur la santé ?

    OpenAIRE

    Bercot, Régine

    2012-01-01

    Nous envisagerons la maladie comme un processus engagé en vue d'une adaptation à un nouvel équilibre et la santé, non comme une absence de maladie, mais comme un processus de construction du bien être engageant le cadre social et les individus. Nous interrogerons la question de la mesure de la santé au travail en nous centrant sur l'enquête Sumer. Le travail est potentiellement générateur de bien être et de souffrance. Après avoir rappelé les grandes lignes de construction de cette enquête no...

  20. Development of Slewing Mirror Telescope Optical System for the UFFO-pathfinder

    DEFF Research Database (Denmark)

    Jeong, S.; Nam, J.W.; Ahn, K.-B.

    2013-01-01

    The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chrétien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin2 in Field of View and ...

  1. Slewing Mirror Telescope and the Data-Acquisition System for the UFFO-Pathfinder

    DEFF Research Database (Denmark)

    Lim, H.; Ahmad, S.; Barrillon, P.

    2013-01-01

    The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understanding. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst A...

  2. Observation of early photons from gamma-ray bursts with the Lomonosov / UFFO-pathfinder

    DEFF Research Database (Denmark)

    Jeong, S.; Brandt, Søren; Budtz-Jørgensen, Carl

    2014-01-01

    UFFO-pathfinder is a pioneering space mission to observe the early evolution of Gamma-ray Bursts using a fast slewing strategy. It consists of the Slewing Mirror Telescope, for rapid pointing at UV/optical wavelengths and the UFFO Burst Alert and Trigger Telescope. It has a total weight of ~ 20 k...

  3. Do Integrated Children's Services Improve Children's Outcomes?: Evidence from England's Children's Trust Pathfinders

    Science.gov (United States)

    O'Brien, Margaret; Bachmann, Max O.; Jones, Natalia R.; Reading, Richard; Thoburn, June; Husbands, Chris; Shreeve, Ann; Watson, Jacqueline

    2009-01-01

    Thirty-five children's trust pathfinders, local cross-sector partnerships, were introduced across England in 2003 to promote greater integration in children's services. Using administrative performance data, this paper tracks yearly trends in child service outputs and child well-being outcomes from 1997 to 2004 in these local areas, including the…

  4. Effective pathfinding for four-wheeled robot based on combining Theta* and hybrid A* algorithms

    Directory of Open Access Journals (Sweden)

    Віталій Геннадійович Михалько

    2016-07-01

    Full Text Available Effective pathfinding algorithm based on Theta* and Hybrid A* algorithms was developed for four-wheeled robot. Pseudocode for algorithm was showed and explained. Algorithm and simulator for four-wheeled robot were implemented using Java programming language. Algorithm was tested on U-obstacles, complex maps and for parking problem

  5. A Strategy to Characterize the LISA-Pathfinder Cold Gas Thruster System

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; Gallegos, J.; Garcia Marirrodriga, C.; Gerndt, R.; Gesa, L. I.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martin, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mendes, L.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    The cold gas micro-propulsion system that will be used during the LISA-Pathfinder mission will be one of the most important component used to ensure the "free-fall" of the enclosed test masses. In this paper we present a possible strategy to characterize the effective direction and amplitude gain of each of the 6 thrusters of this system.

  6. Global Climate Change Pathfinder: A Guide to Information Resources. Second Edition.

    Science.gov (United States)

    Pintozzi, Chestalene; Jones, Douglas E.

    This pathfinder is a guide to scientific and technical aspects of global climate change including meteorological and climatological aspects; biological, agricultural, and public policy implications; and the chemical processes involved. Sources are arranged by type of publication and include: (1) 10 reference sources; (2) 12 bibliographies; (3) 44…

  7. LINC-NIRVANA Pathfinder: testing the next generation of wave front sensors at LBT

    Science.gov (United States)

    Conrad, Albert R.; Arcidiacono, Carmelo; Baumeister, Harald; Bergomi, Maria; Bertram, Thomas; Berwein, Juergen; Biddick, Chris; Bizenberger, Peter; Brangier, Matthieu; Briegel, Florian; Brunelli, Alessandro; Brynnel, Joar; Busoni, Lorenzo; Cushing, Norm; De Bonis, Fulvio; De La Pena, Michele; Esposito, Simone; Farinato, Jacopo; Fini, Luca; Green, Richard F.; Herbst, Tom; Hofferbert, Ralph; Kittmann, Frank; Kuerster, Martin; Laun, Werner; Meschke, Daniel; Mohr, Lars; Pavlov, Aleksei; Pott, Jorg-Uwe; Puglisi, Alfio; Ragazzoni, Roberto; Rakich, Andrew; Rohloff, Ralf-Rainer; Trowitzsch, Jan; Viotto, Valentina; Zhang, Xianyu

    2012-07-01

    LINC-NIRVANA will employ four wave front sensors to realize multi-conjugate correction on both arms of a Fizeau interferometer for LBT. Of these, one of the two ground-layer wave front sensors, together with its infrared test camera, comprise a stand-alone test platform for LINC-NIRVANA. Pathfinder is a testbed for full LINC-NIRVANA intended to identify potential interface problems early in the game, thus reducing both technical, and schedule, risk. Pathfinder will combine light from multiple guide stars, with a pyramid sensor dedicated to each star, to achieve ground-layer AO correction via an adaptive secondary: the 672-actuator thin shell at the LBT. The ability to achieve sky coverage by optically coadding light from multiple stars has been previously demonstrated; and the ability to achieve correction with an adaptive secondary has also been previously demonstrated. Pathfinder will be the first system at LBT to combine both of these capabilities. Since reporting our progress at A04ELT2, we have advanced the project in three key areas: definition of specific goals for Pathfinder tests at LBT, more detail in the software design and planning, and calibration. We report on our progress and future plans in these three areas, and on the project overall.

  8. Optimal path-finding through mental exploration based on neural energy field gradients.

    Science.gov (United States)

    Wang, Yihong; Wang, Rubin; Zhu, Yating

    2017-02-01

    Rodent animal can accomplish self-locating and path-finding task by forming a cognitive map in the hippocampus representing the environment. In the classical model of the cognitive map, the system (artificial animal) needs large amounts of physical exploration to study spatial environment to solve path-finding problems, which costs too much time and energy. Although Hopfield's mental exploration model makes up for the deficiency mentioned above, the path is still not efficient enough. Moreover, his model mainly focused on the artificial neural network, and clear physiological meanings has not been addressed. In this work, based on the concept of mental exploration, neural energy coding theory has been applied to the novel calculation model to solve the path-finding problem. Energy field is constructed on the basis of the firing power of place cell clusters, and the energy field gradient can be used in mental exploration to solve path-finding problems. The study shows that the new mental exploration model can efficiently find the optimal path, and present the learning process with biophysical meaning as well. We also analyzed the parameters of the model which affect the path efficiency. This new idea verifies the importance of place cell and synapse in spatial memory and proves that energy coding is effective to study cognitive activities. This may provide the theoretical basis for the neural dynamics mechanism of spatial memory.

  9. A "door-to-door" path-finding approach for indoor navigation

    NARCIS (Netherlands)

    Liu, L.; Zlatanova, S.

    2011-01-01

    Indoor navigation is gaining an increasing interest among researchers in many domains. In many cases users need to orient quickly in complex environments, which is not always the target of current routing algorithms. The paper reviews current indoor path-finding approaches and discusses some of the

  10. On the warm nearshore bias in Pathfinder monthly SST products over Eastern Boundary upwelling systems

    CSIR Research Space (South Africa)

    Dufois, F

    2012-01-01

    Full Text Available , and Benguela Upwelling Systems. This warm bias could at least partly explain the cold bias often found in numerical models of coastal upwelling. The last release of Pathfinder (version 5.2, September 2011) clearly improved the bias found on the previous...

  11. First in...Last Out: History of the U.S. Army Pathfinder (1942-2011)

    Science.gov (United States)

    2014-05-21

    assault in to a large, egg shaped area that extended between Niscemi and Gela, on Sicily’s southern shores. However, the turbulence of war began to...height of 30 feet. In a matter of seconds the Pathfinders had rappelled down dangling ropes into the area, and scrambled into the cover of the trees on

  12. Simulation and template generation for LISA Pathfinder Data Analysis

    Science.gov (United States)

    Rais, Boutheina; Grynagier, Adrien; Diaz-Aguiló, Marc; Armano, Michele

    The LISA PathFinder (LPF) mission is a technology demonstration mission which aims at testing a number of critical technical challenges that the future LISA (Gravitational wave detection in space) mission will face: LPF can be seen as a complex laboratory experiment in space. It is therefore critical to be able to define which measurements and which actuations will be applied during the scientific part of the mission. The LISA Technology Package (LTP), part of ESA's hardware contribution to LPF, outlines hence the importance of developing an appropriate simulation tool in order to test these strate-gies before launch and to analyse the dynamical behaviour of the system during the mission. The detailed model of the simulation can be used in an off-line mode for further planning: cor-rect estimation of timeline priorities, risk factors, duty cycles, data analysis readiness. The Lisa Technology Package Data Analysis (LTPDA) team has developed an object-oriented MATLAB toolbox for general case of data analysis needs. However, to meet specific needs of LPF mis-sion, a template generation tool has been developed. It provides a recognizable data pattern, avoiding the risk of missing the model during mission's analysis. The aim of the template generator tool is to provide tools to analyse LTP system modeled in State Space Model (SSM). The SSM class, the aim of this poster, includes this tools within the LTPDA toolbox. It can be used to generate the time-domain response for any given actuation and/or noise, the frequency response using bode diagrams and the steady state of the system. It allows the user to project noises on system outputs to get spectra of outputs for given input noises spectra. This class is sufficiently general to be used with a variety of systems once the SSM of the system is provided in the library. Furthermore, one of the main objectives of the data analysis for LPF (the estimation of different parameters of the system), can be achieved by a new

  13. Modeling to Mars: a NASA Model Based Systems Engineering Pathfinder Effort

    Science.gov (United States)

    Phojanamongkolkij, Nipa; Lee, Kristopher A.; Miller, Scott T.; Vorndran, Kenneth A.; Vaden, Karl R.; Ross, Eric P.; Powell, Bobby C.; Moses, Robert W.

    2017-01-01

    The NASA Engineering Safety Center (NESC) Systems Engineering (SE) Technical Discipline Team (TDT) initiated the Model Based Systems Engineering (MBSE) Pathfinder effort in FY16. The goals and objectives of the MBSE Pathfinder include developing and advancing MBSE capability across NASA, applying MBSE to real NASA issues, and capturing issues and opportunities surrounding MBSE. The Pathfinder effort consisted of four teams, with each team addressing a particular focus area. This paper focuses on Pathfinder team 1 with the focus area of architectures and mission campaigns. These efforts covered the timeframe of February 2016 through September 2016. The team was comprised of eight team members from seven NASA Centers (Glenn Research Center, Langley Research Center, Ames Research Center, Goddard Space Flight Center IV&V Facility, Johnson Space Center, Marshall Space Flight Center, and Stennis Space Center). Collectively, the team had varying levels of knowledge, skills and expertise in systems engineering and MBSE. The team applied their existing and newly acquired system modeling knowledge and expertise to develop modeling products for a campaign (Program) of crew and cargo missions (Projects) to establish a human presence on Mars utilizing In-Situ Resource Utilization (ISRU). Pathfinder team 1 developed a subset of modeling products that are required for a Program System Requirement Review (SRR)/System Design Review (SDR) and Project Mission Concept Review (MCR)/SRR as defined in NASA Procedural Requirements. Additionally, Team 1 was able to perform and demonstrate some trades and constraint analyses. At the end of these efforts, over twenty lessons learned and recommended next steps have been identified.

  14. Developpement de mesures non destructives, par ondes ultrasonores, d'epaisseurs de fronts de solidification dans les reacteurs metallurgiques

    Science.gov (United States)

    Floquet, Jimmy

    Dans les cuves d'electrolyse d'aluminium, le milieu de reaction tres corrosif attaque les parois de la cuve, ce qui diminue leur duree de vie et augmente les couts de production. Le talus, qui se forme sous l'effet des pertes de chaleur qui maintiennent un equilibre thermique dans la cuve, sert de protection naturelle a la cuve. Son epaisseur doit etre controlee pour maximiser cet effet. Advenant la resorption non voulue de ce talus, les degats generes peuvent s'evaluer a plusieurs centaines de milliers de dollars par cuve. Aussi, l'objectif est de developper une mesure ultrasonore de l'epaisseur du talus, car elle serait non intrusive et non destructive. La precision attendue est de l'ordre du centimetre pour des mesures d'epaisseurs comprenant 2 materiaux, allant de 5 a 20 cm. Cette precision est le facteur cle permettant aux industriels de controler l'epaisseur du talus de maniere efficace (maximiser la protection des parois tout en maximisant l'efficacite energetique du procede), par l'ajout d'un flux thermique. Cependant, l'efficacite d'une mesure ultrasonore dans cet environnement hostile reste a demontrer. Les travaux preliminaires ont permis de selectionner un transducteur ultrasonore a contact ayant la capacite a resister aux conditions de mesure (hautes temperatures, materiaux non caracterises...). Differentes mesures a froid (traite par analyse temps-frequence) ont permis d'evaluer la vitesse de propagation des ondes dans le materiau de la cuve en graphite et de la cryolite, demontrant la possibilite d'extraire l'information pertinente d'epaisseur du talus in fine. Fort de cette phase de caracterisation des materiaux sur la reponse acoustique des materiaux, les travaux a venir ont ete realises sur un modele reduit de la cuve. Le montage experimental, un four evoluant a 1050 °C, instrumente d'une multitude de capteurs thermique, permettra une comparaison de la mesure intrusive LVDT a celle du transducteur, dans des conditions proches de la mesure

  15. NOAA Climate Data Record (CDR) of Reflectance from AVHRR Pathfinder Atmospheres - Extended (PATMOS-x), Version 5.2

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This dataset has been superseded by Version 5.3. The Pathfinder Atmospheres - Extended (PATMOS-x) Reflectance data contain derived atmospheric variables from the...

  16. 4 km NODC/RSMAS AVHRR Pathfinder v.5.0 Sea Surface Temperature (SST) Climatologies (1985-2001)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The 4 km Pathfinder effort at the National Oceanic and Atmospheric Administration (NOAA) National Oceanographic Data Center (NODC) and the University of Miami's...

  17. Arapaho National Wildlife Refuge also Bamforth, Hutton Lake and Pathfinder National Wildlife Refuges: Annual narrative report: Calendar year 1991

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 1991 calendar year. The...

  18. NOAA Climate Data Record (CDR) of Cloud Properties from AVHRR Pathfinder Atmospheres - Extended (PATMOS-x), Version 5.3

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This NOAA Climate Data Record (CDR) of cloud products was produced by the University of Wisconsin using the AVHRR Pathfinder Atmospheres - Extended (PATMOS-X)...

  19. NOAA Climate Data Record (CDR) of Sea Surface Temperature (SST) from AVHRR Pathfinder, Version 5.2

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The AVHRR Pathfinder Version 5.2 Sea Surface Temperature data set (PFV52) is a collection of global, twice-daily 4km sea surface temperature data produced in a...

  20. Annual narrative report: Calendar year 2000: Arapaho National Wildlife Refuge, Bamforth, Hutton Lake, Morenson Lake and Pathfinder National Wildlife Refuges

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, Morenson Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 2000...

  1. Discovery of HI gas in a young radio galaxy at $z = 0.44$ using the Australian SKA Pathfinder

    CERN Document Server

    Allison, J R; Moss, V A; Whiting, M T; Hunstead, R W; Pracy, M B; Curran, S J; Croom, S M; Glowacki, M; Morganti, R; Shabala, S S; Zwaan, M A; Allen, G; Amy, S; Axtens, P; Ball, L; Bannister, K W; Barker, S; Bateman, T; Beresford, R; Bell, M E; Bock, D; Bolton, R; Bowen, M; Boyle, B; Braun, R; Broadhurst, S; Brodrick, D; Brooks, K; Brothers, M; Brown, A; Bunton, J D; Cantrall, C; Carrad, G; Chapman, J; Cheng, W; Chippendale, A P; Chung, Y; Cooray, F; Cornwell, T; Davis, E; de Souza, L; DeBoer, D; Diamond, P; Edwards, P; Ekers, R; Feain, I; Ferris, D; Forsyth, R; Gough, R; Grancea, A; Gupta, N; Guzman, J C; Hampson, G; Harvey-Smith, L; Haskins, C; Hay, S; Hayman, D B; Heywood, I; Hotan, A W; Hoyle, S; Humphreys, B; Indermuehle, B T; Jacka, C; Jackson, C; Jackson, S; Jeganathan, K; Johnston, S; Joseph, J; Kendall, R; Kesteven, M; Kiraly, D; Koribalski, B; Leach, M; Lenc, E; Lensson, E; Li, L; Mackay, S; Macleod, A; Maher, T; Marquarding, M; Marvil, J; McClure-Griffiths, N; McConnell, D; Mickle, S; Mirtschin, P; Norris, R; Neuhold, S; Ng, A; O'Sullivan, J; Pathikulangara, J; Pearce, S; Phillips, C; Popping, A; Qiao, R Y; Reynolds, J E; Rispler, A; Roberts, P; Roxby, D; Sault, R J; Schinckel, A; Serra, P; Shaw, R; Shields, M; Shimwell, T; Storey, M; Sweetnam, T; Troup, E; Turner, B; Tuthill, J; Tzioumis, A; Voronkov, M A; Westmeier, T; Wilson, C; Wilson, T; Wormnes, K; Wu, X

    2015-01-01

    We report the discovery of a new 21cm HI absorption system using commissioning data from the Boolardy Engineering Test Array (BETA) of the Australian Square Kilometre Array Pathfinder (ASKAP). Using the 711.5-1015.5MHz band of ASKAP we were able to conduct a blind search for the 21cm line in a continuous redshift range between $z =$ 0.4-1.0, which has, until now, remained largely unexplored. The absorption line, detected at $z = 0.44$ towards the GHz-peaked spectrum radio source PKSB1740$-$517, is confirmed by optical spectroscopy, using the Gemini South telescope, to be intrinsic to the early-type host galaxy. We detect a broad component at 0.2 per cent of the continuum, demonstrating ASKAP's excellent capability for performing a future wide-field survey for HI absorption at these redshifts. The [OIII] and [OI] emission lines in the Gemini spectrum are broad and have double-peaked structures, pointing to outflowing ionised gas. Archival data from the XMM-Newton satellite exhibit an absorbed X-ray spectrum th...

  2. Mesure du rayonnement naturel pour la modélisation de la température des organes : application aux fruits

    OpenAIRE

    Marquier, André; Adam, Boris; Guilioni, Lydie; Saudreau, Marc; Chelle, Michaël; Sinoquet, Herve

    2009-01-01

    Cet article présente une expérimentation mise en place dans un projet innovant du département Environnement et agronomie (EA). Nous développons, plus particulièrement les principes de la mesure du rayonnement naturel à l’aide d’un bilanmètre de chez Kipp & Zonen : les capteurs qui le constituent, les grandeurs mesurées et les précautions à prendre lors de son utilisation notamment dans le domaine de l’infrarouge thermique. Ensuite nous montrons l’intérêt de telles mesures lors de la validatio...

  3. Mesure ambulatoire de la pression artérielle, son utilité en pratique quotidienne

    OpenAIRE

    Krzesinski, Jean-Marie

    1994-01-01

    Si la nécessité du traitement de l'hypertension artérielle est un fait accepté de façon universelle, la question à propos des niveaux de pression artérielle qui méritent une intervention reste débattue. Cette difficulté trouve son origine dans une telle variabilité de la pression artérielle que les mesures au cabinet de consultation représentent seulement une vue limitée de son réel profil sur 24 heures. Le développement d'enregistreurs portatifs de la pression artérielle par méthode non i...

  4. MESURE NON INVASIVE DU DÉBIT AORTIQUE PAR VOIE OESOPHAGIÈNNE

    OpenAIRE

    Lavandier, B.; Cathignol, D.; Muchada, R.; Fady, J.; Birer, A.

    1990-01-01

    Depuis plusieurs années nous avons montré la faisabilité et l'intérêt clinique de la débitmétrie aortique par voie oesophagienne. Une amélioration importante de cette méthode a été apportée par le développement d'un nouveau type de débitmètre associant un imageur T.M. et un vélocimètre Doppler à émission pulsée. Afin de pouvoir mesurer simultanément et de façon continue le diamètre de l'aorte et la vitesse du flux sanguin aussi bien chez l'adulte que chez l'enfant (à l'aide d'une sonde oesoph...

  5. Pas d'image fiable de notre atmosphère sans mesures depuis le sol !

    OpenAIRE

    Mazière, M.; De Backer, H.; Mahieu, Emmanuel; Vander Auwera, J.; Bader, Whitney; V. De Bock; Desmet, F.; Foldes, T; Gielen, C.; Hendrick, F.; Hermans, C.; B. Langerock; Lejeune, Bernard; Mangold, A.; Tudorie, M

    2014-01-01

    Nous sommes actuellement confrontés à une atmosphère en évolution : les concentrations de ce qu’on appelle les gaz à effet de serre augmentent, la quantité d’ozone stratosphérique diminue, en particulier au-dessus de l’Antarctique où elle forme chaque année un ‘trou’ dans la couche d’ozone, et l’air n’est pas tous les jours très sain... Comment pouvons-nous détecter et surveiller ces changements pour, si nécessaire, prendre des mesures pour tenter de les contrecarrer ?...

  6. Réseau de capteurs sans fils : Application à la mesure de vibrations

    OpenAIRE

    NGUYEN VAN PHU, C

    2006-01-01

    Les progrès des techniques électroniques rendent possible le concept de mise en réseau de capteurs intelligents sans fils. Sur cette base matérielle, se sont développées diverses plate formes sans fils dont le Mote est un exemple. La particularité du Mote est qu'il a servi de support au développement d'un système d'exploitation innovant pour réseaux de capteurs sans fils, TinyOS, qui depuis a été porté sur d'autres capteurs. Le Mote est présenté ainsi qu'une application de mesure sur un pont ...

  7. An Analysis of Coupling between the x1 and x12 Interferometers for LISA Pathfinder

    Science.gov (United States)

    Howard, Brittany

    2017-01-01

    Due to tolerances in the manufacturing process, noise from the jittering of the spacecraft housing LISA Pathfinder (LPF) is appearing in the differential measurement between its two test masses (TM's). This phenomenon manifests as a small but measurable coupling between the readouts of LPF's two heterodyne interferometers, x1 and x12. In this study, two LISA Pathfinder experiments are analyzed using three methods in an effort to characterize and quantify the coupling as well as to potentially identify its source. The main question considered is this: does the coupling change with the absolute displacement between the TM's? As a result of this work, reliable values for coupling between LPF's x1 and x12 interferometers are found, and they are seen to depend on the absolute displacement between the test masses to some degree. Completed at the Albert Einstein Institute for Gravitational Physics under the International REU program from the University of Florida.

  8. Neural network interpolation of the magnetic field for the LISA Pathfinder Diagnostics Subsystem

    CERN Document Server

    Diaz-Aguilo, Marc; García-Berro, Enrique

    2011-01-01

    LISA Pathfinder is a science and technology demonstrator of the European Space Agency within the framework of its LISA mission, which aims to be the first space-borne gravitational wave observatory. The payload of LISA Pathfinder is the so-called LISA Technology Package, which is designed to measure relative accelerations between two test masses in nominal free fall. Its disturbances are monitored and dealt by the diagnostics subsystem. This subsystem consists of several modules, and one of these is the magnetic diagnostics system, which includes a set of four tri-axial fluxgate magnetometers, intended to measure with high precision the magnetic field at the positions of the test masses. However, since the magnetometers are located far from the positions of the test masses, the magnetic field at their positions must be interpolated. It has been recently shown that because there are not enough magnetic channels, classical interpolation methods fail to derive reliable measurements at the positions of the test m...

  9. William Herschel Telescope site characterization using the MOAO pathfinder CANARY on-sky data

    CERN Document Server

    Martin, O A; Gendron, E; Rousset, G; Vidal, F; Morris, T J; Basden, A G; Myers, R M; Ono, Y H; Neichel, B; Fusco, T

    2016-01-01

    Canary is the Multi-Object Adaptive Optics (MOAO) pathfinder for the future MOAO-assisted Integral-Field Units (IFU) proposed for Extremely Large Telescopes (ELT). The MOAO concept relies on tomographically reconstructing the turbulence using multiple measurements along different lines of sight. Tomography requires the knowledge of the statistical turbulence parameters, commonly recovered from the system telemetry using a dedicated profiling technique. For demonstration purposes with the MOAO pathfinder Canary , this identification is performed thanks to the Learn & Apply (L&A) algorithm, that consists in model- fitting the covariance matrix of WFS measurements dependent on relevant parameters: $C_n^2(h)$ profile, outer scale profile and system mis-registration. We explore an upgrade of this algorithm, the Learn 3 Steps (L3S) approach, that allows one to dissociate the identification of the altitude layers from the ground in order to mitigate the lack of convergence of the required empirical covarianc...

  10. Capteurs monopodes pour mesures accélérométriques

    Science.gov (United States)

    Delaite, R.; Valentin, J.-P.

    1993-08-01

    A new design for accelerometric measurements sensors is described. It uses a plate vibrating in thickness shear mode, maintained by the means of a single holder located at the crystal edge. This mounting does cancel the mechanical and thermal stresses which generally modify the sensor output signal. So the ratio signal/noise of a thickness shear accelerometer is improved and the intrinsic sensitivity is multiplied by a factor 40, by comparison with the sensitivity of a thickness shear plate bonded by the means of two opposite holders. Un nouveau dispositif destiné aux mesures d'accélération est présenté. Il met en œuvre une lame vibrant en cisaillement d'épaisseur, fixée à sa structure de maintien par l'intermédiaire d'une unique liaison. Ce montage permet d'éliminer les contraintes mécaniques et thermiques qui perturbent habituellement le signal de mesure, et qui sont liées soit au montage des éléments du capteur, soit aux variations rapides de température qui interviennent lors de la mise en fonctionnement du capteur. Le rapport signal/bruit d'un accéléromètre à lame vibrant en cisaillement d'épaisseur s'en trouve amélioré et la sensibilité à l'accélération est multipliée par un facteur 40, comparée à celle d'un capteur qui serait constitué d'une lame vibrant en cisaillement d'épaisseur, fixée par deux liaisons diamétralement opposées.

  11. Pathfinder. Volume 8, Number 6, November/December 2010

    Science.gov (United States)

    2010-12-01

    global digital elevation model ever devel- oped from a single commercial sensor, while also planning its next-generation SAR system. South Korea is... digitally . As a baseline, the system is nominally a 1:500,000-scale map skin, augmented with com- mercially sourced aeronautical data. In the initial... Comunity Operating Referencing Station, or CORS, sites and provided training and other support. Afghanistan’s current geodetic surveying ca

  12. Indoor A* Pathfinding Through an Octree Representation of a Point Cloud

    Science.gov (United States)

    Rodenberg, O. B. P. M.; Verbree, E.; Zlatanova, S.

    2016-10-01

    There is a growing demand of 3D indoor pathfinding applications. Researched in the field of robotics during the last decades of the 20th century, these methods focussed on 2D navigation. Nowadays we would like to have the ability to help people navigate inside buildings or send a drone inside a building when this is too dangerous for people. What these examples have in common is that an object with a certain geometry needs to find an optimal collision free path between a start and goal point. This paper presents a new workflow for pathfinding through an octree representation of a point cloud. We applied the following steps: 1) the point cloud is processed so it fits best in an octree; 2) during the octree generation the interior empty nodes are filtered and further processed; 3) for each interior empty node the distance to the closest occupied node directly under it is computed; 4) a network graph is computed for all empty nodes; 5) the A* pathfinding algorithm is conducted. This workflow takes into account the connectivity for each node to all possible neighbours (face, edge and vertex and all sizes). Besides, a collision avoidance system is pre-processed in two steps: first, the clearance of each empty node is computed, and then the maximal crossing value between two empty neighbouring nodes is computed. The clearance is used to select interior empty nodes of appropriate size and the maximal crossing value is used to filter the network graph. Finally, both these datasets are used in A* pathfinding.

  13. The Ultraviolet Spectro-Coronagraph Pathfinder Mission for the Detection of Coronal Suprathermal Seed Particles

    Science.gov (United States)

    Strachan, Leonard; Laming, J. Martin; Ko, Yuan-Kuen; Korendyke, Clarence M.; Tun Beltran, Samuel; Socker, Dennis G.; Brown, Charles; Provornikova, Elena

    2016-05-01

    The Ultraviolet Spectro-Coronagraph (UVSC) Pathfinder is a Naval Research Laboratory experiment designed to make the first detection of suprathermal seed particles close to the Sun. It uses an innovative “stacked” occulting system to significantly increase the effective light gathering power of a traditional, 1-meter length, externally occulted coronagraph. The external occultation in combination with a low scatter variable line spaced grating provide the stray light suppression needed to measure non-Maxwellian departures in the wings of the H Lyman alpha emission line profile. After the removal of other factors, these departures may be interpreted as the signature of suprathermal tails of the proton velocity distribution in the corona. UVSC Pathfinder will provide information on the origins and spatial/temporal variability of proton seed particle populations. We will discuss the accuracy needed to make such measurements and describe how the results can be used to develop a capability for predicting the onset of Solar Energetic Particle (SEP) storms. The experiment is scheduled for a launch by the DoD Space Test Program in late 2018/early 2019 and should have excellent overlap with the Solar Orbiter and Solar Probe Plus missions.UVSC Pathfinder is supported by funds from the Chief of Naval Research (via the NRL basic research program) and from NASA (via NDPR NNG13WF951 and NNH16AC29I).

  14. The end-to-end testbed of the Optical Metrology System on-board LISA Pathfinder

    CERN Document Server

    Steier, Frank; Marín, Antonio F García; Gerardi, Domenico; Heinzel, Gerhard; Danzmann, Karsten; 10.1088/0264-9381/26/9/094010

    2012-01-01

    LISA Pathfinder is a technology demonstration mission for the Laser Interferometer Space Antenna (LISA). The main experiment on-board LISA Pathfinder is the so-called LISA Technology Package (LTP) which has the aim to measure the differential acceleration between two free-falling test masses with an accuracy of 3x10^(-14) ms^(-2)/sqrt[Hz] between 1 mHz and 30 mHz. This measurement is performed interferometrically by the Optical Metrology System (OMS) on-board LISA Pathfinder. In this paper we present the development of an experimental end-to-end testbed of the entire OMS. It includes the interferometer and its sub-units, the interferometer back-end which is a phasemeter and the processing of the phasemeter output data. Furthermore, 3-axes piezo actuated mirrors are used instead of the free-falling test masses for the characterisation of the dynamic behaviour of the system and some parts of the Drag-free and Attitude Control System (DFACS) which controls the test masses and the satellite. The end-to-end testbe...

  15. Review of A* (A Star) Navigation Mesh Pathfinding as the Alternative of Artificial Intelligent for Ghosts Agent on the Pacman Game

    OpenAIRE

    Moh. Zikky

    2016-01-01

    Shortest pathfinding problem has become a populer issue in Game’s Artificial Intelligent (AI). This paper discussed the effective way to optimize the shortest pathfinding problem, namely Navigation Mesh (NavMesh). This method is very interesting because it has a large area of implementation, especially in games world. In this paper, NavMesh was implemented by using A* (A star) algorithm and examined in Unity 3D game engine. A* was an effective algorithm in shortest pathfinding problem because...

  16. Comparaison instrumentale de la mesure des précipitations en climat méditerranéen semi-aride

    OpenAIRE

    Brunel, Jean-Pierre

    1986-01-01

    La pluie est un élément important du cycle de l'eau mesuré à l'aide d'appareils très divers. A partir des données d'une station agrométéorologique du Nord de la Tunisie (zone semi-aride), il est montré dans quelles proportions peuvent varier les précipitations mesurées par différents capteurs. L'influence du vent est mise en évidence dans l'écart observé entre pluie mesurée au sol et pluie mesurée au-dessus du sol. (Résumé d'auteur)

  17. Les fondements de la mesure du temps comment les fréquences atomiques règlent le monde

    CERN Document Server

    Audoin, Claude

    1998-01-01

    La mesure du temps fondée sur des propriétés atomiques est née en 1955, avec le premier étalon de fréquence à jet de césium. Depuis, les horloges atomiques ne cessent de progresser et sont au coeur de nombreuses activités, telles que les comparaisons de temps, l'unification mondiale de l'heure ou la recherche en astronomie, géodésie, géophysique, télécommunications, etc. Cet ouvrage fournira des réponses détaillées au lecteur intéressé par la mesure du temps appliquée aux divers domaines cités.

  18. Absolute measurement of {beta} emitters with a 4 {pi} counter; Mesure absolue des emetteurs {beta} au compteur 4 {pi}

    Energy Technology Data Exchange (ETDEWEB)

    Le Gallic, Y. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1959-06-15

    The object of this work is to investigate the conditions under which the activity of {beta}-emitting radionuclides may be measured with a maximum of precision, and as a result to study the relevant corrections. The various problems relating to activity measurements with a 4 {pi} counter have been examined successively: - comparison of 4 {pi}, GM and proportional counters; - study of the preparation of sources; - corrections on the counting of sources; - self-absorption; - correction for absorption. The precision obtained on these measurements varies from 1.2 to 3 per cent, with the result that the 4 {pi} counter can be considered a very satisfactory calibration instrument. (author) [French] Le but de ce travail est de rechercher les conditions permettant d'obtenir avec le maximum de precision, la mesure de l'activite des radionuclides se desintegrant par emission et par consequent d'etudier les corrections qui s'y rapportent. Nous avons examine successivement les differents problemes se rapportant aux mesures d'activite au compteur 4 {pi}: - Comparaison des compteurs 4 {pi}, GM et proportionnel; - etude de la preparation des sources; - corrections sur la numeration des sources; - auto-absorption; - correction d'absorption. La precision obtenue dans ces mesures, variant de 1,2 a 3 pour cent, on peut donc considerer le compteur 4 {pi} comme un instrument d'etalonnage tres satisfaisant. (auteur)

  19. Zebrafish foxP2 zinc finger nuclease mutant has normal axon pathfinding.

    Directory of Open Access Journals (Sweden)

    Lingyan Xing

    Full Text Available foxP2, a forkhead-domain transcription factor, is critical for speech and language development in humans, but its role in the establishment of CNS connectivity is unclear. While in vitro studies have identified axon guidance molecules as targets of foxP2 regulation, and cell culture assays suggest a role for foxP2 in neurite outgrowth, in vivo studies have been lacking regarding a role for foxP2 in axon pathfinding. We used a modified zinc finger nuclease methodology to generate mutations in the zebrafish foxP2 gene. Using PCR-based high resolution melt curve analysis (HRMA of G0 founder animals, we screened and identified three mutants carrying nonsense mutations in the 2(nd coding exon: a 17 base-pair (bp deletion, an 8bp deletion, and a 4bp insertion. Sequence analysis of cDNA confirmed that these were frameshift mutations with predicted early protein truncations. Homozygous mutant fish were viable and fertile, with unchanged body morphology, and no apparent differences in CNS apoptosis, proliferation, or patterning at embryonic stages. There was a reduction in expression of the known foxP2 target gene cntnap2 that was rescued by injection of wild-type foxP2 transcript. When we examined axon pathfinding using a pan-axonal marker or transgenic lines, including a foxP2-neuron-specific enhancer, we did not observe any axon guidance errors. Our findings suggest that foxP2 is not necessary for axon pathfinding during development.

  20. Shh signaling guides spatial pathfinding of raphespinal tract axons by multidirectional repulsion

    Institute of Scientific and Technical Information of China (English)

    Lijuan Song; Yuehui Liu; YangYu; Xin Duan; Shening Qi; Yaobo Liu

    2012-01-01

    Relatively little is known about the molecular mechanisms underlying spatial pathfinding in the descending serotonergic raphespinal tract (RST) in the developing spinal cord,one of the most important nerve pathways for pain,sensory and motor functions.We provide evidence that ventral floor plate-secreted Sonic hedgehog (Shh) is responsible for the establishment of decreasing gradients in both the anterior-to-posterior (A-P) and the medialto-lateral (M-L) directions in the ventral spinal cord during serotonergic RST axon projection.Downstream components of the Shh pathway,Patched 1 (Ptch1) and Smoothened (Smo),were expressed in the serotonergic caudal raphe nuclei and enriched in the descending serotonergic RST axons.Diffusible Shh repulsion of serotonergic RST axons was shown to be mediated by Shh-Ptch1 interactions and derepression of Smo.Using a co-culture assay,we showed that A-P graded repulsion mediated by Shh signaling pushed the serotonergic axons caudally through the ventral spinal cord and M-L graded repulsion mediated by Shh signaling simultaneously restricted the serotonergic axons to the ventral and ventral-lateral funiculus.Prominent pathfinding errors of serotonergic RST axons were observed in various Shh,Ptch1 and Smo mutants.We conclude that Shh signaling-mediated multidirectional repulsion is required to push descending serotonergic RST axons in the A-P direction,and to restrict these axons to the ventral and ventral-lateral funiculus in the M-L direction.This is the first demonstration that Shh signalingmediated muitidirectional repulsion of serotonergic RST axons maintains spatial axon pathfinding in the developing spinal cord.

  1. Shh signaling guides spatial pathfinding of raphespinal tract axons by multidirectional repulsion.

    Science.gov (United States)

    Song, Lijuan; Liu, Yuehui; Yu, Yang; Duan, Xin; Qi, Shening; Liu, Yaobo

    2012-04-01

    Relatively little is known about the molecular mechanisms underlying spatial pathfinding in the descending serotonergic raphespinal tract (RST) in the developing spinal cord, one of the most important nerve pathways for pain, sensory and motor functions. We provide evidence that ventral floor plate-secreted Sonic hedgehog (Shh) is responsible for the establishment of decreasing gradients in both the anterior-to-posterior (A-P) and the medial-to-lateral (M-L) directions in the ventral spinal cord during serotonergic RST axon projection. Downstream components of the Shh pathway, Patched 1 (Ptch1) and Smoothened (Smo), were expressed in the serotonergic caudal raphe nuclei and enriched in the descending serotonergic RST axons. Diffusible Shh repulsion of serotonergic RST axons was shown to be mediated by Shh-Ptch1 interactions and derepression of Smo. Using a co-culture assay, we showed that A-P graded repulsion mediated by Shh signaling pushed the serotonergic axons caudally through the ventral spinal cord and M-L graded repulsion mediated by Shh signaling simultaneously restricted the serotonergic axons to the ventral and ventral-lateral funiculus. Prominent pathfinding errors of serotonergic RST axons were observed in various Shh, Ptch1 and Smo mutants. We conclude that Shh signaling-mediated multidirectional repulsion is required to push descending serotonergic RST axons in the A-P direction, and to restrict these axons to the ventral and ventral-lateral funiculus in the M-L direction. This is the first demonstration that Shh signaling-mediated multidirectional repulsion of serotonergic RST axons maintains spatial axon pathfinding in the developing spinal cord.

  2. A phased approach to commissioning MCAO: Status and plans for the Linc-Nirvana Pathfinder

    Science.gov (United States)

    Conrad, Al; Bertram, Thomas; Kürster, Martin; Herbst, Tom; Ragazzoni, Roberto; Farinato, Jacopo; Viotto, Valentina; Bergomi, Maria; Brunelli, Alessandro; Arcidiacono, Carmelo; Bizenberger, Peter; Briegel, Florian; Hofferbert, Ralph; Gässler, Wolfgang; Meschke, Daniel; Mohr, Lars; Baumeister, Harald; Zhang, Xianyu; Trowitzsch, Jan; Berwein, Jürgen; Kittmann, Frank; Pott, Jorg-Uwe; Rohloff, Ralf-Rainer; Bonis, De Fulvio

    2011-09-01

    Layer-oriented multi-conjugate adaptive optics (MCAO) systems apply two or more wavefront-sensor/deformable-mirror (WFS/DM) pairs, each conjugate to a different turbulent layer in the atmosphere. Because these pairs apply correction in series, they are largely decoupled from one another, lending them to a phased commissioning approach. Commissioning instruments on large telescopes, while almost always successful in the end, can be, experience has shown, inefficient and difficult to schedule. For Linc-Nirvana we plan to take advantage of the natural decoupling between the ground-layer subsystem (a 12-star pyramid WFS operating in conjunction with the LBT adaptive secondary) and the mid-high subsystem (an 8-star pyramid WFS working in conjunction with a Xynetics 349 actuator DM) to mitigate the difficulties that have been experienced commissioning complex instruments on large, over-subscribed, telescopes. Pathfinder is a test-bed, consisting of only those subsystems needed to operate, stand-alone, one of the two Linc-Nirvana ground-layer subsystems. The Pathfinder effort will tease out top-level interface issues; while at the same time providing a valuable characterization of the Mount Graham ground-layer. To what extent will this ground-layer system provide a seeing-corrected image to the next WFS/DM pair in the Linc-Nirvana system: the mid-high wavefront-sensor (MHWS)? We will present status and plans for the Linc-Nirvana Pathfinder effort, a novel approach for commissioning MCAO systems on large telescopes.

  3. A simple neural network model of the hippocampus suggesting its pathfinding role in episodic memory retrieval.

    Science.gov (United States)

    Samsonovich, Alexei V; Ascoli, Giorgio A

    2005-01-01

    The goal of this work is to extend the theoretical understanding of the relationship between hippocampal spatial and memory functions to the level of neurophysiological mechanisms underlying spatial navigation and episodic memory retrieval. The proposed unifying theory describes both phenomena within a unique framework, as based on one and the same pathfinding function of the hippocampus. We propose a mechanism of reconstruction of the context of experience involving a search for a nearly shortest path in the space of remembered contexts. To analyze this concept in detail, we define a simple connectionist model consistent with available rodent and human neurophysiological data. Numerical study of the model begins with the spatial domain as a simple analogy for more complex phenomena. It is demonstrated how a nearly shortest path is quickly found in a familiar environment. We prove numerically that associative learning during sharp waves can account for the necessary properties of hippocampal place cells. Computational study of the model is extended to other cognitive paradigms, with the main focus on episodic memory retrieval. We show that the ability to find a correct path may be vital for successful retrieval. The model robustly exhibits the pathfinding capacity within a wide range of several factors, including its memory load (up to 30,000 abstract contexts), the number of episodes that become associated with potential target contexts, and the level of dynamical noise. We offer several testable critical predictions in both spatial and memory domains to validate the theory. Our results suggest that (1) the pathfinding function of the hippocampus, in addition to its associative and memory indexing functions, may be vital for retrieval of certain episodic memories, and (2) the hippocampal spatial navigation function could be a precursor of its memory function.

  4. The readout system and the trigger algorithm implementation for the UFFO Pathfinder

    Science.gov (United States)

    Na, G. W.; Ahmad, S.; Barrillon, P.; Brandt, S.; Budtz-Jørgensen, C.; Castro-Tirado, A. J.; Chen, P.; Choi, Y. J.; Connell, P.; Dagoret-Campagne, S.; Eyles, C.; Grossan, B.; Huang, M.-H. A.; Jeong, S.; Jung, A.; Kim, J. E.; Kim, M. B.; Kim, S.-W.; Kim, Y. W.; Krasnov, Aleksey S.; Lee, J.; Lim, H.; Linder, E. V.; Liu, T.-C.; Lund, N.; Min, K. W.; Nam, J. W.; Park, I. H.; Panasyuk, M. I.; Ripa, J.; Reglero, V.; Rodrigo, J. M.; Smoot, G. F.; Suh, J. E.; Svertilov, S.; Vedenkin, N.; Wang, M.-Z.; Yashin, I.

    2012-09-01

    Since the launch of the SWIFT, Gamma-Ray Bursts (GRBs) science has been much progressed. Especially supporting many measurements of GRB events and sharing them with other telescopes by the Gamma-ray Coordinate Network (GCN) have resulted the richness of GRB events, however, only a few of GRB events have been measured within a minute after the gamma ray signal. This lack of sub-minute data limits the study for the characteristics of the UV-optical light curve of the short-hard type GRB and the fast-rising GRB. Therefore, we have developed the telescope named the Ultra-Fast Flash Observatory (UFFO) Pathfinder, to take the sub-minute data for the early photons from GRB. The UFFO Pathfinder has a coded-mask X-ray camera to search the GRB location by the UBAT trigger algorithm. To determine the direction of GRB as soon as possible it requires the fast processing. We have ultimately implemented all algorithms in field programmable gate arrays (FPGA) without microprocessor. Although FPGA, when compared with microprocessor, is generally estimated to support the fast processing rather than the complex processing, we have developed the implementation to overcome the disadvantage and to maximize the advantage. That is to measure the location as accurate as possible and to determine the location within the sub-second timescale. In the particular case for a accuracy of the X-ray trigger, it requires special information from the satellite based on the UFFO central control system. We present the implementation of the UBAT trigger algorithm as well as the readout system of the UFFO Pathfinder.

  5. H I observations of two new dwarf galaxies: Pisces A and B with the SKA Pathfinder KAT-7

    Science.gov (United States)

    Carignan, C.; Libert, Y.; Lucero, D. M.; Randriamampandry, T. H.; Jarrett, T. H.; Oosterloo, T. A.; Tollerud, E. J.

    2016-03-01

    Context. Pisces A and Pisces B are the only two galaxies found via optical imaging and spectroscopy out of 22 Hi clouds identified in the GALFAHI survey as dwarf galaxy candidates. Aims: We derive the Hi content and kinematics of Pisces A and B. Methods: Our aperture synthesis Hi observations used the seven-dish Karoo Array Telescope (KAT-7), which is a pathfinder instrument for MeerKAT, the South African precursor to the mid-frequency Square Kilometre Array (SKA-MID). Results: The low rotation velocities of ~5 km s-1 and ~10 km s-1 in Pisces A and B, respectively, and their Hi content show that they are really dwarf irregular galaxies (dIrr). Despite that small rotation component, it is more the random motions ~9-11 km s-1 that provide most of the gravitational support, especially in the outer parts. The study of their kinematics, especially the strong gradients of random motions, suggest that those two dwarf galaxies are not yet in equilibrium. Conclusions: These Hi- rich galaxies may be indicative of a large population of dwarfs at the limit of detectability. However, such gas-rich dwarf galaxies will most likely never be within the virial radius of MW-type galaxies and become subhalo candidates. Systems such as Pisces A and B are more likely to be found at a few Mpc s from MW-type galaxies. The final FITS cube is only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/587/L3

  6. Mesure de la concentration absolue de SiO parspectroscopie d'absorption UV

    Science.gov (United States)

    Coursimault, F.; Motret, O.; Viladrosa, R.; Pouvesle, J. M.

    2003-06-01

    Le but de cette étude est de développer un diagnostic de mesure de concentration de Si0 adapté à un procédé industriel de dépôt d'oxydes de silicium sur polymères par décharge a barrière diélectrique atmosphérique (DBD). Deux méthodes spectroscopiques basées sur des techniques d'absorption et d'auto-absorption ont été développées. La concentration de Si0 a été estimée par ajustement des spectres synthétiques calculés sur les spectres expérimentaux. Ces deux méthodes permettent de suivre l'évolution temporelle de Si0 durant les phases de décharge et de post-décharge.

  7. Towards a Framework for Generating Tests to Satisfy Complex Code Coverage in Java Pathfinder

    Science.gov (United States)

    Staats, Matt

    2009-01-01

    We present work on a prototype tool based on the JavaPathfinder (JPF) model checker for automatically generating tests satisfying the MC/DC code coverage criterion. Using the Eclipse IDE, developers and testers can quickly instrument Java source code with JPF annotations covering all MC/DC coverage obligations, and JPF can then be used to automatically generate tests that satisfy these obligations. The prototype extension to JPF enables various tasks useful in automatic test generation to be performed, such as test suite reduction and execution of generated tests.

  8. Open access and knowledge sharing: reflections on the Pathfinder projects and Open Access Good Practice initiative

    Directory of Open Access Journals (Sweden)

    Hannah DeGroff

    2016-07-01

    Full Text Available The following article provides a selection of reflections from a number of higher education institutions and their staff about participation in the UK-wide Pathfinder project scheme. These nine projects (comprising 30 institutions form the core of the Jisc-funded Open Access Good Practice initiative. They have produced a wide range of outputs which endorse and encourage best practice when implementing open access across institutions. Each project has a blog where progress and outputs can be tracked. Details are listed at the end of this article.

  9. The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment

    DEFF Research Database (Denmark)

    Schofield, J.T.; Barnes, J.R.; Crisp, D.

    1997-01-01

    The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment measured the vertical density, pressure, and temperature structure of the martian atmosphere from the surface to 160 km, and monitored surface meteorology and climate for 83 sols (1 sol = 1 martian day = 24.......7 hours). The atmospheric structure and the weather record are similar to those observed by the Viking 1 lander (VL-1) at the same latitude, altitude, and season 21 years ago, but there are differences related to diurnal effects and the surface properties of the landing site. These include a cold...

  10. Midline governs axon pathfinding by coordinating expression of two major guidance systems.

    Science.gov (United States)

    Liu, Qing-Xin; Hiramoto, Masaki; Ueda, Hitoshi; Gojobori, Takashi; Hiromi, Yasushi; Hirose, Susumu

    2009-05-15

    Formation of the neural network requires concerted action of multiple axon guidance systems. How neurons orchestrate expression of multiple guidance genes is poorly understood. Here, we show that Drosophila T-box protein Midline controls expression of genes encoding components of two major guidance systems: Frazzled, ROBO, and Slit. In midline mutant, expression of all these molecules are reduced, resulting in severe axon guidance defects, whereas misexpression of Midline induces their expression. Midline is present on the promoter regions of these genes, indicating that Midline controls transcription directly. We propose that Midline controls axon pathfinding through coordinating the two guidance systems.

  11. Implications of Mars Pathfinder data for the accretion history of the terrestrial planets.

    Science.gov (United States)

    Bertka, C M; Fei, Y

    1998-09-18

    Accretion models of the terrestrial planets often assume planetary bulk compositions with nonvolatile element abundance ratios equivalent to those of C1 carbonaceous chondrites. The moment of inertia factor of Mars reported by the Pathfinder team is inconsistent with a bulk planet C1 Fe/Si ratio or Fe content, which suggests that C1 chondrite accretion models are insufficient to explain the formation of Mars and the other terrestrial planets. Future planetary accretion models will have to account for variations in bulk Fe/Si ratios among the terrestrial planets.

  12. Thermo-elastic induced phase noise in the LISA Pathfinder spacecraft

    OpenAIRE

    Gibert, F; Nofrarias, M; Karnesis, N; Gesa, L.; Martín, V.; Mateos, I; Lobo, A; Flatscher, R.; Gerardi, D; Burkhardt, J.; Gerndt, R.; Robertson, D; Ward, H; McNamara, P; Guzman, F.

    2014-01-01

    During the On-Station Thermal Test campaign of the LISA Pathfinder the data and diagnostics subsystem was tested in nearly space conditions for the first time after integration in the satellite. The results showed the compliance of the temperature measurement system, obtaining temperature noise around $10^{-4}\\,{\\rm K}\\, {\\rm Hz}^{-1/2}$ in the frequency band of $1-30\\;{\\rm mHz}$. In addition, controlled injection of heat signals to the suspension struts anchoring the LISA Technology Package ...

  13. A New Approach in Agent Path-Finding using State Mark Gradients

    Directory of Open Access Journals (Sweden)

    Florin Leon

    2005-01-01

    Full Text Available Since searching is one of the most important problem-solving methods, especially in Artificial Intelligence where it is often difficult to devise straightforward solutions, it has been given continuous attention by researchers. In this paper a new algorithm for agent path-finding is presented. Our approach is based on environment marking during exploration. We tested the performances of Q-learning and Learning Real-Time A* algorithm for three proposed mazes and then a comparison was made between our algorithm, two variants of Q-learning and LRTA* algorithm.

  14. ERASMUS-F: pathfinder for an E-ELT 3D instrumentation

    Science.gov (United States)

    Kelz, Andreas; Roth, Martin M.; Bacon, Roland; Bland-Hawthorn, Joss; Nicklas, Harald E.; Bryant, Julia J.; Colless, Matthew; Croom, Scott; Ellis, Simon; Fleischmann, Andreas; Gillingham, Peter; Haynes, Roger; Hopkins, Andrew; Kosmalski, Johan; O'Byrne, John W.; Olaya, Jean-Christophe; Rambold, William N.; Robertson, Gordon

    2010-07-01

    ERASMUS-F is a pathfinder study for a possible E-ELT 3D-instrumentation, funded by the German Ministry for Education and Research (BMBF). The study investigates the feasibility to combine a broadband optical spectrograph with a new generation of multi-object deployable fibre bundles. The baseline approach is to modify the spectrograph of the Multi-Unit Spectroscopic Explorer (MUSE), which is a VLT integral-field instrument using slicers, with a fibre-fed input. Taking advantage of recent developments in astrophotonics, it is planed to equip such an instrument with fused fibre bundles (hexabundles) that offer larger filling factors than dense-packed classical fibres. The overall project involves an optical and mechanical design study, the specifications of a software package for 3Dspectrophotometry, based upon the experiences with the P3d Data Reduction Software and an investigation of the science case for such an instrument. As a proof-of-concept, the study also involves a pathfinder instrument for the VLT, called the FIREBALL project.

  15. Relevance and feasibility of Diagnostics Subsystems in LISA PathFinder and LISA

    Science.gov (United States)

    Lobo, Alberto; Grimani, Catia; Canizares, Priscilla; Chmeissani, Mokhtar; Diaz-Aguilo, Marc; Conchillo, Aleix; Gesa, Lluis; Lloro, Ivan; Mateos, Ignacio; Nofrarias, Miquel; Ramos-Castro, Juan; Sanjuan, Josep; Sopuerta, Carlos

    LISA PathFinder will fly equipped with a Diagnostics Subsystem which includes: 1) a Radi-ation Monitor, providing almost real time charged particle counting and spectral resolution, 2) a thermal diagnostics set with high sensitivity temperature sensors and precision heaters, and 3) four fluxgate vector magnetometers plus a pair of induction coils. The role of this in-strumentation in LISA PathFinder is to provide the necessary tools to evaluate the effect of charging, temperature and magnetic fluctuations on the interferometer readout. The use of this is to understand how the mentioned fluctuations in the LTP (LISA Technology Package) can be modelled, then use the measured data to quantify their contribution to the overall LTP noise. In this presentation we will review the LPF Diagnostics System, recently delivered for LTP and spacecraft integration. We will also make some considerations on the meaning of the diagnostics for the future LISA, and propose lines of action to meet the more severe requirements which LISA will impose on environmental conditions.

  16. Charge-Induced Force Noise on Free-Falling Test Masses: Results from LISA Pathfinder

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J. T.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; de Deus Silva, M.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E. D.; Flatscher, R.; Freschi, M.; Gallegos, J.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gibert, F.; Giardini, D.; Giusteri, R.; Grimani, C.; Grzymisch, J.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Killow, C. J.; Korsakova, N.; Lloro, I.; Liu, L.; López-Zaragoza, J. P.; Maarschalkerweerd, R.; Madden, S.; Mance, D.; Martín, V.; Martin-Polo, L.; Martino, J.; Martin-Porqueras, F.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mendes, L.; Moroni, A.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D. I.; Rozemeijer, H.; Rivas, F.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C.; Sumner, T. J.; Texier, D.; Thorpe, J. I.; Trenkel, C.; Vetrugno, D.; Vitale, S.; Wanner, G.; Ward, H.; Wass, P. J.; Wealthy, D.; Weber, W. J.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.; LISA Pathfinder Collaboration

    2017-04-01

    We report on electrostatic measurements made on board the European Space Agency mission LISA Pathfinder. Detailed measurements of the charge-induced electrostatic forces exerted on free-falling test masses (TMs) inside the capacitive gravitational reference sensor are the first made in a relevant environment for a space-based gravitational wave detector. Employing a combination of charge control and electric-field compensation, we show that the level of charge-induced acceleration noise on a single TM can be maintained at a level close to 1.0 fm s-2 Hz-1 /2 across the 0.1-100 mHz frequency band that is crucial to an observatory such as the Laser Interferometer Space Antenna (LISA). Using dedicated measurements that detect these effects in the differential acceleration between the two test masses, we resolve the stochastic nature of the TM charge buildup due to interplanetary cosmic rays and the TM charge-to-force coupling through stray electric fields in the sensor. All our measurements are in good agreement with predictions based on a relatively simple electrostatic model of the LISA Pathfinder instrument.

  17. Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results

    Science.gov (United States)

    Armano, M.; Audley, H.; Auger, G.; Baird, J. T.; Bassan, M.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Caleno, M.; Carbone, L.; Cavalleri, A.; Cesarini, A.; Ciani, G.; Congedo, G.; Cruise, A. M.; Danzmann, K.; de Deus Silva, M.; De Rosa, R.; Diaz-Aguiló, M.; Di Fiore, L.; Diepholz, I.; Dixon, G.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fichter, W.; Fitzsimons, E. D.; Flatscher, R.; Freschi, M.; García Marín, A. F.; García Marirrodriga, C.; Gerndt, R.; Gesa, L.; Gibert, F.; Giardini, D.; Giusteri, R.; Guzmán, F.; Grado, A.; Grimani, C.; Grynagier, A.; Grzymisch, J.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hoyland, D.; Hueller, M.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johann, U.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C. J.; Lobo, J. A.; Lloro, I.; Liu, L.; López-Zaragoza, J. P.; Maarschalkerweerd, R.; Mance, D.; Martín, V.; Martin-Polo, L.; Martino, J.; Martin-Porqueras, F.; Madden, S.; Mateos, I.; McNamara, P. W.; Mendes, J.; Mendes, L.; Monsky, A.; Nicolodi, D.; Nofrarias, M.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Raïs, B.; Ramos-Castro, J.; Reiche, J.; Robertson, D. I.; Rozemeijer, H.; Rivas, F.; Russano, G.; Sanjuán, J.; Sarra, P.; Schleicher, A.; Shaul, D.; Slutsky, J.; Sopuerta, C. F.; Stanga, R.; Steier, F.; Sumner, T.; Texier, D.; Thorpe, J. I.; Trenkel, C.; Tröbs, M.; Tu, H. B.; Vetrugno, D.; Vitale, S.; Wand, V.; Wanner, G.; Ward, H.; Warren, C.; Wass, P. J.; Wealthy, D.; Weber, W. J.; Wissel, L.; Wittchen, A.; Zambotti, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2016-06-01

    We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density of 5.2 ±0.1 fm s-2/√{Hz } , or (0.54 ±0.01 ) ×10-15 g/√{Hz } , with g the standard gravity, for frequencies between 0.7 and 20 mHz. This value is lower than the LISA Pathfinder requirement by more than a factor 5 and within a factor 1.25 of the requirement for the LISA mission, and is compatible with Brownian noise from viscous damping due to the residual gas surrounding the test masses. Above 60 mHz the acceleration noise is dominated by interferometer displacement readout noise at a level of (34.8 ±0.3 ) fm /√{Hz } , about 2 orders of magnitude better than requirements. At f ≤0.5 mHz we observe a low-frequency tail that stays below 12 fm s-2/√{Hz } down to 0.1 mHz. This performance would allow for a space-based gravitational wave observatory with a sensitivity close to what was originally foreseen for LISA.

  18. Expansion of the piriform cortex contributes to corticothalamic pathfinding defects in Gli3 conditional mutants.

    Science.gov (United States)

    Amaniti, Eleni-Maria; Fu, Chaoying; Lewis, Sean; Saisana, Marina; Magnani, Dario; Mason, John O; Theil, Thomas

    2015-02-01

    The corticothalamic and thalamocortical tracts play essential roles in the communication between the cortex and thalamus. During development, axons forming these tracts have to follow a complex path to reach their target areas. While much attention has been paid to the mechanisms regulating their passage through the ventral telencephalon, very little is known about how the developing cortex contributes to corticothalamic/thalamocortical tract formation. Gli3 encodes a zinc finger transcription factor widely expressed in telencephalic progenitors which has important roles in corticothalamic and thalamocortical pathfinding. Here, we conditionally inactivated Gli3 in dorsal telencephalic progenitors to determine its role in corticothalamic tract formation. In Emx1Cre;Gli3(fl/fl) mutants, only a few corticothalamic axons enter the striatum in a restricted dorsal domain. This restricted entry correlates with a medial expansion of the piriform cortex. Transplantation experiments showed that the expanded piriform cortex repels corticofugal axons. Moreover, expression of Sema5B, a chemorepellent for corticofugal axons produced by the piriform cortex, is similarly expanded. Finally, time course analysis revealed an expansion of the ventral pallial progenitor domain which gives rise to the piriform cortex. Hence, control of lateral cortical development by Gli3 at the progenitor level is crucial for corticothalamic pathfinding.

  19. Coupling characterization and noise studies of the optical metrology system onboard the LISA Pathfinder mission.

    Science.gov (United States)

    Hechenblaikner, Gerald; Gerndt, Rüdiger; Johann, Ulrich; Luetzow-Wentzky, Peter; Wand, Vinzenz; Audley, Heather; Danzmann, Karsten; Garcia-Marin, Antonio; Heinzel, Gerhard; Nofrarias, Miquel; Steier, Frank

    2010-10-10

    We describe the first investigations of the complete engineering model of the optical metrology system (OMS), a key subsystem of the LISA Pathfinder science mission to space. The latter itself is a technological precursor mission to LISA, a spaceborne gravitational wave detector. At its core, the OMS consists of four heterodyne Mach-Zehnder interferometers, a highly stable laser with an external modulator, and a phase meter. It is designed to monitor and track the longitudinal motion and attitude of two floating test masses in the optical reference frame with (relative) precision in the picometer and nanorad range, respectively. We analyze sensor signal correlations and determine a physical sensor noise limit. The coupling parameters between motional degrees of freedom and interferometer signals are analytically derived and compared to measurements. We also measure adverse cross-coupling effects originating from system imperfections and limitations and describe algorithmic mitigation techniques to overcome some of them. Their impact on system performance is analyzed within the context of the Pathfinder mission.

  20. A Wind Tunnel Study on the Mars Pathfinder (MPF) Lander Descent Pressure Sensor

    Science.gov (United States)

    Soriano, J. Francisco; Coquilla, Rachael V.; Wilson, Gregory R.; Seiff, Alvin; Rivell, Tomas

    2001-01-01

    The primary focus of this study was to determine the accuracy of the Mars Pathfinder lander local pressure readings in accordance with the actual ambient atmospheric pressures of Mars during parachute descent. In order to obtain good measurements, the plane of the lander pressure sensor opening should ideally be situated so that it is parallel to the freestream. However, due to two unfavorable conditions, the sensor was positioned in locations where correction factors are required. One of these disadvantages is due to the fact that the parachute attachment point rotated the lander's center of gravity forcing the location of the pressure sensor opening to be off tangent to the freestream. The second and most troublesome factor was that the lander descends with slight oscillations that could vary the amplitude of the sensor readings. In order to accurately map the correction factors required at each sensor position, an experiment simulating the lander descent was conducted in the Martian Surface Wind Tunnel at NASA Ames Research Center. Using a 115 scale model at Earth ambient pressures, the test settings provided the necessary Reynolds number conditions in which the actual lander was possibly subjected to during the descent. In the analysis and results of this experiment, the readings from the lander sensor were converted to the form of pressure coefficients. With a contour map of pressure coefficients at each lander oscillatory position, this report will provide a guideline to determine the correction factors required for the Mars Pathfinder lander descent pressure sensor readings.

  1. A torsion pendulum test of the Lisa Pathfinder free-fall mode

    Science.gov (United States)

    Russano, Giuliana; Dolesi, Rita; Cavalleri, Antonella; Hueller, Mauro; Vitale, Stefano; Weber, William Joseph; Tu, HaiBo

    The LISA Pathfinder geodesic explorer mission for gravitational wave astronomy aims to demonstrate the proof of a low acceleration noise level. The relative acceleration between two test masses free falling in orbit is perturbed by the presence of a larger constant relative acceleration that must be actively compensated in order to keep the test particles centered inside an orbiting apparatus. The actuation force applied to compensate this effect introduces a dominant source of force noise. To suppress this noise source, a “free-fall” actuation control scheme has been designed: actuation is limited to brief impulses, with test masses in free fall in between two “kicks”, with this actuation-free motion then analyzed for the remaining sources of acceleration ultra noise. In this work, we will discuss and present preliminary data for an on-ground torsion pendulum experiment to test this technique, and the associated analysis algorithms, at a level nearing the sub-femto-g/sqrt(Hz) performance required for LISA Pathfinder.

  2. The fax-1 nuclear hormone receptor regulates axon pathfinding and neurotransmitter expression.

    Science.gov (United States)

    Much, J W; Slade, D J; Klampert, K; Garriga, G; Wightman, B

    2000-02-01

    Specification of neuron identity requires the activation of a number of discrete developmental programs. Among these is pathway selection by growth cones: in order for a neuron's growth cone to respond appropriately to guidance cues presented by other cells or the extracellular matrix, the neuron must express genes to mediate the response. The fax-1 gene of C. elegans is required for pathfinding of axons that extend along the ventral nerve cord. We show that fax-1 is also required for pathfinding of axons in the nerve ring, the largest nerve bundle in the nematode, and for normal expression of FMRFamide-like neurotransmitters in the AVK interneurons. The fax-1 gene encodes a member of the superfamily of nuclear hormone receptors and has a DNA-binding domain related to the human PNR and Drosophila Tailless proteins. We observe fax-1 expression in embryonic neurons, including the AVK interneurons, just prior to axon extension, but after neurogenesis. These data suggest that fax-1 coordinately regulates the transcription of genes that function in the selection of axon pathways, neurotransmitter expression and, perhaps, other aspects of the specification of neuron identity.

  3. Characterizing Semaphorin-Mediated Effects on Sensory and Motor Axon Pathfinding and Connectivity During Embryonic Development.

    Science.gov (United States)

    Huettl, Rosa Eva; Huber, Andrea B

    2017-01-01

    How are precise connectivity to peripheral targets and corresponding sensory-motor networks established during developmental innervation of the vertebrate extremities? The formation of functional sensory-motor circuits requires highly appropriate temporal and spatial regulation of axon growth which is achieved through the combination of different molecular mechanisms such as communication between heterotypic fiber systems, axon-environment, or axon-glia interactions that ensure proper fasciculation and accurate pathfinding to distal targets. Family members of the class 3 semaphorins and their cognate receptors, the neuropilins, were shown to govern various events during wiring of central and peripheral circuits, with mice lacking Sema3-Npn signaling showing deficits in timing of growth, selective fasciculation, guidance fidelity, and coupling of sensory axon growth to motor axons at developmental time points. Given the accuracy with which these processes have to interact in a stepwise manner, deficiency of the smallest cog in the wheel may impact severely on the faithful establishment and functionality of peripheral circuitries, ultimately leading to behavioral impairments or even cause the death of the animal. Reliable quantitative analyses of sensory-motor fasciculation, extension, and guidance of axons to their cognate target muscles and the skin during development, but also assessment of physiological and behavioral consequences at adult age, are therefore a necessity to extend our understanding of the molecular mechanisms of peripheral circuit formation. In this chapter we provide a detailed methodology to characterize class 3 semaphorin-mediated effects on peripheral sensory and motor axon pathfinding and connectivity during embryonic development.

  4. Improving Markov Chain Monte Carlo algorithms in LISA Pathfinder Data Analysis

    Science.gov (United States)

    Karnesis, N.; Nofrarias, M.; Sopuerta, C. F.; Lobo, A.

    2012-06-01

    The LISA Pathfinder mission (LPF) aims to test key technologies for the future LISA mission. The LISA Technology Package (LTP) on-board LPF will consist of an exhaustive suite of experiments and its outcome will be crucial for the future detection of gravitational waves. In order to achieve maximum sensitivity, we need to have an understanding of every instrument on-board and parametrize the properties of the underlying noise models. The Data Analysis team has developed algorithms for parameter estimation of the system. A very promising one implemented for LISA Pathfinder data analysis is the Markov Chain Monte Carlo. A series of experiments are going to take place during flight operations and each experiment is going to provide us with essential information for the next in the sequence. Therefore, it is a priority to optimize and improve our tools available for data analysis during the mission. Using a Bayesian framework analysis allows us to apply prior knowledge for each experiment, which means that we can efficiently use our prior estimates for the parameters, making the method more accurate and significantly faster. This, together with other algorithm improvements, will lead us to our main goal, which is no other than creating a robust and reliable tool for parameter estimation during the LPF mission.

  5. Ascending Midbrain Dopaminergic Axons Require Descending GAD65 Axon Fascicles for Normal Pathfinding

    Directory of Open Access Journals (Sweden)

    Claudia Marcela Garcia-Peña

    2014-06-01

    Full Text Available The Nigrostriatal pathway (NSP is formed by dopaminergic axons that project from the ventral midbrain to the dorsolateral striatum as part of the medial forebrain bundle. Previous studies have implicated chemotropic proteins in the formation of the NSP during development but little is known of the role of substrate-anchored signals in this process. We observed in mouse and rat embryos that midbrain dopaminergic axons ascend in close apposition to descending GAD65-positive axon bundles throughout their trajectory to the striatum. To test whether such interaction is important for dopaminergic axon pathfinding, we analyzed transgenic mouse embryos in which the GAD65 axon bundle was reduced by the conditional expression of the diphtheria toxin. In these embryos we observed dopaminergic misprojection into the hypothalamic region and abnormal projection in the striatum. In addition, analysis of Robo1/2 and Slit1/2 knockout embryos revealed that the previously described dopaminergic misprojection in these embryos is accompanied by severe alterations in the GAD65 axon scaffold. Additional studies with cultured dopaminergic neurons and whole embryos suggest that NCAM and Robo proteins are involved in the interaction of GAD65 and dopaminergic axons. These results indicate that the fasciculation between descending GAD65 axon bundles and ascending dopaminergic axons is required for the stereotypical NSP formation during brain development and that known guidance cues may determine this projection indirectly by instructing the pathfinding of the axons that are part of the GAD65 axon scaffold.

  6. Visualizing Mars Using Virtual Reality: A State of the Art Mapping Technique Used on Mars Pathfinder

    Science.gov (United States)

    Stoker, C.; Zbinden, E.; Blackmon, T.; Nguyen, L.

    1999-01-01

    We describe an interactive terrain visualization system which rapidly generates and interactively displays photorealistic three-dimensional (3-D) models produced from stereo images. This product, first demonstrated in Mars Pathfinder, is interactive, 3-D, and can be viewed in an immersive display which qualifies it for the name Virtual Reality (VR). The use of this technology on Mars Pathfinder was the first use of VR for geologic analysis. A primary benefit of using VR to display geologic information is that it provides an improved perception of depth and spatial layout of the remote site. The VR aspect of the display allows an operator to move freely in the environment, unconstrained by the physical limitations of the perspective from which the data were acquired. Virtual Reality offers a way to archive and retrieve information in a way that is intuitively obvious. Combining VR models with stereo display systems can give the user a sense of presence at the remote location. The capability, to interactively perform measurements from within the VR model offers unprecedented ease in performing operations that are normally time consuming and difficult using other techniques. Thus, Virtual Reality can be a powerful a cartographic tool. Additional information is contained in the original extended abstract.

  7. Detection of Porous and Permeable Formations: From Laboratory Measurements to Seismic Measurements Détection des formations poreuses et perméables : des mesures de laboratoire aux mesures sismiques

    Directory of Open Access Journals (Sweden)

    Mari J.L.

    2012-09-01

    Full Text Available We present a seismic processing method which shows that it is possible to extract new attributes from seismic sections, leading to a better understanding of the distribution of the porous and permeable bodies. The attributes are also used to detect the impermeable layers. The methodology is based on laboratory experiments which have shown that a formation permeability indicator can be obtained via the computation of 4 input data: P-wave frequency and attenuation, porosity and specific surface. The procedure has been firstly conducted in acoustic logging to estimate permeability of porous layers and to detect water inflows [Mari et al. (2011 Phys. Chem. Earth 36, 17, 1438-1449]. In seismic, the processing is performed in order to measure these parameters. The analytic signal is used to compute the instantaneous frequency and attenuation (Q factor. The porosity and specific surface are computed from seismic impedances obtained by acoustic inversion of the migrated seismic sections. The input parameters are used to compute a new index named Ik-Seis factor (Indicator (I of permeability (k from acoustic or seismic (Seis data. The potential of the proposed procedure is demonstrated via a field case, both in full waveform acoustic logging and in seismic surveying. The example shows that the Ik-Seis factor can be used to map both the distribution of the permeable bodies in the carbonate formations and the non permeable shaly layers associated with the Callovo-Oxfordian claystone. Dans le but d’avoir une meilleure comprehension de la distribution des corps poreux et permeables d’une formation geologique, nous montrons que de nouveaux attributs peuvent etre extraits des donnees sismiques. Les attributs peuvent etre egalement utilises pour detecter les niveaux impermeables. La methodologie est basee sur des mesures experimentales effectuees en laboratoire, qui ont montre qu’un indicateur de permeabilite peut etre obtenu a partir de quatre grandeurs

  8. Aimant PS: controle de l'etat des sertissages internes des PFW mesures effectues surl'ensemble des aimants du PS pendant le grand arret 2004/2006

    CERN Document Server

    Ottaviani, J

    2005-01-01

    Les sertissages (douilles), utilisés pour raccorder les méplats du circuit principal des PFW à leurs câbles d’alimentation, présentent parfois des défauts de réalisation qui entraînent une résistance électrique anormale. Pour mettre en évidence ces défauts, la résistance des 4 sertissages des nappes polaires est mesurée. Les nappes sont alimentées avec un courant efficace nominal de 80A.Les mesures sont effectuées entre le bornier de connexions des 4 câbles d’alimentation des PFW et les circuits auxiliaires correspondants (Pick-ups brasés sur les enroulements). De ces mesures (câble d’alimentation et une courte partie du circuit principal) est déduite la valeur de la résistance du sertissage qui en assure la liaison. A la mesure des résistances des sertissages des nappes polaires supérieures s’ajoute la résistance des câbles qui assurent la liaison entre borniers. Dans le cadre de la rénovation des aimants du PS, les 100 unités on été mesurées.

  9. Dangerosité, longues peines de prison et mesures préventives en Allemagne

    Directory of Open Access Journals (Sweden)

    Axel Dessecker

    2009-10-01

    Full Text Available S’appuyant sur les statistiques des condamnations officielles en Allemagne, notre article entend donner un aperçu de l’évolution historique de la peine d’emprisonnement à perpétuité, de la détention préventive ainsi que des ordonnances de détention en milieu hospitalier pour personnes souffrant de troubles mentaux. En Allemagne, la peine d’emprisonnement à perpétuité est actuellement la punition la plus sévère, mais son rôle était moins important du temps de la peine capitale. La détention préventive et les ordonnances de détention en milieu hospitalier sont, elles, toutes deux perçues comme des mesures préventives dont la durée d’exécution apparaît d’emblée indéterminée. Alors que la question des détentions préventives est largement débattue aujourd’hui, les condamnations prononcées par les cours ont légèrement augmenté. Quant aux ordonnances, elles semblent toujours plus nombreuses.The article gives an overview on the historical development of life sentences, preventive detention, and hospital orders for mentally disordered offenders in Germany on the basis of official conviction statistics. The life sentence is the most severe punishment today, while its role was less important as long as capital punishment existed. Preventive detention and hospital orders both are viewed as preventive measures, and they are indefinite from the beginning. While preventive detention is widely discussed today, convictions by the courts have been increasing from a low level. The level of hospital orders is much higher today. Full Text

  10. Dangerosité, longues peines de prison et mesures préventives en Allemagne

    Directory of Open Access Journals (Sweden)

    Axel Dessecker

    2012-05-01

    Full Text Available S’appuyant sur les statistiques des condamnations officielles en Allemagne, notre article entend donner un aperçu de l’évolution historique de la peine d’emprisonnement à perpétuité, de la détention préventive ainsi que des ordonnances de détention en milieu hospitalier pour personnes souffrant de troubles mentaux. En Allemagne, la peine d’emprisonnement à perpétuité est actuellement la punition la plus sévère, mais son rôle était moins important du temps de la peine capitale. La détention préventive et les ordonnances de détention en milieu hospitalier sont, elles, toutes deux perçues comme des mesures préventives dont la durée d’exécution apparaît d’emblée indéterminée. Alors que la question des détentions préventives est largement débattue aujourd’hui, les condamnations prononcées par les cours ont légèrement augmenté. Quant aux ordonnances, elles semblent toujours plus nombreuses.The article gives an overview on the historical development of life sentences, preventive detention, and hospital orders for mentally disordered offenders in Germany on the basis of official conviction statistics. The life sentence is the most severe punishment today, while its role was less important as long as capital punishment existed. Preventive detention and hospital orders both are viewed as preventive measures, and they are indefinite from the beginning. While preventive detention is widely discussed today, convictions by the courts have been increasing from a low level. The level of hospital orders is much higher today. Full Text

  11. Mars Pathfinder

    Science.gov (United States)

    Murdin, P.

    2000-11-01

    First of NASA's Discovery missions. Launched in December 1996 and arrived at Mars on 4 July 1997. Mainly intended as a technology demonstration mission. Used airbags to cushion the landing on Mars. The Carl Sagan Memorial station returned images of an ancient flood plain in Ares Vallis. The 10 kg Sojourner rover used an x-ray spectrometer to study the composition of rocks and travelled about 100 ...

  12. AVHRR Pathfinder version 5.3 level 3 collated (L3C) global 4km sea surface temperature

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The AVHRR Pathfinder Version 5.3 (PFV53) L3C Sea Surface Temperature data set is a collection of global, twice-daily (Day and Night) 4km sea surface temperature...

  13. Using the Hierarchical Pathfinding A* Algorithm in GIS to Find Paths through Rasters with Nonuniform Traversal Cost

    Directory of Open Access Journals (Sweden)

    Harri Antikainen

    2013-10-01

    Full Text Available A fair amount of research has been carried out on pathfinding problems in the context of transportation networks, whereas pathfinding in off-network space has received far less interest. In geographic information systems (GIS, the latter is usually associated with the cost surface method, which allows optimum paths to be calculated through rasters in which the value of each cell depicts the cost of traversal through that cell. One of the problems with this method is computational expense, which may be very high with large rasters. In this study, a pathfinding method called Hierarchical Pathfinding A* (HPA*, based on an abstraction strategy, is investigated as an alternative to the traditional approach. The aim of this study is to enhance the method to make it more suitable for calculating paths over cost rasters with nonuniform traversal cost. The method is implemented in GIS and tested with actual data. The results indicate that by taking into account the information embedded in the cost raster, paths of relatively good quality can be calculated while effecting significant savings in computational effort compared to the traditional, nonhierarchical approach.

  14. Mesure par conductimetrie de la receptivite aux maladies fongiques et du niveau de resistance induite par elicitation. Etude sur 3 modeles experimentaux

    OpenAIRE

    Molot, P.M.; Mas, P.; Pivot, V; Bruneteau, M; Staron, T; Ferriere, H.; Lemaire, J.M.

    1992-01-01

    L’appréciation des dégâts parasitaires, souvent difficile à évaluer, peut être effectuée par des mesures conductimétriques; en effet, les cellules altérées libèrent davantage d’électrolytes que les cellules saines dans le milieu extérieur, dont on mesure la conductance. Cette méthode peut être utilisée dans différents cas, notamment lorsqu’il y a attaque au niveau racinaire. On mesure alors la conductance de l’eau dans laquelle baignent des racines contaminées (piment - Phytophthora capsici, ...

  15. Translation balance for measuring magnetic susceptibilities at high or low temperatures (1962); Balance de translation pour la mesure des susceptibilites magnetiques a haute ou basse temperature (1962)

    Energy Technology Data Exchange (ETDEWEB)

    Blaise, A.; Peuch, M.A. [Commissariat a l' Energie Atomique, Grenoble (France). Centre d' Etudes Nucleaires

    1962-07-01

    A translation balance is described for the measurement of the magnetic susceptibilities of liquids or solids in the temperature range from 1.7 to 1400 deg. K. Measurements are made within a magnetic field adjustable from 3400 to 16000 oersteds, in any desired atmosphere. Susceptibilities between 10{sup -8} and 10{sup -4} u.e.m. C.G.S., can be measured. (authors) [French] La balance de translation decrite ici permet la mesure des susceptibilites magnetiques des liquides ou des solides dans la gamme de temperature allant de 1,7 a 1400 deg. K. Les mesures sont effectuees dans un champ magnetique ajustable de 3400 a 16000 oersteds, sous atmosphere controlee. La gamme des mesures de susceptibilite s'etend de 10{sup -8} a 10{sup -4} u.e.m. C.G.S. (auteurs)

  16. Conception et mesures du capital-marque des marques de distributeurs : une application au secteur de la grande distribution

    OpenAIRE

    Jara, Magali

    2008-01-01

    Ce papier tente de définir et de mesurer une première partie du cadre conceptuel du capital-marque des MDD (marques de distributeurs). Pour ce faire, les travaux de Keller (1993) ainsi que les apports théoriques des recherches sur les services dans le secteur de la distribution sont mobilisés. Puis, le modèle conceptuel est précisé par des entretiens individuels de consommateurs. Après une analyse de contenu, un modèle principal du capital-marque des MDD est proposé ajoutant les dimensions d'...

  17. Chemical analyses of martian soil and rocks obtained by the Pathfinder Alpha Proton X-ray spectrometer

    Energy Technology Data Exchange (ETDEWEB)

    Economou, Thanasis E-mail: tecon@tecon.uchicago.edu

    2001-06-01

    The US Mars Pathfinder spacecraft, which landed on the red planet on the 4th of July 1997, carried an Alpha Proton X-ray Spectrometer (APXS) that obtained the chemical composition of martian soil and rocks. The principles of the APXS operation are based on three interactions of alpha particles with matter: Rutherford alpha backscattering; ({alpha}, p) nuclear reactions; and X-ray generation by charged particles and X-ray excitation. The APXS, as was implemented on the Pathfinder mission, uses for all three modes of operation a monoenergetic beam of alpha particles from about 40 mCi of {sup 244}Cm radioisotope. It employs Si charged particle detectors for alpha and proton modes and a specially designed silicon PIN detector for its X-ray mode that does not require cooling for its operation. The APXS can detect all of the elements (except H and He) present above a few tenths of a percent for all major elements and several hundred ppm for many minor and trace elements. The APXS on Pathfinder was transported to various locations on the martian surface by the Sojourner rover which enabled it to analyze multiple soil and rock samples selected by the science team from the lander camera images. The APXS performed excellently under the adverse martian environment conditions and provided important information about the chemical composition of the martian soil and rocks. All of the analyzed rocks at the Pathfinder site were found to have high concentrations of silica, sulfur and iron, and low in magnesium, similar to those of the terrestrial basaltic andesites and definitely different from the SNC meteorites that are believed to have originated from Mars. All of the soil samples analyzed by the APXS have similar composition and are very close to the soil analyses obtained by the two Viking missions. The information derived from the Pathfinder APXS has significant implications about the origin and evolution of planet Mars. (author)

  18. Contrôlabilité : Suivi des mesures de CFL réalisées avec des pneumatiques AIPCR 07 et ASTM 07

    OpenAIRE

    Cerezo, Véronique; CENTRE D'ETUDES TECHNIQUES DE L'EQUIPEMENT DE LYON - CETE LYON; LABORATOIRE REGIONAL DES PONTS ET CHAUSSEES DE LYON - CETE DE LYON - LRPC LYON

    2010-01-01

    L'étude a pour objet l'étude du comportement des pneumatiques ASTM 07 et AIPCR 07 par rapport à celui des pneus standards d'essais AIPCR 98 utilisés pour les mesures de coefficient de frottement longitudinal. Tout d'abord, les pneumatiques ASTM 07 et AIPCR 07 semblent plus tendres que les pneus AIPCR 98. Il est nécessaire de les laisser vieillir quelques temps afin de revenir à des niveaux équivalents à ceux des pneus AIPCR 98 utilisés depuis une dizaine d'années en France pour les mesures de...

  19. LISA and LISA PathFinder, the endeavour to detect low frequency GWs

    Science.gov (United States)

    Araújo, H.; Boatella, C.; Chmeissani, M.; Conchillo, A.; García-Berro, E.; Grimani, C.; Hajdas, W.; Lobo, A.; Martínez, Ll; Nofrarias, M.; Ortega, J. A.; Puigdengoles, C.; Ramos-Castro, J.; Sanjuán, J.; Wass, P.; Xirgu, X.

    2007-05-01

    This is a review about LISA and its technology demonstrator, LISAPathFinder. We first describe the conceptual problems which need to be overcome in order to set up a working interferometric detector of low frequency Gravitational Waves (GW), then summarise the solutions to them as currently conceived by the LISA mission team. This will show that some of these solutions require new technological abilities which are still under development, and which need proper test before being fully implemented. LISAPathFinder (LPF) is the the testbed for such technologies. The final part of the paper will address the ideas and concepts behind the PathFinder as well as their impact on LISA.

  20. LISA and LISA PathFinder, the endeavour to detect low frequency GWs

    Energy Technology Data Exchange (ETDEWEB)

    Araujo, H [Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2BW (United Kingdom); Boatella, C [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Chmeissani, M [Institut de Fisica d' Altes Energies (IFAE), Edifici C, Universitat Autonoma de Barcelona, 08193 Bellaterra (Barcelona) (Spain); Conchillo, A [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Garcia-Berro, E [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Grimani, C [Universita degli Studi di Urbino, and INFN Florence, Istituto di Fisica, Via Santa Chiara 27, 61029 Urbino (Italy); Hajdas, W [Department of Particles and Matter, Paul Scherrer Institut, ODRA 120, 5232 Villigen (Switzerland); Lobo, A [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Martinez, L [AtIpic, Parc Tecnologic del Valles, 08290 Cerdanyola del Valles, Barcelona (Spain); Nofrarias, M [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Ortega, J A [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Puigdengoles, C [Institut de Fisica d' Altes Energies (IFAE), Edifici C, Universitat Autonoma de Barcelona, 08193 Bellaterra (Barcelona) (Spain); Ramos-Castro, J [Departament d' Enginyeria Electronica, UPC, Campus Nord, Edif. C4, Jordi Girona 1-3, 08034 Barcelona (Spain); Sanjuan, J [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain); Wass, P [Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2BW (United Kingdom); Xirgu, X [Institut d' Estudis Espacials de Catalunya (IEEC), Edifici Nexus, Gran Capita 2-4, 08034 Barcelona (Spain)

    2007-05-15

    This is a review about LISA and its technology demonstrator, LISAPathFinder. We first describe the conceptual problems which need to be overcome in order to set up a working interferometric detector of low frequency Gravitational Waves (GW), then summarise the solutions to them as currently conceived by the LISA mission team. This will show that some of these solutions require new technological abilities which are still under development, and which need proper test before being fully implemented. LISAPathFinder (LPF) is the the testbed for such technologies. The final part of the paper will address the ideas and concepts behind the PathFinder as well as their impact on LISA.

  1. Initial Results from ST7-Disturbance Reduction System on LISA Pathfinder

    Science.gov (United States)

    Dunn, Charles; Barela, Phillip; Cutler, Curt; Denzin, Richard; Franklin, Garth; Gorelik, Jacb; Hsu, Oscar; Javidnia, Shahram; Li, Irena; Maghami, Peiman; Marrese-Reading, Colleen; Mehta, Jitendra; O'Donnell, James; Romero-Wolf, Andrew; Slutsky, Jacob; Thorpe, Ira; Umfress, S. Harper; Ziemer, John

    2017-01-01

    The European Space Agency LISA Pathfinder spacecraft was launched on December, 2, 2015 carrying the NASA contribution ST7-Disturbance Reduction System (ST7-DRS). The objective of ST7-DRS is to demonstrate drag-free control and noise reduction technologies for future missions, especially a future space-based gravitational wave observatory. The system consists of a pair of Colloid Micro-Newton Thruster clusters and a computer with control algorithms. Data from the host platform is used for inertial and attitude sensing. ST7-DRS was initially powered on in January 2016 for an on-orbit check out and was fully commissioned in late June and early July. This presentation will report results relative to the 0.1 micro-Newton/ rt Hertz thrust noise requirement and the 10 nanometer/rt Hertz position control requirement. Preliminary extended mission results will be discussed. The work described here was funded by NASA.

  2. State-space modelling for heater induced thermal effects on LISA Pathfinder's Test Masses

    CERN Document Server

    Gibert, Ferran; Diaz-Aguiló, Marc; Lobo, Alberto; Karnesis, Nikolaos; Mateos, Ignacio; Sanjuán, Josep; Lloro, Ivan; Gesa, Lluís; Martín, Víctor; 10.1088/1742-6596/363/1/012044

    2012-01-01

    The OSE (Offline Simulations Environment) simulator of the LPF (LISA Pathfinder) mission is intended to simulate the different experiments to be carried out in flight. Amongst these, the thermal diagnostics experiments are intended to relate thermal disturbances and interferometer readouts, thereby allowing the subtraction of thermally induced interferences from the interferometer channels. In this paper we report on the modelling of these simulated experiments, including the parametrisation of different thermal effects (radiation pressure effect, radiometer effect) that will appear in the Inertial Sensor environment of the LTP (LISA Technology Package). We report as well how these experiments are going to be implemented in the LTPDA toolbox, which is a dedicated tool for LPF data analysis that will allow full traceability and reproducibility of the analysis thanks to complete recording of the processes.

  3. Thermo-elastic induced phase noise in the LISA Pathfinder spacecraft

    Science.gov (United States)

    Gibert, F.; Nofrarias, M.; Karnesis, N.; Gesa, L.; Martín, V.; Mateos, I.; Lobo, A.; Flatscher, R.; Gerardi, D.; Burkhardt, J.; Gerndt, R.; Robertson, D. I.; Ward, H.; McNamara, P. W.; Guzmán, F.; Hewitson, M.; Diepholz, I.; Reiche, J.; Heinzel, G.; Danzmann, K.

    2015-02-01

    During the on-station thermal test campaign of the LISA Pathfinder, the diagnostics subsystem was tested in nearly space conditions for the first time after integration in the satellite. The results showed the compliance of the temperature measurement system, obtaining temperature noise around {{10}-4} K H{{z}-1/2} in the frequency band 1-30 mHz. In addition, controlled injection of heat signals to the suspension struts anchoring the LISA Technology Package (LTP) core assembly to the satellite structure allowed us to experimentally estimate, for the first time, the phase noise contribution through thermo-elastic distortion of the LTP interferometer, the satellite's main instrument. Such contribution was found to be at {{10}-12} mH{{z}-1/2}, a factor of 30 below the measured noise at the lower end of the measurement bandwidth (1 mHz).

  4. The eLISA gravitational reference sensor and its test aboard LISA Pathfinder

    Science.gov (United States)

    Weber, William Joseph; Dolesi, Rita; Vitale, Stefano

    The upcoming LISA Pathfinder (LPF) mission represents the state-of-the-art in realizing a set of free-falling reference test masses for gravitational wave astronomy. The key hardware for achieving the smallest possible deviation from pure geodesic motion lies in the gravitational reference sensor or GRS. We present the GRS designed for achieving sub-femto-g/sqrt{mathrm{Hz}} performance with LPF and eLISA and discuss our current experimental estimates for the upcoming mission, including the latest results from the flight hardware test campaigns. Finally, we will address the LPF in-flight tests that will complete our physical model for test mass acceleration noise for eLISA and other possible experimental gravitational measurements in space.

  5. The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array

    Science.gov (United States)

    McConnell, D.; Allison, J. R.; Bannister, K.; Bell, M. E.; Bignall, H. E.; Chippendale, A. P.; Edwards, P. G.; Harvey-Smith, L.; Hegarty, S.; Heywood, I.; Hotan, A. W.; Indermuehle, B. T.; Lenc, E.; Marvil, J.; Popping, A.; Raja, W.; Reynolds, J. E.; Sault, R. J.; Serra, P.; Voronkov, M. A.; Whiting, M.; Amy, S. W.; Axtens, P.; Ball, L.; Bateman, T. J.; Bock, D. C.-J.; Bolton, R.; Brodrick, D.; Brothers, M.; Brown, A. J.; Bunton, J. D.; Cheng, W.; Cornwell, T.; DeBoer, D.; Feain, I.; Gough, R.; Gupta, N.; Guzman, J. C.; Hampson, G. A.; Hay, S.; Hayman, D. B.; Hoyle, S.; Humphreys, B.; Jacka, C.; Jackson, C. A.; Jackson, S.; Jeganathan, K.; Joseph, J.; Koribalski, B. S.; Leach, M.; Lensson, E. S.; MacLeod, A.; Mackay, S.; Marquarding, M.; McClure-Griffiths, N. M.; Mirtschin, P.; Mitchell, D.; Neuhold, S.; Ng, A.; Norris, R.; Pearce, S.; Qiao, R. Y.; Schinckel, A. E. T.; Shields, M.; Shimwell, T. W.; Storey, M.; Troup, E.; Turner, B.; Tuthill, J.; Tzioumis, A.; Wark, R. M.; Westmeier, T.; Wilson, C.; Wilson, T.

    2016-09-01

    We describe the performance of the Boolardy Engineering Test Array, the prototype for the Australian Square Kilometre Array Pathfinder telescope. Boolardy Engineering Test Array is the first aperture synthesis radio telescope to use phased array feed technology, giving it the ability to electronically form up to nine dual-polarisation beams. We report the methods developed for forming and measuring the beams, and the adaptations that have been made to the traditional calibration and imaging procedures in order to allow BETA to function as a multi-beam aperture synthesis telescope. We describe the commissioning of the instrument and present details of Boolardy Engineering Test Array's performance: sensitivity, beam characteristics, polarimetric properties, and image quality. We summarise the astronomical science that it has produced and draw lessons from operating Boolardy Engineering Test Array that will be relevant to the commissioning and operation of the final Australian Square Kilometre Array Path telescope.

  6. Bayesian Inference for LISA Pathfinder using Markov Chain Monte Carlo Methods

    CERN Document Server

    Ferraioli, Luigi; Plagnol, Eric

    2012-01-01

    We present a parameter estimation procedure based on a Bayesian framework by applying a Markov Chain Monte Carlo algorithm to the calibration of the dynamical parameters of a space based gravitational wave detector. The method is based on the Metropolis-Hastings algorithm and a two-stage annealing treatment in order to ensure an effective exploration of the parameter space at the beginning of the chain. We compare two versions of the algorithm with an application to a LISA Pathfinder data analysis problem. The two algorithms share the same heating strategy but with one moving in coordinate directions using proposals from a multivariate Gaussian distribution, while the other uses the natural logarithm of some parameters and proposes jumps in the eigen-space of the Fisher Information matrix. The algorithm proposing jumps in the eigen-space of the Fisher Information matrix demonstrates a higher acceptance rate and a slightly better convergence towards the equilibrium parameter distributions in the application to...

  7. In-flight thermal experiments for LISA Pathfinder: Simulating temperature noise at the Inertial Sensors

    Science.gov (United States)

    Gibert, F.; Nofrarias, M.; Armano, M.; Audley, H.; Auger, G.; Baird, J.; Binetruy, P.; Born, M.; Bortoluzzi, D.; Brandt, N.; Bursi, A.; Caleno, M.; Cavalleri, A.; Cesarini, A.; Cruise, M.; Danzmann, K.; Diepholz, I.; Dolesi, R.; Dunbar, N.; Ferraioli, L.; Ferroni, V.; Fitzsimons, E.; Freschi, M.; Gallegos, J.; García Marirrodriga, C.; Gerndt, R.; Gesa, Ll; Giardini, D.; Giusteri, R.; Grimani, C.; Harrison, I.; Heinzel, G.; Hewitson, M.; Hollington, D.; Hueller, M.; Huesler, J.; Inchauspé, H.; Jennrich, O.; Jetzer, P.; Johlander, B.; Karnesis, N.; Kaune, B.; Korsakova, N.; Killow, C.; Lloro, I.; Maarschalkerweerd, R.; Madden, S.; Maghami, P.; Mance, D.; Martín, V.; Martin-Porqueras, F.; Mateos, I.; McNamara, P.; Mendes, J.; Mendes, L.; Moroni, A.; Paczkowski, S.; Perreur-Lloyd, M.; Petiteau, A.; Pivato, P.; Plagnol, E.; Prat, P.; Ragnit, U.; Ramos-Castro, J.; Reiche, J.; Romera Perez, J. A.; Robertson, D.; Rozemeijer, H.; Russano, G.; Sarra, P.; Schleicher, A.; Slutsky, J.; Sopuerta, C. F.; Sumner, T.; Texier, D.; Thorpe, J.; Trenkel, C.; Tu, H. B.; Vetrugno, D.; Vitale, S.; Wanner, G.; Ward, H.; Waschke, S.; Wass, P.; Wealthy, D.; Wen, S.; Weber, W.; Wittchen, A.; Zanoni, C.; Ziegler, T.; Zweifel, P.

    2015-05-01

    Thermal Diagnostics experiments to be carried out on board LISA Pathfinder (LPF) will yield a detailed characterisation of how temperature fluctuations affect the LTP (LISA Technology Package) instrument performance, a crucial information for future space based gravitational wave detectors as the proposed eLISA. Amongst them, the study of temperature gradient fluctuations around the test masses of the Inertial Sensors will provide as well information regarding the contribution of the Brownian noise, which is expected to limit the LTP sensitivity at frequencies close to 1 mHz during some LTP experiments. In this paper we report on how these kind of Thermal Diagnostics experiments were simulated in the last LPF Simulation Campaign (November, 2013) involving all the LPF Data Analysis team and using an end-to-end simulator of the whole spacecraft. Such simulation campaign was conducted under the framework of the preparation for LPF operations.

  8. A GPU-based Correlator X-engine Implemented on the CHIME Pathfinder

    CERN Document Server

    Denman, Nolan; Bandura, Kevin; Connor, Liam; Dobbs, Matt; Fandino, Mateus; Halpern, Mark; Hincks, Adam; Hinshaw, Gary; Höfer, Carolin; Klages, Peter; Masui, Kiyoshi; Parra, Juan Mena; Newburgh, Laura; Recnik, Andre; Shaw, Richard; Sigurdson, Kris; Smith, Kendrick; Vanderlinde, Keith

    2015-01-01

    We present the design and implementation of a custom GPU-based compute cluster that provides the correlation X-engine of the CHIME Pathfinder radio telescope. It is among the largest such systems in operation, correlating 32,896 baselines (256 inputs) over 400MHz of radio bandwidth. Making heavy use of consumer-grade parts and a custom software stack, the system was developed at a small fraction of the cost of comparable installations. Unlike existing GPU backends, this system is built around OpenCL kernels running on consumer-level AMD GPUs, taking advantage of low-cost hardware and leveraging packed integer operations to double algorithmic efficiency. The system achieves the required 105TOPS in a 10kW power envelope, making it among the most power-efficient X-engines in use today.

  9. Theory and modeling of the magnetic field measurement in LISA PathFinder

    CERN Document Server

    Diaz-Aguilo, M; Lobo, A

    2009-01-01

    The magnetic diagnostics subsystem of the LISA Technology Package (LTP) on board the LISA PathFinder (LPF) spacecraft includes a set of four tri-axial fluxgate magnetometers, intended to measure with high precision the magnetic field at their respective positions. However, their readouts do not provide a direct measurement of the magnetic field at the positions of the test masses, and hence an interpolation method must be designed and implemented to obtain the values of the magnetic field at these positions. However, such interpolation process faces serious difficulties. Indeed, the size of the interpolation region is excessive for a linear interpolation to be reliable while, on the other hand, the number of magnetometer channels does not provide sufficient data to go beyond the linear approximation. We describe an alternative method to address this issue, by means of neural network algorithms. The key point in this approach is the ability of neural networks to learn from suitable training data representing t...

  10. The Australian Square Kilometre Array Pathfinder: Performance of the Boolardy Engineering Test Array

    CERN Document Server

    McConnell, D; Bannister, K; Bell, M E; Bignall, H E; Chippendale, A P; Edwards, P G; Harvey-Smith, L; Hegarty, S; Heywood, I; Hotan, A W; Indermuehle, B T; Lenc, E; Marvil, J; Popping, A; Raja, W; Reynolds, J E; Sault, R J; Serra, P; Voronkov, M A; Whiting, M; Amy, S W; Axtens, P; Ball, L; Bateman, T J; Bock, D C -J; Bolton, R; Brodrick, D; Brothers, M; Brown, A J; Bunton, J D; Cheng, W; Cornwell, T; DeBoer, D; Feain, I; Gough, R; Gupta, N; Guzman, J C; Hampson, G A; Hay, S; Hayman, D B; Hoyle, S; Humphreys, B; Jacka, C; Jackson, C A; Jackson, S; Jeganathan, K; Joseph, J; Koribalski, B S; Leach, M; Lensson, E S; MacLeod, A; Mackay, S; Marquarding, M; McClure-Griffiths, N M; Mirtschin, P; Mitchell, D; Neuhold, S; Ng, A; Norris, R; Pearce, S; Qiao, R Y; Schinckel, A E T; Shields, M; Shimwell, T W; Storey, M; Troup, E; Turner, B; Tuthill, J; Tzioumis, A; Wark, R M; Westmeier, T; Wilson, C; Wilson, T

    2016-01-01

    We describe the performance of the Boolardy Engineering Test Array (BETA), the prototype for the Australian Square Kilometre Array Pathfinder telescope ASKAP. BETA is the first aperture synthesis radio telescope to use phased array feed technology, giving it the ability to electronically form up to nine dual-polarization beams. We report the methods developed for forming and measuring the beams, and the adaptations that have been made to the traditional calibration and imaging procedures in order to allow BETA to function as a multi-beam aperture synthesis telescope. We describe the commissioning of the instrument and present details of BETA's performance: sensitivity, beam characteristics, polarimetric properties and image quality. We summarise the astronomical science that it has produced and draw lessons from operating BETA that will be relevant to the commissioning and operation of the final ASKAP telescope.

  11. EUSO-BALLOON a pathfinder for detecting UHECR's from the edge of space

    Directory of Open Access Journals (Sweden)

    Scotti V.

    2013-06-01

    Full Text Available EUSO-Balloon has been conceived as a pathfinder mission for JEM-EUSO, to perform an end-to-end test of the subsystems and components, and to prove the global detection chain while improving our knowledge of the atmospheric and terrestrial UV background. Through a series of stratospheric balloon flights performed by the French Space Agency CNES, EUSO-BALLOON will serve as an evolutive test-bench for all the key technologies of JEM-EUSO. EUSO-Balloon also has the potential to detect Extensive Air Showers from above, marking a key milestone in the development of UHECR science, and paving the way for any future large scale, space-based UHECR observatory.

  12. Pathfinder: multiresolution region-based searching of pathology images using IRM.

    Science.gov (United States)

    Wang, J Z

    2000-01-01

    The fast growth of digitized pathology slides has created great challenges in research on image database retrieval. The prevalent retrieval technique involves human-supplied text annotations to describe slide contents. These pathology images typically have very high resolution, making it difficult to search based on image content. In this paper, we present Pathfinder, an efficient multiresolution region-based searching system for high-resolution pathology image libraries. The system uses wavelets and the IRM (Integrated Region Matching) distance. Experiments with a database of 70,000 pathology image fragments have demonstrated high retrieval accuracy and high speed. The algorithm can be combined with our previously developed wavelet-based progressive pathology image transmission and browsing algorithm and is expandable for medical image databases.

  13. Hierarchical Pathfinding and AI-Based Learning Approach in Strategy Game Design

    Directory of Open Access Journals (Sweden)

    Le Minh Duc

    2008-01-01

    Full Text Available Strategy game and simulation application are an exciting area with many opportunities for study and research. Currently most of the existing games and simulations apply hard coded rules so the intelligence of the computer generated forces is limited. After some time, player gets used to the simulation making it less attractive and challenging. It is also costly and tedious to incorporate new rules for an existing game. The main motivation behind this research project is to improve the quality of artificial intelligence- (AI- based on various techniques such as qualitative spatial reasoning (Forbus et al., 2002, near-optimal hierarchical pathfinding (HPA* (Botea et al., 2004, and reinforcement learning (RL (Sutton and Barto, 1998.

  14. Thermo-elastic induced phase noise in the LISA Pathfinder spacecraft

    CERN Document Server

    Gibert, Ferran; Karnesis, Nikolaos; Gesa, Lluís; Martín, Víctor; Mateos, Ignacio; Lobo, Alberto; Flatscher, Reinhold; Gerardi, Domenico; Burkhardt, Johannes; Guzmán, Felipe; Heinzel, Gerhard; Danzmann, Karsten

    2014-01-01

    During the On-Station Thermal Test campaign of the LISA Pathfinder the data and diagnostics subsystem was tested in nearly space conditions for the first time after integration in the satellite. The results showed the compliance of the temperature measurement system, obtaining temperature noise around $10^{-4}\\,{\\rm K}\\, {\\rm Hz}^{-1/2}$ in the frequency band of $1-30\\;{\\rm mHz}$. In addition, controlled injection of heat signals to the suspension struts anchoring the LISA Technology Package (LTP) Core Assembly to the satellite structure allowed to experimentally estimate for the first time the phase noise contribution through thermo-elastic distortion of the LTP interferometer, the satellite's main instrument. Such contribution was found to be at $10^{-12}\\,{\\rm m}\\, {\\rm Hz}^{-1/2}$, a factor of 30 below the measured noise at the lower end of the measurement bandwidth ($1\\,{\\rm mHz}$).

  15. Pathfinding the Flight Advanced Stirling Convertor Design with the ASC-E3

    Science.gov (United States)

    Wong, Wayne A.; Wilson, Kyle; Smith, Eddie; Collins, Josh

    2012-01-01

    The Advanced Stirling Convertor (ASC) was initially developed by Sunpower, Inc. under contract to NASA Glenn Research Center (GRC) as a technology development project. The ASC technology fulfills NASA's need for high efficiency power convertors for future Radioisotope Power Systems (RPS). Early successful technology demonstrations between 2003 to 2005 eventually led to the expansion of the project including the decision in 2006 to use the ASC technology on the Advanced Stirling Radioisotope Generator (ASRG). Sunpower has delivered 22 ASC convertors of progressively mature designs to date to GRC. Currently, Sunpower with support from GRC, Lockheed Martin Space System Company (LMSSC), and the Department of Energy (DOE) is developing the flight ASC-F in parallel with the ASC-E3 pathfinders. Sunpower will deliver four pairs of ASC-E3 convertors to GRC which will be used for extended operation reliability assessment, independent validation and verification testing, system interaction tests, and to support LMSSC controller verification. The ASC-E3 and -F convertors are being built to the same design and processing documentation and the same product specification. The initial two pairs of ASC-E3 are built before the flight units and will validate design and processing changes prior to implementation on the ASC-F flight convertors. This paper provides a summary on development of the ASC technology and the status of the ASC-E3 build and how they serve the vital pathfinder role ahead of the flight build for ASRG. The ASRG is part of two of the three candidate missions being considered for selection for the Discovery 12 mission.

  16. Using Pathfinder Networks to Discover Alignment between Expert and Consumer Conceptual Knowledge from Online Vaccine Content.

    Science.gov (United States)

    Amith, Muhammad; Cunningham, Rachel; Savas, Lara S; Boom, Julie; Schvaneveldt, Roger; Tao, Cui; Cohen, Trevor

    2017-08-17

    This study demonstrates the use of distributed vector representations and Pathfinder Network Scaling (PFNETS) to represent online vaccine content created by health experts and by laypeople. By analyzing a target audience's conceptualization of a topic, domain experts can develop targeted interventions to improve the basic health knowledge of consumers. The underlying assumption is that the content created by different groups reflects the mental organization of their knowledge. Applying automated text analysis to this content may elucidate differences between the knowledge structures of laypeople (heath consumers) and professionals (health experts). This paper utilizes vaccine information generated by laypeople and health experts to investigate the utility of this approach. We used an established technique from cognitive psychology, Pathfinder Network Scaling to infer the structure of the associational networks between concepts learned from online content using methods of distributional semantics. In doing so, we extend the original application of PFNETS to infer knowledge structures from individual participants, to infer the prevailing knowledge structures within communities of content authors. The resulting graphs reveal opportunities for public health and vaccination education experts to improve communication and intervention efforts directed towards health consumers. Our efforts demonstrate the feasibility of using an automated procedure to examine the manifestation of conceptual models within large bodies of free text, revealing evidence of conflicting understanding of vaccine concepts among health consumers as compared with health experts. Additionally, this study provides insight into the differences between consumer and expert abstraction of domain knowledge, revealing vaccine-related knowledge gaps that suggest opportunities to improve provider-patient communication. Copyright © 2017. Published by Elsevier Inc.

  17. Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results.

    Science.gov (United States)

    Armano, M; Audley, H; Auger, G; Baird, J T; Bassan, M; Binetruy, P; Born, M; Bortoluzzi, D; Brandt, N; Caleno, M; Carbone, L; Cavalleri, A; Cesarini, A; Ciani, G; Congedo, G; Cruise, A M; Danzmann, K; de Deus Silva, M; De Rosa, R; Diaz-Aguiló, M; Di Fiore, L; Diepholz, I; Dixon, G; Dolesi, R; Dunbar, N; Ferraioli, L; Ferroni, V; Fichter, W; Fitzsimons, E D; Flatscher, R; Freschi, M; García Marín, A F; García Marirrodriga, C; Gerndt, R; Gesa, L; Gibert, F; Giardini, D; Giusteri, R; Guzmán, F; Grado, A; Grimani, C; Grynagier, A; Grzymisch, J; Harrison, I; Heinzel, G; Hewitson, M; Hollington, D; Hoyland, D; Hueller, M; Inchauspé, H; Jennrich, O; Jetzer, P; Johann, U; Johlander, B; Karnesis, N; Kaune, B; Korsakova, N; Killow, C J; Lobo, J A; Lloro, I; Liu, L; López-Zaragoza, J P; Maarschalkerweerd, R; Mance, D; Martín, V; Martin-Polo, L; Martino, J; Martin-Porqueras, F; Madden, S; Mateos, I; McNamara, P W; Mendes, J; Mendes, L; Monsky, A; Nicolodi, D; Nofrarias, M; Paczkowski, S; Perreur-Lloyd, M; Petiteau, A; Pivato, P; Plagnol, E; Prat, P; Ragnit, U; Raïs, B; Ramos-Castro, J; Reiche, J; Robertson, D I; Rozemeijer, H; Rivas, F; Russano, G; Sanjuán, J; Sarra, P; Schleicher, A; Shaul, D; Slutsky, J; Sopuerta, C F; Stanga, R; Steier, F; Sumner, T; Texier, D; Thorpe, J I; Trenkel, C; Tröbs, M; Tu, H B; Vetrugno, D; Vitale, S; Wand, V; Wanner, G; Ward, H; Warren, C; Wass, P J; Wealthy, D; Weber, W J; Wissel, L; Wittchen, A; Zambotti, A; Zanoni, C; Ziegler, T; Zweifel, P

    2016-06-10

    We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density of 5.2±0.1  fm s^{-2}/sqrt[Hz], or (0.54±0.01)×10^{-15}  g/sqrt[Hz], with g the standard gravity, for frequencies between 0.7 and 20 mHz. This value is lower than the LISA Pathfinder requirement by more than a factor 5 and within a factor 1.25 of the requirement for the LISA mission, and is compatible with Brownian noise from viscous damping due to the residual gas surrounding the test masses. Above 60 mHz the acceleration noise is dominated by interferometer displacement readout noise at a level of (34.8±0.3)  fm/sqrt[Hz], about 2 orders of magnitude better than requirements. At f≤0.5  mHz we observe a low-frequency tail that stays below 12  fm s^{-2}/sqrt[Hz] down to 0.1 mHz. This performance would allow for a space-based gravitational wave observatory with a sensitivity close to what was originally foreseen for LISA.

  18. Mesure de la fraction d'evenements a quatre quarks dans les desintegrations multihadroniques du boson Z au LEP

    Science.gov (United States)

    Lefebvre, Eric

    Cette thèse propose de tester la Chromodynamique Quantique (QCD) en effectuant une mesure précise d'une des trois constantes fondamentales du groupe de symétrie SU(3) utilisé pour décrire la physique des interactions fortes. Cette constante fondamentale, appelée TF, est reliée à certains états finaux spécifiques des désintégrations du Z0. Ces états apparaissent sous forme de perturbations du deuxième ordre en as et sont illustrés par des diagrammes de Feynman. À cet ordre, la chromodynamique prévoit deux types de diagrammes de Feynman distincts; le premier contient, un quark, un antiquark et deux gluons, et le second, deux quarks et deux antiquarks. La constante TF est directement proportionnelle à la fraction d'événements à deux quarks et deux antiquarks qui est l'objet de notre mesure. Notre mesure est fondée sur l'étude des événements à quatre partons dans l'état final. Ces quatre partons, en s'hadronisant, produisent quatre jets de particules qui peuvent être détectés expérimentalement et identifiés à l'aide d'algorithmes de reconstruction des jets. Des observables angulaires nous permettent de faire une discrimination parmi les états finaux de la désintégration du Z0, et ainsi déterminer la valeur de la fraction d'événements à deux quarks et deux antiquarks fq. Cette fraction peut s'exprimer par le rapport de la fraction observée expérimentalement fexq sur la fraction théorique fthq , R4q=fex qfthq. Afin d'améliorer la mesure de cette fraction et de diminuer le bruit causé par une contamination des événements d'ordres supérieurs, nous avons développe une méthode d'extrapolation. Cette méthode s'appuie sur la caractérisation de l'espace de phase des événements, exprimée par les paramètres yij. Les mesures de R4q que nous obtenons sont: R4q=2,27+0,29 -0,56 à l'aide d'une méthode conventionnelle avec la condition de sélection y34 > 0,020 > y45, et R4q=1,22+0,56 -0,71 à l'aide de notre méthode d

  19. Science Programs for a 2-m Class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope

    National Research Council Canada - National Science Library

    J. S. Lawrence; M. C. B. Ashley; J. A. Bailey; C. Blake; T. R. Bedding; J. Bland-Hawthorn; I. A. Bond; K. Glazebrook; M. G. Hidas; G. Lewis; S. N. Longmore; S. T. Maddison; S. Mattila; V. Minier; S. D. Ryder; R. Sharp; C. H. Smith; J. W. V. Storey; C. G. Tinney; P. Tuthill; A. J. Walsh; W. Walsh; M. Whiting; T. Wong; D. Woods; P. C. M. Yock

    2005-01-01

    .... Pathfinder for an International Large Optical Telescope (PILOT) is a proposed 2 m telescope, to be built at Dome C in Antarctica, able to exploit these conditions for conducting astronomy at optical and infrared wavelengths...

  20. AVHRR Pathfinder Version 5.2 Level 3 Collated (L3C) Global 4km Sea Surface Temperature for 1981-2012

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The AVHRR Pathfinder Version 5.2 Sea Surface Temperature data set (PFV52) is a collection of global, twice-daily 4km sea surface temperature data produced in a...

  1. 4 km AVHRR Pathfinder v5.0 Global Day-Night Sea Surface Temperature Monthly and Yearly Averages, 1985-2009 (NODC Accession 0077816)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This data set contains a set of monthly and yearly global day-night sea surface temperature averages, derived from the AVHRR Pathfinder Version 5 sea surface...

  2. 4 km NODC/RSMAS AVHRR Pathfinder Version 5.0 and 5.1 Daily Harmonic Climatologies (1982-2008) (NODC Accession 0071181)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession contains a global, 4km daily sea surface temperature climatology derived from harmonic analysis of the AVHRR Pathfinder Version 5.0 and 5.1 sea...

  3. 4 km NODC/RSMAS AVHRR Pathfinder Version 5.0 and 5.1 Monthly Harmonic Climatologies (1982-2008) (NODC Accession 0075098)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession contains a global, 4km monthly sea surface temperature climatology derived from harmonic analysis of the AVHRR Pathfinder Version 5.0 and 5.1 sea...

  4. NOAA Climate Data Record (CDR) of Reflectance and Brightness Temperatures from AVHRR Pathfinder Atmospheres - Extended (PATMOS-x), Version 5.3

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This NOAA Climate Data Record (CDR) of AVHRR reflectance and brightness temperatures was produced by the University of Wisconsin using the AVHRR Pathfinder...

  5. New Insights into the Geology of the Mars Pathfinder Landing Site from Spectral and Morphologic Analysis of the 12-Color Superpan Panorama

    Science.gov (United States)

    Murchie, S.; Barnouin-Jha, O.; Barnouin-Jha, K.; Bishop, J.; Johnson, J.; McSween, H.; Morris, R.

    2003-07-01

    The Pathfinder landing site contains a second lithology in addition to gray rock, consistent with highlands excavated from beneath a veneer of northern plains. Many rocks have cemented coatings that formed during an early, probably wetter climate.

  6. Arapaho National Wildlife Refuge also Bamforth, Hutton Lake, Morenson Lake and Pathfinder National Wildlife Refuges: Annual narrative report: Calendar year 1997

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, Morenson Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 1997...

  7. 4 km NODC/RSMAS AVHRR Pathfinder Version 5.0 and 5.1 5-day Harmonic Climatologies (1982-2008) (NODC Accession 0071182)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession contains a global, 4km 5-day sea surface temperature climatology derived from harmonic analysis of the AVHRR Pathfinder Version 5.0 and 5.1 sea...

  8. Arapaho National Wildlife Refuge also Bamforth, Hutton Lake, Morenson Lake and Pathfinder National Wildlife Refuges: Annual narrative report: Calendar year 1995

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, Morenson Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 1995...

  9. Arapaho National Wildlife Refuge also Bamforth, Hutton Lake, Morenson Lake and Pathfinder National Wildlife Refuges: Annual narrative report: Calendar year 1994

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, Morenson Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 1994...

  10. Arapaho National Wildlife Refuge also Bamforth, Hutton Lake, Morenson Lake and Pathfinder National Wildlife Refuges: Annual narrative report: Calendar year 1993

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — This annual narrative report for Arapaho NWR, Bamforth NWR, Hutton Lake NWR, Morenson Lake NWR, and Pathfinder NWR outlines Refuge accomplishments during the 1993...

  11. Quality Assurance statistics for AVHRR Pathfinder Version 5.2 L3-Collated (L3C) sea surface temperature in global and selected regions (NODC Accession 0111871)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — These quality monitoring data for Pathfinder Version 5.2 (PFV5.2) Sea Surface Temperature (SST) are based on the concept of a Rich Inventory developed by the...

  12. La mesure des performances corporelles extraordinaires dans les métiers du sport, du luxe et de l’art

    Directory of Open Access Journals (Sweden)

    Stéphane Héas

    2009-10-01

    Full Text Available La mesure des performances est aujourd’hui omniprésente dans les sports. Cette quantification corporelle n’étonne plus outre mesure. Elle est devenue sociologique. Les affaires de dopage ne fragilisent pas cette tendance. Les performances sportives de l’élite mondiale sont devenues très éloignées de ce que le commun des mortels peut envisager. Elles sont incroyables et pourtant réelles. Parfois, une fraction de seconde seulement sépare le bonheur de la victoire de la désillusion d’une défaite. En dehors des arènes sportives, d’autres performances sont réalisées. C’est le cas par exemple des équilibristes, des «nez» dans de nombreux secteurs (viniculture, cosmétique, etc., des contorsionnistes, des imitateurs, etc. A travers 21 entretiens, nous esquissons l’étendue des performances réalisées, donc leurs mesures multiples. Comment ces performances, le plus souvent chiffrées (en nombre de fragrances testées par jour, en minutes d’équilibre maintenu sur un rouleau, etc., sont-elles vécues? Les exercices et les excès corporels sont devenus leur quotidien, la mesure, leur étalon… qu’ils tentent de maintenir ou de varier avec l’âge, à mesure que leurs capacités déclinent.

  13. Experiments and Spectral Studies of Martian Volcanic Rocks: Implications for the Origin of Pathfinder Rocks and Soils

    Science.gov (United States)

    Rutherford, Malcolm J.; Mustard, Jack; Weitz, Catherine

    2002-01-01

    The composition and spectral properties of the Mars Pathfinder rocks and soils together with the identification of basaltic and andesitic Mars terrains based on Thermal Emission Spectrometer (TES) data raised interesting questions regarding the nature and origin of Mars surface rocks. We have investigated the following questions: (1) are the Pathfinder rocks igneous and is it possible these rocks could have formed by known igneous processes, such as equilibrium or fractional crystallization, operating within SNC magmas known to exist on Mars? If it is possible, what P (depth) and PH2O conditions are required? (2) whether TES-based interpretations of plagioclase-rich basalt and andesitic terrains in the south and north regions of Mars respectively are unique. Are the surface compositions of these regions plagioclase-rich, possibly indicating the presence of old AI-rich crust of Mars, or are the spectra being affected by something like surface weathering processes that might determine the spectral pyroxene to plagioclase ratio?

  14. Laboratory results and status update for Pathfinder, the LINC-NIRVANA NGS ground-layer AO subsystem

    Science.gov (United States)

    Kopon, Derek; Conrad, Al; Bertram, Thomas; Herbst, Tom; Kürster, Martin; Berwein, Juergen; Ragazzoni, Roberto; Farinato, Jacopo; Viotto, Valentina; Bergomi, Maria; Rohloff, Ralf-Rainer; Baumeister, Harald; De Bonis, Fulvio; Hofferbert, Ralph; Brunelli, Alessandro; Arcidiacono, Carmelo; Pott, Jörg-Uwe; Bizenberger, Peter; Briegel, Florian; Meschke, Daniel; Mohr, Lars; Zhang, Xianyu; Kittmann, Frank

    2013-12-01

    The full LINC-NIRVANA instrument will be one of the most complex ground-based astronomical systems ever built. It will consist of multiple subsystems, including two multi-conjugate ground layer AO systems (MCAO) that drive the LBT adaptive secondaries, two mid-high layer AO systems with their own Xynetics 349 actuator DM's, a fringe tracker, and a beam combiner. In order to mitigate risk, we take a modular approach to instrument testing and commissioning by decoupling these subsystems individually. The first subsystem tested on-sky will be one of the ground-layer AO systems, part of a test-bed known as the Pathfinder. The Pathfinder consists of a 12-star pyramid WFS that drives one of the LBT's adaptive secondaries, a support structure known as "The Foot," and the infrared test camera (IRTC), which is used for acquisition and alignment. The 12 guide stars are acquired by moveable arms called "star enlargers," each of which contains its own optical path. The Pathfinder will be shipped from MPIA in Heidelberg, Germany to the LBT mountain lab on Mt. Graham, Arizona in February. The system will be unpacked, assembled in the LBT clean room, and internally optically aligned. We present the results of our system tests, including star enlarger alignment and system alignment. We also present our immediate plans for on-sky closed loop tests on the LBT scheduled for early Fall. Because plans for all ELTs call for ground layer correction, the Pathfinder provides valuable preliminary information not only for the full LINC-NIRVANA system, but also for future advanced MCAO systems.

  15. Pathfinder first light: alignment, calibration, and commissioning of the LINC-NIRVANA ground-layer adaptive optics subsystem

    Science.gov (United States)

    Kopon, Derek; Conrad, Al; Arcidiacono, Carmelo; Herbst, Tom; Viotto, Valentina; Farinato, Jacopo; Bergomi, Maria; Ragazzoni, Roberto; Marafatto, Luca; Baumeister, Harald; Bertram, Thomas; Berwein, Jürgen; Briegel, Florian; Hofferbert, Ralph; Kittmann, Frank; Kürster, Martin; Mohr, Lars; Radhakrishnan, Kalyan

    2014-08-01

    We present descriptions of the alignment and calibration tests of the Pathfinder, which achieved first light during our 2013 commissioning campaign at the LBT. The full LINC-NIRVANA instrument is a Fizeau interferometric imager with fringe tracking and 2-layer natural guide star multi-conjugate adaptive optics (MCAO) systems on each eye of the LBT. The MCAO correction for each side is achieved using a ground layer wavefront sensor that drives the LBT adaptive secondary mirror and a mid-high layer wavefront sensor that drives a Xinetics 349 actuator DM conjugated to an altitude of 7.1 km. When the LINC-NIRVANA MCAO system is commissioned, it will be one of only two such systems on an 8-meter telescope and the only such system in the northern hemisphere. In order to mitigate risk, we take a modular approach to commissioning by decoupling and testing the LINC-NIRVANA subsystems individually. The Pathfinder is the ground-layer wavefront sensor for the DX eye of the LBT. It uses 12 pyramid wavefront sensors to optically co-add light from natural guide stars in order to make four pupil images that sense ground layer turbulence. Pathfinder is now the first LINC-NIRVANA subsystem to be fully integrated with the telescope and commissioned on sky. Our 2013 commissioning campaign consisted of 7 runs at the LBT with the tasks of assembly, integration and communication with the LBT telescope control system, alignment to the telescope optical axis, off-sky closed loop AO calibration, and finally closed loop on-sky AO. We present the programmatics of this campaign, along with the novel designs of our alignment scheme and our off-sky calibration test, which lead to the Pathfinder's first on-sky closed loop images.

  16. Apical root canal transportation of different pathfinding systems and their effects on shaping ability of ProTaper Next

    OpenAIRE

    Turker, Sevinc Aktemur; Uzunoglu, Emel

    2015-01-01

    Background This study aimed to compare glide path preparation of different pathfinding systems and their effects on the apical transportation of ProTaper Next (Dentsply Maillefer, Ballaigues, Switzerland) in mesial root canals of extracted human mandibular molars, using digital subtraction radiography. Material and Methods The mesial canals of 40 mandibular first molars (with curvature angles between 25° and 35°) were selected for this study. The specimens were divided randomly into 4 groups ...

  17. William Herschel Telescope site characterization using the MOAO pathfinder CANARY on-sky data

    Science.gov (United States)

    Martin, O. A.; Correia, C. M.; Gendron, E.; Rousset, G.; Vidal, F.; Morris, T. J.; Basden, A. G.; Myers, R. M.; Ono, Y. H.; Neichel, B.; Fusco, T.

    2016-07-01

    CANARY is the Multi-Object Adaptive Optics (MOAO) pathfinder for the future MOAO-assisted Integral-Field Units (IFU) proposed for Extremely Large Telescopes (ELT). The MOAO concept relies on tomographically reconstructing the turbulence using multiple measurements along different lines of sight. Tomography requires the knowledge of the statistical turbulence parameters, commonly recovered from the system telemetry using a dedicated profiling technique. For demonstration purposes with the MOAO pathfinder CANARY, this identification is performed thanks to the Learn & Apply (L&A) algorithm, that consists in model-fitting the covariance matrix of WFS measurements dependant on relevant parameters: Cn2(h) profile, outer scale profile and system mis-registration. We explore an upgrade of this algorithm, the Learn 3 Steps (L3S) approach, that allows one to dissociate the identification of the altitude layers from the ground in order to mitigate the lack of convergence of the required empirical covariance matrices therefore reducing the required length of data time-series for reaching a given accuracy. For nominal observation conditions, the L3S can reach the same level of tomographic error in using five times less data frames than the L&A approach. The L3S technique has been applied over a large amount of CANARY data to characterize the turbulence above the William Herschel Telescope (WHT). These data have been acquired the 13th, 15th, 16th, 17th and 18th September 2013 and we find 0.67"/8.9m/3.07m.s-1 of total seeing/outer scale/wind-speed, with 0.552"/9.2m/2.89m.s-1 below 1.5 km and 0.263"/10.3m/5.22m.s-1 between 1.5 and 20 km. We have also determined the high altitude layers above 20 km, missed by the tomographic reconstruction on CANARY , have a median seeing of 0.187" and have occurred 16% of observation time.

  18. Selection and Assessment of Predictions of the Mars Pathfinder Landing Site

    Science.gov (United States)

    Golombek, M. P.; Moore, H. J.; Haldemann, A. F. C.; Cook, R. A.; Parker, T. J.; Schofield, J. T.

    1998-01-01

    The successful landing of the Mars Pathfinder spacecraft on Mars allows the review of the process of selecting the landing site and assessing predictions made for the site based on Viking and Earth-based data. Selection of the landing site for Mars Pathfinder was a two-phase process. The first phase took place from October 1993 to June 1994 and involved: initial identification of engineering constraints, definition of environmental conditions at the site for spacecraft design, and evaluation of the scientific potential of different landing sites. This phase culminated with the first "Mars Pathfinder Landing Site Workshop", held at the Lunar and Planetary Institute in Houston, Texas on April 18-19, 1994, in which suggested approaches and landing sites were solicited from the entire scientific community. A preliminary site was selected by the project for design purposes in June 1994. The second phase took place from July 1994 to March 1996 and involved: developing criteria for evaluating site safety using images and remote sensing data, testing of the spacecraft and landing subsystems (with design improvements) to establish quantitative engineering constraints on landing site characteristics, evaluating all potential landing sites on Mars, and certification of the site by the project. This phase included a second open workshop, "Mars Pathfinder Landing Site Workshop II: Characteristics of the Ares Vallis Region and Field Trips in the Channeled Scabland, Washington" held in Spokane and Moses Lake September 24-30, 1995 and formal acceptance of the site by NASA Headquarters. Engineering constraints on Pathfinder landing sites were developed from the initial design of the spacecraft and the entry, descent and landing scenario. The site must be within 5 degrees of the subsolar latitude at the time of landing (15N for maximum solar power and flexible communications with Earth. It also must be below 0 km elevation to enable enough time for the parachute to bring the lander

  19. Techniques for the measurement of the contamination of air; Technique de mesure de la contamination de l'air

    Energy Technology Data Exchange (ETDEWEB)

    Labeyrie, J. [Commissariat a l' Energie Atomique, Saclay (France).Centre d' Etudes Nucleaires

    1960-07-01

    This lecture has been given at the International Symposium of Riso 1959. Methods for measuring radioactive content of the atmosphere are described, and main results found at Saclay are given, for the following contaminants: Rn, Tn and their daughter, H-3, C-14, A-41, Kr-85, I-131, and fission products as a whole. (author) [French] Ce texte est celui d'une conference-rapport prononcee au Colloque International de Riso en 1959. On indique les techniques de mesures de la contamination radioactive de l'atmosphere et les principaux resultats obtenus jusqu'ici au CEA pour: Rn et Tn et leurs derives, H-3, C-14, A-41, Kr-85, I-131, et l'ensemble des produits de fission. (auteur)

  20. Radiation measurements in the reactors G 2 and G 3; Mesures de rayonnement aupres des piles G 2 - G 3

    Energy Technology Data Exchange (ETDEWEB)

    Chassany, J.Ph.; Estournel, R. [Commissariat a l' Energie Atomique, Centre de Production de Plutonium, Marcoule (France). Centre d' Etudes Nucleaires

    1964-07-01

    The results are given of numerous radiation measurements: - for the various working sites - for the various zones (circuit room,etc) - during the discharging operations - far various active materials (CO{sub 2}, plugs etc). They show that in general the protection has been suitably designed and that the majority of radio-protection problems are due to the elements activated in the pile and transported outside the vessel. (authors) [French] Les resultats de nombreuses mesures d'irradiation sont donnes - pour les differents lieux de travail - pour diverses zones (salle de tuyauteries, etc.) - pendant les operations de dechargement - pour differents materiaux actives (CO{sub 2}, bouchons, etc.) Ils montrent que les protections ont ete en general correctement dimensionnees et que la majorite des problemes de radioprotection est constituee par les elements actives dans la pile, transportes a l'exterieur du caisson. (auteurs)

  1. Mesure de la qualité des services d’enseignement et restructuration des secteurs éducatifs

    OpenAIRE

    Vinokur, Annie

    2012-01-01

    L’article de Romuald Normand a décrit la genèse, aux États-Unis, du mouvement de mobilisation des technologies de mesure de la qualité pour rationaliser la pédagogie scolaire sur le modèle industriel. Ce modèle tend maintenant à s’étendre à l’évaluation de la qualité des producteurs de services d’enseignement et à se déployer à l’échelle mondiale dans le but d’accroître l’efficacité des secteurs éducatifs et de réguler leur transnationalisation. On tente ici d’en montrer la fonctionnalité – m...

  2. Evaluation mécanique d'une dalle précontrainte par mesure de la courbure

    OpenAIRE

    COLLIN, B; TONNOIR, B

    2001-01-01

    L'évaluation mécanique d'un ouvrage d'art a été réalisée en utilisant conjointement, et pour la première fois sur une dalle isostatique en béton précontraint, deux prototypes de courburemètre du réseau des LPC. Cette évaluation s'est appuyée sur des mesures, faites en plusieurs sections, des variations de courbure causées par la circulation sur l'ouvrage d'un convoi de caractéristiques connues. D'un point de vue pratique, la facilité d'utilisation des courburemètres, simplement posés sur la c...

  3. Mesure Objective De L'attenuation et De L'effet D'occlusion Des Protecteurs Auditifs a Partir Des Potentiels Evoques Stationnaires et Multiples =

    Science.gov (United States)

    Valentin, Olivier

    Selon l'Organisation mondiale de la sante, le nombre de travailleurs exposes quotidiennement a des niveaux de bruit prejudiciables a leur audition est passe de 120 millions en 1995 a 250 millions en 2004. Meme si la reduction du bruit a la source devrait etre toujours privilegiee, la solution largement utilisee pour lutter contre le bruit au travail reste la protection auditive individuelle. Malheureusement, le port des protecteurs auditifs n'est pas toujours respecte par les travailleurs car il est difficile de fournir un protecteur auditif dont le niveau d'attenuation effective est approprie a l'environnement de travail d'un individu. D'autre part, l'occlusion du canal auditif induit une modification de la perception de la parole, ce qui cree un inconfort incitant les travailleurs a retirer leurs protecteurs. Ces deux problemes existent parce que les methodes actuelles de mesure de l'effet d'occlusion et de l'attenuation sont limitees. Les mesures objectives basees sur des mesures microphoniques intra-auriculaires ne tiennent pas compte de la transmission directe du son a la cochlee par conduction osseuse. Les mesures subjectives au seuil de l'audition sont biaisees a cause de l'effet de masquage aux basses frequences induit par le bruit physiologique. L'objectif principal de ce travail de these de doctorat est d'ameliorer la mesure de l'attenuation et de l'effet d'occlusion des protecteurs auditifs intra-auriculaires. L'approche generale consiste a : (i) verifier s'il est possible de mesurer l'attenuation des protecteurs auditifs grâce au recueil des potentiels evoques stationnaires et multiples (PEASM) avec et sans protecteur auditif (protocole 1), (ii) adapter cette methodologie pour mesurer l'effet d'occlusion induit par le port de protecteur auditifs intra-auriculaires (protocole 2), et (iii) valider chaque protocole par l'intermediaire de mesures realisees sur sujets humains. Les resultats du protocole 1 demontrent que les PEASM peuvent etre utilises pour

  4. SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results

    CERN Document Server

    Dolag, Klaus; Sunyaev, Rashid

    2015-01-01

    We calculate the one-point probability density distribution functions (PDF) and the power spectra of the thermal and kinetic Sunyaev-Zeldovich (tSZ and kSZ) effects and the mean Compton Y parameter using the Magneticum Pathfinder simulations, state-of-the-art cosmological hydrodynamical simulations of a large cosmological volume of (896 Mpc/h)^3. These simulations follow in detail the thermal and chemical evolution of the intracluster medium as well as the evolution of super-massive black holes and their associated feedback processes. We construct full-sky maps of tSZ and kSZ from the light-cones out to z=0.17, and one realization of 8.8x8.8 degree wide, deep light-cone out to z=5.2. The local universe at z=1.18x10^{-6} for \\Omega_m=0.272 and \\sigma_8=0.809. Nearly half (~ 5x10^{-7}) of the signal comes from halos below a virial mass of 10^{13}M_\\odot/h. Scaling this to the Planck 2015 parameters, we find =1.57x10^{-6}. The PDF and the power spectrum of kSZ from our simulation agree broadly with the previous ...

  5. PETER: A Hardware Simulator for the Test Mass-GRS System of LISA Pathfinder

    Science.gov (United States)

    Marconi, L.; Stanga, R.; Bassan, M.; De Marchi, F.; Pucacco, G.; Visco, M.; Di Fiore, L.; De Rosa, R.; Garufi, F.

    2013-01-01

    Each LISA PathFinder test mass (TM) will be sensitive to forces along all its 6 Degrees of Freedom (DoFs). Extensive ground testing is required in order to evaluate the influence of cross-talks from the read-out and actuator channels. In the INFN laboratory of Firenze we have developed a facility for a good representation of the free fall conditions of the TM on flight. A hollow replica of a TM hanging from a double torsion pendulum can move inside a Gravitational Reference Sensor (GRS) with quasi free fall condition on two Dofs, in the frequency band (0.1 ÷ 100)mHz. On both DoFs, the target residual accelerations (yet to be achieved) at the low end frequency range are ≤ 3 × 10-13ms-2, limited by the thermal noise of the fibres. At higher frequencies, the sensitivity is limited by the readout noise of the readout, a replica of the flight electronics. After a long commissioning, we are now in operating conditions, and can carry out a series of experiments to better qualify the interaction between TM and GRS. In this paper we will show some significant qualification measurements and a first scientific measurements, i.e. the measurement and compensation of the DC bias in the GRS using two independent channels, as well as a measurement of the residual acceleration of the translational DoF, with the feedback loop closed on the rotational one, and viceversa.

  6. SISTINE: a pathfinder for FUV imaging spectroscopy on future NASA astrophysics missions

    Science.gov (United States)

    Fleming, Brian T.; France, Kevin; Nell, Nicholas; Kruczek, Nicholas; Kane, Robert; Green, James; Quijada, Manuel A.; Del Hoyo, Javier; Siegmund, Oswald

    2016-07-01

    The University of Colorado ultraviolet sounding rocket program presents the motivation and design capabilities of the new Suborbital Imaging Spectrograph for Transition Region Irradiance from Nearby Exoplanet host stars (SISTINE). SISTINE is a pathfinder for future UV space instrumentation, incorporating advanced broadband refl ective mirror coatings and large format borosilicate microchannel plate detectors that address technology gaps identified by the NASA Cosmic Origins program. The optical design capitalizes on new capabilities enabled by these technologies to demonstrate optical pathlengths in a sounding rocket envelope that would otherwise require a prohibitive effective area penalty in the 1020 - 1150 Å bandpass. This enables SISTINE to achieve high signal-to-noise observations of emission lines from planet-hosting dwarf stars with moderate spectral resolution (R 10,000) and sub-arcsecond angular imaging. In this proceedings, we present the scientific motivation for a moderate resolution imaging spectrograph, the design of SISTINE, and the enabling technologies that make SISTINE, and future advanced FUV-sensitive instrumentation, possible.

  7. A torsion pendulum ground test of the LISA Pathfinder Free-fall mode

    CERN Document Server

    Russano, Giuliana

    2016-01-01

    LISA Pathfinder is the technological demonstrator space mission for the future gravitational waves observatory in space eLISA, with the aim of measure the differential acceleration between free-falling test masses orbiting in the same apparatus at a level of 30 fm/s-2Hz-1/2 at 1 mHz. Because the satellite can't follow the two masses at the same time, the second mass must be forced to follow either the other one or the spacecraft. The actuation force applied to compensate this effect introduces a dominant source of force noise in the mission noise budget at frequency near and below the mHz. The free-fall mode actuation control scheme has been designed to suppress this noise source and avoid actuation instabilities: actuation is limited to brief periodic impulses, with test masses in free fall in between two kicks. This actuation-free motion is then analyzed for the remaining sources of acceleration ultra noise. A free-fall mode parallel testing has been successfully implemented on torsion pendulum facility at ...

  8. Constraints on LISA Pathfinder's self-gravity: design requirements, estimates and testing procedures

    CERN Document Server

    Ferroni, Valerio

    2016-01-01

    LISA Pathfinder satellite has been launched on 3th December 2015 toward the Sun-Earth first Lagrangian point (L1) where the LISA Technology Package (LTP), which is the main science payload, will be tested. With its cutting-edge technology, the LTP will provide the ability to achieve unprecedented geodesic motion residual acceleration measurements down to the order of $3 \\times 10^{-14}\\,\\mathrm{m/s^2/{Hz^{1/2}}}$ within the $1-30\\,\\mathrm{mHz}$ frequency band. The presence of the spacecraft itself is responsible of the local gravitational field which will interact with the two proof test-masses. Potentially, such a force interaction might prevent to achieve the targeted free-fall level originating a significant source of noise. We balanced this gravitational force with sub $\\mathrm{nm/s^2}$ accuracy, guided by a protocol based on measurements of the position and the mass of all parts that constitute the satellite, via finite element calculation tool estimates. In the following, we will introduce requirements,...

  9. OBSERVATION OF EARLY PHOTONS FROM GAMMA-RAY BURSTS WITH THE LOMONOSOV/UFFO-PATHFINDER

    Directory of Open Access Journals (Sweden)

    S. Jeong

    2014-01-01

    Full Text Available UFFO-pathfinder es la misi ́on pionera para observar la evoluci ́on temprana de los Estallidos de Rayos Gamma u s a n d o s u e s t r a t e g i a d e a p u n t a d o r ́ a p i d o . E s t ́ a e q u i p a d o c o n e l S l e w i n g M i r r o r T e l e s c o p e p a r a a p u n t a d o r ́ a p i d o en las longitudes de onda ́ Opticas y Ultravioleta, al mismo tiempo que tien e el telescopio de Estallidos y Alerta UFFO. Tiene un total de ∼ 20 kg de peso y ser ́a lanzado a bordo de un sat ́elite ruso al final del 2014. Los d e t a l l e s d e l i n s t r u m e n t o y s u d e s e m p e ̃ n o s o n d i s c u t i d o s b r e v e m e n t e a c ́ a.

  10. An Efficient Real-time Data Pipeline for the CHIME Pathfinder Radio Telescope X-Engine

    CERN Document Server

    Recnik, Andre; Denman, Nolan; Hincks, Adam D; Hinshaw, Gary; Klages, Peter; Vanderlinde, Keith

    2015-01-01

    The CHIME Pathfinder is a new interferometric radio telescope that uses a hybrid FPGA/GPU FX correlator. The GPU-based X-engine of this correlator processes over 819 Gb/s of 4+4-bit complex astronomical data from N=256 inputs across a 400 MHz radio band. A software framework is presented to manage this real-time data flow, which allows each of 16 processing servers to handle 51.2 Gb/s of astronomical data, plus 8 Gb/s of ancillary data. Each server receives data in the form of UDP packets from an FPGA F-engine over the eight 10 GbE links, combines data from these packets into large (32MB-256MB) buffered frames, and transfers them to multiple GPU co-processors for correlation. The results from the GPUs are combined and normalized, then transmitted to a collection server, where they are merged into a single file. Aggressive optimizations enable each server to handle this high rate of data; allowing the efficient correlation of 25 MHz of radio bandwidth per server. The solution scales well to larger values of N ...

  11. Alignment Test Results of the JWST Pathfinder Telescope Mirrors in the Cryogenic Environment

    Science.gov (United States)

    Whitman, Tony L.; Wells, Conrad; Hadaway, James; Knight, J. Scott; Lunt, Sharon

    2016-01-01

    After integration of the Optical Telescope Element (OTE) to the Integrated Science Instrument Module (ISIM) to become the OTIS, the James Webb Space Telescope OTIS is tested at NASAs Johnson Space Center (JSC) in the cryogenic vacuum Chamber A for alignment and optical performance. The alignment of the mirrors comprises a sequence of steps as follows: The mirrors are coarsely aligned using photogrammetry cameras with reflective targets attached to the sides of the mirrors. Then a multi-wavelength interferometer is aligned to the 18-segment primary mirror using cameras at the center of curvature to align reflected light from the segments and using fiducials at the edge of the primary mirror. Once the interferometer is aligned, the 18 primary mirror segments are then adjusted to optimize wavefront error of the aggregate mirror. This process phases the piston and tilt positions of all the mirror segments. An optical fiber placed at the Cassegrain focus of the telescope then emits light towards the secondary mirror to create a collimated beam emitting from the primary mirror. Portions of the collimated beam are retro-reflected from flat mirrors at the top of the chamber to pass through the telescope to the SI detector. The image on the detector is used for fine alignment of the secondary mirror and a check of the primary mirror alignment using many of the same analysis techniques used in the on-orbit alignment. The entire process was practiced and evaluated in 2015 at cryogenic temperature with the Pathfinder telescope.

  12. Theoretical foundations for on-ground tests of LISA PathFinder thermal diagnostics

    CERN Document Server

    Lobo, A; Ramos-Castro, J; Sanjuan, J; Lobo, Alberto; Nofrarias, Miquel; Ramos-Castro, Juan; Sanjuan, Josep

    2006-01-01

    This paper reports on the methods and results of a theoretical analysis to design an insulator which must provide a thermally quiet environment to test on ground delicate temperature sensors and associated electronics. These will fly on board ESA's LISA PathFinder (LPF) mission as part of the thermal diagnostics subsystem of the LISA Test-flight Package (LTP). We evaluate the heat transfer function (in frequency domain) of a central body of good thermal conductivity surrounded by a layer of a very poorly conducting substrate. This is applied to assess the materials and dimensions necessary to meet temperature stability requirements in the metal core, where sensors will be implanted for test. The analysis is extended to evaluate the losses caused by heat leakage through connecting wires, linking the sensors with the electronics in a box outside the insulator. The results indicate that, in spite of the very demanding stability conditions, a sphere of outer diameter of the order one metre is sufficient.

  13. Scientific Potential of DECIGO Pathfinder and Testing GR with Space-Borne Gravitational Wave Interferometers

    CERN Document Server

    Yagi, Kent

    2013-01-01

    DECIGO Pathfinder (DPF) has an ability to detect gravitational waves from galactic intermediate-mass black hole binaries. If the signal is detected, it would be possible to determine parameters of the binary components. Furthermore, by using future space-borne gravitational wave interferometers, it would be possible to test alternative theories of gravity in the strong field regime. In this review article, we first explain how the detectors like DPF and DECIGO/BBO work and discuss the expected event rates. Then, we review how the observed gravitational waveforms from precessing compact binaries with slightly eccentric orbits can be calculated both in general relativity and in alternative theories of gravity. For the latter, we focus on Brans-Dicke and massive gravity theories. After reviewing these theories, we show the results of the parameter estimation with DPF using the Fisher analysis. We also discuss a possible joint search of DPF and ground-based interferometers. Then, we show the results of testing al...

  14. Alignment test results of the JWST Pathfinder Telescope mirrors in the cryogenic environment

    Science.gov (United States)

    Whitman, Tony L.; Wells, Conrad; Hadaway, James B.; Knight, J. Scott; Lunt, Sharon

    2016-07-01

    After integration of the Optical Telescope Element (OTE) to the Integrated Science Instrument Module (ISIM) to become the OTIS, the James Webb Space Telescope OTIS is tested at NASA's Johnson Space Center (JSC) in the cryogenic vacuum Chamber A for alignment and optical performance. The alignment of the mirrors comprises a sequence of steps as follows: The mirrors are coarsely aligned using photogrammetry cameras with reflective targets attached to the sides of the mirrors. Then a multi-wavelength interferometer is aligned to the 18-segment primary mirror using cameras at the center of curvature to align reflected light from the segments and using fiducials at the edge of the primary mirror. Once the interferometer is aligned, the 18 primary mirror segments are then adjusted to optimize wavefront error of the aggregate mirror. This process phases the piston and tilt positions of all the mirror segments. An optical fiber placed at the Cassegrain focus of the telescope then emits light towards the secondary mirror to create a collimated beam emitting from the primary mirror. Portions of the collimated beam are retro-reflected from flat mirrors at the top of the chamber to pass through the telescope to the Science Instrument (SI) detector. The image on the detector is used for fine alignment of the secondary mirror and a check of the primary mirror alignment using many of the same analysis techniques used in the on-orbit alignment. The entire process was practiced and evaluated in 2015 at cryogenic temperature with the Pathfinder telescope.

  15. CubeSats as pathfinders for planetary detection: the FIRST-S satellite

    Science.gov (United States)

    Lacour, S.; Lapeyrère, V.; Gauchet, L.; Arroud, S.; Gourgues, R.; Martin, G.; Heidmann, S.; Haubois, X.; Perrin, G.

    2014-08-01

    The idea behind FIRST (Fibered Imager foR a Single Telescope) is to use single-mode fibers to combine multiple apertures in a pupil plane as such as to synthesize a bigger aperture. The advantages with respect to a pure imager are i) relaxed tolerance on the pointing and cophasing, ii) higher accuracy in phase measurement, and iii) availability of compact, precise, and active single-mode optics like Lithium Niobate. The latter point being a huge asset in the context of a space mission. One of the problems of DARWIN or SIM-like projects was the difficulty to find low cost pathfinders missions. But the fact that Lithium Niobate optic is small and compact makes it easy to test through small nanosats missions. Moreover, they are commonly used in the telecom industry, and have already been tested on communication satellites. The idea of the FIRST-S demonstrator is to spatialize a 3U CubeSat with a Lithium Niobate nulling interferometer. The technical challenges of the project are: star tracking, beam combination, and nulling capabilities. The optical baseline of the interferometer would be 30 cm, giving a 2.2AU spatial resolution at distance of 10 pc. The scientific objective of this mission would be to study the visible emission of exozodiacal light in the habitable zone around the closest stars.

  16. CubeSats as pathfinders for planetary detection: the FIRST-S satellite

    CERN Document Server

    Lacour, S; Gauchet, L; Arroud, S; Gourgues, R; Martin, G; Heidmann, S; Haubois, X; Perrin, G

    2014-01-01

    The idea behind FIRST (Fibered Imager foR a Single Telescope) is to use single-mode fibers to combine multiple apertures in a pupil plane as such as to synthesize a bigger aperture. The advantages with respect to a pure imager are i) relaxed tolerance on the pointing and cophasing, ii) higher accuracy in phase measurement, and iii) availability of compact, precise, and active single-mode optics like Lithium Niobate. The latter point being a huge asset in the context of a space mission. One of the problems of DARWIN or SIM-like projects was the difficulty to find low cost pathfinders missions. But the fact that Lithium Niobate optic is small and compact makes it easy to test through small nanosats missions. Moreover, they are commonly used in the telecom industry, and have already been tested on communication satellites. The idea of the FIRST-S demonstrator is to spatialize a 3U CubeSat with a Lithium Niobate nulling interferometer. The technical challenges of the project are: star tracking, beam combination, ...

  17. Concept of Science Data Management for the Korea Pathfinder Lunar Orbiter

    Science.gov (United States)

    Kim, Joo Hyeon

    2016-10-01

    South Korea has a plan to explore the Moon in 2018 or 2019. For the plan, the Korea Aerospace Research Institute which is a government funded research institute kicked off the Korea Lunar Exploration Development Program in January, 2016 in support of Ministry of Science, ICT and Future Planning, South Korea.As the 1st stage mission of the program, named as the Korea Pathfinder Lunar Orbiter(KPLO), will perform acquisition of high resolution images and science data for investigation of lunar environment as well as the core technology demonstration and validation for space explorations. The scientific instruments consists of three Korean domestic developed science instruments except an imaging instrument and several foreign provided instruments. We are developing a science data management plan to encourage scientific activities using science data acquired by the science instruments.I introduce the Korean domestic developed science instruments and present concept of the science data management plan for data delivery, processing, and distribution for the science instruments.

  18. Carboxypeptidase A6 in zebrafish development and implications for VIth cranial nerve pathfinding.

    Directory of Open Access Journals (Sweden)

    Peter J Lyons

    Full Text Available Carboxypeptidase A6 (CPA6 is an extracellular protease that cleaves carboxy-terminal hydrophobic amino acids and has been implicated in the defective innervation of the lateral rectus muscle by the VIth cranial nerve in Duane syndrome. In order to investigate the role of CPA6 in development, in particular its potential role in axon guidance, the zebrafish ortholog was identified and cloned. Zebrafish CPA6 was secreted and interacted with the extracellular matrix where it had a neutral pH optimum and specificity for C-terminal hydrophobic amino acids. Transient mRNA expression was found in newly formed somites, pectoral fin buds, the stomodeum and a conspicuous condensation posterior to the eye. Markers showed this tissue was not myogenic in nature. Rather, the CPA6 localization overlapped with a chondrogenic site which subsequently forms the walls of a myodome surrounding the lateral rectus muscle. No other zebrafish CPA gene exhibited a similar expression profile. Morpholino-mediated knockdown of CPA6 combined with retrograde labeling and horizontal eye movement analyses demonstrated that deficiency of CPA6 alone did not affect either VIth nerve development or function in the zebrafish. We suggest that mutations in other genes and/or enhancer elements, together with defective CPA6 expression, may be required for altered VIth nerve pathfinding. If mutations in CPA6 contribute to Duane syndrome, our results also suggest that Duane syndrome can be a chondrogenic rather than a myogenic or neurogenic developmental disorder.

  19. LISA Pathfinder test-mass charging during galactic cosmic-ray flux short-term variations

    Science.gov (United States)

    Grimani, C.; Fabi, M.; Lobo, A.; Mateos, I.; Telloni, D.

    2015-02-01

    Metal free-floating test masses aboard the future interferometers devoted to gravitational wave detection in space are charged by galactic and solar cosmic rays with energies \\gt 100 MeV/n. This process represents one of the main sources of noise in the lowest frequency band (\\lt 10-3 Hz) of these experiments. We study here the charging of the LISA Pathfinder (LISA-PF) gold-platinum test masses due to galactic cosmic-ray (GCR) protons and helium nuclei with the Fluka Monte Carlo toolkit. Projections of the energy spectra of GCRs during the LISA-PF operations in 2015 are considered. This work was carried out on the basis of the solar activity level and solar polarity epoch expected for LISA-PF. The effects of GCR short-term variations are evaluated here for the first time. Classical Forbush decreases, GCR variations induced by the Sun rotation, and fluctuations in the LISA-PF frequency bandwidth are discussed.

  20. SZ effects in the Magneticum Pathfinder simulation: comparison with the Planck, SPT, and ACT results

    Science.gov (United States)

    Dolag, K.; Komatsu, E.; Sunyaev, R.

    2016-12-01

    We calculate the one-point probability density distribution functions (PDF) and the power spectra of the thermal and kinetic Sunyaev-Zeldovich (tSZ and kSZ) effects and the mean Compton Y parameter using the Magneticum Pathfinder simulations, state-of-the-art cosmological hydrodynamical simulations of a large cosmological volume of (896 Mpc h-1)3. These simulations follow in detail the thermal and chemical evolution of the intracluster medium as well as the evolution of supermassive black holes and their associated feedback processes. We construct full-sky maps of tSZ and kSZ from the light-cones out to z = 0.17, and one realization of 8.8° × 8.8° deep light-cone out to z = 5.2. The local universe at z half (≈5 × 10-7) of the signal comes from haloes below a virial mass of 1013 M⊙ h-1. Scaling this to the Planck 2015 parameters, we find bar{Y}=1.57× {}10^{-6}.

  1. The LTP Experiment on LISA Pathfinder: Operational Definition of TT Gauge in Space

    CERN Document Server

    Armano, Michele

    2011-01-01

    The European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) are planning the Laser Interferometer Space Antenna (LISA) mission in order to detect GW. The need of accurate testing of free-fall and knowledge of noise in a space environment similar to LISA's is considered mandatory a pre-phase for the project. Therefore the LISA Pathfinder mission has been designed by ESA to fly the LISA Technology Package (LTP), aiming at testing free-fall by measuring the residual acceleration between two test-bodies in the dynamical scheme we address as "drag-free". The spectral map of the residual acceleration as function of frequency will convey information on the local noise level, thus producing a picture of the environmental working conditions for LISA itself. The thesis contains abundant material on the problem of compensating static gravity, the development of a theory of orthogonalization of reference and cross-talk for the LTP experiment. The construction of the laser detection proced...

  2. Selection and Assessment of Predictions of the Mars Pathfinder Landing Site

    Science.gov (United States)

    Golombek, M. P.; Moore, H. J.; Haldemann, A. F. C.; Cook, R. A.; Parker, T. J.; Schofield, J. T.

    1998-01-01

    The successful landing of the Mars Pathfinder spacecraft on Mars allows the review of the process of selecting the landing site and assessing predictions made for the site based on Viking and Earth-based data. Selection of the landing site for Mars Pathfinder was a two-phase process. The first phase took place from October 1993 to June 1994 and involved: initial identification of engineering constraints, definition of environmental conditions at the site for spacecraft design, and evaluation of the scientific potential of different landing sites. This phase culminated with the first "Mars Pathfinder Landing Site Workshop", held at the Lunar and Planetary Institute in Houston, Texas on April 18-19, 1994, in which suggested approaches and landing sites were solicited from the entire scientific community. A preliminary site was selected by the project for design purposes in June 1994. The second phase took place from July 1994 to March 1996 and involved: developing criteria for evaluating site safety using images and remote sensing data, testing of the spacecraft and landing subsystems (with design improvements) to establish quantitative engineering constraints on landing site characteristics, evaluating all potential landing sites on Mars, and certification of the site by the project. This phase included a second open workshop, "Mars Pathfinder Landing Site Workshop II: Characteristics of the Ares Vallis Region and Field Trips in the Channeled Scabland, Washington" held in Spokane and Moses Lake September 24-30, 1995 and formal acceptance of the site by NASA Headquarters. Engineering constraints on Pathfinder landing sites were developed from the initial design of the spacecraft and the entry, descent and landing scenario. The site must be within 5 degrees of the subsolar latitude at the time of landing (15N for maximum solar power and flexible communications with Earth. It also must be below 0 km elevation to enable enough time for the parachute to bring the lander

  3. STUDY ON APPLICATION OF COMPOSITE PATHFINDING STRATEGY IN MOBILE PHONE GAME%复合寻路策略在手机游戏中的应用研究

    Institute of Scientific and Technical Information of China (English)

    胡文艺; 邓威; 阚瑷珂; 姜雪娇

    2014-01-01

    复合寻路算法成功应用于手机游戏CrazyWar。该寻路算法包含三个寻路模块:直线寻路模块、A*寻路模块、航点寻路模块。提出的复合寻路算法先通过航点算法得到一个总体的大致路径,再在寻路精细方面由直线寻路模块和A*寻路模块处理,从而解决了A*寻路模块中随搜索地图增长而资源消耗也呈几何增长、大范围搜索耗时过长以及提高估值因子所带来的路径准确度降低的缺点。通过理论分析和实际应用表明:复合寻路算法在寻路速度、资源消耗、寻路效果上均优于单一寻路算法,具有很好的推广性与实用价值。%The composite pathfinding algorithm is successfully applied in the mobile phone game Crazywar.This pathfinding algorithm con-tains three pathfinding modules:the linear pathfinding module,the A* pathfinding module and the waypoint pathfinding module.The com-posite pathfinding algorithm put forward in this paper gets a general rough path through waypoint algorithm at first,then the fine aspect of pathfinding is dealt with by linear pathfinding module and A* pathfinding module,which solves the disadvantages in A* pathfinding module that resource consumption increases geometrically as map searching increases,long time consuming when searching range is wide,and path veracity decreases when estimation value of factor is improved.It is indicated through theoretical analysis and practical application that the composite pathfinding algorithm has good popularisation and practical value since it outperforms the single pathfinding algorithm in pathfinding speed,resource consumption and pathfinding effect.

  4. Vitesse moyenne d'un écoulement à surface libre à partir de mesures des vitesses de surface par une méthode LSPIV

    OpenAIRE

    Rion, Guillaume

    2017-01-01

    Ce travail de fin d'études a pour but d'évaluer la précision d'une technique de mesure non intrusive de vitesse de surface : la LSPIV. Le principe de cette technique de mesure est basé sur l'analyse de séquences d'images horodatées. La LSPIV, acronyme de "Large Scale Particle Image Velocimetry" repose sur l'identification du déplacement de traceurs visibles à la surface de l'eau. Une vitesse de surface est déduite du déplacement de particules entre deux images successives et de l'intervalle d...

  5. Mesures in situ et à haute fréquence de la chimie d’un cours d’eau par spectrophotométrie UV-visible

    OpenAIRE

    Faucheux, Mikaël; Fovet, Ophélie

    2014-01-01

    La variabilité de la chimie d’un cours d’eau se manifeste sur des périodes courtes comme l’événement de crue (quelques heures), mais aussi plus longues, saisonnières, pluriannuelles et décennales. La mesure en continu de la qualité de l’eau est délicate. Les méthodes classiques et standardisées se basent sur des prélèvements d’eau dont les concentrations sont ensuite mesurées en laboratoire. Les contraintes liées au prélèvement, au stockage et aux coûts limitent donc fortement l’accès à des s...

  6. Mesure des fluctuations de température dans un résonateur équipant un système thermoacoustique

    OpenAIRE

    Poignand, Gaëlle; Berson, Arganthaël; Blanc Benon, Philippe; Comte-Bellot, Geneviève; Jondeau, Emmanuel

    2010-01-01

    National audience; Dans les systèmes thermoacoustiques, les fluctuations de température présentent un caractère fortement non-linéaire aux extrémités du stack. La connaissance de ces fluctuations est essentielle dans la détermination et l'optimisation des transferts de chaleur entre le stack et les échangeurs de chaleur et demande la mise au point de nouvelles méthodes de mesure. Cette étude présente une méthode de mesures des fluctuations de température le long d'un résonateur thermoacoustiq...

  7. Mesure de l'inconnexe d'une fonction aléatoire (théorie de la prévisibilité)

    OpenAIRE

    Ravussin, Pierre Emile; Baatard, François

    2008-01-01

    La notion de mesure d'une grandeur physique est définie au sens de la mécanique aléatoire. Les équations générales de l'hydrodynamique sont données en exemple. Un modèle mathématique de prévision basé sur des mesures physiques est formulé, tout d'abord dans un cas à une dimension, puis dans un champ tridimensionnel de vecteurs turbulents. § 1 Introduction. Dès 1966, j'ai été chargé dans le cadre du groupe E.P.U.L. - I.S.M., comprenant le service de la protection de l'air (Dr. A. Junod) et la ...

  8. Integration and Testing of the Inertial Sensor for LISA Pathfinder mission

    Science.gov (United States)

    Sarra, Paolo

    High-precision technologies are essential for space-borne gravitational wave observatory, but full on-ground testing is not feasible. The ESA (European Space Agency) mission LISA Pathfinder (LPF) is aimed to perform in-flight verification of these key technologies, among them the Inertial Sensor, also known as Gravitational Reference Sensor (GRS). The core of the Inertial Sensor is the gravitational reference test mass: a cube of 46 mm made of Au/Pt used as mirror of the LPF interferometer. The “free floating” test mass is surrounded by a capacitive sensor providing the information to perform the “drag-free” control loop required to keep the spacecraft centred with respect to some fiducial points. The Inertial Sensor is equipped with two mechanisms. The caging and venting mechanism lock the test mass during on-ground activities and at launch. It also open the valve for Inertial Sensor venting to space. The grabbing, positioning and release mechanism controls the test mass during in-flight operational phases from caged to free-floating condition. Charge control of the free floating test mass is performed by illuminating its surface, or the electrodes surfaces, with UV light. The Inertial Sensor is equipped with optical fibers and feed-throughs for UV photons supply. Another key component of the Inertial Sensor is the balance mass. Balance masses are required to null the self-gravitational fields seen by the test mass. The test mass, the sensing electrodes, the mechanisms, the balance masses and the UV optical fibers are accommodated inside a dedicated high-vacuum chamber. The vacuum chamber is maintained in static vacuum during on-ground phase an then vented to space to provide the required in-flight vacuum environment around the test mass. A challenging alignment accuracy is required for the manufacturing, assembly and integration of the various equipment composing the Inertial Sensor. In particular for the test mass and the capacitance sensor micron level

  9. Shuttle Laser Altimeter (SLA): A pathfinder for space-based laser altimetry and lidar

    Science.gov (United States)

    Bufton, Jack; Blair, Bryan; Cavanaugh, John; Garvin, James

    1995-01-01

    The Shuttle Laser Altimeter (SLA) is a Hitchhiker experiment now being integrated for first flight on STS-72 in November 1995. Four Shuttle flights of the SLA are planned at a rate of about a flight every 18 months. They are aimed at the transition of the Goddard Space Flight Center airborne laser altimeter and lidar technology to low Earth orbit as a pathfinder for operational space-based laser remote sensing devices. Future alser altimeter sensors such as the Geoscience Laser Altimeter System (GLAS), an Earth Observing System facility instrument, and the Multi-Beam Laser Altimeter (MBLA), the land and vegetation laser altimeter for the NASA TOPSAT (Topography Satellite) Mission, will utilize systems and approaches being tested with SLA. The SLA Instrument measures the distance from the Space Shuttle to the Earth's surface by timing the two-way propagation of short (approximately 10 na noseconds) laser pulses. laser pulses at 1064 nm wavelength are generated in a laser transmitter and are detected by a telescope equipped with a silicon avalanche photodiode detector. The SLA data system makes the pulse time interval measurement to a precision of about 10 nsec and also records the temporal shape of the laser echo from the Earth's surface for interpretation of surface height distribution within the 100 m diam. sensor footprint. For example, tree height can be determined by measuring the characteristic double-pulse signature that results from a separation in time of laser backscatter from tree canopies and the underlying ground. This is accomplished with a pulse waveform digitizer that samples the detector output with an adjustable resolution of 2 nanoseconds or wider intervals in a 100 sample window centered on the return pulse echo. The digitizer makes the SLA into a high resolution surface lidar sensor. It can also be used for cloud and atmospheric aerosol lidar measurements by lengthening the sampling window and degrading the waveform resolution. Detailed test

  10. Mesures de procédure spéciales et respect des droits de l'homme Rapport général

    NARCIS (Netherlands)

    Vervaele, J.A.E.

    2009-01-01

    Le but du rapport général est de mener une analyse comparative des rapports nationaux en vue de présenter les processus de transformation des systèmes de justice pénale internes, en particulier du procès pénal, étant donné que des mesures procédurales spéciales sont introduites pour appréhender le t

  11. On the role of radiation monitors on board LISA Pathfinder and future space interferometers

    Science.gov (United States)

    Grimani, C.; Boatella, C.; Chmeissani, M.; Fabi, M.; Finetti, N.; Laurenza, M.; Lobo, A.; Mateos, I.; Storini, M.

    2012-05-01

    LISA (Laser Interferometer Space Antenna) and its precursor mission LISA Pathfinder (LISA-PF) will carry particle monitors for noise diagnostics. It was proposed to build and place radiation detectors on board the ASTROD missions as well. We present here a study of the solar energetic particle (SEP) events that the LISA-PF radiation monitors are able to detect above the galactic cosmic-ray (GCR) background predicted at the time of the mission data taking in 2015. In order to optimize the correlation between radiation monitor measurements and gravitational sensor test-mass charging, the energy threshold for particles traversing both detectors should be approximately the same. In LISA-PF, the radiation monitor particle energy cut-off was conservatively set at 75 MeV per nucleon (MeV/n) for protons and ion normal incidence, while the minimum energy of the same particles reaching the test masses is 100 MeV/n. We find that SEP events detectable on LISA-PF are characterized by peak fluxes and fluences at energies >75 MeV/n larger than about 45%, on average, with respect to those at energies >100 MeV/n. We conclude that for an accurate correlation between radiation monitor count rates and test-mass charging, it is mandatory to benefit from absolute flux measurements of both galactic and high-energy solar particles provided by experiments carrying magnetic spectrometers in space at the time of LISA-PF (PAMELA, AMS). On the other hand, the role of the radiation detectors on board LISA-PF is crucial allowing for SEP event onset and dynamics monitoring.

  12. Spectral heterogeneity on Phobos and Deimos: HiRISE observations and comparisons to Mars Pathfinder results

    Science.gov (United States)

    Thomas, N.; Stelter, R.; Ivanov, A.; Bridges, N.T.; Herkenhoff, K. E.; McEwen, A.S.

    2011-01-01

    The High-Resolution Imaging Science Experiment (HiRISE) onboard Mars Reconnaissance Orbiter (MRO) has been used to observe Phobos and Deimos at spatial scales of around 6 and 20 m/px, respectively. HiRISE (McEwen et al.; JGR, 112, CiteID E05S02, DOI: 10.1029/2005JE002605, 2007) has provided, for the first time, high-resolution colour images of the surfaces of the Martian moons. When processed, by the production of colour ratio images for example, the data show considerable small-scale heterogeneity, which might be attributable to fresh impacts exposing different materials otherwise largely hidden by a homogenous regolith. The bluer material that is draped over the south-eastern rim of the largest crater on Phobos, Stickney, has been perforated by an impact to reveal redder material and must therefore be relatively thin. A fresh impact with dark crater rays has been identified. Previously identified mass-wasting features in Stickney and Limtoc craters stand out strongly in colour. The interior deposits in Stickney appear more inhomogeneous than previously suspected. Several other local colour variations are also evident. Deimos is more uniform in colour but does show some small-scale inhomogeneity. The bright streamers (Thomas et al.; Icarus, 123, 536556,1996) are relatively blue. One crater to the south-west of Voltaire and its surroundings appear quite strongly reddened with respect to the rest of the surface. The reddening of the surroundings may be the result of ejecta from this impact. The spectral gradients at optical wavelengths observed for both Phobos and Deimos are quantitatively in good agreement with those found by unresolved photometric observations made by the Imager for Mars Pathfinder (IMP; Thomas et al.; JGR, 104, 90559068, 1999). The spectral gradients of the blue and red units on Phobos bracket the results from IMP. ?? 2010 Elsevier Ltd. All rights reserved.

  13. Integrin antagonists affect growth and pathfinding of ventral motor nerves in the trunk of embryonic zebrafish.

    Science.gov (United States)

    Becker, Thomas; McLane, Mary Ann; Becker, Catherina G

    2003-05-01

    Integrins are thought to be important receptors for extracellular matrix (ECM) components on growing axons. Ventral motor axons in the trunk of embryonic zebrafish grow in a midsegmental pathway through an environment rich in ECM components. To test the role of integrins in this process, integrin antagonists (the disintegrin echistatin in native and recombinant form, as well as the Arg-Gly-Asp-Ser peptide) were injected into embryos just prior to axon outgrowth at 14-16 h postfertilization (hpf). All integrin antagonists affected growth of ventral motor nerves in a similar way and native echistatin was most effective. At 24 hpf, when only the three primary motor axons per trunk hemisegment had grown out, 80% (16 of 20) of the embryos analyzed had abnormal motor nerves after injection of native echistatin, corresponding to 19% (91 of 480) of all nerves. At 33 hpf, when secondary motor axons were present in the pathway, 100% of the embryos were affected (24 of 24), with 20% of all nerves analyzed (196 of 960) being abnormal. Phenotypes comprised abnormal branching (64% of all abnormal nerves) and truncations (36% of all abnormal nerves) of ventral motor nerves at 24 hpf and mostly branching of the nerves at 33 hpf (94% of all abnormal nerves). Caudal branches were at least twice as frequent as rostral branches. Surrounding trunk tissue and a number of other axon fascicles were apparently not affected by the injections. Thus integrin function contributes to both growth and pathfinding of axons in ventral motor nerves in the trunk of zebrafish in vivo.

  14. Regenerative Responses and Axon Pathfinding of Retinal Ganglion Cells in Chronically Injured Mice

    Science.gov (United States)

    Yungher, Benjamin J.; Ribeiro, Márcio; Park, Kevin K.

    2017-01-01

    Purpose Enhanced regeneration of retinal ganglion cell (RGC) axons can be achieved by modification of numerous neuronal-intrinsic factors. However, axon growth initiation and the pathfinding behavior of these axons after traumatic injury remain poorly understood outside of acute injury paradigms, despite the clinical relevance of more chronic settings. We therefore examined RGC axon regeneration following therapeutic delivery that is postponed until 2 months after optic nerve crush injury. Methods Optic nerve regeneration was induced by virally mediated (adeno-associated virus) ciliary neurotrophic factor (AAV-CNTF) administered either immediately or 56 days after optic nerve crush in wild-type or Bax knockout (KO) mice. Retinal ganglion nerve axon regeneration was assessed 21 and 56 days after viral injection. Immunohistochemical analysis of RGC injury signals and extrinsic factors in the optic nerve were also examined at 5 and 56 days post crush. Results In addition to sustained expression of injury response proteins in surviving RGCs, we observe axon regrowth in wild-type and apoptosis-deficient Bax KO mice following AAV-CNTF treatment. Fewer instances of aberrant axon growth are seen, at least in the area near the lesion site, in animals given treatment 56 days after crush injury compared to the animals given treatment immediately after injury. We also find evidence of long distance growth into a visual target in Bax KO mice despite postponed initiation of this regenerative program. Conclusions These studies provide evidence against an intrinsic critical period for RGC axon regeneration or degradation of injury signals. Regeneration results from Bax KO mice imply highly sustained regenerative capacity in RGCs, highlighting the importance of long-lasting neuroprotective strategies as well as of RGC axon guidance research in chronically injured animals. PMID:28324115

  15. The Drosophila immunoglobulin gene turtle encodes guidance molecules involved in axon pathfinding

    Directory of Open Access Journals (Sweden)

    Al-Anzi Bader

    2009-08-01

    Full Text Available Abstract Background Neuronal growth cones follow specific pathways over long distances in order to reach their appropriate targets. Research over the past 15 years has yielded a large body of information concerning the molecules that regulate this process. Some of these molecules, such as the evolutionarily conserved netrin and slit proteins, are expressed in the embryonic midline, an area of extreme importance for early axon pathfinding decisions. A general model has emerged in which netrin attracts commissural axons towards the midline while slit forces them out. However, a large number of commissural axons successfully cross the midline even in the complete absence of netrin signaling, indicating the presence of a yet unidentified midline attractant. Results The evolutionarily conserved Ig proteins encoded by the turtle/Dasm1 genes are found in Drosophila, Caenorhabditis elegans, and mammals. In Drosophila the turtle gene encodes five proteins, two of which are diffusible, that are expressed in many areas, including the vicinity of the midline. Using both molecular null alleles and transgenic expression of the different isoforms, we show that the turtle encoded proteins function as non-cell autonomous axonal attractants that promote midline crossing via a netrin-independent mechanism. turtle mutants also have either stalled or missing axon projections, while overexpression of the different turtle isoforms produces invasive neurons and branching axons that do not respect the histological divisions of the nervous system. Conclusion Our findings indicate that the turtle proteins function as axon guidance cues that promote midline attraction, axon branching, and axonal invasiveness. The latter two capabilities are required by migrating axons to explore densely packed targets.

  16. Mesure asymétrie avant-arriere des quarks lourds a LEP1 avec le détecteur OPAL

    CERN Document Server

    Lafoux, H

    A partir de l'ensemble des données accumulées par OPAL au cours de la première phase de fonctionnement du LEP, nous avons mesuré l'asymétrie avant-arrière des quarks b et c au voisinage du pic du Zo. Utilisant une méthode traditionnelle, basée sur la détection des leptons produits dans les désintégrations semi-leptoniques des hadrons lourds, nous avons cherché à optimiser chaque étape de la mesure, en mettant en œuvre les algorithmes les plus appropriés. Le recours aux réseaux de neurones artificiels s'est en particulier avéré d'une grande utilité lorsque le problème à résoudre impliquait la prise en compte simultanée de multiples sources d'informations, d'origine et de nature très variées. Nos résultats sont en bon accord avec ceux des autres mesures effectuées à LEP et compatibles avec les prédictions du Modèle Standard pour un quark top de 174 ± 31 GeV/c2 et un boson de Higgs de masse comprise entre 60 et 1000 GeV/c2

  17. Electronic temperature measurement on the deca II plasma using the Bremsstrahlung; Mesure de la temperature electronique du plasma de deca II par etude du rayonnement de freinage

    Energy Technology Data Exchange (ETDEWEB)

    Dumas, A. [Commissariat a l' Energie Atomique, Fontenay-aux-Roses (France). Centre d' Etudes Nucleaires

    1967-06-01

    The electronic temperature of the DECA II machine's plasma is determined by studying the Bremsstrahlung. Two types of detectors are used for this measurement, a set scintillator-photo-multiplicator and a photoelectric effect detector with a massive silver target. The method used is the classical 'absorbent method', The absorbents used are thin formvar foils whose thickness is between 600 and 12 500 angstrom. The measurements done in two different working conditions of the DECA II machine have given: Te {approx_equal} 200 eV in the first case and Te {approx_equal} 70 eV in the second case. (author) [French] Nous avons determine la temperature electronique du plasma de la machine DECA II par l'etude du rayonnement de freinage. Pour cette mesure nous avons utilise deux types de detecteurs: des ensembles scintillateur-photomultiplicateur et un detecteur a effet photoelectrique a cible massive en argent. La methode utilisee pour cette mesure est la classique methode des absorbants. Nous avons utilise des feuilles de format tres mince (de 600 a 12 500 angstrom) comme absorbant. Les mesures faites dans deux regimes de travail differents de la machine DECA II nous ont conduit a: Te {approx_equal} 200 eV dans un cas et Te {approx_equal} eV dans l'autre cas. (auteur)

  18. Aspects et mesure de la qualité de vie : évolution et renouvellement des tableaux de bord métropolitains

    Directory of Open Access Journals (Sweden)

    Pierre J. Hamel

    2008-02-01

    Full Text Available La mesure de la qualité de vie à l’intérieur des espaces urbains préoccupe les administrations publiques depuis nombre d’années. Cet article passe en revue les modèles de mesure de la qualité de vie développés par les métropoles canadiennes. Il s’interroge sur l’évolution de ces modèles de mesure et sur leur capacité à rendre compte des différentes problématiques désormais associées à la notion de qualité de vie comme le développement social, l’environnement, la société du risque, les ambiances urbaines ou la compétitivité urbaine.For a number of years now, government bodies at all levels have been concerned with measuring quality of life within urban areas. This paper reviews the models used by Canada’s metropolises to measure quality of life. It examines how the models have evolved and their capacity to consider various issues which have become associated with the notion of quality of life, such as social development, environment, risk society, urban surroundings, or urban competitiveness.

  19. Mesure des stades de developpement du sapin baumier (Abies balsamea [L.] Mill.) par teledetection des maxima locaux sur images a tres haute resolution

    Science.gov (United States)

    Demers, Alain

    L'objectif principal de cette these est d'identifier les parametres cles pour lier le developpement morphologique de la cime du sapin baumier (Abies balsamea [L.] Mill.) aux patrons de reflectance qu'elle genere sur une image aerienne a haute resolution. La quantite et la distribution spatiale des aiguilles dans le sapin dependent de la structure des branches. Un mecanisme de ramification particulier (la reiteration) ressort comme le parametre cle pour lier l'augmentation de la biomasse foliaire et la forme de la branche. Les reiterats forment des agglomerats de feuillage qui engendrent des inegalites dans les patrons de reflectance de la cime. La reflectance est plus elevee ou il y a une forte concentration de reiterats (maximum local). On demontre que le developpement du sapin baumier se mesure au moyen de l'analyse des maxima locaux de la cime sur une image. La biomasse de l'arbre se mesure par la teledetection et l'analyse des patrons de reflectance de la cime, c'est-a-dire la mesure du niveau de reiteration par le decompte des maxima locaux de la cime. Cette etude demontre qu'il est possible de proceder a l'inventaire du volume de bois d'un peuplement par la teledetection de l'architecture des arbres.

  20. CALCUL DU DEPHASAGE A LA REFLEXION ET DES INDICES OPTIQUES DE L’ALLIAGE AMORPHE PD30Y70 A PARTIR DE LA MESURE DE SA REFLEXION

    Directory of Open Access Journals (Sweden)

    H BELBAH

    2002-06-01

    Full Text Available Les couches minces de l’alliage amorphe de composition Pd30Y70 sont déposées par pulvérisation cathodique sur des substrats en silice, sous un vide de 10-7 Torr. Les couches obtenues sont opaques et par conséquent leur transmission est nulle. Le spectre de réflexion de Pd30Y70  est mesuré dans le domaine d’énergie entre 0,5 et 6,2 eV. Cette mesure sert au calcul du déphasage à la réflexion de l’alliage à partir de l’intégrale de Kramers-Kronig. Les valeurs mesurées de la réflexion et les valeurs calculées du déphasage à la réflexion permettent de remonter aux constantes optiques (indices de réfraction et d’extinction de l’alliage et à sa structure électronique à partir des spectres d’absorption optique calculés. Le spectre d’absorption optique de Pd30Y70 amorphe est dominé par deux structures dont l’une est due aux états 4d de Pd centrée autour de 4 eV et l’autre aux états 4d de Y aux basses énergies.

  1. Mesures de contrôle en psychiatrie : impacts cliniques et juridiques de la recherche interprétative

    Directory of Open Access Journals (Sweden)

    EMMANUELLE BERNHEIM

    2009-01-01

    Full Text Available L’utilisation des mesures de contrôle (isolement et contention est une pratique très controversée en psychiatrie, tant sur les plans thérapeutique que légal. Le projet de recherche dont il est question dans cet article vise à mettre au jour l’expérience subjective des infirmières et des patients, dans un objectif d’amélioration des pratiques cliniques. La valorisation du discours des patients, à travers une posture épistémologique interprétative, se heurte aux exigences peu adaptées de comités d’éthique de la recherche habitués aux caractéristiques de la recherche positiviste. Pourtant, c’est par la mise au jour des expériences des usagers que des progrès, tant au niveau clinique que juridique, ont pu être faits dans le passé. Aujourd’hui, la recherche doit servir à redonner une place aux patients, non seulement au sein de l’hôpital, mais également au sein de la société.

  2. La thèse de Feldstein-Horioka: Ue mesure de la mobilité internationale du capital

    Directory of Open Access Journals (Sweden)

    de Sousa Andrade Alberto Joao

    2007-01-01

    Full Text Available (portugalski Nous présentons la thèse de Feldstein-Horioka (F-H sur la mobilité du capital et les développements qu’elle a suscités. Il s’agit d’une thèse qui est très ouverte à la possibilité de réfutation et dont l’histoire illustre bien la pensée méthodologique nonnaïve de Karl Popper: les discussions sur sa réfutation, en parallèle avec les tentatives de consolidation ("d’immunisation", au sens de K. Popper, ont conduit à de nouvelles lectures sur la mobilité du capital. Ces efforts de consolidation (d’ "immunization" ont conduit cette thèse à intégrer des nouvelles méthodologies économétriques et à changer partiellement son objet, en mesurant aussi la soutenabilité externe. La thèse de F-H constitue un cas exemplaire d’intégration de l’analyse théorique et d’analyse empirique.

  3. The nuclear quadrupole moment mesured with Nuclear Quadrupole Resonance NQR : Principle and definition

    CERN Document Server

    Belfkir, Mohamed

    2016-01-01

    The nuclear quadruple moment is a fundamental character associated to the nuclei, this moment is related to the not purely spherical distribution in the nuclei, indeed its measure allows us to survey the geometric deformation of the nuclei of its spherical shape. The measurement methods of the quadruple moment is to study the electrical energy hyperfine interaction between the quadruple moment and the electric field gradient due to atomics electrons, one of the methods is the nuclear quadruple resonance NQR which is observed at the transitions between energy levels splits by the effect of the quadruple interaction and induced by a radio frequency field.

  4. Distinct Igneous APXS Rock Compositions on Mars from Pathfinder, MER and MSL

    Science.gov (United States)

    Gellert, Ralf; Arvidson, Raymond; Clark, Benton, III; Ming, Douglas W.; Morris, Richard V.; Squyres, Steven W.; Yen, Albert S.

    2015-01-01

    The alpha particle x-ray spectrometer (APXS) on all four Mars Rovers returned geochemical data from about 1000 rocks and soils along the combined traverses of over 50 kilometers. Here we discuss rocks likely of igneous origin, which might represent source materials for the soils and sediments identified along the traverses. Adirondack-type basalts, abundant in the plains of Gusev Crater, are primitive, olivine bearing basalts. They resemble in composition the basaltic soils encountered at all landing sites, except the ubiquitous elevated S, Cl and Zn in soils. They have been postulated to represent closely the average Martian crust composition. The recently identified new Martian meteorite Black Beauty has similar overall geochemical composition, very distinct from the earlier established SNC meteorites. The rim of the Noachian crater Endeavour, predating the sulfate-bearing Burns formation at Meridiani Planum, also resembles closely the composition of Adirondack basalts. At Gale Crater, the MSL Curiosity rover identified a felsic rock type exemplified by the mugearitic float rock JakeM, which is widespread along the traverse at Gale. While a surprise at that time, possibly related more evolved, alkaline rocks had been previously identified on Mars. Spirit encountered the Wishstone rocks in the Columbia Hills with approx. 6% Na2O+K2O, 15 % Al2O3 and low 12% FeO. Pathfinder rocks with elevated K and Na and >50% SiO2 were postulated to be andesitic. Recently Opportunity encountered the rock JeanBaptisteCharbonneau with >15% Al2O3, >50% SiO2 and approx. 10% FeO. A common characteristic all these rocks is the very low abundance of Cr, Ni and Zn, and an Fe/Mn ratio of about 50, indicating an unaltered Fe mineralogy. Beside these likely igneous rock types, which occurred always in several rocks, a few unique rocks were encountered, e.g. Bounce Rock, a pyroxene-bearing ejecta rock fragment resembling the Shergottite EETA 79001B meteorite. The APXS data can be used to

  5. Qualifciation test series of the indium needle FEEP micro-propulsion system for LISA Pathfinder

    Science.gov (United States)

    Scharlemann, C.; Buldrini, N.; Killinger, R.; Jentsch, M.; Polli, A.; Ceruti, L.; Serafini, L.; DiCara, D.; Nicolini, D.

    2011-11-01

    The Laser Interferometer Space Antenna project (LISA) is a co-operative program between ESA and NASA to detect gravitational waves by measuring distortions in the space-time fabric. LISA Pathfinder is the precursor mission to LISA designed to validate the core technologies intended for LISA. One of the enabling technologies is the micro-propulsion system based on field emission thrusters necessary to achieve the uniquely stringent propulsion requirements. A consortium consisting of Astrium GmbH and the University of Applied Sciences Wiener Neustadt (formerly AIT) was commissioned by ESA to develop and qualify the micro-propulsion system based on the Indium Needle FEEP technology. Several successful tests have verified the proper Needle Field Emission Electric Propulsion (FEEP) operation and the thermal and mechanical design of subcomponents of the developed system. For all functional tests, the flight representative Power Control Unit developed by SELEX Galileo S.p.A (also responsible for the Micro-Propulsion Subsystem (MPS) development) was used. Measurements have shown the exceptional stability of the thruster. An acceptance test of one Thruster Cluster Assembly (TCA) over 3600 h has shown the stable long term operation of the developed system. During the acceptance test compliance to all the applicable requirements have been shown such as a thrust resolution of 0.1 μN, thrust range capability between 0 and 100 μN, thrust overshoot much lower than the required 0.3 μN+3% and many others. In particular important is the voltage stability of the thruster (±1% over the duration of the testing) and the confirmation of the very low thrust noise. Based on the acceptance test the lifetime of the thruster is expected to exceed 39,000 h generating a total impulse bit of 6300 Ns at an average thrust level of 50 μN. A flight representative qualification model of the Needle FEEP Cluster Assembly (DM1) equipped with one active TCA has performed a qualification program

  6. Laying the Foundation for Space-based Gravitational Wave Detection: LISA Pathfinder, the LISA Test Package, and ST7-DRS

    Science.gov (United States)

    Thorpe, James

    2014-08-01

    Efforts to develop space-based observatories of gravitational waves, such as the long-standing Laser Interferometer Space Antenna (LISA) or the more recent eLISA concept that motivated ESA’s selection of a gravitational wave mission for the L3 Mission Opportunity, have traditionally been praised for their scientific potential and criticized for their technological readiness. The LISA Pathfinder (LPF) mission is a dedicated technology demonstrator for such missions. Led by ESA and a consortium of European national agencies and with a minority contribution from NASA, LPF will demonstrate several key technologies for the LISA concept. LPF includes two scientific payloads: the European LISA Technology Package (LTP) and the NASA-provided ST7-DRS. The mission will place two test masses in drag-free flight and measure the relative acceleration between them. This measurement will validate a number of technologies that are critical to LISA-like gravitational wave instruments including sensing and control of the test masses, drag-free control laws, micro-Newton thrusters, and picometer-level laser metrology. LPF is currently in the late stages of integration and test and is planned to launch in 2015. We will present the current status of the LISA Pathfinder mission and the LTP and ST7-DRS payloads as well as the expected impact on the larger gravitational-wave effort.

  7. Laboratory Results and Status Update for Pathfinder at LBT, The LINC-NIRVANA NGS Ground- Layer AO Subsystem

    CERN Document Server

    Kopon, Derek; Bertram, Thomas; Herbst, Tom; Kürster, Martin; Berwein, Jürgen; Ragazzoni, Roberto; Farinato, Jacopo; Viotto, Valentina; Bergomi, Maria; Rohloff, Ralf-Rainer; Baumeister, Harald; De Bonis, Fulvio; Hofferbert, Ralph; Brunelli, Alessandro; Arcidiacono, Carmelo; Pott, Jorg-Uwe; Bizenberger, Peter; Briegel, Florian; Meschke, Daniel; Mohr, Lars; Zhang, Xianyu; Kittmann, Frank

    2014-01-01

    The full LINC-NIRVANA instrument will be one of the most complex ground-based astronomical systems ever built. It will consist of multiple subsystems, including two multi-conjugate ground layer AO systems (MCAO) that drive the LBT adaptive secondaries, two mid-high layer AO systems with their own Xynetics 349 actuator DM's , a fringe tracker, a beam combiner, and the NIR science camera. In order to mitigate risk, we take a modular approach to instrument testing and commissioning by decoupling these subsystems individually. The first subsystem tested on-sky will be one of the ground-layer AO systems, part of a test-bed known as the Pathfinder. The Pathfinder consists of a 12-star pyramid wavefront sensor (PWFS) that drives one of the LBT's adaptive secondaries, a support structure known as "The Foot," and the infrared test camera (IRTC), which is used for acquisition and alignment. The 12 natural guide stars are acquired by moveable arms called "star enlargers," each of which contains its own optical path. The...

  8. Pathfinder first light: alignment, calibration, and commissioning of the LINC-NIRVANA ground-layer adaptive optics subsystem

    CERN Document Server

    Kopon, Derek; Arcidiacono, Carmelo; Herbst, Tom; Viotto, Valentina; Farinato, Jacopo; Bergomi, Maria; Ragazzoni, Roberto; Marafatto, Luca; Baumeister, Harald; Bertram, Thomas; Berwein, Jürgen; Briegel, Florian; Hofferbert, Ralph; Kittmann, Frank; Kürster, Martin; Mohr, Lars; Radhakrishnan, Kalyan

    2014-01-01

    We present descriptions of the alignment and calibration tests of the Pathfinder, which achieved first light during our 2013 commissioning campaign at the LBT. The full LINC-NIRVANA instrument is a Fizeau interferometric imager with fringe tracking and 2-layer natural guide star multi-conjugate adaptive optics (MCAO) systems on each eye of the LBT. The MCAO correction for each side is achieved using a ground layer wavefront sensor that drives the LBT adaptive secondary mirror and a mid-high layer wavefront sensor that drives a Xinetics 349 actuator DM conjugated to an altitude of 7.1 km. When the LINC-NIRVANA MCAO system is commissioned, it will be one of only two such systems on an 8-meter telescope and the only such system in the northern hemisphere. In order to mitigate risk, we take a modular approach to commissioning by decoupling and testing the LINC-NIRVANA subsystems individually. The Pathfinder is the ground-layer wavefront sensor for the DX eye of the LBT. It uses 12 pyramid wavefront sensors to opt...

  9. The Ultraviolet Spectro-Coronagraph (UVSC) Pathfinder Experiment for the Remote Detection of Suprathermal Seed Particles: Instrument Status

    Science.gov (United States)

    Strachan, Leonard; Laming, J. Martin; Ko, Yuan-Kuen; Tun Beltran, Samuel; Korendyke, Clarence M.; Brown, Charles M.; Socker, Dennis G.; Galysh, Ivan J.; Finne, Theodore T.; Eisenhower, Kevin C.; Brechbiel, David J.; Noya, Mario; Provornikova, Elena; Gardner, Larry D.

    2017-08-01

    The largest solar energetic particle (SEP) storms are produced by fast coronal mass ejection (CME) shocks. Efficient shock acceleration of ambient particles requires a near sun reservoir of suprathermal (proton) seed particles. However, the requisite seed particle reservoir has not been detected near the sun where CME shocks first appear. We are developing the Ultraviolet Spectro-Coronagraph (UVSC) Pathfinder space experiment to test for the presence or absence of the requisite suprathermal proton seed particle population within 3 solar radii of sun-center. In this poster, we present the instrument design concept, its development status, and the expected experimental results. The ultimate goal for the experiment is to demonstrate how such measurements can be used as a part of a future SEP space weather warning system. UVSC Pathfinder is scheduled to be launched in 2019 by the DoD Space Test Program. It is supported by funds from the Chief of Naval Research (via the NRL basic research program) and from NASA (via NDPR NNG13WF951 and NNH16AC29I).

  10. Extragalactic radio surveys in the pre-Square Kilometre Array era

    Science.gov (United States)

    Simpson, Chris

    2017-07-01

    The era of the Square Kilometre Array is almost upon us, and pathfinder telescopes are already in operation. This brief review summarizes our current knowledge of extragalactic radio sources, accumulated through six decades of continuum surveys at the low-frequency end of the electromagnetic spectrum and the extensive complementary observations at other wavelengths necessary to gain this understanding. The relationships between radio survey data and surveys at other wavelengths are discussed. Some of the outstanding questions are identified and prospects over the next few years are outlined.

  11. Results From Mars Show Electrostatic Charging of the Mars Pathfinder Sojourner Rover

    Science.gov (United States)

    Kolecki, Joseph C.; Siebert, Mark W.

    1998-01-01

    Indirect evidence (dust accumulation) has been obtained indicating that the Mars Pathfinder rover, Sojourner, experienced electrostatic charging on Mars. Lander camera images of the Sojourner rover provide distinctive evidence of dust accumulation on rover wheels during traverses, turns, and crabbing maneuvers. The sol 22 (22nd Martian "day" after Pathfinder landed) end-of-day image clearly shows fine red dust concentrated around the wheel edges with additional accumulation in the wheel hubs. A sol 41 image of the rover near the rock "Wedge" (see the next image) shows a more uniform coating of dust on the wheel drive surfaces with accumulation in the hubs similar to that in the previous image. In the sol 41 image, note particularly the loss of black-white contrast on the Wheel Abrasion Experiment strips (center wheel). This loss of contrast was also seen when dust accumulated on test wheels in the laboratory. We believe that this accumulation occurred because the Martian surface dust consists of clay-sized particles, similar to those detected by Viking, which have become electrically charged. By adhering to the wheels, the charged dust carries a net nonzero charge to the rover, raising its electrical potential relative to its surroundings. Similar charging behavior was routinely observed in an experimental facility at the NASA Lewis Research Center, where a Sojourner wheel was driven in a simulated Martian surface environment. There, as the wheel moved and accumulated dust (see the following image), electrical potentials in excess of 100 V (relative to the chamber ground) were detected by a capacitively coupled electrostatic probe located 4 mm from the wheel surface. The measured wheel capacitance was approximately 80 picofarads (pF), and the calculated charge, 8 x 10(exp -9) coulombs (C). Voltage differences of 100 V and greater are believed sufficient to produce Paschen electrical discharge in the Martian atmosphere. With an accumulated net charge of 8 x 10(exp

  12. Review of A* (A Star Navigation Mesh Pathfinding as the Alternative of Artificial Intelligent for Ghosts Agent on the Pacman Game

    Directory of Open Access Journals (Sweden)

    Moh. Zikky

    2016-08-01

    Full Text Available Shortest pathfinding problem has become a populer issue in Game’s Artificial Intelligent (AI. This paper discussed the effective way to optimize the shortest pathfinding problem, namely Navigation Mesh (NavMesh. This method is very interesting because it has a large area of implementation, especially in games world. In this paper, NavMesh was implemented by using A* (A star algorithm and examined in Unity 3D game engine. A* was an effective algorithm in shortest pathfinding problem because its optimization was made with effective tracing using segmentation line. Pac-Man game was chosen as the example of the shortest pathfinding by using NavMesh in Unity 3D. A* algorithm was implemented on the enemies of Pac-Man (three ghosts,  which path was designed by using NavMesh concept. Thus, the movement of ghosts in catching Pac-Man was the result of this review of the effectiveness of this concept. In further research, this method could be implemented on several optimization programmes, such as Geographic Information System (GIS, robotics, and statistics.

  13. Discovery of H I gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder

    NARCIS (Netherlands)

    Allison, J. R.; Sadler, E. M.; Moss, V. A.; Whiting, M. T.; Hunstead, R. W.; Pracy, M. B.; Curran, S. J.; Croom, S. M.; Glowacki, M.; Morganti, R.; Shabala, S. S.; Zwaan, M. A.; Allen, G.; Amy, S. W.; Axtens, P.; Ball, L.; Bannister, K. W.; Barker, S.; Bell, M. E.; Bock, D. C.-J.; Bolton, R.; Bowen, M.; Boyle, B.; Braun, R.; Broadhurst, S.; Brodrick, D.; Brothers, M.; Brown, A.; Bunton, J. D.; Cantrall, C.; Chapman, J.; Cheng, W.; Chippendale, A. P.; Chung, Y.; Cooray, F.; Cornwell, T.; DeBoer, D.; Diamond, P.; Edwards, P. G.; Ekers, R.; Feain, I.; Ferris, R. H.; Forsyth, R.; Gough, R.; Grancea, A.; Gupta, N.; Guzman, J. C.; Hampson, G.; Harvey-Smith, L.; Haskins, C.; Hay, S.; Hayman, D. B.; Heywood, I.; Hotan, A. W.; Hoyle, S.; Humphreys, B.; Indermuehle, B. T.; Jacka, C.; Jackson, C.; Jackson, S.; Jeganathan, K.; Johnston, S.; Joseph, J.; Kendall, R.; Kesteven, M.; Kiraly, D.; Koribalski, B. S.; Leach, M.; Lenc, E.; Lensson, E.; Mackay, S.; Macleod, A.; Marquarding, M.; Marvil, J.; McClure-Griffiths, N.; McConnell, D.; Mirtschin, P.; Norris, R. P.; Neuhold, S.; Ng, A.; O'Sullivan, J.; Pathikulangara, J.; Pearce, S.; Phillips, C.; Popping, A.; Qiao, R. Y.; Reynolds, J. E.; Roberts, P.; Sault, R. J.; Schinckel, A.; Serra, P.; Shaw, R.; Shields, M.; Shimwell, T.; Storey, M.; Sweetnam, T.; Troup, E.; Turner, B.; Tuthill, J.; Tzioumis, A.; Voronkov, M. A.; Westmeier, T.; Wilson, C. D.

    2015-01-01

    We report the discovery of a new 21-cm H I absorption system using commissioning data from the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP). Using the 711.5-1015.5 MHz band of ASKAP we were able to conduct a blind search for the 21-cm line in a

  14. GASKAP -- The Galactic ASKAP Survey

    CERN Document Server

    Dickey, J M; Gibson, S J; Gomez, J F; Imai, H; Jones, P; Stanimirovic, S; van Loon, J Th; Walsh, A; Alberdi, A; Anglada, G; Uscanga, L; Arce, H; Bailey, M; Begum, A; Wakker, B; Bekhti, N Ben; Kalberla, P; Winkel, B; Bekki, K; For, B -Q; Staveley-Smith, L; Westmeier, T; Burton, M; Cunningham, M; Dawson, J; Ellingsen, S; Diamond, P; Green, J A; Hill, A S; Koribalski, B; McConnell, D; Rathborne, J; Voronkov, M; Douglas, K A; English, J; Ford, H A; Foster, T; Gomez, Y; Green, A; Bland-Hawthorn, J; Gulyaev, S; Hoare, M; Joncas, G; Kang, J-H; Kerton, C R; Koo, B-C; Leahy, D; Lo, N; Lockman, F J; Migenes, V; Nakashima, J; Zhang, Y; Nidever, D; Peek, J E G; Tafoya, D; Tian, W; Wu, D

    2012-01-01

    A survey of the Milky Way disk and the Magellanic System at the wavelengths of the 21-cm atomic hydrogen (HI) line and three 18-cm lines of the OH molecule will be carried out with the Australian Square Kilometre Array Pathfinder telescope. The survey will study the distribution of HI emission and absorption with unprecedented angular and velocity resolution, as well as molecular line thermal emission, absorption, and maser lines. The area to be covered includes the Galactic plane (|b|< 10deg) at all declinations south of delta = +40deg, spanning longitudes 167deg through 360deg to 79deg at b=0deg, plus the entire area of the Magellanic Stream and Clouds, a total of 13,020 square degrees. The brightness temperature sensitivity will be very good, typically sigma_T ~ 1 K at resolution 30arcsec and 1 km/s. The survey has a wide spectrum of scientific goals, from studies of galaxy evolution to star formation, with particular contributions to understanding stellar wind kinematics, the thermal phases of the inte...

  15. High speed pulsed magnetic fields measurements, using the Faraday effect; Mesures de champs magnetiques pulses rapides a l'aide de l'effet Faraday

    Energy Technology Data Exchange (ETDEWEB)

    Dillet, A. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1964-12-01

    For these measures, the information used is the light polarization plane rotation induced by the magnetic field in a glass probe. This rotation is detected using a polarizer-analyzer couple. The detector is a photomultiplier used with high-current and pulsed light. In a distributed magnet (gap: 6 x 3 x 3 cm) magnetic fields to measure are 300 gauss, lasting 0.1 {mu}s, with rise times {<=} 35 ns, repetition rate: 1/s. An oscilloscope is used to view the magnetic field from the P.M. plate signal. The value of the field is computed from a previous static calibration. Magnetic fields from 50 to 2000 gauss (with the probe now used) can be measured to about 20 gauss {+-} 5 per cent, with a frequency range of 30 MHz. (author) [French] Pour faire de telles mesures, on utilise comme information la rotation du plan de polarisation de la lumiere provoquee par le champ magnetique dans une sonde en verre. On detecte cette rotation au moyen d'un polariseur et d'un analyseur, qui sont regles a 45 deg. pour conserver un phenomene lineaire. Le detecteur est un photomultiplicateur travaillant en fort courant en lumiere pulsee. Dans un aimant distribue d'entrefer 6 x 3 x 3 cm, on obtient des champs magnetiques a mesurer de 300 gauss, durant 0.1 {mu}s, avec des temps de montee {<=} 35 ns; au taux de 1 fois par seconde. L'observation du champ se fait sur oscilloscope a partir du signal de plaque du P.M. La valeur absolue du champ est obtenue au moyen d'un etalonnage statique prealable. On peut ainsi mesurer a 20 gauss et {+-} 5 pour cent pres environ des champs magnetiques de 50 a 2000 gauss (avec la sonde actuelle) et avec une bande passante de 30 MHz. (auteur)

  16. Coexpression of high-voltage-activated ion channels Kv3.4 and Cav1.2 in pioneer axons during pathfinding in the developing rat forebrain.

    Science.gov (United States)

    Huang, Chia-Yi; Chu, Dachen; Hwang, Wei-Chao; Tsaur, Meei-Ling

    2012-11-01

    Precise axon pathfinding is crucial for establishment of the initial neuronal network during development. Pioneer axons navigate without the help of preexisting axons and pave the way for follower axons that project later. Voltage-gated ion channels make up the intrinsic electrical activity of pioneer axons and regulate axon pathfinding. To elucidate which channel molecules are present in pioneer axons, immunohistochemical analysis was performed to examine 14 voltage-gated ion channels (Kv1.1-Kv1.3, Kv3.1-Kv3.4, Kv4.3, Cav1.2, Cav1.3, Cav2.2, Nav1.2, Nav1.6, and Nav1.9) in nine axonal tracts in the developing rat forebrain, including the optic nerve, corpus callosum, corticofugal fibers, thalamocortical axons, lateral olfactory tract, hippocamposeptal projection, anterior commissure, hippocampal commissure, and medial longitudinal fasciculus. We found A-type K⁺ channel Kv3.4 in both pioneer axons and early follower axons and L-type Ca²⁺ channel Cav1.2 in pioneer axons and early and late follower axons. Spatially, Kv3.4 and Cav1.2 were colocalized with markers of pioneer neurons and pioneer axons, such as deleted in colorectal cancer (DCC), in most fiber tracts examined. Temporally, Kv3.4 and Cav1.2 were expressed abundantly in most fiber tracts during axon pathfinding but were downregulated beginning in synaptogenesis. By contrast, delayed rectifier Kv channels (e.g., Kv1.1) and Nav channels (e.g., Nav1.2) were absent from these fiber tracts (except for the corpus callosum) during pathfinding of pioneer axons. These data suggest that Kv3.4 and Cav1.2, two high-voltage-activated ion channels, may act together to control Ca²⁺ -dependent electrical activity of pioneer axons and play important roles during axon pathfinding.

  17. VAST: An ASKAP Survey for Variables and Slow Transients

    CERN Document Server

    Murphy, Tara; Kaplan, David L; Banyer, Jay; Bell, Martin E; Bignall, Hayley E; Bower, Geoffrey C; Cameron, Robert; Coward, David M; Cordes, James M; Croft, Steve; Curran, James R; Djorgovski, S G; Farrell, Sean A; Frail, Dale A; Gaensler, B M; Galloway, Duncan K; Gendre, Bruce; Green, Anne J; Hancock, Paul J; Johnston, Simon; Kamble, Atish; Law, Casey J; Lazio, T Joseph W; Lo, Kitty K; Macquart, Jean-Pierre; Rea, Nanda; Rebbapragada, Umaa; Reynolds, Cormac; Ryder, Stuart D; Schmidt, Brian; Soria, Roberto; Stairs, Ingrid H; Tingay, Steven J; Torkelsson, Ulf; Wagstaff, Kiri; Walker, Mark; Wayth, Randall B; Williams, Peter K G

    2012-01-01

    The Australian Square Kilometre Array Pathfinder (ASKAP) will give us an unprecedented opportunity to investigate the transient sky at radio wavelengths. In this paper we present VAST, an ASKAP survey for Variables and Slow Transients. VAST will exploit the wide-field survey capabilities of ASKAP to enable the discovery and investigation of variable and transient phenomena from the local to the cosmological, including flare stars, intermittent pulsars, X-ray binaries, magnetars, extreme scattering events, interstellar scintillation, radio supernovae and orphan afterglows of gamma ray bursts. In addition, it will allow us to probe unexplored regions of parameter space where new classes of transient sources may be detected. In this paper we review the known radio transient and variable populations and the current results from blind radio surveys. We outline a comprehensive program based on a multi-tiered survey strategy to characterise the radio transient sky through detection and monitoring of transient and va...

  18. LA MESURE DE LA CREATION DE VALEUR ORGANISATIONNELLE : LE CAS D'UNE ENTREPRISE DU SECTEUR DE LA GESTION DE PATRIMOINE

    OpenAIRE

    Cappelletti, Laurent; Khouatra, Djamel

    2002-01-01

    International audience; Cette communication présente une méthode de mesure de la création de valeur organisationnelle d'une entreprise, à partir d'une étude de cas consistant en une recherche-intervention conduite de 1999 à 2000. L'hypothèse centrale qui est développée est que la création de valeur organisationnelle contribue à la création de valeur économique future.

  19. Mesures de contraintes in-situ. Méthode de relaxation des carottes Measuring in-Situ Stresses. Relaxation Method with Core Samples

    Directory of Open Access Journals (Sweden)

    Perreau P.

    2006-11-01

    Full Text Available Dans cet article, on se propose de présenter les premiers résultats de l'étude de la méthode d'évaluation des contraintes par mesure de déformations différées d'une carotte après son extraction. Le travail correspondant a été réalisé dans le cadre du projet ARTEP Fracturation hydraulique . Les principes de cette méthode et les quelques éléments d'interprétation récemment publiés dans la littérature sont exposés dans un premier temps. Les résultats de deux campagnes de mesures sur deux puits de la SNEA-P (Soudron, novembre 1985 et Lanot, juillet 1986 sont ensuite présentés. Ces essais ont mis en évidence que les déformations différées d'une carotte dues au relachement des contraintes sont effectivement mesurables. Cependant, une interprétation quantitative de ces mesures nécessite une amélioration des conditions expérimentales (stabilisation thermique, stabilisation de l'état de saturation. This article describes the first results of research on a method of evaluating stresses by measuring the differred deformations of a core sample after it has been extracted. The corresponding research was done within the framework of an ARTEP project on Hydraulic Fracturing . The principles of this method and several interpretation aspects published recently in the literature are described in the first part. Then the results of two measurement campaigns using two SNEA-P wells (Soudron in November 1985 and Lanot in July 1986 are described. These tests revealed that the differed deformations of a core sample due to the relaxing of stresses can effectively be measured. However, a quantitative interpretation of these measurements requires an improvement to be made in the experimental conditions (thermal stabilization, stabilization of the state of saturation.

  20. Etude en laboratoire des performances de l'appareil DiSCmini pour la mesure des aérosols submicroniques

    OpenAIRE

    Bau, Sébastien; Witschger, O.

    2015-01-01

    En plus de la composition chimique, la taille des particules et la concentration sont parmi les principaux paramètres utilisés pour caractériser l'exposition aux nanoparticules dispersées dans l'air. Pour évaluer les expositions professionnelles, l'utilisation d’instruments de mesure en temps réel sont recommandés dans les stratégies récentes publiées. Parmi les dispositifs portables individuels permettant d’évaluer l'exposition aux aérosols de nanoparticules en milieu de travail, le DiSCmini...

  1. Observation of polarised hard X-ray emission from the Crab by the PoGOLite Pathfinder

    CERN Document Server

    Chauvin, M; Jackson, M; Kamae, T; Kawano, T; Kiss, M; Kole, M; Mikhalev, V; Moretti, E; Olofsson, G; Rydström, S; Takahashi, H; Iyudin, A; Arimoto, M; Fukazawa, Y; Kataoka, J; Kawai, N; Mizuno, T; Ryde, F; Tajima, H; Takahashi, T; Pearce, M

    2015-01-01

    We have measured the linear polarisation of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the polarisation fraction and angle stands to disentangle geometrical and physical effects, thereby providing information on the pulsar wind geometry and magnetic field environment. Measurements are conducted using the PoGOLite Pathfinder - a balloon-borne polarimeter. Polarisation is determined by measuring the azimuthal Compton scattering angle of incident X-rays in an array of plastic scintillators housed in an anticoincidence well. The polarimetric response has been characterised prior to flight using both polarised and unpolarised calibration sources. We address possible systematic effects through observations of a background field. The measured polarisation fraction for the integrated Crab light-curve is ($18.4^{+9.8}_{-10.6}$)%, corresponding to an upper limit (99% credibility) of 42.4%, for a polarisation angle of ($...

  2. Dynamic Control System Performance during Commissioning of the Space Technology 7-Disturbance Reduction System Experiment of LISA Pathfinder

    Science.gov (United States)

    Hsu, Oscar; Maghami, Peiman; O’Donnell, James R., Jr.; Ziemer, John; Romero-Wolf, Andrew

    2017-01-01

    The Space Technology-7 Disturbance Reduction System (DRS) launched aboard the European Space Agency's LISA Pathfinder spacecraft on December 3, 2015, after more than a decade in development. DRS consists of three primary components: an Integrated Avionics Unit (IAU), Colloidal MicroNewton Thrusters, and Dynamic Control System (DCS) algorithms implemented on the IAU. During the portions of the mission in which the DRS was under control, the DCS was responsible for controlling the spacecraft and the free-floating test masses that were part of the LISA Test Package. The commissioning period was originally divided into two periods: before propulsion separation and after propulsion separation. A recommissioning period was added after an anomaly occurred in the thruster system. The paper will describe the activities used to commission DRS, present results from the commissioning of the DCS and the recommissioning activities per-formed after the thruster anomaly.

  3. Multi-Agent Pathfinding with n Agents on Graphs with n Vertices: Combinatorial Classification and Tight Algorithmic Bounds

    DEFF Research Database (Denmark)

    Förster, Klaus-Tycho; Groner, Linus; Hoefler, Torsten

    2017-01-01

    We investigate the multi-agent pathfinding (MAPF) problem with $n$ agents on graphs with $n$ vertices: Each agent has a unique start and goal vertex, with the objective of moving all agents in parallel movements to their goal s.t.~each vertex and each edge may only be used by one agent at a time....... We give a combinatorial classification of all graphs where this problem is solvable in general, including cases where the solvability depends on the initial agent placement. Furthermore, we present an algorithm solving the MAPF problem in our setting, requiring O(n²) rounds, or O(n³) moves...... of individual agents. Complementing these results, we show that there are graphs where Omega(n²) rounds and Omega(n³) moves are required for any algorithm....

  4. Characterization of the JWST Pathfinder Mirror Dynamics Using the Center of Curvature Optical Assembly (CoCOA)

    Science.gov (United States)

    Wells, C.; Hadaway, J.; Olczak, G.; Cosentino, J.; Johnston, J.; Whitman, T.; Connolly, M.; Chaney, D.; Knight, J.; Telfer, R.

    2016-01-01

    The JWST (James Webb Space Telescope) Optical Telescope Element (OTE) consists of a 6.6 meter clear aperture, 18-segment primary mirror, all-reflective, three-mirror anastigmat operating at cryogenic temperatures. To verify performance of the primary mirror, a full aperture center of curvature optical null test is performed under cryogenic conditions in Chamber A at NASA Johnson Space Center using an instantaneous phase measuring interferometer. After phasing the mirrors during the JWST Pathfinder testing, the interferometer is utilized to characterize the mirror relative piston and tilt dynamics under different facility configurations. The correlation between the motions seen on detectors at the focal plane and the interferometer validates the use of the interferometer for dynamic investigations. The success of planned test hardware improvements will be characterized by the multi-wavelength interferometer (MWIF) at the Center of Curvature Optical Assembly (CoCOA).

  5. Characterization of the JWST Pathfinder mirror dynamics using the center of curvature optical assembly (CoCOA)

    Science.gov (United States)

    Wells, Conrad; Hadaway, James B.; Olczak, Gene; Cosentino, Joseph; Johnston, John D.; Whitman, Tony; Connolly, Mark; Chaney, David; Knight, J. Scott; Telfer, Randal

    2016-07-01

    The James Webb Space Telescope (JWST) Optical Telescope Element (OTE) consists of a 6.6 m clear aperture, 18 segment primary mirror, all-reflective, three-mirror anastigmat operating at cryogenic temperatures. To verify performance of the primary mirror, a full aperture center of curvature optical null test is performed under cryogenic conditions in Chamber A at the National Aeronautics and Space Administration (NASA) Johnson Space Center (JSC) using an instantaneous phase measuring interferometer. After phasing the mirrors during the JWST Pathfinder testing, the interferometer is utilized to characterize the mirror relative piston and tilt dynamics under different facility configurations. The correlation between the motions seen on detectors at the focal plane and the interferometer validates the use of the interferometer for dynamic investigations. The success of planned test hardware improvements will be characterized by the multi-wavelength interferometer (MWIF) at the Center of Curvature Optical Assembly (CoCOA).

  6. Performance of the primary mirror center-of-curvature optical metrology system during cryogenic testing of the JWST Pathfinder telescope

    Science.gov (United States)

    Hadaway, James B.; Wells, Conrad; Olczak, Gene; Waldman, Mark; Whitman, Tony; Cosentino, Joseph; Connolly, Mark; Chaney, David; Telfer, Randal

    2016-07-01

    The James Webb Space Telescope (JWST) primary mirror (PM) is 6.6 m in diameter and consists of 18 hexagonal segments, each 1.5 m point-to-point. Each segment has a six degree-of-freedom hexapod actuation system and a radius of-curvature (RoC) actuation system. The full telescope will be tested at its cryogenic operating temperature at Johnson Space Center. This testing will include center-of-curvature measurements of the PM, using the Center-of-Curvature Optical Assembly (COCOA) and the Absolute Distance Meter Assembly (ADMA). The COCOA includes an interferometer, a reflective null, an interferometer-null calibration system, coarse and fine alignment systems, and two displacement measuring interferometer systems. A multiple-wavelength interferometer (MWIF) is used for alignment and phasing of the PM segments. The ADMA is used to measure, and set, the spacing between the PM and the focus of the COCOA null (i.e. the PM center-of-curvature) for determination of the ROC. The performance of these metrology systems was assessed during two cryogenic tests at JSC. This testing was performed using the JWST Pathfinder telescope, consisting mostly of engineering development and spare hardware. The Pathfinder PM consists of two spare segments. These tests provided the opportunity to assess how well the center-of-curvature optical metrology hardware, along with the software and procedures, performed using real JWST telescope hardware. This paper will describe the test setup, the testing performed, and the resulting metrology system performance. The knowledge gained and the lessons learned during this testing will be of great benefit to the accurate and efficient cryogenic testing of the JWST flight telescope.

  7. Evaluation of the mechanical behaviour of PathFile and ProGlider pathfinding nickel-titanium rotary instruments.

    Science.gov (United States)

    Elnaghy, A M; Elsaka, S E

    2015-09-01

    To assess and compare the resistance to cyclic fatigue, torsional stress, bending and buckling of ProGlider (PG; Dentsply Maillefer, Ballaigues, Switzerland) instruments with PathFile (PF; Dentsply Maillefer) pathfinding nickel-titanium rotary instruments. Size 16, .02 taper PG and PF instruments were rotated in simulated canals until failure, and the number of cycles to failure (NCF) was recorded to evaluate their cyclic fatigue resistance. Torsional strength was measured using a torsiometer after fixing rigidly the apical 5 mm of the instrument. A scanning electron microscope was used to characterize the topographic features of the fracture surfaces of the instruments. The instruments were evaluated for bending resistance using a cantilever-bending test. The buckling resistance was measured by recording the maximum load required to form a lateral elastic displacement along the file axis using a universal testing machine. Data were statistically analysed using independent t-tests. Statistical significance was set at P < 0.05. ProGlider instrument had a significantly higher flexibility, higher resistance to cyclic fatigue and torsional stress than PF instruments (P < 0.05). The fractured cross-sectional surfaces revealed typical features of cyclic fatigue and torsional fractures. There was no significant difference in the maximum load needed to buckle the two instruments tested (P = 0.082). ProGlider NiTi pathfinding instrument manufactured from M-Wire alloy had enhanced mechanical properties, including higher flexibility, higher resistance to cyclic fatigue and torsional stress compared with PathFile instrument made of conventional NiTi alloy. © 2014 International Endodontic Journal. Published by John Wiley & Sons Ltd.

  8. AN IMPROVED GROUP INTELLIGENCE PATHFINDING ALGORITHM%一种改进的群体智能寻路算法

    Institute of Scientific and Technical Information of China (English)

    徐翔; 黄敏

    2012-01-01

    以游戏中群体智能角色的路径搜索为研究背景,提出一种改进的群体智能寻路算法.该方法把游戏寻路过程划分成三个阶段:第一阶段为预处理阶段,针对特定的目标点,采取逆向路径搜索策略,建立最优解路径表.第二阶段,针对动态障碍物的避让,运用实时A*算法生成局部动态路径,并与初始路径进行拼接.第三阶段,对找到的路径进行关键点优化和Catmull-Rom 样条平滑处理.实验结果表明该方法在游戏开发中的实用价值.%Taking path search of group intelligent agents in games as the research background, the paper proposes an improved group intelligent pathfinding algorithm. This method divides the whole process of game pathfinding into three stages. The first stage is the pre-treatment stage, aiming at the specific target, it takes reverse path search strategy and establishes the optimal solution path table. In second stage, for the situation of dynamic obstacles avoidance, it uses A* algorithm to generate partial Wai dynamic path, and stitches with the initial path. The third stage optimises the key-point of the found path and smoothes it with Catmull-Rom splines. Experimental results demonstrate the practical value of the method in game development.

  9. Comprehensive measurements in 4 {pi} geometry for radio-active samples having a low {beta}-activity (1962); Ensemble de mesure'en geometrie 4 {pi} pour echantillons radioactifs de faible activite {beta} (1962)

    Energy Technology Data Exchange (ETDEWEB)

    Colomer, J.; Valentin, M. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1961-07-01

    The realisation is described of a comprehensive measurement system having low background noise and, as well as a lead-wall protection, an electronic protection made up of a plastic scintillator placed in anticoincidence with the 4 {pi} counter used for making the measurements. The apparatus is described and its performance discussed. (authors) [French] Realisation d'un ensemble de mesures ayant un faible bruit de fond en utilisant en plus d'une protection par murs de Pb, une protection electronique constituee par un scintillateur plastique mis en ainticoincidence avec le compteur 4 {pi} utilise pour faire les mesures. L'appareillage est decrit et ses performances discutees. (auteurs)

  10. Mesures de déplacements en dynamique par lumière structurée. Compte-rendu d'expérimentations du 27-28 mars 2007

    OpenAIRE

    Muzet, Valérie; MALEK, Mokrane; Cottineau, Louis Marie

    2007-01-01

    L'objectif de cette étude était d'étudier le comportement du capteur optique implanté sur un poids lourd par des essais sur site et de mesurer les vibrations en différents points du camion. Les mesures de vibrations devant permettre à la fois de rechercher les zones les plus appropriées pour le montage des capteurs optiques et de définir les vibrations à éliminer par le montage qui fixera le capteur optique sur le camion

  11. Erreurs induites par l’utilisation d’un capteur de grande taille, un ceptomètre par exemple, pour calculer un coefficient d’extinction à partir de la mesure des rayonnements transmis sous une culture

    OpenAIRE

    Tournebize, Régis; Cornet, Denis; BONHOMME, Raymond

    2010-01-01

    L’estimation des rayonnements solaires interceptés par une culture est une donnée devenue courante en agronomie pour évaluer sa production. Cette estimation est le plus souvent faite à partir de la seule mesure de l’indice foliaire LAI et l’utilisation d’un coefficient d’extinction des rayonnements K. Ce coefficient K est souvent évalué à partir de mesures ponctuelles de l’indice foliaire et de la fraction des rayonnements solaires transmis sous une culture TR, en utilisant la for...

  12. La socialisation au travail comme indicateur de développement professionnel : analyse des approches basées sur la mesure

    Directory of Open Access Journals (Sweden)

    Stéphane Martineau

    2011-06-01

    Full Text Available Cet article porte sur un aspect particulier du développement professionnel c’est-à-dire la socialisation professionnelle (ou organisationnelle. Plus spécifiquement, ce sont certains des aspects méthodologiques des recherches qui sont ici étudiés. Ainsi, les auteurs conduisent une réflexion critique sur les différents outils de mesure les plus utilisés dans les recherches sur la socialisation professionnelle. Les principales insuffisances des recherches sont identifiées et des pistes de perfectionnement des outils sont esquissées. Ils s’interrogent par ailleurs sur la pertinence des approches basées sur la mesure du processus de socialisation professionnelle.This article focuses on a particular aspect of professional development which is professional or organizational socialization. More specifically, some methodological aspects of research on professional socialization are studied here. Thus, the authors conduct a critical analysis on the various measurement tools used in the research on professional socialization. The main shortcomings of the research are identified and possible development tools are outlined. In addition, they also question the relevance of the approaches based on the measure of the process of professional socialization.

  13. Measurements of spectral indices in homogeneous multiplying media; Mesures d'indices de spectre dans les milieux multiplicateurs homogenes

    Energy Technology Data Exchange (ETDEWEB)

    Bruna, J.G.; Brunet, J.P.; Clouet D' Orval, Ch.; Verriere, Ph.; Kremser, J.; Moret-Bailly, J.; Tellier, H. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1964-07-01

    Methods for computation of spectra in light water are developed at Saclay and it is interesting to carry out at the same time experimental studies of simple media such as solutions of fissionable salts which allow quite direct comparisons with computed values. The spectral indices measurements were made with two small fission chambers, one containing deposited plutonium, the other deposited uranium 235. Their response, when neutron spectrum is modified, allows to study the epithermal part of the flux. The media studied with these chambers are fissionable solutions (of plutonium or 90 per cent enriched uranium) which were made critical in bare cylindrical geometry in the Alecto reactor. If the ratio of the chambers is normalized to unity in a Maxwell spectrum, then the noted variation of the ratio of the counts Pu chamber/ U{sup 235} chamber reaches 1,4 in the range of the studied concentrations. (authors) [French] Des calculs de spectres dans l'eau legere sont mis au point a Saclay et il est interessant de mener parallelement des etudes experimentale sur des milieux simples tels que des solutions de sels fissiles, qui permettent des comparaisons tres directes avec les valeurs calculees. On a choisi d'effectuer des mesures d' 'indices de spectres' a l'aide de de deux petites chambres a fission contenant des depots, l'une de plutonium, l'autre d'uranium 235. Leur reponse lorsque le spectre des neutrons est modifie permet d'etudier la partie epithermique du flux. Les milieux etudies a l'aide de ces chambres sont des solutions fissiles (plutonium ou uranium enrichi a 90 pour cent) rendus critiques, en geometrie cylindrique nue, dans le reacteur Alecto. Si le rapport des chambres est normalise a un dans un spectre de Maxwell, la variation constatee du rapport des comptages chambre Pu/ chambre U{sup 235} atteint, dans les gammes de concentrations etudiees, 1,4. (auteurs)

  14. 4 km NODC/RSMAS AVHRR Pathfinder v5.0 and Interim v5.0 Sea Surface Temperature (SST) Data and v5.1 SST Data for 1981-2009

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — The 4 km Pathfinder effort at the National Oceanic and Atmospheric Administration (NOAA) National Oceanographic Data Center (NODC) and the University of Miami's...

  15. 4 km NODC/RSMAS AVHRR Pathfinder v5 Seasonal and Annual Day-Night Sea Surface Temperature Climatologies for 1982-2009 for the Gulf of Mexico (NODC Accession 0072888)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession contains a set of sea surface temperature climatologies for the Gulf of Mexico (GOM), derived from the AVHRR Pathfinder Version 5 sea surface...

  16. Resistivity measurements using a direct current induction method (1963); Mesure de resistivite par la methode d'induction en courant continu (1963)

    Energy Technology Data Exchange (ETDEWEB)

    Delaplace, J.; Hillairet, J. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1964-07-01

    The conventional methods for measuring electrical resistivities necessitate the fixing of electrical contacts on the sample either mechanically or by soldering. Furthermore it is also necessary to carry,out the measurements on low cross-section samples which are not always easy to obtain. Our direct-current induction method on the other hand requires no contacts and can easily be applied to samples of large cross-section. The sample is placed in a uniform magnetic field; at the moment when the current is cut, eddy currents appear in the sample which tend to oppose the disappearance of the field. The way in which the magnetic flux decreases in the sample makes it possible to determine the resistivity of the material. This method has been applied to samples having diameters of between 1 and 30 mm in the case of metals which are good conductors. It gives a value for the local resistivity and makes it possible to detect any variation along a sample. The measurements can be carried out at all temperature from a few degrees absolute to 500 deg. C. We have used the induction method to follow the purification of beryllium by zone-melting; it is in effect possible to estimate the purity of a material by resistivity measurements. We have measured the resistivity along each bar treated by the zone-melting technique and have thus, localised the purest section. High temperature measurements have been carried out on uranium carbide and on iron-aluminium alloys. This method constitutes an interesting means of investigation the resistivity of solid materials. Its accuracy and rapidity make it particularly adapted both to fundamental research and to production control. (authors) [French] Les methodes classiques de mesure de resistivite electrique imposent la realisation sur l'echantillon de contacts electriques obtenus soit mecaniquement, soit par soudure. En outre, elles demandent, le plus souvent, d'effectuer les mesures sur des echantillons de faible section qu

  17. Exploring for Galaxies in the First Billion Years with Hubble and Spitzer - Pathfinding for JWST

    Science.gov (United States)

    Illingworth, Garth D.

    2017-01-01

    Hubble has revolutionized the field of distant galaxies through its deep imaging surveys, starting with the Hubble Deep Field (HDF) in 1995. That first deep survey revealed galaxies at redshift z~1-3 that provided insights into the development of the Hubble sequence. Each new HST instrument has explored new regimes, through the peak of star formation at z~2-3, just 2-3 billion years after the Big Bang, to our first datasets at a billion years at z~6, and then earlier to z~11. HST's survey capabilities were enhanced by 40X with ACS, and then similarly with the WFC3/IR, which opened up the first billion years to an unforeseen degree. I will discuss what we have learned from the remarkable HST and Spitzer imaging surveys (HUDF, GOODS, HUDF09/12 and CANDELS), as well as surveys of clusters like the Hubble Frontier Fields (HFF). Lensing clusters provide extraordinary opportunities for characterizing the faintest earliest galaxies, but also present extraordinary challenges. Together these surveys have resulted in the measurement of the volume density of galaxies in the first billion years down to astonishingly faint levels. The role of faint galaxies in reionizing the universe is still much-discussed, but there is no doubt that such galaxies contribute greatly to the UV ionizing flux, as shown by deep luminosity function studies. Together Hubble and Spitzer have also established the stellar-mass buildup over 97% of cosmic history. Yet some of the greatest surprises have come from the discovery of very luminous galaxies at z~8-11, around 400-650 million years after the Big Bang. Spectroscopic followup by Keck of some of these very rare, bright galaxies has confirmed redshifts from z~7 to z~9, and revealed, surprisingly, strong Lyα emission near the peak of reionization when the HI fraction in the IGM is high. The recent confirmation of a z=11.1 galaxy, just 400 million years after the Big Bang, by a combination of Hubble and Spitzer data, moved Hubble into JWST territory

  18. Aimant PS - Contrôle de l'Etat de 28 Sertissages Internes des PFW - Mesures Effectuées pendant le Grand Arrêt 2003/2004

    CERN Document Server

    Ottaviani, J

    2004-01-01

    Les sertissages (douilles), utilisés pour raccorder les méplats du circuit principal des PFW à leurs câbles d'alimentation, présentent parfois des défauts de réalisation qui entraînent une résistance électrique anormale. Pour mettre en évidence ces défauts, on mesure la résistance des 4 sertissages des nappes polaires. Les nappes sont alimentées avec un courant efficace nominal de 80A. On effectue les mesures entre le bornier de connexions des 4 câbles d'alimentation des PFW et les circuits auxiliaires correspondants (Pick-ups brasés sur les enroulements). De ces mesures (câble d'alimentation et une courte partie du circuit principal), on en déduit la valeur de la résistance du sertissage qui en assure la liaison. A la mesure des résistances des sertissages des nappes polaires supérieures s'ajoute la résistance des câbles qui assurent la liaison entre borniers.

  19. Lidiam - direct-link computer for the photo measurement apparatus of a bubble chamber; Lidiam - liaison directe d'une calculatrice aux appareils de mesure de photos de chambre a bulles

    Energy Technology Data Exchange (ETDEWEB)

    Deler, B. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1964-07-01

    The treatment of bubble chamber pictures can be considerably improved by connecting conventional measuring machines to a small computer providing continuous control of the later as well as the immediate detection of errors and their immediate corrections. The computer will also perform first processing of the measured data. In addition the system described will improve the effective yield of each apparatus and facilitates the control of the data. A description is given here of the apparatus and of some future extensions. (author) [French] L'exploitation des cliches de chambre a bulles peut etre sensiblement amelioree par la jonction directe des appareils de mesure a une calculatrice qui permettra la detection immediate des erreurs et leurs corrections, le controle continu des appareils et un premier traitement des evenements mesures. De plus, le rendement effectif des appareils de mesure sera notablement augmente et la gestion ainsi que l'exploitation des mesures grandement facilitees. Nous presentons ici la description d'un dispositif de ce genre ainsi que les projets d'extensions envisagees.

  20. Pathfinder, Volume 7, Number 5, September/October 2009. Charting the Sea and Sky

    Science.gov (United States)

    2009-10-01

    tsunamis and military exercises. Technology has also accelerated support for maritime missions: our Digital Nautical Chart ( DNC ®) is the only complete...global digital chart set in the world. The DNC ®, updated every 28 days, aggregates hydrographic and bathymetric data along with information about...harbor and port facilities, imagery, surveys and user feedback. The DNC ® is available via CD and the World Wide Web. To support our mission partners in

  1. On-ground testing of the role of adhesion in the LISA-Pathfinder test mass injection phase

    Science.gov (United States)

    Bortoluzzi, D.; Zanoni, C.; Conklin, J. W.

    2017-05-01

    Many space missions share the need to fly a free-falling body inside the spacecraft, as a reference for navigation and/or as a probe for the local gravitational field. When a mechanism is required to cage such an object during the launch phase, the need arises to release it to free-fall once the operational phase must be initiated in orbit. The criticality of this phase increases when the mechanical interfaces between the body and the mechanism are affected by adhesion and the actuation authority of the control system on the free-falling body is limited. Both conditions are realized in the LISA Pathfinder mission, which aims at injecting a gold-coated 2 kg cubic test mass into a nearly perfect geodesic trajectory to demonstrate the readiness of the developed technology for in-space gravity wave detection. The criticality of adhesion is widely recognized in space technology, because it can affect and jeopardize the functionality of mechanisms, when arising between moving parts. In the LISA Pathfinder case, metallic adhesion potentially plays a relevant role, mainly for two reasons. First, thanks to its properties (ductility, high surface energy) the gold coating on the proof mass easily produces cold weldings, especially in vacuum conditions. Second, the detachment of the proof mass from the releasing device occurs abruptly and a relevant influence of the separation velocity is expected on the strength of the welding. This can produce an excessive velocity of the proof mass at the retraction of the releasing device for the following capture and centring phase on behalf of the control system. A testing activity is performed to characterize the dynamic behaviour of the adhesive bonds between the proof mass and the releasing device, which can be used to predict their contribution on the residual velocity of the proof mass after in-flight release. The study of such a dynamic phenomenon sets some challenging requirements on the measurement technique, both on the

  2. Pratique de la mesure ambulatoire de la pression artérielle à Brazzaville (Congo): données préliminaires

    OpenAIRE

    Ikama, Stéphane Méo; Nsitou, Bernice Mesmer; Makani, Jospin; Ellenga-Mbolla, Bertrand; Ondze-Kafata, Louis Igor; Mongo-Ngamami, Solange Flore; Nkalla-Lambi, Mûnka; Gombet, Thierry Raoul; Kimbally-Kaky, Gisèle

    2015-01-01

    Introduction Évaluer l'apport de la MAPA dans la prise en charge de l'hypertension artérielle à Brazzaville. Méthodes Cette étude transversale descriptive a été menée à Brazzaville entre janvier 2011 et décembre 2013 (soit 36 mois). Elle a inclus une série consécutive de 1040 patients ayant bénéficié d'une Mesure Ambulatoire de la Pression Artérielle. Nous avons utilisé le TONOPORT V et le logiciel Cardiosoft 6.51 de GE Health Care, respectivement pour l'enregistrement et l'analyse des donnée...

  3. Application expérimentale du bilan de puissance réactive à la mesure de l'anche de saxophone

    OpenAIRE

    Boutillon, Xavier; Gibiat, V.

    1994-01-01

    La notion de bilan de puissance réactive permet de lier le fonctionnement d'une anche modélisée par un ressort à celui du résonateur qu'elle excite. Un instrument à anche simple ne joue pas exactement sur les fréquences des pics d'impédance. Chaque partiel du tuyau absorbe donc (ou fournit) une puissance réactive. Leur somme algébrique est égale à celle fournie par le ressort qui représente l'anche. Sur le plan expérimental, nous avons mesuré le spectre de pression interne d'un saxophone et s...

  4. Mesure de la Polarisation des Lambda Produits dans les Collisions Positron-Electron AU Lep a L'aide du Detecteur Opal

    Science.gov (United States)

    Vandenplas, Denis

    Le Modele Standard est le cadre theorique general qui, jusqu'a present, a permis l'interpretation de tous les resultats experimentaux en physique des hautes energies. Cette theorie decrit, entre autres, la production d'une paire de particules elementaires, formee d'un quark et d'un antiquark, a partir de la desintegration de l'un des bosons mediateurs de l'interaction faible, le Z^0. Cependant, dans ce cas precis, la transformation subsequente des quarks primaires en particules reelles, un processus appele hadronisation, n'est decrite qu'a l'aide de modeles phenomenologiques. Afin de sonder les mecanismes de l'hadronisation, cette these presente la mesure du transfert du spin d'un quark etrange primaire a une particule appelee Lambda lors des desintegrations hadroniques du Z^0. L'etude a ete realisee dans le cadre de la collaboration OPAL, une des quatre experiences menees au collisionneur LEP, la ou des electrons et des positrons sont acceleres jusqu'a une energie commune, sqrt{s} = {rm E_ {cm}}, voisine de l'energie de production du rm Z^0, M_{Z ^0} egale a 91.3 GeV. La theorie electrofaible precise la direction du spin, c'est-a-dire la polarisation, d'un quark etrange primaire provenant de la desintegration d'un Z ^0. Quant a lui, le modele des quarks etablit que l'orientation du spin d'un Lambda est directement reliee a la polarisation du quark etrange dont il provient. La question est de determiner dans quelle mesure la polarisation du quark primaire est transmise au Lambda a la suite du processus de l'hadronisation, decrit dans le cadre de la ChromoDynamique Quantique. Une estimation, qui tient compte de tous ces differents aspects theoriques, evalue a 30% la polarisation des Lambda dont l'impulsion est superieure a 15 GeV/c. La mesure experimentale de la polarisation repose sur l'identification des Lambda a partir de la reconstitution de la desintegration Lambdato ppi^-. Ce processus, qui se deroule par le biais de l'interaction faible, viole la parite car

  5. Etablissement de tests permettant de mesurer l'impact sur les performances de la sécurisation d'IPv6 par IPsec

    OpenAIRE

    Bernard, Nicolas

    2002-01-01

    Magistère d'Informatique et Modélisation. Rapport de stage.; Ce document explique comment s'effectue la sécurisation des réseaux IPv6 à l'aide du protocole IPsec. Il présente, dans le contexte du système FreeBSD, comment est réalisée l'implémentation d'IPsec, sa configuration statique et dynamique. Il décrit ensuite les différents outils de mesure de performance utilisés et leur portage sur IPv6. Il présente enfin les résultats des tests réalisés au sein du laboratoire.

  6. Fundamental Performance Determining Factors of the Ultrahigh-Precision Space-Borne Optical Metrology System for the LISA Pathfinder mission

    CERN Document Server

    Hechenblaikner, Gerald

    2013-01-01

    The LISA Pathfinder mission to space employs an optical metrology system (OMS) at its core to measure the distance and attitude between two freely floating test-masses to picometer and nanorad accuracy, respectively, within the measurement band of [1 mHz, 30 mHz]. The OMS is based upon an ultra-stable optical bench with 4 heterodyne interferometers from which interference signals are read-out and processed by a digital phase-meter. Laser frequency noise, power fluctuations and optical path-length variations are suppressed to uncritical levels by dedicated control loops so that the measurement performance approaches the sensor limit imposed by the phase-meter. The system design is such that low frequency common mode noise which affects the read-out phase of all four interferometers is generally well suppressed by subtraction of a reference phase from the other interferometer signals. However, high frequency noise directly affects measurement performance and its common mode rejection depends strongly on the rel...

  7. Stem-loop binding protein is required for retinal cell proliferation, neurogenesis, and intraretinal axon pathfinding in zebrafish.

    Science.gov (United States)

    Imai, Fumiyasu; Yoshizawa, Asuka; Matsuzaki, Ayako; Oguri, Eri; Araragi, Masato; Nishiwaki, Yuko; Masai, Ichiro

    2014-10-01

    In the developing retina, neurogenesis and cell differentiation are coupled with cell proliferation. However, molecular mechanisms that coordinate cell proliferation and differentiation are not fully understood. In this study, we found that retinal neurogenesis is severely delayed in the zebrafish stem-loop binding protein (slbp) mutant. SLBP binds to a stem-loop structure at the 3'-end of histone mRNAs, and regulates a replication-dependent synthesis and degradation of histone proteins. Retinal cell proliferation becomes slower in the slbp1 mutant, resulting in cessation of retinal stem cell proliferation. Although retinal stem cells cease proliferation by 2 days postfertilization (dpf) in the slbp mutant, retinal progenitor cells in the central retina continue to proliferate and generate neurons until at least 5dpf. We found that this progenitor proliferation depends on Notch signaling, suggesting that Notch signaling maintains retinal progenitor proliferation when faced with reduced SLBP activity. Thus, SLBP is required for retinal stem cell maintenance. SLBP and Notch signaling are required for retinal progenitor cell proliferation and subsequent neurogenesis. We also show that SLBP1 is required for intraretinal axon pathfinding, probably through morphogenesis of the optic stalk, which expresses attractant cues. Taken together, these data indicate important roles of SLBP in retinal development.

  8. Observation of polarized hard X-ray emission from the Crab by the PoGOLite Pathfinder

    Science.gov (United States)

    Chauvin, M.; Florén, H.-G.; Jackson, M.; Kamae, T.; Kawano, T.; Kiss, M.; Kole, M.; Mikhalev, V.; Moretti, E.; Olofsson, G.; Rydström, S.; Takahashi, H.; Iyudin, A.; Arimoto, M.; Fukazawa, Y.; Kataoka, J.; Kawai, N.; Mizuno, T.; Ryde, F.; Tajima, H.; Takahashi, T.; Pearce, M.

    2016-02-01

    We have measured the linear polarization of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the polarization fraction and angle stands to disentangle geometrical and physical effects, thereby providing information on the pulsar wind geometry and magnetic field environment. Measurements are conducted using the PoGOLite Pathfinder - a balloon-borne polarimeter. Polarization is determined by measuring the azimuthal Compton scattering angle of incident X-rays in an array of plastic scintillators housed in an anticoincidence well. The polarimetric response has been characterized prior to flight using both polarized and unpolarized calibration sources. We address possible systematic effects through observations of a background field. The measured polarization fraction for the integrated Crab light curve is 18.4^{+9.8}_{-10.6} per cent, corresponding to an upper limit (99 per cent credibility) of 42.4 per cent, for a polarization angle of (149.2 ± 16.0)°.

  9. Coupling of relative intensity noise and pathlength noise to the length measurement in the optical metrology system of LISA Pathfinder

    Science.gov (United States)

    Wittchen, Andreas; the LPF Collaboration

    2017-05-01

    LISA Pathfinder is a technology demonstration mission for the space-based gravitational wave observatory, LISA. It demonstrated that the performance requirements for the interferometric measurement of two test masses in free fall can be met. An important part of the data analysis is to identify the limiting noise sources. [1] This measurement is performed with heterodyne interferometry. The performance of this optical metrology system (OMS) at high frequencies is limited by sensing noise. One such noise source is Relative Intensity Noise (RIN). RIN is a property of the laser, and the photodiode current generated by the interferometer signal contains frequency dependant RIN. From this electric signal the phasemeter calculates the phase change and laser power, and the coupling of RIN into the measurement signal depends on the noise frequency. RIN at DC, at the heterodyne frequency and at two times the heterodyne frequency couples into the phase. Another important noise at high frequencies is path length noise. To reduce the impact this noise is suppressed with a control loop. Path length noise not suppressed will couple directly into the length measurement. The subtraction techniques of both noise sources depend on the phase difference between the reference signal and the measurement signal, and thus on the test mass position. During normal operations we position the test mass at the interferometric zero, which is optimal for noise subtraction purposes. This paper will show results from an in-flight experiment where the test mass position was changed to make the position dependant noise visible.

  10. Influence of brain-derived neurotrophic factor on pathfinding of dentate granule cell axons, the hippocampal mossy fibers

    Directory of Open Access Journals (Sweden)

    Tamura Makoto

    2009-01-01

    Full Text Available Abstract Mossy fibers, the dentate granule cell axons, are generated throughout an animal's lifetime. Mossy fiber paths and synapses are primarily restricted to the stratum lucidum within the CA3 region. Brain-derived neurotrophic factor (BDNF, a neurotrophin family protein that activates Trk neurotrophin receptors, is highly expressed in the stratum lucidum in an activity-dependent manner. The addition of a Trk neurotrophin receptor inhibitor, K252a, to cultured hippocampal slices induced aberrant extension of mossy fibers into ectopic regions. BDNF overexpression in granule cells ameliorated the mossy fiber pathway abnormalities caused by a submaximal dose of K252a. A similar rescue was observed when BDNF was expressed in CA3 pyramidal cells, most notably in mossy fibers distal to the expression site. These findings are the first to clarify the role of BDNF in mossy fiber pathfinding, not as an attractant cue but as a regulator, possibly acting in a paracrine manner. This effect of BDNF may be as a signal for new fibers to fasciculate and extend further to form synapses with neurons that are far from active BDNF-expressing synapses. This mechanism would ensure the emergence of new independent dentate gyrus-CA3 circuits by the axons of new-born granule cells.

  11. Influence of brain-derived neurotrophic factor on pathfinding of dentate granule cell axons, the hippocampal mossy fibers.

    Science.gov (United States)

    Tamura, Makoto; Tamura, Naohiro; Ikeda, Takamitsu; Koyama, Ryuta; Ikegaya, Yuji; Matsuki, Norio; Yamada, Maki K

    2009-01-31

    Mossy fibers, the dentate granule cell axons, are generated throughout an animal's lifetime. Mossy fiber paths and synapses are primarily restricted to the stratum lucidum within the CA3 region. Brain-derived neurotrophic factor (BDNF), a neurotrophin family protein that activates Trk neurotrophin receptors, is highly expressed in the stratum lucidum in an activity-dependent manner. The addition of a Trk neurotrophin receptor inhibitor, K252a, to cultured hippocampal slices induced aberrant extension of mossy fibers into ectopic regions. BDNF overexpression in granule cells ameliorated the mossy fiber pathway abnormalities caused by a submaximal dose of K252a. A similar rescue was observed when BDNF was expressed in CA3 pyramidal cells, most notably in mossy fibers distal to the expression site. These findings are the first to clarify the role of BDNF in mossy fiber pathfinding, not as an attractant cue but as a regulator, possibly acting in a paracrine manner. This effect of BDNF may be as a signal for new fibers to fasciculate and extend further to form synapses with neurons that are far from active BDNF-expressing synapses. This mechanism would ensure the emergence of new independent dentate gyrus-CA3 circuits by the axons of new-born granule cells.

  12. 游戏中路径搜索算法研究%Research on Pathfinding Algorithm in Games

    Institute of Scientific and Technical Information of China (English)

    韩玮

    2012-01-01

    Pathfinding is a core component of most games, the best-known algorithm is the A* search, but the A* algorithm can be woefully inadequate for achieving the kind of realistic movement requires in games. This paper introduces the A* algorithm and analyzes it' s path problem, proposes a smooth algorithm, which solves the problem of A* in games.%路径搜索是游戏中非常重要的一部分,A*算法是最常用的搜索算法,但是使用A*算法搜索出的路径的真实性常常不能让人满意.本文介绍A*搜索算法及存在的路径问题,针对该算法在游戏中暴露的问题,提出一种平滑改进的算法,较好地解决了这个问题.

  13. Mesure du taux de couverture du sol pour estimer les principales caractéristiques d’une culture de colza avant montaison

    Directory of Open Access Journals (Sweden)

    Denoroy Pascal

    2000-01-01

    Full Text Available L’étude de paramètres biologiques en expérimentation au champ est fastidieuse et les mesures directes sur échantillons de plantes induisent des problèmes pratiques, en particulier pour le suivi hivernal des cultures (durée du prélèvement, conservation, rapidité de traitement…, qui limitent leur utilisation à un petit nombre d’essais. Aussi, en général, peu de mesures sont réalisées en cours de végétation et, si on dispose de résultats finals, on n’a guère d’informations quantitatives intermédiaires, en particulier sur la dynamique d’installation de la culture. Ces informations permettraient pourtant de mieux analyser les sources de variation des résultats par une analyse de différents processus de la croissance : mise en place de la surface foliaire, accumulation de la matière sèche, absorption des minéraux… Il serait donc utile de disposer de méthodes permettant d’estimer des variables d’état biologiques en cours de culture tout en minimisant le temps et les moyens nécessaires au recueil des données. Ce qui suit fait état des résultats obtenus dans une étude concernant l’intérêt d’utiliser de simples photographies verticales pour estimer diverses grandeurs caractérisant une culture de colza au stade rosette. Ces travaux font suite à des résultats publiés précédemment, d’une part, sur blé [1] et d’autre part, sur maïs et betterave [2].

  14. Measurement of the electronic density of ionised media by hyper frequency methods; Mesure de la densite electronique des milieux ionises par des methodes hyperfrequences

    Energy Technology Data Exchange (ETDEWEB)

    Consoli, T. [Commissariat a l' Energie Atomique, Saclay (France).Centre d' Etudes Nucleaires

    1960-07-01

    Within the limits of the I.N.S.T.N. courses on plasmas, this analytical study summarizes the articles quoted in the references on hyper-frequency techniques for the measurement of electronic density of an ionised gas. It is neither exhaustive nor complete and further details may be obtained by referring to the works mentioned. The first part, devoted to the theoretical side, concert the propagation of electromagnetic waves ionised media and the excitation of stationary raves in electromagnetic cavities. The second part deals with the measurement techniques themselves. It includes those techniques which hare become classic, and also more recent ones being developed in various laboratories and in the Service of Applied Physics at Saclay. (author) [French] Dans le cadre des cours sur les plasmas a l'l.N.S.T. cette etude d'analyse resume les articles cites en bibliographie sur les techniques hyperfrequences pour la mesure de la densite electronique d'un gas ionise. Elle n'est ni exhaustive, ni complete. Pour plus de details on voudra bien se rapporter aux travaux mentionnes. La premiere partie consacree a des rappels theoriques, concerne la propagation des ondes electromagnetiques dans les milieux ionises et sur l'excitation d'ondes stationnaires dans les cavites electromagnetiques. La seconde se rapporte aux techniques de mesures proprement dites. On a fait figurer dans cette partie des techniques devenues classiques et celles plus recentes en cours d'etudes dans divers laboratoires et au Service de Physique Appliquee a SACLAY. (auteur)

  15. Predictions for ASKAP Neutral Hydrogen Surveys

    CERN Document Server

    Duffy, Alan R; Staveley-Smith, Lister; Bernyk, Maksym; Croton, Darren J; Koribalski, Barbel S; Gerstmann, Derek; Westerlund, Stefan

    2012-01-01

    The Australian Square Kilometer Array Pathfinder (ASKAP) will revolutionise our knowledge of gas-rich galaxies in the Universe. Here we present predictions for two proposed extragalactic ASKAP neutral hydrogen (HI) emission-line surveys, based on semi-analytic models applied to cosmological N-body simulations. The ASKAP HI All-Sky Survey, known as WALLABY, is a shallow 3 Pi survey (z = 0 - 0.26) which will probe the mass and dynamics of over 600,000 galaxies. A much deeper small-area HI survey, called DINGO, aims to trace the evolution of HI from z = 0 - 0.43, a cosmological volume of 40 million Mpc^3, detecting potentially 100,000 galaxies. The high-sensitivity 30 antenna ASKAP core (diameter ~2 km) will provide an angular resolution of 30 arcsec (at z=0). Our simulations show that the majority of galaxies detected in WALLABY (87.5%) will be resolved. About 5000 galaxies will be well resolved, i.e. more than five beams (2.5 arcmin) across the major axis, enabling kinematic studies of their gaseous disks. Thi...

  16. The Primordial Anisotropy Polarization Pathfinder Array (PAPPA): Instrument Overview and Status

    Science.gov (United States)

    Chuss, David

    2006-01-01

    PAPPA is a balloon-based experiment designed to measure the polarization of the Cosmic Microwave Background using candidate technology for an eventual Inflation Probe mission. It will survey a 20 x 20 degree patch of sky with 1 degree angular resolution covering 3 passbands centered at 100,200 and 300 GHz. Detection will be accomplished via antenna-coupled transition edge sensors (TESs) with SQUID-based readouts. In the eventual flight package, band defining filters and MEMS-based polarization modulators will be incorporated into the superconducting microstrip transmission lines that terminate in resistors that are thermally coupled to the TESs. The MEMS switches will allow on-chip polarization modulation that is faster than significant detector gain variations. The initial configuration will incorporate a simplified focal plane augmented by quasioptical polarization modulation. We describe the overall instrument design and present a summary of the current progress.

  17. Propriétés d'un fil quantique connecté à des fils de mesure

    Science.gov (United States)

    Safi, Inès.

    étique. Afin d'identifier les flux d'électrons incident et transmis, des fils intermédiaires sans interactions sont introduits, et le système global est traité comme un liquide de Tomonaga-Luttinger inhomogène. La transmission du flux est parfaite dans la limite stationnaire : un électron incident est transmis en une série de charges partielles spatialement séparées dont la somme vaut l'unité. Il est par ailleurs remarquable que les parties charge et spin transmises restent séparées dans le fil externe sans interactions. La conductance est déduite de la transmission parfaite suivant un argument analogue à celui de l'approche de diffusion. Elle peut aussi être reliée exactement à la transmission en modélisant les réservoirs par un potentiel électrostatique externe fixé. Elle est donc égale à e2/h pour une portée finie arbitraire des interactions. Ce résultat de conductance a été confirmé par des observations expérimentales récentes sur les fils quantiques (Tarucha et al. et Yacoby et al.) dont la conductance présente un plateau à e2/h dans la limite balistique (haute température). Ceci contredit le consensus général jusque-là admis, prédisant en particulier une réduction de la conductance par des interactions répulsives qui devient encore plus importante pour des interactions à longue portée. Le transport dynamique est développé en présence des contacts. La conservation globale de la charge est assurée en tenant compte d'une grille avoisinante. Les coefficients de conductance dynamiques sont exprimés en fonction de la transmission et de la réflexion des plasmons, qui dépendent eux-mêmes des interactions. Il est possible d'étendre cette approche à des fils de mesure avec interactions, quoique des hypothèses supplémentaires sont nécessaires. Par ailleurs, dans le cas usuel d'interactions invariantes par translation, ce travail en donne une revue relativement complète, en suivant des méthodes différentes et en d

  18. ASKAP and MeerKAT surveys of the Magellanic Clouds

    CERN Document Server

    van Loon, Jacco Th

    2010-01-01

    The Magellanic Clouds are a stepping stone from the overwhelming detail of the Milky Way in which we are immersed, to the global characteristics of galaxies both in the nearby and distant universe. They are interacting, gas-rich dwarf galaxies of sub-solar metallicity, not unlike the building blocks that assembled the large galaxies that dominate groups and clusters, and representative of the conditions at the height of cosmic star formation. The Square Kilometre Array (SKA) can make huge strides in understanding galactic metabolism and the ecological processes that govern star formation, by observations of the Magellanic Clouds and other, nearby Magellanic-type irregular galaxies. Two programmes with SKA Pathfinders attempt to pave the way: the approved Galactic ASKAP Spectral Line Survey (GASKAP) includes a deep survey in HI and OH of the Magellanic Clouds, whilst MagiKAT is proposed to perform more detailed studies of selected regions within the Magellanic Clouds - also including Faraday rotation measureme...

  19. Mesure par interférométrie laser du mouvement d'une particule proche d'une paroi

    Science.gov (United States)

    Assou, Y.; Joyeux, D.; Azouni, A.; Feuillebois, F.

    1991-02-01

    , et l'alignement de la sphère dans le montage optique sont relativement peu critiques. Les sphères utilisées sont des billes de roulements à billes, de 4 et 5 × 10^{-3} m de diamètre. La précision sur le déplacement de la sphère est de l'ordre de 2 × 10^{-8} m. Le signal d'interférence est digitalisé et stocké dans un micro-ordinateur. Le traitement des données permet alors d'obtenir le coefficient de frottement f^T_zz de la sphère en mouvement tout près de la paroi. La variation de f^T_zz avec l'intervalle sans dimension \\varepsilon (rapport de l'intervalle entre la sphère et la paroi au rayon de la sphère) permet de distinguer trois régions: (i) Une région où \\varepsilon est petit mais au moins 10 fois plus grand que la rugosité non dimensionnelle (rapport de l'échelle de la rugosité au rayon de la sphère) ; le résultat expérimental est alors en très bon accord avec la formule f^T_zz = 1/\\varepsilon démontrée en théorie de la lubrification, formule valable pour une sphère lisse. (ii) Lorsque \\varepsilon décroît pour devenir de l'ordre de grandeur de la rugosité non dimensionnelle, le coefficient de frottement est alors inférieur à Il E. La technique ouvre ainsi une nouvelle voie à l'étude des effets de rugosité en hydrodynamique. (iii) La technique permet de mesurer des intervalles de l'ordre de 10^{-8} m et pourrait ainsi être utilisée dans l'étude des forces à courte portée.

  20. Slit and Netrin-1 guide cranial motor axon pathfinding via Rho-kinase, myosin light chain kinase and myosin II

    Directory of Open Access Journals (Sweden)

    Drescher Uwe

    2010-06-01

    Full Text Available Abstract Background In the developing hindbrain, cranial motor axon guidance depends on diffusible repellent factors produced by the floor plate. Our previous studies have suggested that candidate molecules for mediating this effect are Slits, Netrin-1 and Semaphorin3A (Sema3A. It is unknown to what extent these factors contribute to floor plate-derived chemorepulsion of motor axons, and the downstream signalling pathways are largely unclear. Results In this study, we have used a combination of in vitro and in vivo approaches to identify the components of floor plate chemorepulsion and their downstream signalling pathways. Using in vitro motor axon deflection assays, we demonstrate that Slits and Netrin-1, but not Sema3A, contribute to floor plate repulsion. We also find that the axon pathways of dorsally projecting branchiomotor neurons are disrupted in Netrin-1 mutant mice and in chick embryos expressing dominant-negative Unc5a receptors, indicating an in vivo role for Netrin-1. We further demonstrate that Slit and Netrin-1 signalling are mediated by Rho-kinase (ROCK and myosin light chain kinase (MLCK, which regulate myosin II activity, controlling actin retrograde flow in the growth cone. We show that MLCK, ROCK and myosin II are required for Slit and Netrin-1-mediated growth cone collapse of cranial motor axons. Inhibition of these molecules in explant cultures, or genetic manipulation of RhoA or myosin II function in vivo causes characteristic cranial motor axon pathfinding errors, including the inability to exit the midline, and loss of turning towards exit points. Conclusions Our findings suggest that both Slits and Netrin-1 contribute to floor plate-derived chemorepulsion of cranial motor axons. They further indicate that RhoA/ROCK, MLCK and myosin II are components of Slit and Netrin-1 signalling pathways, and suggest that these pathways are of key importance in cranial motor axon navigation.

  1. Automatic remote sensing detection of the convective boundary layer structure over flat and complex terrain using the novel PathfinderTURB algorithm

    Science.gov (United States)

    Poltera, Yann; Martucci, Giovanni; Hervo, Maxime; Haefele, Alexander; Emmenegger, Lukas; Brunner, Dominik; Henne, stephan

    2016-04-01

    We have developed, applied and validated a novel algorithm called PathfinderTURB for the automatic and real-time detection of the vertical structure of the planetary boundary layer. The algorithm has been applied to a year of data measured by the automatic LIDAR CHM15K at two sites in Switzerland: the rural site of Payerne (MeteoSwiss station, 491 m, asl), and the alpine site of Kleine Scheidegg (KSE, 2061 m, asl). PathfinderTURB is a gradient-based layer detection algorithm, which in addition makes use of the atmospheric variability to detect the turbulent transition zone that separates two low-turbulence regions, one characterized by homogeneous mixing (convective layer) and one above characterized by free tropospheric conditions. The PathfinderTURB retrieval of the vertical structure of the Local (5-10 km, horizontal scale) Convective Boundary Layer (LCBL) has been validated at Payerne using two established reference methods. The first reference consists of four independent human-expert manual detections of the LCBL height over the year 2014. The second reference consists of the values of LCBL height calculated using the bulk Richardson number method based on co-located radio sounding data for the same year 2014. Based on the excellent agreement with the two reference methods at Payerne, we decided to apply PathfinderTURB to the complex-terrain conditions at KSE during 2014. The LCBL height retrievals are obtained by tilting the CHM15K at an angle of 19 degrees with respect to the horizontal and aiming directly at the Sphinx Observatory (3580 m, asl) on the Jungfraujoch. This setup of the CHM15K and the processing of the data done by the PathfinderTURB allows to disentangle the long-transport from the local origin of gases and particles measured by the in-situ instrumentation at the Sphinx Observatory. The KSE measurements showed that the relation amongst the LCBL height, the aerosol layers above the LCBL top and the gas + particle concentration is all but

  2. Future HI Surveys on the road to the SKA

    CERN Document Server

    Braun, Robert

    2007-01-01

    In this short contribution we consider what types of surveys might be optimally pursued with path-finding instruments of 1%, 10% and finally 100% of the projected SKA sensitivity from the perspective of scientific applications that utilize the red-shifted 21 cm emission line. Achieving interesting HI galaxy sample sizes with 1% SKA surveys requires very substantial survey durations, of about 1000 days. Good sampling (log(N)~5) down to below M_HI* can then be achieved out to z=0.2 over 8000 deg^2 of survey area or even to z=0.5 over 800 deg^2. The same surveys will permit the resolved imaging of order 1000 galaxies in each of several red-shift bins as well as detection of faint neutral filaments in the vicinity of galaxies with a column density of about 10^18 cm^-2. Once 10% SKA sensitivities are achieved, then ground-breaking surveys are possible with only 100 day duration. Sample sizes of log(N)~6 extending below M_HI* are possible over 800 deg^2 out to z=0.5 and over 80 deg^2 out to z=1. Such surveys will p...

  3. Se déplacer en voiture à Boston : essai de mesure de circulation en temps réel par usage des floating car data (données flottantes automobiles

    Directory of Open Access Journals (Sweden)

    Gérald Billard

    2015-12-01

    Full Text Available Comment mesurer les temps de trajets réels des automobilistes dans les métropoles américaines ? Tout en introduisant la problématique de l’adaptation de l’urbanisme aux nouveaux enjeux de la mobilité aux États-Unis, cet article a pour objectif simple d’exposer une méthodologie développée afin de mesurer l’accessibilité d’un lieu donné. L’originalité de cette méthode est l’exploitation des données en ligne fournies en temps réel par le site TomTom.

  4. Appareillage automatisé de mesure simultanée du pouvoir thermoélectrique et de la conductivité électrique. Application à l'étude de couches polymères semi-conductrices

    OpenAIRE

    Moliton, André; Ratier, Bernard; Moreau, C.; Froyer, G.

    1991-01-01

    Nous présentons dans cet article un système de mesure simultanée de la conductivité σ, et du pouvoir thermoélectrique S : il permet des mesures en fonction de la température (entre 130 K et 360 K) dans le cas de couches semi-conductrices relativement fragiles. A titre d'application, nous indiquons les résultats que nous avons obtenus dans le cas de couches polymères (PPP) implantées avec des ions sodium: alors que seule une semi-conduction par défaut est générée par de fortes énergies d'impla...

  5. Vapour pressure studies of uranium dioxide UO{sub 2} by the effusion method; Mesure de la tension de vapeur du bioxyde d'uranium UO{sub 2} par la methode d'effusion

    Energy Technology Data Exchange (ETDEWEB)

    Ohse, R.W. [Commissariat a l' Energie Atomique, Fontenay-aux-Roses (France). Centre d' Etudes Nucleaires

    1965-07-01

    A high temperature apparatus for vapour pressure measurements by Knudsen effusion method is described. Sample is heated in a tungsten cell in an electronic bombardment furnace. Several critical factors affecting the accuracy of measurements such as: - temperature distribution and measurement in the effusion cell, - CLAUSING factor and molecular flow, - compatibility between cell material and sample heated, are discussed with careful attention. Vapour pressure of UO{sub 2} has been studied between 2200 and 2800 K. Experimental points fit a curve expressed by: logP{sub mm} = 12.4264 - (3.3184/T * 10{sup 4}/T) which is in good agreement with previous results of literature. (author) [French] On decrit un appareil destine a la mesure des tensions de vapeur par la methode d'effusion de KNUDSEN. L'echantillon contenu dans une cellule en tungstene est chauffe par bombardement electronique. Apres examen critique des divers facteurs affectant l'exactitude des mesures, a savoir: - homogeneite et mesure de la temperature dans la cellule d'effusion, - facteur de 'CLAUSING' et loi de distribution en cosinus des molecules effusees, - compatibilite a chaud entre le materiau de la cellule et le materiau etudie. On a procede a la mesure de la tension de vapeur de UO{sub 2} qui est relativement bien connue. Entre 2200 et 2800 K les points experimentaux se placent sur une courbe: logP{sub mm} = 12.4264 - (3.3184/T * 10{sup 4}/T) en bon accord avec les valeurs citees dans la litterature. (auteur)

  6. Alternatives to imprisonment: opportunities and problems in Germany / Mesures alternatives à l’incarcération : opportunités et problèmes en Allemagne

    Directory of Open Access Journals (Sweden)

    Bahr Alexander

    2016-12-01

    Full Text Available L'articolo fornisce una breve panoramica sulla normativa tedesco in materia di misure alternative alla detenzione. Vengono successivamente presentati i dati statistici relativi agli istituti penitenziari tedeschi e gli autori riflettono sulle problematiche principali della situazione attuale delle carceri tedesche. Inoltre, sulla base di dati statistici e di esempi pratici, l'articolo presenta una panoramica complessiva sulle misure alternative in Germania e sullo stato dell’arte della ricerca. Infine, gli autori sottolineano il ruolo e la prospettiva delle vittime, arrivando alla conclusione che una serie di iniziative e di progetti sono già stati avviati, ma che è ancora troppo presto per poter giungere a delle conclusioni. Cet article donne un aperçu du cadre juridique allemand des mesures alternatives à l’incarcération. Des données statistiques sur les prison allemandes et sur les détenus sont ensuite présentées. Les auteurs s’interrogent sur certains des principaux problèmes liés à la situation actuelle des prisons allemandes. De plus, cet article donne un aperçu global des mesures alternatives en Allemagne par le biais de données statistiques et d’exemples concrets. S’ensuit l’état des évaluations scientifiques et de la recherche. Enfin, les auteurs valorisent le rôle et la perspective des victimes, toutefois dans leurs conclusions ils soulignent que nombreux sont les programmes et les initiatives déjà commencés, mais qu’il est cependant encore trop tôt pour dresser un bilan. The article provides a short overview on the German legal framework regarding alternatives to imprisonment. Then statistical data about German prisons and their inmates are presented and the authors reflect on some major problems of the contemporary situation in German prisons. Furthermore, the article gives a comprehensive overview on alternative measures in Germany by statistical data and examples from the practice. Then the state

  7. Pollution odorante par les moteurs Diesel. Mesure des odeurs d'échappement Odorous Pollution by Diesel Engines. Measuring Exhaust Odors

    Directory of Open Access Journals (Sweden)

    Degobert P.

    2006-11-01

    Full Text Available Les études de mesure d'odeur Diesel ont commencé en 1956 aux États-Unis, en particulier pour réduire le niveau odorant des autobus. Cet article expose d'abord les mécanismes de formation des odorants puis les études américaines, qui ont abouti en 1973 à l'odorimètre Arthur D. Little, basé sur l'analyse par chromatographie liquide de l'échappement, et ses corrélations avec les données sensorielles recueillies dans des conditions particulières. Les économies d'énergie dans les villes européennes entraînent un accroissement du nombre de véhicules Diesel, ce qui peut amener un niveau odorant incompatible avec le bien-être. C'est pourquoi l'Institut Français du Pétrole (IFP étudie actuellement les odeurs Diesel, pour mettre au point des méthodes de mesure fiables, partant de la chromatographie liquide type Arthur D. Little (ADL et de l'évaluation sensorielle. Les résultats actuels montrent qu'à moins de progrès importants en analyse chimique, l'évaluation sensorielle reste la méthode la plus fiable. Les perspectives futures basées sur l'olfactomètre différentiel Mac Leod sont présentées. Research was beg un in the United States in 1956 on the medsurementof diesel engine odors, and especially on reducing the odor from diesel city buses. This article begins by describing the mechanisms of odor formation and then goes on ta, review US research which resulted in the Arthur D. Little odormeter in 1973, based on a liquid chromatography analysis of exhaust and its corrélations with sensory data gathered under specific conditions. Energy conservation in European cities is tending ta, increase the number of diesel vehicles and possibly ta, create an odor level that is incompatible with humal well-being. This is why Institut Français du Pétrole (IFP is now investigating diesel eng ine odors for the purpose of developing reliable measuring methods based on liquid chromatography of the Arthur D. Little (ADl type and on

  8. Les principes distributifs des mesures d’insertion des jeunes à l’épreuve du longitudinal Youth integration measures and their criteria tested by a longitudinal approach

    Directory of Open Access Journals (Sweden)

    Léa Lima

    2009-07-01

    Full Text Available La sélection des bénéficiaires des mesures d’action sociale relève d’un problème éthique qui fait l’objet d’une intense activité cognitive et normative de la part d’acteurs publics outillés par l’expertise. Or, l’examen historique des principes distributifs mobilisés dans les politiques d’insertion des jeunes donne à voir la reformulation des référentiels de l’action publique dans un cadre longitudinal ainsi que ses effets sur les présupposés éthiques des politiques. Le principe de discrimination positive consistant à redistribuer les chances d’insertion en faveur des jeunes les moins formés a été énoncé au sein d’une représentation instantanéiste de l’insertion des jeunes. Il perd de sa validité avec l’institutionnalisation des trajectoires. L’éthique de l’accompagnement du parcours qui devient dominante dans les années 1990 perd de vue les inégalités entre groupes de niveau de formation au profit d’une démarche d’organisation de carrières ascendantes permises par les mesures d’action sociale disponibles.Targeting social programs is an ethical problem for administrators. Therefore, they develop an intense cognitive and normative activity with the help of experts in economics. The history of how funds are allocated in support of youth integration policies shows the longitudinal reframing of public policy and its impact on ethical principles. The principle of affirmative action consisting in redistributing offers among less qualified youth has been formulated according to a static representation of youth integration. It loses its validity with the institutionalization of individual itineraries. The ethic of pathway support that became dominant in the 1990s lost sight of the inequality between groups levels of qualification no longer appeared relevant and gave way to the organization of upwardly mobile careers made possible by the social programs at hand.

  9. A*算法在游戏寻路中的应用%Application of A * Algorithm in Game Path-finding Development

    Institute of Scientific and Technical Information of China (English)

    胡正红; 张俊花

    2012-01-01

    Path-finding is the basic problem for game designing to solve. Usually, it is completed by breadth-first search algo- rithm. In this paper, it focuses on the feature of path-finding in " Picture Matching" game to analyze in detail the application of A * Algorithm in the game, points out the composition of evaluation function, and then gives the improved realization of A * Algorithm combining With the actual condition.%寻路问题是游戏设计解决的基本问题,通常采用广度优先搜索算法完成。针对“连连看”游戏的路径搜索特点,详细地分析了A*算法在其中的应用,确认最初估价函数的构成,结合实际应用情况,给出了A*算法的改进及实现。

  10. Perturbations of microRNA function in mouse dicer mutants produce retinal defects and lead to aberrant axon pathfinding at the optic chiasm.

    Directory of Open Access Journals (Sweden)

    Rita Pinter

    Full Text Available BACKGROUND: During development axons encounter a variety of choice points where they have to make appropriate pathfinding decisions. The optic chiasm is a major decision point for retinal ganglion cell (RGC axons en route to their target in order to ensure the correct wiring of the visual system. MicroRNAs (miRNAs belong to the class of small non-coding RNA molecules and have been identified as important regulators of a variety of processes during embryonic development. However, their involvement in axon guidance decisions is less clear. METHODOLOGY/PRINCIPAL FINDINGS: We report here that the early loss of Dicer, an essential protein for the maturation of miRNAs, in all cells of the forming retina and optic chiasm leads to severe phenotypes of RGC axon pathfinding at the midline. Using a conditional deletion approach in mice, we find in homozygous Dicer mutants a marked increase of ipsilateral projections, RGC axons extending outside the optic chiasm, the formation of a secondary optic tract and a substantial number of RGC axons projecting aberrantly into the contralateral eye. In addition, the mutant mice display a microphthalmia phenotype. CONCLUSIONS: Our work demonstrates an important role of Dicer controlling the extension of RGC axons to the brain proper. It indicates that miRNAs are essential regulatory elements for mechanisms that ensure correct axon guidance decisions at the midline and thus have a central function in the establishment of circuitry during the development of the nervous system.

  11. Thermal, intermediate and fast neutron flux measurements using activation detectors; Mesure des flux de neutrons thermiques, intermediaires et rapides au moyen de detecteurs par activation

    Energy Technology Data Exchange (ETDEWEB)

    Brisbois, J.; Lott, M.; Manent, G. [Commissariat a l' Energie Atomique, Fontenay-aux-Roses (France). Centre d' Etudes Nucleaires

    1964-07-01

    The problem of neutron flux measurements using activation detectors is studied in the particular case of protection research. It is shown how it possible, it is possible, using a known thermal flux, to organise a coherent calibration system for all the detectors. The rapid neutron detectors are calibrated with respect to a reference detector (phosphorus) in a natural uranium converter; the intermediate neutron detectors with respect to gold in the axial channel of ZOE. This method makes it possible to minimise the errors due to the activation cross-sections. A brief description is given of the counting room of the Pile Safety Study Service, as well of the practical utilisation characteristics of the counters employed. (authors) [French] Le probleme de la mesure des flux de neutrons au moyen de detecteurs par activation est etudie dans le cas particulier des etudes de protections. On montre comment, a partir d'un flux thermique connu, on peut organiser un systeme coherent d'etalonnage de tous les detecteurs. Les detecteurs de neutrons rapides sont etalonnes par rapport a un detecteur de reference (phosphore) dans un convertisseur en uranium naturel; les detecteurs de neutrons intermediaires, par rapport a l'or dans le canal axial de ZOE, Cette methode permet de minimiser les erreurs dues aux sections efficaces d'activation. On decrit sommairement la salle de comptage du Service d'Etudes de Protections de Piles et on indique les caracteristiques d'emploi pratique des detecteurs utilises. (auteurs)

  12. Measurement of the absolute values of cross-sections in neutron photoproduction (1962); Mesure de sections efficaces de photoproduction de neutrons en valeur absolue (1962)

    Energy Technology Data Exchange (ETDEWEB)

    Schuhl, C. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1962-07-01

    The absolute values of photoneutrons production cross-sections for the case of intermediate and heavy nuclei (lanthanium, cerium, tantalum, gold, lead and bismuth) are determined with an error of 15 per cent. The results obtained agree with theories in which the giant resonance is explained by the collective motion of the protons against the neutrons. The effect of the nuclear deformation on the shape of the giant resonance is seen in the case of Ta{sup 181}, it will be possible to determine the quadrupole momenta of deformed nuclei with a good accuracy when we shall increase the statistics of measurements. (author) [French] Les sections efficaces de production de photoneutrons par divers noyaux moyens et lourds (lanthane, cerium, tantale, or, plomb et bismuth) sont determinees en valeur absolue avec une erreur relative de 15 pour cent. Les resultats obtenus s'accordent avec les theories qui interpretent la resonance geante par un mouvement collectif des protons par rapport aux neutrons. L'influence de la deformation du noyau sur la forme de la resonance geante est soulignee dans le cas de {sup 181}Ta pour lequel elle se decompose en deux pics. Une amelioration de la statistique des mesures permettra de determiner les moments quadrupolaires des noyaux deformes avec une meilleure precision. (auteur)

  13. UTILISATION DES DONNEES SATELLITAIRES POUR L’ESTIMATION DU COEFFICIENT DE REFLECTANCE BIDIRECTIONNELLE REEL A L’AIDE DE MESURES SATELLITAIRES.

    Directory of Open Access Journals (Sweden)

    S TOURTA

    2015-06-01

    Full Text Available La télédétection est l’ensemble des connaissances et techniques utilisées pour déterminer les caractéristiques physiques d’objets par des mesures effectuées à distance, sans contact matériel avec ceux-ci. La télédétection  englobe tout le processus qui consiste à capter et à enregistrer l’énergie d’un rayonnement électromagnétique émis ou réfléchi, à traiter et à analyser l’information, pour ensuite mettre en application cette information. Le rayonnement solaire est atténué par les différents constituants atmosphériques tels que les molécules, les aérosols, les gaz, les gouttelettes nuageuses ou les cristaux de glace. Le but de ce travail est l’estimation du coefficient de réflectance bidirectionnelle sur le site de TAMANRASSET, en utilisant le modèle analytique à bande large, pour les trois heurs de prise  d’images à pleine résolution, 9h00, 12h00, 15h00 temps universel, et pour des jours de ciel clair à année 1999.

  14. Apport d'une approche géostatique dans l'interprétation des mesures de diagraphies différées Enhancing Well Log Interpretation by Using a Geostatistical Approach

    Directory of Open Access Journals (Sweden)

    Denis A.

    2006-12-01

    Full Text Available Nous proposons d'étudier et d'interpréter les données diagraphiques issues de macro-dispositifs en tenant compte, pour chaque mesure, du volume investi. Les macrodispositifs, en raison de leur géométrie, ont un effet intégrateur important sur la mesure diagraphique. Ceci se traduit pour ces dispositifs par une définition ou résolution verticale médiocre. De plus, dans la plupart des cas, le pas d'échantillonnage de la mesure le long du forage est inférieur à la résolution verticale de l'outil : les volumes investis se chevauchent, d'où des données qui ne sont plus additives. Une approche géostatistique des données diagraphiques nous permet d'étudier l'influence de l'effet intégrateur de l'outil sur la valeur de la mesure et de proposer trois méthodes de régularisation des données. Leur objectif est de rendre les données additives par une transformation des supports de mesure (volumes investis. Nous montrerons ainsi par une étude sur des signaux réels et synthétiques puis par l'intermédiaire d'une interprétation combinée de plusieurs diagraphies, qu'une simple régularisation des supports de mesure permet d'une part d'obtenir une information plus rigoureuse avec la mesure diagraphique, et d'autre part d'accroître les possibilités des macrodispositifs et tout particulièrement leur résolution verticale. We propose to study macro logging techniques data by taking into account for each measure the volume affected by the physical process. The volume of sediment affected by a measure carried out with a logging tool (sonic logs, density logs, etc. depends on the nature of the surrounding formations and on the setting of the instrument. The various parameters which influence the measurement are: the source-detector spacing, the spacing between detectors, the sampling interval along a well, and the volume of material considered (the measured entity. Depending on the tool, the measured entity can be either cylindrical

  15. Nouvelles: KEK: B pour BELLE; NA48 mesure la violation directe de CP; LEL: le laser à électrons libres dépasse le kilowatt; Le LEP à 100 pour 100; Tour d'honneur au RHIC; Mesures de précision; Etude sur les modes de gestion du village planétaire; Conférence PANIC99 à Uppsala; Rencontre électron-noyau à HERA; LPP, Doubna célèbre une décennie; Les physiciens auscultent le photon; Aimants chauds venus du froid

    CERN Multimedia

    1999-01-01

    Nouvelles: KEK: B pour BELLE; NA48 mesure la violation directe de CP; LEL: le laser à électrons libres dépasse le kilowatt; Le LEP à 100 pour 100; Tour d'honneur au RHIC; Mesures de précision; Etude sur les modes de gestion du village planétaire; Conférence PANIC99 à Uppsala; Rencontre électron-noyau à HERA; LPP, Doubna célèbre une décennie; Les physiciens auscultent le photon; Aimants chauds venus du froid

  16. Prevalence of sealants in relation to dental caries on the permanent molars of 12 and 15-year-old Greek adolescents. A national pathfinder survey

    Directory of Open Access Journals (Sweden)

    Mamai-Homata Eleni

    2011-02-01

    Full Text Available Abstract Background The use of sealants as an effective measure for the prevention of pit and fissure caries in children has been well documented by several studies; either they are used on an individual or on a public health basis. In order to plan and establish a national preventive program with sealants in a community, it is mandatory to know the epidemiological pattern of caries along with other variables influencing their use and effectiveness. Aims: To assess the utilization and distribution pattern of pit and fissure sealants on the first and second permanent molars of Greek adolescents and to evaluate whether the existing usage of sealants and some socio-demographic factors are correlated to caries prevalence on the population examined Methods A stratified cluster sample of 2481 Greek adolescents was selected according to WHO guidelines (1224 twelve and 1,257 fifteen-year-old, living in urban and rural areas in 11 districts within the country. Five calibrated examiners carried out clinical examinations, recording caries experience at the dentine threshold (BASCD criteria and presence or absence of sealants along with Socio-demographic indicators associated with oral health. Mann Whitney and Pearson's chi-square non parametric tests were utilized for assessing the data. The level of significance was p Results Sealants utilization varied considerably within the different districts, with 8,3% of the 12 and 8,0% of the 15-year-old adolescents having at least one sealed molar. Sealants reduced DMFS scores by 11% in the 12-year-olds and by 24% in the 15-year-olds, while 15-year-old adolescents from rural areas had a statistically significant (p = 0.002 less chance of having sealants (71% compared to children from urban areas. Girls had higher chance to receive sealants in both age groups (26% for the 12 and 19% for the 15-year-old as well as patients that visited the dentist for prevention compared to those visiting the dentist because they thought they needed a restoration or because they were in pain. Conclusions The finding that sealants reduced DMFS scores despite their very low utilization, along with the high prevalence of dental caries found on the occlusal surfaces of the posterior teeth of Greek adolescents, is calling for a national preventive program with sealants which could eliminate caries to a larger extent.

  17. JAVA PathFinder

    Science.gov (United States)

    Mehhtz, Peter

    2005-01-01

    JPF is an explicit state software model checker for Java bytecode. Today, JPF is a swiss army knife for all sort of runtime based verification purposes. This basically means JPF is a Java virtual machine that executes your program not just once (like a normal VM), but theoretically in all possible ways, checking for property violations like deadlocks or unhandled exceptions along all potential execution paths. If it finds an error, JPF reports the whole execution that leads to it. Unlike a normal debugger, JPF keeps track of every step how it got to the defect.

  18. The Millimeter Astronomy Legacy Team 90 GHz Survey (MALT90) and ALMA

    CERN Document Server

    Foster, Jonathan B; Jackson, James M; Longmore, Steve N; Whitaker, Scott; Hoq, Sadia

    2013-01-01

    ALMA will revolutionize our understanding of star formation within our galaxy, but before we can use ALMA we need to know where to look. The Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey is a large international project to map the molecular line emission of over 2,000 dense clumps in the Galactic plane. MALT90 serves as a pathfinder for ALMA, providing a large public database of dense molecular clumps associated with high-mass star formation. In this proceedings, we describe the survey parameters and share early science highlights from the survey, including (1) a comparison between galactic and extragalactic star formation relations, (2) chemical trends in MALT90 clumps, (3) the distribution of high-mass star formation in the Milky Way, and (4) a discussion of the Brick, the target of successful ALMA Cycle 0 and Cycle 1 proposals.

  19. The Millimeter Astronomy Legacy Team 90 GHz Survey (MALT90) and ALMA

    Science.gov (United States)

    Foster, J.; Rathborne, J.; Jackson, J.; Longmore, S.; Whitaker, S.; Hoq, S.

    2013-10-01

    ALMA will revolutionize our understanding of star formation within our galaxy, but before we can use ALMA we need to know where to look. The Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey is a large international project to map the molecular line emission of over 2,000 dense clumps in the Galactic plane. MALT90 serves as a pathfinder mission for ALMA, providing a large public database of dense molecular clumps associated with high-mass star formation. In this proceedings, we describe the survey parameters and share early science highlights from the survey, including (1) a comparison between galactic and extragalactic star formation relations, (2) chemical trends in MALT90 clumps, (3) the distribution of high-mass star formation in the Milky Way, and (4) a discussion of the “Brick”, the target of successful ALMA Cycle 0 and Cycle 1 proposals.

  20. "Suntelligence" Survey

    Science.gov (United States)

    ... to the American Academy of Dermatology's "Suntelligence" sun-smart survey. Please answer the following questions to measure ... be able to view a ranking of major cities suntelligence based on residents' responses to this survey. ...

  1. Survey Says

    Science.gov (United States)

    McCarthy, Susan K.

    2005-01-01

    Survey Says is a lesson plan designed to teach college students how to access Internet resources for valid data related to the sexual health of young people. Discussion questions based on the most recent available data from two national surveys, the Youth Risk Behavior Surveillance-United States, 2003 (CDC, 2004) and the National Survey of…

  2. Automated detection of extended sources in radio maps: progress from the SCORPIO survey

    Science.gov (United States)

    Riggi, S.; Ingallinera, A.; Leto, P.; Cavallaro, F.; Bufano, F.; Schillirò, F.; Trigilio, C.; Umana, G.; Buemi, C. S.; Norris, R. P.

    2016-08-01

    Automated source extraction and parametrization represents a crucial challenge for the next-generation radio interferometer surveys, such as those performed with the Square Kilometre Array (SKA) and its precursors. In this paper, we present a new algorithm, called CAESAR (Compact And Extended Source Automated Recognition), to detect and parametrize extended sources in radio interferometric maps. It is based on a pre-filtering stage, allowing image denoising, compact source suppression and enhancement of diffuse emission, followed by an adaptive superpixel clustering stage for final source segmentation. A parametrization stage provides source flux information and a wide range of morphology estimators for post-processing analysis. We developed CAESAR in a modular software library, also including different methods for local background estimation and image filtering, along with alternative algorithms for both compact and diffuse source extraction. The method was applied to real radio continuum data collected at the Australian Telescope Compact Array (ATCA) within the SCORPIO project, a pathfinder of the Evolutionary Map of the Universe (EMU) survey at the Australian Square Kilometre Array Pathfinder (ASKAP). The source reconstruction capabilities were studied over different test fields in the presence of compact sources, imaging artefacts and diffuse emission from the Galactic plane and compared with existing algorithms. When compared to a human-driven analysis, the designed algorithm was found capable of detecting known target sources and regions of diffuse emission, outperforming alternative approaches over the considered fields.

  3. Mesures experimentales de l'impact des revetements hydrophobeset superhydrophobes sur la trainee et la portance d'un profil aerodynamique propre et glace

    Science.gov (United States)

    Villeneuve, Eric

    Ce projet, realise a la demande du Laboratoire International des Materiaux Antigivre, a pour but de mesurer et definir experimentalement l'impact de revetements hydrophobes sur les coefficients de trainee et de portance d'un profil NACA 0012. Pour ce faire, la balance aerodynamique du LIMA devait tout d'abord etre amelioree afin d'offrir une sensibilite suffisante pour realiser le projet. Plusieurs ameliorations ont ete faites, comme le changement des cellules de charge, la diminution du nombre de cellules de charge, le changement du cadre de la balance, etc. Une fois ces ameliorations terminees, la reproductibilite, l'exactitude et la sensibilite ont ete valides afin de s'assurer de la fiabilite des resultats offerts par la balance. Pour les angles d'attaque etudies avec les revetements, soient -6° et 0°, la balance a une reproductibilite de +/-2,06% a 360 000 de nombre de Reynolds. Pour valider la sensibilite, des essais a -6° et 0° d'angle d'attaque et des nombres de Reynolds de 360 000 et 500 000 ont ete faits avec des papiers sables. Les resultats de ces essais ont permis de, tracer des courbes de tendances du coefficient de trainee du NACA 0012 en fonction de la rugosite de surface et d'etablir la valeur de la sensibilite de la balance a +/-8 mu m. Cinq revetements populaires ont ete choisis pour l'experimentation, soient le Wearlon, le Staclean, le Hirec, le Phasebreak ainsi que le Nusil. Les revetements sont soumis aux memes conditions experimentales que les papiers sables, et une rugosite equivalente est trouvee par extrapolation des resultats. Cependant, les rugosites equivalentes de surfaces different entre -6° et 0°. Les essais avec le Staclean et le Hirec donnent des coefficients de trainee equivalent a ceux avec l'aluminium, alors que le Wearlon, le Nusil et le Phasebreak donnent une augmentation du coefficient de trainee de 13%, 17% et 25% respectivement par rapport a l'aluminium. Pour les coefficients de portance, la balance ne detecte pas l

  4. Développement d'outils de mesure pour l'amélioration du procédé d'impression offset

    Science.gov (United States)

    Boumaïza, K.; Baudin, G.; Catusse, R.; Viallet, A.

    1999-03-01

    The offset printing process rests primarily on the balance between ink and damping solution. However, this balance remains difficult to realize. The corresponding wastes of time and into consumable (ink, paper and damping solution) are harmful for the industrialist, the consumer and the environment. The main feature of this work is to control and thus to optimize these flux. With this intention, two optical sensors functioning in reflection were developed. A laser with receiving photodiode for the control of damping solution film thickness, and an optical fiber related to a photoelectric sensor for control of ink film thickness. The current study aims at the calibration of these two sensors for respectively the control of water and ink flux in the offset press. Le procédé d'impression offset repose essentiellement sur l'équilibre entre la solution de mouillage et l'encre. Toutefois, cet équilibre reste une tâche difficile à réaliser. Les pertes en temps et en consommables (encre, papier, solution de mouillage) correspondantes sont nuisibles à la fois pour l'industriel, le consommateur et l'environnement. L'objectif de ce travail est de contrôler et donc d'optimiser ces flux pour un tirage donné. Pour ce faire, deux capteurs de type optique fonctionnant en réflexion ont été développés. Un laser avec photodiode réceptrice pour le contrôle du film de solution de mouillage, et une fibre optique liée à un capteur photoélectrique pour le contrôle du film d'encre. L'étude actuelle vise la mise en ouvre et l'étalonnage de ces deux capteurs pour la mesure et le contrôle des films respectifs d'eau et d'encre dans la presse offset.

  5. Investigation on the monthly variation of cirrus optical properties over the Indian subcontinent using cloud-aerosol lidar and infrared pathfinder satellite observation (Calipso)

    Science.gov (United States)

    Dhaman, Reji K.; Satyanarayana, Malladi; Jayeshlal, G. S.; Mahadevan Pillai, V. P.; Krishnakumar, V.

    2016-05-01

    Cirrus clouds have been identified as one of the atmospheric component which influence the radiative processes in the atmosphere and plays a key role in the Earth Radiation Budget. CALIPSO (Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation) is a joint NASA-CNES satellite mission designed to provide insight in understanding of the role of aerosols and clouds in the climate system. This paper reports the study on the variation of cirrus cloud optical properties of over the Indian sub - continent for a period of two years from January 2009 to December 2010, using cloud-aerosol lidar and infrared pathfinder satellite observations (Calipso). Indian Ocean and Indian continent is one of the regions where cirrus occurrence is maximum particularly during the monsoon periods. It is found that during the south-west monsoon periods there is a large cirrus cloud distribution over the southern Indian land masses. Also it is observed that the north-east monsoon periods had optical thick clouds hugging the coast line. The summer had large cloud formation in the Arabian Sea. It is also found that the land masses near to the sea had large cirrus presence. These cirrus clouds were of high altitude and optical depth. The dependence of cirrus cloud properties on cirrus cloud mid-cloud temperature and geometrical thickness are generally similar to the results derived from the ground-based lidar. However, the difference in macrophysical parameter variability shows the limits of space-borne-lidar and dissimilarities in regional climate variability and the nature and source of cloud nuclei in different geographical regions.

  6. Calcul numérique accéléré de mesures de performance sur les modèles Markoviens appliqués aux systèmes informatiques et de télécommunications

    Science.gov (United States)

    Ghaddar, A.; Sinno, N.

    2005-05-01

    La complexité du phénomène de files d'attente dans les systèmes informatiques et télécommunications nécessite leur simulation par des modèles Markoviens pour les mesures de performance, mesure des délais d'attente au niveau des routeurs pour le modèle informatique et l'étude de la gestion des appels téléphoniques pour le modèle des circuits téléphoniques. L'optimisation des méthodes numériques de résolution des équations relatives à ces deux modèles va permettre d' ídentifier les critères de convergence rapide vers les états stationnaires correspondant à ces mesures.

  7. An Improved Airborne Wind Measurement Technique for the NAE (National Aeronautical Establishment) Twin Otter (Nouvelle Methode De Mesure Du Vent En Vol a Bord Du Twin Otter De L’ena)

    Science.gov (United States)

    1989-11-01

    filtre de Kalman , laquelle rdsout ce probl~me et permet de mesurer le vent avec une exactitude sup6rieure A celle des anciennes m6thodes. D’apr6s les...premiers r6sultats bases sur ’application d’un filtre de Kalman aux donn6es des essaip en vol du Twin Otter, il semble qu’il soit possible d’obtenir...actually degrading wind computation accuracy compared with older techniques. A new wind measurement technique, based on a Kalman filter integrated

  8. NOAA Daily 25km Global Optimally Interpolated Sea Surface Temperature (OISST) in situ and AVHRR analysis supplemented with AVHRR Pathfinder Version 5.0 climatological SST for inland and coastal pixels, 1981-09-01 through 2010-12-31 (NODC Accession 0071180)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This accession contains the daily 25km global Optimally Interpolated Sea Surface Temperature (OISST) in situ and AVHRR analysis, supplemented with AVHRR Pathfinder...

  9. The Detection of an Extremely Bright Fast Radio Burst in a Phased Array Feed Survey

    Science.gov (United States)

    Bannister, K. W.; Shannon, R. M.; Macquart, J.-P.; Flynn, C.; Edwards, P. G.; O'Neill, M.; Osłowski, S.; Bailes, M.; Zackay, B.; Clarke, N.; D'Addario, L. R.; Dodson, R.; Hall, P. J.; Jameson, A.; Jones, D.; Navarro, R.; Trinh, J. T.; Allison, J.; Anderson, C. S.; Bell, M.; Chippendale, A. P.; Collier, J. D.; Heald, G.; Heywood, I.; Hotan, A. W.; Lee-Waddell, K.; Madrid, J. P.; Marvil, J.; McConnell, D.; Popping, A.; Voronkov, M. A.; Whiting, M. T.; Allen, G. R.; Bock, D. C.-J.; Brodrick, D. P.; Cooray, F.; DeBoer, D. R.; Diamond, P. J.; Ekers, R.; Gough, R. G.; Hampson, G. A.; Harvey-Smith, L.; Hay, S. G.; Hayman, D. B.; Jackson, C. A.; Johnston, S.; Koribalski, B. S.; McClure-Griffiths, N. M.; Mirtschin, P.; Ng, A.; Norris, R. P.; Pearce, S. E.; Phillips, C. J.; Roxby, D. N.; Troup, E. R.; Westmeier, T.

    2017-05-01

    We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducted in a wide-field fly’s-eye configuration using the phased-array-feed technology deployed on the array to instantaneously observe an effective area of 160 deg2, and achieve an exposure totaling 13200 deg2 hr . We constrain the position of FRB 170107 to a region 8\\prime × 8\\prime in size (90% containment) and its fluence to be 58 ± 6 Jy ms. The spectrum of the burst shows a sharp cutoff above 1400 MHz, which could be due to either scintillation or an intrinsic feature of the burst. This confirms the existence of an ultra-bright (> 20 Jy ms) population of FRBs.

  10. Engineering surveying

    CERN Document Server

    Schofield, W

    2001-01-01

    The aim of Engineering Surveying has always been to impart and develop a clear understanding of the basic topics of the subject. The author has fully revised the book to make it the most up-to-date and relevant textbook available on the subject.The book also contains the latest information on trigonometric levelling, total stations and one-person measuring systems. A new chapter on satellites ensures a firm grasp of this vitally important topic.The text covers engineering surveying modules for civil engineering students on degree courses and forms a reference for the engineering surveying module in land surveying courses. It will also prove to be a valuable reference for practitioners.* Simple clear introduction to surveying for engineers* Explains key techniques and methods* Details reading systems and satellite position fixing

  11. New instruments and methods for measuring the concentration of radioactive products in the atmosphere; Appareils recents et methodes nouvelles pour la mesure de la concentration des produits radioactifs dans l'atmosphere

    Energy Technology Data Exchange (ETDEWEB)

    Jehanno, C.; Blanc, A.; Lallemant, C.; Roux, G. [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires

    1959-07-01

    . (author) [French] Differents enregistreurs pour aerosols radioactifs ont ete realises pour mesurer la pollution de l'atmosphere des laboratoires ou l'atmosphere exterieure. EAR 600. - Permet de mesurer en continu instantanement et 3 a 10 heures apres le prelevement des concentrations d'aerosols emetteurs {alpha} ou {beta} allant de quelques 10{sup -11} a quelques 10{sup -8} curies par metre cube d'air. EAR 800. - Permet de mesurer en continu des concentrations d'aerosols emetteurs {alpha} allant de 10{sup -11} a 10{sup -5} curie par metre cube d'air, et des concentrations d'aerosols emetteurs {beta} allant de 10{sup -11} a 10{sup -1} curie par metre cube d'air. EAR PLUTONIUM. - Permet de detecter en quelques minutes 1000 DMP (2.10{sup -9} curie par metre cube) et en 8 heures 1 DMP (2.10{sup -12} curie par metre cube). Deux methodes sont utilisees pour separer l'activite due au plutonium de celle due aux derives du radon et du thoron: a) par discrimination d'amplitude, b) par les coincidences (a,b) RaC' et ThC-ThC'. SP 4. - Monte sur jeep, cet ensemble permet la mesure de l'irradiation produite au sol par le panache des piles. La sensibilite est de 5{mu}R/h. A.D.I.R. - Cet appareil autonome et portatif est destine a la mesure instantanee des teneurs en radon de l'atmosphere des mines. Il permet de mesurer des teneurs de l'air variant entre 0,4 et 400.10{sup -10} curie par litre d'air (0,4 et 400 DPM). La mesure des retombees radioactives est faite apres collection de cette activite par un pluviometre special comportant une surface adhesive et une cartouche de resines echangeuses d'ions. La radioactivite des retombees varie entre quelques 10{sup -9} et quelques 10{sup -7} curie par metre carre et par mois. La mesure des concentrations de l'atmosphere en produits de fission est faite apres collection sur papier filtre. Les concentrations mesurees dans l'air au niveau du sol varient

  12. Appareillage automatisé de mesure simultanée du pouvoir thermoélectrique et de la conductivité électrique. Application à l'étude de couches polymères semi-conductrices

    Science.gov (United States)

    Moliton, A.; Ratier, B.; Moreau, C.; Froyer, G.

    1991-05-01

    In this paper, we present an automatized system for simultaneous measurement of conductivity σ, and thermoelectric power S : measurements are allowed for temperatures ranging from 130 K to 360 K on brittle semiconductor layers. As an example of the application, results obtained in the case of polymer (PPP) layers implanted with Na ions are presented : with high energy implantation (E = 250 keV) we observe only a defect semiconduction of p type while at low energy (30 keV) an electronic n type conduction appears. Nous présentons dans cet article un système de mesure simultanée de la conductivité σ, et du pouvoir thermoélectrique S : il permet des mesures en fonction de la température (entre 130 K et 360 K) dans le cas de couches semi-conductrices relativement fragiles. A titre d'application, nous indiquons les résultats que nous avons obtenus dans le cas de couches polymères (PPP) implantées avec des ions sodium: alors que seule une semi-conduction par défaut est générée par de fortes énergies d'implantation (E = 250 keV ), il apparaît une semiconduction induite par le dopage n lors d'implantations à basse énergie (E = 30 keV ).

  13. Développement humain, développement durable et « pays en développement » : comment articuler et mesurer les différentes dimensions ?

    Directory of Open Access Journals (Sweden)

    Bruno Boidin

    2004-02-01

    Full Text Available Cet article cherche à préciser la place qu’occupent les différentes dimensions du développement durable au sein de l’analyse économique du développement, et en particulier les dimensions humaine et sociale. Ceci nous amène à considérer les relations complexes entre les différents actifs (santé, éducation, capital social…, marquées par des effets d’irréversibilité qui peuvent remettre en cause la durabilité. Se pose alors la question de la mesure du développement durable prenant en compte ces articulations entre les dimensions. Une grille d’évaluation des mesures synthétiques du développement durable est proposée et appliquée à une sélection d’indicateurs.This article seeks to specify the place of various dimensions of sustainable development within development economics, in particular human and social dimensions. This leads us to consider the complex relations between the various assets (health, education, social capital…, characterized by irreversibility effects which can jeopardize sustainability. It is therefore necessary to find a measure of sustainable development, taking into account these interactions between dimensions. We propose criteria to evaluate synthetic measurements of sustainable development, and apply them to selected indicators.

  14. Characterization of Rock Wettability Though Dielectric Measurements Caractérisation de la mouillabilité des roches au moyen de mesures diélectriques

    Directory of Open Access Journals (Sweden)

    Bona N.

    2006-12-01

    Full Text Available The wettability of glass filters and Berea sandstone was investigated using the electric response in the interval 10² - 10 (to the power of 8 Hz. The natural wettability of the materials was modified to get two different sets of samples, one with strong water and the other with strong oil wettability. The samples were saturated to various degrees up to 40% with deionized water or brine. Measurements showed that the electric responses of water-wet and oil-wet samples were markedly different and more complex than those predicted by two standard models. The dispersivity and the loss tangent were found to be the most suitable parameters to check the wettability of the samples. La mouillabilité de filtres de verre et de grès de Béréa a été caractérisée par leur réponse électrique dans l'intervalle 10² - 10 puissance 8 Hz. Au moyen de traitements appropriés, la mouillabilité naturelle des matériaux a été modifiée afin d'obtenir deux séries différentes d'échantillons ayant respectivement de fortes mouillabilités à l'eau et à l'huile. Les échantillons ont été saturés à des degrés variés (pas plus de 40 % avec de l'eau permutée ou de la saumure. Les mesures ont montré que les réponses électriques des échantillons mouillables à l'eau ou mouillables à l'huile étaient nettement différentes et plus compliquées que celles prédites par deux modèles standard. En outre, on a pu constater que la dispersivité et la tangente de pertes constituent les paramètres les plus pertinents pour caractériser la mouillabilité des échantillons.

  15. Quels indicateurs pour mesurer le développement professionnel dans les métiers adressés à autrui ?

    Directory of Open Access Journals (Sweden)

    Thierry Piot

    2011-06-01

    Full Text Available Cet article propose des indicateurs destinés à mesurer le développement professionnel dans les métiers adressés à autrui. La première partie s’intéresse à la genèse de la notion de développement professionnel, issue de la rationalisation induite par la seconde modernité ; elle indique que les métiers adressés à autrui sont tenus d’articuler une rationalisation forte et une rationalisation faible. Puis, nous présentons le cadre de la didactique professionnelle, particulièrement pertinent pour s’intéresser à l’analyse du travail d’interaction humaine et mettre au jour ses dilemmes. À partir d’une recherche empirique concernant des formateurs d’une école d’aides-soignants, nous proposons, à partir d’une lecture plurielle qui prend en compte les compétences et l’identité professionnelle, cinq indicateurs qui sont l’objet d’un traitement afin d’être comparables, car c’est la cohérence entre les informations recueillies qui nous paraît rendre le mieux compte, malgré les limites, de la notion de développement professionnel dans les métiers adressés à autrui.What indicators should be used to measure professional development in non-teaching support occupations? This article proposes the use of indicators in these occupations. The first part considers the origin of the concept of professional development, coming from the rationalisation caused by the “second modernity”. This part indicates that these occupations are linked to both a strong and a weak rationalisation. The second part presents the framework for professional development that is particularly relevant to the analysis of social interaction and the updating its dilemmas. Starting from empirical research involving the trainers at a school for care assistants, five indicators are proposed for the competencies and professional identity that are sufficiently comparable for the best generalisations, despite all limitations, to support

  16. Élaboration, fiabilité et utilisation d’un outil de mesure de l’environnement alimentaire dans les supermarchés de quatre quartiers de Montréal (Canada

    Directory of Open Access Journals (Sweden)

    Élise Jalbert-Arsenault

    2017-01-01

    Full Text Available Introduction : L’environnement alimentaire constitue un domaine propice si l'on veut influencer les habitudes alimentaires de la population. Cette étude visait à élaborer un outil de mesure de l’environnement alimentaire dans les commerces et à caractériser l’environnement alimentaire dans un secteur de Montréal (Canada possédant un niveau de revenu de faible à moyen. Méthodologie : Nous avons développé un outil, la Mesure de l’environnement alimentaire du consommateur dans les supermarchés (MEAC-S et nous l’avons mis à l’essai pour en confirmer la fiabilité. Nous avons utilisé la MEAC-S pour évaluer l’environnement alimentaire de consommation de 17 supermarchés dans quatre quartiers de Montréal. Nous avons mesuré la longueur d’étalage, la diversité, le prix, le nombre de présentoirs et la position en magasin des fruits et légumes (FL et des produits alimentaires ultra-transformés (PAUT. Nous avons également évalué la qualité des FL frais. La taille du magasin a été estimée en utilisant la longueur totale d’étalage mesurée pour toutes les catégories d’aliments. Nous avons effectué des corrélations de Spearman entre ces indicateurs de l’environnement alimentaire. Résultats : Les analyses de fiabilité ont donné des résultats satisfaisants pour la plupart des indicateurs. La caractérisation de l’environnement alimentaire a révélé une grande variabilité de la longueur d’étalage, de la diversité et du prix des FL entre les supermarchés ainsi qu’une mise en valeur disproportionnée des PAUT. Le nombre de présentoirs de PAUT hors de leur emplacement principal de vente variait de 7 à 26 et ces produits occupaient de 8 à 33 positions stratégiques en magasin, alors que le nombre de présentoirs hors de l’emplacement principal de vente de FL frais était supérieur à 1 dans seulement 2 des 17 magasins évalués et qu’ils occupaient un maximum de 2 emplacements strat

  17. Synchrotron Emission from Dark Matter Annihilation: Predictions for Constraints from Non-detections of Galaxy Clusters with New Radio Surveys

    CERN Document Server

    Storm, Emma; Splettstoesser, Megan; Profumo, Stefano

    2016-01-01

    The annihilation of dark matter particles is expected to yield a broad radiation spectrum via the production of Standard Model particles in astrophysical environments. In particular, electrons and positrons from dark matter annihilation produce synchrotron radiation in the presence of magnetic fields. Galaxy clusters are the most massive collapsed structures in the universe, and are known to host microGauss-scale magnetic fields. They are therefore ideal targets to search for, or to constrain the synchrotron signal from dark matter annihilation. In this work we use the expected sensitivities of several planned surveys from the next generation of radio telescopes to predict the constraints on dark matter annihilation models which will be achieved in the case of non-detections of diffuse radio emission from galaxy clusters. Specifically, we consider the Tier 1 and 2 surveys planned for the Low Frequency Array (LOFAR) at 120 MHz, the EMU survey planned for the Australian Square Kilometre Array Pathfinder (ASKAP)...

  18. THE TIME DOMAIN SPECTROSCOPIC SURVEY: VARIABLE SELECTION AND ANTICIPATED RESULTS

    Energy Technology Data Exchange (ETDEWEB)

    Morganson, Eric; Green, Paul J. [Harvard Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138 (United States); Anderson, Scott F.; Ruan, John J. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Myers, Adam D. [Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071 (United States); Eracleous, Michael; Brandt, William Nielsen [Department of Astronomy and Astrophysics, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA 16802 (United States); Kelly, Brandon [Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93106-9530 (United States); Badenes, Carlos [Department of Physics and Astronomy and Pittsburgh Particle Physics, Astrophysics and Cosmology Center (PITT PACC), University of Pittsburgh, 3941 O’Hara St, Pittsburgh, PA 15260 (United States); Bañados, Eduardo [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); Blanton, Michael R. [Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003 (United States); Bershady, Matthew A. [Department of Astronomy, University of Wisconsin, 475 N. Charter St., Madison, WI 53706 (United States); Borissova, Jura [Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, Playa Ancha, Casilla 5030, and Millennium Institute of Astrophysics (MAS), Santiago (Chile); Burgett, William S. [GMTO Corp, Suite 300, 251 S. Lake Ave, Pasadena, CA 91101 (United States); Chambers, Kenneth, E-mail: emorganson@cfa.harvard.edu [Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822 (United States); and others

    2015-06-20

    We present the selection algorithm and anticipated results for the Time Domain Spectroscopic Survey (TDSS). TDSS is an Sloan Digital Sky Survey (SDSS)-IV Extended Baryon Oscillation Spectroscopic Survey (eBOSS) subproject that will provide initial identification spectra of approximately 220,000 luminosity-variable objects (variable stars and active galactic nuclei across 7500 deg{sup 2} selected from a combination of SDSS and multi-epoch Pan-STARRS1 photometry. TDSS will be the largest spectroscopic survey to explicitly target variable objects, avoiding pre-selection on the basis of colors or detailed modeling of specific variability characteristics. Kernel Density Estimate analysis of our target population performed on SDSS Stripe 82 data suggests our target sample will be 95% pure (meaning 95% of objects we select have genuine luminosity variability of a few magnitudes or more). Our final spectroscopic sample will contain roughly 135,000 quasars and 85,000 stellar variables, approximately 4000 of which will be RR Lyrae stars which may be used as outer Milky Way probes. The variability-selected quasar population has a smoother redshift distribution than a color-selected sample, and variability measurements similar to those we develop here may be used to make more uniform quasar samples in large surveys. The stellar variable targets are distributed fairly uniformly across color space, indicating that TDSS will obtain spectra for a wide variety of stellar variables including pulsating variables, stars with significant chromospheric activity, cataclysmic variables, and eclipsing binaries. TDSS will serve as a pathfinder mission to identify and characterize the multitude of variable objects that will be detected photometrically in even larger variability surveys such as Large Synoptic Survey Telescope.

  19. The Time Domain Spectroscopic Survey: Variable Selection and Anticipated Results

    Science.gov (United States)

    Morganson, Eric; Green, Paul J.; Anderson, Scott F.; Ruan, John J.; Myers, Adam D.; Eracleous, Michael; Kelly, Brandon; Badenes, Carlos; Bañados, Eduardo; Blanton, Michael R.; Bershady, Matthew A.; Borissova, Jura; Brandt, William Nielsen; Burgett, William S.; Chambers, Kenneth; Draper, Peter W.; Davenport, James R. A.; Flewelling, Heather; Garnavich, Peter; Hawley, Suzanne L.; Hodapp, Klaus W.; Isler, Jedidah C.; Kaiser, Nick; Kinemuchi, Karen; Kudritzki, Rolf P.; Metcalfe, Nigel; Morgan, Jeffrey S.; Pâris, Isabelle; Parvizi, Mahmoud; Poleski, Radosław; Price, Paul A.; Salvato, Mara; Shanks, Tom; Schlafly, Eddie F.; Schneider, Donald P.; Shen, Yue; Stassun, Keivan; Tonry, John T.; Walter, Fabian; Waters, Chris Z.

    2015-06-01

    We present the selection algorithm and anticipated results for the Time Domain Spectroscopic Survey (TDSS). TDSS is an Sloan Digital Sky Survey (SDSS)-IV Extended Baryon Oscillation Spectroscopic Survey (eBOSS) subproject that will provide initial identification spectra of approximately 220,000 luminosity-variable objects (variable stars and active galactic nuclei across 7500 deg2 selected from a combination of SDSS and multi-epoch Pan-STARRS1 photometry. TDSS will be the largest spectroscopic survey to explicitly target variable objects, avoiding pre-selection on the basis of colors or detailed modeling of specific variability characteristics. Kernel Density Estimate analysis of our target population performed on SDSS Stripe 82 data suggests our target sample will be 95% pure (meaning 95% of objects we select have genuine luminosity variability of a few magnitudes or more). Our final spectroscopic sample will contain roughly 135,000 quasars and 85,000 stellar variables, approximately 4000 of which will be RR Lyrae stars which may be used as outer Milky Way probes. The variability-selected quasar population has a smoother redshift distribution than a color-selected sample, and variability measurements similar to those we develop here may be used to make more uniform quasar samples in large surveys. The stellar variable targets are distributed fairly uniformly across color space, indicating that TDSS will obtain spectra for a wide variety of stellar variables including pulsating variables, stars with significant chromospheric activity, cataclysmic variables, and eclipsing binaries. TDSS will serve as a pathfinder mission to identify and characterize the multitude of variable objects that will be detected photometrically in even larger variability surveys such as Large Synoptic Survey Telescope.

  20. Mesurer la santé mentale positive au Canada : validation des concepts du Continuum de santé mentale – Questionnaire abrégé

    Directory of Open Access Journals (Sweden)

    Heather Orpana

    2017-01-01

    Full Text Available Introduction : La santé mentale positive est de plus en plus reconnue comme un élément central des politiques et des programmes en matière de santé publique. On a déterminé au Canada que le Continuum de santé mentale - Questionnaire abrégé (CSM-QA constituait un outil de mesure prometteur qu'il fallait intégrer aux enquêtes d'évaluation de la santé mentale positive de la population. Ce questionnaire vise à évaluer un modèle à trois facteurs de santé mentale positive : le bien-être émotionnel, le bien-être social et le bien-être psychologique. Cette étude a pour but de déterminer si le CSM-QA offre une mesure adéquate de la santé mentale positive des Canadiens adultes. Méthodologie : Nous avons réalisé une analyse factorielle confirmatoire (AFC à l'aide des données de l'Enquête sur la santé dans les collectivités canadiennes - Santé mentale de 2012 (ESCC-SM. Nous avons également effectué une validation croisée du modèle à l'aide des données de l'Enquête sur la santé dans les collectivités canadiennes - Composante annuelle (ESCC - Composante annuelle de 2011-2012. Nous avons examiné la validité reliée à un critère dans le cadre d'analyses de corrélation entre les scores des sous-échelles du CSM-QA et les concepts positifs (comme la satisfaction à l'égard de la vie et négatifs (comme la détresse psychologique associés. Résultats : Nous avons confirmé la validité du modèle à trois facteurs du bien-être émotionnel, social et psychologique dans le cadre d'une AFC de deux échantillons distincts, et ce, après avoir intégré les quatre erreurs corrélées entre les questions relatives à l'échelle du bien-être social. Nous avons observé, comme prévu, des corrélations significatives entre le bien-être émotionnel, psychologique et social et les concepts associés. Le coefficient alpha de Cronbach était de 0,82 pour les sous-échelles du bien-être émotionnel et du bien

  1. Surveying Humaness

    DEFF Research Database (Denmark)

    Markussen, Randi; Gad, Christopher

    Christopher Gad. Ph.d. Dept. of Information and Media Studies Randi Markussen. Associate Professor, Dept. of Information and Media Studies. rmark@imv.au.dk   Abstract:   Surveying humanness -politics of care improvement   For various reasons we both were subjected to a specific survey procedure...... and development of a large collection of biological and psychological symptoms and psycho-social problems. However, the surveys say nothing about how the information will be of use to the people who answer the procedure or how this scientific intervention will be put to use more specifically within the public...... carried out in a Danish county in order to improve treatment of people who have suffered from long-term illnesses. The surveys concern not only feed back on how people experience their present and past interaction with the social services and health care system; they also ask people to indicate the state...

  2. Surveying Humaness

    DEFF Research Database (Denmark)

    Markussen, Randi; Gad, Christopher

    Christopher Gad. Ph.d. Dept. of Information and Media Studies Randi Markussen. Associate Professor, Dept. of Information and Media Studies. rmark@imv.au.dk   Abstract:   Surveying humanness -politics of care improvement   For various reasons we both were subjected to a specific survey procedure...... and development of a large collection of biological and psychological symptoms and psycho-social problems. However, the surveys say nothing about how the information will be of use to the people who answer the procedure or how this scientific intervention will be put to use more specifically within the public...... be imagined as a positive end, as ‘making explicit’ (in a popular psychological perspective) is considered to be therapeutic and good in itself? We will discuss those questions from a Foucaultian and ANT perspective, where one does not accept that pre-existing subjects are exposed to survey procedures...

  3. Survey Data

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Cleaned and QCd data for the Fishing Effort Survey. Questions on fishing and other out are asked on weather and outdoor activity, including fishing trips. Used for...

  4. A Study to Compare the Failure Rates of Current Space Shuttle Ground Support Equipment with the New Pathfinder Equipment and Investigate the Effect that the Proposed GSE Infrastructure Upgrade Might Have to Reduce GSE Infrastructure Failures

    Science.gov (United States)

    Kennedy, Barbara J.

    2004-01-01

    The purposes of this study are to compare the current Space Shuttle Ground Support Equipment (GSE) infrastructure with the proposed GSE infrastructure upgrade modification. The methodology will include analyzing the first prototype installation equipment at Launch PAD B called the "Pathfinder". This study will begin by comparing the failure rate of the current components associated with the "Hardware interface module (HIM)" at the Kennedy Space Center to the failure rate of the neW Pathfinder components. Quantitative data will be gathered specifically on HIM components and the PAD B Hypergolic Fuel facility and Hypergolic Oxidizer facility areas which has the upgraded pathfinder equipment installed. The proposed upgrades include utilizing industrial controlled modules, software, and a fiber optic network. The results of this study provide evidence that there is a significant difference in the failure rates of the two studied infrastructure equipment components. There is also evidence that the support staff for each infrastructure system is not equal. A recommendation to continue with future upgrades is based on a significant reduction of failures in the new' installed ground system components.

  5. Rover imaging system for the Mars rover/sample return mission

    Science.gov (United States)

    1993-02-01

    In the past year, the conceptual design of a panoramic imager for the Mars Environmental Survey (MESUR) Pathfinder was finished. A prototype camera was built and its performace in the laboratory was tested. The performance of this camera was excellent. Based on this work, we have recently proposed a small, lightweight, rugged, and highly capable Mars Surface Imager (MSI) instrument for the MESUR Pathfinder mission. A key aspect of our approach to optimization of the MSI design is that we treat image gathering, coding, and restoration as a whole, rather than as separate and independent tasks. Our approach leads to higher image quality, especially in the representation of fine detail with good contrast and clarity, without increasing either the complexity of the camera or the amount of data transmission. We have made significant progress over the past year in both the overall MSI system design and in the detailed design of the MSI optics. We have taken a simple panoramic camera and have upgraded it substantially to become a prototype of the MSI flight instrument. The most recent version of the camera utilizes miniature wide-angle optics that image directly onto a 3-color, 2096-element CCD line array. There are several data-taking modes, providing resolution as high as 0.3 mrad/pixel. Analysis tasks that were performed or that are underway with the test data from the prototype camera include the following: construction of 3-D models of imaged scenes from stereo data, first for controlled scenes and later for field scenes; and checks on geometric fidelity, including alignment errors, mast vibration, and oscillation in the drive system. We have outlined a number of tasks planned for Fiscal Year '93 in order to prepare us for submission of a flight instrument proposal for MESUR Pathfinder.

  6. Contrôle de l'état des sertissages internes des PFW mesures effectuées sur l'ensemble des aimants du PS après la rénovation de 26 aimants et avant le redémarrage de 2006

    CERN Document Server

    Ottaviani, J

    2006-01-01

    Les sertissages (douilles), utilisés pour raccorder les méplats du circuit principal des PFW à leurs câbles d'alimentation, présentent parfois des défauts de réalisation qui entraînent une résistance électrique anormale. Pour mettre en évidence ces défauts, on mesure la résistance des 4 sertissages des nappes polaires. Les nappes sont alimentées avec un courant efficace nominal de 80A. On effectue les mesures entre le bornier de connexions des 4 câbles d'alimentation des PFW et les circuits auxiliaires correspondants (Pick-ups brasés sur les enroulements). De ces mesures (câble d'alimentation et une courte partie du circuit principal), on en déduit la valeur de la résistance du sertissage qui en assure la liaison. A la mesure des résistances des sertissages des nappes polaires supérieures s'ajoute la résistance des câbles qui assurent la liaison entre borniers. Durant le grand arrêt, 26 aimants, entièrement rénovés et équipés de nouvelles bobines et PFW, ont été remis dans l'ann...

  7. Et. réact. $e^{+} e^{-} \\to e^{+} e^{-} \\gamma$, $e^{+} e^{-} \\to e^{+} e^{-} e^{+} e^{-}$ et $e^{+} e^{-} \\to e^{+} e ^{-} \\mu^{+} \\mu^{-}$ pour la calibrat. cristaux BGO calorim. électromagn. L3,, CERN, mesure luminosité LEP

    CERN Document Server

    Rayo, F

    1989-01-01

    Et. réact. $e^{+} e^{-} \\to e^{+} e^{-} \\gamma$, $e^{+} e^{-} \\to e^{+} e^{-} e^{+} e^{-}$ et $e^{+} e^{-} \\to e^{+} e ^{-} \\mu^{+} \\mu^{-}$ pour la calibrat. cristaux BGO calorim. électromagn. L3,, CERN, mesure luminosité LEP

  8. Étude du détecteur de traces de l'expérience NEMO3. Simulation de la mesure de l'ultra-faible radioactivité en ${208}^TL$ des sources de l'expérience NEMO3 candidates à la double désintégration $\\beta$ sans émission de neutrino

    CERN Document Server

    Errahmane, K

    2001-01-01

    Étude du détecteur de traces de l'expérience NEMO3. Simulation de la mesure de l'ultra-faible radioactivité en ${208}^TL$ des sources de l'expérience NEMO3 candidates à la double désintégration $\\beta$ sans émission de neutrino

  9. Énergie nucléaire. Mesure de la radioactivité dans l'environnement. Eau. Mesurage de l'indice de radioactivité bêta globale en équivalent strontium 90 et yttrium 90 dans l'eau peu chargée en sels.

    CERN Document Server

    Association Française de Normalisation. Paris

    1997-01-01

    Énergie nucléaire. Mesure de la radioactivité dans l'environnement. Eau. Mesurage de l'indice de radioactivité bêta globale en équivalent strontium 90 et yttrium 90 dans l'eau peu chargée en sels.

  10. Rock Permeability and Fluid Pressure At the Ktb. Implications from Laboratory-And Drill Hole-Measurements Perméabilité des roches et pression dans le KTB : enseignements tirés des mesures de laboratoire et des mesures en puits

    Directory of Open Access Journals (Sweden)

    Zimmermann G.

    2006-12-01

    Full Text Available Rock permeability and the fluid pressure were investigated at different scales at the two drill holes of the Continental Deep Drilling Program (KTB. Drill hole tests and fluid inclusion investigations both implicate the existence of hydrostatic fluid pressure in situ with respect to salinity of the formation fluid. Matrix permeability and in situ values from hydraulic tests differ up to three decades with higher values in situ. Further on, the pressure dependence of core permeability and in situ determined values differ significantly. All these observed effects support the well known theory of scale variance. This conclusion is supported by observations of hydraulic communications between both drill holes. These scale effects implicate a pronounced hydraulic heterogeneity of the KTB surroundings. Therefore, stochastic network modelling with parameters derived from structural borehole measurements and under the consideration of the observed permeabilities were performed. Under the presumption of existing driving forces fluid transport takes place dominantly on discrete connected pathways characterised by fracture width, fracture length and fracture orientation and is subordinate in the rock matrix. La perméabilité des roches et la pression des fluides ont été étudiées à différentes échelles sur les deux forages du Programme continental de forage profond - Continental Deep Drilling Program (KTB. Les essais de puits et les recherches d'inclusions de fluides impliquent l'existence d'une pression de fluide fonction de la salinité du fluide de formation. Les valeurs déduites des essais de puits dépassent largement les perméabilités matricielles, l'écart allant jusqu'à trois ordres de grandeur. De plus, l'évolution de la perméabilité mesurée sur échantillon en fonction de la pression et celle déterminée in situ diffèrent largement. Ces observations renforcent la théorie bien connue des effets d'échelle. Cette conclusion est

  11. TRES survey of variable diffuse interstellar bands

    Science.gov (United States)

    Law, Charles J.; Milisavljevic, Dan; Crabtree, Kyle N.; Johansen, Sommer L.; Patnaude, Daniel J.; Margutti, Raffaella; Parrent, Jerod T.; Drout, Maria R.; Sanders, Nathan E.; Kirshner, Robert P.; Latham, David W.

    2017-09-01

    Diffuse interstellar bands (DIBs) are absorption features commonly observed in optical/near-infrared spectra of stars and thought to be associated with polyatomic molecules that comprise a significant reservoir of organic material in the Universe. However, the central wavelengths of almost all DIBs do not correspond with electronic transitions of known atomic or molecular species and the specific physical nature of their carriers remains inconclusive despite decades of observational, theoretical and experimental research. It is well established that DIB carriers are located in the interstellar medium, but the recent discovery of time-varying DIBs in the spectra of the extragalactic supernova SN 2012ap suggests that some may be created in massive star environments. Here, we report evidence of short time-scale (∼10-60 d) changes in DIB absorption line substructure towards 3 of 17 massive stars observed as part of a pathfinder survey of variable DIBs conducted with the 1.5-m Tillinghast telescope and Tillinghast Reflector Echelle Spectrograph (TRES) at Fred L. Whipple Observatory. The detections are made in high-resolution optical spectra (R ∼ 44 000) having signal-to-noise ratios of 5-15 around the 5797 and 6614 Å features, and are considered significant but requiring further investigation. We find that these changes are potentially consistent with interactions between stellar winds and DIB carriers in close proximity. Our findings motivate a larger survey to further characterize these variations and may establish a powerful new method for probing the poorly understood physical characteristics of DIB carriers.

  12. IMPLEMENTATION OF PATHFINDING ON GAME MAPS BASED A-STAR ALGORITHM AND COMPARE THE PERFORMANCES OF VARIOUS ALGORITHMS%基于A*算法的游戏地图寻路实现及性能比较

    Institute of Scientific and Technical Information of China (English)

    邱磊

    2011-01-01

    在A*算法描述的基础上,给出了基于分层寻路思想的A*算法优化方法及划分游戏地图的6种方式.针对26×20=520个节点的游戏地图,利用栅格法按8方向连接对游戏地图进行了划分,分别采用Dijkstra算法、双向宽度优先搜索算法、A*(曼哈顿距离)算法、A*(欧氏距离)算法、A*(切比雪夫距离)算法和动态A*算法5种算法进行了寻路仿真实验,对比分析了各种寻路算法的性能.实验结果表明A*算法是各种寻路算法中扩展节点数量最少和计算耗时最短的一种算法;当采用不同的启发式函数,A*寻路时扩展的节点数量也不同,因此选择一个高效的启发式函数对A*算法是至关重要的.%After A* algorithm's description, given an optimization method of A* algorithm based on hierarchical pathfinding and then the six ways of dividing game map. For a given game map including 44X44 = 1 936 nodes, using the grid-method to divide game map according to the 8-direction connection, and respectively adopt Dijkstra algorithm, Bi-directional breadth first search algorithm, A* (Manhattan distance) algorithm, A* (Euclidean distance) algorithm, A* (Chebyshev distance) algorithm and dynamic A* algorithm to emulate the process of pathfinding, in order to compare the performance of various pathfinding algorithms, the experimental results show that A* algorithm is an algorithm which expanding the number of nodes is the least and time-consuming of calculating is the shortest than other pathfinding algorithms. At the same time, when using different heuristic function, A* path-finding algorithm expand the number of nodes are also different, so choosing an efficient heuristic function for A* algorithm is essential.

  13. Dynamic method for the measurement of Young'S modulus. Application to nuclear graphites; Methode de mesure dynamique du module d'Young. Application aux graphites nucleaires

    Energy Technology Data Exchange (ETDEWEB)

    Pattou, F.; Trutt, J.C

    1963-07-01

    A dynamic method has been developed for measuring Young's modulus and the rigidity modulus using the 'Forster Elastomat'. The principle consists in the determination of the resonance frequencies of graphite samples submitted to transverse, longitudinal, and torsional vibrations. The first two modes of vibration make it possible to calculate the elasticity modulus or the Young's modulus E, the third mode makes possible the calculation of the rigidity modulus G. The relationships from which the moduli E and G are measured are given. A systematic study has been made of graphite samples produced by extrusion or compression and submitted afterwards to one or several impregnations with pitch. For graphites made from the same coke by the same method, a linear relationship has been found for Young's modulus as a function of the apparent density. For the same apparent density, graphites made from different starting materials have generally different Young's moduli that bear a relationship to the crystalline characteristics of the material. The measurements of the rigidity modulus C made on different graphites also show the influence of crystallite orientation. (authors) [French] Une methode de mesure dynamique du module d'Young et du module de rigidite du graphite utilisant 'l'Elastomat Forster' a ete mise au point. Le principe consiste a determiner les frequences de resonance d'echantillons de graphite soumis a des vibrations transversales, longitudinales et de torsion. Les deux premiers modes de vibration permettent de calculer le module d'elasticite ou module d'Young E, le troisieme mode de vibration permet de calculer le module de rigidite G. Apres avoir decrit la methode de mesure, on rappelle les relations qui permettent de calculer les modules E et G. L'etude systematique d'echantillons de graphite, fabriques par filage ou pressage et ayant subi eventuellement une ou plusieurs impregnations au

  14. Optimising a balloon-borne polarimeter in the hard X-ray domain: From the PoGOLite Pathfinder to PoGO+

    Science.gov (United States)

    Chauvin, M.; Jackson, M.; Kawano, T.; Kiss, M.; Kole, M.; Mikhalev, V.; Moretti, E.; Takahashi, H.; Pearce, M.

    2016-09-01

    PoGOLite is a balloon-borne hard X-ray polarimeter dedicated to the study of point sources. Compton scattered events are registered using an array of plastic scintillator units to determine the polarisation of incident X-rays in the energy range 20-240 keV. In 2013, a near circumpolar balloon flight of 14 days duration was completed after launch from Esrange, Sweden, resulting in a measurement of the linear polarisation of the Crab emission. Building on the experience gained from this Pathfinder flight, the polarimeter is being modified to improve performance for a second flight in 2016. Such optimisations, based on Geant4 Monte Carlo simulations, take into account the source characteristics, the instrument response and the background environment which is dominated by atmospheric neutrons. This paper describes the optimisation of the polarimeter and details the associated increase in performance. The resulting design, PoGO+, is expected to improve the Minimum Detectable Polarisation (MDP) for the Crab from 19.8% to 11.1% for a 5 day flight. Assuming the same Crab polarisation fraction as measured during the 2013 flight, this improvement in MDP will allow a 5σ constrained result. It will also allow the study of the nebula emission only (Crab off-pulse) and Cygnus X-1 if in the hard state.

  15. Science Programs for a 2 m-class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope

    CERN Document Server

    Burton, M G; Ashley, M C B; Bailey, J A; Blake, C; Bedding, T R; Bland-Hawthorn, J; Bond, I A; Glazebrook, K; Hidas, M G; Lewis, G; Longmore, S N; Maddison, S T; Mattila, S; Minier, V; Ryder, S D; Sharp, R; Smith, C H; Storey, J W V; Tinney, C G; Tuthill, P; Walsh, A J; Walsh, W; Whiting, M; Wong, T; Woods, D; Yock, P C M

    2004-01-01

    The cold, dry and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-mm wavelengths to be found on the Earth. PILOT is a proposed 2 m telescope, to be built at Dome C in Antarctica, able to exploit these conditions for conducting astronomy at optical and infrared wavelengths. While PILOT is intended as a pathfinder towards the construction of future grand-design facilities, it will also be able to undertake a range of fundamental science investigations in its own right. This paper provides the performance specifications for PILOT, including its instrumentation. It then describes the kinds of science projects that it could best conduct. These range from planetary science to the search for other solar systems, from star formation within the Galaxy to the star formation history of the Universe, and from gravitational lensing caused by exo-planets to that produced by the cosmic web of dark matter. PILOT would be particularly powerful for w...

  16. Optimising a balloon-borne polarimeter in the hard X-ray domain: from the PoGOLite Pathfinder to PoGO+

    CERN Document Server

    Chauvin, Maxime; Kawano, Takafumi; Kiss, Mózsi; Kole, Merlin; Mikhalev, Victor; Moretti, Elena; Takahashi, Hiromitsu; Pearce, Mark

    2016-01-01

    PoGOLite is a balloon-borne hard X-ray polarimeter dedicated to the study of point sources. Compton scattered events are registered using an array of plastic scintillator units to determine the polarisation of incident X-rays in the energy range 20 - 240 keV. In 2013, a near circumpolar balloon flight of 14 days duration was completed after launch from Esrange, Sweden, resulting in a measurement of the linear polarisation of the Crab emission. Building on the experience gained from this Pathfinder flight, the polarimeter is being modified to improve performance for a second flight in 2016. Such optimisations, based on Geant4 Monte Carlo simulations, take into account the source characteristics, the instrument response and the background environment which is dominated by atmospheric neutrons. This paper describes the optimisation of the polarimeter and details the associated increase in performance. The resulting design, PoGO+, is expected to improve the Minimum Detectable Polarisation (MDP) for the Crab from ...

  17. The Use of the Molecular Adsorber Coating Technology to Mitigate Vacuum Chamber Contamination During Pathfinder Testing for the James Webb Space Telescope

    Science.gov (United States)

    Abraham, Nithin S.; Hasegawa, Mark M.; Wooldridge, Eve M.; Henderson-Nelson, Kelly A.

    2016-01-01

    As a coating made of highly porous zeolite materials, the Molecular Adsorber Coating (MAC) was developed to capture outgassed molecular contaminants, such as hydrocarbons and silicones. For spaceflight applications, the adsorptive capabilities of the coating can alleviate on-orbit outgassing concerns on or near sensitive surfaces and instruments within the spacecraft. Similarly, this sprayable paint technology has proven to be significantly beneficial for ground based space applications, in particular, for vacuum chamber environments. This paper describes the recent use of the MAC technology during Pathfinder testing of the Optical Ground Support Equipment (OGSE) for the James Webb Space Telescope (JWST) at NASA Johnson Space Center (JSC). The coating was used as a mitigation tool to entrap persistent outgassed contaminants, specifically silicone based diffusion pump oil, from within JSC's cryogenic optical vacuum chamber test facility called Chamber A. This paper summarizes the sample fabrication, installation, laboratory testing, post-test chemical analysis results, and future plans for the MAC technology, which was effectively used to protect the JWST test equipment from vacuum chamber contamination.

  18. Pratique de la mesure ambulatoire de la pression artérielle à Brazzaville (Congo): données préliminaires

    Science.gov (United States)

    Ikama, Stéphane Méo; Nsitou, Bernice Mesmer; Makani, Jospin; Ellenga-Mbolla, Bertrand; Ondze-Kafata, Louis Igor; Mongo-Ngamami, Solange Flore; Nkalla-Lambi, Mûnka; Gombet, Thierry Raoul; Kimbally-Kaky, Gisèle

    2015-01-01

    Introduction Évaluer l'apport de la MAPA dans la prise en charge de l'hypertension artérielle à Brazzaville. Méthodes Cette étude transversale descriptive a été menée à Brazzaville entre janvier 2011 et décembre 2013 (soit 36 mois). Elle a inclus une série consécutive de 1040 patients ayant bénéficié d'une Mesure Ambulatoire de la Pression Artérielle. Nous avons utilisé le TONOPORT V et le logiciel Cardiosoft 6.51 de GE Health Care, respectivement pour l'enregistrement et l'analyse des données. Les seuils fixés sur les moyennes de 24H étaient une PA 130/80 mmHg pour la confirmation de l'HTA. Résultats Il s'agissait de 573 hommes (55%) et de 467 femmes (45%), âgés en moyenne de 51,7 ± 10,6 ans (extrêmes: 22 et 89 ans). L'indication de la MAPA était à visée thérapeutique dans 627 cas (60,3%), à visée diagnostique dans 410 cas (39,4%), et dans trois cas une suspicion d'effet « blouse blanche ». Dans l'indication à visée diagnostique, l'HTA était confirmée dans 303 cas (74%). La moyenne nycthémérale était de 139 ± 12 mmHg pour la PAS et 89,7 ± 9,6 mmHg pour la PAD; 141,2 ± 13,9 mmHg de PAS et 92,4 ± 10,0 mmHg de PAD en période diurne; 131,1 ± 13,5 mmHg de PAS et 80,7 ± 9,9 mmHg de PAD en période nocturne. Dans l'indication à visée thérapeutique, l'HTA était contrôlée chez 220 patients (35%). La moyenne nycthémérale était de 139 ± 14 mmHg pour la PAS et 88,1 ± 10 mmHg pour la PAD. Les moyennes diurnes et nocturnes étaient respectivement de 140,7 ± 14,0 mmHg et 133,1 ± 16,2 mmHg pour la PAS, 90,3 ± 10,5 et 81,1 ± 10,9 mmHg pour la PAD. Le protocole antihypertenseur utilisé était une monothérapie dans 126 cas (22%), une bithérapie dans 270 cas (47%), une trithérapie dans 149 cas (26%), une quadrithérapie et plus dans 29 cas (5%). Conclusion Cette étude préliminaire a montré l'importance de la MAPA comme outil de diagnostic et d’évaluation thérapeutique. Son utilisation rationnelle dans notre

  19. La distance en formation aux langues par visioconférence : dimensions, mesures, conséquences Distance in Language Training via Videoconferencing: Dimensions, Evaluation, and Consequences

    Directory of Open Access Journals (Sweden)

    Elke Nissen

    2003-12-01

    Full Text Available Nous comparons deux situations de formation en anglais, l'une présentielle et l'autre par visioconférence, à l'aide d'une série d'indicateurs tirés de la littérature mais rarement réunis dans une seule et même étude. Sur un corpus de 18 enregistrements vidéoscopiques de séquences de formation individuelles (9 en situation présentielle vs 9 en visioconférence, nous avons analysé la nature des échanges verbaux, mais aussi relevé et dénombré de nombreux indices gestuels, tantôt caractéristiques de l'implication du sujet dans la relation pédagogique, tantôt révélateurs de son habileté à manipuler le dispositif technique, le tout doublé d'un questionnaire adressé à l'apprenant. Si certaines différences significatives sont conformes à d'autres travaux du même type, il apparaît que des variables pourtant connues comme discriminatrices de ces deux situations ne le sont pas ou révèlent des tendances inverses à celles attendues. Plus largement, la nature des contrastes que nous avons observés renvoie à la manière d'appréhender la mesure de la distance et à la connaissance que nous avons de son influence sur l'apprentissage d'une langue vivante étrangère. Nous proposons alors de considérer la distance davantage comme un paramètre contextuel plutôt que comme une caractéristique déterminée par la situation.This study compares two types of English lessons, one face-to-face and the other via videoconferencing. The different indicators used come from the literature in the field, but have rarely been gathered in one single study. Based on these indicators, 18 video recordings of individual training sessions (9 face to face vs. 9 via video conferencing were analysed. The onus was put on the analysis of verbal interaction as well as the number of gestures, some of them revealing the implication of the learner in the pedagogical relationship, others revealing the learner's technical awareness. In addition, the

  20. A research approach to support the empowerment of alternatives to prison / Une approche de recherche pour soutenir le renforcement des mesures alternatives à l’incarcération

    Directory of Open Access Journals (Sweden)

    Gregori Emilio

    2016-12-01

    Full Text Available Il Progetto Europeo “Reducing prison population: advanced tools of justice in Europe” è stato finanziato dalla Commissione Europea al fine di migliorare la conoscenza e lo scambio di misure innovative di pratiche alternative alla detenzione, sia nella fase pre-processuale, sia in quella dell’esecuzione della pena. La progettazione delle linee guida per l'attuazione di alternative alla detenzione in tutti i paesi europei e del pacchetto formativo, indirizzato al personale che lavora nei servizi che si occupano di alternative alla prigione, è stata preceduta da diverse attività di ricerca svolte in sette paesi europei (Italia, Lettonia, Scozia, Francia, Bulgaria, Romania e Germania. Questo articolo descrive la metodologia utilizzata nelle attività di ricerca e la gestione di queste ultime, condotte in diversi paesi e indirizzate ad una popolazione complessa. Le projet européen « Reducing Prison Population: advanced tools of justice in Europe » a été financé par la Commission Européenne afin d’améliorer la connaissance et d’échanger les approches innovantes de mesures alternatives à l’incarcération, avant comme après le procès. La définition de lignes directrices pour la mise en ɶuvre des alternatives à l’incarcération dans chaque pays européen et du dossier de formation conçu à l’intention du personnel des services offrant des alternatives à la prison, a été précédé par des recherches menées dans sept pays européens (Italie, Lettonie, Écosse, France, Bulgarie, Roumanie et Allemagne. Cet article décrit la méthodologie de recherche utilisée dans ce projet et la gestion des différentes activités menées dans plusieurs pays et ciblées sur une population complexe. The European Project “Reducing prison population: advanced tools of justice in Europe” was funded by the European Commission in order to improve the knowledge and to exchange innovative measures of practices alternative to

  1. Mesures de procédure spéciales et respect des droits de l'homme Rapport général

    Directory of Open Access Journals (Sweden)

    John A.E. Vervaele

    2009-10-01

    Full Text Available Le but du rapport général est de mener une analyse comparative des rapports nationaux en vue de présenter les processus de transformation des systèmes de justice pénale internes, en particulier du procès pénal, étant donné que des mesures procédurales spéciales sont introduites pour appréhender le terrorisme et la criminalité organisée, et de voir si cela a conduit les pays à se départir de leur propres règles fondamentales, procédures, principes et standards des droits de l’homme applicables. Partant de la prémisse qu’un système intégré de droit pénal a trois dimensions – la protection des individus (la dimension de bouclier, la mise à disposition d’instruments d’application de la loi (la dimension d’épée et les contrôles et équilibres c’est-à-dire la séparation des pouvoirs (la dimension constitutionnelle – le rapport fournit un aperçu d’ensemble des transformations corrélées, surtout dans la procédure d’enquête préliminaire, qui les ont affectées toutes les trois dans trois vagues de « guerre » (contre la drogue, le crime organisé et le terrorisme. Dans beaucoup de pays, les garanties procédurales et les principes qui protègent contre la violation du droit à un procès équitable sont considérés comme un fardeau du point de vue de l’efficacité de l’application de la loi à la criminalité grave. Ces réformes se sont traduites par une claire extension de l’état répressif et un estompement des distinctions classiques, et ne favorisent pas la primauté du droit. La focalisation sur la sécurité publique et les investigations contraignantes préventives sapent le système de justice pénale. Avec l’usage croissant du système de justice criminelle comme instrument de régulation du présent et/ou de l’avenir plutôt que de sanction d’un comportement passé, et un procès pénal dans lequel l’enquête préliminaire ne concerne pas la recherche de la v

  2. Engineering surveying

    CERN Document Server

    Schofield, W

    2007-01-01

    Engineering surveying involves determining the position of natural and man-made features on or beneath the Earth's surface and utilizing these features in the planning, design and construction of works. It is a critical part of any engineering project. Without an accurate understanding of the size, shape and nature of the site the project risks expensive and time-consuming errors or even catastrophic failure.Engineering Surveying 6th edition covers all the basic principles and practice of this complex subject and the authors bring expertise and clarity. Previous editions of this classic text have given readers a clear understanding of fundamentals such as vertical control, distance, angles and position right through to the most modern technologies, and this fully updated edition continues that tradition.This sixth edition includes:* An introduction to geodesy to facilitate greater understanding of satellite systems* A fully updated chapter on GPS, GLONASS and GALILEO for satellite positioning in surveying* Al...

  3. Fiabilité intra- et inter-examinateur du dynamomètre MicroFET2 pour la flexion et l'extension du genou: une étude transversale avec répétition des mesures

    OpenAIRE

    Indermühle, Caroline; Henguely, Dunja; Mittaz Hager, Anne-Gabrielle

    2016-01-01

    L’évaluation de la force musculaire est un élément essentiel de la prise en charge physiothérapeutique. Le testing manuel se révèle subjectif et peu précis pour quantifier la force lorsqu’elle est élevée. L’objectivité est pourtant nécessaire et dépend de la qualité des mesures. Les dynamomètres manuels, tels que le microFET2 ont été développés afin de démontrer l’efficacité des traitements de manière objective. Notre objectif est donc de conduire une étude, avec un protocole standardisé...

  4. Spectromètre de mesures diélectriques automatisé dans le domaine de température (77 K - 380 K) et dans l'intervalle continu de fréquence (500 Hz -1 MHz)

    OpenAIRE

    Moliton, A.; Decossas, F.; Moliton, J.-P.

    1980-01-01

    Nous décrivons un dispositif de mesures diélectriques automatisé ; les échantillons, solides ou liquides, peuvent être étudiés en fréquence entre 500 Hz et 1 MHz pour une température variant entre 77 K et 380 K. L'exploitation des résultats est particulièrement rapide ; à titre d'exemple, nous donnons pour deux corps les courbes ε = f (T, v) qui condensent dans une représentation à trois dimensions les variations des paramètres diélectriques (ε' et ε") en fonction de la température et de la f...

  5. Référés libertés sur les mesures d’assignation à résidence : Un contrôle juridictionnel de façade

    OpenAIRE

    Belghiti, Kenza; Korchi, Nina

    2015-01-01

    L’audience de référé de la Section du contentieux du Conseil d’État du vendredi 11 décembre 2015 sur la question des assignations à résidence réunissait sept requérant.e.s, tous militants politiques défendant des idées écologistes. C’est la première fois que la Section du contentieux du Conseil d’État avait l’opportunité de se prononcer sur les mesures adoptées dans le cadre de l’état d’urgence. Au même moment, le Conseil d’État se réunissait en formation consultative pour rendre un avis sur ...

  6. Turbulence et intermittence dans les énergies marines : mesures à haute fréquence en laboratoire de la relation entre puissance produite par une hydrolienne et turbulence

    OpenAIRE

    Duran Medina, Olmo; Schmitt, Francois; Calif, Rudy; Gaurier, Benoit; Germain, Gregory

    2014-01-01

    A partir de données à haute fréquence acquises pendant une longue période de temps, on cherche à déterminer les différentes caractéristiques de l’écoulement généré au bassin d’essais à houle et courant d’IFREMER à Boulogne-Sur-Mer. Ces données mesurées avec un système LDV permettent de caractériser la turbulence et les fluctuations de la vitesse du courant incident. Les conditions contrôlées du bassin et les longues périodes d’acquisition du système LDV nous donneront une bonne estimation des...

  7. Etude et description d'un nouveau thermofluxmètre permettant la mesure simultanée des flux thermiques et des variations de température

    OpenAIRE

    Ravalitera, G.; Cornet, M.; Duthoit, B.; Thery, P.

    1982-01-01

    Les résultats concernant l'effet thermoélectrique dans les feuilles minces recouvertes d'un dépôt électrolytique ont permis la réalisation de plusieurs types de cellules fluxmétriques. Une thermopile de conception nouvelle a été réalisée en intégrant un grand nombre de thermoéléments sur une feuille conductrice de faible épaisseur. La tension apparaissant aux bornes du circuit thermoélectrique est proportionnelle au flux thermique traversant la surface de mesure. La résistance interne varie a...

  8. Apport de la mesure de la pression artérielle centrale ambulatoire dans la caractérisation phénotypique de la démence de type Alzheimer

    OpenAIRE

    HEINTZE, A.

    2014-01-01

    Dans les pays développés, la prévalence des démences est de 5% chez les plus de 65ans et doublerait pour chaque tranche d'âge de 10 ans. Avec le vieillissement de la population, le nombre de personnes atteintes de démence augmente chaque année, ce qui pose le problème de trouver rapidement des thérapies et mesures de prévention efficaces. Il est connu que l'hypertension artérielle (HTA) est un facteur de risque pour certaines démences. De plus, de récentes études démontrent que la pression...

  9. Unitat autònoma remota, d'adquisició de mesures metereològiques de propòsit general i de baix cost per aplicacions domèstiques

    OpenAIRE

    Augé Alomà, Albert

    2009-01-01

    Resum El projecte explica l’estudi del disseny d’una unitat d’adquisició de mesures meteorològiques de propòsit general i de baix cost per aplicacions domèstiques. El sistema dissenyat és una unitat compacta i simple amb alimentació autònoma mitjançant panells fotovoltaics i bateries reforçades amb unes piles de reserva per tal d’assegurar una alimentació elèctrica continua i que utilitza una connexió wireless estàndard per comunicar-se amb un PC que recollirà les dades. ...

  10. Algorithme de positionnement d'une passerelle à mouvements compensés à partir de mesures inertielles et lidar pour les opérations de maintenance des parcs éoliens offshore

    OpenAIRE

    Merriaux, Pierre; Boutteau, Rémi; Vasseur, Pascal; Savatier, Xavier

    2014-01-01

    National audience; Cet article étudie la faisabilité d'un système extéroceptif pour le pilotage d'une passerelle à mouvements compensés sans contact utilisable dans les opérations de maintenance des parcs éoliens en mer. Notre étude montre que les systèmes actuels basés uniquement sur des centrales inertielles ne sont pas assez précis pour garantir le maintien de la passerelle sans un arrimage mécanique. A partir de la mesure d'un lidar 2D nous proposons une méthode temps réel de suivi de la ...

  11. Happiness Survey

    Institute of Scientific and Technical Information of China (English)

    2011-01-01

    Are Chinese people happy in today’s fast-paced, modern society? What are the sources of their happiness? In today’s rapidly developing economy, is happiness closely related to wealth or not? A recent happiness survey conducted in China gives some answers.

  12. Measurement of a neutral particle flux by a thermal method using the junction temperature effect; Mesure d'un flux de particules neutres par une methode thermique mettant a contribution l'effet de temperature des jonctions

    Energy Technology Data Exchange (ETDEWEB)

    Caron, Anthime [Commissariat a l' Energie Atomique, Saclay (France). Centre d' Etudes Nucleaires. Services Scientifiques

    1966-07-01

    Among all the methods suitable for measuring neutral particle fluxes obtained by proton charge exchange in an organic gas, the thermal method has been chosen. The energy imparted by the neutral particles to the target in the form of heat leads to the latter temperature increasing; this temperature is usually followed with a thermocouple. In order to increase the sensitivity and the elegance of the apparatus the thermocouple has been replaced by a junction whose characteristics are known to vary with temperature. A calibration is carried out using a beam of charged particles. The response obtained is linear. Measurements have been made with a power of up to 1 mW; the accuracy increases with the energy provided; for 4 joules an accuracy of 10 per cent is obtained. The apparatus may be improved in particular by extending the measurement range towards low power values, and by increasing the accuracy. (author) [French] Parmi toutes les methodes utilisees pour la mesure d'un flux de particules neutres, obtenues par echange de charge de protons dans un gaz organique, nous avons choisi la methode thermique. L'energie cedee par les particules neutres a la cible sous forme de chaleur provoque une elevation de temperature de celle-ci; cette temperature est habituellement reperee par thermocouple. Pour accroitre la sensibilite et la finesse de l'appareillage, nous avons substitue au thermocouple une jonction dont on sait que les caracteristiques varient avec la temperature. Un etalonnage est realise par un faisceau de particules chargees. La reponse obtenue est lineaire. Des puissances de l'ordre du mW ont ete mesurees; la precision croit avec l'energie apportee; elle est de 10 pour cent quand celle-ci est de 4 joules. L'appareillage peut etre notablement perfectionne, pour reculer la gamme des mesures vers les basses puissances et accroitre la precision. (auteur)

  13. What Are Probability Surveys?

    Science.gov (United States)

    The National Aquatic Resource Surveys (NARS) use probability-survey designs to assess the condition of the nation’s waters. In probability surveys (also known as sample-surveys or statistical surveys), sampling sites are selected randomly.

  14. AMIsurvey, chimenea and other tools: Automated imaging for transient surveys with existing radio-observatories

    CERN Document Server

    Staley, Tim D

    2015-01-01

    In preparing the way for the Square Kilometre Array and its pathfinders, there is a pressing need to begin probing the transient sky in a fully robotic fashion using the current generation of radio telescopes. Effective exploitation of such surveys requires a largely automated data-reduction process. This paper introduces an end-to-end automated reduction pipeline, AMIsurvey, used for calibrating and imaging data from the Arcminute Microkelvin Imager Large Array. AMIsurvey makes use of several component libraries which have been packaged separately for open-source release. The most scientifically significant of these is chimenea, which implements a telescope agnostic algorithm for automated imaging of pre-calibrated multi-epoch radio-synthesis data, making use of CASA subroutines for the underlying image-synthesis operations. At a lower level, AMIsurvey relies upon two libraries, drive-ami and drive-casa, built to allow use of mature radio-astronomy software packages from within Python scripts. These packages...

  15. Survey Expectations

    OpenAIRE

    Martin Weale

    2005-01-01

    This paper focusses on survey expectations and discusses their uses for testing and modeling of expectations. Alternative models of expectations formation are reviewed and the importance of allowing for heterogeneity of expectations is emphasized. A weak form of the rational expectations hypothesis which focusses on average expectations rather than individual expectations is advanced. Other models of expectations formation, such as the adaptive expectations hypothesis, are briefly discussed. ...

  16. Survey Expectations

    OpenAIRE

    Pesaran, M.H.; Weale, M.

    2005-01-01

    This paper focuses on survey expectations and discusses their uses for testing and modeling of expectations. Alternative models of expectations formation are reviewed and the importance of allowing for heterogeneity of expectations is emphasized. A weak form of the rational expectations hypothesis which focuses on average expectations rather than individual expectations is advanced. Other models of expectations formation, such as the adaptive expectations hypothesis, are briefly discussed. Te...

  17. Survey expectations

    OpenAIRE

    Pesaran, Mohammad Hashem; Weale, Martin R.

    2005-01-01

    This paper focuses on survey expectations and discusses their uses for testing and modeling of expectations. Alternative models of expectations formation are reviewed and the importance of allowing for heterogeneity of expectations is emphasized. A weak form of the rational expectations hypothesis which focuses on average expectations rather than individual expectations is advanced. Other models of expectations formation, such as the adaptive expectations hypothesis, are briefly discussed. Te...

  18. Surveying Education

    DEFF Research Database (Denmark)

    Enemark, Stig

    2009-01-01

    In relation to surveying education there is one big question to be asked: Is the role of the surveyors changing? In a global perspective the answer will be "Yes". There is a big swing that could be entitled "From Measurement to Management". This does not imply that measurement is no longer a rele...... on an efficient interaction between education, research, and professional practice.......In relation to surveying education there is one big question to be asked: Is the role of the surveyors changing? In a global perspective the answer will be "Yes". There is a big swing that could be entitled "From Measurement to Management". This does not imply that measurement is no longer....... In surveying education there are a range of other challenges to be faced. These relate to the focus on learning to learn; the need for flexible curriculum to deal with constant change; the move towards introducing virtual academy; the demand for creating a quality culture; and the perspective of lifelong...

  19. Microvesicles but Not Exosomes from Pathfinder Cells Stimulate Functional Recovery of the Pancreas in a Mouse Streptozotocin-Induced Diabetes Model.

    Science.gov (United States)

    McGuinness, Dagmara; Anthony, Diana F; Moulisova, Vladimira; MacDonald, Alasdair I; MacIntyre, Alan; Thomson, Jacqueline; Nag, Abhijeet; Davies, R Wayne; Shiels, Paul G

    2016-06-01

    Pathfinder cells (PCs), a novel cell type derived from the pancreas of adult rats, have been demonstrated to stimulate recovery of tissue structure and function in two animal models of acute tissue damage to date-streptozotocin (STZ)-induced diabetes and ischemia-reperfusion damage to the kidney. In repaired tissue, PCs and their progeny typically represent only 0.02% of the repaired tissue, suggesting that they act via a paracrine mechanism on native cells in the damaged area. Extracellular vesicles are strong candidates for mediating such a paracrine effect. Therefore, we studied the effects of two PC-derived extracellular vesicle fractions on tissue repair in the STZ diabetes model, one containing primarily microvesicles and the second containing predominantly exosomes. Treatment of STZ-induced diabetic mice with the microvesicles preparation led to blood glucose, insulin, glucagon, and C-peptide levels similar to those found with PC treatment. Furthermore, analysis of the histopathology of the pancreas indicated islet regeneration. In contrast, the exosome fraction demonstrated no repair activity, and STZ diabetic mice treated with exosome preparations had blood glucose values that were indistinguishable from those of vehicle-only treated controls. Therefore, we conclude that exosomes play no part in PC action as detected by this assay, whereas microvesicles provide all or a large component of the paracrine activity of PCs. Because they act to stimulate repair of multiple tissues, PC-derived microvesicles may similarly have the potential to stimulate repair of many damaged tissues, identifying a very significant cell-free therapeutic opportunity in regenerative medicine.

  20. Daily snow cover estimation from Advanced Very High Resolution Radiometer Polar Pathfinder data over Northern Hemisphere land surfaces during 1982-2004

    Science.gov (United States)

    Zhao, Hongxu; Fernandes, Richard

    2009-03-01

    The Global Climate Observing System has identified the need for systematic global daily snow cover data sets over land. Current in situ snow cover data sets have limited spatial coverage while satellite-based snow cover records have either limited historical extent or limited temporal and spatial resolution because of cloud cover or specific sensor availability. NOAA Advanced Very High Resolution Radiometer (AVHRR) data offers nearly complete daily global coverage of the Northern Hemisphere, extending back to the early 1980s with successors slated to continue into the next decade. In this paper, we apply a new algorithm, Snowcover, to estimate daily snow cover, including periods of cloudy conditions, from AVHRR Polar Pathfinder (APP) data over Northern Hemisphere land surfaces. This new snow cover product is compared to snow cover estimates derived from long-term in situ snow depth measurements over Canada and the northern Eurasia. The APP snow cover maps showed an 80% agreement rate or better at 95% of the in situ sites. This performance was comparable to the agreement of MODIS 0.05 degree snow cover products over the same sites; although the MODIS product was only retrieved ˜20% of the time corresponding to clear sky conditions in contrast to over 95% of the time with the APP snow product. The almost continuously temporal and spatial coverage for the past 23 years from 1982 to 2004 over Northern Hemisphere makes the new daily snow cover product especially suitable for analysis of large-scale patterns of spring snowmelt in association with variability of circumpolar climate and ecological parameters.