WorldWideScience

Sample records for stellarator primeras medidas

  1. First Toroidal Rotation Measurements of Protons and Impurities in the TJ-II Stellarator; Primeras Medidas de Rotacion Toroidal de Protones e Impurezas en el Stellarator TJ-II

    Energy Technology Data Exchange (ETDEWEB)

    Rapisarda, D.; Zurro, B.; Baciero, A.

    2006-07-01

    First absolute toroidal rotation measurements in the TJ-II stellarator, by using passive emission spectroscopy, are presented. The wavelength calibration is performed by using a spectral system which combines the spectra coming from the plasma and from a lamp in real time. Measurements have been made both for protons and some impurity ions (C4+, He+), in discharges created by electron cyclotron resonance heating, and in discharges with neutral beam injection heating. In addition, a description of the systems as well as the calibration procedures an data analysis is addressed. (Author) 10 refs.

  2. La primera verdad inconveniente

    Directory of Open Access Journals (Sweden)

    Michel ODENT

    2010-12-01

    Full Text Available A partir de una perspectiva fisiológica para analizar la evolución de la humanidad desde los inicios hasta los días actuales, el autor identifica la especie “Homo superpredador” como prevalente en la actualidad, que presenta gran potencial de agresión y dificultad para la convivencia. A medida que las estrategias básicas de sobrevivencia de los grupos humanos son la dominación de la naturaleza y de otros grupos humanos, las sociedades exitosas son las que transmitirán de generación en generación A primeira verdade inconveniente1 The prime inconvenient truth La primera verdad inconveniente REFLEXÕES SOBRE HUMANIZAÇÃO E A REALIDADE DOS SERVIÇOS REFLECTIONS ON HUMANIZATION AND THE REALITY OF HEALTH SERVICES REFLEXIONES SOBRE LA HUMANIZACIÓN Y LA REALIDAD DE LOS SERVICIOS 62 // Rev Tempus Actas Saúde Col creencias y rituales que amplifican el potencial de agresión y moderan la capacidad de amar. Considerando los aspectos emergentes de expresión génica y períodos críticos para la interacción génica con el medio ambiente, el autor consigue asociar las características del Homo superpredador con la forma por el cual los bebés nacen. En una época en que es vital reflexionar sobre la sobrevivencia de la humanidad, mas que en la de grupos específicos, el autor pondera se sería utópico inducir deliberada y conscientemente la llegada del Homo Ecologicus como una nueva variedad de especie humana, a través de un proceso posible de modulación epigenética. Este objetivo implica en un cuestionamiento: Será la fisiología moderna suficientemente poderosa para redescubrir las necesidades básicas de la mujer en el trabajo de parto y de su bebé, a pesar de siglos de socialización del parto y nacimiento y del condicionamiento cultural profundamente arraigado?

  3. Hacia una definición de la medida

    OpenAIRE

    Parot, Jean Jacques

    2012-01-01

    Hacia una definición de la medida A. Primera situación Un granjero va al mercado para vender a) Una gallina (20 pesos) b) Un bulto de naranjas (45 pesos) c) Un pate (38 pesos) d) Una docena de huevos (12 pesos)

  4. Medidas antidumping: instrumento del neoproteccionismo

    OpenAIRE

    Fernando Gutiérrez Solsona

    1994-01-01

    El objetivo fundamental de este trabajo se puede expresar fácilmente: demostrar que las medidas antidumping, que hoy en día son tan utilizadas por la Unión Europea (U.E.) y por los Estados Unidos (EE. UU.), tienen exclusivamente un fin proteccionista. Proteccionismo entendido en el sentido económico, esto es proteger a los sectores nacionales frente a la competencia extranjera, porque los primeros son menos eficientes que los segundos.

  5. Stellar formation

    CERN Document Server

    Reddish, V C

    1978-01-01

    Stellar Formation brings together knowledge about the formation of stars. In seeking to determine the conditions necessary for star formation, this book examines questions such as how, where, and why stars form, and at what rate and with what properties. This text also considers whether the formation of a star is an accident or an integral part of the physical properties of matter. This book consists of 13 chapters divided into two sections and begins with an overview of theories that explain star formation as well as the state of knowledge of star formation in comparison to stellar structure

  6. Stellar remnants

    CERN Document Server

    Kawaler, S D; Srinivasan, G

    1997-01-01

    This volume examines the internal structure, origin and evolution of white dwarfs, neutron stars and black holes, all objects at the final stage of stellar evolution. It covers topics such as: pulsation of white dwarfs; millisecond pulsars; and the dynamics around black holes.

  7. Stellar winds

    International Nuclear Information System (INIS)

    Weymann, R.J.

    1978-01-01

    It is known that a steady outflow of material at comparable rates of mass loss but vastly different speeds is now known to be ubiquitous phenomenon among both the luminous hot stars and the luminous but cool red giants. The flows are probably massive enough in both cases to give rise to significant effects on stellar evolution and the mass balance between stars and the interstellar medium. The possible mechanisms for these phenomena as well as the methods of observation used are described. In particular, the mass-loss processes in stars other than the sun that also involve a steady flow of matter are considered. The evidence for their existence is described, and then the question of whether the process thought to produce the solar wind is also responsible for producing these stellar winds is explored

  8. Stellarator physics

    International Nuclear Information System (INIS)

    1990-07-01

    This document consists of the proceedings of the Seventh International Workshop on Stellarators, held in Oak Ridge, Tennessee, USA, 10-14 April, 1989. The document consists of a summary of presentations, an overview of experimental results, and papers presented at the workshop on transport, impurities and divertors, diagnostics, ECH confinement experiments, equilibrium and stability studies, RF heating, confinement, magnetic configurations, and new experiments. Refs, figs and tabs

  9. Stellar evolution

    CERN Document Server

    Meadows, A J

    2013-01-01

    Stellar Evolution, Second Edition covers the significant advances in the understanding of birth, life, and death of stars.This book is divided into nine chapters and begins with a description of the characteristics of stars according to their brightness, distance, size, mass, age, and chemical composition. The next chapters deal with the families, structure, and birth of stars. These topics are followed by discussions of the chemical composition and the evolution of main-sequence stars. A chapter focuses on the unique features of the sun as a star, including its evolution, magnetic fields, act

  10. EL DERECHO A LA EDUCACIÓN Y ATENCIÓN DE LA PRIMERA INFANCIA EN AMÉRICA LATINA

    Directory of Open Access Journals (Sweden)

    Ana Ancheta Arrabal

    2013-01-01

    Full Text Available Estudiamos aquí algunos de los factores que ayudan a comprender la situación actual del primero de los objetivos de la Educación para Todos en América Latina. Así, planteamos un marco que delimita la realidad socio-histórica de la región en lo que respecta al bienestar y la exclusión social como elementos que condicionan los procesos de desarrollo para, después, atender al progreso y situación de expansión de la educación y atención de la primera infancia, especialmente para los grupos más vulnerables de las sociedades latinoamericanas. Finalmente, analizamos las medidas y acciones planteadas para intentar hacer posible el derecho a una educación y atención de calidad y equidad para la primera infancia.

  11. "Kipling y su sorprendente primera novela"

    Directory of Open Access Journals (Sweden)

    Yván Pozuelo Andrés

    2013-01-01

    Full Text Available Rudyard Kipling aludió a la masonería en varias decenas de escritos. Su fama como escritor le situó en un lugarprivilegiado en las listas confeccionadas por los mediosmasónicos sobre ilustres masones. Sin embargo, suprimer relato de éxito internacional,El Hombre que quiso ser Rey, apenas fue citado entre las obras quemencionaban a la Orden, ni demasiado estudiado. Contrariamente a lo que podría pensarse de un masón queescribe empleando referencias masónicas, Kipling no cayó en la simplicidad del elogio. Así pues, este estudioenfocado a esta primera novela de Kipling pretende, desde el campo académico, abrir las puertas, en el espaciohistoriográfico hispanoamericano, al análisis de este autor y de su obra en clave masónica.

  12. Reseña en primera persona

    Directory of Open Access Journals (Sweden)

    Fernández Vara, Guillermo

    2005-02-01

    Full Text Available Agradezco sinceramente la oportunidad que se me brinda para dar mi opinión, para contar mis impresiones, para ofrecer mis reflexiones o para, simplemente, expresar mis certidumbres y mis dudas, que de todo hay en un mundo tan complejo como es el de la sanidad. Hace casi diez años que me senté por primera vez en el Consejo Interterritorial del Sistema Nacional de Salud. Gobernaba por entonces en España el PSOE y lo haría hasta Marzo de 1996, era Ministra de Sanidad y Consumo una persona a la que quiero mucho y respeto más, Mª Ángeles Amador. Conoceré luego a cuatro ministros más, J.M. Romay, C. Villalobos, A. Pastor y E. Salgado.…

  13. Stellar astrophysics

    International Nuclear Information System (INIS)

    1988-01-01

    Enhanced mass loss occurs at critical stages in the evolution of stars over a wide range of stellar mass. Observationally, these stages are difficult to identify because of their short duration and because the star is often obscured by dust which condenses in the ejecta. A study of a G-type star, of which only the outer envelope was directly visible, was undertaken by the South African Astronomical Observatory (SAAO). The star itself was obscured by dust clouds and its light was only feebly seen by reflection from some of these clouds. Other studies of the galaxy undertaken by the SAAO include observations of the following: the extreme carbon star IRAS 15194-5115; RV Tauri and T Tauri stars; pre-main sequence stars; the properties of circumstellar dust; rotational modulation and flares on RS CVn and BY Dra stars; heavy-element stars; hydrogen-deficient stars; the open cluster NGC6192; stars in Omega Centauri, and lunar occulations of stars. Simultaneous x-ray, radio and optical data of the flare star YZ CMi were also obtained. 1 fig

  14. Stellar Metamorphosis:

    Science.gov (United States)

    2002-01-01

    [TOP LEFT AND RIGHT] The Hubble Space Telescope's Wide Field and Planetary Camera 2 has captured images of the birth of two planetary nebulae as they emerge from wrappings of gas and dust, like butterflies breaking out of their cocoons. These images highlight a fleeting phase in the stellar burnout process, occurring just before dying stars are transformed into planetary nebulae. The left-hand image is the Cotton Candy nebula, IRAS 17150-3224; the right-hand image, the Silkworm nebula, IRAS 17441-2411. Called proto-planetary nebulae, these dying stars have been caught in a transition phase between a red giant and a planetary nebula. This phase is only about 1,000 years long, very short in comparison to the 1 billion-year lifetime of a star. These images provide the earliest snapshots of the transition process. Studying images of proto-planetary nebulae is important to understanding the process of star death. A star begins to die when it has exhausted its thermonuclear fuel - hydrogen and helium. The star then becomes bright and cool (red giant phase) and swells to several tens of times its normal size. It begins puffing thin shells of gas off into space. These shells become the star's cocoon. In the Hubble images, the shells are the concentric rings seen around each nebula. But the images also reveal the nebulae breaking out from those shells. The butterfly-like wings of gas and dust are a common shape of planetary nebulae. Such butterfly shapes are created by the 'interacting winds' process, in which a more recent 'fast wind' - material propelled by radiation from the hot central star - punches a hole in the cocoon, allowing the nebula to emerge. (This 'interacting wind' theory was first proposed by Dr. Sun Kwok to explain the origin of planetary nebulae, and has been subsequently proven successful in explaining their shapes.) The nebulae are being illuminated by light from the invisible central star, which is then reflected toward us. We are viewing the nebulae

  15. Mirror Coronograph for Argentina (MICA). Primera Luz

    Science.gov (United States)

    Stenborg, G.; Epple, A.; Schwenn, R.; Francile, C.; Rovira, M.

    En Julio de 1997 se terminó con la primera parte de la instalación del ``Coronógrafo de Espejo para la Argentina'' en la estación de altura Carlos U. Cesco (El Leoncito), gracias al esfuerzo de la gente del Max Planck Institut für Aeronomie (Alemania), del OAFA y del IAFE. Dicho coronógrafo forma parte de un programa de ciencia bilateral entre Alemania y Argentina. El propósito del mismo, en conjunción con otros telescopios solares y terrestres, es contribuir a un mejor entendimiento de cuestiones fundamentales de la física solar. Para ello, ya está observando la corona de emisión en el verde (Fe XIV), rojo (Fe X) y Hα entre 1.05 y 2 radios solares aproximadamente. El diseño del instrumento, el cual fuera ya presentado en esta misma reunión en La Plata en 1996, es esencialmente similar al del telescopio LASCO-C1 a bordo del Solar Heliospheric Observatory (SOHO). La adquisición de datos se realiza con un CCD de 1280x1024 pixels, codificando en 12 bits, pudiendo ser el mismo operado en forma remota. En esta reunión presentaremos algunas de las observaciones realizadas durante la puesta a punto del instrumento en el período julio-setiembre de 1997. Asimismo expondremos cómo y por qué sus resultados complementarán a los de su par en el espacio.

  16. Inmunidad bucal en la primera infancia

    Directory of Open Access Journals (Sweden)

    Enrique Rotemberg Wilf

    Full Text Available La aparición precoz de enfermedades bucales infecciosas y transmisibles en niños, como caries dentales y enfermedad periodontal, resulta de un desequilibrio entre los mecanismos defensivos del huésped y la virulencia de microorganismos presentes en el medio bucal, a favor de estos últimos. La erupción dentaria que comienza desde el primer año de vida brinda nuevos hábitat a las bacterias en el medio bucal como la superficie del esmalte dental y el surco gingival en el paradencio de inserción dentaria, propicios para el desarrollo de especies bacterianas cariogénicas y/o paradenciopáticas. Este desarrollo es favorecido por condiciones adversas como dieta rica en azúcares fermentables, higiene bucal deficitaria, malposiciones dentarias, escasa secreción salival, hábitos prolongados nocivos como succión no nutritiva, respiración bucal, masticación mínima por ingesta de alimentos que casi no requieren procesamiento para ser deglutidos. Es prioritario controlar los circuitos de infectividad bucal, especialmente durante la primera infancia, cuando el sistema inmune del niño aún está inmaduro y comienza a tomar contacto con antígenos. La madre por el estrecho vínculo físico con su hijo resulta el principal transmisor de gérmenes, sumado a la fase de reconocimiento oral del niño de su propio cuerpo y el entorno. Pese a ello el niño cuenta desde el nacimiento con mecanismos de defensa innatos y otros adquiridos pasivamente en la gestación y a través de la lactancia materna, que dificultan el desarrollo de enfermedades infecciosas bucales y sistémicas

  17. Advanced stellarator power plants

    International Nuclear Information System (INIS)

    Miller, R.L.

    1994-01-01

    The stellarator is a class of helical/toroidal magnetic fusion devices. Recent international progress in stellarator power plant conceptual design is reviewed and comparisons in the areas of physics, engineering, and economics are made with recent tokamak design studies

  18. Sistema ultra-sonico para medida volumetrica

    OpenAIRE

    Isaias Ferreira da Silva

    1999-01-01

    Resumo: Um método inovador para a medida do volume de um líquido dentro de um recipiente fechado é proposto. A motivação deste trabalho é a aplicação do método para a medida do volume de combustível dentro de um tanque de automóvel. Este método se baseia no fenômeno de reverberação sonora que relaciona o tempo de decaimento da intensidade do som dentro de um ambiente com o seu volume. Este tempo, conhecido como tempo de reverberação, está associado ao volume vazio dentro do recipiente, ao mat...

  19. Medidas de la felicidad nacional bruta

    NARCIS (Netherlands)

    R. Veenhoven (Ruut)

    2009-01-01

    textabstractResumen. La felicidad está abriéndose hueco en la agenda política, lo cual reclama medir el éxito alcanzado por los distintos países en crear felicidad para un gran número de personas, de un modo análogo a las medidas del éxito en la creación de riqueza, como el PNB. La felicidad se

  20. Stellar structure and evolution

    International Nuclear Information System (INIS)

    Kippernhahn, R.; Weigert, A.

    1990-01-01

    This book introduces the theory of the internal structure of stars and their evolution in time. It presents the basic physics of stellar interiors, methods for solving the underlying equations, and the most important results necessary for understanding the wide variety of stellar types and phenomena. The evolution of stars is discussed from their birth through normal evolution to possibly spectacular final stages. Chapters on stellar oscillations and rotation are included

  1. Models for stellar flares

    International Nuclear Information System (INIS)

    Cram, L.E.; Woods, D.T.

    1982-01-01

    We study the response of certain spectral signatures of stellar flares (such as Balmer line profiles and the broad-band continuum) to changes in atmospheric structure which might result from physical processes akin to those thought to occur in solar flares. While each physical process does not have a unique signature, we can show that some of the observed properties of stellar flares can be explained by a model which involves increased pressures and temperatures in the flaring stellar chromosphere. We suggest that changes in stellar flare area, both with time and with depth in the atmosphere, may play an important role in producing the observed flare spectrum

  2. Stellar Physics 2: Stellar Evolution and Stability

    CERN Document Server

    Bisnovatyi-Kogan, Gennady S

    2011-01-01

    "Stellar Physics" is a an outstanding book in the growing body of literature on star formation and evolution. Not only does the author, a leading expert in the field, very thoroughly present the current state of knowledge on stellar physics, but he handles with equal care the many problems that this field of research still faces. A bibliography with well over 1000 entries makes this book an unparalleled reference source. "Stellar Evolution and Stability" is the second of two volumes and can be read, as can the first volume "Fundamental Concepts and Stellar Equilibrium," as a largely independent work. It traces in great detail the evolution of protostars towards the main sequence and beyond this to the last stage of stellar evolution, with the corresponding vast range from white dwarfs to supernovae explosions, gamma-ray bursts and black hole formation. The book concludes with special chapters on the dynamical, thermal and pulsing stability of stars. This second edition is carefully updated in the areas of pre...

  3. Medidas de pobreza: un enfoque alternativo

    OpenAIRE

    Lazzari, Luisa L; Fernández, María José

    2006-01-01

    Una medida creíble de pobreza e indigencia puede ser un poderoso instrumento para concentrar la atención del policymaker en las condiciones de vida de los pobres. Las opciones elegidas para fijarlas tienen gran importancia para las decisiones políticas a tomar. El método indirecto o enfoque del ingreso parte de la valorización de una Canasta Básica Alimentaria (CBA) que determina la cantidad de calorías mínimas necesarias para satisfacer las necesidades biológicas básicas de...

  4. Medidas de administración pesquera.

    OpenAIRE

    2014-01-01

    En el Titulo II de la Ley General de Pesca y Acuicultura "De la Administración de las Pesquerías", específicamente en facultades de conservación de los recursos hidrobiológicos, se establece lo siguiente: En cada área de pesca, independiente del régimen de acceso a que se encuentre sometida, el Ministerio, mediante decreto supremo fundado, podrá establecer una o más prohibiciones o medidas de administración de recursos hidrobiológicos. Esta presentación que proporciona información refere...

  5. Stellar photometry and polarimetry

    International Nuclear Information System (INIS)

    Golay, M.; Serkowski, K.

    1976-01-01

    A critical review of progress made in stellar photometry and polarimetry over the period 1973-1975 is presented. Reports of photometric measurements from various observatories throughout the world are summarized. The summary of work on stellar polarimetry lists the review papers, the catalogues and lists of standard stars, and descriptions of new observing techniques. (B.R.H.)

  6. Medidas tipográficas: un recuento

    Directory of Open Access Journals (Sweden)

    Oriol Moret Viñals

    2015-07-01

    Full Text Available Breve repaso al desarrollo de la concepción métrica en la tipografía en plomo, alternativa y complemento de la visión habitual en lo que conocemos como “tipometría”. Se parte de una noción amplia de medida: el factor cuantitativo se dilata con la articulación de relaciones proporcionales e integra la dimensión cualitativa de los sistemas métricos tradicionales. La tipografía se considera bajo presupuestos similares: como sistema articulado de piezas materiales cuyas magnitudes contienen usos y valores específicos, más allá de su simple expresión numérica. Con tales premisas, se revisan fuentes documentales significativas del “período de la imprenta manual”. Su examen, vinculado a los usos y costumbres de oficio, desvela la distinta aproximación métrica, que puede resumirse en tres fases evolutivas: hermética, intensiva, expansiva –como recogen las referencias de los cuerpos tipográficos: adjetivas, sustantivas, numéricas. Se proporciona así un marco para apreciar el cambio de sentido en las medidas tipográficas hasta nuestros días.

  7. Compact stellarators as reactors

    International Nuclear Information System (INIS)

    Lyon, J.F.; Valanju, P.; Zarnstorff, M.C.; Hirshman, S.; Spong, D.A.; Strickler, D.; Williamson, D.E.; Ware, A.

    2001-01-01

    Two types of compact stellarators are examined as reactors: two- and three-field-period (M=2 and 3) quasi-axisymmetric devices with volume-average =4-5% and M=2 and 3 quasi-poloidal devices with =10-15%. These low-aspect-ratio stellarator-tokamak hybrids differ from conventional stellarators in their use of the plasma-generated bootstrap current to supplement the poloidal field from external coils. Using the ARIES-AT model with B max =12T on the coils gives Compact Stellarator reactors with R=7.3-8.2m, a factor of 2-3 smaller R than other stellarator reactors for the same assumptions, and neutron wall loadings up to 3.7MWm -2 . (author)

  8. VIOLENCIA DE GÉNERO EN LAS UNIVERSIDADES: INVESTIGACIONES Y MEDIDAS PARA PREVENIRLA

    Directory of Open Access Journals (Sweden)

    Rosa Larena

    2010-12-01

    Full Text Available Normal 0 21 false false false ES ZH-TW X-NONE MicrosoftInternetExplorer4 En este artículo recogemos los resultados de la investigación “Violencia de género en las universidades españolas”, la primera investigación que analiza la violencia de género en el contexto universitario en España. Las investigaciones sobre esta clase de violencia en el ámbito internacional muestran, por un lado, que es una realidad existente en la universidad, de la misma forma que lo es en otros ámbitos sociales. Por otro lado, el análisis de las actuaciones implementadas por universidades de prestigio muestra la existencia de diferentes medidas para prevenirla y superarla. Estas evidencias, contrastadas con las percepciones de diferentes colectivos de la comunidad universitaria sobre la aplicabilidad de estas medidas en las universidades españolas, son el punto de partida para iniciar el desarrollo de medidas que erradiquen la violencia de género en nuestras universidades. In this article we present the findings from the research “Gender violence in Spanish universities”, the first study that analyses gender violence in the university context in Spain. Studies on gender violence at the international level show, on the one hand, that gender violence is a reality that exists in universities, in the same way that it exists in other social contexts. On the other hand, the analysis of the actions implemented in prestigious universities shows the existence of measures to prevent and overcome it. Contrasting these evidences with the perceptions of different university collectives about the applicability of these measures in Spanish universities is the starting point to develop measures to eradicate gender violence in our universities.

  9. Anuncian primera produccion controlada de anti-atomos frios

    CERN Document Server

    2002-01-01

    "Un equipo internacional que trabaja con el desacelerador de antiprotones del CERN, en Ginebra, ha conseguido la primera produccion controlada de miles de atomos de hidrogeno de baja energia, lo que facilitara en el futuro los analisis de precision en varias disciplinas cientificas" (1 page).

  10. Aportes de la psicología forense a la aplicación de medidas alternativas a la privatización de la libertad en la administración de justicia penal

    OpenAIRE

    Corach, Irene; Di Tella, Yago

    2009-01-01

    Nuestro país no cuenta con estadísticas (oficiales o no oficiales) sobre la aplicación de medidas alternativas a la privación de libertad y tampoco con estudios cualitativos que den cuenta de su eficacia y eficiencia. Es en este sentido que nuestro Proyecto se propone en sus objetivos generales generar un mapa de la situación de las medidas alternativas en Ciudad Autónoma de Buenos Aires y Provincia de Buenos Aires, en términos estadísticos La investigación se propone establecer por primera v...

  11. Stellarator-Spheromak

    International Nuclear Information System (INIS)

    Moroz, P.E.

    1997-03-01

    A novel concept for magnetic plasma confinement, Stellarator-Spheromak (SSP), is proposed. Numerical analysis with the classical-stellarator-type outboard stellarator windings demonstrates a number of potential advantages of SSP for controlled nuclear fusion. Among the main ones are: simple and compact magnet coil configuration, absence of material structures (e.g. magnet coils or conducting walls) in the center of the torus, high rotational transform, and a possibility of MHD equilibria with very high β (pressure/magnetic pressure) of the confined plasma

  12. Double-helix stellarator

    International Nuclear Information System (INIS)

    Moroz, P.E.

    1997-09-01

    A new stellarator configuration, the Double-Helix Stellarator (DHS), is introduced. This novel configuration features a double-helix center post as the only helical element of the stellarator coil system. The DHS configuration has many unique characteristics. One of them is the extreme low plasma aspect ratio, A ∼ 1--1.2. Other advantages include a high enclosed volume, appreciable rotational transform, and a possibility of extreme-high-β MHD equilibria. Moreover, the DHS features improved transport characteristics caused by the absence of the magnetic field ripple on the outboard of the torus. Compactness, simplicity and modularity of the coil system add to the DHS advantages for fusion applications

  13. Wimps and stellar structure

    International Nuclear Information System (INIS)

    Bouquet, A.; Salati, P.

    1988-01-01

    We present the results of an analytic approximation to compute the effects of WIMPs on stellar structures in a self-consistent way. We examine in particular the case of the Sun and of horizontal branch stars

  14. Principles of Stellar Interferometry

    CERN Document Server

    Glindemann, Andreas

    2011-01-01

    Over the last decade, stellar interferometry has developed from a specialist tool to a mainstream observing technique, attracting scientists whose research benefits from milliarcsecond angular resolution. Stellar interferometry has become part of the astronomer’s toolbox, complementing single-telescope observations by providing unique capabilities that will advance astronomical research. This carefully written book is intended to provide a solid understanding of the principles of stellar interferometry to students starting an astronomical research project in this field or to develop instruments and to astronomers using interferometry but who are not interferometrists per se. Illustrated by excellent drawings and calculated graphs the imaging process in stellar interferometers is explained starting from first principles on light propagation and diffraction wave propagation through turbulence is described in detail using Kolmogorov statistics the impact of turbulence on the imaging process is discussed both f...

  15. Convection and stellar oscillations

    DEFF Research Database (Denmark)

    Aarslev, Magnus Johan

    2017-01-01

    for asteroseismology, because of the challenges inherent in modelling turbulent convection in 1D stellar models. As a result of oversimplifying the physics near the surface, theoretical calculations systematically overestimate the oscillation frequencies. This has become known as the asteroseismic surface effect. Due...... to lacking better options, this frequency difference is typically corrected for with ad-hoc formulae. The topic of this thesis is the improvement of 1D stellar convection models and the effects this has on asteroseismic properties. The source of improvements is 3D simulations of radiation...... atmospheres to replace the outer layers of stellar models. The additional turbulent pressure and asymmetrical opacity effects in the atmosphere model, compared to convection in stellar evolution models, serve to expand the atmosphere. The enlarged acoustic cavity lowers the pulsation frequencies bringing them...

  16. DE LA PRIMERA A LA SEGUNDA GENERACION DE REFORMAS DEL ESTADO EN AMERICA LATINA: GIRO IDEOLOGICO Y CAMBIO CONCEPTUAL

    Directory of Open Access Journals (Sweden)

    García Chourio José Guillermo

    2003-08-01

    Full Text Available

    García Chourio, José Guillermo. "De la Primera a la Segunda Generacion de Reformas del Estado en America Latina: Giro Ideologico y Cambio Conceptual", Cuadernos de Economía, V. XXII, n. 38, Bogota, 2003, paginas 95-125.

    Este trabajo explora la orientacion ideologica y conceptual que ha guiado el proceso de reformas economicas en America Latina, diferenciando la puesta en marcha de las medidas en dos generaciones. Partimos de la idea de que la transicion entre  generaciones  obedece a las reformas iniciales, producto de las experiencias del fracaso y oposicion que han tenido los ajustes. Se concluye que existio un giro conceptual, expresado por el paso del enfoque de las expectativas racionales, el cual sustento una politica de choques externos mediante medidas de ajuste y de reduccion del estado para disciplinar a los agentes economicos, al enfoque neoinstitucional, que concibe las reformas como un proceso de creacion de instituciones acordes para el buen funcionamiento del mercado, reconociendose ahora al Estado como mecanismo basico para reducir los costos de transaccion de dichos agentes en el mercado.

  17. Oscillations in stellar atmospheres

    International Nuclear Information System (INIS)

    Costa, A.; Ringuelet, A.E.; Fontenla, J.M.

    1989-01-01

    Atmospheric excitation and propagation of oscillations are analyzed for typical pulsating stars. The linear, plane-parallel approach for the pulsating atmosphere gives a local description of the phenomenon. From the local analysis of oscillations, the minimum frequencies are obtained for radially propagating waves. The comparison of the minimum frequencies obtained for a variety of stellar types is in good agreement with the observed periods of the oscillations. The role of the atmosphere in the globar stellar pulsations is thus emphasized. 7 refs

  18. La primera producción literaria de Vargas Vila

    Directory of Open Access Journals (Sweden)

    Alberto Miramón

    1965-05-01

    Full Text Available Es siempre curioso y en grado sumo instructivo, indagar las primicias literarias de los grandes escritores. Bien pueden no ser sus primeras producciones las más importantes y valiosas muestras de su ingenio en el conjunto total de sus obras; pero esas páginas, que generalmente suelen olvidar cuando ya son famosos, tienen singulares características para la comprensión sicológica de sus autores.

  19. PREFACE: A Stellar Journey A Stellar Journey

    Science.gov (United States)

    Asplund, M.

    2008-10-01

    The conference A Stellar Journey was held in Uppsala, Sweden, 23 27June 2008, in honour of Professor Bengt Gustafsson's 65th birthday. The choice of Uppsala as the location for this event was obvious given Bengt's long-standing association with the city stemming back to his school days. With the exception of a two-year postdoc stint in Copenhagen, five years as professor at Stockholm University and two years as director of the Sigtuna foundation, Bengt has forged his illustrious professional career at Uppsala University. The symposium venue was Museum Gustavianum, once the main building of the oldest university in Scandinavia. The title of the symposium is a paraphrasing of Bengt's popular astronomy book Kosmisk Resa (in English: Cosmic Journey) written in the early eighties. I think this aptly symbolizes his career that has been an astronomical voyage from near to far, from the distant past to the present. The original book title was modified slightly to reflect that most of his work to date has dealt with stars in one way or another. In addition it also gives credit to Bengt's important role as a guiding light for a very large number of students, colleagues and collaborators, indeed for several generations of astronomers. For me personally, the book Kosmisk Resa bears particular significance as it has shaped my life rather profoundly. Although I had already decided to become an astronomer, when I first read the book as a 14-year-old I made up my mind then and there that I would study under Bengt Gustafsson and work on stars. Indeed I have remained true to this somewhat audacious resolution. I suspect that a great number of us have similar stories how Bengt has had a major influence on our lives, whether on the professional or personal level. Perhaps Bengt's most outstanding characteristic is his enthralling enthusiasm. This is equally true whether he is pondering some scientific conundrum, supervising students or performing in front of an audience, be it an

  20. Stellar magnetic activity

    International Nuclear Information System (INIS)

    Schrijver, C.J.

    1986-01-01

    The stellar emission in the chromospheric Ca II H+K lines is compared with the coronal soft X-ray emission, measuring the effects of non-radiative heating in the outer atmosphere at temperatures differing two orders of magnitude. The comparison of stellar flux densities in Ca II H+K and X-rays is extended to fluxes from the transition-region and the high-temperature chromosphere. The stellar magnetic field is probably generated in the differentially rotating convective envelope. The relation between rotation rate and the stellar level of activity measured in chromospheric, transition-region, and coronal radiative diagnostics is discovered. X-ray observations of the binary λ Andromedae are discussed. The departure of M-type dwarfs from the main relations, and the implications for the structure of the chromospheres of these stars are discussed. Variations of the average surface flux densities of the Sun during the 11-year activity cycle agree with flux-flux relations derived for other cool stars, suggesting that the interpretation of the stellar relations may be furthered by studying the solar analogue in more detail. (Auth.)

  1. Introduction to stellar structure

    CERN Document Server

    Maciel, Walter J

    2016-01-01

    In the first part of this book, the author presents the basic properties of the stellar interior and describes them thoroughly, along with deriving the main stellar structure equations of temperature, density, pressure and luminosity, among others. The process and application of solving these equations is explained, as well as linking these results with actual observations.  The second part of the text describes what happens to a star over time, and how to determine this by solving the same equations at different points during a star’s lifetime. The fate of various stars is quite different depending on their masses, and this is described in the final parts of the book. This text can be used for an upper level undergraduate course or an introductory graduate course on stellar physics.

  2. The Galactic stellar disc

    International Nuclear Information System (INIS)

    Feltzing, S; Bensby, T

    2008-01-01

    The study of the Milky Way stellar discs in the context of galaxy formation is discussed. In particular, we explore the properties of the Milky Way disc using a new sample of about 550 dwarf stars for which we have recently obtained elemental abundances and ages based on high-resolution spectroscopy. For all the stars we also have full kinematic information as well as information about their stellar orbits. We confirm results from previous studies that the thin and the thick discs have distinct abundance patterns. But we also explore a larger range of orbital parameters than what has been possible in our previous studies. Several new results are presented. We find that stars that reach high above the Galactic plane and have eccentric orbits show remarkably tight abundance trends. This implies that these stars formed out of well-mixed gas that had been homogenized over large volumes. We find some evidence that suggest that the event that most likely caused the heating of this stellar population happened a few billion years ago. Through a simple, kinematic exploration of stars with super-solar [Fe/H], we show that the solar neighbourhood contains metal-rich, high velocity stars that are very likely associated with the thick disc. Additionally, the HR1614 moving group and the Hercules and Arcturus stellar streams are discussed and it is concluded that, probably, a large fraction of the groups and streams so far identified in the disc are the result of evolution and interactions within the stellar disc rather than being dissolved stellar clusters or engulfed dwarf galaxies.

  3. Transport in stellarators

    International Nuclear Information System (INIS)

    Maassberg, H.; Brakel, R.; Burhenn, R.; Gasparino, U.; Grigull, P.; Kick, M.; Kuehner, G.; Ringler, H.; Sardei, F.; Stroth, U.; Weller, A.

    1993-01-01

    The local electron and ion heat transport as well as the particle and impurity transport properties in stellarators are reviewed. In this context, neoclassical theory is used as a guideline for the comparison of the experimental results of the quite different confinement concepts. At sufficiently high temperatures depending on the specific magnetic configuration, neoclassical predictions are confirmed by experimental findings. The confinement properties in the LMFP collisionality regime are discussed with respect to the next stellarator generation, for which at higher temperatures the neoclassical transport is expected to become more important. (orig.)

  4. Solar and stellar oscillations

    International Nuclear Information System (INIS)

    Fossat, E.

    1981-01-01

    We try to explain in simple words what a stellar oscillation is, what kind of restoring forces and excitation mechanisms can be responsible for its occurence, what kind of questions the theoretician asks to the observer and what kind of tools the latter is using to look for the answers. A selected review of the most striking results obtained in the last few years in solar seismology and the present status of their consequences on solar models is presented. A brief discussion on the expected extension towards stellar seismology will end the paper. A selected bibliography on theory as well as observations and recent papers is also included. (orig.)

  5. PROPRIEDADES PSICOMÉTRICAS DE INSTRUMENTOS DE MEDIDAS: BASES CONCEITUAIS E MÉTODOS DE AVALIAÇÃO–PARTE I

    Directory of Open Access Journals (Sweden)

    Maria Elena Echevarría-Guanilo

    2017-01-01

    Full Text Available Objetivo: presentar y discutir bases conceptuales y métodos de evaluaciones que fundamentan importantes propiedades de instrumentos de medidas. En esta primera parte, se presentan y discute los conceptos de confiabilidad, responsividad e interpretabilidad, citados ejemplos de las principales formas de evaluación de esas propiedades. Método: estudio teórico basado en la literatura internacional y nacional y en los instrumentos Consensus-based Standards for the selection of health Measurement Instruments y Evaluating the Measurement of Patient-Reported Outcomes que contemplan conceptos de evaluación de instrumentos para la evaluación de los resultados de los pacientes. Resultados: en este enfoque, se puede percibir que todavía hay divergencias en algunas descripciones conceptuales. Sin embargo, los autores resaltan la importancia de la confiabilidad para evaluar el instrumento de medida. Se destaca la importancia del conocimiento del Modelo Conceptual, de las propiedades de medidas y de los diferentes métodos de evaluación para garantizar, principalmente en estudio de validación de instrumentos, resultados confiables y válidos. Conclusiones : se concluye que la discusión presentada sobre la confiabilidad, responsividad e interpretabilidad contribuye a los profesionales de la salud en el conocimiento teórico y sentido crítico en la elección de instrumentos y en la conducción de análisis sobre esas propiedades de medida.

  6. VladBot. Robot para posicionamiento de medida

    OpenAIRE

    Plata Rueda, Ángel

    2013-01-01

    VladBot es un robot autónomo diseñado para posicionar en interiores un micrófono de medida. Este prototipo puede valorar la idea de automatizar medidas acústicas en interiores mediante un robot autónomo. Posee dos ruedas motrices y una rueda loca. Ésta rueda loca aporta maniobrabilidad al robot. Un soporte extensible hecho de aluminio sostiene el micrófono de medida. VladBot ha sido diseñado con tecnologías de bajo coste y bajo una plataforma abierta, Arduino. Arduino es una plataforma el...

  7. The fundamentals of stellar astrophysics

    International Nuclear Information System (INIS)

    Collins, G.W. II.

    1989-01-01

    A broad overview of theoretical stellar astrophysics is presented in a textbook intended for graduate students. Chapters are devoted to fundamental principles, assumptions, theorems, and polytropes; energy sources and sinks; the flow of energy through the star and the construction of stellar models; the theory of stellar evolution; relativistic stellar structure; the structure of distorted stars; stellar pulsation and oscillation. Also discussed are the flow of radiation through the stellar atmosphere, the solution of the radiative-transfer equation, the environment of the radiation field, the construction of a stellar model atmosphere, the formation and shape of spectral lines, LTE breakdown, illuminated and extended stellar atmospheres, and the transfer of polarized radiation. Diagrams, graphs, and sample problems are provided. 164 refs

  8. Študija primera: Volkswagnova afera Diesel-gate

    OpenAIRE

    Hočevar, Gregor

    2016-01-01

    Namen diplomskega dela je osredotočiti se na primer »Diesel-gate«, škandal z goljufanjem emisijskih testov, ki je izbruhnil lansko leto in v katerega je bil vpleten Volkswagen. Naš glavni cilj diplomskega dela je analizirati razloge za nastali škandal in preučiti posledice, ki jih Volkswagnovo ravnanje prinaša. Poleg same študije primera smo v diplomskem delu pozornost namenili tudi gospodarski kriminaliteti kot področju, kamor bi lahko uvrstili Volkswagnovo ravnanje, ter goljufijo oz. potroš...

  9. Carmen Dauset Moreno, primera musa del cine estadounidense

    OpenAIRE

    Mora Contreras, Francisco Javier

    2014-01-01

    Este artículo se propone analizar la importancia de la bailarina española Carmen Dauset Moreno para la historia del cine. Conocida en el mundo del vaudeville como Carmencita, fue la primera mujer que apareció en dos breves películas para kinetoscopio realizadas en el estudio de Edison en marzo de 1894. En este sentido, el artículo trata de contextualizar la aparición de la artista española en estas películas y plantea cuestiones sobre el significado de las mismas en el desarrollo de las fases...

  10. Progress Toward Attractive Stellarators

    International Nuclear Information System (INIS)

    Neilson, G.H.; Bromberg, L.; Brown, T.G.; Gates, D.A.; Ku, L.P.; Zarnstorff, M.C.; Boozer, A.H.; Harris, J.H.; Meneghini, O.; Mynick, H.E.; Pomphrey, N.; Reiman, A.H.; Xanthopoulos, P.

    2011-01-01

    The quasi-axisymmetric stellarator (QAS) concept offers a promising path to a more compact stellarator reactor, closer in linear dimensions to tokamak reactors than previous stellarator designs. Concept improvements are needed, however, to make it more maintainable and more compatible with high plant availability. Using the ARIES-CS design as a starting point, compact stellarator designs with improved maintenance characteristics have been developed. While the ARIES-CS features a through-the-port maintenance scheme, we have investigated configuration changes to enable a sector-maintenance approach, as envisioned for example in ARIES AT. Three approaches are reported. The first is to make tradeoffs within the QAS design space, giving greater emphasis to maintainability criteria. The second approach is to improve the optimization tools to more accurately and efficiently target the physics properties of importance. The third is to employ a hybrid coil topology, so that the plasma shaping functions of the main coils are shared more optimally, either with passive conductors made of high-temperature superconductor or with local compensation coils, allowing the main coils to become simpler. Optimization tools are being improved to test these approaches.

  11. Stellar population synthesis

    International Nuclear Information System (INIS)

    Pickles, A.J.

    1989-01-01

    The techniques used to derive astrophysically useful information from observations of the integrated light of composite stellar systems are briefly reviewed. A synthesis technique, designed to separate and describe on a standard system the competing effects of age and metallicity variations is introduced, and illustrated by its application to the study of the history of star formation in bright elliptical galaxies in clusters. (author)

  12. Relativistic stellar dynamics

    International Nuclear Information System (INIS)

    Contopoulos, G.

    1983-01-01

    In this paper, three main areas of relativistic stellar dynamics are reviewed: (a) The dynamics of clusters, or nuclei of galaxies, of very high density; (b) The dynamics of systems containing a massive black hole; and (c) The dynamics of particles (and photons) in an expanding Universe. The emphasis is on the use of orbit perturbations. (Auth.)

  13. Compact stellarator coils

    International Nuclear Information System (INIS)

    Pomphrey, N.; Berry, L.A.; Boozer, A.H.

    2001-01-01

    Experimental devices to study the physics of high-beta (β>∼4%), low aspect ratio (A<∼4.5) stellarator plasmas require coils that will produce plasmas satisfying a set of physics goals, provide experimental flexibility, and be practical to construct. In the course of designing a flexible coil set for the National Compact Stellarator Experiment, we have made several innovations that may be useful in future stellarator design efforts. These include: the use of Singular Value Decomposition methods for obtaining families of smooth current potentials on distant coil winding surfaces from which low current density solutions may be identified; the use of a Control Matrix Method for identifying which few of the many detailed elements of the stellarator boundary must be targeted if a coil set is to provide fields to control the essential physics of the plasma; the use of Genetic Algorithms for choosing an optimal set of discrete coils from a continuum of potential contours; the evaluation of alternate coil topologies for balancing the tradeoff between physics objective and engineering constraints; the development of a new coil optimization code for designing modular coils, and the identification of a 'natural' basis for describing current sheet distributions. (author)

  14. Stellar Structure and Evolution

    CERN Document Server

    Kippenhahn, Rudolf; Weiss, Achim

    2013-01-01

    This long-awaited second edition of the classical textbook on Stellar Structure and Evolution by Kippenhahn and Weigert is a thoroughly revised version of the original text. Taking into account modern observational constraints as well as additional physical effects such as mass loss and diffusion, Achim Weiss and Rudolf Kippenhahn have succeeded in bringing the book up to the state-of-the-art with respect to both the presentation of stellar physics and the presentation and interpretation of current sophisticated stellar models. The well-received and proven pedagogical approach of the first edition has been retained. The book provides a comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The models developed to explain the stability, dynamics and evolution of the stars are presented and great care is taken to detail the various stages in a star’s life. Just as the first edition, which remained a standard work for more than 20 years after its...

  15. 8. stellarator workshop

    International Nuclear Information System (INIS)

    1991-07-01

    The technical reports in this collection of papers were presented at the 8th International Workshop on Stellarators, and International Atomic Energy Agency Technical Committee Meeting. They include presentations on transport, magnetic configurations, fluctuations, equilibrium, stability, edge plasma and wall aspects, heating, diagnostics, new concepts and reactor studies. Refs, figs and tabs

  16. Stellar wind theory

    International Nuclear Information System (INIS)

    Summers, D.

    1980-01-01

    The theory of stellar winds as given by the equations of classical fluid dynamics is considered. The equations of momentum and energy describing a steady, spherically symmetric, heat-conducting, viscous stellar wind are cast in a dimensionless form which involves a thermal conduction parameter E and a viscosity parameter γ. An asymptotic analysis is carried out, for fixed γ, in the cases E→O and E→infinity (corresponding to small and large thermal conductivity, respectively), and it is found that it is possible to construct critical solutions for the wind velocity and temperature over the entire flow. The E→O solution represents a wind which emanates from the star at low, subsonic speeds, accelerates through a sonic point, and then approaches a constant asymptotic speed, with its temperature varying as r/sup -4/3/ at large distances r from the star; the E→infinity solution represents a wind which, after reaching an approximately constant speed, with temperature varying as r/sup -2/7/, decelerates through a diffuse shock and approaches a finite pressure at infinity. A categorization is made of all critical stellar wind solutions for given values of γ and E, and actual numerical examples are given. Numerical solutions are obtained by integrating upstream 'from infinity' from initial values of the flow parameters given by appropriate asymptotic expansions. The role of viscosity in stellar wind theory is discussed, viscous and inviscid stellar wind solutions are compared, and it is suggested that with certain limitations, the theory presented may be useful in analyzing winds from solar-type stars

  17. Medida de similitud basada en saliencia

    Directory of Open Access Journals (Sweden)

    Sergio Domínguez

    2012-10-01

    quantifying saliency of feature values, for combining them during a comparison process and, eventually, to weight that feature attending to the result of the combination, are introduced as well. The results for the evaluation of this similarity measure in an image based content retrieval task are presented, as well as their comparison with those obtained using euclidean distance in the same task. Both are validated by volunteers who labelled the retrieved sets. Palabras clave: Bases de datos de imágenes, recuperación basada en contenido, medidas de similitud, modelos perceptuales, análisis de imágenes, Keywords: Image databases, content based retrieval, similarity measures, perceptual models, image analysis

  18. Ion transport in stellarators

    International Nuclear Information System (INIS)

    Ho, D.D.M.; Kulsrud, R.M.

    1985-09-01

    Stellarator ion transport in the low-collisionality regime with a radial electric field is calculated by a systematic expansion of the drift-Boltzmann equation. The shape of the helical well is taken into account in this calculation. It is found that the barely trapped ions with three to four times the thermal energy give the dominant contribution to the diffusion. Expressions for the ion particle and energy fluxes are derived

  19. Violencia de género en el ámbito universitario. Medidas para su superación.

    Directory of Open Access Journals (Sweden)

    Consol Aguilar Ródenas

    2009-01-01

    Full Text Available Este artículo expone parte de los resultados de la primera investigación sobre violencia de género en las universidades españolas. A partir de la revisión de investigaciones internacionales, mostramos que la violencia de género tiene una presencia importante en las universidades. Posteriormente, identificamos medidas para la prevención y superación de la violencia de género que ya se están desarrollando en algunas de las universidades de más prestigio internacional. Ambos aspectos son el punto de partida para el estudio de la violencia de género en las universidades españolas y para el diseño de medidas que contribuyan a su superación.---------------------------------------------------------------------This article contains some of the results from the first research on gender violence in Spanish universities. Based on a review of international research, we demonstrate that gender violence is prevalent in universities. Subsequently, we identify measures to prevent and overcome gender violence which are already being developed in some of the most prestigious international universities. Both of these aspects are the starting off point to study gender violence in Spanish universities and to design measures which contribute towards overcoming it.

  20. Status of stellarator research

    International Nuclear Information System (INIS)

    Wobig, H.

    1985-01-01

    In recent years main activities in stellarator research were focussed on production and investigation of currentless plasmas. Several heating methods have been applied: electron cyclotron heating, ion cyclotron heating and neutral beam injection. The parameters achieved in HELIOTRON E and W VII-A are: antin 20 m 3 , Tsub(i) <= 1 keV. The confinement is improved as compared with ohmically heated discharges. By ECRH (P = 200 kW) it is possible to heat electrons up to 1.4 keV, confinement in this regime is dominated already by trapped particle effects. Toroidal currents up to 2 kA - either bootstrap currents or externally driven currents - were observed. High β-values (antiβ = 2%) have been obtained in HELIOTRON E, in this regime already pressure driven MHD-modes were observed. Future experiments (ATF-1 and W VII-AS) will extend the parameter regime to temperatures of several keV. These experiments will give important information about critical problems of the stellarator line (β-limit, neoclassical confinement impurity transport). A few reactor studies of stellarators exist, attention is mainly concentrated on technical problems of the modular coil system

  1. LA PRIMERA MODERNIZACION DE LA CAFICULTURA COSTARRICENSE (1890-1950.

    Directory of Open Access Journals (Sweden)

    Carlos Naranjo Gutiérrez

    2011-08-01

    Full Text Available En el curso de las dos últimas décadas en nuestro país vienen presentándose con frecuencia, una serie de solventes trabajos realizados por un sinnúmero de investigadores de diversas disciplinas de las ciencias sociales relacionados con la historia agraria. Desde diferentes enfoques, nos han permitido aproximarnos más de cerca a la evolución del agro costarricense. Sin embargo, a pesar de estos indiscutibles adelantos, continúan existiendo grandes disparidades entre los temas.Dados estos precedentes nuestro estudio va a tratar de ubicarse al otro lado de la ribera, pues el propósito central es revelar que los cafetales de la primera mitad del siglo XX experimentaron profundas renovaciones técnicas.

  2. LA PRIMERA MODERNIZACION DE LA CAFICULTURA COSTARRICENSE (1890-1950.

    Directory of Open Access Journals (Sweden)

    Carlos Naranjo Gutiérrez

    1999-07-01

    Full Text Available En el curso de las dos últimas décadas en nuestro país vienen presentándose con frecuencia, una serie de solventes trabajos realizados por un sinnúmero de investigadores de diversas disciplinas de las ciencias sociales relacionados con la historia agraria. Desde diferentes enfoques, nos han permitido aproximarnos más de cerca a la evolución del agro costarricense. Sin embargo, a pesar de estos indiscutibles adelantos, continúan existiendo grandes disparidades entre los temas.Dados estos precedentes nuestro estudio va a tratar de ubicarse al otro lado de la ribera, pues el propósito central es revelar que los cafetales de la primera mitad del siglo XX experimentaron profundas renovaciones técnicas.

  3. Estudio definitivo de la derivación a Lima de las aguas de la cuenca alta del río Mantaro (Primera fase): informe final

    OpenAIRE

    Ministerio de Vivienda y Construcción; Proyecto Transvase Mantaro; Binnie & Partners

    1981-01-01

    Contiene la primera fase del estudio final de derivación de agua a Lima desde la cuenca superior del Río Mantaro, abarcando tópicos tales como los costos del control de la contaminación en el Río Mantaro y la medida en que podría utilizarse el agua subterránea en los valles de los Ríos Rímac, Chillón y Lurín. Este estudio tiene como objetivo principal la preparación de un Plan Integral que comprenda un plan de desarrollo que satisfaga la demanda de agua para uso urbano y agrícola en la Gra...

  4. Evaluación de anemia ferropénica en la primera infancia del Municipio de Sonsón-Antioquia, 2007

    OpenAIRE

    Castillo Salgado, Tulia Isabel; Pérez Escobar, Rocío

    2014-01-01

    Objetivo: Determinar la prevalencia de anemia por deficiencia de hierro en niños de la primera infancia del municipio de Sonsón – Antioquia, en el año 2007. Metodología: Se realizó un estudio descriptivo transversal en 391 niños de 0 a 84 meses de edad del Municipio de Sonsón, Antioquia. Se estudiaron los parámetros de hemoglobina y ferritina sérica utilizando puntos de corte de la Organización Mundial de la Salud (OMS). Se calcularon las medidas de frecuencia y de resumen y los intervalos de...

  5. Mutaciones de los usos del agua en la agricultura española durante la primera década del siglo XXI

    Directory of Open Access Journals (Sweden)

    Alfredo Morales Gil

    2010-01-01

    Full Text Available El análisis de la dinámica de cambio de los regadíos españoles en la primera década del siglo XXI es el objetivo de esta investigación. Éstos se caracterizan, grosso modo, por un continuo incremento de la superficie y la implantación de la modalidad de riego localizado. Éste aumento, a diferencia de décadas anteriores, se debe en gran medida a la expansión que han registrado las superficies ocupadas por olivar, viñedo y algunos cereales, cultivos tradicionalmente de secano, en comarcas que, con anterioridad a estas fechas, no tenían tradición en las prácticas del regadío, frente a la atonía de aprovechamientos como hortalizas o ciertos frutales.

  6. Entre leyes y votos. La legislación electoral en la Nueva Granada durante la primera mitad del siglo XIX

    Directory of Open Access Journals (Sweden)

    Edwin Andrés Monsalvo Mendoza

    2012-07-01

    Full Text Available El presente artículo muestra —a partir del análisis de las normas electorales compiladas en la Codificación Nacional—, el papel que jugó la legislación electoral colombiana en los comicios durante la primera mitad de siglo XIX. El interés principal se centra en la descripción y análisis de los requisitos para ser sufragante y elector, el desarrollo de las elecciones parroquiales, las transgresiones a las normas y el papel de los jueces durante los comicios. Nuestra hipótesis es que las normas se iban construyendo en la medida que las prácticas electorales hacían necesario su regulación.

  7. THE ADVANCED STELLAR COMPASS

    DEFF Research Database (Denmark)

    Jørgensen, John Leif; Liebe, Carl Christian

    1997-01-01

    The science objective of the Danish Geomagnetic Research Satellite "Ørsted" is to map the magnetic field of the Earth, with a vector precision of a fraction of a nanotesla. This necessitates an attitude reference instrument with a precision of a few arcseconds onboard the satellite. To meet...... this demand the Advanced Stellar Compass (ASC), a fully autonomous miniature star tracker, was developed. This ASC is capable of both solving the "lost in space" problem and determine the attitude with arcseconds precision. The development, principles of operation and instrument autonomy of the ASC...

  8. Physics of Stellar Convection

    Science.gov (United States)

    Arnett, W. David

    2009-05-01

    We review recent progress using numerical simulations as a testbed for development of a theory of stellar convection, much as envisaged by John von Newmann. Necessary features of the theory, non-locality and fluctuations, are illustrated by computer movies. It is found that the common approximation of convection as a diffusive process presents the wrong physical picture, and improvements are suggested. New observational results discussed at the conference are gratifying in their validation of some of our theoretical ideas, especially the idea that SNIb and SNIc events are related to the explosion of massive star cores which have been stripped by mass loss and binary interactions [1

  9. Aprestamiento: saberes y prácticas de una experiencia en educación musical para la primera infancia

    Directory of Open Access Journals (Sweden)

    María Teresa Martínez Azcárate

    2016-06-01

    Full Text Available En este artículo se muestra el resultado de la sistematización de la experiencia en educación musical para la primera infancia, denominada aprestamiento, desarrollada en el Taller de Música. Consiste en una propuesta surgida desde la pedagogía musical, estructurada en 6 componentes de clases que organizan y estructuran los contenidos, para favorecer aspectos del desarrollo de niños entre 2 y 5 años, época en la cual el estímulo recibido contribuye a facilitar los procesos de iniciación a la lectoescritura musical y la práctica instrumental. La experiencia realizada por la maestra María Teresa Martínez, reconocida en el medio pedagógico musical como “Pitti Martinez”, refleja la comprensión adquirida a lo largo de los años sobre la importancia de la música en los procesos de desarrollo físico, emocional, cognitivo y social de los niños, con el fin de aportar a su presente y a su futuro, y de esta forma contribuir en alguna medida a una sociedad más amable.

  10. Medida de espessura de filmes finos com interferometro de haidinger

    OpenAIRE

    Elisabeth Andreoli de Oliveira

    1987-01-01

    Resumo: Apresentamos um método não destrutivo para medida de espessura de filmes finos transparentes depositados em substratos transparentes, usando um interferômetro de Haidinger. A partir das frações de interferência, medidas para vários comprimentos de onda, e do índice de refração para um único comprimento de onda, determinamos a espessura do filme e sua dispersão cromática, através de um procedimento analítico-numérico Abstract: We introduce a non-destructive method for the thickness ...

  11. Stellar axion models

    Energy Technology Data Exchange (ETDEWEB)

    Nowakowski, Daniel; Kuster, Markus; Meister, Claudia V.; Fuelbert, Florian; Hoffmann, Dieter H.H. [TU Darmstadt (Germany). Institut fuer Kernphysik; Weiss, Achim [Max-Planck-Institut fuer Astrophysik, Garching (Germany)

    2010-07-01

    An axion helioscope is typically operated to observe the sun as an axion source. Additional pointings at celestial sources, e.g. stars in other galaxies, result in possible detections of axions from distant galactic objects. For the observation of supplementary axion sources we therefore calculate the thereotical axion flux from distant stars by extending axionic flux models for the axion Primakoff effect in the sun to other main sequence stars. The main sequence star models used for our calculations are based on full stellar structure calculations. To deduce the effective axion flux of stellar objects incident on the Earth the All-Sky catalogue was used to obtain the spectral class and distance of the stars treated. Our calculations of the axion flux in the galactic plane show that for a zero age main sequence star an maximum axion flux of {phi}{sub a}=303.43 cm{sup -2}s{sup -1} could be expected. Furthermore we present estimates of axion fluxes from time-evolved stars.

  12. The DEMO Quasisymmetric Stellarator

    Directory of Open Access Journals (Sweden)

    Geoffrey B. McFadden

    2010-02-01

    Full Text Available The NSTAB nonlinear stability code solves differential equations in conservation form, and the TRAN Monte Carlo test particle code tracks guiding center orbits in a fixed background, to provide simulations of equilibrium, stability, and transport in tokamaks and stellarators. These codes are well correlated with experimental observations and have been validated by convergence studies. Bifurcated 3D solutions of the 2D tokamak problem have been calculated that model persistent disruptions, neoclassical tearing modes (NTMs and edge localized modes (ELMs occurring in the International Thermonuclear Experimental Reactor (ITER, which does not pass the NSTAB simulation test for nonlinear stability. So we have designed a quasiaxially symmetric (QAS stellarator with similar proportions as a candidate for the demonstration (DEMO fusion reactor that does pass the test [1]. The configuration has two field periods and an exceptionally accurate 2D symmetry that furnishes excellent thermal confinement and good control of the prompt loss of alpha particles. Robust coils are found from a filtered form of the Biot-Savart law based on a distribution of current over a control surface for the coils and the current in the plasma defined by the equilibrium calculation. Computational science has addressed the issues of equilibrium, stability, and transport, so it remains to develop an effective plan to construct the coils and build a diverter.

  13. Crisis financiera global y la emergencia de nuevas arquitecturas financieras para el desarrollo (primera parte

    Directory of Open Access Journals (Sweden)

    Ilene Grabel

    2012-09-01

    Full Text Available La crisis actual está resultando productiva en cuanto a experimentación institucional, en el debate y puesta en práctica de arquitecturas financieras del mundo en desarrollo. El empuje hacia tal experimentación surgió desde la crisis financiera de Asia del Este de 1997-98, la cual provocó que algunos países en desarrollo tomaran medidas para protegerse de turbulencias futuras, sanciones del Fondo Monetario Internacional (FMI, y la intromisión en su espacio de decisiones políticas. En este trabajo se argumenta que hay claras y diversas indicaciones que la arquitectura financiera global ahora está evolucionando de manera que contribuye a una nueva heterogeneidad institucional. En algunas innovaciones institucionales y políticas se ve la emergencia de una arquitectura financiera que está mucho menos ligada a los Estados Unidos (US y al FMI, que había sido lo normal en las ultimas décadas. Además, el creciente poder económico, la autoestima y el protagonismo de quienes formulan las políticas económicas en algunos países en desarrollo (y al mismo tiempo, la incertidumbre correspondiente acerca de las economías de US y Europa están trastornando los modos tradicionales de gobernabilidad financiera y dispersando el poder a lo largo del sistema financiero global. La presente entrega es una versión actualizada de la presentada en marzo 2012, preparada como un Background Paper para el Informe sobre Desarrollo Humando, 2012, A Changing World and the Rise of the Global South. Agradezco el Programa de las Naciones Unidas para el Desarrollo por su apoyo a esta investigación; la cual se benefició de los comentarios de George DeMartino y la ayuda de investigación ejemplar de Ryan Economy, Ann Job, and Art Chambers. La traducción al español estuvo a cargo de Wesley Marshall y Eugenia Correa. Ola Financiera presenta la primera parte en este número; la segunda parte aparecerá en Ola Financiera Número 13 (enero-abril de 2013.

  14. Proceso experiencial: comprendiendo al ser humano en primera persona

    Directory of Open Access Journals (Sweden)

    Alberto De Castro

    2012-01-01

    Full Text Available Este es un artículo de revisión y reflexión teórica acerca de los fundamentos psicológicos del proceso experiencial de los seres humanos. Este artículo nació de la necesidad de situar en primera persona la participación y postura psicológica que los seres humanos asumen en la vida cotidiana a partir de los significados, valores e intenciones que tratan de afirmar ante las distintas experiencias, situaciones y determinismos que enfrentan. A partir de la revisión de distintos autores contemporáneos, de conclusiones basadas en experiencia clínica y de los resultados de distintas investigaciones fenomenológicas hermenéuticas, se concluye que el proceso experiencial implica y está caracterizado por la interrelación entre los conceptos de deseo, voluntad, sentido, valoración, consciencia e intencionalidad.

  15. Referéndum en Costa Rica: la primera experiencia

    Directory of Open Access Journals (Sweden)

    Max Alberto Esquivel Faerron

    2008-07-01

    Full Text Available El artículo aborda los distintos mecanismos de democracia directa regulados en el ordenamiento jurídico costarricense, profundizando en el instituto del referéndum. Se centra en analizar, con apoyo en datos estadísticos, la primera experiencia de la aplicación del referéndum en Costa Rica, relativo a la aprobación del Tratado de Libre Comercio entre República Dominicana, Centroamérica y Estados Unidos. Como parte de este estudio, el autor desarrolla, desde el punto de vista doctrinario y de derecho comparado, temas medulares del referéndum que fueron motivo de amplia discusión, tales como: el carácter excepcional de este instituto -contra poniéndolo con el listado de las solicitudes de recolección de firmas presentadas ante el Tribunal-, la fiscalización del proceso, la posición del Poder Ejecutivo a favor de una de las tesis en contienda, el financiamiento de las campañas propagandísticas, la información ciudadana sobre el tema de la consulta y la participación de los medios de comunicación.

  16. A catalog of stellar spectrophotometry

    Science.gov (United States)

    Adelman, S. J.; Pyper, D. M.; Shore, S. N.; White, R. E.; Warren, W. H., Jr.

    1989-01-01

    A machine-readable catalog of stellar spectrophotometric measurements made with rotating grating scanner is introduced. Consideration is given to the processes by which the stellar data were collected and calibrated with the fluxes of Vega (Hayes and Latham, 1975). A sample page from the spectrophotometric catalog is presented.

  17. Quasisymmetry equations for conventional stellarators

    International Nuclear Information System (INIS)

    Pustovitov, V.D.

    1994-11-01

    General quasisymmetry condition, which demands the independence of B 2 on one of the angular Boozer coordinates, is reduced to two equations containing only geometrical characteristics and helical field of a stellarator. The analysis is performed for conventional stellarators with a planar circular axis using standard stellarator expansion. As a basis, the invariant quasisymmetry condition is used. The quasisymmetry equations for stellarators are obtained from this condition also in an invariant form. Simplified analogs of these equations are given for the case when averaged magnetic surfaces are circular shifted torii. It is shown that quasisymmetry condition can be satisfied, in principle, in a conventional stellarator by a proper choice of two satellite harmonics of the helical field in addition to the main harmonic. Besides, there appears a restriction on the shift of magnetic surfaces. Thus, in general, the problem is closely related with that of self-consistent description of a configuration. (author)

  18. Monitoreo neurointensivo en pediatría (III: Tratamiento. Medidas generales

    Directory of Open Access Journals (Sweden)

    Eduardo M. Pleguezuelo Rodríguez

    2001-06-01

    Full Text Available Se informa que con el neuromonitoreo y el manejo intensivo del traumatismo craneoencefálico grave, se han identificado un grupo de fenómenos fisiopatológicos diferentes, los cuales requieren de medidas disímiles y específicas para cada paciente, lo que hace más racional el tratamiento de ellos. De la misma manera esto ha propiciado que cambien radicalmente las concepciones acerca de antiguos patrones terapéuticos establecidos durante muchos años; ejemplo de esto es el cambio en la reposición hídrica de ellos, los cuales antes se mantenían sobre una vertiente seca y hoy se preconiza la euvolemia estricta, la sustitución de la hiperventilación de rutina por la ventilación optimizada, cambios en la política del uso de agentes osmóticos, la terapia barbitúrica y la craneotomía descompresiva en casos de hipertensión intracraneal refractaria a medidas terapéuticas convencionales. En este trabajo se hace una revisión actualizada de las principales medidas terapéuticas utilizadas en estos pacientes, acorde con lo que plantean los lineamientos para el tratamiento del traumatismo craneal grave de la Asociación Americana de Cirujanos Neurológicos y los del consorcio europeo para la lesión cerebral. Las medidas terapéuticas utilizadas en estos pacientes se dividen en 2 fases. En este tercer trabajo de actualización se aborda el manejo de la primera fase que corresponde a la estabilización urgente inicial antes de establecer la medición de la presión intracraneal (PIC, así como las medidas generales de la segunda fase una vez iniciado el monitoreo de la PIC. Principios terapéuticos que desde hace algunos años se vienen utilizando en el Hospital provincial General y el Hospital Pediátrico Provincial Docente de Camagüey para el manejo del trauma craneal grave, los cuales se basan en medidas iniciales en la recepción, acorde con lo que plantean los principios del soporte vital avanzado en trauma para la reanimaci

  19. Nucleosynthesis in stellar explosions

    Energy Technology Data Exchange (ETDEWEB)

    Woosley, S.E.; Axelrod, T.S.; Weaver, T.A.

    1983-01-01

    The final evolution and explosion of stars from 10 M/sub solar/ to 10/sup 6/ M/sub solar/ are reviewed with emphasis on factors affecting the expected nucleosynthesis. We order our paper in a sequence of decreasing mass. If, as many suspect, the stellar birth function was peaked towards larger masses at earlier times (see e.g., Silk 1977; but also see Palla, Salpeter, and Stahler 1983), this sequence of masses might also be regarded as a temporal sequence. At each stage of Galactic chemical evolution stars form from the ashes of preceding generations which typically had greater mass. A wide variety of Type I supernova models, most based upon accreting white dwarf stars, are also explored using the expected light curves, spectra, and nucleosynthesis as diagnostics. No clearly favored Type I model emerges that is capable of simultaneously satisfying all three constraints.

  20. Nucleosynthesis in stellar explosions

    International Nuclear Information System (INIS)

    Woosley, S.E.; Axelrod, T.S.; Weaver, T.A.

    1983-01-01

    The final evolution and explosion of stars from 10 M/sub solar/ to 10 6 M/sub solar/ are reviewed with emphasis on factors affecting the expected nucleosynthesis. We order our paper in a sequence of decreasing mass. If, as many suspect, the stellar birth function was peaked towards larger masses at earlier times (see e.g., Silk 1977; but also see Palla, Salpeter, and Stahler 1983), this sequence of masses might also be regarded as a temporal sequence. At each stage of Galactic chemical evolution stars form from the ashes of preceding generations which typically had greater mass. A wide variety of Type I supernova models, most based upon accreting white dwarf stars, are also explored using the expected light curves, spectra, and nucleosynthesis as diagnostics. No clearly favored Type I model emerges that is capable of simultaneously satisfying all three constraints

  1. Remarks on stellar clusters

    International Nuclear Information System (INIS)

    Teller, E.

    1985-01-01

    In the following, a few simple remarks on the evolution and properties of stellar clusters will be collected. In particular, globular clusters will be considered. Though details of such clusters are often not known, a few questions can be clarified with the help of primitive arguments. These are:- why are spherical clusters spherical, why do they have high densities, why do they consist of approximately a million stars, how may a black hole of great mass form within them, may they be the origin of gamma-ray bursts, may their invisible remnants account for the missing mass of our galaxy. The available data do not warrant a detailed evaluation. However, it is remarkable that exceedingly simple models can shed some light on the questions enumerated above. (author)

  2. L = ± 1 stellarator

    International Nuclear Information System (INIS)

    Kikuchi, T.; Shiina, S.; Saito, K.; Gesso, H.; Aizawa, M.; Kawakami, I.

    1985-01-01

    We report the magnetic field configuration of helical magnetic axis stellarator. The magnetic field configuration is composed of large l=1 field and small l=-1 and l=0(bumpy) fields. The large l=1 field (combined with the small l=-1 field) is used to form helical magnetic axis with the helical curvature much larger than the toroidal curvature, which provides the high limiting values of β. The small l=-1 field, furthermore, as well as the large l=1 field reduces the Pfirsch-Schlueter currents by combining with l=0 field. Therefore, the large l=1 field and the combination of three field components may be favourable for the increase of limiting β value

  3. Evolution of stellar systems

    International Nuclear Information System (INIS)

    Vader, P.

    1981-01-01

    The stellar systems of which the evolution will be considered in this thesis, are either galaxies, which contain about 10 11 stars, or binary systems, which consist of only two stars. It is seen that binary systems can give us some insight into the relative age of the nucleus of M31. The positive correlation between the metal content of a galaxy and its mass, first noted for elliptical galaxies, seems to be a general property of galaxies of all types. The observed increase of metallicity with galaxy mass is too large to be accounted for by differences in the evolutionary stage of galaxies. To explain the observed correlation it is proposed that a relatively larger proportion of massive stars is formed in more massive galaxies. The physical basis is that the formation of massive stars seems to be tied to the enhanced gas-dynamical activity in more massive galaxies. A specific aspect of the production of heavy elements by massive stars is investigated in some detail. In 1979 a cluster of 18 point X-ray sources within 400 pc of the centre of M31 was detected with the Einstein satellite. This is a remarkable result since no equivalent of this cluster has been observed in the nucleus of our own Galaxy, which otherwise is very similar to that of M31. An explanation for this phenomenon is proposed, suggesting that X-ray binaries are the products of the long-term evolution of nova systems. (Auth.)

  4. Stellar extreme ultraviolet astronomy

    International Nuclear Information System (INIS)

    Cash, W.C. Jr.

    1978-01-01

    The design, calibration, and launch of a rocket-borne imaging telescope for extreme ultraviolet astronomy are described. The telescope, which employed diamond-turned grazing incidence optics and a ranicon detector, was launched November 19, 1976, from the White Sands Missile Range. The telescope performed well and returned data on several potential stellar sources of extreme ultraviolet radiation. Upper limits ten to twenty times more sensitive than previously available were obtained for the extreme ultraviolet flux from the white dwarf Sirius B. These limits fall a factor of seven below the flux predicted for the star and demonstrate that the temperature of Sirius B is not 32,000 K as previously measured, but is below 30,000 K. The new upper limits also rule out the photosphere of the white dwarf as the source of the recently reported soft x-rays from Sirius. Two other white dwarf stars, Feige 24 and G191-B2B, were observed. Upper limits on the flux at 300 A were interpreted as lower limits on the interstellar hydrogen column densities to these stars. The lower limits indicate interstellar hydrogen densitites of greater than .02 cm -3 . Four nearby stars (Sirius, Procyon, Capella, and Mirzam) were observed in a search for intense low temperature coronae or extended chromospheres. No extreme ultraviolet radiation from these stars was detected, and upper limits to their coronal emisson measures are derived

  5. Mapping stellar surface features

    International Nuclear Information System (INIS)

    Noah, P.V.

    1987-01-01

    New photometric and spectroscopic observations of the RS Canum Venaticorum binaries Sigma Geminorum and UX Arietis are reported along with details of the Doppler-imaging program SPOTPROF. The observations suggest that the starspot activity on Sigma Gem has decreased to 0.05 magnitude in two years. A photometric spot model for September 1984 to January 1985 found that a single spot covering 2% of the surface and 1000 K cooler than the surrounding photosphere could model the light variations. Equivalent-width observations contemporaneous with the photometric observations did not show any significant variations. Line-profile models from SPOTPROF predict that the variation of the equivalent width of the 6393 A Fe I line should be ∼ 1mA. Photometric observations of UX Ari from January 1984 to March 1985 show an 0.3 magnitude variation indicating a large spot group must cover the surface. Contemporaneous spectroscopic observations show asymmetric line profiles. The Doppler imaging and the photometric light-curve models were used in an iterative method to describe the stellar surface-spot distribution and successfully model both the photometric and the spectroscopic variations

  6. SI: The Stellar Imager

    Science.gov (United States)

    Carpenter, Kenneth G.; Schrijver, Carolus J.; Karovska, Margarita

    2006-01-01

    The ultra-sharp images of the Stellar Imager (SI) will revolutionize our view of many dynamic astrophysical processes: The 0.1 milliarcsec resolution of this deep-space telescope will transform point sources into extended sources, and simple snapshots into spellbinding evolving views. SI s science focuses on the role of magnetism in the Universe, particularly on magnetic activity on the surfaces of stars like the Sun. SI s prime goal is to enable long-term forecasting of solar activity and the space weather that it drives in support of the Living With a Star program in the Exploration Era by imaging a sample of magnetically active stars with enough resolution to map their evolving dynamo patterns and their internal flows. By exploring the Universe at ultra-high resolution, SI will also revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magnetohydrodynamically controlled structures and processes in the Universe.

  7. Stellar Presentations (Abstract)

    Science.gov (United States)

    Young, D.

    2015-12-01

    (Abstract only) The AAVSO is in the process of expanding its education, outreach and speakers bureau program. powerpoint presentations prepared for specific target audiences such as AAVSO members, educators, students, the general public, and Science Olympiad teams, coaches, event supervisors, and state directors will be available online for members to use. The presentations range from specific and general content relating to stellar evolution and variable stars to specific activities for a workshop environment. A presentation—even with a general topic—that works for high school students will not work for educators, Science Olympiad teams, or the general public. Each audience is unique and requires a different approach. The current environment necessitates presentations that are captivating for a younger generation that is embedded in a highly visual and sound-bite world of social media, twitter and U-Tube, and mobile devices. For educators, presentations and workshops for themselves and their students must support the Next Generation Science Standards (NGSS), the Common Core Content Standards, and the Science Technology, Engineering and Mathematics (STEM) initiative. Current best practices for developing relevant and engaging powerpoint presentations to deliver information to a variety of targeted audiences will be presented along with several examples.

  8. El trabajo en Smith: valor o medida del valor?

    Directory of Open Access Journals (Sweden)

    Adolfo Rodríguez Herrera

    2016-12-01

    Este artículo revisa los conceptos desarrollados por Smith para formular su teoría del valor (valor, precio real y valor de  cambio. Nuestra interpretación de sus textos sobre el valor no coincide con la que tradicionalmente se ha hecho. De acuerdo con nuestra interpretación, no sería correcta la crítica de Ricardo y Marx a la posición de Smith sobre el papel del trabajo como medida de valor. Para estos autores, Smith no es consistente al proponer que el valor de una mercancía es definido o medido como la cantidad de trabajo necesaria para producirla y simultáneamente como la cantidad de trabajo que puede ser comprada por esta mercancía. Tratamos de demostrar que para Smith el trabajo tiene un doble papel –como fuente y como medida del valor–, y que a ello se debe la confusión generada por su uso de algunos términos: Smith propone el trabajo como una medida de valor porque lo concibe como una fuente de valor. Con esta interpretación queda claro, paradójicamente, que la teoría del valor trabajo de Smith corresponde sustancialmente con la que más tarde desarrollarán Ricardo y Marx.

  9. Turbulence optimisation in stellarator experiments

    Energy Technology Data Exchange (ETDEWEB)

    Proll, Josefine H.E. [Max-Planck/Princeton Center for Plasma Physics (Germany); Max-Planck-Institut fuer Plasmaphysik, Wendelsteinstr. 1, 17491 Greifswald (Germany); Faber, Benjamin J. [HSX Plasma Laboratory, University of Wisconsin-Madison, Madison, WI 53706 (United States); Helander, Per; Xanthopoulos, Pavlos [Max-Planck/Princeton Center for Plasma Physics (Germany); Lazerson, Samuel A.; Mynick, Harry E. [Plasma Physics Laboratory, Princeton University, P.O. Box 451 Princeton, New Jersey 08543-0451 (United States)

    2015-05-01

    Stellarators, the twisted siblings of the axisymmetric fusion experiments called tokamaks, have historically suffered from confining the heat of the plasma insufficiently compared with tokamaks and were therefore considered to be less promising candidates for a fusion reactor. This has changed, however, with the advent of stellarators in which the laminar transport is reduced to levels below that of tokamaks by shaping the magnetic field accordingly. As in tokamaks, the turbulent transport remains as the now dominant transport channel. Recent analytical theory suggests that the large configuration space of stellarators allows for an additional optimisation of the magnetic field to also reduce the turbulent transport. In this talk, the idea behind the turbulence optimisation is explained. We also present how an optimised equilibrium is obtained and how it might differ from the equilibrium field of an already existing device, and we compare experimental turbulence measurements in different configurations of the HSX stellarator in order to test the optimisation procedure.

  10. Optimizing Stellarators for Turbulent Transport

    International Nuclear Information System (INIS)

    Mynick, H.E.; Pomphrey, N.; Xanthopoulos, P.

    2010-01-01

    Up to now, the term 'transport-optimized' stellarators has meant optimized to minimize neoclassical transport, while the task of also mitigating turbulent transport, usually the dominant transport channel in such designs, has not been addressed, due to the complexity of plasma turbulence in stellarators. Here, we demonstrate that stellarators can also be designed to mitigate their turbulent transport, by making use of two powerful numerical tools not available until recently, namely gyrokinetic codes valid for 3D nonlinear simulations, and stellarator optimization codes. A first proof-of-principle configuration is obtained, reducing the level of ion temperature gradient turbulent transport from the NCSX baseline design by a factor of about 2.5.

  11. Stellar magnetic activity and exoplanets

    Directory of Open Access Journals (Sweden)

    Vidotto A.A.

    2017-01-01

    Full Text Available It has been proposed that magnetic activity could be enhanced due to interactions between close-in massive planets and their host stars. In this article, I present a brief overview of the connection between stellar magnetic activity and exoplanets. Stellar activity can be probed in chromospheric lines, coronal emission, surface spot coverage, etc. Since these are manifestations of stellar magnetism, these measurements are often used as proxies for the magnetic field of stars. Here, instead of focusing on the magnetic proxies, I overview some recent results of magnetic field measurements using spectropolarimetric observations. Firstly, I discuss the general trends found between large-scale magnetism, stellar rotation, and coronal emission and show that magnetism seems to be correlated to the internal structure of the star. Secondly, I overview some works that show evidence that exoplanets could (or not act as to enhance the activity of their host stars.

  12. Geological prospecting in La Primera area (Caballo Torcido) Fotoplano M-25 Mal Abrigo San Jose town

    International Nuclear Information System (INIS)

    Coronel, N.; Techera, J.; Pias, J.; Ramos, E.; De Souza, S.

    1990-01-01

    This work describes the prospection results in La Primera (Caballo Torcido) area in San Jose town. In this zone has been extracted metallic minerals, sediments and multielement soil samples to detect geochemical anomalies.

  13. Superbanana orbits in stellarator geometries

    International Nuclear Information System (INIS)

    Derr, J.A.; Shohet, J.L.

    1979-04-01

    The presence of superbanana orbit types localized to either the interior or the exterior of stellarators and torsatrons is numerically investigated for 3.5 MeV alpha particles. The absence of the interior superbanana in both geometries is found to be due to non-conservation of the action. Exterior superbananas are found in the stellarator only, as a consequence of the existence of closed helical magnetic wells. No superbananas of either type are found in the torsatron

  14. On origin of stellar clusters

    International Nuclear Information System (INIS)

    Tovmasyan, G.M.

    1977-01-01

    The ratios of the gas component of the mass of young stellar clusters to their stellar mass are considered. They change by more than four orders from one cluster to another. The results are in direct contradiction with the hypothesis of formation of cluster stars from a preliminarily existing gas cloud by its condensation, and they favour the Ambartsumian hypothesis of the joint origin of stars and gas clouds from superdense protostellar matter

  15. El logos en el De incarnatione Verbi de Atanasio: Una primera aproximación

    Directory of Open Access Journals (Sweden)

    Sergio Zañartu

    2007-01-01

    Full Text Available El autor, apoyado en el uso de múltiples vocablos, nos ofrece una aproximación al Logos en el De incarnatione Verbi de Atanasio, sin descuidar su conexión con el Contra Gentes. Las dos causas principales de la Encarnación son: la victoria sobre la muerte y la reconstitución del hombre según la imagen. Respecto a la primera, además del pago sacrificial de la deuda, destaca sobre todo que la vida desplaza a la muerte, que estaba entrelazada con el cuerpo, porque el Logos es la El cuerpo de Cristo pasa de incorruptible a inmortal en la resurrección, lo que se extiende a todos, dada la semejanza del cuerpo del Logos con el nuestro. Respecto a la segunda causa, el hombre es reconstruido según la imagen, porque en el cuerpo de Cristo está la misma imagen del Padre, que es el Logos, quien, mediante sus obras, nos vuelve a enseñar sobre el Padre. Porque ser según la imagen, es conocer a Dios. Estas obras del Logos encarnado incluyen, en buena medida, la derrota de los griegos idolátricos, y del judaismo que tenía la promesa, por el cristianismo. Atanasio nos presenta, pues, una esplendorosa teología del Logos Dios, creador (providente y salvador, pero pasa en silencio el alma de JesúsThe author of this article, supported by the utilization of multiple terms, offers us an approximation to the concept of Logos in De incarnatione Verbi of Athanasius, without discarding its connection with Contra Gentes. The two principal causes of the Incarnation are: the victory over death, and the reconstitution of man according the image. Regarding the first, apart from the sacrificial payment of debt, it highlights above all the fact that life displaces death, which was interlinked with the body, because the Logos is the The body of Christ passes from the incorruptible to the immortal in the Resurrection, which extends to all, given the similarity of the body of the Logos to our own. Regarding the second cause, man is reconstructed according to the

  16. Engineering aspects of compact stellarators

    International Nuclear Information System (INIS)

    Nelson, B.E.; Benson, R.D.; Brooks, A.

    2003-01-01

    Compact stellarators could combine the good confinement and high beta of a tokamak with the inherently steady state, disruption-free characteristics of a stellarator. Two U.S. compact stellarator facilities are now in the conceptual design phase: the National Compact Stellarator Experiment (NCSX) and the Quasi- Poloidal Stellarator (QPS). NCSX has a major radius of 1.4 m and a toroidal field up to 2 T. The primary feature of both NCSX and QPS is the set of modular coils that provide the basic magnetic configuration. These coils represent a major engineering challenge due to the complex shape, precise geometric accuracy, and high current density of the windings. The winding geometry is too complex for conventional hollow copper conductor construction. Instead, the modular coils will be wound with flexible, multi strand cable conductor that has been compacted to a 75% copper packing fraction. Inside the NCSX coil set and surrounding the plasma is a highly contoured vacuum vessel. The vessel consists of three identical, 120 deg. segments that are bolted together at double sealed joints. The QPS device has a major radius of 0.9 m, a toroidal field of 1 T, and an aspect ratio of only 2.7. Instead of an internal vacuum vessel, the QPS modular coils will operate in an external vacuum tank. (author)

  17. Stellar Oxygen Abundances

    Science.gov (United States)

    King, Jeremy

    1994-04-01

    This dissertation addresses several issues concerning stellar oxygen abundances. The 7774 {\\AA} O I triplet equivalent widths of Abia & Rebolo [1989, AJ, 347, 186] for metal-poor dwarfs are found to be systematically too high. I also argue that current effective temperatures used in halo star abundance studies may be ~150 K too low. New color-Teff relations are derived for metal-poor stars. Using the revised Teff values and improved equivalent widths for the 7774A O I triplet, the mean [O/Fe] ratio for a handful of halo stars is found to be +0.52 with no dependence on Teff or [Fe/H]. Possible cosmological implications of the hotter Teff scale are discussed along with additional evidence supporting the need for a higher temperature scale for metal-poor stars. Our Teff scale leads to a Spite Li plateau value of N(Li)=2.28 +/- 0.09. A conservative minimal primordial value of N(Li)=2.35 is inferred. If errors in the observations and models are considered, consistency with standard models of Big Bang nucleosynthesis is still achieved with this larger Li abundance. The revised Teff scale raises the observed B/Be ratio of HD 140283 from 10 to 12, making its value more comfortably consistent with the production of the observed B and Be by ordinary spallation. Our Teff values are found to be in good agreement with values predicted from both the Victoria and Yale isochrone color-Teff relations. Thus, it appears likely that no changes in globular cluster ages would result. Next, we examine the location of the break in the [O/Fe] versus [Fe/H] plane in a quantitative fashion. Analysis of a relatively homogeneous data set does not favor any unique break point in the range -1.7 /= -3), in agreement with the new results for halo dwarfs. We find that the gap in the observed [O/H] distribution, noted by Wheeler et al. [1989, ARAA, 27, 279], persists despite the addition of more O data and may betray the occurrence of a hiatus in star formation between the end of halo formation and

  18. Trabajos en espacios confinados. Riesgos y medidas preventivas

    OpenAIRE

    Fernández, Sergio

    2012-01-01

    La ejecución de trabajos en espacios confinados resulta una necesidad en diversos sectores como por ejemplo en la industria química, redes de alcantarillado, construcción de barcos, en pozos,… con el fin desarrollar diversas tareas como limpiezas, inspecciones interiores, trabajos de pintura, reparaciones varias,… lo que implica la implantación de medidas especiales y rigurosas a planificar y llevar a cabo. Los riesgos que presentan la ejecución de estos trabajos en espacios confinados ...

  19. Plan de negocios de la empresa Random; pantalones a medida

    OpenAIRE

    Marsal Josa, Armando

    2017-01-01

    Este trabajo trata de la realización del Plan de Negocio de Random, idea de negocio que consiste en una startup que diseña y vende pantalones tipo vaquero y chino a medida, pudiendo el comprador elegir, de entre una serie de detalles de motivos navajos ofrecidos por la marca, la forma de personalizarlos. Tendrán un precio asequible, intermedio entre las grandes marcas (Zara...) y las marcas tradicionales (Levi’s...). Se pretende dar salida a un producto artesanal y de calidad, aprovechando un...

  20. A Medida socioeducativa de internação

    OpenAIRE

    Meggiato, Jaqueline da Rosa

    2011-01-01

    Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro Sócio-Econômico, Programa de Pós-Graduação em Serviço Social, Florianópolis, 2011 O presente trabalho teve como preocupação central, investigar as diferentes correntes teóricas sobre o Direito da Criança e do Adolescente caracterizando-se, assim, como pesquisa de caráter teórico. A partir dessa investigação buscou-se entender os fundamentos que influenciam os magistrados em suas decisões pela medida socioeducativa de i...

  1. Planets, stars and stellar systems

    CERN Document Server

    Bond, Howard; McLean, Ian; Barstow, Martin; Gilmore, Gerard; Keel, William; French, Linda

    2013-01-01

    This is volume 3 of Planets, Stars and Stellar Systems, a six-volume compendium of modern astronomical research covering subjects of key interest to the main fields of contemporary astronomy. This volume on “Solar and Stellar Planetary Systems” edited by Linda French and Paul Kalas presents accessible review chapters From Disks to Planets, Dynamical Evolution of Planetary Systems, The Terrestrial Planets, Gas and Ice Giant Interiors, Atmospheres of Jovian Planets, Planetary Magnetospheres, Planetary Rings, An Overview of the Asteroids and Meteorites, Dusty Planetary Systems and Exoplanet Detection Methods. All chapters of the handbook were written by practicing professionals. They include sufficient background material and references to the current literature to allow readers to learn enough about a specialty within astronomy, astrophysics and cosmology to get started on their own practical research projects. In the spirit of the series Stars and Stellar Systems published by Chicago University Press in...

  2. Evaluación de anemia ferropénica en la primera infancia del Municipio de Sonsón-Antioquia, 2007

    Directory of Open Access Journals (Sweden)

    Tulia Isabel Castillo Salgado

    2014-12-01

    Full Text Available Objetivo: Determinar la prevalencia de anemia por deficiencia de hierro en niños de la primera infancia del municipio de Sonsón – Antioquia, en el año 2007. Metodología: Se realizó un estudio descriptivo transversal en 391 niños de 0 a 84 meses de edad del Municipio de Sonsón, Antioquia. Se estudiaron los parámetros de hemoglobina y ferritina sérica utilizando puntos de corte de la Organización Mundial de la Salud (OMS. Se calcularon las medidas de frecuencia y de resumen y los intervalos de confianza para proporciones y las pruebas de estadística paramétrica y no paramétrica. Resultados: La prevalencia de anemia ferropénica fue de 4,3% y la media de ferritina sérica y de hemoglobina para la población del estudio fue de 29,9 ng/mL y 12,6 g/dL respectivamente. Adicionalmente se halló significancia estadística de la prevalencia de anemia ferropénica por grupo de edad (p<0,0001; pero no se encontró significancia estadística de la  prevalencia de anemia con el sexo (p= 1,0000.  Conclusión: La prevalencia de anemia ferropénica en los niños de la primera infancia del Municipio de Sonsón fue baja de acuerdo con los parámetros de hemoglobina y ferritina sérica establecidos por la OMS, hay variación de la anemia ferropénica por grupo de edad pero no por sexo.

  3. Camiones y dumpers: medidas de seguridad. (Tercera parte

    Directory of Open Access Journals (Sweden)

    Chinchilla, M.

    1963-04-01

    Full Text Available Safety measures to be adopted in connection with any type of work should be those that are specifically adequate for the kind of risks involved, for it is just as wrong to adopt measures that are too ellaborate as not to take any at all. Two kinds of safety measures can be considered: those applying to the personnel, and those that protect the equipment. The efficiency and trouble free completion of the work will depend on the nature of the safety measures that are taken. Accidents are easy to avoid in general if the right safety precautions are taken. Such accidents involve both moral and financial damage, and a consequent loss of efficiency.Las medidas de seguridad que deberán adoptarse en cualquier trabajo serán las precisas, puesto que puede ser tan perjudicial señalar demasiadas como no señalar ninguna. Pueden considerarse dos tipos de medidas de seguridad: las concernientes a la seguridad del personal y las referentes a la maquinaria empleada. De la determinación de unas y otras, así como de su exacta observancia, dependerá que el trabajo se realice de forma eficaz y sin contratiempos, fácilmente evitables, por otra parte, que acarrearían consecuencias de tipo moral y económico, con el consiguiente descenso del rendimiento obtenido.

  4. Stellar CME candidates: towards a stellar CME-flare relation

    Science.gov (United States)

    Paraskevi Moschou, Sofia; Drake, Jeremy J.; Cohen, Ofer; Alvarado-Gomez, Julian D.; Garraffo, Cecilia

    2018-06-01

    For decades the Sun has been the only star that allowed for direct CME observations. Recently, with the discovery of multiple extrasolar systems, it has become imperative that the role of stellar CMEs be assessed in the context of exoplanetary habitability. Solar CMEs and flares show a higher association with increasing flaring energy, with strong flares corresponding to large and fast CMEs. As argued in earlier studies, extrasolar environments around active stars are potentially dominated by CMEs, as a result of their extreme flaring activity. This has strong implications for the energy budget of the system and the atmospheric erosion of orbiting planets.Nevertheless, with current instrumentation we are unable to directly observe CMEs in even the closest stars, and thus we have to look for indirect techniques and observational evidence and signatures for the eruption of stellar CMEs. There are three major observational techniques for tracing CME signatures in other stellar systems, namely measuring Type II radio bursts, Doppler shifts in UV/optical lines or transient absorption in the X-ray spectrum. We present observations of the most probable stellar CME candidates captured so far and examine the different observational techniques used together with their levels of uncertainty. Assuming that they were CMEs, we try to asses their kinematic and energetic characteristics and place them in an extension of the well-established solar CME-flare energy scaling law. We finish by discussing future observations for direct measurements.

  5. CAMBIOS EN LA DISTRIBUCIÓN DEL INGRESO FAMILIAR EN COSTA RICA DURANTE LA PRIMERA DÉCADA DEL SIGLO XXI

    Directory of Open Access Journals (Sweden)

    Juan Diego Trejos S.

    2013-03-01

    Full Text Available Costa Rica no sigue durante la primera década del siglo XXI la tendencia observada para la mayoría de los países de la región, que experimentan una reducción de la desigualdad en la distribución del ingreso familiar per cápita. Durante la primera mitad de esa década sí se produce una reducción en la desigualdad pero se revierte en el quinquenio siguiente. Para estudiar esos cambios se utiliza una desagregación de la desigualdad, medida por el coeficiente de Gini, por fuentes de ingreso, usando 12 fuentes distintas. Los resultados señalan que la reducción de la desigualdad en la primera mitad de la década, se da en un contexto de crecimiento económico pero estancamiento de los ingresos reales, que se concentra en los estratos de mayores ingresos. Esto implica que la reducción de la desigualdad se concentró en la reducción de los ingresos reales de las fuentes con mayor poder concentrador (elasticidades Gini ingreso mayor a la unidad y cambios marginales positivos, como lo son los ingresos laborales de los más calificados, las rentas del capital y las pensiones contributivas. En la segunda mitad de la década, el repunte de la desigualdad se produce por un aumento significativo de los ingresos reales de todas las fuentes, pero principalmente de las que tienen un impacto concentrador que no puede ser neutralizado por la expansión de las fuentes que reducen la desigualdad (ingresos laborales de los trabajadores no calificados y las transferencias estatales. Los resultados sugieren la necesidad de aplicar una política de salarios mínimos más activa, reforzar los programas de apoyo productivo para el sector informal, ampliar la oferta de trabajadores más calificados a través de la política educativa y ampliar las transferencias monetarias hacia los más pobres, lo que requiere de una reforma tributaria.

  6. Science with Synthetic Stellar Surveys

    Science.gov (United States)

    Sanderson, Robyn Ellyn

    2018-04-01

    A new generation of observational projects is poised to revolutionize our understanding of the resolved stellar populations of Milky-Way-like galaxies at an unprecedented level of detail, ushering in an era of precision studies of galaxy formation. In the Milky Way itself, astrometric, spectroscopic and photometric surveys will measure three-dimensional positions and velocities and numerous chemical abundances for stars from the disk to the halo, as well as for many satellite dwarf galaxies. In the Local Group and beyond, HST, JWST and eventually WFIRST will deliver pristine views of resolved stars. The groundbreaking scale and dimensionality of this new view of resolved stellar populations in galaxies challenge us to develop new theoretical tools to robustly compare these surveys to simulated galaxies, in order to take full advantage of our new ability to make detailed predictions for stellar populations within a cosmological context. I will describe a framework for generating realistic synthetic star catalogs and mock surveys from state-of-the-art cosmological-hydrodynamical simulations, and present several early scientific results from, and predictions for, resolved stellar surveys of our Galaxy and its neighbors.

  7. Maximum stellar iron core mass

    Indian Academy of Sciences (India)

    An analytical method of estimating the mass of a stellar iron core, just prior to core collapse, is described in this paper. The method employed depends, in part, upon an estimate of the true relativistic mass increase experienced by electrons within a highly compressed iron core, just prior to core collapse, and is significantly ...

  8. Maximum stellar iron core mass

    Indian Academy of Sciences (India)

    60, No. 3. — journal of. March 2003 physics pp. 415–422. Maximum stellar iron core mass. F W GIACOBBE. Chicago Research Center/American Air Liquide ... iron core compression due to the weight of non-ferrous matter overlying the iron cores within large .... thermal equilibrium velocities will tend to be non-relativistic.

  9. Integrated Circuit Stellar Magnitude Simulator

    Science.gov (United States)

    Blackburn, James A.

    1978-01-01

    Describes an electronic circuit which can be used to demonstrate the stellar magnitude scale. Six rectangular light-emitting diodes with independently adjustable duty cycles represent stars of magnitudes 1 through 6. Experimentally verifies the logarithmic response of the eye. (Author/GA)

  10. Stellar dynamics and black holes

    Indian Academy of Sciences (India)

    Chandrasekhar's most important contribution to stellar dynamics was the concept of dynamical friction. I briefly review that work, then discuss some implications of Chandrasekhar's theory of gravitational encounters for motion in galactic nuclei. Author Affiliations. David Merritt1. Department of Physics, Rochester Institute ...

  11. TEM turbulence optimisation in stellarators

    Science.gov (United States)

    Proll, J. H. E.; Mynick, H. E.; Xanthopoulos, P.; Lazerson, S. A.; Faber, B. J.

    2016-01-01

    With the advent of neoclassically optimised stellarators, optimising stellarators for turbulent transport is an important next step. The reduction of ion-temperature-gradient-driven turbulence has been achieved via shaping of the magnetic field, and the reduction of trapped-electron mode (TEM) turbulence is addressed in the present paper. Recent analytical and numerical findings suggest TEMs are stabilised when a large fraction of trapped particles experiences favourable bounce-averaged curvature. This is the case for example in Wendelstein 7-X (Beidler et al 1990 Fusion Technol. 17 148) and other Helias-type stellarators. Using this knowledge, a proxy function was designed to estimate the TEM dynamics, allowing optimal configurations for TEM stability to be determined with the STELLOPT (Spong et al 2001 Nucl. Fusion 41 711) code without extensive turbulence simulations. A first proof-of-principle optimised equilibrium stemming from the TEM-dominated stellarator experiment HSX (Anderson et al 1995 Fusion Technol. 27 273) is presented for which a reduction of the linear growth rates is achieved over a broad range of the operational parameter space. As an important consequence of this property, the turbulent heat flux levels are reduced compared with the initial configuration.

  12. EL NUDO DEL MUNDO. SUBJETIVIDAD Y ONTOLOGÍA DE LA PRIMERA PERSONA

    Directory of Open Access Journals (Sweden)

    Pedro Enrique García Ruiz

    2009-01-01

    Full Text Available Este ensayo busca mostrar la relevancia de la perspectiva de la primera persona a través de un enfo-que fenomenológico. Frente a la negativa de las distintas tendencias de la filosofía de la mente analítica, las ciencias cognitivas y las neurociencias de considerar la realidad de los estados mentales como fenómenos subjetivos, se esboza una revisión de la cuestión con la finalidad de señalar la relación entre la experiencia subjetiva y una ontología de la primera persona.

  13. Stellar Parameters for Trappist-1

    Science.gov (United States)

    Van Grootel, Valérie; Fernandes, Catarina S.; Gillon, Michael; Jehin, Emmanuel; Manfroid, Jean; Scuflaire, Richard; Burgasser, Adam J.; Barkaoui, Khalid; Benkhaldoun, Zouhair; Burdanov, Artem; Delrez, Laetitia; Demory, Brice-Olivier; de Wit, Julien; Queloz, Didier; Triaud, Amaury H. M. J.

    2018-01-01

    TRAPPIST-1 is an ultracool dwarf star transited by seven Earth-sized planets, for which thorough characterization of atmospheric properties, surface conditions encompassing habitability, and internal compositions is possible with current and next-generation telescopes. Accurate modeling of the star is essential to achieve this goal. We aim to obtain updated stellar parameters for TRAPPIST-1 based on new measurements and evolutionary models, compared to those used in discovery studies. We present a new measurement for the parallax of TRAPPIST-1, 82.4 ± 0.8 mas, based on 188 epochs of observations with the TRAPPIST and Liverpool Telescopes from 2013 to 2016. This revised parallax yields an updated luminosity of {L}* =(5.22+/- 0.19)× {10}-4 {L}ȯ , which is very close to the previous estimate but almost two times more precise. We next present an updated estimate for TRAPPIST-1 stellar mass, based on two approaches: mass from stellar evolution modeling, and empirical mass derived from dynamical masses of equivalently classified ultracool dwarfs in astrometric binaries. We combine them using a Monte-Carlo approach to derive a semi-empirical estimate for the mass of TRAPPIST-1. We also derive estimate for the radius by combining this mass with stellar density inferred from transits, as well as an estimate for the effective temperature from our revised luminosity and radius. Our final results are {M}* =0.089+/- 0.006 {M}ȯ , {R}* =0.121+/- 0.003 {R}ȯ , and {T}{eff} = 2516 ± 41 K. Considering the degree to which the TRAPPIST-1 system will be scrutinized in coming years, these revised and more precise stellar parameters should be considered when assessing the properties of TRAPPIST-1 planets.

  14. Targeted Optimization of Quasi-Symmetric Stellarators

    International Nuclear Information System (INIS)

    Hegna, Chris C.; Talmadge, J. N.

    2016-01-01

    The proposed research focuses on targeted areas of plasma physics dedicated to improving the stellarator concept. Research was pursued in the technical areas of edge/divertor physics in 3D configurations, magnetic island physics in stellarators, the role of 3D shaping on microinstabilities and turbulent transport and energetic ion confinement in stellarators.

  15. Targeted Optimization of Quasi-Symmetric Stellarators

    Energy Technology Data Exchange (ETDEWEB)

    Hegna, Chris C. [Univ. of Wisconsin, Madison, WI (United States). Dept. of Engineering Physics; Anderson, D. T. [Univ. of Wisconsin, Madison, WI (United States); Talmadge, J. N. [Univ. of Wisconsin, Madison, WI (United States)

    2016-10-06

    The proposed research focuses on targeted areas of plasma physics dedicated to improving the stellarator concept. Research was pursued in the technical areas of edge/divertor physics in 3D configurations, magnetic island physics in stellarators, the role of 3D shaping on microinstabilities and turbulent transport and energetic ion confinement in stellarators.

  16. Nuevo criterio de complejidad utilizando una medida de eficiencia

    OpenAIRE

    Munduate del Río, Arantza; Pérez Prados, Antonio; Cano Sevilla, Francisco J.

    1995-01-01

    Centrado en el campo de los árboles de decisión, este trabajo estudia la forma de selección de un árbol óptimo entre los posibles árbo1es obtenidos a partir del análisis de un conjunto de datos, utilizando para ello una cantidad criterio que combina linealmente dos medidas de la calidad de un árbol: el error de resustitución y la eficiencia. Analizando el efecto de un proceso de poda en la cantidad criterio se obtiene una sucesión finita de subárboles rnínimos óptimamente podados del árbol má...

  17. Refração atmosferica nas medidas Doppler

    OpenAIRE

    Oliveira, Leonardo Castro de

    1990-01-01

    Orientador: Jose Bittencourt de Andrade Dissertação (mestrado) - Universidade Federal do Parana. Setor de Tecnologia Resumo: Esta dissertação tem por objetivo realizar investigações referentes à refração atmosférica nas medidas Doppler. São considerados quatro modelos para correção troposférica, e o modelo de duas frequências para a correção da refração ionosférica . São também testados de diferentes fontes de dados meteorológicos. Todos os testes são feitos utilizando-se o programa GEO...

  18. Estudio de medidas y proyectos de movilidad ambiental en el entorno europeo

    OpenAIRE

    Moya González, Luis

    2011-01-01

    Índice Introducción Tablas resumen de medidas ambientales sobre movilidad Medidas específicas para ciudades históricas Mejora del transporte públicoGestión de automóvilesVehículos compartidosInnovación en vehículos y carburantesTransporte de mercancíasBicicletasPeatonesGestión: demanda, incentivos, etcOtras medidasMedidas coordinadas y planes integrales Experiencias europeasLa situación en EspañaProgramas y proyectos subvencionados Programas de la Unión EuropeaProyectos internacionales no vin...

  19. Primera hembra conocida de Megathecla gigantea (Hewitson, 1867 (Lepidoptera: Lycaenidae: Eumaeini

    Directory of Open Access Journals (Sweden)

    Gerardo Lamas

    2013-06-01

    Full Text Available Se reporta la primera hembra conocida de la extremadamente rara especie amazónica Megathecla gigantea (Hewitson, 1867, de Perú, Loreto, Tierra Hermosa. Se ofrece algunas notas sobre su comportamiento y hábitat.

  20. Characterizing stellar and exoplanetary environments

    CERN Document Server

    Khodachenko, Maxim

    2015-01-01

    In this book an international group of specialists discusses studies of exoplanets subjected to extreme stellar radiation and plasma conditions. It is shown that such studies will help us to understand how terrestrial planets and their atmospheres, including the early Venus, Earth and Mars, evolved during the host star’s active early phase. The book presents an analysis of findings from Hubble Space Telescope observations of transiting exoplanets, as well as applications of advanced numerical models for characterizing the upper atmosphere structure and stellar environments of exoplanets. The authors also address detections of atoms and molecules in the atmosphere of “hot Jupiters” by NASA’s Spitzer telescope. The observational and theoretical investigations and discoveries presented are both timely and important in the context of the next generation of space telescopes. 
 The book is divided into four main parts, grouping chapters on exoplanet host star radiation and plasma environments, exoplanet u...

  1. Modular Stellarator Fusion Reactor concept

    International Nuclear Information System (INIS)

    Miller, R.L.; Krakowski, R.A.

    1981-08-01

    A preliminary conceptual study is made of the Modular Stellarator Reactor (MSR). A steady-state ignited, DT-fueled, magnetic fusion reactor is proposed for use as a central electric-power station. The MSR concept combines the physics of the classic stellarator confinement topology with an innovative, modular-coil design. Parametric tradeoff calculations are described, leading to the selection of an interim design point for a 4-GWt plant based on Alcator transport scaling and an average beta value of 0.04 in an l = 2 system with a plasma aspect ratio of 11. The physics basis of the design point is described together with supporting magnetics, coil-force, and stress computations. The approach and results presented herein will be modified in the course of ongoing work to form a firmer basis for a detailed conceptual design of the MSR

  2. Hydromagnetic instability in a stellarator

    Energy Technology Data Exchange (ETDEWEB)

    Kruskal, M D; Gottlieb, M B; Johnson, J L; Goldman, L M [Project Matterhorn, Princeton University, Princeton, NJ (United States)

    1958-07-01

    It was noted that when there is a uniform externally imposed longitudinal field much larger than the field of the discharge current, one should expect instabilities in the form of a lateral displacement of the plasma column into a helix of large pitch. At the wavelength of fastest growth the e-folding time approximates the time it takes a sound wave in the plasma to traverse the radius of the plasma column. This problem has been re-examines under the conditions which might be expected to occur in the stellarator during ohmic heating, including the presence of external conductors. The theory is applied to the stellarator; and it is shown that the external conductors are in fact unimportant. The important effects due to the finite length of the Machine are discussed and the effects of more general current distributions are considered. The results from the experiments are given.

  3. ACCELERATED FITTING OF STELLAR SPECTRA

    Energy Technology Data Exchange (ETDEWEB)

    Ting, Yuan-Sen; Conroy, Charlie [Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Rix, Hans-Walter [Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany)

    2016-07-20

    Stellar spectra are often modeled and fitted by interpolating within a rectilinear grid of synthetic spectra to derive the stars’ labels: stellar parameters and elemental abundances. However, the number of synthetic spectra needed for a rectilinear grid grows exponentially with the label space dimensions, precluding the simultaneous and self-consistent fitting of more than a few elemental abundances. Shortcuts such as fitting subsets of labels separately can introduce unknown systematics and do not produce correct error covariances in the derived labels. In this paper we present a new approach—Convex Hull Adaptive Tessellation (chat)—which includes several new ideas for inexpensively generating a sufficient stellar synthetic library, using linear algebra and the concept of an adaptive, data-driven grid. A convex hull approximates the region where the data lie in the label space. A variety of tests with mock data sets demonstrate that chat can reduce the number of required synthetic model calculations by three orders of magnitude in an eight-dimensional label space. The reduction will be even larger for higher dimensional label spaces. In chat the computational effort increases only linearly with the number of labels that are fit simultaneously. Around each of these grid points in the label space an approximate synthetic spectrum can be generated through linear expansion using a set of “gradient spectra” that represent flux derivatives at every wavelength point with respect to all labels. These techniques provide new opportunities to fit the full stellar spectra from large surveys with 15–30 labels simultaneously.

  4. Grigori Kuzmin and Stellar Dynamics

    Directory of Open Access Journals (Sweden)

    Zeeuw P. Tim de

    2011-06-01

    Full Text Available Grigori Kuzmin was a very gifted dynamicist and one of the towering figures in the distinguished history of the Tartu Observatory. He obtained a number of important results in relative isolation which were later rediscovered in the West. This work laid the foundation for further advances in the theory of stellar systems in dynamical equilibrium, thereby substantially increasing our understanding of galaxy dynamics.

  5. Geometry Dependence of Stellarator Turbulence

    International Nuclear Information System (INIS)

    Mynick, H.E.; Xanthopoulos, P.; Boozer, A.H.

    2009-01-01

    Using the nonlinear gyrokinetic code package GENE/GIST, we study the turbulent transport in a broad family of stellarator designs, to understand the geometry-dependence of the microturbulence. By using a set of flux tubes on a given flux surface, we construct a picture of the 2D structure of the microturbulence over that surface, and relate this to relevant geometric quantities, such as the curvature, local shear, and effective potential in the Schrodinger-like equation governing linear drift modes

  6. Models of hot stellar systems

    International Nuclear Information System (INIS)

    Van Albada, T.S.

    1986-01-01

    Elliptical galaxies consist almost entirely of stars. Sites of recent star formation are rare, and most stars are believed to be several billion years old, perhaps as old as the Universe itself (--10/sup 10/ yrs). Stellar motions in ellipticals show a modest amount of circulation about the center of the system, but most support against the force of gravity is provided by random motions; for this reason ellipticals are called 'hot' stellar systems. Spiral galaxies usually also contain an appreciable amount of gas (--10%, mainly atomic hydrogen) and new stars are continually being formed out of this gas, especially in the spiral arms. In contrast to ellipticals, support against gravity in spiral galaxies comes almost entirely from rotation; random motions of the stars with respect to rotation are small. Consequently, spiral galaxies are called 'cold' stellar systems. Other than in hot systems, in cold systems the collective response of stars to variations in the force field is an essential part of the dynamics. The present overview is limited to mathematical models of hot systems. Computational methods are also discussed

  7. MEDIDAS DE NÚCLEO INFLACIONARIO PARA COSTA RICA

    Directory of Open Access Journals (Sweden)

    Gabriela Saborío Muñoz

    2003-07-01

    Full Text Available En este documento se elaboran y evalúan medidas alternativas de núcleo inflacionario para Costa Rica. La idea fundamental contempla al núcleo inflacionario como un indicador de la tendencia subyacente de la inflación capaz de capturar el componente del cambio total de precios común a todos los bienes y servicios, cuya persistencia se mantendría en el mediano y largo plazo y que excluye los cambios en los precios relativos de estos. La medida de núcleo inflacionario seleccionada se contrasta con el Índice de Núcleo Inflacionario (INI, indicador de inflación subyacente actualmente utilizado por el Banco Central de Costa Rica (BCCR.El Índice Subyacente de Inflación (ISI, definido como una medida de núcleo inflacionario que excluye un 30,7% del peso total del Índice de Precios al Consumidor (IPC, refleja más fielmente la tendencia subyacente de la inflación y logra capturar el movimiento más permanente del nivel general de precios, aislando las variaciones en precios relativos. Además, el ISI es fácil de calcular e interpretar lo cual ayuda a incrementar la transparencia y credibilidad de la política monetaria. También es un indicador oportuno, aumentando su valor para los que formulan la política monetaria. Por último, el ISI supera algunas de las limitaciones del INI, como son la falta de un criterio estadístico para definir el punto de corte de los bienes y servicios a excluir y el alto porcentaje del peso total del IPC eliminado. AbstractThis paper builds and evaluates several alternative measures of core inflation for Costa Rica. The chosen measure of core inflation is contrasted with the core inflation index (INI, which is the indicator of underlying inflation used today by the Central Bank of Costa Rica (BCCR. The main idea is that core inflation is a good indicator of the underlying inflation and catches the part of overall price change common to all the goods and services that is expected to persist in the

  8. Cestos, gestos y género, en los azulejos portugueses de la primera mitad del siglo XX

    Directory of Open Access Journals (Sweden)

    Mingote Calderón, José Luis

    2014-12-01

    Full Text Available This paper offers a partial approach to the diverse content of Portuguese tile panels during the first half of the 20th century. Tile panels are found in a wide range of buildings such as train stations, markets, squares, fountains, shops, private homes, etc. showing the image of peasants through an elite perspective. In addition, images are classified according to the nationalist point of view of the «people.» The copy of previous images, mostly photographic ones, communicates a sense of realism and truth which appears well reflected in both in the material elements and the gestures using them. This fact does not prevent the ideological interpretation of the images. The choice of scene themes intends to reflect the existing regional diversity starting from an ideological selection. The data collected shows the prevalence of some aspects and puts special emphases on vine issues and, particularly, on grape harvest. Other issues represented include the olive harvest, activities related to cereals, the collection of seaweed for field manuring. Less represented are scenes of markets.Este trabajo ofrece una aproximación parcial al variado contenido de los paneles de azulejos portugueses de la primera mitad del siglo XX que se encuentran en una amplia gama de edificios: estaciones de tren, mercados, plazas, fuentes, comercios, casas particulares, etc. En ellos, las imágenes de los campesinos aparecen filtradas por la óptica de las élites y están categorizadas por la interpretación nacionalista del «pueblo». La copia de imágenes previas, mayoritariamente fotográficas, transmite una sensación de realismo y de veracidad, plasmada tanto en los elementos materiales como en los gestos de uso de los mismos. Algo que no impide la existencia de una interpretación ideológica de las imágenes. La elección de las escenas pretende reflejar la variedad regional a través de una selección ideológica. En la documentación recopilada priman

  9. Results of Compact Stellarator Engineering Trade Studies

    International Nuclear Information System (INIS)

    Brown, Tom; Bromberg, L.; Cole, M.

    2009-01-01

    A number of technical requirements and performance criteria can drive stellarator costs, e.g., tight tolerances, accurate coil positioning, low aspect ratio (compactness), choice of assembly strategy, metrology, and complexity of the stellarator coil geometry. With the completion of a seven-year design and construction effort of the National Compact Stellarator Experiment (NCSX) it is useful to interject the NCSX experience along with the collective experiences of the NCSX stellarator community to improving the stellarator configuration. Can improvements in maintenance be achieved by altering the stellarator magnet configuration with changes in the coil shape or with the combination of trim coils? Can a mechanical configuration be identified that incorporates a partial set of shaped fixed stellarator coils along with some removable coil set to enhance the overall machine maintenance? Are there other approaches that will simplify the concepts, improve access for maintenance, reduce overall cost and improve the reliability of a stellarator based power plant? Using ARIES-CS and NCSX as reference cases, alternative approaches have been studied and developed to show how these modifications would favorably impact the stellarator power plant and experimental projects. The current status of the alternate stellarator configurations being developed will be described and a comparison made to the recently designed and partially built NCSX device and the ARIES-CS reactor design study

  10. Results of Compact Stellarator Engineering Trade Studies

    International Nuclear Information System (INIS)

    Brown, T.; Bromberg, L.; Cole, M.

    2009-01-01

    A number of technical requirements and performance criteria can drive stellarator costs, e.g., tight tolerances, accurate coil positioning, low aspect ratio (compactness), choice of assembly strategy, metrology, and complexity of the stellarator coil geometry. With the completion of a seven-year design and construction effort of the National Compact Stellarator Experiment (NCSX) it is useful to interject the NCSX experience along with the collective experiences of the NCSX stellarator community to improving the stellarator configuration. Can improvements in maintenance be achieved by altering the stellarator magnet configuration with changes in the coil shape or with the combination of trim coils? Can a mechanical configuration be identified that incorporates a partial set of shaped fixed stellarator coils along with some removable coil set to enhance the overall machine maintenance? Are there other approaches that will simplify the concepts, improve access for maintenance, reduce overall cost and improve the reliability of a stellarator based power plant? Using ARIES-CS and NCSX as reference cases, alternative approaches have been studied and developed to show how these modifications would favorably impact the stellarator power plant and experimental projects. The current status of the alternate stellarator configurations being developed will be described and a comparison made to the recently designed and partially built NCSX device and the ARIES-CS reactor design study.

  11. Futebol libertário: compromisso social na medida

    Directory of Open Access Journals (Sweden)

    Fábio Silvestre Silva

    Full Text Available Baseados na Constituição de 1988 e no Estatuto da Criança e do Adolescente, de 1990, o Centro de Defesa dos Direitos da Criança e do Adolescente de Interlagos (CEDECA Interlagos traz um relato de experiência de uma metodologia alternativa de acompanhamento de adolescentes inseridos em medidas socioeducativas em meio aberto na região da Capela do Socorro e Parelheiros. Essa proposta utiliza o futebol como meio que possibilita ao adolescente refletir sobre sua realidade e suas práticas cotidianas, reconhecendo suas possibilidades de se desenvolver como sujeito de direito e de se tornar protagonista no que diz respeito às ações que busquem sua promoção social e a construção e o exercício da cidadania ativa. É possível observar que, com esse tipo de linguagem, mais próximo do desejo desses jovens, os mesmos atribuem um novo sentido ao acompanhamento a que foram submetidos. Na lógica socioeducativa, procuram superar obstáculos no sentido de buscar cada vez mais seu protagonismo, sua autoria, para reafirmar o que o ato infracional revelou, que é a busca por ser sujeito.

  12. Presiones medidas en la base de una losa de fondo con juntas paralelas al flujo en un canal

    Directory of Open Access Journals (Sweden)

    Edwin Hurtado Orobio

    2009-01-01

    Full Text Available Se estudió si las aristas traseras de las juntas longitudinales de una losa de piso, fija al fondo de un canal con flujo supercrítico, convierten energía cinética en energía de presión en el rango de números de Froude de 2,84 a 10,12. En cada prueba, se midió la presión en 16 puntos de su cara inferior, con transductores piezoresistivos en tres líneas longitudinales: una central con 8 sensores y dos laterales, a lado y lado de la primera, con cuatro sensores cada una. De esta forma, se determinó la distribución de las presiones medias debajo de la losa ensayada, similar a las usadas en obras civiles para evitar la acción erosiva de la turbulencia de un flujo supercrítico. El análisis de las presiones medidas muestra que, aún cuando las caras superiores del piso del canal y del bloque protector estén en el mismo plano horizontal, las aristas traseras de las juntas longitudinales transforman energía de velocidad en energía de presión. Así, se ha detectado un factor que interviene en la generación de la fuerza hidrodinámica que levanta revestimientos de diverso tipos de estructuras, hasta ahora ignorado en el estudio de este problema.

  13. Stellarator fusion neutronics research in Australia

    International Nuclear Information System (INIS)

    Zimin, S.; Cross, R.C.

    1997-01-01

    The new status of the H-INF Heliac Stellaralor as a National Facility and the signed international Implementing Agreement on 'Collaboration in the Development of the Stellarator Concept' represents a significant encouragement for further fusion research in Australia. In this report the future of fusion research in Australia is discussed with special attention being paid to the importance of Stellarator power plant studies and in particular stellarator fusion neutronics. The main differences between tokamak and stellarator neutronics analyses are identified, namely the neutron wall loading, geometrical modelling and total heating in in-vessel reactor components including toroidal field (TF) coils. Due to the more complicated nature of stellarator neutronics analyses, simplified approaches to fusion neutronics already developed for tokamaks are expected to be even more important and widely used for designing a Conceptual Stellarator Power Plant

  14. On the universal stellar law

    Science.gov (United States)

    Krot, Alexander

    In this work, we consider a statistical theory of gravitating spheroidal bodies to derive and develop the universal stellar law for extrasolar systems. Previously, the statistical theory for a cosmogonic body forming (so-called spheroidal body)has been proposed [1-3]. This theory starts from the conception for forming a spheroidal body inside a gas-dust protoplanetary nebula; it permits us to derive the form of distribution functions, mass density, gravitational potentials and strengths both for immovable and rotating spheroidal bodies as well as to find the distribution function of specific angular momentum[1-3]. If we start from the conception for forming a spheroidal body as a protostar (in particular, proto-Sun) inside a prestellar (presolar) nebula then the derived distribution functions of particle (as well as the mass density of an immovable spheroidal body) characterizes the first stage of evolution: from a prestellar molecular cloud (the presolar nebula) to the forming core of protostar (the proto-Sun) together with its shell as a stellar nebula (the solar nebula). This work derives the equation of state of an ideal stellar substance based on conception of gravitating spheroidal body. Using this equation, we obtain the universal stellar law (USL) for the planetary systems connecting temperature, size and mass of each of stars. This work also considers the Solar corona in the connection with USL. Then it is accounting under calculation of the ratio of temperature of the Solar corona to effective temperature of the Sun’ surfaceand modification of USL. To test justice of the modified USLfor different types of stars, the temperature of stellar corona is estimated. The prediction of parameters of stars is carrying out by means of the modified USL,as well as the Hertzsprung-Russell’s dependence [5-7]is derivedby means of USL directly. This paper also shows that knowledge of some characteristics for multi-planet extrasolar systems refines own parameters of

  15. Multiplicity in Early Stellar Evolution

    Science.gov (United States)

    Reipurth, B.; Clarke, C. J.; Boss, A. P.; Goodwin, S. P.; Rodríguez, L. F.; Stassun, K. G.; Tokovinin, A.; Zinnecker, H.

    Observations from optical to centimeter wavelengths have demonstrated that multiple systems of two or more bodies is the norm at all stellar evolutionary stages. Multiple systems are widely agreed to result from the collapse and fragmentation of cloud cores, despite the inhibiting influence of magnetic fields. Surveys of class 0 protostars with millimeter interferometers have revealed a very high multiplicity frequency of about 2/3, even though there are observational difficulties in resolving close protobinaries, thus supporting the possibility that all stars could be born in multiple systems. Near-infrared adaptive optics observations of class I protostars show a lower binary frequency relative to the class 0 phase, a declining trend that continues through the class II/III stages to the field population. This loss of companions is a natural consequence of dynamical interplay in small multiple systems, leading to ejection of members. We discuss observational consequences of this dynamical evolution, and its influence on circumstellar disks, and we review the evolution of circumbinary disks and their role in defining binary mass ratios. Special attention is paid to eclipsing PMS binaries, which allow for observational tests of evolutionary models of early stellar evolution. Many stars are born in clusters and small groups, and we discuss how interactions in dense stellar environments can significantly alter the distribution of binary separations through dissolution of wider binaries. The binaries and multiples we find in the field are the survivors of these internal and external destructive processes, and we provide a detailed overview of the multiplicity statistics of the field, which form a boundary condition for all models of binary evolution. Finally, we discuss various formation mechanisms for massive binaries, and the properties of massive trapezia.

  16. Physics of Compact Advanced Stellarators

    International Nuclear Information System (INIS)

    Zarnstorff, M.C.; Berry, L.A.; Brooks, A.; Fredrickson, E.; Fu, G.-Y.; Hirshman, S.; Hudson, S.; Ku, L.-P.; Lazarus, E.; Mikkelsen, D.; Monticello, D.; Neilson, G.H.; Pomphrey, N.; Reiman, A.; Spong, D.; Strickler, D.; Boozer, A.; Cooper, W.A.; Goldston, R.; Hatcher, R.; Isaev, M.; Kessel, C.; Lewandowski, J.; Lyon, J.; Merkel, P.; Mynick, H.; Nelson, B.E.; Nuehrenberg, C.; Redi, M.; Reiersen, W.; Rutherford, P.; Sanchez, R.; Schmidt, J.; White, R.B.

    2001-01-01

    Compact optimized stellarators offer novel solutions for confining high-beta plasmas and developing magnetic confinement fusion. The 3-D plasma shape can be designed to enhance the MHD stability without feedback or nearby conducting structures and provide drift-orbit confinement similar to tokamaks. These configurations offer the possibility of combining the steady-state low-recirculating power, external control, and disruption resilience of previous stellarators with the low-aspect ratio, high beta-limit, and good confinement of advanced tokamaks. Quasi-axisymmetric equilibria have been developed for the proposed National Compact Stellarator Experiment (NCSX) with average aspect ratio 4-4.4 and average elongation of approximately 1.8. Even with bootstrap-current consistent profiles, they are passively stable to the ballooning, kink, vertical, Mercier, and neoclassical-tearing modes for beta > 4%, without the need for external feedback or conducting walls. The bootstrap current generates only 1/4 of the magnetic rotational transform at beta = 4% (the rest is from the coils), thus the equilibrium is much less nonlinear and is more controllable than similar advanced tokamaks. The enhanced stability is a result of ''reversed'' global shear, the spatial distribution of local shear, and the large fraction of externally generated transform. Transport simulations show adequate fast-ion confinement and thermal neoclassical transport similar to equivalent tokamaks. Modular coils have been designed which reproduce the physics properties, provide good flux surfaces, and allow flexible variation of the plasma shape to control the predicted MHD stability and transport properties

  17. STELLAR MASS DEPENDENT DISK DISPERSAL

    International Nuclear Information System (INIS)

    Kennedy, Grant M.; Kenyon, Scott J.

    2009-01-01

    We use published optical spectral and infrared (IR) excess data from nine young clusters and associations to study the stellar mass dependent dispersal of circumstellar disks. All clusters older than ∼3 Myr show a decrease in disk fraction with increasing stellar mass for solar to higher mass stars. This result is significant at about the 1σ level in each cluster. For the complete set of clusters we reject the null hypothesis-that solar and intermediate-mass stars lose their disks at the same rate-with 95%-99.9% confidence. To interpret this behavior, we investigate the impact of grain growth, binary companions, and photoevaporation on the evolution of disk signatures. Changes in grain growth timescales at fixed disk temperature may explain why early-type stars with IR excesses appear to evolve faster than their later-type counterparts. Little evidence that binary companions affect disk evolution suggests that photoevaporation is the more likely mechanism for disk dispersal. A simple photoevaporation model provides a good fit to the observed disk fractions for solar and intermediate-mass stars. Although the current mass-dependent disk dispersal signal is not strong, larger and more complete samples of clusters with ages of 3-5 Myr can improve the significance and provide better tests of theoretical models. In addition, the orbits of extra-solar planets can constrain models of disk dispersal and migration. We suggest that the signature of stellar mass dependent disk dispersal due to photoevaporation may be present in the orbits of observed extra-solar planets. Planets orbiting hosts more massive than ∼1.6 M sun may have larger orbits because the disks in which they formed were dispersed before they could migrate.

  18. Radiation transfer and stellar atmospheres

    Science.gov (United States)

    Swihart, T. L.

    This is a revised and expanded version of the author's Basic Physics of Stellar Atmospheres, published in 1971. The equation of transfer is considered, taking into account the intensity and derived quantities, the absorption coefficient, the emission coefficient, the source function, and special integrals for plane media. The gray atmosphere is discussed along with the nongray atmosphere, and aspects of line formation. Topics related to polarization are explored, giving attention to pure polarized radiation, general polarized radiation, transfer in a magnetic plasma, and Rayleigh scattering and the sunlit sky. Physical and astronomical constants, and a number of problems related to the subjects of the book are presented in an appendix.

  19. Drift waves in a stellarator

    International Nuclear Information System (INIS)

    Bhattacharjee, A.; Sedlak, J.E.; Similon, P.L.; Rosenbluth, M.N.; Ross, D.W.

    1982-11-01

    We investigate the eigenmode structure of drift waves in a straight stellarator using the ballooning mode formalism. The electrons are assumed to be adiabatic and the ions constitute a cold, magnetized fluid. The effective potential has an overall parabolic envelope but is modulated strongly by helical ripples along B. We have found two classes of solutions: those that are strongly localized in local helical wells, and those that are weakly localized and have broad spatial extent. The weakly localized modes decay spatially due to the existence of Mathieu resonances between the periods of the eigenfunction and the effective potential

  20. Helical axis stellarator equilibrium model

    International Nuclear Information System (INIS)

    Koniges, A.E.; Johnson, J.L.

    1985-02-01

    An asymptotic model is developed to study MHD equilibria in toroidal systems with a helical magnetic axis. Using a characteristic coordinate system based on the vacuum field lines, the equilibrium problem is reduced to a two-dimensional generalized partial differential equation of the Grad-Shafranov type. A stellarator-expansion free-boundary equilibrium code is modified to solve the helical-axis equations. The expansion model is used to predict the equilibrium properties of Asperators NP-3 and NP-4. Numerically determined flux surfaces, magnetic well, transform, and shear are presented. The equilibria show a toroidal Shafranov shift

  1. Neutrino transport in stellar matter

    International Nuclear Information System (INIS)

    Basdevant, J.L.

    1985-09-01

    We reconsider the neutrino transport problem in dense stellar matter which has a variety of applications among which the participation of neutrinos to the dynamics of type II supernova explosions. We describe the position of the problem and make some critiscism of previously used approximation methods. We then propose a method which is capable of handling simultaneously the optically thick, optically thin, and intermediate regimes, which is of crucial importance in such problems. The method consists in a simulation of the transport process and can be considered exact within numerical accuracy. We, finally exhibit some sample calculations which show the efficiency of the method, and present interesting qualitative physical features

  2. Characterizing Convection in Stellar Atmospheres

    International Nuclear Information System (INIS)

    Tanner, Joel; Basu, Sarbani; Demarque, Pierre; Robinson, Frank

    2011-01-01

    We perform 3D radiative hydrodynamic simulations to study the properties of convection in the superadiabatic layer of stars. The simulations show differences in both the stratification and turbulent quantities for different types of stars. We extract turbulent pressure and eddy sizes, as well as the T-τ relation for different stars and find that they are sensitive to the energy flux and gravity. We also show that contrary to what is usually assumed in the field of stellar atmospheres, the structure and gas dynamics of simulations of turbulent atmospheres cannot be parameterized with T eff and log(g) alone.

  3. On modular stellarator reactor coils

    International Nuclear Information System (INIS)

    Rau, F.; Harmeyer, E.; Kisslinger, J.; Wobig, H.

    1985-01-01

    Modular twisted coils are discussed which produce magnetic fields of the Advanced Stellarator WENDELSTEIN VII-AS type. Reducing the number coils/FP offers advantage for maintenance of coils, but increases the magnetic ripple and B m /B o . Computation of force densities within the coils of ASR and ASB yield local maximum values of about 80 and 180 MN/m 3 , respectively. A system of mutual coil support is being developed. Twisted coils in helical arrangement provide a reactor-sized HELIAC system. In order to reduce the magnetic ripple, a large number of 14 coils/FP in special arrangement is used

  4. Stellar orbits around Sgr A*

    International Nuclear Information System (INIS)

    Trippe, S; Gillessen, S; Ott, T; Eisenhauer, F; Paumard, T; Martins, F; Genzel, R; Schoedel, R; Eckart, A; Alexander, T

    2006-01-01

    In this article we present and discuss the latest results from the observations of stars (''S-stars'') orbiting Sgr A* . With improving data quality the number of observed S-stars has increased substantially in the last years. The combination of radial velocity and proper motion information allows an ever more precise determination of orbital parameters and of the mass of and the distance to the supermassive black hole in the centre of the Milky Way. Additionally, the orbital solutions allow us to verify an agreement between the NIR source Sgr A* and the dynamical centre of the stellar orbits to within 2 mas

  5. Recent advances in stellarator optimization

    Science.gov (United States)

    Gates, D. A.; Boozer, A. H.; Brown, T.; Breslau, J.; Curreli, D.; Landreman, M.; Lazerson, S. A.; Lore, J.; Mynick, H.; Neilson, G. H.; Pomphrey, N.; Xanthopoulos, P.; Zolfaghari, A.

    2017-12-01

    Computational optimization has revolutionized the field of stellarator design. To date, optimizations have focused primarily on optimization of neoclassical confinement and ideal MHD stability, although limited optimization of other parameters has also been performed. The purpose of this paper is to outline a select set of new concepts for stellarator optimization that, when taken as a group, present a significant step forward in the stellarator concept. One of the criticisms that has been leveled at existing methods of design is the complexity of the resultant field coils. Recently, a new coil optimization code—COILOPT++, which uses a spline instead of a Fourier representation of the coils,—was written and included in the STELLOPT suite of codes. The advantage of this method is that it allows the addition of real space constraints on the locations of the coils. The code has been tested by generating coil designs for optimized quasi-axisymmetric stellarator plasma configurations of different aspect ratios. As an initial exercise, a constraint that the windings be vertical was placed on large major radius half of the non-planar coils. Further constraints were also imposed that guaranteed that sector blanket modules could be removed from between the coils, enabling a sector maintenance scheme. Results of this exercise will be presented. New ideas on methods for the optimization of turbulent transport have garnered much attention since these methods have led to design concepts that are calculated to have reduced turbulent heat loss. We have explored possibilities for generating an experimental database to test whether the reduction in transport that is predicted is consistent with experimental observations. To this end, a series of equilibria that can be made in the now latent QUASAR experiment have been identified that will test the predicted transport scalings. Fast particle confinement studies aimed at developing a generalized optimization algorithm are also

  6. Introduction to stellar astrophysics. V. 1

    International Nuclear Information System (INIS)

    Boehm-Vitense, E.

    1989-01-01

    This textbook introduces basic elements of fundamental astronomy and astrophysics which serve as a foundation for understanding the structure, evolution, and observed properties of stars. The first half of the book explains how stellar motions, distances, luminosities, colours, radii, masses and temperatures are measured or derived. The author then shows how data of these sorts can be arranged to classify stars through their spectra. Stellar rotation and stellar magnetic fields are introduced. Stars with peculiar spectra and pulsating stars also merit special attention. The endpoints of stellar evolutions are briefly described. There is a separate chapter on the Sun and a final one on interstellar absorption. (author)

  7. Sobre las primeras ediciones del De re aedificatoria de Leon Battista Alberti

    Directory of Open Access Journals (Sweden)

    Suárez Quevedo, Diego

    2008-07-01

    Full Text Available El artículo glosa las dos primeras ediciones del De re aedificatoria de Alberti, ambas en latín, respectivamente de Florencia (1485, que es la edición princeps, y París (1512, a partir de los ejemplares conservados en la Biblioteca Histórica Marqués de Valdecilla. Al mismo tiempo establecer una visión paralela, entre la publicación de la primera, y la gestación y construcción del complejo de Poggio a Caiano, por parte de Lorenzo di Piero di Cosimo de’Medici (1449-1492, el Magnífico. Concluye con un acercamiento a la traducción española del De re efectuada por Francisco Lozano, y publicada en 1582, también tomando como referente el ejemplar de la Biblioteca Histórica.

  8. DESPRECIADOS Y DESECHADOS. ITINERARIO DE LA CANUTOFOBIA EN CHILE EN LA PRIMERA MITAD DEL SIGLO XX

    Directory of Open Access Journals (Sweden)

    Miguel Ángel Mansilla

    2007-12-01

    Full Text Available Este artículo analiza testimonios y relatos publicados en las Revistas Fuego de Pentecostés (RFP sobre la discriminación e intolerancia religiosa que vivieron los pentecostales chilenos en la primera mitad del siglo XX. Se describen las formas y los espacios en que se materializaron dichas actitudes y prejuicios explicitadas en distintas metáforas ignominiosas como canutos y locos, sufridos principalmente en los templos pentecostales, predicaciones callejeras y el trabajo.

  9. Primera cita de Sternopsylla distincta speciosa (Siphonaptera: Ischnopsyllidae para la provincia de Jujuy, Argentina

    Directory of Open Access Journals (Sweden)

    Analía G. AUTINO

    2005-01-01

    Full Text Available Se cita por primera vez para Jujuy la presencia de pulgas ectoparásitas de murciélagos, habiéndose registrado a Sternopsylla distincta speciosa Johnson sobre Tadarida brasiliensis (Geoffroy (Chiroptera: Vespertilionidae. Además se presentan comentarios sobre caracteres de morfología externa y estructuras genitales de las subespecies Sternopsylla distincta speciosa Johnson y Sternopsylla distincta distincta (Rothschild.

  10. Magnetohydrodynamic instabilities in a stellarator

    International Nuclear Information System (INIS)

    Matsuoka, K.; Miyamoto, K.; Ohasa, K.; Wakatani, M.

    1977-05-01

    Numerical studies of stability on kink and resistive tearing modes in a linear stellarator are presented for various current profiles and helical fields. In the case of an l = 2 helical field, a magnetic shear vanishes and the stability diagram is given by the straight lines with iota sup(σ) + iota sup(delta) = const., where iota sup(σ) is a rotational transform due to the plasma current and iota sup(delta) is due to the helical field. In the l = 2 stellarator with chi sup(delta) > 0.5, the m.h.d. stability against kink and tearing modes is improved compared with that in tokamaks. While an l = 3 helical component exists, the magnetic shear plays an important role in the stability properties. The stability diagrams become fairly complex; however, they can be explained by properties of the Euler equation. It should be noted that the internal kink modes become more unstable than in tokamaks by the l = 3 helical field. (auth.)

  11. Neoclassical transport simulations for stellarators

    International Nuclear Information System (INIS)

    Turkin, Y.; Beidler, C. D.; Maassberg, H.; Murakami, S.; Wakasa, A.; Tribaldos, V.

    2011-01-01

    The benchmarking of the thermal neoclassical transport coefficients is described using examples of the Large Helical Device (LHD) and TJ-II stellarators. The thermal coefficients are evaluated by energy convolution of the monoenergetic coefficients obtained by direct interpolation or neural network techniques from the databases precalculated by different codes. The temperature profiles are calculated by a predictive transport code from the energy balance equations with the ambipolar radial electric field estimated from a diffusion equation to guarantee a unique and smooth solution, although several solutions of the ambipolarity condition may exist when root-finding is invoked; the density profiles are fixed. The thermal transport coefficients as well as the ambipolar radial electric field are compared and very reasonable agreement is found for both configurations. Together with an additional W7-X case, these configurations represent very different degrees of neoclassical confinement at low collisionalities. The impact of the neoclassical optimization on the energy confinement time is evaluated and the confinement times for different devices predicted by transport modeling are compared with the standard scaling for stellarators. Finally, all configurations are scaled to the same volume for a direct comparison of the volume-averaged pressure and the neoclassical degree of optimization.

  12. Evaluación de medidas técnicas introducidas en las redes del litoral de Ciudad de La Habana. Parte I

    Directory of Open Access Journals (Sweden)

    Olga Susana Suárez

    2011-10-01

    Full Text Available En el trabajo se reportan los primeros resultados alcanzados en la evaluación de las medidas técnicas introducidas en las redes del litoral de Ciudad de la Habana en el proceso de rehabilitación de las redes de distribución que tiene lugar dentro de la Revolución Energética. Estas medidas fueron, principalmente, la sustitución de aisladores deporcelana por poliméricos y el cambio de las crucetas de maderas por crucetas de hierro. En esta primera parte, los resultados de un exhaustivo ciclo de ensayos de laboratorio de los parámetros eléctricos del aislador polimérico ISOELECTRIC, ciclos de ensayos de contaminación natural y contaminación artificial así como los resultados de la inspección de campo después de entre 3 y 6 meses de instalación permiten recomendar la suspensión de la instalación de este tipo de aisladores en el litoral habanero y realizar un estricto control de los ya instalados paraevitar situaciones complejas de operación. In this paper are reported the first achieved results in relation to the technical procedures applied in the littoral distribution network of Havana City in the process of distribution network rehabilitation that takes place inside the Energetic Revolution. These procedures were mainly the substitution of the porcelain for polymeric insulator. In thisfirst part, the results of the an exhaustive laboratorial test cycles of the electric parameters of ISOELECTRIC polymeric insulator, natural and artificial contamination test cycles, as well as visual inspection results after three and six moths of installation, have allowed to suggest the suspension of the installation of this type of insulators in thiszone and to carry out a strict control of those previously installed in order to avoid complex situations of operation.

  13. El prejuicio racial en Brasil: medidas comparativas O preconceito racial no Brasil: medidas comparativas Racial prejudice in Brazil: comparative measures

    Directory of Open Access Journals (Sweden)

    Ana Maria Lacerda Teixeira Pires

    2010-04-01

    Full Text Available El estudio trataba de medir las manifestaciones del prejuicio racial en una muestra de la población brasileña, utilizando las escalas de racismo moderno de McConahay, Hardee y Batts (1981 y la escala de racismo cordial de Turra y Venturi (1995 y Venturi (2003. Se aplicó los cuestionarios a un total de 101 estudiantes de diversas universidades en la región sur de Brasil. Los resultados muestran que las dos escalas difieren entre si respecto a captar las expresiones del prejuicio. Las personas declararon mayor racismo moderno que racismo cordial. También hemos estudiado las variables que influyen en el prejuicio racial declarado por los participantes. La variable género y orientación a la dominancia social son variables que predicen el racismo moderno en la muestra estudiada. Los participantes indicaron, en mayor medida, la manifestación del prejuicio racial de forma encubierta y lo hacen más abiertamente cuando hay la posibilidad del contacto personal y estrecho.O estudo avaliou as manifestações de preconceito racial em uma amostra da população brasileira, usando escalas de racismo moderno de McConahay, Hardee e Batts (1981, escala racismo cordial do Datafolha (1995 e Venturi, G. (2003. Os questionários foram aplicados a um total de 101 estudantes de várias universidades da região sul do Brasil. Os resultados mostram que as duas escalas diferem entre si sobre como capturar as expressões de preconceito. As pessoas relataram mais racismo moderno que racismo cordial. Estudamos também as variáveis que influenciam o preconceito racial declarado pelos participantes. As variáveis gênero e orientação à dominância social são preditores do racismo moderno na amostra estudada. Os participantes indicaram, em maior medida, a manifestação do preconceito racial dissimulado e o fazem mais abertamente quando existe a possibilidade do contato pessoal e estreito.This study measured the manifestations of racial prejudice in a sample of

  14. Resonancia magnética cardiaca: medidas lineales y volumétricas en adultos sanos

    OpenAIRE

    Heredia Sánchez, Fabian Mauricio; Cabezas, Andrés Mauricio

    2015-01-01

    Introducción: La gran mayoría de las medidas de normalidad utilizadas para la interpretación de resonancia cardiaca son extrapoladas de las medidas de ecocardiografía. Los limitados registros de medidas de normalidad se encuentran ajustados en poblaciones extranjeras, no hay registros en latinoamericanos. Objetivo: Determinar las dimensiones cardiacas utilizando resonancia magnética en una población de personas sin antecedente médicos con repercusión cardiaca para lograr una muestra de val...

  15. Stellar Spectral Classification with Locality Preserving Projections ...

    Indian Academy of Sciences (India)

    With the help of computer tools and algorithms, automatic stellar spectral classification has become an area of current interest. The process of stellar spectral classification mainly includes two steps: dimension reduction and classification. As a popular dimensionality reduction technique, Principal Component Analysis (PCA) ...

  16. Enhanced-confinement class of stellarators

    International Nuclear Information System (INIS)

    Mynick, H.E.; Chu, T.K.; Boozer, A.H.

    1981-08-01

    A class of stellarators has been found in which the transport is reduced by an order of magnitude from transport in conventional stellarators, by localizing the helical ripple to the inside of the torus. The reduction is observed in numerical experiments and explained theoretically

  17. Theories for convection in stellar atmospheres

    International Nuclear Information System (INIS)

    Nordlund, Aa.

    1976-02-01

    A discussion of the fundamental differences between laboratory convection in a stellar atmosphere is presented. The shortcomings of laterally homogeneous model atmospheres are analysed, and the extent to which these shortcoming are avoided in the two-component representation is discussed. Finally a qualitative discussion on the scaling properties of stellar granulation is presented. (Auth.)

  18. Structure of stellar hydroxyl masers

    International Nuclear Information System (INIS)

    Reid, M.J.; Muhleman, D.O.; Moran, J.M.; Johnston, K.J.; Schwartz, P.R.

    1977-01-01

    This paper presents the results of two spectral-line very long baseline (VLB) interferometric experiments on stellar OH masers. These masers are usually associated with long-period variable stars, and exhibit a characteristic double-peaked 1612 MHz OH spectrum. The sources IRC +10011, R Aql, and U Ori were carefully studied in order to determine the spatial structure of their masers. Maser components in these sources exhibited a complex structure which can be interpreted in terms of ''core-halo'' models. For these sources, the emission at any velocity appears to originate from a small (approximately-less-than0.''03) region of brightness approximately-greater-than10 9 K, and from a large (approximately-greater-than0.''5) region of brightness approximately-less-than10 8 K. In IRC+10011, ''core'' components in the two OH peaks probably are separated by less than the apparent size of the ''halos.'' A map of the low-velocity emission of U Ori with a resolution of 0.''01 indicates that the ''cores'' are distributed over a region of only 0.''2. This region is smaller than the apparent sizes of the ''halos.'' Other sources surveyed to determine apparent maser sizes include IRC+50137, OH 1821--12, OH 1837--05, OH 26.5+0.6, W43 A, and VX Sgr at 1612 MHz; and W Hya, R Aql, and IRC--10529 at 1667 MHz. The results of all VLB observations of 1612 MHz stellar OH masers are summarized.The apparent sizes of the strongest components (''halos'') of stellar OH masers typically are approximately-greater-than0.''5, corresponding to linear dimensions of approximately-greater-than3 x 10 15 cm. These surprisingly large sizes imply brightness temperatures much lower than those observed in most other types of astronomical masers. The large sizes rule out models of the 1612 MHz OH masers that require contracting or rotating circumstellar envelopes to explain the double-peaked OH spectra, or that try to explain the apparent maser sizes in terms of interstellar or interplanetary scattering

  19. Wisconsin torsatron/stellarator program, FY 1989

    International Nuclear Information System (INIS)

    Shohet, J.L.; Anderson, D.T.; Anderson, F.S.B.; Talmadge, J.N.

    1988-07-01

    This proposal documents recent activities within the University of Wisconsin-Madison Torsatron/Stellarator Laboratory and presents plans for future research activities for a three year period. Research efforts have focused on fundamental stellarator physics issues through experimental investigations on the Interchangeable Module Stellarator (IMS) and the Proto-Cleo Stellarator. Theoretical activities and studies of new configurations are being undertaken to support and broaden the experimental program. Experimental research at the Torsatron Stellarator Laboratory has been primarily concerned with effects induced through electron-cyclotron resonant frequency plasma production and heating in the IMS device. Plasma electric fields have been shown to play a major role in particle transport and confinement in IMS. ECRF heating at 6 kG has produced electron tail populations in agreement with Monte-Carlo models. Electric and magnetic fields have been shown to alter the particle flows to the IMS modular divertors. 48 refs

  20. Astrospheres and Solar-like Stellar Winds

    Directory of Open Access Journals (Sweden)

    Wood Brian E.

    2004-07-01

    Full Text Available Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM. These interaction regions are called "astrospheres", analogous to the "heliosphere" surrounding the Sun. The heliosphere and astrospheres contain a population of hydrogen heated by charge exchange processes that can produce enough H I Ly alpha absorption to be detectable in UV spectra of nearby stars from the Hubble Space Telescope (HST. The amount of astrospheric absorption is a diagnostic for the strength of the stellar wind, so these observations have provided the first measurements of solar-like stellar winds. Results from these stellar wind studies and their implications for our understanding of the solar wind are reviewed here. Of particular interest are results concerning the past history of the solar wind and its impact on planetary atmospheres.

  1. Stellarmak a hybrid stellarator: Spheromak

    International Nuclear Information System (INIS)

    Hartman, C.W.

    1980-01-01

    This paper discusses hybridization of modified Stellarator-like transform windings (T-windings) with a Spheromak or Field-Reversed-Mirror configuration. This configuration, Stellarmak, retains the important topological advantage of the Spheromak or FRM of having no plasma linking conductors or blankets. The T-windings provide rotational transformation in toroidal angle of the outer poloidal field lines, in effect creating a reversed B/sub Toroidal/ Spheromak or adding average B/sub T/ to the FRM producing higher shear, increased limiting β, and possibly greater stability to kinks and tilt. The presence of field ripple in the toroidal direction may be sufficient to inhibit cancellation of directed ion current by electron drag to allow steady state operation with the toroidal as well as poloidal current maintained by neutral beams

  2. Stellar Equilibrium in Semiclassical Gravity.

    Science.gov (United States)

    Carballo-Rubio, Raúl

    2018-02-09

    The phenomenon of quantum vacuum polarization in the presence of a gravitational field is well understood and is expected to have a physical reality, but studies of its backreaction on the dynamics of spacetime are practically nonexistent outside of the specific context of homogeneous cosmologies. Building on previous results of quantum field theory in curved spacetimes, in this Letter we first derive the semiclassical equations of stellar equilibrium in the s-wave Polyakov approximation. It is highlighted that incorporating the polarization of the quantum vacuum leads to a generalization of the classical Tolman-Oppenheimer-Volkoff equation. Despite the complexity of the resulting field equations, it is possible to find exact solutions. Aside from being the first known exact solutions that describe relativistic stars including the nonperturbative backreaction of semiclassical effects, these are identified as a nontrivial combination of the black star and gravastar proposals.

  3. On rapid rotation in stellarators

    International Nuclear Information System (INIS)

    Helander, Per

    2008-01-01

    The conditions under which rapid plasma rotation may occur in a three-dimensional magnetic field, such as that of a stellarator, are investigated. Rotation velocities comparable to the ion thermal speed are found to be attainable only in magnetic fields which are approximately isometric. In an isometric magnetic field the dependence of the magnetic field strength B on the arc length l along the field is the same for all field lines on each flux surface ψ. Only in fields where the departure from exact isometry, B=B(ψ,l), is of the order of the ion gyroradius divided by the macroscopic length scale are rotation speeds comparable to the ion thermal speed possible. Moreover, it is shown that the rotation must be in the direction of the vector ∇ψx∇B. (author)

  4. Magnetohydodynamics stability of compact stellarators

    International Nuclear Information System (INIS)

    Fu, G.Y.; Ku, L.P.; Cooper, W.A.; Hirshman, S.H.

    2000-01-01

    Recent stability results of external kink modes and vertical modes in compact stellarators are presented. The vertical mode is found to be stabilized by externally generated poloidal flux. A simple stability criterion is derived in the limit of large aspect ratio and constant current density. For a wall at infinite distance from the plasma, the amount of external flux needed for stabilization is given by Fi = (k2 minus k)=(k2 + 1), where k is the axisymmetric elongation and Fi is the fraction of the external rotational transform. A systematic parameter study shows that the external kink mode in QAS can be stabilized at high beta (approximately 5%) without a conducting wall by magnetic shear via 3D shaping. It is found that external kinks are driven by both parallel current and pressure gradient. The pressure contributes significantly to the overall drive through the curvature term and the Pfirsch-Schluter current

  5. NEMO: A Stellar Dynamics Toolbox

    Science.gov (United States)

    Barnes, Joshua; Hut, Piet; Teuben, Peter

    2010-10-01

    NEMO is an extendible Stellar Dynamics Toolbox, following an Open-Source Software model. It has various programs to create, integrate, analyze and visualize N-body and SPH like systems, following the pipe and filter architecture. In addition there are various tools to operate on images, tables and orbits, including FITS files to export/import to/from other astronomical data reduction packages. A large growing fraction of NEMO has been contributed by a growing list of authors. The source code consist of a little over 4000 files and a little under 1,000,000 lines of code and documentation, mostly C, and some C++ and Fortran. NEMO development started in 1986 in Princeton (USA) by Barnes, Hut and Teuben. See also ZENO (ascl:1102.027) for the version that Barnes maintains.

  6. Una medida de inflación subyacente exclusion-based para el Perú

    OpenAIRE

    Hauer, Erik Sebastián

    2015-01-01

    Hay poco consenso en la literatura sobre el diseño y evaluación de medidas de inflación subyacente. Estudios previos han mostrado que las medidas más técnicas de influencia limitada tienen mejor rendimiento empírico. Sin embargo, es deseado que las medidas de inflación subyacente sean lo más transparentes y replicables posibles, lo cual usualmente resulta en medidas más simples “exclusion-based”. A este respecto, se utiliza una nueva metodología de extracción de señal a la inflación para enco...

  7. Neoclassical transport in stellarators - a comparison of conventional stellarator/torsatrons with the advanced stellarator, Wendelstein 7X

    Energy Technology Data Exchange (ETDEWEB)

    Beidler, C D [Max-Planck-Institut fuer Plasmaphysik, Garching (Germany)

    1991-01-01

    A general expression for the magnitude of a stellarator's magnetic field, in terms of a Fourier decomposition, is too complicated to lend itself easily to analytic transport calculations. The great majority of stellarator-type devices, however, may be accurately described if one retains only those harmonics with m=0 and m=1. In the long-mean-free-path regime an analytical approximation to the particle's bounce-averaged kinetic equation can then be found. Using a numerical solution of this equation, it is possible to calculate the particle and heat fluxes due to helical-ripple transport in stellarators throughout the entire long-mean-free-path regime. 3 figs.

  8. MEDIDA SOCIOEDUCATIVA DE INTERNAÇÃO: ESTRATÉGIA PUNITIVA OU PROTETIVA?

    Directory of Open Access Journals (Sweden)

    Andrea Cristina Coelho Scisleski

    2015-12-01

    Full Text Available ResumoEste artigo problematiza como os jovens em conflito com a lei são administrados nas medidas socioeducativas de internação e busca a discussão das diferenças entre as formas de atender aqueles que recebem medidas de proteção e aqueles que recebem medidas socioeducativas. No que concerne à gestão, encontra-se uma separação na administração das medidas de proteção e das medidas socioeducativas em meio aberto, geridas pela Assistência Social, e as medidas socioeducativas de internação, geridas pela Segurança Pública. A pesquisa se desenvolveu pelo método cartográfico, que abrangeu entrevistas realizadas com profissionais do sistema socioeducativo, visitas às unidades de internação, leitura de processos jurídicos e oitivas de audiências na Vara da Infância e da Juventude. Conclui-se que a proteção integral preconizada pelo ECA não atinge todos, como é o caso dos adolescentes em conflito com a lei que estão internados, tendo seus direitos violados em prol da manutenção da segurança da população.

  9. RAZLIKE MED PODJETNIKI IN PODJETNICAMI V SLOVENIJI: ŠTUDIJA PRIMERA

    OpenAIRE

    Sekavčnik, Marjeta

    2013-01-01

    Namen diplomskega seminarja je bil ugotoviti kakšne so razlike med podjetniki in podjetnicami v Sloveniji in zakaj do njih prihaja. Tega smo se lotili tako, da smo diplomski seminar razdelili na dva večja dela in sicer na teoretični in empirični del oz. študijo primera. Pri teoretičnem delu smo se najprej seznanili z osnovnimi pojmi podjetništva, spoznali kakšni so razlogi (motivi) podjetnikov in podjetnic, da se odločijo za podjetniško kariero, ugotovili kakšne so njihove osebnostne znači...

  10. La premsa valenciana en la primera dècada del segle XXI

    OpenAIRE

    Martínez Sanchis, Francesc; González i Montserrat Jurado, José Luis; Doménech Fabregat, Hugo

    2011-01-01

    La premsa valenciana d'informació general en la primera dècada del segle XXI es caracteritza per l'aposta multimèdia dels grans diaris regionals, el domini del castellà com a llengua de comunicació i una forta expansió deis periódics gratuïts impresos i els diaris digitals. La premsa actual continua tenint la província com a límit. No hi ha una premsa regional de forta implantació en tot el territori valencià. In the first decade of the 21st century, the Valencia...

  11. La vigilancia de factores vinculados al desarrollo, el aprendizaje y la salud en la primera infancia

    OpenAIRE

    Ojeda del Valle, Mayra

    2012-01-01

    Se desarrollaron tres investigaciones entre 1997-2007 con el objetivo de perfeccionar la vigilancia de los factores vinculados al desarrollo, el aprendizaje y la salud en la primera infancia. Fueron identificados factores asociados al desarrollo y a la respuesta adaptativa de los niños asistentes a instituciones infantiles, se evaluaron indicadores del neurodesarrollo infantil asociados al aprendizaje escolar en la Atención Primaria y se realizó la pesquisa de factores de riesgo en niños pree...

  12. Hydrodynamics and stellar winds an introduction

    CERN Document Server

    Maciel, Walter J

    2014-01-01

    Stellar winds are a common phenomenon in the life of stars, from the dwarfs like the Sun to the red giants and hot supergiants, constituting one of the basic aspects of modern astrophysics. Stellar winds are a hydrodynamic phenomenon in which circumstellar gases expand towards the interstellar medium. This book presents an elementary introduction to the fundamentals of hydrodynamics with an application to the study of stellar winds. The principles of hydrodynamics have many other applications, so that the book can be used as an introduction to hydrodynamics for students of physics, astrophysics and other related areas.

  13. Ultraviolet photometry of stellar populations in galaxies

    International Nuclear Information System (INIS)

    Deharveng, J.M.

    1981-01-01

    The UV flux of stellar populations, which is essentially emitted by young stars, conveys information on the process of star formation and its recent history. However, the evaluation of the flux arising from the young stellar component may be difficult. In the case of late type galaxies it is hampered by the extinction and the effect of scattered stellar radiation. In the case of early type galaxies, the star formation, if any, has to be disentangled from the contribution of hot evolved stars and of a possible 'active' phenomenon. A review of observations and results relevant two cases is presented [fr

  14. Helical post stellarator. Part 1: Vacuum configuration

    International Nuclear Information System (INIS)

    Moroz, P.E.

    1997-08-01

    Results on a novel type of stellarator configuration, the Helical Post Stellarator (HPS), are presented. This configuration is different significantly from all previously known stellarators due to its unique geometrical characteristics and unique physical properties. Among those are: the magnetic field has only one toroidal period (M = 1), the plasma has an extremely low aspect ratio, A ∼ 1, and the variation of the magnetic field, B, along field lines features a helical ripple on the inside of the torus. Among the main advantages of a HPS for a fusion program are extremely compact, modular, and simple design compatible with significant rotational transform, large plasma volume, and improved particle transport characteristics

  15. Medidas automatizadas de psicrômetro de termopar aspirado versus não aspirado

    Directory of Open Access Journals (Sweden)

    Antonio Ribeiro da Cunha

    2014-06-01

    Full Text Available O termopar ou par termoelétrico é utilizado na obtenção da temperatura do ar com ótima precisão, sensibilidade e com grande vantagem sobre o termômetro de mercúrio ou álcool, pois geram sinais elétricos que podem ser armazenados em sistemas automatizados. No entanto, quando se trata da obtenção da umidade relativa a partir de termopar, o processo se torna mais cauteloso devido a outros fatores envolvidos. Neste estudo, avaliaram-se dois conjuntos psicrômetros de termopar, aspirado e não aspirado, em relação a um conjunto Vaisala, no período de 17 a 31/01/2008 (15 dias. A partir de medidas de temperaturas de bulbos seco e úmido foram obtidas medidas da umidade relativa, e com isso, foi possível compará-las com as medidas obtidas pelo conjunto Vaisala. Os dois tipos de psicrômetros apresentaram precisão e exatidão nas medidas de temperatura do ar, e apenas precisão nas medidas de umidade relativa do ar, sendo que o psicrômetro aspirado foi o mais preciso. Apesar do psicrômetro não aspirado ter apresentado menor precisão nas medidas, ele é mais robusto porque independe do micro-ventilador de 12 VDC, o que faz dele um sensor com menos riscos de medidas inadequadas. Ambos os psicrômetros, aspirado e não aspirado, não medem com exatidão a umidade relativa do ar no período noturno.

  16. Stellar X-Ray Polarimetry

    Science.gov (United States)

    Swank, J.

    2011-01-01

    Most of the stellar end-state black holes, pulsars, and white dwarfs that are X-ray sources should have polarized X-ray fluxes. The degree will depend on the relative contributions of the unresolved structures. Fluxes from accretion disks and accretion disk corona may be polarized by scattering. Beams and jets may have contributions of polarized emission in strong magnetic fields. The Gravity and Extreme Magnetism Small Explorer (GEMS) will study the effects on polarization of strong gravity of black holes and strong magnetism of neutron stars. Some part of the flux from compact stars accreting from companion stars has been reflected from the companion, its wind, or accretion streams. Polarization of this component is a potential tool for studying the structure of the gas in these binary systems. Polarization due to scattering can also be present in X-ray emission from white dwarf binaries and binary normal stars such as RS CVn stars and colliding wind sources like Eta Car. Normal late type stars may have polarized flux from coronal flares. But X-ray polarization sensitivity is not at the level needed for single early type stars.

  17. Stellar recipes for axion hunters

    Energy Technology Data Exchange (ETDEWEB)

    Giannotti, Maurizio [Physical Sciences, Barry University, 11300 NE 2nd Ave., Miami Shores, FL 33161 (United States); Irastorza, Igor G.; Redondo, Javier [Departamento de Física Teórica, Universidad de Zaragoza, Pedro Cerbuna 12, E-50009, Zaragoza (Spain); Ringwald, Andreas; Saikawa, Ken' ichi, E-mail: mgiannotti@barry.edu, E-mail: igor.irastorza@cern.ch, E-mail: jredondo@unizar.es, E-mail: andreas.ringwald@desy.de, E-mail: kenichi.saikawa@desy.de [Theory Group, Deutsches Elektronen-Synchrotron DESY, Notkestraße 85, D-22607 Hamburg (Germany)

    2017-10-01

    There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new sub-keV mass pseudoscalar Nambu-Goldstone boson with tiny couplings to photons, electrons, and nucleons. An attractive possibility is to identify this particle with the axion—the hypothetical pseudo Nambu-Goldstone boson predicted by the Peccei-Quinn solution to the strong CP problem. We explore this possibility in terms of a DFSZ-type axion and of a KSVZ-type axion/majoron, respectively. Both models allow a good global fit to the data, prefering an axion mass around 10 meV. We show that future axion experiments—the fifth force experiment ARIADNE and the helioscope IAXO—can attack the preferred mass range from the lower and higher end, respectively. An axion in this mass range can also be the main constituent of dark matter.

  18. Stellar recipes for axion hunters

    Energy Technology Data Exchange (ETDEWEB)

    Giannotti, Maurizio [Barry Univ., Miami Shores, FL (United States). Physical Sciences; Irastorza, Igor G. [Zaragoza Univ. (Spain). Dept. de Fisica Teorica; Redondo, Javier [Zaragoza Univ. (Spain). Dept. de Fisica Teorica; Max-Planck-Institut fuer Physik, Muenchen (Germany); Ringwald, Andreas; Saikawa, Ken' ichi [DESY, Hamburg (Germany). Theory Group

    2017-08-15

    There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new sub-keV mass pseudoscalar Nambu-Goldstone boson with tiny couplings to photons, electrons, and nucleons. An attractive possibility is to identify this particle with the axion - the hypothetical pseudo Nambu-Goldstone boson predicted by the Peccei-Quinn solution to the strong CP problem. We explore this possibility in terms of a DFSZ-type axion and of a KSVZ-type axion/majoron, respectively. Both models allow a good global fit to the data, prefering an axion mass around 10 meV. We show that future axion experiments - the fifth force experiment ARIADNE and the helioscope IAXO - can attack the preferred mass range from the lower and higher end, respectively. An axion in this mass range can also be the main constituent of dark matter.

  19. Stellar recipes for axion hunters

    International Nuclear Information System (INIS)

    Giannotti, Maurizio; Ringwald, Andreas; Saikawa, Ken'ichi

    2017-08-01

    There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new sub-keV mass pseudoscalar Nambu-Goldstone boson with tiny couplings to photons, electrons, and nucleons. An attractive possibility is to identify this particle with the axion - the hypothetical pseudo Nambu-Goldstone boson predicted by the Peccei-Quinn solution to the strong CP problem. We explore this possibility in terms of a DFSZ-type axion and of a KSVZ-type axion/majoron, respectively. Both models allow a good global fit to the data, prefering an axion mass around 10 meV. We show that future axion experiments - the fifth force experiment ARIADNE and the helioscope IAXO - can attack the preferred mass range from the lower and higher end, respectively. An axion in this mass range can also be the main constituent of dark matter.

  20. Stellar core collapse and supernova

    International Nuclear Information System (INIS)

    Wilson, J.R.; Mayle, R.; Woosley, S.E.; Weaver, T.

    1985-04-01

    Massive stars that end their stable evolution as their iron cores collapse to a neutron star or black hole long been considered good candidates for producing Type II supernovae. For many years the outward propagation of the shock wave produced by the bounce of these iron cores has been studied as a possible mechanism for the explosion. For the most part, the results of these studies have not been particularly encouraging, except, perhaps, in the case of very low mass iron cores or very soft nuclear equations of state. The shock stalls, overwhelmed by photodisintegration and neutrino losses, and the star does not explode. More recently, slow late time heating of the envelope of the incipient neutron star has been found to be capable of rejuvenating the stalled shock and producing an explosion after all. The present paper discusses this late time heating and presents results from numerical calculations of the evolution, core collapse, and subsequent explosion of a number of recent stellar models. For the first time they all, except perhaps the most massive, explode with reasonable choices of input physics. 39 refs., 17 figs., 1 tab

  1. Stellar convection and dynamo theory

    Energy Technology Data Exchange (ETDEWEB)

    Jennings, R L

    1989-10-01

    In considering the large scale stellar convection problem the outer layers of a star are modelled as two co-rotating plane layers coupled at a fluid/fluid interface. Heating from below causes only the upper fluid to convect, although this convection can penetrate into the lower fluid. Stability analysis is then used to find the most unstable mode of convection. With parameters appropriate to the Sun the most unstable mode is steady convection in thin cells (aspect ratio {approx equal} 0.2) filling the convection zone. There is negligible vertical motion in the lower fluid, but considerable thermal penetration, and a large jump in helicity at the interface, which has implications for dynamo theory. An {alpha}{omega} dynamo is investigated in isolation from the convection problem. Complexity is included by allowing both latitudinal and time dependence in the magnetic fields. The nonlinear dynamics of the resulting partial differential equations are analysed in considerable detail. On varying the main control parameter D (the dynamo number), many transitions of behaviour are found involving many forms of time dependence, but not chaos. Further, solutions which break equatorial symmetry are common and provide a theoretical explanation of solar observations which have this symmetry. Overall the behaviour was more complicated than expected. In particular, there were multiple stable solutions at fixed D, meaning that similar stars can have very different magnetic patterns, depending upon their history. (author).

  2. Collapsing stellar cores and supernovae

    Energy Technology Data Exchange (ETDEWEB)

    Epstein, R J [Nordisk Inst. for Teoretisk Atomfysik, Copenhagen (Denmark); Noorgaard, H [Nordisk Inst. for Teoretisk Atomfysik, Copenhagen (Denmark); Chicago Univ., IL (USA). Enrico Fermi Inst.); Bond, J R [Niels Bohr Institutet, Copenhagen (Denmark); California Inst. of Tech., Pasadena (USA). W.K. Kellogg Radiation Lab.)

    1979-05-01

    The evolution of a stellar core is studied during its final quasi-hydrostatic contraction. The core structure and the (poorly known) properties of neutron rich matter are parametrized to include most plausible cases. It is found that the density-temperature trajectory of the material in the central part of the core (the core-center) is insensitive to nearly all reasonable parameter variations. The central density at the onset of the dynamic phase of the collapse (when the core-center begins to fall away from the rest of the star) and the fraction of the emitted neutrinos which are trapped in the collapsing core-center depend quite sensitively on the properties of neutron rich matter. We estimate that the amount of energy Ecm which is imparted to the core-mantle by the neutrinos which escape from the imploded core-center can span a large range of values. For plausible choices of nuclear and model parameters Ecm can be large enough to yield a supernova event.

  3. Opinión sobre el rol y perfil del educador para la primera infancia

    Directory of Open Access Journals (Sweden)

    Beatriz Elena Zapata

    2010-10-01

    Full Text Available En este artículo presentamos los resultados consolidados de la investigación desarrollada entre Chile y Colombia “Opinión que se tiene sobre el rol del profesional de la educación para la primera infancia en dos países latinoamericanos”, una descripción levantada desde las opiniones aportadas por comunidades diversas (directivos docentes, docentes, apoderados de la educación, familias , estudiantes y profesionales de otras áreas; estudio de carácter cualitativo explicativo en el cual participan 10 universidades, miembros de la Omep (Organización Mundial de Educación Preescolar. El estudio tuvo como propósito la caracterización del rol y perfil del educador para la primera infancia, el cual se realiza desde el enfoque de competencias y en el marco de las Políticas Públicas que a nivel de Latinoamérica se han gestado en las últimas décadas en torno a la atención integral y educación de los niños y niñas.

  4. ANTECEDENTES HISTÓRICOS DEL ESTUDIO DEL CRECIMIENTO GENERAL Y CRANEOFACIAL HUMANO EN LA PRIMERA INFANCIA

    Directory of Open Access Journals (Sweden)

    Laila Yaned González Bejarano

    2012-01-01

    Full Text Available En la primera infancia de 0 a 3 años, el crecimiento general y craneofacial muestra grandes cambios en cuanto a velocidad, tamaño, forma y función, atribuidos a factores genéticos y ambientales. La presente revisión pretende profundizar en los estudios de crecimiento general y craneofacial en edades tempranas, realizados a partir del siglo XVIII que han servido como referente para entender su comportamiento, variabilidad y conocer los factores determinantes que puedan influir en su curso normal; tales como la nutrición, las condiciones socioeconómicas, ecogeográficas de salud general y oral. A nivel craneofacial, los estudios longitudinales y  transversales son los más utilizados y la antropometría la principal técnica de medición. Colombia requiere de estudios que caractericen el crecimiento craneofacial en la primera infancia para entender la normalidad y construir patrones de referencia que apoyen  los programas de promoción de la salud, el diagnóstico y tratamiento quirúrgico correctivo en niños con malformaciones.

  5. Cambios en la mentalización de los afectos en maestras de primera infancia

    Directory of Open Access Journals (Sweden)

    2013-10-01

    Full Text Available En el artículo presentamos el impacto que tuvo sobre la elaboración de los afectos un programa de intervención para favorecer la mentalización, dirigido a diez maestras de primera infancia de la ciudad de Cali. El objetivo fue identificar cambios en el modo de representación y en el nivel de tolerancia de los afectos. El método utilizado fue descriptivo. Evaluamos la forma de representación y el nivel de tolerancia de los afectos basándonos en las categorías del instrumento Verbal Elaboration of Affect (VEA propuesto por Lecours y Bouchard. Se utilizaron narraciones de eventos dolorosos recordados por las maestras al inicio y al final del programa. Los resultados mostraron que hubo cambios positivos en la mentalización del afecto. No obstante en la discusión dejamos abierta la pregunta sobre su permanencia en el tiempo y señalamos la importancia que tiene que las maestras de primera infancia tengan la oportunidad de elaborar sus experiencias emocionales infantiles.

  6. LA COLECTIVIDAD BRITÁNICA EN VALPARAÍSO DURANTE LA PRIMERA MITAD DEL SIGLO XX

    Directory of Open Access Journals (Sweden)

    BALDOMERO ESTRADA TURRA

    2006-06-01

    Full Text Available En este trabajo analizamos la importancia de la colectividad británica en el desarrollo económico de Valparaíso (Chile, pese a su limitada presencia, durante la primera mitad del siglo XX. Se hace notar el predominio de la colectividad el comercio internacional como también en la actividad industrial especialmente en aquellas que poseían un mayor desarrollo tecnológico. La disminución de la importancia económica y también demográfica de la colectividad británica en Valparaíso, a partir de la década de 1920, se relaciona directamente con la perdida de influencia británica, en nuestro Continente, luego de la Primera Guerra MundialIn this work we analyze the importance of the british immigrants in the economic development of Valparaiso during the first half of twenty century. We highlight their predominance in the international trade and in the industrial activity especially those that reveal a high technological development. The economic and demographic decline of the british immigrants from 1920 is in close relation with the lost of the british influence in Latin America after the First World War

  7. Diagnostics for the National Compact Stellarator Experiment

    International Nuclear Information System (INIS)

    Stratton, B.C.; Johnson, D.; Feder, R.; Fredrickson, E.; Neilson, H.; Takahashi, H.; Zarnstorf, M.; Cole, M.; Goranson, P.; Lazarus, E.; Nelson, B.

    2003-01-01

    The status of planning of the National Compact Stellarator Experiment (NCSX) diagnostics is presented, with the emphasis on resolution of diagnostics access issues and on diagnostics required for the early phases of operation

  8. Stellar Spectral Classification with Locality Preserving Projections ...

    Indian Academy of Sciences (India)

    School of Computer and Control Engineering, North University of China,. Taiyuan 030051 ... (2013) was used to mine the association rules of a stellar ... of the graph, we then compute a transformation matrix which maps the data points to.

  9. The relation between stellar evolution and cosmology

    International Nuclear Information System (INIS)

    Tayler, R.J.

    1984-01-01

    Observations of star clusters combined with the theory of stellar evolution enable us to estimate the ages of stars while cosmological observations and theories give us a value for the age of the Universe. This is the most important interaction between cosmology and stellar evolution because it is clearly necessary that stars are younger than the Universe. Stellar evolution also plays an important role in relating the present chemical composition of the Universe to its original composition. The author restricts the review to a discussion of the relation between stellar evolution and the big bang cosmological theory because there is such a good qualitative agreement between the hot big bang theory and observations. (Auth.)

  10. Evaluating Stellarator Divertor Designs with EMC3

    Science.gov (United States)

    Bader, Aaron; Anderson, D. T.; Feng, Y.; Hegna, C. C.; Talmadge, J. N.

    2013-10-01

    In this paper various improvements of stellarator divertor design are explored. Next step stellarator devices require innovative divertor solutions to handle heat flux loads and impurity control. One avenue is to enhance magnetic flux expansion near strike points, somewhat akin to the X-Divertor concept in Tokamaks. The effect of judiciously placed external coils on flux deposition is calculated for configurations based on the HSX stellarator. In addition, we attempt to optimize divertor plate location to facilitate the external coil placement. Alternate areas of focus involve altering edge island size to elucidate the driving physics in the edge. The 3-D nature of stellarators complicates design and necessitates analysis of new divertor structures with appropriate simulation tools. We evaluate the various configurations with the coupled codes EMC3-EIRENE, allowing us to benchmark configurations based on target heat flux, impurity behavior, radiated power, and transitions to high recycling and detached regimes. Work supported by DOE-SC0006103.

  11. Development of the stellarator/heliotron research

    International Nuclear Information System (INIS)

    Iiyoshi, A.

    1991-05-01

    The author reviewed the history of the development of the stellarator/heliotron system, and pointed out the important role of the radial electric field in plasma transport in helical devices. (J.P.N.)

  12. Radiative otacity tables for 40 stellar mixtures

    International Nuclear Information System (INIS)

    Cox, A.N.; Tabor, J.E.

    1976-01-01

    Using improved methods, radiative opacities for 40 mixtures of elements are given for use in calculations of stellar structure, stellar evolution, and stellar pulsation. The major improvements over previous Los Alamos data are increased iron abundance in the composition, better allowance for the continuum depression for bound electrons, and corrections in some bound-electron energy levels. These opacities have already been widely used, and represent a relatively homogeneous set of data for stellar structures. Further improvements to include more bound-bound (line) transitions by a smearing technique and to include molecular absorptions are becoming available, and in a few years these tables, as well as all previous tables, will be outdated. At high densities the conduction of energy will dominate radiation flow, and this effect must be added separately

  13. STELLAR ATMOSPHERES, ATMOSPHERIC EXTENSION, AND FUNDAMENTAL PARAMETERS: WEIGHING STARS USING THE STELLAR MASS INDEX

    Energy Technology Data Exchange (ETDEWEB)

    Neilson, Hilding R.; Lester, John B. [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON, M5S 3H4 (Canada); Baron, Fabien; Norris, Ryan; Kloppenborg, Brian, E-mail: neilson@astro.utoronto.ca [Center for High Angular Resolution Astronomy, Department of Physics and Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302-5060 (United States)

    2016-10-20

    One of the great challenges of understanding stars is measuring their masses. The best methods for measuring stellar masses include binary interaction, asteroseismology, and stellar evolution models, but these methods are not ideal for red giant and supergiant stars. In this work, we propose a novel method for inferring stellar masses of evolved red giant and supergiant stars using interferometric and spectrophotometric observations combined with spherical model stellar atmospheres to measure what we call the stellar mass index, defined as the ratio between the stellar radius and mass. The method is based on the correlation between different measurements of angular diameter, used as a proxy for atmospheric extension, and fundamental stellar parameters. For a given star, spectrophotometry measures the Rosseland angular diameter while interferometric observations generally probe a larger limb-darkened angular diameter. The ratio of these two angular diameters is proportional to the relative extension of the stellar atmosphere, which is strongly correlated to the star’s effective temperature, radius, and mass. We show that these correlations are strong and can lead to precise measurements of stellar masses.

  14. Does the stellar distribution flare? A comparison of stellar scale heights with LAB H I data

    Energy Technology Data Exchange (ETDEWEB)

    Kalberla, P. M. W.; Kerp, J.; Dedes, L. [Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn (Germany); Haud, U., E-mail: pkalberla@astro.uni-bonn.de [Tartu Observatory, 61602 Tõravere (Estonia)

    2014-10-10

    The question of whether the stellar populations in the Milky Way take part in the flaring of scale heights as observed for the H I gas is a matter of debate. Standard mass models for the Milky Way assume a constant scale height for each of the different stellar distributions. However, there is mounting evidence that at least some of the stellar distributions reach, at large galactocentric distances, high altitudes, which are incompatible with a constant scale height. We discuss recent observational evidence for stellar flaring and compare it with H I data from the Leiden/Argentine/Bonn survey. Within the systemic and statistical uncertainties we find a good agreement between both.

  15. The WEGA Stellarator: Results and Prospects

    International Nuclear Information System (INIS)

    Otte, M.; Andruczyk, D.; Koenig, R.; Laqua, H. P.; Lischtschenko, O.; Marsen, S.; Schacht, J.; Podoba, Y. Y.; Wagner, F.; Warr, G. B.; Holzhauer, E.; Howard, J.; Krupnik, L.; Zhezhera, A.; Urban, J.; Preinhalter, J.

    2008-01-01

    In this article an overview is given on results from magnetic flux surface measurements, applied ECR heating scenarios for 2.45 GHz and 28 GHz, fluctuation and transport studies and plasma edge biasing experiments performed in the WEGA stellarator. Examples for the development of new diagnostics and the machine control system are given that will be used at Wendelstein 7-X stellarator, which is currently under construction in Greifswald

  16. Cosmic abundances: The impact of stellar duplicity

    OpenAIRE

    Jorissen, A.; Van Eck, S.

    2004-01-01

    The mass-transfer scenario links chemical peculiarities with stellar duplicity for an increasing number of stellar classes (classical and dwarf barium stars, subgiant and giant CH stars, S stars without technetium, yellow symbiotic stars, WIRRING stars, Abell-35-like nuclei of planetary nebulae...). Despite these successes, the mass-transfer scenario still faces several problems: What is the mass-transfer mode? Why orbital elements of dwarf barium stars do not fully match those of the classic...

  17. The Stellar-Dynamical Oeuvre James Binney

    Indian Academy of Sciences (India)

    tribpo

    of the eigenvalues of M. The variation of the stellar density from point to point .... of Σ,(ΔΕ)2 , where ∆ Ε is the change in energy that a star suffers during a binary ... could use these results to calculate the relaxation time in a stellar system if he .... the region of enhanced density that tails behind it like a wake behind a ship. By.

  18. Weakly interacting massive particles and stellar structure

    International Nuclear Information System (INIS)

    Bouquet, A.

    1988-01-01

    The existence of weakly interacting massive particles (WIMPs) may solve both the dark matter problem and the solar neutrino problem. Such particles affect the energy transport in the stellar cores and change the stellar structure. We present the results of an analytic approximation to compute these effects in a self-consistent way. These results can be applied to many different stars, but we focus on the decrease of the 8 B neutrino flux in the case of the Sun

  19. Close stellar encounters in globular clusters

    International Nuclear Information System (INIS)

    Bailyn, C.D.

    1989-01-01

    Stellar encounters are expected to produce a variety of interesting objects in the cores of globular clusters, either through the formation of binaries by tidal capture, or direct collisions. Here, I describe several attempts to observe the products of stellar encounters. In particular, the use of color maps has demonstrated the existence of a color gradient in the core of M15, which seems to be caused by a population of faint blue objects concentrated towards the cluster center. (author)

  20. On plasma radiative properties in stellar conditions

    International Nuclear Information System (INIS)

    Turck-Chieze, S.; Delahaye, F.; Gilles, D.; Loisel, G.; Piau, L.; Loisel, G.

    2009-01-01

    The knowledge of stellar evolution is evolving quickly thanks to an increased number of opportunities to scrutinize the stellar internal plasma properties by stellar seismology and by 1D and 3D simulations. These new tools help us to introduce the internal dynamical phenomena in stellar modeling. A proper inclusion of these processes supposes a real confidence in the microscopic physics used, partly checked by solar or stellar acoustic modes. In the present paper we first recall which fundamental physics has been recently verified by helioseismology. Then we recall that opacity is an important ingredient of the secular evolution of stars and we point out why it is necessary to measure absorption coefficients and degrees of ionization in the laboratory for some well identified astrophysical conditions. We examine two specific experimental conditions which are accessible to large laser facilities and are suitable to solve some interesting questions of the stellar community: are the solar internal radiative interactions properly estimated and what is the proper role of the opacity in the excitation of the non-radial modes in the envelop of the β Cepheids and the Be stars? At the end of the paper we point out the difficulties of the experimental approach that we need to overcome. (authors)

  1. Comparative studies of stellarator and tokamak transport

    Energy Technology Data Exchange (ETDEWEB)

    Stroth, U; Burhenn, R; Geiger, J; Giannone, L.; Hartfuss, H J; Kuehner, G; Ledl, L; Simmet, E E; Walter, H [Max-Planck-Inst. fuer Plasmaphysik, IPP-Euratom Association, Garching (Germany); ECRH Team; W7-AS Team

    1997-09-01

    Transport properties in the W7-AS stellarator and in tokamaks are compared. The parameter dependences and the absolute values of the energy confinement time are similar. Indications are found that the density dependence, which is usually observed in stellarator confinement, can vanish above a critical density. The density dependence in stellarators seems to be similar to that in the linear ohmic confinement regime, which, in small tokamaks, extends to high density values, too. Because of the similarity in the gross confinement properties, transport in stellarators and tokamaks should not be dominated by the parameters which are very different in the two concepts, i.e. magnetic shear, major rational values of the rotational transform and plasma current. A difference in confinement is that there exists evidence for pinches in the particle and, possibly, energy transport channels in tokamaks whereas in stellarators no pinches have been observed, so far. In order to study the effect of plasma current and toroidal electric fields, stellarator discharges were carried out with an increasing amount of plasma current. From these experiments, no clear evidence of a connection of pinches with these parameters is found. The transient response in W7-AS plasmas can be described in terms of a non-local model. As in tokamaks, also cold pulse experiments in W7-AS indicate the importance of non-local transport. (author). 8 refs, 5 figs.

  2. desarrollo y validación de un instrumento de medida

    Directory of Open Access Journals (Sweden)

    Arménio Rego

    2005-01-01

    Full Text Available El artículo describe cómo un instrumento de medida de la Inteligencia Emocional fue construido y validado. Cuatro etapas fueron seguidas: 1 Fueron escritos 96 ítems con base en la literatura y en trabajo propio de los autores; 2 Fue elaborado un cuestionario y aplicado a una muestra de 339 individuos; 3 Se procedió a un análisis factorial de las componentes principales; 4 Se relacionaron los factores emergentes con una medida de satisfacción con la vida. Los resultados sugirieron una solución factorial de seis componentes. Las consistencias internas de las escalas son invariablemente superiores a 0.70. Las seis dimensiones explican el 29% de la varianza de la medida de satisfacción con la vida

  3. La reconversión del estado durante la primera gobernación de Duhalde en la provincia de Buenos Aires The State's Process of Reform in Province of Buenos Aires during Duhalde's First Government

    Directory of Open Access Journals (Sweden)

    María Cecilia Erbetta

    2011-06-01

    Full Text Available El objetivo principal de este trabajo es mostrar el inicio en la provincia de Buenos Aires, a partir de la ley 11.184, del proceso de reforma del Estado provincial durante la primera gobernación de Eduardo Duhalde. Esto es, indagar en qué medida el contexto le otorga sentido a las prácticas y discursos de sus protagonistas, a fin de comprender cómo conviven simultáneamente una política de ajuste con la llegada de nuevos fondos de origen federal.O objetivo principal deste trabalho é mostrar o início na província de Buenos Aires, a partir da lei 11.184, do processo de reforma do Estado provincial durante o primeiro governo de Eduardo Duhalde. Isto é, indagar em que medida o contexto outorga sentido às práticas e discursos de seus protagonistas, a fim de compreender como convive simultaneamente uma política de ajuste com a chegada de novos fundos de origem federal.The principal aim of this article is to describe the beginnings of the Provincial State's process of reform in the Province of Buenos Aires, which started with the law 11.184, during Eduardo Duhalde's first government,. This is, to study in which way the context gives sense to the practices and speeches of its main actors, in order to understand how an adjustment policy coexists with the arrival of new public funds of federal origin.

  4. Use of the stellarator expansion to investigate plasma equilibrium in modular stellarators

    International Nuclear Information System (INIS)

    Anania, G.; Johnson, J.L.; Weimer, K.E.

    1982-11-01

    A numerical code utilizing a large-aspect ratio, small-helical-distortion expansion is developed and used to investigate the effect of plasma currents on stellarator equilibrium. Application to modular stellarator configurations shows that a large rotational transform, and hence large coil deformation, is needed to achieve high-beta equilibria

  5. Consecuencias de las medidas no arancelarias impuestas a Colombia por Ecuador y Argentina

    OpenAIRE

    Perez Giraldo, Johanna Sembelly; Vargas, William

    2016-01-01

    Con la apertura económica y comercial ha aumentado la negociación de acuerdos comerciales por medio de los cuales los países han logrado tener acceso preferencial libre de aranceles aduaneros. Esta dinámica ha incrementado el uso de medidas no arancelaria como instrumentos para controlar y restringir el acceso a los mercados de los países. Por lo expuesto, esta investigación presenta y analiza las medidas no arancelarias que fueron aplicadas a Colombia por Ecuador y Argentina desde el año 201...

  6. Ilustração de incertezas em medidas utilizando experimentos de queda livre

    OpenAIRE

    Coluci,Vitor R.; Paulino,Guilherme; Souza,Diego C. de; Vasconcelos,Elba P.R.

    2013-01-01

    O conhecimento da incerteza de uma medida é crucial para obter conclusões a partir de resultados experimentais. Erros aleatórios, comuns em experimentos, produzem uma distribuição dos valores medidos que segue o formato gaussiano. Neste trabalho desenvolvemos uma montagem baseada no fenômeno de queda livre para auxiliar na ilustração do conceito de incerteza em medidas. Os tempos de queda de um objeto foram obtidos automaticamente pela placa Arduino e exibidos na forma de um histograma na tel...

  7. Aplicaciones de los modelos multinivel al análisis de medidas repetidas en estudios longitudinales

    OpenAIRE

    María Victoria Zunzunegui; María Jesús García de Yébenes; Mathieu Forster; María Dolores Aguilar Conesa; Angel Rodríguez Laso; Ángel Otero

    2004-01-01

    Este trabajo es una introducción al análisis de medidas repetidas en estudios longitudinales. Se utiliza un marco analítico con dos etapas, ajustando modelos jerárquicos lineales con dos niveles. El primer nivel corresponde a la ocasión (tiempo) de medida y el segundo al individuo. Estos modelos estadísticos proceden de las ciencias sociales, en las que se han utilizado durante más de 25 años para analizar datos en organizaciones con múltiples niveles. Su aplicación permi...

  8. LAS MEDIDAS PREVENTIVAS AMBIENTALES, UNA APROXIMACIÓN DESDE EL DERECHO ADMINISTRATIVO.

    Directory of Open Access Journals (Sweden)

    Iván Andrés Páez Páez

    2013-05-01

    Full Text Available Las medidas preventivas previstas en el régimen sancionatorio ambiental sonuna especie de las medidas cautelares consagradas en el ordenamiento jurídicocolombiano, aunque con algunas particularidades propias de su ámbito deaplicación, que es el derecho ambiental. El artículo realiza una aproximaciónrespecto al contenido, alcance, antecedentes y justificación de las medidaspreventivas ambientales desde la óptica del derecho administrativo y comomanifestación de una de las funciones del ejecutivo, cual es el mantenimientodel orden público.

  9. Nodo sensor para la medida ambiental de CO2, temperatura y humedad

    OpenAIRE

    Jara Burgos, Marcos

    2007-01-01

    En este documento se describe el diseño y la implementación de un nodo sen-sor para la medida ambiental del nivel de CO2, la temperatura y la humedad relativa. El sistema se basa en un interfaz directo sensor a microcontrolador para las medidas de temperatura y humedad relativa, mientras que para el sensor de CO2 se basa en una conversión analógica digital. El sistema utiliza un sensor resistivo para medir la temperatura, un sensor capacitivo para medir la humedad relativa y un sensor...

  10. Medidas preventivas, correctoras y compensatorias del impacto ecológico de carreteras

    OpenAIRE

    Aizpurúa Giráldez, Nerea

    2011-01-01

    Las medidas preventivas, correctoras y compensatorias empleadas en los proyectos de carretera son uno de los elementos clave para conseguir la integración ambiental de estas infraestructuras. De ellas dependerá que los posibles impactos ambientales generados durante su construcción y explotación no supongan un detrimento inadmisible de la calidad ambiental. La tipología de medidas que se vienen aplicando desde hace más de veinte años en durante el proceso de Evaluación de Impacto Ambiental (E...

  11. La arquitectura de la primera modernidad en San Miguel de Tucumán, Argentina

    Directory of Open Access Journals (Sweden)

    Susana Villavicencio

    2013-12-01

    A partir del estudio de material planimétrico y fotográfico de los ejemplos de la Primera Modernidad (1935-1950 en San Miguel de Tucumán, se elaboró un cuerpo de conocimiento que se confrontó con datos de la historia local, dando como resultado el registro de un período peculiar de la historia de la ciudad. Este conjunto de obras, ubicadas en su mayoría en el área central de San Miguel de Tucumán, conforma un patrimonio arquitectónico no reconocido que debe ser difundido y merece ser valorado por la sociedad con el objeto de ser preservado para las futuras generaciones. 

  12. Primeras experiencias con la radioterapia en Santa Fe de Bogotá

    Directory of Open Access Journals (Sweden)

    Álvaro Javier Idrovo

    1997-07-01

    Full Text Available Muy poco tiempo después del descubrimiento de los rayos X por Wilhelm Conrad Rontgen el 8 de noviembre de 1895, mientras seguía los principios también recién descubiertos por Philipp Lenard en experimentos con tubos de rayos catódicos, se comenzaron a describir en laboratorios de Alemania, Estados Unidos, Inglaterra y Francia reacciones similares a las quemaduras solares y dolor ocular asociados a la exposición a radiaciones ionizantes. Algunas de estas primeras descripciones fueron publicadas en revistas como Nature, Science, The Lancet, The British Medical Journal y The Scientific American por autores de gran reputación como Thomas A. Edison, S. Winton, Stanton, J. Daniel, W.L. Dudley, R.L. Bowen, L.G. Stevens y N. Tesla.

  13. El ejercito del imperio neoasirio : las primeras máquinas de asedio

    Directory of Open Access Journals (Sweden)

    Rubén Sáez Abad

    2005-01-01

    Full Text Available Resulta muy importante para conocer los ingenios de asedio empleados en el mundo antiguo el estudio de las primeras máquinas usadas en el Imperio Asirio. Assurnasirpal fue el primero en emplear torres de asedio móviles y pesadas y arietes móviles. Bajo su reinado, también aparece el primer uso de unidades de zapadores, especializados en la escalada con escalas y debilitamiento de murallas con hachas y palancas.It´s very important to Know the siege engines used in the ancient world the study of the first machines that were used in the Asirian Empire. Assurnasirpal was the first to employ heavy, mobile siege towers and the mobile battering ram. Under his reign there appears the first use of units of wall-breakers, who specialized in climbing scaling ladders and weakening defensive walls with axes and levers.

  14. Stellar Firework in a Whirlwind

    Science.gov (United States)

    2007-09-01

    VLT Image of Supernova in Beautiful Spiral Galaxy NGC 1288 Stars do not like to be alone. Indeed, most stars are members of a binary system, in which two stars circle around each other in an apparently never-ending cosmic ballet. But sometimes, things can go wrong. When the dancing stars are too close to each other, one of them can start devouring its partner. If the vampire star is a white dwarf - a burned-out star that was once like our Sun - this greed can lead to a cosmic catastrophe: the white dwarf explodes as a Type Ia supernova. In July 2006, ESO's Very Large Telescope took images of such a stellar firework in the galaxy NGC 1288. The supernova - designated SN 2006dr - was at its peak brightness, shining as bright as the entire galaxy itself, bearing witness to the amount of energy released. ESO PR Photo 39/07 ESO PR Photo 39/07 SN 2006dr in NGC 1288 NGC 1288 is a rather spectacular spiral galaxy, seen almost face-on and showing multiple spiral arms pirouetting around the centre. Bearing a strong resemblance to the beautiful spiral galaxy NGC 1232, it is located 200 million light-years away from our home Galaxy, the Milky Way. Two main arms emerge from the central regions and then progressively split into other arms when moving further away. A small bar of stars and gas runs across the centre of the galaxy. The first images of NGC 1288, obtained during the commissioning period of the FORS instrument on ESO's VLT in 1998, were of such high quality that they have allowed astronomers [1] to carry out a quantitative analysis of the morphology of the galaxy. They found that NGC 1288 is most probably surrounded by a large dark matter halo. The appearance and number of spiral arms are indeed directly related to the amount of dark matter in the galaxy's halo. The supernova was first spotted by amateur astronomer Berto Monard. On the night of 17 July 2006, Monard used his 30-cm telescope in the suburbs of Pretoria in South Africa and discovered the supernova as an

  15. FORMACION DEL DISCURSO EN SALUD MENTAL EN LA PRIMERA MITAD DEL SIGLO XX

    Directory of Open Access Journals (Sweden)

    Mónica Mojica Perilla

    2013-03-01

    Full Text Available La formación del discurso en salud mental durante la primera mitad del siglo XX tiene en el Movimiento de Higiene Mental y en el Comité Nacional de Higiene Mental sus principales influencias. Como depositarios de un estilo de pensamiento biomédico, los dos entes mencionados tomaron la vocería en el campo de la salud mental, el cual para la época bajo estudio adolecía de una clara diferenciación conceptual. Con el objeto de comprender la influencia que ejerció este estilo de pensamiento en la formación del discurso en salud mental durante la primera mitad del siglo XX, se desarrollo una revisión de literatura de la época, empleando para tal fin una propuesta teórica que combinó el análisis del discurso de Michel Foucault y la sociología del conocimiento de Ludwik Fleck. Los resultados evidencian una hegemonía del estilo de pensamiento biomédico para abordar la salud mental, representada principalmente en el empleo de la prevención como estrategia de trabajo; de igual forma se constató que fueron los médicos, psiquiatras y salubristas de la época quienes asumieron para sí, como colectivo de pensamiento, la autoridad para hablar y actuar sobre la salud mental de la población, relegando a un segundo plano otros colectivos de pensamiento.

  16. Estudio comparativo de aisladores sísmicos FPS de primera y segunda generación.

    OpenAIRE

    Vergara Navarrete, Cynthia Fernanda

    2014-01-01

    Se presenta el marco teórico sobre el diseño de los aisladores FPS (Frictional Pendulum System) de la Primera y Segunda Generación; de acuerdo a los últimos avances realizados por la Universidad de Buffalo. Concretamente por Constantinou et al (2011). Se realiza, el análisis sísmico de tres estructuras de hormigón armado de tres, cinco y ocho pisos, de forma convencional y con aisladores sísmicos FPS de Primera y Segunda generación, dando como resultado que las edificaciones con aisladores sí...

  17. sunstardb: A Database for the Study of Stellar Magnetism and the Solar-stellar Connection

    Science.gov (United States)

    Egeland, Ricky

    2018-05-01

    The “solar-stellar connection” began as a relatively small field of research focused on understanding the processes that generate magnetic fields in stars and sometimes lead to a cyclic pattern of long-term variability in activity, as demonstrated by our Sun. This area of study has recently become more broadly pertinent to questions of exoplanet habitability and exo-space weather, as well as stellar evolution. In contrast to other areas of stellar research, individual stars in the solar-stellar connection often have a distinct identity and character in the literature, due primarily to the rarity of the decades-long time-series that are necessary for studying stellar activity cycles. Furthermore, the underlying stellar dynamo is not well understood theoretically, and is thought to be sensitive to several stellar properties, e.g., luminosity, differential rotation, and the depth of the convection zone, which in turn are often parameterized by other more readily available properties. Relevant observations are scattered throughout the literature and existing stellar databases, and consolidating information for new studies is a tedious and laborious exercise. To accelerate research in this area I developed sunstardb, a relational database of stellar properties and magnetic activity proxy time-series keyed by individual named stars. The organization of the data eliminates the need for the problematic catalog cross-matching operations inherent when building an analysis data set from heterogeneous sources. In this article I describe the principles behind sunstardb, the data structures and programming interfaces, as well as use cases from solar-stellar connection research.

  18. Indicators of Mass in Spherical Stellar Atmospheres

    Science.gov (United States)

    Lester, John B.; Dinshaw, Rayomond; Neilson, Hilding R.

    2013-04-01

    Mass is the most important stellar parameter, but it is not directly observable for a single star. Spherical model stellar atmospheres are explicitly characterized by their luminosity ( L⋆), mass ( M⋆), and radius ( R⋆), and observations can now determine directly L⋆ and R⋆. We computed spherical model atmospheres for red giants and for red supergiants holding L⋆ and R⋆ constant at characteristic values for each type of star but varying M⋆, and we searched the predicted flux spectra and surface-brightness distributions for features that changed with mass. For both stellar classes we found similar signatures of the stars’ mass in both the surface-brightness distribution and the flux spectrum. The spectral features have been use previously to determine log 10(g), and now that the luminosity and radius of a non-binary red giant or red supergiant can be observed, spherical model stellar atmospheres can be used to determine a star’s mass from currently achievable spectroscopy. The surface-brightness variations of mass are slightly smaller than can be resolved by current stellar imaging, but they offer the advantage of being less sensitive to the detailed chemical composition of the atmosphere.

  19. Stellarator Coil Design and Plasma Sensitivity

    International Nuclear Information System (INIS)

    Ku, Long-Poe; Boozer, Allen H.

    2010-01-01

    The rich information contained in the plasma response to external magnetic perturbations can be used to help design stellarator coils more effectively. We demonstrate the feasibility by first devel oping a simple, direct method to study perturbations in stellarators that do not break stellarator symmetry and periodicity. The method applies a small perturbation to the plasma boundary and evaluates the resulting perturbed free-boundary equilibrium to build up a sensitivity matrix for the important physics attributes of the underlying configuration. Using this sensitivity information, design methods for better stellarator coils are then developed. The procedure and a proof-of-principle application are given that (1) determine the spatial distributions of external normal magnetic field at the location of the unperturbed plasma boundary to which the plasma properties are most sen- sitive, (2) determine the distributions of external normal magnetic field that can be produced most efficiently by distant coils, (3) choose the ratios of the magnitudes of the the efficiently produced magnetic distributions so the sensitive plasma properties can be controlled. Using these methods, sets of modular coils are found for the National Compact Stellarator Experiment (NCSX) that are either smoother or can be located much farther from the plasma boundary than those of the present design.

  20. Development of code PRETOR for stellarator simulation

    International Nuclear Information System (INIS)

    Dies, J.; Fontanet, J.; Fontdecaba, J.M.; Castejon, F.; Alejandre, C.

    1998-01-01

    The Department de Fisica i Enginyeria Nuclear (DFEN) of the UPC has some experience in the development of the transport code PRETOR. This code has been validated with shots of DIII-D, JET and TFTR, it has also been used in the simulation of operational scenarios of ITER fast burnt termination. Recently, the association EURATOM-CIEMAT has started the operation of the TJ-II stellarator. Due to the need of validating the results given by others transport codes applied to stellarators and because all of them made some approximations, as a averaging magnitudes in each magnetic surface, it was thought suitable to adapt the PRETOR code to devices without axial symmetry, like stellarators, which is very suitable for the specific needs of the study of TJ-II. Several modifications are required in PRETOR; the main concerns to the models of: magnetic equilibrium, geometry and transport of energy and particles. In order to solve the complex magnetic equilibrium geometry the powerful numerical code VMEC has been used. This code gives the magnetic surface shape as a Fourier series in terms of the harmonics (m,n). Most of the geometric magnitudes are also obtained from the VMEC results file. The energy and particle transport models will be replaced by other phenomenological models that are better adapted to stellarator simulation. Using the proposed models, it is pretended to reproduce experimental data available from present stellarators, given especial attention to the TJ-II of the association EURATOM-CIEMAT. (Author)

  1. ON THE ORIGIN OF STELLAR MASSES

    International Nuclear Information System (INIS)

    Krumholz, Mark R.

    2011-01-01

    It has been a longstanding problem to determine, as far as possible, the characteristic masses of stars in terms of fundamental constants; the almost complete invariance of this mass as a function of the star-forming environment suggests that this should be possible. Here I provide such a calculation. The typical stellar mass is set by the characteristic fragment mass in a star-forming cloud, which depends on the cloud's density and temperature structure. Except in the very early universe, the latter is determined mainly by the radiation released as matter falls onto seed protostars. The energy yield from this process is ultimately set by the properties of deuterium burning in protostellar cores, which determines the stars' radii. I show that it is possible to combine these considerations to compute a characteristic stellar mass almost entirely in terms of fundamental constants, with an extremely weak residual dependence on the interstellar pressure and metallicity. This result not only explains the invariance of stellar masses, it resolves a second mystery: why fragmentation of a cold, low-density interstellar cloud, a process with no obvious dependence on the properties of nuclear reactions, happens to select a stellar mass scale such that stellar cores can ignite hydrogen. Finally, the weak residual dependence on the interstellar pressure and metallicity may explain recent observational hints of a smaller characteristic mass in the high-pressure, high-metallicity cores of giant elliptical galaxies.

  2. Collisionless microinstabilities in stellarators. II. Numerical simulations

    International Nuclear Information System (INIS)

    Proll, J. H. E.; Xanthopoulos, P.; Helander, P.

    2013-01-01

    Microinstabilities exhibit a rich variety of behavior in stellarators due to the many degrees of freedom in the magnetic geometry. It has recently been found that certain stellarators (quasi-isodynamic ones with maximum-J geometry) are partly resilient to trapped-particle instabilities, because fast-bouncing particles tend to extract energy from these modes near marginal stability. In reality, stellarators are never perfectly quasi-isodynamic, and the question thus arises whether they still benefit from enhanced stability. Here, the stability properties of Wendelstein 7-X and a more quasi-isodynamic configuration, QIPC, are investigated numerically and compared with the National Compact Stellarator Experiment and the DIII-D tokamak. In gyrokinetic simulations, performed with the gyrokinetic code GENE in the electrostatic and collisionless approximation, ion-temperature-gradient modes, trapped-electron modes, and mixed-type instabilities are studied. Wendelstein 7-X and QIPC exhibit significantly reduced growth rates for all simulations that include kinetic electrons, and the latter are indeed found to be stabilizing in the energy budget. These results suggest that imperfectly optimized stellarators can retain most of the stabilizing properties predicted for perfect maximum-J configurations

  3. Review of stellarator research world wide

    International Nuclear Information System (INIS)

    Shonet, J.L.

    1987-01-01

    The world-wide effort in stellarators has evolved considerably during the past few years. Stellarator facilities are located in the Australia, Federal Republic of Germany, Japan, the Soviet Union, Spain, the United Kingdom and the United States. Dimensions of stellarators range from less than 20 centimeters in major radius to more than 2 meters, and magnetic field values between 0.2 Tesla to more than 3.0 Tesla. Stellarators are made in a variety of magnetic configurations with wide ranges of toroidal aspect ratios and methods of generating the stellarator magnetic surfaces. In particular, continuous helical coils, twisted modular coils, or twisted vacuum chambers all provide different means to generate nested toroidal magnetic surfaces without the need for currents flowing in the plasma. The goal of present day experiments is to accumulate a physics data base. This is being done by increasing electron and ion temperatures with non-ohmic heating, by transport and scaling studies considering neoclassical scaling, global scaling, effects of electric fields, the bootstrap current and magnetic islands. Higher betas are being attempted by designing suitable magnetic configurations, pellet injection and/or minimizing transport losses. Plasma-wall interactions and particle control are being examined by divertor, pumped-limiter and carbonization experiments

  4. The Stellar Imager (SI)"Vision Mission"

    Science.gov (United States)

    Carpenter, Ken; Danchi, W.; Leitner, J.; Liu, A.; Lyon, R.; Mazzuca, L.; Moe, R.; Chenette, D.; Karovska, M.; Allen, R.

    2004-01-01

    The Stellar Imager (SI) is a "Vision" mission in the Sun-Earth Connection (SEC) Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar magnetic activity and its impact on life in the Universe. The science goals of SI require an ultra-high angular resolution, at ultraviolet wavelengths, on the order of 100 micro-arcsec and thus baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (less than 20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. SI's resolution will make it an invaluable resource for many other areas of astrophysics, including studies of AGN s, supernovae, cataclysmic variables, young stellar objects, QSO's, and stellar black holes. ongoing mission concept and technology development studies for SI. These studies are designed to refine the mission requirements for the science goals, define a Design Reference Mission, perform trade studies of selected major technical and architectural issues, improve the existing technology roadmap, and explore the details of deployment and operations, as well as the possible roles of astronauts and/or robots in construction and servicing of the facility.

  5. Geometric phase modulation for stellar interferometry

    International Nuclear Information System (INIS)

    Roy, M.; Boschung, B.; Tango, W.J.; Davis, J.

    2002-01-01

    Full text: In a long baseline optical interferometer, the fringe visibility is normally measured by modulation of the optical path difference between the two arms of the instruments. To obtain accurate measurements, the spectral bandwidth must be narrow, limiting the sensitivity of the technique. The application of geometric phase modulation technique to stellar interferometry has been proposed by Tango and Davis. Modulation of the geometric phase has the potential for improving the sensitivity of optical interferometers, and specially the Sydney University Stellar Interferometer (SUSI), by allowing broad band modulation of the light signals. This is because a modulator that changes the geometric phase of the signal is, in principle, achromatic. Another advantage of using such a phase modulator is that it can be placed in the common path traversed by the two orthogonally polarized beams emerging from the beam combiner in a stellar interferometer. Thus the optical components of the modulator do not have to be interferometric quality and could be relatively easily introduced into SUSI. We have investigated the proposed application in a laboratory-based experiment using a Mach-Zehnder interferometer with white-light source. This can be seen as a small model of an amplitude stellar interferometer where the light source takes the place of the distant star and two corner mirrors replaces the entrance pupils of the stellar interferometer

  6. Stellar Wakes from Dark Matter Subhalos.

    Science.gov (United States)

    Buschmann, Malte; Kopp, Joachim; Safdi, Benjamin R; Wu, Chih-Liang

    2018-05-25

    We propose a novel method utilizing stellar kinematic data to detect low-mass substructure in the Milky Way's dark matter halo. By probing characteristic wakes that a passing dark matter subhalo leaves in the phase-space distribution of ambient halo stars, we estimate sensitivities down to subhalo masses of ∼10^{7}  M_{⊙} or below. The detection of such subhalos would have implications for dark matter and cosmological models that predict modifications to the halo-mass function at low halo masses. We develop an analytic formalism for describing the perturbed stellar phase-space distributions, and we demonstrate through idealized simulations the ability to detect subhalos using the phase-space model and a likelihood framework. Our method complements existing methods for low-mass subhalo searches, such as searches for gaps in stellar streams, in that we can localize the positions and velocities of the subhalos today.

  7. Stellar Wakes from Dark Matter Subhalos

    Science.gov (United States)

    Buschmann, Malte; Kopp, Joachim; Safdi, Benjamin R.; Wu, Chih-Liang

    2018-05-01

    We propose a novel method utilizing stellar kinematic data to detect low-mass substructure in the Milky Way's dark matter halo. By probing characteristic wakes that a passing dark matter subhalo leaves in the phase-space distribution of ambient halo stars, we estimate sensitivities down to subhalo masses of ˜107 M⊙ or below. The detection of such subhalos would have implications for dark matter and cosmological models that predict modifications to the halo-mass function at low halo masses. We develop an analytic formalism for describing the perturbed stellar phase-space distributions, and we demonstrate through idealized simulations the ability to detect subhalos using the phase-space model and a likelihood framework. Our method complements existing methods for low-mass subhalo searches, such as searches for gaps in stellar streams, in that we can localize the positions and velocities of the subhalos today.

  8. Effect of finite β on stellarator transport

    International Nuclear Information System (INIS)

    Mynick, H.E.

    1984-04-01

    A theory of the modification of stellarator transport due to the presence of finite plasma pressure is developed, and applied to a range of stellarator configurations. For many configurations of interest, plasma transport can change by more than an order of magnitude in the progression from zero pressure to the equilibrium β limit of the device. Thus, a stellarator with transport-optimized vacuum fields can have poor confinement at the desired operating β. Without an external compensating field, increasing β tends to degrade confinement, unless the initial field structure is very carefully chosen. The theory permits one to correctly determine this vacuum structure, in terms of the desired structure of the field at a prescribed operating β. With a compensating external field, the deleterious effect of finite β on transport can be partially eliminated

  9. Recent advances in modeling stellar interiors (u)

    Energy Technology Data Exchange (ETDEWEB)

    Guzik, Joyce Ann [Los Alamos National Laboratory

    2010-01-01

    Advances in stellar interior modeling are being driven by new data from large-scale surveys and high-precision photometric and spectroscopic observations. Here we focus on single stars in normal evolutionary phases; we will not discuss the many advances in modeling star formation, interacting binaries, supernovae, or neutron stars. We review briefly: (1) updates to input physics of stellar models; (2) progress in two and three-dimensional evolution and hydrodynamic models; (3) insights from oscillation data used to infer stellar interior structure and validate model predictions (asteroseismology). We close by highlighting a few outstanding problems, e.g., the driving mechanisms for hybrid {gamma} Dor/{delta} Sct star pulsations, the cause of giant eruptions seen in luminous blue variables such as {eta} Car and P Cyg, and the solar abundance problem.

  10. Electron Capture Cross Sections for Stellar Nucleosynthesis

    Directory of Open Access Journals (Sweden)

    P. G. Giannaka

    2015-01-01

    Full Text Available In the first stage of this work, we perform detailed calculations for the cross sections of the electron capture on nuclei under laboratory conditions. Towards this aim we exploit the advantages of a refined version of the proton-neutron quasiparticle random-phase approximation (pn-QRPA and carry out state-by-state evaluations of the rates of exclusive processes that lead to any of the accessible transitions within the chosen model space. In the second stage of our present study, we translate the abovementioned e--capture cross sections to the stellar environment ones by inserting the temperature dependence through a Maxwell-Boltzmann distribution describing the stellar electron gas. As a concrete nuclear target we use the 66Zn isotope, which belongs to the iron group nuclei and plays prominent role in stellar nucleosynthesis at core collapse supernovae environment.

  11. Equilibrium reconstruction in stellarators: V3FIT

    Energy Technology Data Exchange (ETDEWEB)

    Hanson, J.D.; Knowlton, S.F. [Physics Department, Auburn University, Auburn, AL (United States); Hirshman, S.P.; Lazarus, E.A. [Oak Ridge National Laboratory, Oak Ridge, TN (United States); Lao, L.L. [General Atomics, San Diego, CA (United States)

    2003-07-01

    The first section describes a general response function formalism for computing stellarator magnetic diagnostic signals, which is the first step in developing a reconstruction capability. The approach parallels that used in the EFIT two-dimensional (2-D) equilibrium reconstruction code. The second section describes the two codes we have written, V3RFUN and V3POST. V3RFUN computes the response functions for a specified magnetic diagnostic coil, and V3POST uses the response functions calculated by V3RFUN, along with the plasma current information supplied by the equilibrium code VMEC, to compute the expected magnetic diagnostic signals. These two codes are currently being used to design magnetic diagnostic for the NCSX stellarator (at PPPL) and the CTH toroidal hybrid stellarator (at Auburn University). The last section of the paper describes plans for the V3FIT code. (orig.)

  12. The low-luminosity stellar mass function

    International Nuclear Information System (INIS)

    Kroupa, Pavel; Tout, C.A.; Gilmore, Gerard

    1990-01-01

    The stellar mass function for low-mass stars is constrained using the stellar luminosity function and the slope of the mass-luminosity relation. We investigate the range of mass functions for stars with absolute visual magnitude fainter than M V ≅ +5 which are consistent with both the local luminosity function and the rather poorly determined mass-absolute visual magnitude relation. Points of inflexion in the mass-luminosity relation exist because of the effects of H - , H 2 and of other molecules on the opacity and equation of state. The first two of these correspond to absolute magnitudes M V ≅ +7 and M V ≅ +12, respectively, at which structure is evident in the stellar luminosity function (a flattening and a maximum, respectively). Combining the mass-luminosity relation which shows these inflexion points with a peaked luminosity function, we test smooth mass functions in the mass range 0.9-0.1 the solar mass. (author)

  13. Young and Exotic Stellar Zoo

    Science.gov (United States)

    2005-03-01

    Summary Super star clusters are groups of hundreds of thousands of very young stars packed into an unbelievably small volume. They represent the most extreme environments in which stars and planets can form. Until now, super star clusters were only known to exist very far away, mostly in pairs or groups of interacting galaxies. Now, however, a team of European astronomers [1] have used ESO's telescopes to uncover such a monster object within our own Galaxy, the Milky Way, almost, but not quite, in our own backyard! The newly found massive structure is hidden behind a large cloud of dust and gas and this is why it took so long to unveil its true nature. It is known as "Westerlund 1" and is a thousand times closer than any other super star cluster known so far. It is close enough that astronomers may now probe its structure in some detail. Westerlund 1 contains hundreds of very massive stars, some shining with a brilliance of almost one million suns and some two-thousand times larger than the Sun (as large as the orbit of Saturn)! Indeed, if the Sun were located at the heart of this remarkable cluster, our sky would be full of hundreds of stars as bright as the full Moon. Westerlund 1 is a most unique natural laboratory for the study of extreme stellar physics, helping astronomers to find out how the most massive stars in our Galaxy live and die. From their observations, the astronomers conclude that this extreme cluster most probably contains no less than 100,000 times the mass of the Sun, and all of its stars are located within a region less than 6 light-years across. Westerlund 1 thus appears to be the most massive compact young cluster yet identified in the Milky Way Galaxy. PR Photo 09a/05: The Super Star Cluster Westerlund 1 (2.2m MPG/ESO + WFI) PR Photo 09b/05: Properties of Young Massive Clusters Super Star Clusters Stars are generally born in small groups, mostly in so-called "open clusters" that typically contain a few hundred stars. From a wide range of

  14. The Stellar IMF from Isothermal MHD Turbulence

    Science.gov (United States)

    Haugbølle, Troels; Padoan, Paolo; Nordlund, Åke

    2018-02-01

    We address the turbulent fragmentation scenario for the origin of the stellar initial mass function (IMF), using a large set of numerical simulations of randomly driven supersonic MHD turbulence. The turbulent fragmentation model successfully predicts the main features of the observed stellar IMF assuming an isothermal equation of state without any stellar feedback. As a test of the model, we focus on the case of a magnetized isothermal gas, neglecting stellar feedback, while pursuing a large dynamic range in both space and timescales covering the full spectrum of stellar masses from brown dwarfs to massive stars. Our simulations represent a generic 4 pc region within a typical Galactic molecular cloud, with a mass of 3000 M ⊙ and an rms velocity 10 times the isothermal sound speed and 5 times the average Alfvén velocity, in agreement with observations. We achieve a maximum resolution of 50 au and a maximum duration of star formation of 4.0 Myr, forming up to a thousand sink particles whose mass distribution closely matches the observed stellar IMF. A large set of medium-size simulations is used to test the sink particle algorithm, while larger simulations are used to test the numerical convergence of the IMF and the dependence of the IMF turnover on physical parameters predicted by the turbulent fragmentation model. We find a clear trend toward numerical convergence and strong support for the model predictions, including the initial time evolution of the IMF. We conclude that the physics of isothermal MHD turbulence is sufficient to explain the origin of the IMF.

  15. Fundamentos e métodos de medidas de energia dinâmica no SPT

    Directory of Open Access Journals (Sweden)

    Antonio Belincanta

    2000-05-01

    Full Text Available Discutem-se neste trabalho os métodos disponíveis no Brasil e no exterior para a medida da energia transferida às hastes no SPT, apresentando-se inclusive registros típicos dos eventos dinâmicos correspondentes

  16. Ato infracional e medida socioeducativa: representações de adolescentes em L.A.

    Directory of Open Access Journals (Sweden)

    Bianca Izoton Coelho

    2013-01-01

    Full Text Available A pesquisa analisou as representações sociais de ato infracional e medida socioeducativa em adolescentes em conflito com a lei. Utilizou-se, como aporte teórico e metodológico, a Teoria das Representações Sociais. Participaram da pesquisa quarenta e seis adolescentes que cumpriam, há mais de três meses, a medida de Liberdade Assistida. Os dados foram coletados, por meio de entrevistas, com um roteiro semiestruturado e consistiram na técnica das evocações livres por meio dos termos ato infracional e medida socioeducativa. Utilizou-se o software EVOC para análise das evocações emitidas. Os resultados apontaram como caracterização socioeconômica dos adolescentes: renda familiar baixa, baixo nível de escolaridade, local de residência precário, etnias afro-descendentes predominantes e distanciamento da religião. As representações sociais de ato infracional relacionaram-se aos tipos de atos infracionais e às suas causas e consequências. As representações sociais de medida socioeducativa relacionaram-se a ações positivas em que, além da aprendizagem, houve a possibilidade de mudança.

  17. Adolescente em conflito com a lei e medidas socioeducativas: limites e (impossibilidades

    Directory of Open Access Journals (Sweden)

    Francischini, Rosângela

    2005-01-01

    Full Text Available Reinserção social, readaptação, ajustamento social, integração à família e sociedade. Várias são as expressões empregadas para referir-se ao efeito desejado do trabalho com o jovem em conflito com a lei, em cumprimento de medidas socioeducativas, particularmente em privação de liberdade. Parte do aparato legal do Estado, a partir da promulgação do Estatuto da Criança e do Adolescente, significaram, essas medidas, uma chamada à responsabilização do jovens, em face da transgressão cometida. No entanto, avalia-se, o que dá a essas medidas o caráter socioeducativo, fazendo com que o trabalho desenvolvido nas instituições diferencie-se do cumprimento de pena? Estrutura física, formação de recursos humanos, ações educativas e trabalho transdiciplinar são alguns dos aspectos implicados nesta questão. Neste contexto de discussão insere-se o presente artigo, que tem por objetivo discutir o caráter socioeducativo das medidas de privação de liberdade e as possibilidades de reinserção social do jovem em conflito com a lei

  18. Medidas procesales especiales y proteccíon de los derechos humanos Informe general

    NARCIS (Netherlands)

    Vervaele, J.A.E.

    2009-01-01

    El objetivo del informe general es realizar un análisis comparativo de los informes nacionales para evidenciar los procesos de transformación de los sistemas nacionales de justicia penal, en particular del proceso penal, en el que se han introducido medidas procesales especiales para hacer frente al

  19. Students Excited by Stellar Discovery

    Science.gov (United States)

    2011-02-01

    In the constellation of Ophiuchus, above the disk of our Milky Way Galaxy, there lurks a stellar corpse spinning 30 times per second -- an exotic star known as a radio pulsar. This object was unknown until it was discovered last week by three high school students. These students are part of the Pulsar Search Collaboratory (PSC) project, run by the National Radio Astronomy Observatory (NRAO) in Green Bank, WV, and West Virginia University (WVU). The pulsar, which may be a rare kind of neutron star called a recycled pulsar, was discovered independently by Virginia students Alexander Snider and Casey Thompson, on January 20, and a day later by Kentucky student Hannah Mabry. "Every day, I told myself, 'I have to find a pulsar. I better find a pulsar before this class ends,'" said Mabry. When she actually made the discovery, she could barely contain her excitement. "I started screaming and jumping up and down." Thompson was similarly expressive. "After three years of searching, I hadn't found a single thing," he said, "but when I did, I threw my hands up in the air and said, 'Yes!'." Snider said, "It actually feels really neat to be the first person to ever see something like that. It's an uplifting feeling." As part of the PSC, the students analyze real data from NRAO's Robert C. Byrd Green Bank Telescope (GBT) to find pulsars. The students' teachers -- Debra Edwards of Sherando High School, Leah Lorton of James River High School, and Jennifer Carter of Rowan County Senior High School -- all introduced the PSC in their classes, and interested students formed teams to continue the work. Even before the discovery, Mabry simply enjoyed the search. "It just feels like you're actually doing something," she said. "It's a good feeling." Once the pulsar candidate was reported to NRAO, Project Director Rachel Rosen took a look and agreed with the young scientists. A followup observing session was scheduled on the GBT. Snider and Mabry traveled to West Virginia to assist in the

  20. Near-Field Cosmology with Resolved Stellar Populations Around Local Volume LMC Stellar-Mass Galaxies

    Science.gov (United States)

    Carlin, Jeffrey L.; Sand, David J.; Willman, Beth; Brodie, Jean P.; Crnojevic, Denija; Forbes, Duncan; Hargis, Jonathan R.; Peter, Annika; Pucha, Ragadeepika; Romanowsky, Aaron J.; Spekkens, Kristine; Strader, Jay

    2018-06-01

    We discuss our ongoing observational program to comprehensively map the entire virial volumes of roughly LMC stellar mass galaxies at distances of ~2-4 Mpc. The MADCASH (Magellanic Analog Dwarf Companions And Stellar Halos) survey will deliver the first census of the dwarf satellite populations and stellar halo properties within LMC-like environments in the Local Volume. Our results will inform our understanding of the recent DES discoveries of dwarf satellites tentatively affiliated with the LMC/SMC system. This program has already yielded the discovery of the faintest known dwarf galaxy satellite of an LMC stellar-mass host beyond the Local Group, based on deep Subaru+HyperSuprimeCam imaging reaching ~2 magnitudes below its TRGB, and at least two additional candidate satellites. We will summarize the survey results and status to date, highlighting some challenges encountered and lessons learned as we process the data for this program through a prototype LSST pipeline. Our program will examine whether LMC stellar mass dwarfs have extended stellar halos, allowing us to assess the relative contributions of in-situ stars vs. merger debris to their stellar populations and halo density profiles. We outline the constraints on galaxy formation models that will be provided by our observations of low-mass galaxy halos and their satellites.

  1. Optimisation of stellarator systems: Possible ways

    International Nuclear Information System (INIS)

    Cooper, W.A.; Isaev, M.; Leneva, A.E.; Mikhailov, M.; Shafranov, V.D.; Subbotin, A.A.

    2001-01-01

    The results of our search for advanced helical (stellarator) systems with a small number of field periods over the last five years are presented. The comparison of stellarator systems with toroidal (helical or axial) and poloidal directions of the contours with B = constant on the magnetic surface as well as systems with Helias and Heliac-like orientation of the magnetic surfaces cross-sections with respect to the principal normal to the magnetic axis is undertaken. Particular attention is paid to some attractive features of the systems with constant B-lines in the poloidal direction. (author)

  2. Optimisation of stellarator systems: Possible ways

    International Nuclear Information System (INIS)

    Cooper, W.A.; Isaev, M.Yu.; Leneva, A.E.; Mikhailov, M.I.; Sharfranov, V.D.; Subbotin, A.A.

    1999-01-01

    The results of our search for advanced helical (stellarator) systems with a small number of field periods over the last five years are presented. The comparison of stellarator systems with toroidal (helical or axial) and poloidal directions of the contours with B = constant on the magnetic surface as well as systems with Helias and Heliac-like orientation of the magnetic surfaces cross-sections with respect to the principal normal to the magnetic axis is undertaken. Particular attention is paid to some attractive features of the systems with constant B-lines in the poloidal direction. (author)

  3. 3D radiative transfer in stellar atmospheres

    International Nuclear Information System (INIS)

    Carlsson, M

    2008-01-01

    Three-dimensional (3D) radiative transfer in stellar atmospheres is reviewed with special emphasis on the atmospheres of cool stars and applications. A short review of methods in 3D radiative transfer shows that mature methods exist, both for taking into account radiation as an energy transport mechanism in 3D (magneto-) hydrodynamical simulations of stellar atmospheres and for the diagnostic problem of calculating the emergent spectrum in more detail from such models, both assuming local thermodynamic equilibrium (LTE) and in non-LTE. Such methods have been implemented in several codes, and examples of applications are given.

  4. Stellar compass for the Clementine Mission

    Energy Technology Data Exchange (ETDEWEB)

    Wilson, B. [Lawrence Livermore National Lab., CA (United States)

    1994-11-15

    A CCD sensor with 42 x 28 degrees FOV and 576 x 384 pixels was built by the Advanced Technology Program (ATP) in the Physics Department at LLNL. That sensor, called the StarTracker camera, is used on the Clementine Lunar Mapping mission between January and May, 1994. Together with the Stellar Compass software, the StarTracker camera provided a way of identifying its orientation to within about 150 microradians in camera body pitch and yaw. This presentation will be an overview of basically how the Stellar Compass software works, along with showing some of its performance results.

  5. Overdense Plasma Operation in the WEGA Stellarator

    Czech Academy of Sciences Publication Activity Database

    Otte, M.; Laqua, H.P.; Marsen, S.; Podoba, Y.; Preinhaelter, Josef; Stange, T.; Urban, Jakub; Wagner, F.; Zhang, D.

    2010-01-01

    Roč. 50, č. 8 (2010), s. 785-789 ISSN 0863-1042. [International Stellarator/Heliotron Workshop/17th./. Princeton, 12.10.2009-16.10.2009] R&D Projects: GA ČR GA202/08/0419; GA MŠk 7G09042 Institutional research plan: CEZ:AV0Z20430508 Keywords : Stellarator * Bernstein waves * overdense plasma * supra -thermal electrons Subject RIV: BL - Plasma and Gas Discharge Physics Impact factor: 1.006, year: 2010 http://dx.doi.org/10.1002/ctpp.200900053

  6. 176Lu: Cosmic clock or stellar thermometer

    International Nuclear Information System (INIS)

    Ward, R.A.; Beer, H.; Kaeppeler, F.; Wisshak, K.

    1980-12-01

    We quantitatively examine the various experimental and theoretical aspects of the stellar synthesis of the long-lived ground state of 176 Lu (3.6 x 10 10 y). We discuss the various regimes of stellar temperature and free-neutron density in which either: (i) the internal electromagnetic couplings between 176 Lusup(o) and 176 Lusup(m) (3.68 hours) are sufficiently slow that they may be treated as separate nuclei, or (ii) the internal couplings are rapidly able to establish thermal equilibrium between 176 Lusup(o) and 176 Lusup(m). (orig.)

  7. La primera guerra mundial: su tratamiento desde una perspectiva pedagógica fundamentada en el desarrollo de habilidades cognitivas

    OpenAIRE

    Ramos Calderón, Douglas; Murillo Ly, Hugo

    2012-01-01

    El articulo ofrece un nuevo modelo teórico – metodológico para estructurar libros de texto de Estudios Sociales, basado en el desarrollo de las llamadas habilidades cognoscitivas de la historia. Se presenta además la concreción de dicho modelo en un texto histórico o unidad modelo sobre la Primera Guerra Mundial.

  8. Las emociones y su expresión en la primera infancia. Las vías facial y vocal

    Directory of Open Access Journals (Sweden)

    José Luis MARTÍNEZ HERRADOR

    2009-11-01

    Full Text Available El estudio de la expresión emocional a partir de las vías fácil y oral durante la primera infancia adquiere especial significación porque permite conectar con temáticas de gran relevancia para el estudio y la comprensión del desarrollo infantil.

  9. Primera identificación molecular del transgen de la proteína fluorescente roja (RFP en peces Cebra (Danio rerio transgénicos ornamentales introducidos en el Perú

    Directory of Open Access Journals (Sweden)

    Carlos Scotto

    2013-01-01

    Full Text Available En el presente trabajo se identificó por primera vez peces Cebra transgénicos (Danio rerio fluorescentes de color rojo, naranja y rosado introducidos al territorio peruano de acuarios locales utilizando la técnica de PCR para amplificar el transgen RFP perteneciente a la anémona marina Discosoma spp. Se encontró una expresión génica diferencial del transgen de la proteína fluorescente roja (RFP que determinaría una gradiente de bioluminiscencia para cada color entre los peces OVM analizados. Se realizó un análisis de secuencias de las dos variantes de la RFP junto con las seis variantes de la GFP de proteínas fluorescentes existentes en el Genbank que podrían ayudar a identificar rápidamente si son nuevos genes o si son nuevas variantes de éstas proteínas fluorescentes y que podrían ser utilizadas en otros OVMs hidrobiológicos a futuro. De este modo, desarrollar y optimizar las medidas de bioseguridad mediante su oportuna detección a nivel genético molecular.

  10. MEDIDAS DE DESEMPENHO E ONTOLOGIAS: UM ESTUDO BIBLIOMÉTRICO PARA IDENTIFICAÇÃO DO USO DE ONTOLOGIAS PARA O SUPORTE DOS PROCESSOS DE MEDIDAS DE DESEMPENHO

    Directory of Open Access Journals (Sweden)

    Vanderlei Freitas Junior

    2015-09-01

    Full Text Available O presente trabalho se propõe analisar as publicações internacionais acerca do emprego das ontologias no contexto de medidas de desempenho. Para isso, foi realizada uma pesquisa bibliométrica em três bases de dados internacionais: Web of Science, Scopus e IEEE. Essa pesquisa foi desenvolvida em duas grandes etapas: (i busca sistemática da literatura, e (ii análise e síntese das informações bibliométricas. Foram localizados 115 trabalhos, escritos por 362 autores vinculados a 84 instituições de 101 países diferentes e estão publicados em 38 periódicos. Os autores identificaram ainda 981 palavras-chave diferentes em seus estudos. Os estudos, de maneira geral, evidenciam a possibilidade de utilização das ontologias como ferramenta semântica em diversas etapas e momentos do processo de medidas de desempenho, especialmente no que tange à representação do conhecimento e elu-cidação dos indicadores chaves, permitindo a interoperabilidade destes indicadores. A partir da identificação destes estudos o presente trabalho contribui para a compreensão das possibilidades de aplicação das ontologias para o suporte aos pro-cessos de medida de desempenho, realizando o mapeamento das publicações inter-nacionais desta temática e evidenciando a possibilidade de representação do conhecimento envolvido nesta tarefa.

  11. Abuso de las medidas y medidas abusivas. Crítica al pensamiento bibliométrico hegemónico

    OpenAIRE

    GÒMEZ-MORALES, YURI JACK

    2018-01-01

    RESUMEN En este ensayo reflexivo se hace una crítica a la economía política de la medición de la ciencia, la cual se ejemplifica mediante el análisis del factor de impacto como medida de la calidad científica; se explican los mecanismos sociales y culturales que operan en la construcción de estas formas de pensar y actuar hegemónicas; y se advierte sobre las graves consecuencias de este proyecto global para la desinstitucionalización de la ciencia local, y el surgimiento de una ciencia nacion...

  12. Primeras evidencias de arte mueble paleolítico en el sur de Portugal

    Directory of Open Access Journals (Sweden)

    Simón Vallejo, María D.

    2012-06-01

    Full Text Available This paper presents the first evidence for Palaeolithic portable art in Southern Portugal. This include two plaques, dated between 20,500 and 19,500 BP from Solutrean levels from the site of Vale Boi, Western Algarve (Portugal. One of the pieces is a small engraved schist plaque (14,6 × 8,1 mm with abstract lines on one side. The other artefact is an 8 × 5 cm schist plaque. One side is an oxide natural deposit, used to produce dye; the other side has three aurochs and a probable cervid. Stilistic information and the engraving sequence indicate probably production by a single artist. The stylistic characteristics are in full agreement withi those from late Gravettian and early Solutrean art known from Valencia, Andalucia (Spain and the Côa valley (Portugal, thus confirming the absolute AMS dates from the Vale Boi Levels.

    En este trabajo presentamos la primera evidencia de arte mueble paleolítico en el sur de Portugal: dos plaquetas de pizarra procedentes de niveles solutrenses del yacimiento de Vale Boi, zona occidental del Algarve (Portugal. La primera de las piezas es una pequeña placa (14,6 × 8,1 mm que presenta sobre una de sus caras un ideomorfo grabado. La segunda (8 × 5 cm cuenta con una superficie ocupada por óxido de hierro natural de color amarillento, tiene claros indicios de extracción de mineral para producir colorantes. En la superficie opuesta han sido grabados tres uros y una posible cierva. El estilo y secuencia de los grabados apuntan a un solo artista. Las características estilísticas de los zoomorfos concuerdan bien con los rasgos comunes del arte del ciclo Gravetiense final y Solutrense antiguo del País Valenciano, Andalucía y Valle de Côa (Portugal. Esta afinidad sintoniza asimismo con las fechas AMS de los niveles solutrenses de Vale Boi, datados entre ca. 20.500 y 19.500 BP.

  13. Manejo de la primera alimentación del bocachico ( Prochilodus magdalenae.

    Directory of Open Access Journals (Sweden)

    Víctor Atencio-García

    2003-06-01

    Full Text Available En el Centro de Investigación Piscícola de la Universidad de Córdoba se realizaron dos experimentos; en elprimero, el objetivo fue evaluar el efecto de diferentes presas en el manejo de la primera alimentación delbocachico Prochilodus magdalenae y en el segundo, con la mejor presa del ensayo anterior, determinar eltiempo mínimo de manejo de la primera alimentación. En ambos casos las post-larvas fueron sembradas a 50/L en acuario de 5 L. En el primer experimento se evaluaron las siguientes presas: nauplios de Artemia (NA,cistos descapsulados de Artemia (CA, zooplancton silvestre tamizado entre 125-160 µm (Z125-160 y zooplanctonsilvestre tamizado entre 250-400 µm (Z250-400, ofrecidas durante cinco días a razón de 5 Presa/mL. Además,un grupo de post-larvas fue sometida a ayuno. Las mayores ganancias de peso y longitud total la registraron laspost-larvas alimentadas con NA (2.0±1.8 mg, 1.8±0.9 mm y Z250-400 (2.0±1.1 mg, 1.6±0.5 mm. Lasobrevivencia de las post-larvas alimentadas con NA (73.2±10.7% fue mayor a las registradas en los demástratamientos (P0.05. Mientras que latasa de crecimiento específico (G osciló entre 17.1 (5 días y 22.3 %/día (3 días, sin observarse diferenciasestadísticas significativas (P>0.05. Las post-larvas alimentadas durante 3, 5 y 7 días presentaron las mejoressobrevivencias (92.2±6.2, 93.3±4.3, 95.6±3.9% respectivamente cuando fueron sometidas a la prueba deresistencia al estrés. Las post-larvas alimentadas por un solo día mostraron la menor sobrevivencia al sersometidas a esta prueba (87±1%. Los resultados del estudio sugieren que nauplios de Artemia o zooplanctonsilvestre en le rango de 250-400 mm, libre de predadores, son presas adecuada para el manejo de la primeraalimentación al menos durante 3 días antes de ser sembradas en estanques en tierra.

  14. Ambitious Survey Spots Stellar Nurseries

    Science.gov (United States)

    2010-08-01

    -dimensional geometry of the Magellanic system. Chris Evans from the VMC team adds: "The VISTA images will allow us to extend our studies beyond the inner regions of the Tarantula into the multitude of smaller stellar nurseries nearby, which also harbour a rich population of young and massive stars. Armed with the new, exquisite infrared images, we will be able to probe the cocoons in which massive stars are still forming today, while also looking at their interaction with older stars in the wider region." The wide-field image shows a host of different objects. The bright area above the centre is the Tarantula Nebula itself, with the RMC 136 cluster of massive stars in its core. To the left is the NGC 2100 star cluster. To the right is the tiny remnant of the supernova SN1987A (eso1032). Below the centre are a series of star-forming regions including NGC 2080 - nicknamed the "Ghost Head Nebula" - and the NGC 2083 star cluster. The VISTA Magellanic Cloud Survey is one of six huge near-infrared surveys of the southern sky that will take up most of the first five years of operations of VISTA. Notes [1] VISTA ― the Visible and Infrared Survey Telescope for Astronomy ― is the newest telescope at ESO's Paranal Observatory in northern Chile. VISTA is a survey telescope working at near-infrared wavelengths and is the world's largest survey telescope. Its large mirror, wide field of view and very sensitive detectors will reveal a completely new view of the southern sky. The telescope is housed on the peak adjacent to the one hosting ESO's Very Large Telescope (VLT) and shares the same exceptional observing conditions. VISTA has a main mirror that is 4.1 m across. In photographic terms it can be thought of as a 67-megapixel digital camera with a 13 000 mm f/3.25 mirror lens. More information ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries

  15. The “Building Blocks” of Stellar Halos

    Directory of Open Access Journals (Sweden)

    Kyle A. Oman

    2017-08-01

    Full Text Available The stellar halos of galaxies encode their accretion histories. In particular, the median metallicity of a halo is determined primarily by the mass of the most massive accreted object. We use hydrodynamical cosmological simulations from the apostle project to study the connection between the stellar mass, the metallicity distribution, and the stellar age distribution of a halo and the identity of its most massive progenitor. We find that the stellar populations in an accreted halo typically resemble the old stellar populations in a present-day dwarf galaxy with a stellar mass ∼0.2–0.5 dex greater than that of the stellar halo. This suggests that had they not been accreted, the primary progenitors of stellar halos would have evolved to resemble typical nearby dwarf irregulars.

  16. Deriving stellar parameters with the SME software package

    Science.gov (United States)

    Piskunov, N.

    2017-09-01

    Photometry and spectroscopy are complementary tools for deriving accurate stellar parameters. Here I present one of the popular packages for stellar spectroscopy called SME with the emphasis on the latest developments and error assessment for the derived parameters.

  17. Stellar chemical signatures and hierarchical galaxy formation

    NARCIS (Netherlands)

    Venn, KA; Irwin, M; Shetrone, MD; Tout, CA; Hill, [No Value; Tolstoy, E

    To compare the chemistries of stars in the Milky Way dwarf spheroidal (dSph) satellite galaxies with stars in the Galaxy, we have compiled a large sample of Galactic stellar abundances from the literature. When kinematic information is available, we have assigned the stars to standard Galactic

  18. Equilibrium 𝛽-limits in classical stellarators

    Science.gov (United States)

    Loizu, J.; Hudson, S. R.; Nührenberg, C.; Geiger, J.; Helander, P.

    2017-12-01

    A numerical investigation is carried out to understand the equilibrium -limit in a classical stellarator. The stepped-pressure equilibrium code (Hudson et al., Phys. Plasmas, vol. 19 (11), 2012) is used in order to assess whether or not magnetic islands and stochastic field-lines can emerge at high . Two modes of operation are considered: a zero-net-current stellarator and a fixed-iota stellarator. Despite the fact that relaxation is allowed (Taylor, Rev. Mod. Phys., vol. 58 (3), 1986, pp. 741-763), the former is shown to maintain good flux surfaces up to the equilibrium -limit predicted by ideal-magnetohydrodynamics (MHD), above which a separatrix forms. The latter, which has no ideal equilibrium -limit, is shown to develop regions of magnetic islands and chaos at sufficiently high , thereby providing a `non-ideal -limit'. Perhaps surprisingly, however, the value of at which the Shafranov shift of the axis reaches a fraction of the minor radius follows in all cases the scaling laws predicted by ideal-MHD. We compare our results to the High-Beta-Stellarator theory of Freidberg (Ideal MHD, 2014, Cambridge University Press) and derive a new prediction for the non-ideal equilibrium -limit above which chaos emerges.

  19. Stellar Sources of Gamma-ray Bursts

    OpenAIRE

    Luchkov, B. I.

    2011-01-01

    Correlation analysis of Swift gamma-ray burst coordinates and nearby star locations (catalog Gliese) reveals 4 coincidences with good angular accuracy. The random probability is 4\\times 10^{-5}, so evidencing that coincident stars are indeed gamma-ray burst sources. Some additional search of stellar gamma-ray bursts is discussed.

  20. Benchmarking the Multidimensional Stellar Implicit Code MUSIC

    Science.gov (United States)

    Goffrey, T.; Pratt, J.; Viallet, M.; Baraffe, I.; Popov, M. V.; Walder, R.; Folini, D.; Geroux, C.; Constantino, T.

    2017-04-01

    We present the results of a numerical benchmark study for the MUltidimensional Stellar Implicit Code (MUSIC) based on widely applicable two- and three-dimensional compressible hydrodynamics problems relevant to stellar interiors. MUSIC is an implicit large eddy simulation code that uses implicit time integration, implemented as a Jacobian-free Newton Krylov method. A physics based preconditioning technique which can be adjusted to target varying physics is used to improve the performance of the solver. The problems used for this benchmark study include the Rayleigh-Taylor and Kelvin-Helmholtz instabilities, and the decay of the Taylor-Green vortex. Additionally we show a test of hydrostatic equilibrium, in a stellar environment which is dominated by radiative effects. In this setting the flexibility of the preconditioning technique is demonstrated. This work aims to bridge the gap between the hydrodynamic test problems typically used during development of numerical methods and the complex flows of stellar interiors. A series of multidimensional tests were performed and analysed. Each of these test cases was analysed with a simple, scalar diagnostic, with the aim of enabling direct code comparisons. As the tests performed do not have analytic solutions, we verify MUSIC by comparing it to established codes including ATHENA and the PENCIL code. MUSIC is able to both reproduce behaviour from established and widely-used codes as well as results expected from theoretical predictions. This benchmarking study concludes a series of papers describing the development of the MUSIC code and provides confidence in future applications.

  1. Microlensing and the physics of stellar atmospheres

    NARCIS (Netherlands)

    Sackett, PD; Menzies, JW; Sackett, PD

    2001-01-01

    The simple physics of microlensing provides a well understood tool with which to probe the atmospheres of distant stars in the Galaxy and Local Group with high magnification and resolution. Recent results in measuring stellar surface structure through broad band photometry and spectroscopy of high

  2. Evolution and seismic tools for stellar astrophysics

    CERN Document Server

    Monteiro, Mario JPFG

    2008-01-01

    A collection of articles published by the journal "Astrophysics and Space Science, Volume 316, Number 1-4", August 2008. This work covers 10 evolution codes and 9 oscillation codes. It is suitable for researchers and research students working on the modeling of stars and on the implementation of seismic test of stellar models.

  3. STELLAR TRANSITS IN ACTIVE GALACTIC NUCLEI

    International Nuclear Information System (INIS)

    Béky, Bence; Kocsis, Bence

    2013-01-01

    Supermassive black holes (SMBHs) are typically surrounded by a dense stellar population in galactic nuclei. Stars crossing the line of site in active galactic nuclei (AGNs) produce a characteristic transit light curve, just like extrasolar planets do when they transit their host star. We examine the possibility of finding such AGN transits in deep optical, UV, and X-ray surveys. We calculate transit light curves using the Novikov-Thorne thin accretion disk model, including general relativistic effects. Based on the expected properties of stellar cusps, we find that around 10 6 solar mass SMBHs, transits of red giants are most common for stars on close orbits with transit durations of a few weeks and orbital periods of a few years. We find that detecting AGN transits requires repeated observations of thousands of low-mass AGNs to 1% photometric accuracy in optical, or ∼10% in UV bands or soft X-ray. It may be possible to identify stellar transits in the Pan-STARRS and LSST optical and the eROSITA X-ray surveys. Such observations could be used to constrain black hole mass, spin, inclination, and accretion rate. Transit rates and durations could give valuable information on the circumnuclear stellar clusters as well. Transit light curves could be used to image accretion disks with unprecedented resolution, allowing us to resolve the SMBH silhouette in distant AGNs.

  4. Robust Modeling of Stellar Triples in PHOEBE

    Science.gov (United States)

    Conroy, Kyle E.; Prsa, Andrej; Horvat, Martin; Stassun, Keivan G.

    2017-01-01

    The number of known mutually-eclipsing stellar triple and multiple systems has increased greatly during the Kepler era. These systems provide significant opportunities to both determine fundamental stellar parameters of benchmark systems to unprecedented precision as well as to study the dynamical interaction and formation mechanisms of stellar and planetary systems. Modeling these systems to their full potential, however, has not been feasible until recently. Most existing available codes are restricted to the two-body binary case and those that do provide N-body support for more components make sacrifices in precision by assuming no stellar surface distortion. We have completely redesigned and rewritten the PHOEBE binary modeling code to incorporate support for triple and higher-order systems while also robustly modeling data with Kepler precision. Here we present our approach, demonstrate several test cases based on real data, and discuss the current status of PHOEBE's support for modeling these types of systems. PHOEBE is funded in part by NSF grant #1517474.

  5. On the collapse of iron stellar cores

    International Nuclear Information System (INIS)

    Barkat, Z.; Rakavy, G.; Reiss, Y.; Wilson, J.R.

    1975-01-01

    The collapse of iron stellar cores is investigated to see whether the outward shock produced by the bounce at neutron star density is sufficient to burn appreciable amounts of the envelope around the iron core. Several models were tried, and in all cases no appreciable burn took place; hence no explosion results from the collapse of these models

  6. Modular Stellarator Reactor conceptual design study

    International Nuclear Information System (INIS)

    Miller, R.L.; Bathke, C.G.

    1983-01-01

    A conceptual design study of the Modular Stellarator Reactor is summarized. The physics basis of the approach is elucidated with emphasis on magnetics performance optimization. Key engineering features of the fusion power core are described. Comparisons with an analogous continuous-helical-coil (torsatron) system are made as the basis of a technical and economic assessment

  7. Summary of the Advanced Stellar Compass

    DEFF Research Database (Denmark)

    Jørgensen, John Leif

    1997-01-01

    The current version of the Advanced Stellar Compass (ASC) is an improved implementation of the instrument developed for the Danish Geomagnetic Research Satellite Ørsted. The Ørsted version was successfully tested in space on the NASA sounding rocket "Thunderstorm III", that was launched September 2...

  8. Neutrino confinement in collapsing stellar cores

    International Nuclear Information System (INIS)

    Chung, K.C.

    1987-01-01

    Neutrino confinement is expected to occur in the core of highly evolved stars, leading to the formation of a degenerate neutrino gas. The main neutrino sources are briefly reviewed and the neutrino processes relevant to the neutrino opacity in the stellar matter are discussed. Implications for the equation of state of neutrino-trapped matter are examined. (author) [pt

  9. Survey of the MAgellanic Stellar History -- SMASH

    NARCIS (Netherlands)

    Nidever, David; Olsen, Knut; Besla, Gurtina; Gruendl, Robert; Saha, Abhijit; Gallart, Carme; Olszewski, Edward W.; Munoz, Ricardo; Monelli, Matteo; Kunder, Andrea; Kaleida, Catherine; Walker, Alistair; Stringfellow, Guy; Zaritsky, Dennis; van der Marel, Roeland; Blum, Robert; Vivas, Kathy; Chu, You-Hua; Martin, Nicolas; Conn, Blair; Noel, Noelia; Majewski, Steven; Jin, Shoko; Kim, Hwihyun; Cioni, Maria-Rosa; Bell, Eric; Monachesi, Antonela; de Boer, Thomas

    Over the last several years, various discoveries have drastically altered our view of the iconic Magellanic Clouds (MCs), the nearest interacting galaxy system. The best evidence is now that they are on first infall into the Milky Way, that their stellar populations extend much further than

  10. The evolution of stellar exponential discs

    NARCIS (Netherlands)

    Ferguson, AMN; Clarke, CJ

    2001-01-01

    Models of disc galaxies which invoke viscosity-driven radial flows have long been known to provide a natural explanation for the origin of stellar exponential discs, under the assumption that the star formation and viscous time-scales are comparable. We present models which invoke simultaneous star

  11. Modular stellarator reactor conceptual design study

    International Nuclear Information System (INIS)

    Miller, R.L.; Krakowski, R.A.; Bathke, C.G.

    1983-01-01

    A conceptual design study of the Modular Stellarator Reactor is summarized. The physics basis of the approach is elucidated with emphasis on magnetics performance optimization. Key engineering features of the fusion power core are described. Comparisons with an analogous continuous-helical-coil (torsatron) system are made as the basis of a technical and economic assessment

  12. The Stellar Imager (SI) Mission Concept

    Science.gov (United States)

    Carpenter, Kenneth G.; Schrijver, Carolus J.; Lyon, Richard G.; Mundy, Lee G.; Allen, Ronald J.; Armstrong, Thomas; Danchi, William C.; Karovska, Margarita; Marzouk, Joe; Mazzuca, Lisa M.; hide

    2002-01-01

    The Stellar Imager (SI) is envisioned as a space-based, UV-optical interferometer composed of 10 or more one-meter class elements distributed with a maximum baseline of 0.5 km. It is designed to image stars and binaries with sufficient resolution to enable long-term studies of stellar magnetic activity patterns, for comparison with those on the sun. It will also support asteroseismology (acoustic imaging) to probe stellar internal structure, differential rotation, and large-scale circulations. SI will enable us to understand the various effects of the magnetic fields of stars, the dynamos that generate these fields, and the internal structure and dynamics of the stars. The ultimate goal of the mission is to achieve the best-possible forecasting of solar activity as a driver of climate and space weather on time scales ranging from months up to decades, and an understanding of the impact of stellar magnetic activity on life in the Universe. In this paper we describe the scientific goals of the mission, the performance requirements needed to address these goals, the "enabling technology" development efforts being pursued, and the design concepts now under study for the full mission and a possible pathfinder mission.

  13. The Space Stellar Photometry Mission COROT: Asteroseismology ...

    Indian Academy of Sciences (India)

    tribpo

    detect giant extra solar planets (detectable by spectroscopy from the ground) and determine their albedo. As COROT is devoted to stellar photometry, aiming at both a high precision and a long observation time, the search for exoplanets by the transit method can easily be integrated in the payload and in the mission profile.

  14. Teaching stellar interferometry with polymer optical fibers

    Science.gov (United States)

    Illarramendi, M. A.; Arregui, L.; Zubia, J.; Hueso, R.; Sanchez-Lavega, A.

    2017-08-01

    In this manuscript we show the design of a simple experiment that reproduces the operation of the Michelson stellar interferometer by using step-index polymer optical fibers. The emission of stellar sources, single or binary stars, has been simulated by the laser light emerging from the output surface of the 2 meter-long polymer optical fiber. This light has an emission pattern that is similar to the emission pattern of stellar sources - circular, uniform, spatially incoherent, and quasi-monochromatic. Light coming from the fiber end faces passes through two identical pinholes located on a lid covering the objective of a small telescope, thus producing interference. Interference fringes have been acquired using a camera that is coupled to a telescope. The experiments have been carried out both outdoors in the daytime and indoors. By measuring the fringe visibilities, we have determined the size of our artificial stellar sources and the distance between them, when placing them at distances of 54 m from the telescope in the indoor measurements and of 75 m in the outdoor ones.

  15. Plea for stellarator funding raps tokamaks

    International Nuclear Information System (INIS)

    Blake, M.

    1992-01-01

    The funding crunch in magnetic confinement fusion development has moved the editor of a largely technical publication to speak out on a policy issue. James A. Rome, who edits Stellarator News from the Fusion Energy Division at Oak Ridge National Laboratory, wrote an editorial that appeared on the front page of the May 1992 issue. It was titled open-quotes The US Stellarator Program: A Time for Renewal,close quotes and while it focused chiefly on that subject (and lamented the lack of funding for the operation of the existing ATF stellarator at Oak Ridge), it also cited some of the problems inherent in the mainline MCF approach--the tokamak--and stated that if the money can be found for further tokamak design upgrades, it should also be found for stellarators. Rome wrote, open-quotes There is growing recognition in the US, and elsewhere, that the conventional tokamak does not extrapolate to a commercially competitive energy source except with very high field coils ( 1000 MWe).close quotes He pointed up open-quotes the difficulty of simultaneously satisfying conflicting tokamak requirements for efficient current drive, high bootstrap-current fraction, complete avoidance of disruptions, adequate beta limits, and edge-plasma properties compatible with improved (H-mode) confinement and acceptable erosion of divertor plates.close quotes He then called for support for the stellarator as open-quotes the only concept that has performance comparable to that achieved in tokamaks without the plasma-current-related limitations listed above.close quotes

  16. Elfos, creación literaria y artística en la primera infancia

    Directory of Open Access Journals (Sweden)

    BLANCA LUCÍA BUSTAMANTE VÉLEZ

    2010-01-01

    Full Text Available Artículo producto de la investigación denominada "Elfos, creación literaria y artística en la primera infancia", que explora el mundo escritural del infante a partir de un diagnóstico sobre creación literaria y artística, realizado con los niños y niñas de transición del Instituto Técnico Gonzalo Suárez Rendón y el Jardín Infantil de la Universidad Pedagógica y Tecnológica de Colombia. Se aplicaron estrategias de enseñanza-aprendizaje en las dos instituciones educativas citadas, a partir del diseño y desarrollo de talleres en los que se utilizaron materiales artísticos y en los cuales se pudo evidenciar la capacidad creativa e imaginativa de los niños. La investigación propone una manera novedosa de estimular la creatividad en los niños de preescolar para crear hábitos de lectura y escritura como expresión literaria y artística, a la vez que fomenta el desarrollo de habilidades y el mejoramiento de su proceso de aprendizaje.

  17. Peritajes psicológicos forenses en decisiones judiciales de primera instancia en delitos sexuales

    Directory of Open Access Journals (Sweden)

    Milena M. Rudas

    2016-01-01

    Full Text Available Se analiza la importancia de los informes psicológicos forenses en la toma de decisiones judiciales de primera instancia en delitos sexuales en la ciudad de Barranquilla (Colombia mediante un enfoque cuantitativo de alcance descriptivo. Se analizaron diversas variables con el propósito de categorizar si en las sentencias judiciales se menciona la pericial por el juez al momento de dictarlas, y cuál es el valor diferencial de los informes psicológicos forenses. También se revisó la concordancia entre la decisión final del juez y los resultados plasmados en el informe psicológico. Como conclusión significativa se obtuvo que en el 80 % de las sentencias hubo mención a la pericial por el juez al fundamentar su decisión; en un 80 % de los casos el juez tomó la decisión de manera concordante con los resultados del informe psicológico. Como conclusión se plantea que para la Administración de Justicia se requiere personal auxiliar especializado y que el psicólogo jurídico en función forense funge como fuente directa de conocimiento, y se constituye en un medio de convicción apreciable.

  18. Autoestima e idioma inglés: una primera discusión

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    Raúl Montes de Oca Rodríguez

    2005-01-01

    Full Text Available El artículo “Autoestima e idioma inglés: una primera discusión”, trata sobre la importancia que reviste la parte afectiva en el aprendizaje, en este caso, de una lengua extranjera como el inglés, en el medio costarricense. En ese sentido, se da una visión de lo que la ciencia cognoscitiva y las corrientes humanísticas proponen en cuanto a aprendizaje, rendimiento académico y aprendizaje de una lengua extranjera se refiere. Seguidamente, se hace un recorrido histórico del tema autoestima y se definen términos como autoestima, autoestima baja y alta. Además se analiza el aspecto adquisición/aprendizaje de un idioma y se ubica el tema en el sistema educativo costarricense. También se discute la situación de la enseñanza-aprendizaje de idiomas en nuestro medio y los aspectos que relacionan lo afectivo con el aprendizaje del inglés

  19. La matematización de los procesos químicos. Primera parte

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    Rómulo Gallego Badillo

    2012-04-01

    Full Text Available Dada la extensión del presente aporte se ha decidido dividirlo en dos partes. En la primera se adelanta una reconstrucción de la historia del modelo cinético molecular de los gases y de la termodinámica clásica, y se realiza una aproximación al análisis epistemológico. En la segunda se intenta también una reconstrucción histórica de la creación de la fisicoquímica como disciplina científica y la introducción de la mirada desde la termodinámica clásica de los procesos químicos, asumidos como sistemas y como “máquinas térmicas”. Se irá más allá de la inicialmente designada como “dinámica química”. El objetivo consiste en elaborar una explicación admisible que dé cuenta de la introducción en el discurso químico, de una matemática de mayor complejidad que la propia del álgebra, dentro de la cual se construyó, durante la segunda mitad del siglo XIX, la química como ciencia, construcción ésta basada en las leyes ponderales.

  20. La configuración de Oriente Próximo tras la Primera Guerra Mundial

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    Paloma García

    2015-01-01

    Full Text Available Al cumplirse un siglo del estallido de la Primera Guerra Mundial, este trabajo ensaya un balance reflexivo sobre las repercusiones derivadas para Oriente Próximo a partir del conjunto de decisiones políticas, compromisos diplomáticos, acuerdos internacionales y actuaciones institucionales y personales efectuados tanto por los dirigentes y potencias vencedoras como por otros agentes implicados en el complejo proceso post-bélico que, sujeto al artículo 22 del Pacto de la Sociedad de Naciones, quedó marcado por los principios wilsonianos que entonces pretendían definir un nuevo orden mundial. Sin determinismo alguno, quedó trazado así no sólo el mapa político sino también las condiciones que durante décadas definirían la convivencia política de los pueblos afectados, su hipotético progreso económico, social y cultural y, sobre todo, los nexos geopolíticos, objetivos estratégicos y valores civilizatorios que implícita y expresamente traducían el núcleo de unos planes dictados en su mayoría por el interés de las potencias coetáneas.

  1. Violencia social en la primera mitad del siglo XIX mexicano: el caso de las Huastecas

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    Escobar Ohmstede, Antonio

    2009-08-01

    Full Text Available This article looks at the different phases of the violence in the Huasteca space social during the first half of the nineteenth century. It offers a careful analysis of each of the rebellions considering their causes as well as the participation of many groups involved. It analysis the role of Indians, mestizos and mulatoes living in the pueblos and private propieraties and even important members of the elites and finally identifies their alliances and mechanisms of patronage used by these groups.

    El presente artículo observa varias fases de la violencia rural que se dio en un espacio social del noreste de México denominado las Huastecas en la primera mitad del siglo XIX. Se abordan los movimientos sociales atendiendo tanto a sus causas, como a los actores y generadores de la violencia colectiva. Al respecto se analiza el papel de los indígenas, mulatos y mestizos que vivían en los pueblos y en las propiedades privadas y los mecanismos y alianzas que se dieron entre los diversos grupos de poder regional.

  2. The Quasi-Toroidal Stellarator: An Innovative Confinement Experiment

    International Nuclear Information System (INIS)

    Knowlton, S. F.

    2001-01-01

    To develop a new class of stellarators that exhibit improved confinement compared to conventional stellarators. This approach generally makes use of a designed symmetry of the magnetic field strength along a particular coordinate axis in the toroidal geometry of the stellarator, and is referred to as quasi-symmetry

  3. Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions

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    Douglas Rubin

    2011-01-01

    Full Text Available The dense concentration of stars and high-velocity dispersions in the Galactic center imply that stellar collisions frequently occur. Stellar collisions could therefore result in significant mass loss rates. We calculate the amount of stellar mass lost due to indirect and direct stellar collisions and find its dependence on the present-day mass function of stars. We find that the total mass loss rate in the Galactic center due to stellar collisions is sensitive to the present-day mass function adopted. We use the observed diffuse X-ray luminosity in the Galactic center to preclude any present-day mass functions that result in mass loss rates >10-5M⨀yr−1 in the vicinity of ~1″. For present-day mass functions of the form, dN/dM∝M-α, we constrain the present-day mass function to have a minimum stellar mass ≲7M⨀ and a power-law slope ≳1.25. We also use this result to constrain the initial mass function in the Galactic center by considering different star formation scenarios.

  4. Medidas de experiencia e cienciometria para avaliar impacto da producao cientifica

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    Marco Akerman

    2013-08-01

    Full Text Available Propõe-se a “experienciometria” como medida da experiência acadêmica de pesquisadores de modo a complementar a medida consagrada da cienciometria nas avaliações de competências em pesquisa. O artigo baseia-se em parte na produção cientifica do autor, utilizada sob uma perspectiva qualitativa para explorar possibilidades de análise de impactos. Ensaia-se uma síntese com possíveis implicações dessa análise, indicando algumas possibilidades para se avaliar impacto de pesquisas e artigos que não se restrinjam exclusivamente à contagem de números de citações dos autores para o cálculo do fator de impacto.

  5. La medida de la inteligencia emocional en el ámbito psicoeducativo

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    Iratxe Antonio-Agirre

    2017-01-01

    Full Text Available La diversidad individual que alberga la escuela representa un reto ineludible. Para promover el desarrollo integral del alumnado resulta necesario favorecer competencias para la vida, como la inteligencia emocional, que les ayuden a lograr un mejor ajuste sociopersonal y escolar. Sin embargo, la diversidad conceptual en torno a la inteligencia emocional ha contribuido a la proliferación de medidas y ha dificultado la integración de la investigación. En todo caso, atendiendo a las propiedades psicométricas y a las dimensiones que miden, este trabajo recoge los principales instrumentos de medida de la inteligencia emocional que posibilitan una evaluación más rigurosa y exhaustiva del constructo en niños, niñas y adolescentes.

  6. Medida de la eficiencia ambiental en la industria cerámica española

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    Sala Garrido, Ramon

    2008-01-01

    Full Text Available En el trabajo de Färe, Grosskopf y Hernández-Sancho (2004 se propone un índice de eficiencia medioambiental, para medir el grado en el que las empresas generan outputs deseables al mismo tiempo que reducen su outputs no deseables. Este indicador consiste en una ratio entre una medida para outputs deseables y otra para no deseables. Cada uno de ellos está basado en el uso de las funciones distancia. El índice de los outputs deseables mide el éxito de una empresa k en aumentar estos outputs utilizando el mismo número de inputs y generando el mismo nivel de outputs no deseables. Esta medida de eficiencia medioambiental se ha aplicado a la industria de los pavimentos cerámicos sobre una muestra de empresas a las que se ha aplicado un test de Kruskal-Wallis para determinar la utilidad de este indicador.

  7. Medidas de aislamiento en enfermedades transmisibles dentro del ámbito hospitalario

    OpenAIRE

    Villanueva Rábano, Raúl

    2016-01-01

    En el ámbito hospitalario, son un problema frecuente las infecciones nosocomiales, causadas por las enfermedades transmisibles que pasan de unos pacientes a otros. Estas infecciones son potencialmente prevenibles, a través de medidas de aislamiento llevadas a cabo por el personal sanitario y no sanitario encargado de atender al paciente. En este aspecto, el papel del personal de enfermería es de fundamental importancia dado que mantienen un estrecho contacto con el paciente como cuidadores pr...

  8. CONTROL EJECUTIVO Y FLUIDEZ VERBAL EN POBLACIÓN INFANTIL: MEDIDAS CUANTITATIVAS, CUALITATIVAS Y TEMPORALES

    Directory of Open Access Journals (Sweden)

    JULIÁN MARINO

    2011-01-01

    Full Text Available Para evaluar la evocación de palabras asociadas bajo una consigna de prueba de fluidez verbal (PFV se tienen en cuenta la cantidad de palabras producidas, las asociaciones categoriales y fonológicas entre ellas y el tiempo en que son evocadas. A continuación se presenta un estudio que se realizó aplicando PFV semánticas y fonológicas en una población infantil (8 - 12 años de la ciu dad de Granada (España, que tuvo por objetivos: (1 revisar las tradicionales medidas en PFV, (2 actualizar los índices temporales de medición y (3 presentar combinaciones de éstas con el fin de establecer con mayor precisión la participación del control ejecutivo en PFV. Se encontraron resultados significativos entre los que se destaca que la combinación entre la medida temporal de evocación de palabras conjuntas y la cualitativa de palabras en relación cluster podría aislar con mayor fiabilidad el compromiso de funciones ejecutivas como el control inhibitorio y la flexibilidad cognitiva. Esto se determinó empleando medidas de regresión, ingre sando como variables independientes funciones ejecutivas y como variables dependientes cada una de las medidas de Fluidez Verbal. Para la mencionada combinación de palabras conjuntas - palabras en relación cluster (PFV fonológica letra P se halló un R2 de .41 (p = .000 ingresando como variables predictoras el Trail Making B y la parte Color - Palabra de la versión Trenerry del paradigma Stroop (Lezak, 1995. Se describen también otras posibilidades de medición temporales - cualitativas y su posible utilidad clínica y de investigación.

  9. Medidas de bioseguridad adoptadas en el manejo con materiales biológicos en Laboratorios Liorad

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    Nancy Burguet Lago

    2013-03-01

    Full Text Available Introducción: el trabajo con microorganismos puede conllevar a riesgos tanto para el personal que trabaja con los mismos como para el medio ambiente. La existencia de laboratorios de seguridad biológica y la implementación de medidas en la manipulación de los agentes biológicos minimizan el riesgo. Objetivo: evaluar las medidas de bioseguridad adoptadas en el manejo con materiales biológicos en Laboratorios Liorad. Métodos: empleo de una lista de chequeo y análisis de los resultados a través de una Matriz DAFO para valorar si el diseño de la instalación cumple con la bioseguridad. Además establecer un sistema documental para la manipulación de microorganismos y la confección de un plan de capacitación para el personal que trabaja en el laboratorio de control microbiológico. Resultados: la lista de chequeo permitió identificar como principal debilidad el no disponer de un doble pasillo para el traslado del material limpio y sucio. Como fortalezas, cumplir con las prácticas y procesamientos adecuados y el contar con equipos de seguridad biológica. El sistema documental incorporó a los procedimientos establecidos para la manipulación, un acápite referido a la «Peligrosidad y Medidas de Seguridad». El programa de capacitación desarrollado permitió proveer conocimientos específicos referidos a esta temática. Conclusión: las medidas adoptadas en el laboratorio permiten plantear que de manera general se cumplen los requisitos establecidos en materia de Bioseguridad para el trabajo con microorganismos.

  10. Medidas Explícitas e Implícitas de las Actitudes Hacia las Mujeres

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    Manuel Cárdenas

    2009-01-01

    Full Text Available El presente estudio tiene como objeto utilizar el IAT (Implicit Association Test para medir actitudes hacia las mujeres, de modo de comparar dichas evaluaciones de carácter automático con las obtenidas por medio de una medida explícita. Además, los participantes respondieron a un inventario de roles sexuales de modo de ver si los sujetos manejaban el estereotipo dominante asociado a lo femenino y sus efectos sobre el prejuicio. La muestra quedó conformada por 80 estudiantes universitarios. No se detectaron diferencias significativas entre hombres y mujeres en los estereotipos asociados a la mujer, ni en la evaluación que se hace de estas (medida explícita. En la medida de IAT las diferencias entre sexos aparecen, indicando que los hombres muestran una actitud implícita más negativa hacia las mujeres. De este modo se confirma que la aparente disminución del prejuicio que puede constatarse en los cuestionarios podría encubrir el hecho de que las actitudes negativas se mantienen a nivel implícito.

  11. Violência Juvenil e Medidas Socioeducativas: Revisão de Literatura

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    Jacqueline de Oliveira Moreira

    2017-10-01

    Full Text Available RESUMO Neste artigo, partindo do objetivo de compreender a relação entre violência juvenil e a resposta do Estado através das medidas socioeducativas, buscamos explicitar o pano de fundo das pesquisas científicas atuais. Realizamos uma meta-análise dos artigos publicados sobre adolescência e medidas socioeducativas, no campo da psicologia, entre os anos de 2000 e 2012. Concluímos que essa produção nacional pode ser reunida em três grandes categorias: (a prático-experiencial, que apresenta relatos analíticos da prática na aplicação das medidas socioeducativas, privilegiando a experiência concreta; (b político-institucional, que discute criticamente a dimensão política da lógica socioeducativa, detendo-se na análise estrutural de sua legislação e de suas instituições; (c sociocultural, que analisa os determinantes sociais e psíquicos do fenômeno da violência juvenil.

  12. Medidas cautelares innominadas en la protección de los derechos de autor y conexos en Colombia

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    Nixon Jefrey Gil Aguirre

    2016-12-01

    Full Text Available Actualmente, el ejercicio de funciones jurisdiccionales atribuidas a las autoridades administrativas ha generado interpretaciones judiciales confusas, en la aplicación de medidas cautelares innominadas para la protección de derechos de autor y conexos en Colombia; así lo evidencia el análisis realizado a las medidas cautelares descritas en la Ley 1493 del año 2011, que otorgó competencias de inspección, vigilancia y control sobre las sociedades de gestión colectiva de derechos de autor y conexos; en este sentido se requiere describir las funciones jurisdiccionales de la Dirección Nacional de Derecho de Autor respecto a las medidas cautelares y su importancia en la protección de los derechos de autor y conexos, al igual que analizar las medidas cautelares innominadas desde su origen, las características y lo propuesto por la Corte Constitucional en materia de funciones jurisdiccionales de la Dirección Nacional de Derecho de Autor y respecto de la procedencia de las medidas cautelares innominadas como competencia de esta entidad. Se concluye que las medidas cautelares nominadas no son suficientes, y que se hace necesario acudir a las medidas cautelares innominadas, como herramienta jurídica del funcionario administrativo, sin que ello implique arbitrariedad y prejuzgamiento en el proceso.

  13. Stellar Streams Discovered in the Dark Energy Survey

    Energy Technology Data Exchange (ETDEWEB)

    Shipp, N.; et al.

    2018-01-09

    We perform a search for stellar streams around the Milky Way using the first three years of multi-band optical imaging data from the Dark Energy Survey (DES). We use DES data covering $\\sim 5000$ sq. deg. to a depth of $g > 23.5$ with a relative photometric calibration uncertainty of $< 1 \\%$. This data set yields unprecedented sensitivity to the stellar density field in the southern celestial hemisphere, enabling the detection of faint stellar streams to a heliocentric distance of $\\sim 50$ kpc. We search for stellar streams using a matched-filter in color-magnitude space derived from a synthetic isochrone of an old, metal-poor stellar population. Our detection technique recovers four previously known thin stellar streams: Phoenix, ATLAS, Tucana III, and a possible extension of Molonglo. In addition, we report the discovery of eleven new stellar streams. In general, the new streams detected by DES are fainter, more distant, and lower surface brightness than streams detected by similar techniques in previous photometric surveys. As a by-product of our stellar stream search, we find evidence for extra-tidal stellar structure associated with four globular clusters: NGC 288, NGC 1261, NGC 1851, and NGC 1904. The ever-growing sample of stellar streams will provide insight into the formation of the Galactic stellar halo, the Milky Way gravitational potential, as well as the large- and small-scale distribution of dark matter around the Milky Way.

  14. La primera autobiografía femenina en castellano las "Memorias" de Leonor López de Córdoba

    OpenAIRE

    Bellido Bello, Juan Félix

    2006-01-01

    Todos los críticos que se han ocupado de las Memorias de Leonor López de Córdoba insisten en señalarlo como la primera manifestación castellana del género autobiográfico. Pero dicho texto todavía no ha sido suficientemente estudiado ni considerado a la ho Todos los críticos que se han ocupado de las Memorias de Leonor López de Córdoba insisten en señalarlo como la primera manifestación castellana del género autobiográfico. Pero dicho texto todavía no ha sido suficientemente estudiado ni co...

  15. La presencia norteamericana en el agro sinaloense en la primera mitad del siglo XX

    Directory of Open Access Journals (Sweden)

    Hubert Carton de Grammont

    1986-05-01

    Full Text Available El presente artículo nos presenta el panorama del agro sinaloense desde finales del siglo XIX hasta los años treinta, en que el gobierno federal realizó el reparto agrario. Los extranjeros tenían el control económico tanto sobre las tierras, como sobre la producción de cultivos, los ingenios azucareros, las concesiones sobre las redes ferroviarias, etc. En reacción contra la política porfirista de dar facilidades a la inversión extranjera en el país, en particular a la agricultura, los gobiernos pos-revolucionarios se vieron en la necesidad de limitar la influencia y el poder de los extranjeros, especialmente de los norteamericanos en la economía nacional. Después del reparto cardenista se prosiguió al reparto agrario con la apertura de los distritos de riego y la aplicación de la Ley Federal de Aguas. A lo largo de estos años, las compañías norteamericanas salieron poco a poco del sector de la producción agrícola. Sin embargo, al cabo del tiempo, a partir de los sesenta las agroindustrias internacionales volvieron a penetrar con tal fuerza que ahora en gran medida la agricultura mexicana está dominada por el capital agroindustrial extranjero, esencialmente norteamericano.

  16. Características habitacionales en Jujuy, Argentina, en la primera mitad del siglo XX

    Directory of Open Access Journals (Sweden)

    Marcelo Jerez

    2012-08-01

    Full Text Available Este artículo analiza las condiciones habitacionales de la población de la provincia de Jujuy en la primera mitad del siglo XX, a la luz de los cambios y continuidades en el proceso de crecimiento económico local y nacional. Mucho se sabe acerca del problema de la vivienda en Argentina, sobre todo en el ámbito rioplatense, pero poco se ha profundizado sobre sus características e implicancias en otras regiones tales como en el Noroeste. De este modo, al centrar la atención en Jujuy se rescata no sólo la experiencia jujeña, sino también se develan ciertos rasgos habitacionales compartidos en esta región. A lo largo de este estudio se brindan nuevos aportes que son articulados dentro de aquel conocimiento en el nivel nacional y, cuando ello es posible, también discutidos.This paper examines the housing situation of the population of the province of Jujuy in the first half of the twentieth century, in light of the changes and continuance in the process of local economic growth. Much is known about the problem of housing in Argentina, especially in the River Plate area, but little has been deepened on its characteristics and implications in other regions such as the Northwest. Thus, the focus of the observation in Jujuy not only is rescued this provincial experience but it has also revealed certain housing traits shared in this region. In this study it is provided new contributions that are articulated with the national knowledge and, when possible, also discussed.

  17. La primera exposición de esculturas celebrada en el Real Museo de Pinturas

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    Rose-De Viejo, Isadora

    2005-03-01

    Full Text Available Documents preserved in the archives of the Prado Museum and the Madrid Royal Palace, an announcement in the Diario de Madrid and the testimony of a foreign resident, reveal that the first sculptural works exhibited in the then still denominated Royal Painting Museum for a period of fifteen days in January 1827, were two full-length seated portrait statues executed in Rome: Carlos IV (1817 by Ramón Barba and María Luisa de Parma (1816 by José Alvarez Cubero. This must have been a major cultural and political event that until now had not been noted in the literature on the history of the museum.

    Documentos conservados en los archivos del Museo del Prado y del Palacio Real, un anuncio aparecido en el Diario de Madrid y el testimonio de un forastero, revelan que las primeras esculturas expuestas en el entonces todavía denominado Real Museo de Pinturas durante quince días de enero de 1827, fueron dos estatuas sedentes de cuerpo entero ejecutadas en Roma: el Carlos IV (1817 de Ramón Barba y la María Luisa de Parma (1816 de José Alvarez Cubero. Esto debió ser un acontecimiento cultural y político que hasta ahora no se había recogido en la literatura sobre la historia del museo.

  18. PROBLEMAS DE PRIMERA Y SEGUNDA GENERACIÓN EN LA DEMOCRACIA REGIONAL EN MÉXICO

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    Alberto Aziz Nassif

    2003-01-01

    Full Text Available Durante muchos años se pensó que todo el autoritarismo mexicano estaba protegido por un sistema electoral que distorsionaba la voluntad ciudadana y la posibilidad de que hubiera alternancia en el poder. Después de que el sistema electoral generó la competencia y la alternancia en el poder, existió la tentación de pensar que la construcción democrática se llevaría a cabo de forma casi automática. Sin embargo, ahora se puede afirmar que la democracia mexicana tiene problemas importantes que van más lejos que los que rondaban el espacio de los votos y la representación. El trabajo plantea una hipótesis para reflexionar sobre lo que hemos llamado problemas de primera y segunda generación en la democracia mexicana. Los primeros responden a la interrogante: ¿cómo lograr elecciones competidas, asegurar la posibilidad de la alternancia y el pluralismo? Sus problemas son: reglas equitativas, transparencia, y posibilidad de alternancia. La segunda generación de problemas tiene como objetivo central investigar cómo se logran buenos gobiernos o por qué razones no se dan. Se trata de saber cuáles son los márgenes para desterrar los modos autoritarios de gobernar, los abusos de poder, las decisiones arbitrarias, el manejo patrimonial de los recursos públicos y la sistemática corrupción que ha impregnado el espacio público durante décadas. Se toman dos ejemplos regionales, Chihuahua y Jalisco.

  19. CASTIGO FEMENINO EN CHILE DURANTE LA PRIMERA MITAD DEL SIGLO XIX

    Directory of Open Access Journals (Sweden)

    Marcelo Neira Navarro

    2004-12-01

    Full Text Available El presente artículo permitió generar una serie de categorías de castigos femeninos, considerando que durante buena parte del siglo XIX la policía pudo aplicar "justicia correccional", es decir, sancionar delitos menores. De un universo de más de 32.000 arrestos efectuados en la ciudad de Santiago de Chile entre los años 1830 a 1840 y utilizando el criterio "femenino", el levantamiento logró una muestra que alcanzó al 12% del total. Los datos sistematizados permiten señalar que durante la primera mitad del siglo XIX el delito femenino fue parte importante de la actividad represiva en Chile y dio origen a un castigo relacionado a la Cárcel Correccional. Aunque también se observan otras penas como trabajo de casa formal o encierro en monasterios, forman parte de un circuito restrictivo en función del encierro de mujeres.The present article allowed to generate a series of categories of female punishments, considering that during a great part of the XIX century the police could apply "correctional justice", in other words, punish minor offences. In a universe of more than 32,000 arrest in the city of Santiago, Chile between the years 1830 and 1840 and using a "female" criteria, the uprising achieved a sample that reached 12% of the total. The systematized information shows that during the firt half of the xix century the female offence was an important part of the repressive activity in Chile and it gave origin to a punishment related to a correctional. Even though some other punishments were observed such a work in a formal house or monastery confinemet, they formed part of a restricting circuit functioning with the confinement of women.

  20. Modular Stellarator Fusion Reactor (MSR) concept

    International Nuclear Information System (INIS)

    Miller, R.L.; Krakowski, R.A.

    1981-01-01

    A preliminary conceptual study has been made of the Modulator Stellarator Reactor (MSR) as a stedy-state, ignited, DT-fueled, magnetic fusion reactor. The MSR concept combines the physics of classic stellarator confinement with an innovative, modular-coil design. Parametric tradeoff calculations are described, leading to the selection of an interim design point for a 4.8-GWt plant based on Alcator transport scaling and an average beta value of 0.04 in an l = 2 system with a plasma aspect ratio of 11. Neither an economic analysis nor a detailed conceptual engineering design is presented here, as the primary intent of this scoping study is the elucidation of key physics tradeoffs, constraints, and uncertainties for the ultimate power-reactor embodiment

  1. Time variations of stellar water masers

    International Nuclear Information System (INIS)

    Cox, G.G.; Parker, E.A.

    1979-01-01

    The 22-GHz H 2 O spectra of the stars RS Vir, RT Vir, R Aql, W Hya, U Her, S Cr B, Rx Boo, R Crt and VY CMa have been observed at intervals during the period 1974 September -1977 May. Optical and infrared measurements have also been made. New components have been observed in the H 2 O spectra of most of the stars, and the flux density of W Hya reached 2000 Jy near Jd 2442700. The intensities of the three main groups of components in VY CMa varied in phase consistent with a central pump source. In several stars the intensities were very different from those found by earlier observers, showing that stellar H 2 O masers are often not stable for more than a few cycles of the stellar luminosity. For part of the time the H 2 O and infrared intensities of R Aql and RS Vir were anticorrelated. (author)

  2. A Compact Quasi-axisymmetric Stellarator Reactor

    International Nuclear Information System (INIS)

    Ku, L.P.

    2003-01-01

    We report the progress made in assessing the potential of compact, quasi-axisymmetric stellarators as power-producing reactors. Using an aspect ratio A=4.5 configuration derived from NCSX and optimized with respect to the quasi-axisymmetry and MHD stability in the linear regime as an example, we show that a reactor of 1 GW(e) maybe realizable with a major radius *8 m. This is significantly smaller than the designs of stellarator reactors attempted before. We further show the design of modular coils and discuss the optimization of coil aspect ratios in order to accommodate the blanket for tritium breeding and radiation shielding for coil protection. In addition, we discuss the effects of coil aspect ratio on the peak magnetic field in the coils

  3. Excitation of solar and stellar oscillations

    International Nuclear Information System (INIS)

    Baudin, Frederic

    2009-01-01

    In this report for an Accreditation to Supervise Research (HDR), and after an introduction which outlines the potential of helio-seismology, the author addresses the problem of excitation and amplitude of stellar oscillations with respect to their most important aspects, i.e. the theoretical framework of the present understanding of excitation mechanisms, and instrumental influences on measurements which are used to assess excitation rates, the difficulty to perform these measurements, and their analysis in some various cases. Thus, the author addresses excitation mechanisms of stellar oscillation (stochastic excitation, opacity- related excitation, and other excitation mechanisms), the excitation of solar modes (observation and theoretical predictions, influence of magnetic phenomena, solar g modes), and the excitation of modes in other stars (solar-type pulsators, red giants, and not so conventional pulsators such as HD180642 and Be stars like HD49330)

  4. Stellar evolution as seen by mixed modes

    Directory of Open Access Journals (Sweden)

    Mosser Benoît

    2015-01-01

    Full Text Available The detection of mixed modes in subgiants and red giants allows us to monitor stellar evolution from the main sequence to the asymptotic giant branch and draw seismic evolutionary tracks. Quantified asteroseismic definitions that characterize the change in the evolutionary stages have been defined. This seismic information can now be used for stellar modelling, especially for studying the energy transport in the helium burning core or for specifying the inner properties of stars all along their evolution. Modelling will also allow us to study stars identified in the helium subflash stage, high-mass stars either arriving or quitting the secondary clump, or stars that could be in the blue-loop stage.

  5. Physics of stellar evolution and cosmology

    International Nuclear Information System (INIS)

    Goldberg, H.S.; Scadron, M.D.

    1981-01-01

    Astrophysical phenomena are examined on a fundamental level, stressing basic physical laws, in a textbook suitable for a one-semester intermediate course. The ideal gas law, the meaning of temperature, black-body radiation, discrete spectra, and the Doppler effect are introduced and used to study such features of the interstellar medium as 21-cm radiation, nebulae and dust, and the galactic magnetic field. The phases of stellar evolution are discussed, including stellar collapse, quasi-hydrostatic equilibrium, the main sequence, red giants, white dwarves, neutron stars, supernovae, pulsars, and black holes. Among the cosmological topics covered are the implications of Hubble's constant, the red-shift curve, the steady-state universe, the evolution of the big bang (thermal equilibrium, hadron era, lepton era, primordial nucleosynthesis, hydrogen recombination, galaxy formation, and the cosmic fireball), and the future (cold end or big crunch). 72 references

  6. Stellar physics with the ALHAMBRA photometric system

    International Nuclear Information System (INIS)

    Villegas, T Aparicio; Alfaro, E J; Moles, M; Benítez, N; Perea, J; Olmo, A del; Cristóbal-Hornillos, D; Cervio, M; Delgado, R M González; Márquez, I; Masegosa, J; Prada, F; Cabrera-Caño, J; Fernández-Soto, A; Aguerri, J A L; Cepa, J; Broadhurst, T; Castander, F J; Infante, L; Martínez, V J

    2011-01-01

    The ALHAMBRA photometric system was specifically designed to perform a tomography of the Universe in some selected areas. Although mainly designed for extragalactic purposes, its 20 contiguous, equal-width, medium-band photometric system in the optical wavelength range, shows a great capacity for stellar classification. In this contribution we propose a methodology for stellar classification and physical parameter estimation (T eff , log g, [Fe/H], and color excess E(B – V)) based on 18 independent reddening-free Q-values from the ALHAMBRA photometry. Based on the theoretical Spectral library BaSeL 2.2, and applied to 288 stars from the Next Generation spectral Library (NGSL), we discuss the reliability of the method and its dependence on the extinction law used.

  7. Isotope ratio in stellar atmospheres and nucleosynthesis

    International Nuclear Information System (INIS)

    Barbuy, B.L.S.

    1987-01-01

    The determination of isotopic ratios in stellar atmospheres is studied. The isotopic shift of atomic and molecular lines of different species of a certain element is examined. CH and MgH lines are observed in order to obtain the 12 C: 13 C and 24 Mg: 25 Mg: 26 Mg isotpic ratios. The formation of lines in stellar atmospheres is computed and the resulting synthetic spectra are employed to determine the isotopic abundances. The results obtained for the isotopic ratios are compared to predictions of nucleosynthesis theories. Finally, the concept of primary and secondary element is discussed, and these definitions are applied to the observed variations in the abundance of elements as a function of metallicity. (author) [pt

  8. STELLTRANS: A Transport Analysis Suite for Stellarators

    Science.gov (United States)

    Mittelstaedt, Joseph; Lazerson, Samuel; Pablant, Novimir; Weir, Gavin; W7-X Team

    2016-10-01

    The stellarator transport code STELLTRANS allows us to better analyze the power balance in W7-X. Although profiles of temperature and density are measured experimentally, geometrical factors are needed in conjunction with these measurements to properly analyze heat flux densities in stellarators. The STELLTRANS code interfaces with VMEC to find an equilibrium flux surface configuration and with TRAVIS to determine the RF heating and current drive in the plasma. Stationary transport equations are then considered which are solved using a boundary value differential equation solver. The equations and quantities considered are averaged over flux surfaces to reduce the system to an essentially one dimensional problem. We have applied this code to data from W-7X and were able to calculate the heat flux coefficients. We will also present extensions of the code to a predictive capacity which would utilize DKES to find neoclassical transport coefficients to update the temperature and density profiles.

  9. Energetic Particle Estimates for Stellar Flares

    Science.gov (United States)

    Youngblood, Allison; Chamberlin, Phil; Woods, Tom

    2018-01-01

    In the heliosphere, energetic particles are accelerated away from the Sun during solar flares and/or coronal mass ejections where they frequently impact the Earth and other solar system bodies. Solar (or stellar) energetic particles (SEPs) not only affect technological assets, but also influence mass loss and chemistry in planetary atmospheres (e.g., depletion of ozone). SEPs are increasingly recognized as an important factor in assessing exoplanet habitability, but we do not yet have constraints on SEP emission from any stars other than the Sun. Until indirect measurements are available, we must assume solar-like particle production and apply correlations between solar flares and SEPs detected near Earth to stellar flares. We present improved scaling relations between solar far-UV flare flux and >10 MeV proton flux near Earth. We apply these solar scaling relations to far-UV flares from exoplanet host stars and discuss the implications for modeling chemistry and mass loss in exoplanet atmospheres.

  10. On Utmost Multiplicity of Hierarchical Stellar Systems

    Directory of Open Access Journals (Sweden)

    Gebrehiwot Y. M.

    2016-12-01

    Full Text Available According to theoretical considerations, multiplicity of hierarchical stellar systems can reach, depending on masses and orbital parameters, several hundred, while observational data confirm the existence of at most septuple (seven-component systems. In this study, we cross-match the stellar systems of very high multiplicity (six and more components in modern catalogues of visual double and multiple stars to find among them the candidates to hierarchical systems. After cross-matching the catalogues of closer binaries (eclipsing, spectroscopic, etc., some of their components were found to be binary/multiple themselves, what increases the system's degree of multiplicity. Optical pairs, known from literature or filtered by the authors, were flagged and excluded from the statistics. We compiled a list of hierarchical systems with potentially very high multiplicity that contains ten objects. Their multiplicity does not exceed 12, and we discuss a number of ways to explain the lack of extremely high multiplicity systems.

  11. Stellar clusters in the Gaia era

    Science.gov (United States)

    Bragaglia, Angela

    2018-04-01

    Stellar clusters are important for astrophysics in many ways, for instance as optimal tracers of the Galactic populations to which they belong or as one of the best test bench for stellar evolutionary models. Gaia DR1, with TGAS, is just skimming the wealth of exquisite information we are expecting from the more advanced catalogues, but already offers good opportunities and indicates the vast potentialities. Gaia results can be efficiently complemented by ground-based data, in particular by large spectroscopic and photometric surveys. Examples of some scientific results of the Gaia-ESO survey are presented, as a teaser for what will be possible once advanced Gaia releases and ground-based data will be combined.

  12. Dois pesos e duas medidas: uma proposta para discutir a natureza do sistema de unidades de medida na sala de aula

    Directory of Open Access Journals (Sweden)

    Lidiany C. de O. Godoi

    2009-01-01

    Full Text Available http://dx.doi.org/10.5007/2175-7941.2008v25n3p523 Sugerimos neste artigo um plano de ensino que, envolvendo um trabalho interdisciplinar, discuta a natureza do Sistema de Unidades de Medida. Por meio de dinâmicas de grupos, leitura e interpretação de textos históricos, poemas e ilustrações e também através de outras fontes, acreditamos ser possível mostrar que o sistema de unidades de medida adotado atualmente (SI não é um dado natural, mas o resultado de um processo histórico de negociação de significados e, portanto, contingente das relações sociais. A partir da perspectiva dos Estudos Sociais da Ciência (ou Nova História e Sociologia do Conhecimento, apresentamos algumas discussões que envolveram a adoção do Sistema Decimal na França, bem como as dificuldades de sua posterior implementação no Brasil, expressa pela Revolta do Quebra-Quilos. Esperamos que as dinâmicas sugeridas neste trabalho possibilitem aos estudantes reconhecerem a si mesmos como participantes do processo de construção do conhecimento científico através da observação diária das mudanças que conferem novas feições a ele e também da tentativa de tornar mais significativo um tópico do currículo que, muitas vezes, é considerado desinteressante, enfadonho ou simples memorização de grandezas e de suas conversões.

  13. Medida del coeficiente d33 de piezocomposites por interferometría láser

    Directory of Open Access Journals (Sweden)

    Montero de Espinosa, F.

    2002-02-01

    Full Text Available The measurement of piezoelectric coefficient d33 is made using devices like the Berlincourt Meter ®, based on a force generator internally calibrated by a reference piezoelectric element which measures the charge ratio Culomb/Newton. For estructures such as piezoelectric composites, formed by materials of very different elastic properties, the measurements made by the described system present a great dispersión which depends on both the size of the pressing head and the aplied arm pressure. This work presents a set of systematic measurements of d33 for several piezocomposite geometries by means of optical interferometry. These measurements are compared with those obtained with the Berlincourt. It is observed that both techniques render closer results as the net step is reduced.La medida del coeficiente piezoeléctrico d33 se realiza utilizando equipos como el Berlincourt Meter ®, basados en un generador de fuerza calibrado internamente por un elemento piezoeléctrico de referencia que mide la relación de carga, Culombio/ Newton. Estos sistemas están absolutamente contrastados, tomando los grupos de investigación sus medidas como estándar. En el caso de estructuras tales como los composites piezoeléctricos, en los que la estructura está formada por materiales de muy distinta elasticidad, bien por este hecho, bien por la misma estructura, las medidas con el sistema descrito presentan una gran dispersión dependiendo del tamaño de la cabeza presionante y la presión del brazo. Dado que en el modelado de resonadores piezocomposite para su uso en aplicaciones con acoplamiento en aire es necesario conocer dicho parámetro sin incertidumbre, se presentan en el trabajo una serie de medidas sistemáticas de dicho coeficiente para varias geometrías de piezocomposites utilizando interferometría óptica. Se relaciona así mismo estas medidas con el resultado obtenido con el equipo estándar antes referido observando como cuanto más pequeño es

  14. Clustering in the stellar abundance space

    Science.gov (United States)

    Boesso, R.; Rocha-Pinto, H. J.

    2018-03-01

    We have studied the chemical enrichment history of the interstellar medium through an analysis of the n-dimensional stellar abundance space. This work is a non-parametric analysis of the stellar chemical abundance space. The main goal is to study the stars from their organization within this abundance space. Within this space, we seek to find clusters (in a statistical sense), that is, stars likely to share similar chemo-evolutionary history, using two methods: the hierarchical clustering and the principal component analysis. We analysed some selected abundance surveys available in the literature. For each sample, we labelled the group of stars according to its average abundance curve. In all samples, we identify the existence of a main enrichment pattern of the stars, which we call chemical enrichment flow. This flow is set by the structured and well-defined mean rate at which the abundances of the interstellar medium increase, resulting from the mixture of the material ejected from the stars and stellar mass-loss and interstellar medium gas. One of the main results of our analysis is the identification of subgroups of stars with peculiar chemistry. These stars are situated in regions outside of the enrichment flow in the abundance space. These peculiar stars show a mismatch in the enrichment rate of a few elements, such as Mg, Si, Sc and V, when compared to the mean enrichment rate of the other elements of the same stars. We believe that the existence of these groups of stars with peculiar chemistry may be related to the accretion of planetary material on to stellar surfaces or may be due to production of the same chemical element by different nucleosynthetic sites.

  15. Compact stellar object: the formation and structure

    Energy Technology Data Exchange (ETDEWEB)

    Duarte, S.B. [Centro Brasileiro de Pesquisas Fisicas (CBPF/MCT), Rio de Janeiro, RJ (Brazil)

    2012-07-01

    Full text: The formation of compact objects is viewed at the final stages of stellar evolution. The supernova explosion events are then focalized to explain the formation of pulsars, hybrid neutron star and the limit case of the latter, the quark stars. We discuss the stability and structure of these objects in connection with the properties of the hadron and quark-gluon plasma equation of state. The hadron-quark phase transition in deep interior of these objects is discussed taking into account the implications on the density distribution of matter along the radial direction. The role of neutrinos confinement in the ultradense stellar medium in the early stages of pulsar formation is another interesting aspect to be mentioned in this presentation. Recent results for maximum mass of compact stellar objects for different forms of equations of state will be shown, presenting some theoretical predictions for maximum mass of neutron stars allowed by different equations of state assigned to dense stellar medium. Although a density greater than few times the nuclear equilibrium density appears in deep interior of the core, at the crust the density decreases by several orders of magnitude where a variety of hadronic states appears, the 'pasta'-states of hadrons. More externally, a lattice of nuclei can be formed permeated not only by electrons but also by a large amount of free neutrons and protons. These are possible structure of neutron star crust to have the density and pressures with null values at the neutron star surface. The ultimate goal of this talk is to give a short view of the compact star area for students and those who are introducing in this subject. (author)

  16. Future prospects for stellar intensity interferometry

    International Nuclear Information System (INIS)

    Lake, R.J.W.

    2002-01-01

    Full text: The technique of Stellar Intensity lnterferometry (SII) was first successfully demonstrated by Hanbury-Brown in 1956 at Jodrell Bank. SII uses the correlation in intensity fluctuations of starlight as a function of observational baseline to determine angular diameters and other gross features of main sequence stars. In 1962 an observatory was established by Hanbury-Brown in Narrabri NSW. Between 1965 and 1972 the angular diameters of 32 stars covering the spectral range O to F were measured. Orbital parameters of several unresolved binary stars were also determined and attempts were made by the author to directly measure the limb darkening of Sirius and the rotational distortion of Altair. Following the success of the Narrabri SII the Australian Federal Government provided a grant to Sydney University to develop a Very Large SII capable of making observational measurements on about a thousand stars. The development of this VLSII was however shelved in preference to the development of a potentially more sensitive long baseline Michelson Stellar Interferometer. This latter instrument known as SUSI (Sydney University Stellar Interferometer) has been in operation at Narrabri since 1995. Encouraged by the early results of SUSI and their own efforts in the use of active optics to reduce the effects of atmospheric scintillation a number of international observatories are now active in the development of long baseline or large aperture Michelson Stellar Interferometers. However SII while sacrificing sensitivity has a number of technical advantages over MSI as SII is far less sensitive to atmospheric effects and can be readily developed to work over very long baselines. This paper through technical review and theoretical modeling examines how a modern VLSII could be constructed and operated and addresses the limitations to its sensitivity. In particular it examines how existing Australian industry could contribute to the development of a VLSII with sufficient

  17. Detection of stellar oscillations in HWVir

    Directory of Open Access Journals (Sweden)

    Baran Andrzej S.

    2016-08-01

    Full Text Available We present our analysis of K2 observations of the binary system, HWVir. We processed the raw Kepler data and used Fourier analysis to search for periodic signals that could be associated with pulsations. We detect the binary frequency and its harmonic and discovered tens of peaks at both low and high frequencies. We interpreted those to be caused by stellar pulsations. Our discovery means we can apply the tools of asteroseismology to the HWVir system.

  18. Stellarator approach to toroidal plasma confinement

    International Nuclear Information System (INIS)

    Johnson, J.L.

    1981-12-01

    An overview is presented of the development and current status of the stellarator approach to controlled thermonuclear confinement. Recent experimental, theoretical, and systems developments have made this concept a viable option for the evolution of the toroidal confinement program. Some experimental study of specific problems associated with departure from two-dimensional symmetry must be undertaken before the full advantages and opportunities of steady-state, net-current-free operation can be realized

  19. SMASH: Survey of the MAgellanic Stellar History

    Science.gov (United States)

    Nidever, David L.; Olsen, Knut; Walker, Alistair R.; Vivas, A. Katherina; Blum, Robert D.; Kaleida, Catherine; Choi, Yumi; Conn, Blair C.; Gruendl, Robert A.; Bell, Eric F.; Besla, Gurtina; Muñoz, Ricardo R.; Gallart, Carme; Martin, Nicolas F.; Olszewski, Edward W.; Saha, Abhijit; Monachesi, Antonela; Monelli, Matteo; de Boer, Thomas J. L.; Johnson, L. Clifton; Zaritsky, Dennis; Stringfellow, Guy S.; van der Marel, Roeland P.; Cioni, Maria-Rosa L.; Jin, Shoko; Majewski, Steven R.; Martinez-Delgado, David; Monteagudo, Lara; Noël, Noelia E. D.; Bernard, Edouard J.; Kunder, Andrea; Chu, You-Hua; Bell, Cameron P. M.; Santana, Felipe; Frechem, Joshua; Medina, Gustavo E.; Parkash, Vaishali; Serón Navarrete, J. C.; Hayes, Christian

    2017-11-01

    The Large and Small Magellanic Clouds are unique local laboratories for studying the formation and evolution of small galaxies in exquisite detail. The Survey of the MAgellanic Stellar History (SMASH) is an NOAO community Dark Energy Camera (DECam) survey of the Clouds mapping 480 deg2 (distributed over ˜2400 square degrees at ˜20% filling factor) to ˜24th mag in ugriz. The primary goals of SMASH are to identify low surface brightness stellar populations associated with the stellar halos and tidal debris of the Clouds, and to derive spatially resolved star formation histories. Here, we present a summary of the survey, its data reduction, and a description of the first public Data Release (DR1). The SMASH DECam data have been reduced with a combination of the NOAO Community Pipeline, the PHOTRED automated point-spread-function photometry pipeline, and custom calibration software. The astrometric precision is ˜15 mas and the accuracy is ˜2 mas with respect to the Gaia reference frame. The photometric precision is ˜0.5%-0.7% in griz and ˜1% in u with a calibration accuracy of ˜1.3% in all bands. The median 5σ point source depths in ugriz are 23.9, 24.8, 24.5, 24.2, and 23.5 mag. The SMASH data have already been used to discover the Hydra II Milky Way satellite, the SMASH 1 old globular cluster likely associated with the LMC, and extended stellar populations around the LMC out to R ˜ 18.4 kpc. SMASH DR1 contains measurements of ˜100 million objects distributed in 61 fields. A prototype version of the NOAO Data Lab provides data access and exploration tools.

  20. Rate of stellar collapses in the Galaxy

    International Nuclear Information System (INIS)

    Lande, K.; Stephens, W.E.

    1977-01-01

    From an analysis of pulsar spatial and luminosity distributions, the number density of observed pulsars in the local region is determined to be 1.1+-0.4x10 -7 pulsar pc -3 . Multiplication by the detection factor and by the ratio of Galaxy mass to local matter density and division by a mean lifetime of pulsars of 3x10 6 yr suggests a pulsar birth every 4 yr. A stellar collapse might occur even more often. (Auth.)

  1. SMASH: Survey of the MAgellanic Stellar History

    Energy Technology Data Exchange (ETDEWEB)

    Nidever, David L.; Olsen, Knut; Blum, Robert D.; Saha, Abhijit [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Walker, Alistair R.; Vivas, A. Katherina [Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena (Chile); Kaleida, Catherine [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Choi, Yumi; Besla, Gurtina; Olszewski, Edward W. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson AZ, 85721 (United States); Conn, Blair C. [Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611 (Australia); Gruendl, Robert A. [National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, IL 61801 (United States); Bell, Eric F. [Department of Astronomy, University of Michigan, 1085 S. University Avenue, Ann Arbor, MI 48109-1107 (United States); Muñoz, Ricardo R. [Departamento de Astronomía, Universidad de Chile, Camino del Observatorio 1515, Las Condes, Santiago (Chile); Gallart, Carme; Monelli, Matteo [Instituto de Astrofísica de Canarias, La Laguna, Tenerife (Spain); Martin, Nicolas F. [Université de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, F-67000 Strasbourg (France); Monachesi, Antonela [Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching (Germany); De Boer, Thomas J. L. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Johnson, L. Clifton, E-mail: dnidever@noao.edu [Center for Astrophysics and Space Sciences, UC San Diego, 9500 Gilman Drive, La Jolla, CA, 92093-0424 (United States); and others

    2017-11-01

    The Large and Small Magellanic Clouds are unique local laboratories for studying the formation and evolution of small galaxies in exquisite detail. The Survey of the MAgellanic Stellar History (SMASH) is an NOAO community Dark Energy Camera (DECam) survey of the Clouds mapping 480 deg{sup 2} (distributed over ∼2400 square degrees at ∼20% filling factor) to ∼24th mag in ugriz . The primary goals of SMASH are to identify low surface brightness stellar populations associated with the stellar halos and tidal debris of the Clouds, and to derive spatially resolved star formation histories. Here, we present a summary of the survey, its data reduction, and a description of the first public Data Release (DR1). The SMASH DECam data have been reduced with a combination of the NOAO Community Pipeline, the PHOTRED automated point-spread-function photometry pipeline, and custom calibration software. The astrometric precision is ∼15 mas and the accuracy is ∼2 mas with respect to the Gaia reference frame. The photometric precision is ∼0.5%–0.7% in griz and ∼1% in u with a calibration accuracy of ∼1.3% in all bands. The median 5 σ point source depths in ugriz are 23.9, 24.8, 24.5, 24.2, and 23.5 mag. The SMASH data have already been used to discover the Hydra II Milky Way satellite, the SMASH 1 old globular cluster likely associated with the LMC, and extended stellar populations around the LMC out to R  ∼ 18.4 kpc. SMASH DR1 contains measurements of ∼100 million objects distributed in 61 fields. A prototype version of the NOAO Data Lab provides data access and exploration tools.

  2. AFRONTAMIENTO FAMILIAR ANTE LA PRIMERA CRISIS DEL PACIENTE PSIQUIATRICO DEL HOSPITAL MENTAL RUDESINDO SOTO EN EL SEGUNDO SEMESTRE DE 2004

    Directory of Open Access Journals (Sweden)

    Luz Paola Morales-Contreras

    2005-12-01

    Full Text Available Con el propósito de determinar el grado de afrontamiento de la familia del paciente psiquiátrico ante el padecimiento de sus primeras crisis que asisten al Hospital Mental Rudesindo Soto de Cúcuta Norte de Santander, se desarrollo el presente estudio de tipo cuantitativo, descriptivo y de corte transversal. La población de estudio estuvo constituida por 40 cuidadores primarios de los pacientes con primera crisis que ingresaron al Hospital Mental Rudesindo Soto durante el periodo comprendido entre Julio y Octubre de 2004 residentes en Ia ciudad de acutal y su área metropolitana, caracterizados de acuerdo al sexo, edad, parentesco, ocupación y escolaridad, a quienes se aplico el instrumento F-COPES "Escala de Evaluación personal del funcionamiento familiar en situación de crisis", para determinar Ia utilización de los mecanismos de afrontamiento y mecanismo de defensa así como la Búsqueda de redes de apoyo social. De acuerdo al afrontamiento familiar el cuidador primario algunas veces busca redes de apoyo, casi nunca utiliza los mecanismos de defensa y los mecanismos de afrontamiento son utilizados algunas veces. Se concluye principalmente que el grado de afrontamiento de Ia familia del paciente psiquiátrico en su primera crisis es desfavorable.

  3. Stellar Atmospheric Modelling for the ACCESS Program

    Science.gov (United States)

    Morris, Matthew; Kaiser, Mary Elizabeth; Bohlin, Ralph; Kurucz, Robert; ACCESS Team

    2018-01-01

    A goal of the ACCESS program (Absolute Color Calibration Experiment for Standard Stars) is to enable greater discrimination between theoretical astrophysical models and observations, where the comparison is limited by systematic errors associated with the relative flux calibration of the targets. To achieve these goals, ACCESS has been designed as a sub-orbital rocket borne payload and ground calibration program, to establish absolute flux calibration of stellar targets at flight candidates, as well as a selection of A and G stars from the CALSPEC database. Stellar atmosphere models were generated using Atlas 9 and Atlas 12 Kurucz stellar atmosphere software. The effective temperature, log(g), metallicity, and redenning were varied and the chi-squared statistic was minimized to obtain a best-fit model. A comparison of these models and the results from interpolation between grids of existing models will be presented. The impact of the flexibility of the Atlas 12 input parameters (e.g. solar metallicity fraction, abundances, microturbulent velocity) is being explored.

  4. The formation of stellar black holes

    Science.gov (United States)

    Mirabel, Félix

    2017-08-01

    It is believed that stellar black holes (BHs) can be formed in two different ways: Either a massive star collapses directly into a BH without a supernova (SN) explosion, or an explosion occurs in a proto-neutron star, but the energy is too low to completely unbind the stellar envelope, and a large fraction of it falls back onto the short-lived neutron star (NS), leading to the delayed formation of a BH. Theoretical models set progenitor masses for BH formation by implosion, namely, by complete or almost complete collapse, but observational evidences have been elusive. Here are reviewed the observational insights on BHs formed by implosion without large natal kicks from: (1) the kinematics in three dimensions of space of five Galactic BH X-ray binaries (BH-XRBs), (2) the diversity of optical and infrared observations of massive stars that collapse in the dark, with no luminous SN explosions, possibly leading to the formation of BHs, and (3) the sources of gravitational waves (GWs) produced by mergers of stellar BHs so far detected with LIGO. Multiple indications of BH formation without ejection of a significant amount of matter and with no natal kicks obtained from these different areas of observational astrophysics, and the recent observational confirmation of the expected dependence of BH formation on metallicity and redshift, are qualitatively consistent with the high merger rates of binary black holes (BBHs) inferred from the first detections with LIGO.

  5. The Resolved Stellar Population of Leo A

    Science.gov (United States)

    Tolstoy, Eline

    1996-05-01

    New observations of the resolved stellar population of the extremely metal-poor Magellanic dwarf irregular galaxy Leo A in Thuan-Gunn r, g, i, and narrowband Hα filters are presented. Using the recent Cepheid variable star distance determination to Leo A by Hoessel et al., we are able to create an accurate color-magnitude diagram (CMD). We have used the Bavesian inference method described by Tolstoy & Saha to calculate the likelihood of a Monte Carlo simulation of the stellar population of Leo A being a good match to the data within the well understood errors in the data. The magnitude limits on our data are sensitive enough to look back at ~1 Gyr of star formation history at the distance of Leo A. To explain the observed ratio of red to blue stars in the observed CMD, it is necessary to invoke either a steadily decreasing star formation rate toward the present time or gaps in the star formation history. We also compare the properties of the observed stellar population with the known spatial distribution of the H I gas and H II regions to support the conclusions from CMD modeling. We consider the possibility that currently there is a period of diminished star formation in Leo A, as evidenced by the lack of very young stars in the CMD and the faint H II regions. How the chaotic H I distribution, with no observable rotation, fits into our picture of the evolution of Leo A is as yet unclear.

  6. The doubling of stellar black hole nuclei

    Science.gov (United States)

    Kazandjian, Mher V.; Touma, J. R.

    2013-04-01

    It is strongly believed that Andromeda's double nucleus signals a disc of stars revolving around its central supermassive black hole on eccentric Keplerian orbits with nearly aligned apsides. A self-consistent stellar dynamical origin for such apparently long-lived alignment has so far been lacking, with indications that cluster self-gravity is capable of sustaining such lopsided configurations if and when stimulated by external perturbations. Here, we present results of N-body simulations which show unstable counter-rotating stellar clusters around supermassive black holes saturating into uniformly precessing lopsided nuclei. The double nucleus in our featured experiment decomposes naturally into a thick eccentric disc of apo-apse aligned stars which is embedded in a lighter triaxial cluster. The eccentric disc reproduces key features of Keplerian disc models of Andromeda's double nucleus; the triaxial cluster has a distinctive kinematic signature which is evident in Hubble Space Telescope observations of Andromeda's double nucleus, and has been difficult to reproduce with Keplerian discs alone. Our simulations demonstrate how the combination of an eccentric disc and a triaxial cluster arises naturally when a star cluster accreted over a preexisting and counter-rotating disc of stars drives disc and cluster into a mutually destabilizing dance. Such accretion events are inherent to standard galaxy formation scenarios. They are here shown to double stellar black hole nuclei as they feed them.

  7. Intrinsic Turbulence Stabilization in a Stellarator

    Directory of Open Access Journals (Sweden)

    P. Xanthopoulos

    2016-06-01

    Full Text Available The magnetic surfaces of modern stellarators are characterized by complex, carefully optimized shaping and exhibit locally compressed regions of strong turbulence drive. Massively parallel computer simulations of plasma turbulence reveal, however, that stellarators also possess two intrinsic mechanisms to mitigate the effect of this drive. In the regime where the length scale of the turbulence is very small compared to the equilibrium scale set by the variation of the magnetic field, the strongest fluctuations form narrow bandlike structures on the magnetic surfaces. Thanks to this localization, the average transport through the surface is significantly smaller than that predicted at locations of peak turbulence. This feature results in a numerically observed upshift of the onset of turbulence on the surface towards higher ion temperature gradients as compared with the prediction from the most unstable regions. In a second regime lacking scale separation, the localization is lost and the fluctuations spread out on the magnetic surface. Nonetheless, stabilization persists through the suppression of the large eddies (relative to the equilibrium scale, leading to a reduced stiffness for the heat flux dependence on the ion temperature gradient. These fundamental differences with tokamak turbulence are exemplified for the QUASAR stellarator [G. H. Neilson et al., IEEE Trans. Plasma Sci. 42, 489 (2014].

  8. Solar and Stellar X-ray Cycles

    Science.gov (United States)

    Martens, P. C. H.; SADE Team

    2004-05-01

    Stern et al. have shown that Yohkoh-SXT full disk X-ray irradiance shows an 11 year cycle with an max/min amplitude ratio of a factor 30. Similar cyclic X-ray variation in Sun-like stars observed by ROSAT and its predecessors is observed in only a few cases and limited to a factor two or three. We will show, by means of detailed bandpass comparisons, that this discrepancy cannot be ascribed to the differences in energy response between SXT and the stellar soft X-ray detectors. Is the Sun exceptional? After centuries of geocentric and heliocentric worldviews we find this a difficult proposition to entertain. But perhaps the Sun is a member of a small class of late-type stars with large amplitudes in their X-ray cycles. The stellar X-ray observations listed in the HEASARC catalog are too sparse to verify this hypothesis. To resolve these and related questions we have proposed a small low-cost stellar X-ray spectroscopic imager originally called SADE to obtain regular time series from late and early-type stars and accretion disks. This instrument is complimentary to the much more advanced Chandra and XMM-Newton observatories, and allows them to focus on those sources that require their full spatial and spectral resolution. We will describe the basic design and spectroscopic capability of SADE and show it meets the mission requirements.

  9. STELLAR: fast and exact local alignments

    Directory of Open Access Journals (Sweden)

    Weese David

    2011-10-01

    Full Text Available Abstract Background Large-scale comparison of genomic sequences requires reliable tools for the search of local alignments. Practical local aligners are in general fast, but heuristic, and hence sometimes miss significant matches. Results We present here the local pairwise aligner STELLAR that has full sensitivity for ε-alignments, i.e. guarantees to report all local alignments of a given minimal length and maximal error rate. The aligner is composed of two steps, filtering and verification. We apply the SWIFT algorithm for lossless filtering, and have developed a new verification strategy that we prove to be exact. Our results on simulated and real genomic data confirm and quantify the conjecture that heuristic tools like BLAST or BLAT miss a large percentage of significant local alignments. Conclusions STELLAR is very practical and fast on very long sequences which makes it a suitable new tool for finding local alignments between genomic sequences under the edit distance model. Binaries are freely available for Linux, Windows, and Mac OS X at http://www.seqan.de/projects/stellar. The source code is freely distributed with the SeqAn C++ library version 1.3 and later at http://www.seqan.de.

  10. Plasma equilibrium and stability in stellarators

    International Nuclear Information System (INIS)

    Pustovitov, V.D.; Shafranov, V.D.

    1987-01-01

    A review of theoretical methods of investigating plasma equilibrium and stability in stellarators is given. Principles forming the basis of toroidal plasma equilibrium and its stabilization, and the main results of analytical theory and numerical calculations are presented. Configurations with spiral symmetry and usual stellarators with plane axis and spiral fields are considered in detail. Derivation of scalar two-dimensional equations, describing equilibrium in these systems is given. These equations were used to obtain one-dimensional equations for displacement and ellipticity of magnetic surfaces. The model of weak-elliptic displaced surfaces was used to consider the evolution of plasma equilibrium in stellarators after elevation of its pressure: change of profile of rotational transformation after change of plasma pressure, current generation during its fast heating and its successive damping due to finite plasma conductivity were described. The derivation of equations of small oscillations in the form, suitable for local disturbance investigation is presented. These equations were used to obtain Mercier criteria and ballon model equations. General sufficient conditions of plasma stability in systems with magnetic confinement were derived

  11. Ripple transport in helical-axis advanced stellarators - a comparison with classical stellarator/torsatrons

    International Nuclear Information System (INIS)

    Beidler, C.D.; Hitchon, W.N.G.

    1993-08-01

    Calculations of the neoclassical transport rates due to particles trapped in the helical ripples of a stellarator's magnetic field are carried out, based on solutions of the bounce-averaged kinetic equation. These calculations employ a model for the magnetic field strength, B, which is an accurate approximation to the actual B for a wide variety of stellarator-type devices, among which are Helical-Axis Advanced Stellarators (Helias) as well as conventional stellarators and torsatrons. Comparisons are carried out in which it is shown that the Helias concept leads to significant reductions in neoclassical transport rates throughout the entire long-mean-free-path regime, with the reduction being particularly dramatic in the ν -1 regime. These findings are confirmed by numerical simulations. Further, it is shown that the behavior of deeply trapped particles in Helias can be fundamentally different from that in classical stellarator/torsatrons; as a consequence, the beneficial effects of a radial electric field on the transport make themselves felt at lower collision frequency than is usual. (orig.)

  12. BOOK REVIEW: Stellarator and Heliotron Devices

    Science.gov (United States)

    Johnson, John L.

    1999-02-01

    Stellarators and tokamaks are the most advanced devices that have been developed for magnetic fusion applications. The two approaches have much in common; tokamaks have received the most attention because their axisymmetry justifies the use of simpler models and provides a more forgiving geometry. However, recent advances in treating more complicated three dimensional systems have made it possible to design stellarators that are not susceptible to disruptions and do not need plasma current control. This has excited interest recently. The two largest new magnetic experiments in the world are the LHD device, which commenced operation in Toki, Japan, in 1998 and W7-X, which should become operational in Greifswald, Germany, in 2004. Other recently commissioned stellarators, including H-1 in Canberra, Australia, TJ-II in Madrid, Spain, and IMS in Madison, Wisconsin, have joined these in rejuvenating the stellarator programme. Thus, it is most appropriate that the author has made the lecture material that he presents to his students in the Graduate School of Energy Science at Kyoto University available to everyone. Stellarator and Heliotron Devices provides an excellent treatment of stellarator theory. It is aimed at graduate students who have a good understanding of classical mechanics and mathematical techniques. It contains good descriptions and derivations of essentially every aspect of fusion theory. The author provides an excellent qualitative introduction to each subject, pointing out the strengths and weaknesses of the models that are being used and describing our present understanding. He judiciously uses simple models which illustrate the similarities and differences between stellarators and tokamaks. To some extent the treatment is uneven, rigorous derivations starting with basic principles being given in some cases and relations and equations taken from the original papers being used as a starting point in others. This technique provides an excellent training

  13. Características clínicas de los pacientes diabéticos que acuden por primera vez a una consulta nefrológica en hospitales públicos de Lima

    Directory of Open Access Journals (Sweden)

    Percy Herrera Añazco

    2014-01-01

    Full Text Available Introducción: La diabetes mellitus es la principal causa de enfermedad renal crónica y se recomienda una referencia temprana al nefrólogo, ya que se ha reportado peores resultados en pacientes con referencia tardía. Objetivos: Determinar las características de los pacientes diabéticos en su primera consulta nefrológica. Diseño: Estudio multicéntrico, observacional y analítico. Lugar: Hospital Nacional 2 de Mayo, Hospital Nacional Arzobispo Loayza, Hospital Daniel Alcides Carrión y Hospital María Auxiliadora. Participantes: Pacientes diabéticos. Intervenciones: Se estudió a los pacientes en su primera consulta nefrológica entre septiembre 2011 y febrero 2012. Para la descripción se utilizó porcentajes, frecuencias y desviaciones estándar. Principales medidas de resultados: Características clínicas de los pacientes diabéticos. Resultados: Se estudió 200 pacientes diabéticos, con tiempo de diagnóstico promedio de 12,9 años. El 73% recibió educación para autocuidados. El 40% refería que no tomaba sus medicamentos y 57% no seguía su dieta regularmente. El 70% era hipertenso con tiempo de diagnóstico promedio de 4,2 años; 36,5% era obeso, 52,8% sufría de dislipidemia, 10,5% tenía antecedente de enfermedad cardiovascular. El 81,5% refería no haber tenido una evaluación previa de la función renal. El 39,5% tenía hemoglobina glicosilada (HbA1c >7%, 48,5% colesterol >200 mg/dL, 54,5% cLDL>100 mg/dL y 46,5% triglicéridos >150 mg/dL; 57% un tiempo de filtración glomerular<60 mL/min y 37% presentó albuminuria de 300 mg/d o más. Conclusiones: Casi la mitad de los pacientes no seguía las recomendaciones de autocuidados. Debido a los factores de riesgo cardiovascular involucrados en este grupo, se debería reforzar su educación.

  14. The Stellar Imager (SI) Project: Resolving Stellar Surfaces, Interiors, and Magnetic Activity

    Science.gov (United States)

    Carpenter, Kenneth G.; Schrijver, K.; Karovska, M.

    2007-01-01

    The Stellar Imager (SI) is a UV/Optical. Space-Based Interferometer designed to enable 0.1 milli-arcsec (mas) spectral imaging of stellar surfaces and, via asteroseismology, stellar interiors and of the Universe in general. The ultra-sharp images of SI will revolutionize our view of many dynamic astrophysical processes by transforming point sources into extended sources, and snapshots into evolving views. The science of SI focuses on the role of magnetism in the Universe, particularly on magnetic activity on the surfaces of stars like the Sun. Its prime goal is to enable long-term forecasting of solar activity and the space weather that it drives. SI will also revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. In this paper we discuss the science goals, technology needs, and baseline design of the SI mission.

  15. Estimating precise metallicity and stellar mass evolution of galaxies

    Science.gov (United States)

    Mosby, Gregory

    2018-01-01

    The evolution of galaxies can be conveniently broken down into the evolution of their contents. The changing dust, gas, and stellar content in addition to the changing dark matter potential and periodic feedback from a super-massive blackhole are some of the key ingredients. We focus on the stellar content that can be observed, as the stars reflect information about the galaxy when they were formed. We approximate the stellar content and star formation histories of unresolved galaxies using stellar population modeling. Though simplistic, this approach allows us to reconstruct the star formation histories of galaxies that can be used to test models of galaxy formation and evolution. These models, however, suffer from degeneracies at large lookback times (t > 1 Gyr) as red, low luminosity stars begin to dominate a galaxy’s spectrum. Additionally, degeneracies between stellar populations at different ages and metallicities often make stellar population modeling less precise. The machine learning technique diffusion k-means has been shown to increase the precision in stellar population modeling using a mono-metallicity basis set. However, as galaxies evolve, we expect the metallicity of stellar populations to vary. We use diffusion k-means to generate a multi-metallicity basis set to estimate the stellar mass and chemical evolution of unresolved galaxies. Two basis sets are formed from the Bruzual & Charlot 2003 and MILES stellar population models. We then compare the accuracy and precision of these models in recovering complete (stellar mass and metallicity) histories of mock data. Similarities in the groupings of stellar population spectra in the diffusion maps for each metallicity hint at fundamental age transitions common to both basis sets that can be used to identify stellar populations in a given age range.

  16. Habitability in different Milky Way stellar environments: a stellar interaction dynamical approach.

    Science.gov (United States)

    Jiménez-Torres, Juan J; Pichardo, Bárbara; Lake, George; Segura, Antígona

    2013-05-01

    Every Galactic environment is characterized by a stellar density and a velocity dispersion. With this information from literature, we simulated flyby encounters for several Galactic regions, numerically calculating stellar trajectories as well as orbits for particles in disks; our aim was to understand the effect of typical stellar flybys on planetary (debris) disks in the Milky Way Galaxy. For the solar neighborhood, we examined nearby stars with known distance, proper motions, and radial velocities. We found occurrence of a disturbing impact to the solar planetary disk within the next 8 Myr to be highly unlikely; perturbations to the Oort cloud seem unlikely as well. Current knowledge of the full phase space of stars in the solar neighborhood, however, is rather poor; thus we cannot rule out the existence of a star that is more likely to approach than those for which we have complete kinematic information. We studied the effect of stellar encounters on planetary orbits within the habitable zones of stars in more crowded stellar environments, such as stellar clusters. We found that in open clusters habitable zones are not readily disrupted; this is true if they evaporate in less than 10(8) yr. For older clusters the results may not be the same. We specifically studied the case of Messier 67, one of the oldest open clusters known, and show the effect of this environment on debris disks. We also considered the conditions in globular clusters, the Galactic nucleus, and the Galactic bulge-bar. We calculated the probability of whether Oort clouds exist in these Galactic environments.

  17. Stellarator Research Opportunities: A report of the National Stellarator Coordinating Committee

    Energy Technology Data Exchange (ETDEWEB)

    Gates, David A. [Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Anderson, David [University of Wisconsin-Madison

    2017-06-01

    This document is the product of a stellarator community workshop, organized by the National Stellarator Coordinating Committee and referred to as Stellcon, that was held in Cambridge, Massachusetts in February 2016, hosted by MIT. The workshop was widely advertised, and was attended by 40 scientists from 12 different institutions including national labs, universities and private industry, as well as a representative from the Department of Energy. The final section of this document describes areas of community wide consensus that were developed as a result of the discussions held at that workshop. Areas where further study would be helpful to generate a consensus path forward for the US stellarator program are also discussed. The program outlined in this document is directly responsive to many of the strategic priorities of FES as articulated in “Fusion Energy Sciences: A Ten-Year Perspective (2015-2025)” [2]. The natural disruption immunity of the stellarator directly addresses “Elimination of transient events that can be deleterious to toroidal fusion plasma confinement devices” an area of critical importance for the U.S. fusion energy sciences enterprise over the next decade. Another critical area of research “Strengthening our partnerships with international research facilities,” is being significantly advanced on the W7-X stellarator in Germany and serves as a test-bed for development of successful international collaboration on ITER. This report also outlines how materials science as it relates to plasma and fusion sciences, another critical research area, can be carried out effectively in a stellarator. Additionally, significant advances along two of the Research Directions outlined in the report; “Burning Plasma Science: Foundations - Next-generation research capabilities”, and “Burning Plasma Science: Long pulse - Sustainment of Long-Pulse Plasma Equilibria” are proposed.

  18. Stellarator Research Opportunities: A Report of the National Stellarator Coordinating Committee

    Science.gov (United States)

    Gates, D. A.; Anderson, D.; Anderson, S.; Zarnstorff, M.; Spong, D. A.; Weitzner, H.; Neilson, G. H.; Ruzic, D.; Andruczyk, D.; Harris, J. H.; Mynick, H.; Hegna, C. C.; Schmitz, O.; Talmadge, J. N.; Curreli, D.; Maurer, D.; Boozer, A. H.; Knowlton, S.; Allain, J. P.; Ennis, D.; Wurden, G.; Reiman, A.; Lore, J. D.; Landreman, M.; Freidberg, J. P.; Hudson, S. R.; Porkolab, M.; Demers, D.; Terry, J.; Edlund, E.; Lazerson, S. A.; Pablant, N.; Fonck, R.; Volpe, F.; Canik, J.; Granetz, R.; Ware, A.; Hanson, J. D.; Kumar, S.; Deng, C.; Likin, K.; Cerfon, A.; Ram, A.; Hassam, A.; Prager, S.; Paz-Soldan, C.; Pueschel, M. J.; Joseph, I.; Glasser, A. H.

    2018-02-01

    This document is the product of a stellarator community workshop, organized by the National Stellarator Coordinating Committee and referred to as Stellcon, that was held in Cambridge, Massachusetts in February 2016, hosted by MIT. The workshop was widely advertised, and was attended by 40 scientists from 12 different institutions including national labs, universities and private industry, as well as a representative from the Department of Energy. The final section of this document describes areas of community wide consensus that were developed as a result of the discussions held at that workshop. Areas where further study would be helpful to generate a consensus path forward for the US stellarator program are also discussed. The program outlined in this document is directly responsive to many of the strategic priorities of FES as articulated in "Fusion Energy Sciences: A Ten-Year Perspective (2015-2025)" [1]. The natural disruption immunity of the stellarator directly addresses "Elimination of transient events that can be deleterious to toroidal fusion plasma confinement devices" an area of critical importance for the US fusion energy sciences enterprise over the next decade. Another critical area of research "Strengthening our partnerships with international research facilities," is being significantly advanced on the W7-X stellarator in Germany and serves as a test-bed for development of successful international collaboration on ITER. This report also outlines how materials science as it relates to plasma and fusion sciences, another critical research area, can be carried out effectively in a stellarator. Additionally, significant advances along two of the Research Directions outlined in the report; "Burning Plasma Science: Foundations - Next-generation research capabilities", and "Burning Plasma Science: Long pulse - Sustainment of Long-Pulse Plasma Equilibria" are proposed.

  19. Constraining stellar physics from red-giant stars in binaries – stellar rotation, mixing processes and stellar activity

    Directory of Open Access Journals (Sweden)

    Beck P. G.

    2017-01-01

    Full Text Available The unparalleled photometric data obtained by NASA’s Kepler Space Telescope has led to an improved understanding of stellar structure and evolution - in particular for solar-like oscillators in this context. Binary stars are fascinating objects. Because they were formed together, binary systems provide a set of two stars with very well constrained parameters. Those can be used to study properties and physical processes, such as the stellar rotation, dynamics and rotational mixing of elements and allows us to learn from the differences we find between the two components. In this work, we discussed a detailed study of the binary system KIC 9163796, discovered through Kepler photometry. The ground-based follow-up spectroscopy showed that this system is a double-lined spectroscopic binary, with a mass ratio close to unity. However, the fundamental parameters of the components of this system as well as their lithium abundances differ substantially. Kepler photometry of this system allows to perform a detailed seismic analysis as well as to derive the orbital period and the surface rotation rate of the primary component of the system. Indications of the seismic signature of the secondary are found. The differing parameters are best explained with both components located in the early and the late phase of the first dredge up at the bottom of the red-giant branch. Observed lithium abundances in both components are in good agreement with prediction of stellar models including rotational mixing. By combining observations and theory, a comprehensive picture of the system can be drawn.

  20. La importancia de llamarse afinidad química. Parte IV: Las primeras flores

    Directory of Open Access Journals (Sweden)

    Guillermo Salas-Banuet

    2014-01-01

    Full Text Available El vacío de poder producido por el derrumbe del Imperio Romano dejó a la Europa Medieval sumida en un ambiente de luchas. La dominante Iglesia Cristiana de Roma batalló para extenderse y someter a reyes y emperadores. La autoridad del papa Cristiano de Roma realizó un esfuerzo para esclavizar al pensamiento de los creyentes religiosos a la cerrada perspectiva religiosa que se tenía en esas épocas. Sin embargo, fue desde el seno mismo de los fieles de donde surgió la necesidad de ver a la naturaleza y sus leyes de otra manera. El descubrimiento, traducción y difusión de los textos de los pensadores griegos clásicos, permitió iniciar el proceso de independencia del pensamiento europeo, lo que llevó al surgimiento del Renacimiento y la Ilustración. Fue entonces cuando comenzó a utilizase el método inductivo en el afán de encontrar otras maneras de interpretar a la naturaleza y avanzar en el conocimiento. Así, durante el siglo XVI la alquimia fue cuestionada y aparecieron los primeros escritos de una metalurgia empírica, considerados la base de la ciencia moderna; durante el XVII, aún con la existencia de conceptos alquímicos residuales, algunos personajes comenzaron a realizar experimentos, con lo que se establecieron las primeras hipótesis sobre los conceptos y fenómenos químicos clave, los cuales sirvieron de sustento para desarrollar al pensamiento lógico y racional del siglo XVIII, como el relativo a las afinidades, que se basaba en las relaciones entre las sustancias, observadas durante la formación de compuestos y como una analogía de las relaciones humanas. Los trabajos publicados entonces sobre los elementos del proceso del pensamiento, permitieron consolidar los conceptos base relativos al enlace y otros a él relacionados.

  1. El recuerdo de la Primera Guerra Mundial en los antiguos territorios del imperio austrohúngaro

    Directory of Open Access Journals (Sweden)

    Christopher Brennan

    2015-02-01

    Full Text Available En el imperio austrohúngaro inevitablemente emergió una experiencia colectiva de la Gran Guerra. Sin embargo, la disolución repentina del imperio de los Habsburgo y las hostilidades inmediatas entre sus estados sucesores implicaron que nunca se llegó a establecer y cultivar una memoria colectiva. Para cada país, la guerra y sus consecuencias adquirieron sus propias interpretaciones: independencia en el caso de Polonia y Checoslovaquia (ahora la República Checa y Eslovaquia; unión con los compañeros eslavos del Sur para Eslovenia; amargura y resentimiento para Hungría; y traición y confusión para Austria. La mayor parte de estos países se ha reconciliado con la guerra y sus consecuencias (y algunos con su papel en el imperio de los Habsburgo pero otros, sobre todo Hungría, todavía albergan un rencor tan vivo como era cuando su reinado milenario se fracturó (ya hace noventaicinco años. Las vicisitudes del siglo veinte (junto a la apocalíptica Segunda Guerra Mundial y las décadas de Comunismo refrenaron durante mucho tiempo un análisis serio y crítico de la Primera Guerra Mundial. Pero aunque nunca habrá una conciencia colectiva del conflicto entre las gentes que constituyeron el imperio de los Habsburgo, la calidad en aumento de la reciente historiografía sobre el conflicto junto al desvanecimiento de las disputas territoriales y las tensiones nacionales, con tiempo ayudarán a reconstituir la experiencia colectiva del esfuerzo bélico notablemente tenaz del imperio austrohúngaro, del que sus fuerzas imperiales mostraron su unidad y determinación en varios campos de batalla espantosos.

  2. Primera Jornada de Actualización en Patología Oral y Maxilofacial

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    Claudia Patricia Peña Vega

    2017-01-01

    Full Text Available Dedicamos las Lecturas recobradas a las memorias de la “Primera Jornada de Actualización en Patología Oral Y Maxilofacial” de las Facultades de Odontología y Medicina de la Universidad Nacional de Colombia, realizado en septiembre 30 al 01 de octubre del año 2016, bajo la coordinación de la profesora asociada del Departamento de Salud Oral de la universidad Nacional de Colombia, Claudia Patricia Peña Vega. El objetivo general del encuentro fue realizar una jornada académica integral de actualización en el campo de la Patología Oral y Maxilofacial dirigida a los estudiantes, residentes, egresados, profesores, y profesionales odontólogos, médicos, de las diferentes especialidades de interés en el área de la Patología General y Oral que fortalezcan la interdisciplinariedad del diagnóstico en un contexto clínico, académico e investigativo. Con el propósito de actualizar a los odontólogos y médicos en el estado del arte, avances tecnológicos y científicos en los diferentes campos de la Patología Oral y Maxilofacial, fortaleciendo académica y científicamente el campo de la Patología Oral y Maxilofacial, enmarcado como ámbito importante del conocimiento de la Patología General. Proporciona y difunde el Servicio de diagnóstico histopatológico en la Facultad de Odontología de la Universidad Nacional de Colombia. Todo esto, con el objetivo de crear un espacio académico para la presentación de casos clínicos y discusión de temas de interés, con la participación de diferentes expertos Patólogos de diferentes instituciones y creando nexos y vínculos académicos, hospitalarios y científicos con el Departamento de Patología de la Universidad Nacional de Colombia y la Sección Académica de Patología de la Faculta de Odontología de la Universidad Nacional de Colombia.

  3. La itinerancia de la corte de Castilla durante la primera mitad del siglo XV

    Directory of Open Access Journals (Sweden)

    Francisco de Paula CAÑAS GÁLVEZ

    2009-01-01

    Full Text Available El presente trabajo intentará explicar las diferentes causas que hicieron del centro de la meseta el núcleo político y burocrático de la Corona de Castilla y León a finales de la Edad Media. Aquel espacio geográfico, comprendido en sus líneas generales entre Burgos y Toledo, concentró, efectivamente, una parte muy significativa de la actividad política e institucional de la Monarquía en un periodo de especial relevancia en la formación del Estado Moderno en tierras castellanas. Este largo proceso, si bien pergeñado durante los siglos XIII y primera mitad del XIV, únicamente se consolidaría tras la llegada al trono castellano de la nueva dinastía Trastámara, en especial durante los reinados de Enrique III y Juan II, alcanzando su madurez plena en tiempos de los Habsburgo con el asentamiento de la hasta entonces corte itinerante, y de buena parte de su aparato burocrático, en Madrid.Ce travail vise à expliquer les différentes causes qui ont fait du centre de la Meseta le noyau politique et administratif de la couronne de Castille et León. Cet espace géographique, compris grosso modo entre Burgos et Tolède a  effectivement concentré une part importante de la vie politique et institutionnelle de la monarchie à une période cruciale pour la formation de l’État moderne en terre castillane. Ce vaste processus, esquissé au cours du XIIIe siècle et de la première moitié du XIVe siècle, ne s’est consolidé qu’avec l’avènement de la nouvelle dynastie Trastamare, en particulier pendant les règnes d’Henri III et de Jean II, pour atteindre sa pleine maturité au temps des Habsbourg, avec la sédentarisation à Madrid de la cour jusque-là itinérante et d’une  bonne partie de l’appareil bureaucratique.

  4. The Effects of Stellar Dynamics on the Evolution of Young, Dense Stellar Systems

    Science.gov (United States)

    Belkus, H.; van Bever, J.; Vanbeveren, D.

    In this paper, we report on first results of a project in Brussels in which we study the effects of stellar dynamics on the evolution of young dense stellar systems using 3 decades of expertise in massive-star evolution and our population (number and spectral) synthesis code. We highlight an unconventionally formed object scenario (UFO-scenario) for Wolf Rayet binaries and study the effects of a luminous blue variable-type instability wind mass-loss formalism on the formation of intermediate-mass black holes.

  5. Medidas directas e indirectas de las funciones ejecutivas en niños con trastorno de espectro autista

    Directory of Open Access Journals (Sweden)

    María Fernanda Pérez Pichardo

    2018-01-01

    Full Text Available INTRODUCCIÓN: los niños con trastorno del espectro autista (TEA tienen dificultades en las funciones ejecutivas (FE pero se han sugerido discrepancias entre las medidas directas e indirectas.   OBJETIVO: conocer si existen diferencias en las funciones ejecutivas mediante medidas directas e indirectas entre niños con y sin TEA.   MÉTODO: se incluyeron 14 varones entre primero y tercero de primaria, 50% con diagnóstico de TEA y 50% con desarrollo neurotípico, seleccionados por emparejamiento en edad y grado escolar. El promedio de edad de la muestra fue de 7.43 (DE 0.98 años. Se aplicaron las pruebas de Evaluación neuropsicológica de funciones ejecutivas en niños (ENFEN y el Inventario de clasificación comportamental de las funciones ejecutivas (BRIEF.   RESULTADOS: se encontraron diferencias significativas en las medidas de las FE indirectas, pero no en las directas, entre los grupos (p < 0.05. Así mismo, las correlaciones entre las medidas directas e indirectas fueron mayores en el grupo con TEA.   CONCLUSIONES: los niños con TEA son evaluados con más dificultades en las medidas indirectas de las funciones ejecutivas, pero obtienen puntuaciones similares a los niños con desarrollo neurotípico cuando son evaluados en condiciones estructuradas empleando medidas directas.

  6. Confiabilidade da medida de espessuras musculares pela ultrassonografia Reliability of muscle thickness measurements using ultrasound

    Directory of Open Access Journals (Sweden)

    Paulo Sergio Chagas Gomes

    2010-02-01

    Full Text Available OBJETIVO: Determinar a confiabilidade das medidas de espessuras dos músculos flexores e extensores do cotovelo e joelho pela ultrassonografia (US, quantificando o erro típico associado a essas medidas (ETM. MÉTODOS: A confiabilidade (duas medidas interdias foi determinada em 15 voluntários aparentemente saudáveis (oito mulheres, 33,9 ± 11,4 anos, 76 ± 21kg, 170 ± 10cm. As imagens da musculatura flexora (FC e extensora do cotovelo (EC e flexora (FJ e extensora do joelho (EJ foram obtidas pela US bidimensional no modo B, utilizando transdutor de 7,5MHz. As espessuras do tecido muscular compreendidas entre as interfaces com o osso e com o tecido adiposo foram medidas em sítios anatômicos identificados e registrados para ser repetidos na segunda medida. RESULTADOS: A ANOVA não identificou diferenças significativas entre as medidas repetidas. Os coeficientes de correlação intraclasse foram FC = 0,970, EC = 0,971, FJ = 0,555 e EJ = 0,929 (P PURPOSE: To determine the reliability of muscle thickness measurements of elbow and knee flexors and extensors using ultrasound, and to quantify the typical error associated to the measurements (TEM. METHODS: The test-retest reliability was determined in 15 apparently healthy volunteers (8 women, 34 ± 11 years, 76 ± 21 kg, 170 ± 10 cm. The images of elbow flexors (EF and extensors (EE and knee flexors (KF and extensors (KE were obtained using a two dimensional mode B ultrasound instrument with a 7.5 MHz transducer. Muscle thickness between the adipose tissue and bone interfaces were measured at anatomical landmarks previously identified and recorded to assure the exact site for the retest. RESULTS: ANOVA did not identify any significant differences between the repeated measurements. Intraclass correlation coefficients (ICC of each pair of measure were EF = 0.970, EE = 0.971, KF = 0.555 e KE = 0.929 (P < 0.05 for all. The coefficients of variation were 3.9 %, 6.1 %, 6.6 % e 4.6 %, and TEM 1.3 mm, 1

  7. Medida de la dureza de sólidos mediante nanoindentación

    Directory of Open Access Journals (Sweden)

    Alkorta, J.

    2005-10-01

    Full Text Available Hardness is not readily measurable by means of instrumented indentation since the value of the contact area depends on the pile-up or sink-in occurring near the contact surface of the sample. The most widespread method to estimate it by means of the loading/unloading curve of indentation, Oliver and Pharr’s method, deviates, in the extreme cases, up to a 25% from the real values since it only takes into account the elastic deflection. In this work, a new correction based on Oliver and Pharr’s method is proposed that agrees with the numerical calculations. Plastic hardening behaviour of the sample must be known to accurately estimate the contact area.

    La medida de la dureza mediante indentación con registro de carga y desplazamiento no es evidente, dada la incertidumbre sobre el tamaño de huella debido al levantamiento (pile-up o hundimiento (sink-in plásticos de la superficie de la muestra alrededor del indentador. El método más utilizado para la medida de la dureza mediante la curva de carga/descarga de indentación, el de Oliver y Pharr, sólo tiene en cuenta hundimiento elástico, por lo que el error en la medida de la dureza y el módulo de Young puede llegar hasta un 25% en los casos más extremos. En el presente trabajo se discute una posible corrección al método de Oliver y Pharr para una obtención más ajustada del área de contacto de la huella. Esta corrección requiere de un conocimiento a priori o a posteriori del comportamiento plástico del material.

  8. Near-term directions in the World Stellarator Program

    International Nuclear Information System (INIS)

    Lyon, J.F.

    1990-01-01

    Interest in stellarators has increased because of the progress being made in the development of this concept and the inherent advantages of stellarators as candidates for an attractive, steady-state fusion reactor. Three new stellarator experiments started operation in 1988, and three more are scheduled to start in the next few years. In addition, design studies have started on large next-generation stellarator experiments for the mid-1990s. These devices are designed to test four basic approaches to stellarator configuration optimization. Ways in which these devices complement each other in exploring the potential of the stellarator concept and the main issues that they will address during the next decade are described

  9. Normatização de medidas acústicas da voz normal

    Directory of Open Access Journals (Sweden)

    Araújo Simone Adad

    2002-01-01

    Full Text Available Introdução: A análise acústica da voz com o avanço da tecnologia digital surge como um exame complementar promissor para aumentar a precisão diagnóstica em laringologia. Objetivo: Normatização das medidas acústicas de freqüência fundamental, perturbação e ruído na voz normal de brasileiros dos sexos masculino e feminino. Forma de estudo: Clínico prospectivo. Material e Método: Pesquisa no período de março a agosto de 1997, no Ambulatório de Otorrinolaringologia do Hospital das Clínicas da Faculdade de Medicina de Ribeirão Preto da Universidade de São Paulo, com 80 voluntários da cidade de Ribeirão Preto e região, sendo 40 do sexo masculino e 40 do feminino, selecionados por meio de triagem, foram realizadas gravações digitais dos fonemas /a/, /e/ e /i/, originando uma amostra de 240 sinais acústicos submetidos ao Programa de Análise Acústica da Voz, desenvolvido na Escola de Engenharia de São Carlos da Universidade de São Paulo com obtenção das medidas acústicas. Resultados: Foram obtidos valores médios em relação a sexo e fonemas das medidas de: Freqüência fundamental, Jitter (Directional Perturbation Factor, Perturbation Variation Index, Jitter Ratio, Jitter Factor, Period Perturbation Quotient, Shimmer (Directional Perturbation Factor, Amplitude Variation Index, Amplitude Perturbation Quotient, Spectral Noise Level, Harmonic-to-noise ratio, Harmonic-to-noise ratio cepstrum, Normalized Noise Energy e Breathiness ratio. Conclusão: A normatização das medidas acústicas é necessária para conhecer melhor a voz normal. Os valores obtidos são compatíveis em sua grande maioria com à literatura existente.

  10. Medidas de calidad aplicadas a los levantamientos topográficos en Colombia

    OpenAIRE

    Sabogal Lemus, Carlos Augusto

    2016-01-01

    Este trabajo documenta la investigación “Medidas de calidad aplicadas a los levantamientos topográficos en Colombia”; la propuesta metodológica de este documento, tiene como objetivo principal la realización de la evaluación de calidad de un conjunto de datos levantados en campo, para lo cual es necesario revisar los antecedentes de la topografía en Colombia, así como los diferentes sistemas de referencia que gobiernan la cartografía del país -- Previo a realizar una evaluación de calidad, se...

  11. Medidas socioeducativas em meio aberto em Guaíba: entre pressupostos e significados

    OpenAIRE

    Jacques, Luciana Gomes de Lima

    2015-01-01

    No presente estudo, do tipo descritivo e exploratório, de natureza qualitativa, fundamentado no método dialético-crítico, discorre-se sobre os aspectos de proximidade e de distanciamento entre os pressupostos da socioeducação no Sistema Único de Assistência Social (SUAS) e no Sistema Nacional Socioeducativo (SINASE), e analisam-se os significados atribuídos às Medidas Socioeducativas em Meio Aberto (MSE-MA) pelos sujeitos que a protagonizam e/ou que participaram de seu processo de municipaliz...

  12. Medidas de selectividad y sensibilidad en un receptor de AM simplificado

    OpenAIRE

    Przylecki Siwek, Maciej

    2011-01-01

    Se describen las medidas de selectividad y sensibilidad de un receptor de AM simplificado que sólo dispone de una etapa detectora formada por antena de ferrita y un transistor BJT npn polarizado en zona no líneal actuando como un amplificador de clase B. La señal detectada se preamplifica y finalmente se lleva a un amplificador de audio de circuito integrado y al altavoz. Debido a la sencillez la selectividad es variable con la frecuencia de sintonía proporcionando a 392 KHz un...

  13. Pensamiento constructivo como medida de inteligencia emocional en patología dual

    OpenAIRE

    Albalat Alcaraz, Caridad; Fernández Ros, Encarnación; López García, Juan José

    2014-01-01

    Introducción: El objetivo de este estudio es comparar el pensamiento constructivo, una medida de inteligencia emocional, entre una muestra clínica de pacientes adultos diagnosticados de patología dual y una muestra no clínica. Método: Mediante un diseño de investigación comparativo, una muestra no clínica de 835 sujetos se comparó con una muestra de 180 sujetos diagnosticados de patología dual: 78 con trastornos clínicos o del Eje I y102 con trastornos de la personalidad o del ...

  14. Significados de las medidas de tendencia central : un estudio con alumnos universitarios de carreras de humanidades.

    OpenAIRE

    Sayritupac Gutierrez, Javier

    2013-01-01

    En el presente trabajo de investigación se analiza los significados personales e institucionales de las medidas de tendencia central en un estudio con alumnos de primeros ciclos de las carreras de humanidades de la Pontificia Universidad Católica del Perú. Para realizar este análisis se consideró como marco teórico el Enfoque Ontosemiótico de la Cognición e Instrucción Matemática (EOS), el cual nos brindó las herramientas necesarias para el análisis de nuestro objeto de estu...

  15. El tecnoestrés: un estudio del desarrollo de diferentes instrumentos de medida

    OpenAIRE

    Ventura, Mercedes; Llorens Gumbau, Susana; Salanova Soria, Marisa

    2005-01-01

    Onzenes Jornades de Foment de la Investigació de la FCHS (Any 2005-2006) El uso de las Tecnologías de la Información y la Comunicación (TICs) como herramienta de trabajo está teniendo un gran impacto en el mundo laboral. A pesar de que en si misma la tecnología es ‘neutra’ también puede generar consecuencias negativas en los usuarios de TIC quienes pueden sufrir el llamado ‘tecnoestrés’. El concepto y por tanto, la medida de este fenómeno han sufrido diferentes variaciones a lo la...

  16. Medidas de indices de refração de cristais liquidos esmecticos

    OpenAIRE

    Kroin, Teodosio

    1980-01-01

    Dissertação (mestrado) - Universidade Federal de Santa Catarina. Centro de Ciencias Fisicas e Matematicas Mostramos que os cristais líquidos biaxiais podem ter seus índices de refração principais medidos pelo método de Abbe, desde que convenientemente alinhados. Apresentam-se as medidas dos índices de refração das diferentes mesofases e da fase isotrópica do cristal líquido uni-axial 4-butoxibenzilideno-4'- aminoacetofenona em função da temperatura e para três comprimentos de onda. As medi...

  17. Abdominoplastia y pexia de pubis: estandarización de medidas

    OpenAIRE

    O. Ballestas-Campo; A. Pomerane

    2014-01-01

    La abdominoplastia es el procedimiento de elección para corregir la flacidez abdominal, la lipodistrofia supra e infraumbilical y la diástasis de los rectos abdominales. Los nuevos métodos añaden liposucción para definir el contorno corporal. Presentamos una estandarización de medidas para lograr una cicatriz abdominal baja y pexia pubiana en casos de lipodistrofias tipo III y IV de Matarasso. Realizamos un estudio observacional, descriptivo y retrospectivo, evaluando las historias clínicas y...

  18. La educación tributaria como medida para incrementar la recaudación fiscal

    OpenAIRE

    Tapia, Monica; Gaona, Wilmer; Tumbaco, Pedro

    2009-01-01

    La presente tesis está basada en el análisis de la La Educación Tributaria como Medida para Incrementar la Recaudación Fiscal en Ecuador; la importancia de este tema es incrementar la base de contribuyentes, aumentando la Recaudación Fiscal que ayudará a desarrollar planes de inversión y una estabilidad tributaria. Dentro de este estudio es necesario un análisis completo de naturaleza teórica, donde se examinaría la actividad financiera del Estado, la importancia en lo económico, ...

  19. Multiple Stellar Populations in Star Clusters

    Science.gov (United States)

    Piotto, G.

    2013-09-01

    For half a century it had been astronomical dogma that a globular cluster (GC) consists of stars born at the same time out of the same material, and this doctrine has borne rich fruits. In recent years, high resolution spectroscopy and high precision photometry (from space and ground-based observations) have shattered this paradigm, and the study of GC populations has acquired a new life that is now moving it in new directions. Evidence of multiple stellar populations have been identified in the color-magnitude diagrams of several Galactic and Magellanic Cloud GCs where they had never been imagined before.

  20. A Toolbox for Imaging Stellar Surfaces

    Science.gov (United States)

    Young, John

    2018-04-01

    In this talk I will review the available algorithms for synthesis imaging at visible and infrared wavelengths, including both gray and polychromatic methods. I will explain state-of-the-art approaches to constraining the ill-posed image reconstruction problem, and selecting an appropriate regularisation function and strength of regularisation. The reconstruction biases that can follow from non-optimal choices will be discussed, including their potential impact on the physical interpretation of the results. This discussion will be illustrated with example stellar surface imaging results from real VLTI and COAST datasets.

  1. Variance in binary stellar population synthesis

    Science.gov (United States)

    Breivik, Katelyn; Larson, Shane L.

    2016-03-01

    In the years preceding LISA, Milky Way compact binary population simulations can be used to inform the science capabilities of the mission. Galactic population simulation efforts generally focus on high fidelity models that require extensive computational power to produce a single simulated population for each model. Each simulated population represents an incomplete sample of the functions governing compact binary evolution, thus introducing variance from one simulation to another. We present a rapid Monte Carlo population simulation technique that can simulate thousands of populations in less than a week, thus allowing a full exploration of the variance associated with a binary stellar evolution model.

  2. The Advanced Stellar Compass, Development and Operations

    DEFF Research Database (Denmark)

    Jørgensen, John Leif; Liebe, Carl Christian

    1996-01-01

    The science objective of the Danish Geomagnetic Research Satellite "Ørsted" is to map the magnetic field of the Earth, with a vector precision of a fraction of a nanotesla. This necessitates an attitude reference instrument with a precision of a few arcseconds onboard the satellite. To meet...... this demand the Advanced Stellar Compass (ASC), a fully autonomous miniature star tracker, was developed. This ASC is capable of both solving the "lost in space" problem and determine the attitude with arcseconds precision. The development, principles of operation and instrument autonomy of the ASC...

  3. A large stellarator based on modular coils

    International Nuclear Information System (INIS)

    Hamberger, S.M.; Sharp, L.E.; Petersen, L.F.

    1979-06-01

    Although stellarators offer some considerable advantages over tokamaks, difficulties arise in designing large devices due, for instance, to poor plasma access as well as to constructional electromechanical and maintenance problems associated with continous helical windings. This paper describes a design for a fairly large device (major radius 2.1m), based on a set of discrete coil modules arranged in a toroidal configuration to provide the required closed magnetic surfaces, having gaps for unobstructed access to the plasma for diagnostics, etc, and allowing for easy removal for maintenance

  4. ECR heating in L-2M stellarator

    International Nuclear Information System (INIS)

    Grebenshchikov, S.E.; Batanov, G.M.; Fedyanin, O.I.

    1995-01-01

    The first results of ECH experiments in the L-2M stellarator are presented. The main goal of the experiments is to investigate the physics of ECH and plasma confinement at very high values of the volume heating power density. A current free plasma is produced and heated by extraordinary waves at the second harmonic of the electron cyclotron frequency. The experimental results are compared with the numerical simulations of plasma confinement and heating processes based on neoclassical theory using the full matrix of transport coefficients and with LHD-scaling. 4 refs., 2 figs

  5. Advanced Stellar Compass - ROCSAT 2 - Proposal

    DEFF Research Database (Denmark)

    Riis, Troels; Betto, Maurizio; Jørgensen, John Leif

    1998-01-01

    System Integration is supposed to take place at NSPO facilities.The ASC is a highly advanced and autonomous Stellar Reference Unit designed, developed and produced by the Space Instrumentation Group of the Department of Automation of the Technical University of Denmark.The document is structured...... and in section 7 the mechanical and electrical interfaces are given. In section 8 and 9 we address issues like manufacturing, transportation and storage and to conclude in section 10 the requirements imposed by the ASC on the system are given....

  6. Generating physically realizable stellar structures via embedding

    Energy Technology Data Exchange (ETDEWEB)

    Maurya, S.K. [University of Nizwa, Department of Mathematical and Physical Sciences, College of Arts and Science, Nizwa (Oman); Govender, M. [Durban University of Technology, Department of Mathematics, Faculty of Applied Sciences, Durban (South Africa)

    2017-05-15

    In this work we present an exact solution of the Einstein-Maxwell field equations describing compact charged objects within the framework of classical general relativity. Our model is constructed by embedding a four-dimensional spherically symmetric static metric into a five-dimensional flat metric. The source term for the matter field is composed of a perfect fluid distribution with charge. We show that our model obeys all the physical requirements and stability conditions necessary for a realistic stellar model. Our theoretical model approximates observations of neutron stars and pulsars to a very good degree of accuracy. (orig.)

  7. Equilibrium calculations for helical axis stellarators

    International Nuclear Information System (INIS)

    Hender, T.C.; Carreras, B.A.

    1984-04-01

    An average method based on a vacuum flux coordinate system is presented. This average method permits the study of helical axis stellarators with toroidally dominated shifts. An ordering is introduced, and to lowest order the toroidally averaged equilibrium equations are reduced to a Grad-Shafranov equation. Also, to lowest order, a Poisson-type equation is obtained for the toroidally varying corrections to the equilibium. By including these corrections, systems that are toroidally dominated, but with significant helical distortion to the equilibrium, may be studied. Numerical solutions of the average method equations are shown to agree well with three-dimensional calculations

  8. Nonlocal and collective relaxation in stellar systems

    Science.gov (United States)

    Weinberg, Martin D.

    1993-01-01

    The modal response of stellar systems to fluctuations at large scales is presently investigated by means of analytic theory and n-body simulation; the stochastic excitation of these modes is shown to increase the relaxation rate even for a system which is moderately far from instability. The n-body simulations, when designed to suppress relaxation at small scales, clearly show the effects of large-scale fluctuations. It is predicted that large-scale fluctuations will be largest for such marginally bound systems as forming star clusters and associations.

  9. Stellar Disk Truncations: HI Density and Dynamics

    Science.gov (United States)

    Trujillo, Ignacio; Bakos, Judit

    2010-06-01

    Using HI Nearby Galaxy Survey (THINGS) 21-cm observations of a sample of nearby (nearly face-on) galaxies we explore whether the stellar disk truncation phenomenon produces any signature either in the HI gas density and/or in the gas dynamics. Recent cosmological simulations suggest that the origin of the break on the surface brightness distribution is produced by the appearance of a warp at the truncation position. This warp should produce a flaring on the gas distribution increasing the velocity dispersion of the HI component beyond the break. We do not find, however, any evidence of this increase in the gas velocity dispersion profile.

  10. Global Clusters as Laboratories for Stellar Evolution

    Science.gov (United States)

    Catelan, Marcio; Valcarce, Aldo A. R.; Sweigart, Allen V.

    2010-01-01

    Globular clusters have long been considered the closest approximation to a physicist's laboratory in astrophysics, and as such a near-ideal laboratory for (low-mass) stellar evolution, However, recent observations have cast a shadow on this long-standing paradigm, suggesting the presence of multiple populations with widely different abundance patterns, and - crucially - with widely different helium abundances as welL In this review we discuss which features of the Hertzsprung-Russell diagram may be used as helium abundance indicators, and present an overview of available constraints on the helium abundance in globular clusters,

  11. Equilibrium studies of helical axis stellarators

    International Nuclear Information System (INIS)

    Hender, T.C.; Carreras, B.A.; Garcia, L.; Harris, J.H.; Rome, J.A.; Cantrell, J.L.; Lynch, V.E.

    1984-01-01

    The equilibrium properties of helical axis stellarators are studied with a 3-D equilibrium code and with an average method (2-D). The helical axis ATF is shown to have a toroidally dominated equilibrium shift and good equilibria up to at least 10% peak beta. Low aspect ratio heliacs, with relatively large toroidal shifts, are shown to have low equilibrium beta limits (approx. 5%). Increasing the aspect ratio and number of field periods proportionally is found to improve the equilibrium beta limit. Alternatively, increasing the number of field periods at fixed aspect ratio which raises and lowers the toroidal shift improves the equilibrium beta limit

  12. The Resolved Stellar Populations Early Release Science Program

    Science.gov (United States)

    Gilbert, Karoline; Weisz, Daniel; Resolved Stellar Populations ERS Program Team

    2018-06-01

    The Resolved Stellar Populations Early Release Science Program (PI D. Weisz) will observe Local Group targets covering a range of stellar density and star formation histories, including a globular cluster, and ultra-faint dwarf galaxy, and a star-forming dwarf galaxy. Using observations of these diverse targets we will explore a broad science program: we will measure star formation histories, the sub-solar stellar initial mass function, and proper motions, perform studies of evolved stars, and map extinction in the target fields. Our observations will be of high archival value for other science such as calibrating stellar evolution models, studying variable stars, and searching for metal-poor stars. We will determine optimal observational setups and develop data reduction techniques that will be common to JWST studies of resolved stellar populations. We will also design, test, and release point spread function (PSF) fitting software specific to NIRCam and NIRISS, required for the crowded stellar regime. Prior to the Cycle 2 Call for Proposals, we will release PSF fitting software, matched HST and JWST catalogs, and clear documentation and step-by-step tutorials (such as Jupyter notebooks) for reducing crowded stellar field data and producing resolved stellar photometry catalogs, as well as for specific resolved stellar photometry science applications.

  13. ESTIMATION OF DISTANCES TO STARS WITH STELLAR PARAMETERS FROM LAMOST

    Energy Technology Data Exchange (ETDEWEB)

    Carlin, Jeffrey L.; Newberg, Heidi Jo [Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180 (United States); Liu, Chao; Deng, Licai; Li, Guangwei; Luo, A-Li; Wu, Yue; Yang, Ming; Zhang, Haotong [Key Lab of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China); Beers, Timothy C. [Department of Physics and JINA: Joint Institute for Nuclear Astrophysics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Chen, Li; Hou, Jinliang; Smith, Martin C. [Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030 (China); Guhathakurta, Puragra [UCO/Lick Observatory, Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Hou, Yonghui [Nanjing Institute of Astronomical Optics and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Nanjing 210042 (China); Lépine, Sébastien [Department of Physics and Astronomy, Georgia State University, 25 Park Place, Suite 605, Atlanta, GA 30303 (United States); Yanny, Brian [Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Zheng, Zheng, E-mail: jeffreylcarlin@gmail.com [Department of Physics and Astronomy, University of Utah, UT 84112 (United States)

    2015-07-15

    We present a method to estimate distances to stars with spectroscopically derived stellar parameters. The technique is a Bayesian approach with likelihood estimated via comparison of measured parameters to a grid of stellar isochrones, and returns a posterior probability density function for each star’s absolute magnitude. This technique is tailored specifically to data from the Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) survey. Because LAMOST obtains roughly 3000 stellar spectra simultaneously within each ∼5° diameter “plate” that is observed, we can use the stellar parameters of the observed stars to account for the stellar luminosity function and target selection effects. This removes biasing assumptions about the underlying populations, both due to predictions of the luminosity function from stellar evolution modeling, and from Galactic models of stellar populations along each line of sight. Using calibration data of stars with known distances and stellar parameters, we show that our method recovers distances for most stars within ∼20%, but with some systematic overestimation of distances to halo giants. We apply our code to the LAMOST database, and show that the current precision of LAMOST stellar parameters permits measurements of distances with ∼40% error bars. This precision should improve as the LAMOST data pipelines continue to be refined.

  14. The Stellar Imager (SI) - A Mission to Resolve Stellar Surfaces, Interiors, and Magnetic Activity

    International Nuclear Information System (INIS)

    Christensen-Dalsgaard, Joergen; Carpenter, Kenneth G; Schrijver, Carolus J; Karovska, Margarita

    2011-01-01

    The Stellar Imager (SI) is a space-based, UV/Optical Interferometer (UVOI) designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and of the Universe in general. It will also probe via asteroseismology flows and structures in stellar interiors. SI will enable the development and testing of a predictive dynamo model for the Sun, by observing patterns of surface activity and imaging of the structure and differential rotation of stellar interiors in a population study of Sun-like stars to determine the dependence of dynamo action on mass, internal structure and flows, and time. SI's science focuses on the role of magnetism in the Universe and will revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. SI is a 'Landmark/Discovery Mission' in the 2005 Heliophysics Roadmap, an implementation of the UVOI in the 2006 Astrophysics Strategic Plan, and a NASA Vision Mission ('NASA Space Science Vision Missions' (2008), ed. M. Allen). We present here the science goals of the SI Mission, a mission architecture that could meet those goals, and the technology development needed to enable this mission. Additional information on SI can be found at: http://hires.gsfc.nasa.gov/si/.

  15. Direct Imaging of Stellar Surfaces: Results from the Stellar Imager (SI) Vision Mission Study

    Science.gov (United States)

    Carpenter, Kenneth; Schrijver, Carolus; Karovska, Margarita

    2006-01-01

    The Stellar Imager (SI) is a UV-Optical, Space-Based Interferometer designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and stellar interiors (via asteroseismology) and of the Universe in general. SI is identified as a "Flagship and Landmark Discovery Mission'' in the 2005 Sun Solar System Connection (SSSC) Roadmap and as a candidate for a "Pathways to Life Observatory'' in the Exploration of the Universe Division (EUD) Roadmap (May, 2005). The ultra-sharp images of the Stellar Imager will revolutionize our view of many dynamic astrophysical processes: The 0.1 mas resolution of this deep-space telescope will transform point sources into extended sources, and snapshots into evolving views. SI's science focuses on the role of magnetism in the Universe, particularly on magnetic activity on the surfaces of stars like the Sun. SI's prime goal is to enable long-term forecasting of solar activity and the space weather that it drives in support of the Living With a Star program in the Exploration Era. SI will also revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. In this paper we will discuss the results of the SI Vision Mission Study, elaborating on the science goals of the SI Mission and a mission architecture that could meet those goals.

  16. The Stellar Imager (SI) - A Mission to Resolve Stellar Surfaces, Interiors, and Magnetic Activity

    Energy Technology Data Exchange (ETDEWEB)

    Christensen-Dalsgaard, Joergen [Department of Physics and Astronomy, Aarhus University (Denmark); Carpenter, Kenneth G [Code 667 NASA-GSFC, Greenbelt, MD 20771 (United States); Schrijver, Carolus J [LMATC 3251 Hanover St., Bldg. 252, Palo Alto, CA 94304 (United States); Karovska, Margarita, E-mail: jcd@phys.au.d, E-mail: Kenneth.G.Carpenter@nasa.gov, E-mail: schryver@lmsal.com, E-mail: karovska@head.cfa.harvard.edu [60 Garden St., Cambridge, MA 02138 (United States)

    2011-01-01

    The Stellar Imager (SI) is a space-based, UV/Optical Interferometer (UVOI) designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and of the Universe in general. It will also probe via asteroseismology flows and structures in stellar interiors. SI will enable the development and testing of a predictive dynamo model for the Sun, by observing patterns of surface activity and imaging of the structure and differential rotation of stellar interiors in a population study of Sun-like stars to determine the dependence of dynamo action on mass, internal structure and flows, and time. SI's science focuses on the role of magnetism in the Universe and will revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. SI is a 'Landmark/Discovery Mission' in the 2005 Heliophysics Roadmap, an implementation of the UVOI in the 2006 Astrophysics Strategic Plan, and a NASA Vision Mission ('NASA Space Science Vision Missions' (2008), ed. M. Allen). We present here the science goals of the SI Mission, a mission architecture that could meet those goals, and the technology development needed to enable this mission. Additional information on SI can be found at: http://hires.gsfc.nasa.gov/si/.

  17. The Stellar Imager (SI) - A Mission to Resolve Stellar Surfaces, Interiors, and Magnetic Activity

    Science.gov (United States)

    Christensen-Dalsgaard, Jørgen; Carpenter, Kenneth G.; Schrijver, Carolus J.; Karovska, Margarita; Si Team

    2011-01-01

    The Stellar Imager (SI) is a space-based, UV/Optical Interferometer (UVOI) designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and of the Universe in general. It will also probe via asteroseismology flows and structures in stellar interiors. SI will enable the development and testing of a predictive dynamo model for the Sun, by observing patterns of surface activity and imaging of the structure and differential rotation of stellar interiors in a population study of Sun-like stars to determine the dependence of dynamo action on mass, internal structure and flows, and time. SI's science focuses on the role of magnetism in the Universe and will revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in the Universe. SI is a "Landmark/Discovery Mission" in the 2005 Heliophysics Roadmap, an implementation of the UVOI in the 2006 Astrophysics Strategic Plan, and a NASA Vision Mission ("NASA Space Science Vision Missions" (2008), ed. M. Allen). We present here the science goals of the SI Mission, a mission architecture that could meet those goals, and the technology development needed to enable this mission. Additional information on SI can be found at: http://hires.gsfc.nasa.gov/si/.

  18. The Stellar Imager (SI) - A Mission to Resolve Stellar Surfaces, Interiors, and Magnetic Activity

    Science.gov (United States)

    Christensen-Dalsgaard, Jorgen; Carpenter, Kenneth G.; Schrijver, Carolus J.; Karovska, Margarita

    2012-01-01

    The Stellar Imager (SI) is a space-based, UV/Optical Interferometer (UVOI) designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and of the Universe in general. It will also probe via asteroseismology flows and structures in stellar interiors. SI will enable the development and testing of a predictive dynamo model for the Sun, by observing patterns of surface activity and imaging of the structure and differential rotation of stellar interiors in a population study of Sun-like stars to determine the dependence of dynamo action on mass, internal structure and flows, and time. SI's science focuses on the role of magnetism in the Universe and will revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magnetohydrodynamically controlled processes in the Universe. SI is a "LandmarklDiscovery Mission" in the 2005 Heliophysics Roadmap, an implementation of the UVOI in the 2006 Astrophysics Strategic Plan, and a NASA Vision Mission ("NASA Space Science Vision Missions" (2008), ed. M. Allen). We present here the science goals of the SI Mission, a mission architecture that could meet those goals, and the technology development needed to enable this mission

  19. Colinesterasas en sangre total medidas con técnica semicuantitativa y en eritrocitos o plasma medidas con técnicas cuantitativas: relaciones

    Directory of Open Access Journals (Sweden)

    Jaime Carmona-Fonseca

    2007-06-01

    Resultados. Se evaluaron 827 trabajadores. Según la técnica Lovibond® se clasificaron en cuatro categorías: 821 con valores de 75% o más de actividad colinesterásica (categorías 75%, 87,5% y 100% y otros seis con actividad inferior a 75%. Con cada técnica cuantitativa los valores promedios de colinesterasa eritrocitaria y plasmática correspondientes a los cuatro valores de Lovibond® fueron estadísticamente diferentes entre sí. Los promedios de cada técnica cuantitativa fueron mayores a medida que creció el valor de la técnica semicuantitativa. Con Lovibond® se clasificó muy mal (61%-73% la baja actividad enzimática eritrocitaria, pero la clasificación de la baja actividad plasmática fue absolutamente errónea (94%-96%. Conclusión. Es posible estimar en forma adecuada los valores de colinesterasa eritrocitaria o plasmática que corresponden a las técnicas de Michel y EQM® a partir de datos de la técnica Lovibond® y viceversa, pero sólo cuando la actividad colinesterásica es normal, pues Lovibond® tiene una capacidad muy deficiente para identificar como "bajos" los valores que realmente lo son según las pruebas cuantitativas.

  20. Tasa de reincidencia de la delincuencia juvenil de Extremadura. Medidas privativas de libertad Tasa de reincidencia de la delincuencia juvenil de Extremadura. Medidas privativas de libertad

    Directory of Open Access Journals (Sweden)

    Felipe Núñez Izquierdo

    2012-04-01

    Full Text Available Después de más de 10 años de entrada en vigor de la Ley Orgánica 5/2000, de 12 de enero, de Responsabilidad Penal del Menor, se hace imprescindible realizar un estudio sobre la reincidencia juvenil en Extremadura, para conocer el impacto de dicho precepto. No cabe duda que uno de los problemas que más alarma social genera en la población es la delincuencia cometida por los menores con responsabilidad penal. Inicialmente se hace un repaso a la literatura criminológica actual sobre la reincidencia, programas de prevención, tratamiento a menores delincuentes y la evaluación de la eficacia de dichos programas. En el presente trabajo, siguiendo la metodología de otros estudios nacionales como el de Catalunya, analizamos la reincidencia de la delincuencia juvenil en Extremadura, concretamente de las medidas privativas de libertad. Se analizan los expedientes judiciales cerrados de aquellos jóvenes que hubieran finalizado una medida de este tipo en el año 2007 y se realiza el seguimiento de los mismos hasta el año 2010. En el año 2007, 115 jóvenes cumplieron o estaban cumpliendo una medida privativa de libertad en un Centro de Menores o Permanencia Fin de Semana, de los cuales 63 (57 varones y 7 mujeres resultaron pertenecer a la muestra final objeto de análisis. Los resultados obtenidos revelan que la tasa de reincidencia es del 52,4%, similar a la de otras Comunidades Autónomas, como País Vasco o Catalunya, e inferior a la de Asturias. Otro dato relevante es que un 41,9% de los menores objeto de estudio presentaban antecedentes, por lo que se refleja un comienzo en carreras delictivas acorde con los estudios existentes. La presente investigación ayuda a conocer la eficacia de los diferentes programas que se aplican a los menores delincuentes que cumplen medidas de internamiento, así como también hace una crítica de ésta al situarla con una elevada tasa de reincidencia.After more than 10 years of the entry into force of the

  1. The Origin of Stellar Species: constraining stellar evolution scenarios with Local Group galaxy surveys

    Science.gov (United States)

    Sarbadhicary, Sumit; Badenes, Carles; Chomiuk, Laura; Maldonado, Jessica; Caprioli, Damiano; Heger, Mairead; Huizenga, Daniel

    2018-01-01

    Our understanding of the progenitors of many stellar species, such as supernovae, massive and low-mass He-burning stars, is limited because of many poorly constrained aspects of stellar evolution theory. For my dissertation, I have focused on using Local Group galaxy surveys to constrain stellar evolution scenarios by measuring delay-time distributions (DTD). The DTD is the hypothetical occurrence rate of a stellar object per elapsed time after a brief burst of star formation. It is the measured distribution of timescales on which stars evolve, and therefore serves as a powerful observational constraint on theoretical progenitor models. The DTD can be measured from a survey of stellar objects and a set of star-formation histories of the host galaxy, and is particularly effective in the Local Group, where high-quality star-formation histories are available from resolved stellar populations. I am currently calculating a SN DTD with supernova remnants (SNRs) in order to provide the strongest constraints on the progenitors of thermonuclear and core-collapse supernovae. However, most SNRs do not have reliable age measurements and their evolution depends on the ambient environment. For this reason, I wrote a radio light curve model of an SNR population to extract the visibility times and rates of supernovae - crucial ingredients for the DTD - from an SNR survey. The model uses observational constraints on the local environments from multi-wavelength surveys, accounts for missing SNRs and employs the latest models of shock-driven particle acceleration. The final calculation of the SN DTD in the Local Group is awaiting completion of a systematic SNR catalog from deep radio-continuum images, now in preparation by a group led by Dr. Laura Chomiuk. I have also calculated DTDs for the LMC population of RR Lyrae and Cepheid variables, which serve as important distance calibrators and stellar population tracers. We find that Cepheids can have delay-times between 10 Myrs - 1 Gyr

  2. El ajuste en Cuba: ¿Medidas de sobrevivencia o nuevo modelo de desarrollo?

    Directory of Open Access Journals (Sweden)

    Hugo Fazio Vengoa

    1997-06-01

    Full Text Available El propósito del trabajo consiste en analizar la actual etapa por la que atraviesa Cuba y precisar la esencia de las reformas en curso. En una primera parte se señalan las características del modelo cubano de socialismo y los factores internos e internacionales que lo condujeron a una gran crisis. Después de pasar revista sobre la naturaleza del periodo especial, los autores señalan los límites que existen para que los sectores dinámicos en la actual economía cubana puedan convertirse en un nuevo modelo de desarrollo en la isla que le permita preservar su sistema socialista.

  3. SUB-STELLAR COMPANIONS AND STELLAR MULTIPLICITY IN THE TAURUS STAR-FORMING REGION

    International Nuclear Information System (INIS)

    Daemgen, Sebastian; Bonavita, Mariangela; Jayawardhana, Ray; Lafrenière, David; Janson, Markus

    2015-01-01

    We present results from a large, high-spatial-resolution near-infrared imaging search for stellar and sub-stellar companions in the Taurus-Auriga star-forming region. The sample covers 64 stars with masses between those of the most massive Taurus members at ∼3 M ☉ and low-mass stars at ∼0.2 M ☉ . We detected 74 companion candidates, 34 of these reported for the first time. Twenty-five companions are likely physically bound, partly confirmed by follow-up observations. Four candidate companions are likely unrelated field stars. Assuming physical association with their host star, estimated companion masses are as low as ∼2 M Jup . The inferred multiplicity frequency within our sensitivity limits between ∼10-1500 AU is 26.3 −4.9 +6.6 %. Applying a completeness correction, 62% ± 14% of all Taurus stars between 0.7 and 1.4 M ☉ appear to be multiple. Higher order multiples were found in 1.8 −1.5 +4.2 % of the cases, in agreement with previous observations of the field. We estimate a sub-stellar companion frequency of ∼3.5%-8.8% within our sensitivity limits from the discovery of two likely bound and three other tentative very low-mass companions. This frequency appears to be in agreement with what is expected from the tail of the stellar companion mass ratio distribution, suggesting that stellar and brown dwarf companions share the same dominant formation mechanism. Further, we find evidence for possible evolution of binary parameters between two identified sub-populations in Taurus with ages of ∼2 Myr and ∼20 Myr, respectively

  4. SUB-STELLAR COMPANIONS AND STELLAR MULTIPLICITY IN THE TAURUS STAR-FORMING REGION

    Energy Technology Data Exchange (ETDEWEB)

    Daemgen, Sebastian [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5H 3H4 (Canada); Bonavita, Mariangela [The University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Jayawardhana, Ray [Physics and Astronomy, York University, Toronto, Ontario L3T 3R1 (Canada); Lafrenière, David [Department of Physics, University of Montréal, Montréal, QC (Canada); Janson, Markus, E-mail: daemgen@astro.utoronto.ca [Department of Astronomy, Stockholm University, Stockholm (Sweden)

    2015-02-01

    We present results from a large, high-spatial-resolution near-infrared imaging search for stellar and sub-stellar companions in the Taurus-Auriga star-forming region. The sample covers 64 stars with masses between those of the most massive Taurus members at ∼3 M {sub ☉} and low-mass stars at ∼0.2 M {sub ☉}. We detected 74 companion candidates, 34 of these reported for the first time. Twenty-five companions are likely physically bound, partly confirmed by follow-up observations. Four candidate companions are likely unrelated field stars. Assuming physical association with their host star, estimated companion masses are as low as ∼2 M {sub Jup}. The inferred multiplicity frequency within our sensitivity limits between ∼10-1500 AU is 26.3{sub −4.9}{sup +6.6}%. Applying a completeness correction, 62% ± 14% of all Taurus stars between 0.7 and 1.4 M {sub ☉} appear to be multiple. Higher order multiples were found in 1.8{sub −1.5}{sup +4.2}% of the cases, in agreement with previous observations of the field. We estimate a sub-stellar companion frequency of ∼3.5%-8.8% within our sensitivity limits from the discovery of two likely bound and three other tentative very low-mass companions. This frequency appears to be in agreement with what is expected from the tail of the stellar companion mass ratio distribution, suggesting that stellar and brown dwarf companions share the same dominant formation mechanism. Further, we find evidence for possible evolution of binary parameters between two identified sub-populations in Taurus with ages of ∼2 Myr and ∼20 Myr, respectively.

  5. A revelação de abuso sexual: as medidas adotadas pela rede de apoio

    Directory of Open Access Journals (Sweden)

    Luísa Fernanda Habigzang

    Full Text Available O presente estudo identificou e analisou as medidas adotadas pela rede de apoio de crianças e adolescentes após a revelação de abuso sexual. Participaram 40 meninas, entre oito e 16 anos, vítimas de abuso sexual. As medidas de proteção adotadas pela rede foram mapeadas através de entrevista semi-estruturada. A revelação foi feita aos pais em 42,5% da amostra e 92,5% das pessoas acreditaram. O abrigamento ocorreu em 35% dos casos e o restante permaneceu com a família que afastou o agressor. A atitude de confiança da família na revelação e a denúncia da violência constituíram-se em um fator de proteção. Contudo, o alto índice de abrigamento e o não acompanhamento efetivo do afastamento do agressor representaram fatores de risco.

  6. La variable latente calidad medida a través del modelo de Rasch.

    Directory of Open Access Journals (Sweden)

    Guerrero, Mª M.

    1997-01-01

    Full Text Available La obtención de aceites de oliva de calidad requiere unos cuidados especiales en todas y cada una de las sucesivas fases de elaboración de los mismos, es una cadena que comienza en el olivo y termina en el consumo. Condición indispensable para ello es conocer las características organolépticas del aceite (a fin de potenciar sus atributos y eliminar, en la medida de los posible, sus defectos, y la influencia del proceso de elaboración en las mismas. El control y medida de estos caracteres se hará mediante las catas, realizadas por expertos catadores utilizando para ello las fichas de cata del Consejo Oleícola Internacional. El modelo de Rasch, que emplearemos para obtener la evaluación sensorial de los aceites de oliva virgen, nos permitirá no sólo dar una calificación organoléptica global al aceite (que ya podemos realizar sin necesidad de aplicar ningún método, siguiendo la metodología de valoración del Consejo Oleícola Internacional, sino también clasificar y medir los factores sensoriales que intervienen en la calidad, lo que nos permitirá realizar las acciones oportunas encaminadas a obtener aceites de oliva de cualidades óptimas.

  7. The Magellanic Analog Dwarf Companions and Stellar Halos (MADCASH) Survey: Near-Field Cosmology with Resolved Stellar Populations Around Local Volume LMC Stellar-Mass Galaxies

    Science.gov (United States)

    Carlin, Jeffrey L.; Sand, David J.; Willman, Beth; Brodie, Jean P.; Crnojevic, Denija; Peter, Annika; Price, Paul A.; Romanowsky, Aaron J.; Spekkens, Kristine; Strader, Jay

    2017-01-01

    We discuss the first results of our observational program to comprehensively map nearly the entire virial volumes of roughly LMC stellar mass galaxies at distances of ~2-4 Mpc. The MADCASH (Magellanic Analog Dwarf Companions And Stellar Halos) survey will deliver the first census of the dwarf satellite populations and stellar halo properties within LMC-like environments in the Local Volume. These will inform our understanding of the recent DES discoveries of dwarf satellites tentatively affiliated with the LMC/SMC system. We will detail our discovery of the faintest known dwarf galaxy satellite of an LMC stellar-mass host beyond the Local Group, based on deep Subaru+HyperSuprimeCam imaging reaching ~2 magnitudes below its TRGB. We will summarize the survey results and status to date, highlighting some challenges encountered and lessons learned as we process the data for this program through a prototype LSST pipeline. Our program will examine whether LMC stellar mass dwarfs have extended stellar halos, allowing us to assess the relative contributions of in-situ stars vs. merger debris to their stellar populations and halo density profiles. We outline the constraints on galaxy formation models that will be provided by our observations of low-mass galaxy halos and their satellites.

  8. Factores asociados con la cobertura vacunal declarada en la primera infancia: resultados de una encuesta telefónica

    OpenAIRE

    Nebot Manel; Muñoz Enrique; Figueres Marta; Rovira Gloria; Robert Montserrat; Minguell Dolors

    2001-01-01

    Fundamentos: El Plan de Vacunación Continuada de Barcelona permite conocer la cobertura vacunal poblacional a través de un sistema de declaración postal voluntaria de las familias. Estudios anteriores han demostrado que existe una proporción importante de familias que no notifican la vacunación, lo que puede conducir a una infraestimación de la cobertura real. Los objetivos de este estudio son estimar la cobertura vacunal poblacional en la primera infancia y conocer los f...

  9. Primera cita de la Argentina de Ophelimus maskelli (Ashmead (Hymenoptera: Eulophidae y su parasitoide, Closterocerus chamaeleon (Girault (Hymenoptera: Eulophidae

    Directory of Open Access Journals (Sweden)

    Daniel A AQUINO

    2014-01-01

    Full Text Available Se cita por primera vez de la Argentina la presencia de la avispa galí - cola exótica Ophelimus maskelli (Ashmead (Hymenoptera: Eulophidae y su para - sitoide natural, Closterocerus chamaeleon (Girault (Hymenoptera: Eulophidae en Eucalyptus camaldulensis de la provincia de Buenos Aires. Ophelimus maskelli es una especie invasora de origen Australiano que ha sido reportada como plaga de los eucaliptos en numerosos países de Asia, Europa y América. Closterocerus chamaleon es un parasitoide exótico cuyo potencial como biocontrolador de O. maskelli está siendo evaluado en algunos países.

  10. Emporion y las mutaciones de la arquitectura ibérica a la primera Edad de Hierro

    Directory of Open Access Journals (Sweden)

    Pierre MORET

    2009-12-01

    Full Text Available RESUMEN: A partir de las recientes excavaciones de la palaia polis de Empúries, se discute la posibilidad de influjos cruzados entre arquitecturas griega e indígena durante la primera Edad de Hierro en el Languedoc y costas orientales de la península Ibérica.ABSTRACT: Recent excavations at the palaia polis of Emporion (Empúries, Spain give way to a discussion about possible cross-influences between greek domestic architecture and native architecture in Western Languedoc and along the eastern coast of the Iberian Peninsula.

  11. A propósito de la primera traducción en prosa francesa de la "Historia regum Britanniae"

    OpenAIRE

    Simó, Meritxell

    2007-01-01

    El ms. BNF fr. 17177 nos ha conservado la primera traducción en prosa francesa de la Historia Regum Britanniae de Geoffrey de Monmouth, interpolada en la Histoire Ancienne jusqu'à César. Tras una serie de consideraciones preliminares sobre esta traducción, el artículo se centra en el estudio de las dos secciones más interesantes del texto: la Profecía de Merlín y los capítulos consagrados al reinado de Arturo. El artículo comenta las glosas que introduce el autor en la Profe...

  12. Votantes coreanos residentes en el exterior: su historia y el desarrollo de la primera experiencia electoral en Argentina

    OpenAIRE

    Bavoleo, Bárbara

    2018-01-01

    Resumen En las últimas elecciones presidenciales coreanas de diciembre del 2012, los coreanos residentes en el extranjero fueron habilitados para votar por primera vez en la historia de su sistema de gobierno democrático. Se sumaron así a los 180 países, según la base de datos del Instituto para la Democracia y la Asistencia Electoral (IDEA, su sigla en inglés, 2016), que poseen legislación que garantiza la participación electoral de sus ciudadanos en el exterior. La comunidad coreana en Arge...

  13. Pautas orientadoras para la promoción de la salud bucal en la primera infancia para profesionales de salud

    OpenAIRE

    Gloria Esperanza González C.

    2012-01-01

    La salud bucal es parte integral de la salud general del individuo. Lasafecciones bucales más prevalentes en niños son las alteraciones delcrecimiento y desarrollo bucodental, y la caries. Las primeras, generalmente están relacionadas con hábitos orales nocivos, patronesalimentarios inadecuados y la adquisición tardía de funciones comola masticación que generan maloclusiones. La caries, enfermedadcrónica más frecuente en la infancia, causa graves consecuencias enla salud del niño como dolor, ...

  14. Resección hepática asistida con radiofrecuencia bipolar: primeras experiencias con el Surtron SB

    Directory of Open Access Journals (Sweden)

    José Luis González González

    Full Text Available Las resecciones primarias y secundarias del hígado tienen como uno de sus mayores dilemas el sangrado transoperatorio. La introducción de los equipos de radiofrecuencia, en particular el Surtron SB, comienza a dar resultados alentadores. Se presentan las primeras 8 experiencias cubanas con resecciones menores y mayores realizadas con este equipo. Siete de estos pacientes tenían metástasis y uno un hepatocarcinoma. Se practicaron 2 resecciones regladas y 6 atípicas, durante las cuales no hubo complicaciones y solo un paciente necesitó transfusión sanguínea.

  15. Optical Monitoring of Young Stellar Objects

    Science.gov (United States)

    Kar, Aman; Jang-Condell, Hannah; Kasper, David; Findlay, Joseph; Kobulnicky, Henry A.

    2018-06-01

    Observing Young Stellar Objects (YSOs) for variability in different wavelengths enables us to understand the evolution and structure of the protoplanetary disks around stars. The stars observed in this project are known YSOs that show variability in the Infrared. Targets were selected from the Spitzer Space Telescope Young Stellar Object Variability (YSOVAR) Program, which monitored star-forming regions in the mid-infrared. The goal of our project is to investigate any correlation between the variability in the infrared versus the optical. Infrared variability of YSOs is associated with the heating of the protoplanetary disk while accretion signatures are observed in the H-alpha region. We used the University of Wyoming’s Red Buttes Observatory to monitor these stars for signs of accretion using an H-alpha narrowband filter and the Johnson-Cousins filter set, over the Summer of 2017. We perform relative photometry and inspect for an image-to-image variation by observing these targets for a period of four months every two to three nights. The study helps us better understand the link between accretion and H-alpha activity and establish a disk-star connection.

  16. Stellar populations in medium redshift clusters

    International Nuclear Information System (INIS)

    Pickles, A.J.; van der Kruit, P.C.; Pickles, A.J.

    1990-01-01

    We present a set of model isochrone spectra formed by combining stellar spectra in the proportions appropriate to the isochrone tabulations of VandenBerg, together with a Miller-Scalo mass function. The model spectra cover the wave-length range 3000-10000 A and have been constructed for metallicities in the range - 1.0 ≤ [Fe/H] ≤ 0.5, and for isochrone ages of 2 to 15 billion years. The model spectra follow the isochrone tabulations by including contributions from stars along the main sequence and subgiant branch to the base of the giant branch, fully constraining the main sequence turnoff and early post main sequence evolutionary phases. They are useful for deconvolving the competing effects of age and metallicity dispersion in composite systems. Other important components such as Horizontal branch, red giant and asymptotic branch stars are not included explicitly because they are not yet tabulated by VandenBerg, and because their fractional contributions to a composite population are less certain. These components should be added as extra parameters from a stellar library when fitting real composite spectra

  17. Bootstrap currents in stellarators and tokamaks

    International Nuclear Information System (INIS)

    Okamoto, Masao; Nakajima, Noriyoshi.

    1990-09-01

    The remarkable feature of the bootstrap current in stellarators is it's strong dependence on the magnetic field configuration. Neoclassical bootstrap currents in a large helical device of torsatron/heliotron type (L = 2, M = 10, R = 4 m, B = 4 T) is evaluated in the banana (1/ν) and the plateau regime. Various vacuum magnetic field configurations are studied with a view to minimizing the bootstrap current. It is found that in the banana regime, shifting of the magnetic axis and shaping of magnetic surfaces have a remarkable influence on the bootstrap current; a small outward shift of the magnetic axis and vertically elongated magnetic surfaces are favourable for a reduction of the bootstrap current. It is noted, however, that the ripple diffusion in the 1/ν regime has opposite tendency to the bootstrap current; it increases with the outward shift and increases as the plasma cross section is vertically elongated. The comparison will be made between bootstrap currents in stellarators and tokamaks. (author)

  18. A multi-institutional Stellarator Configuration Study

    Science.gov (United States)

    Gates, David

    2017-10-01

    A multi-institutional study aimed at mapping the space of quasi-axisymmetric stellarators has begun. The goal is to gain improved understanding of the dependence of important physics and engineering parameters (e.g. bootstrap current, stability, coil complexity, etc.) on plasma shape (average elongation, aspect ratio, number of periods). In addition, the stellarator optimization code STELLOPT will be upgraded with new capabilities such as improved coil design algorithms such as COILOPT + + and REGCOIL, divertor optimization options, equilibria with islands using the SPEC code, and improved bootstrap current calculations with the SFINCS code. An effort is underway to develop metrics for divertor optimization. STELLOPT has also had numerous improvements to numerical algorithms and parallelization capabilities. Simultaneously, we also are pursuing the optimization of turbulent transport according to the method of proxy functions. Progress made to date includes an elongation scan on quasi-axisymmetric equilibria and an initial comparison between the SFINCS code and the BOOTSJ calculation of bootstrap current currently available in STELLOPT. Further progress on shape scans and subsequent physics analysis will be reported. The status of the STELLOPT upgrades will be described. The eventual goal of this exercise is to identify attractive configurations for future US experimental facilities.. This work is supported by US DoE Contract Number DE-AC02-09CH11466.

  19. Color superconductivity in compact stellar hybrid configurations

    Science.gov (United States)

    Ranea-Sandoval, Ignacio F.; Orsaria, Milva G.; Han, Sophia; Weber, Fridolin; Spinella, William M.

    2017-12-01

    The discovery of pulsars PSR J1614-2230 and PSR J0348+0432 with masses of around 2 M⊙ imposes strong constraints on the equations of state of cold, ultradense matter. If a phase transition from hadronic matter to quark matter were to occur in the inner cores of such massive neutron stars, the energetically favorable state of quark matter would be a color superconductor. In this study, we analyze the stability and maximum mass of such neutron stars. The hadronic phase is described by nonlinear relativistic mean-field models, and the local Nambu-Jona Lasinio model is used to describe quark matter in the 2SC+s quark phase. The phase transition is treated as a Maxwell transition, assuming a sharp hadron-quark interface, and the "constant-sound-speed" (CSS) parametrization is employed to discuss the existence of stellar twin configurations. We find that massive neutron stars such as J1614-2230 and J0348+0432 can only exist on the connected stellar branch but not on the disconnected twin-star branch. The latter can only support stars with masses that are strictly below 2 M⊙ .

  20. Light measurement model to assess software development process improvement Modelo liviano de medidas para evaluar la mejora de procesos de desarrollo de software MLM-PDS

    Directory of Open Access Journals (Sweden)

    Diana Vásquez

    2010-12-01

    de mejora de procesos no es suficiente para decir siuna empresa realmente está obteniendo beneficios, definitivamente una de las primeras acciones en un proyecto de mejora es el poder determinar el estadoactual del proceso. Sólo midiendo es posible conocer el estado de un proceso de manera objetiva, y sólo gracias a esto se pueden planificar estrategias y soluciones acerca delas mejoras a realizar y según los objetivos de la organización. Este artículo propone un modelo liviano de medidas para evaluar un proyecto de mejora deprocesos de software, con el cual se busca ayudar a las empresas de desarrollode software colombianas a determinar si el proceso de mejora que implementan está siendo eficaz con relación a los objetivos y metas establecidas al inicio del proyecto. Esto se lleva a cabo a través del uso de medidas que permiten evaluar el proceso de mejora de sus procesos, facilitando la caracterizaciónde las prácticas actuales de la empresa y la identificación de las debilidades, fortalezas y habilidades de los procesos que son llevados a cabo dentro de ésta, permitiendo controlar y evitar las causas de baja calidad y desviaciones encostos o en planificación.

  1. Una medida de eficiencia de mercado. Un enfoque de teoría de la información

    Directory of Open Access Journals (Sweden)

    Reyna Susana García Ruiz

    2014-01-01

    Full Text Available En este trabajo, con base en el concepto de entropía de Shan-non, se propone una medida de eficiencia de mercado que uti-liza la función de densidad empírica de los rendimientos comoalfabeto para calcular la entropía del sistema y proveer con ellouna medida de eficiencia de mercado. Se demuestra que bajociertas condiciones de ergodicidad y de estacionariedad la en-tropía muestral converge a la entropía del estado dominante,lo que valida el uso de la entropía muestral como medida deeficiencia del sistema. Asimismo, se demuestra que la medidapropuesta es consistente con algunos de los axiomas de Artz-neret al.(1999 acerca de una medida coherente de riesgo. Porúltimo, con fines ilustrativos, se llevan a cabo varias aplicacio-nes de la medida de eficiencia propuesta a distintos mercadosde capitales: DJIA, S&P500, FTSE100 e IPC.

  2. Stellar oscillations in planet-hosting giant stars

    Energy Technology Data Exchange (ETDEWEB)

    Hatzes, Artie P; Zechmeister, Mathias [Thueringer Landessternwarte, Sternwarte 5, D-07778 (Germany)], E-mail: artie@tls-tautenburg.de

    2008-10-15

    Recently a number of giant extrasolar planets have been discovered around giant stars. These discoveries are important because many of these giant stars have intermediate masses in the range 1.2-3 Msun. Early-type main sequence stars of this mass range have been avoided by radial velocity planet search surveys due the difficulty of getting the requisite radial velocity precision needed for planet discoveries. Thus, giant stars can tell us about planet formation for stars more massive than the sun. However, the determination of stellar masses for giant stars is difficult due to the fact that evolutionary tracks for stars covering a wide range of masses converge to the same region of the H-R diagram. We report here on stellar oscillations in three planet-hosting giant stars: HD 13189, {beta} Gem, and {iota} Dra. Precise stellar radial velocity measurements for these stars show variations whose periods and amplitudes are consistent with solar-like p-mode oscillations. The implied stellar masses for these objects based on the characteristics of the stellar oscillations are consistent with the predictions of stellar isochrones. An investigation of stellar oscillations in planet hosting giant stars offers us the possibility of getting an independent determination of the stellar mass for these objects which is of crucial importance for extrasolar planet studies.

  3. First results from stellar occultations in the "GAIA era"

    Science.gov (United States)

    Benedetti-Rossi, G.; Vieira-Martins, R.; Sicardy, B.

    2017-09-01

    Stellar occultation is a powerful technique to study distant solar system bodies. It allows high angular resolution of the occulting body from the analysis of a light curve acquired with high temporal resolution with uncertainties comparable as probes. In the "GAIA era", stellar occultations is now able to obtain even more impressive results such as the presence of atmosphere, rings and topographic features.

  4. Recent advances in non-LTE stellar atmosphere models

    Science.gov (United States)

    Sander, Andreas A. C.

    2017-11-01

    In the last decades, stellar atmosphere models have become a key tool in understanding massive stars. Applied for spectroscopic analysis, these models provide quantitative information on stellar wind properties as well as fundamental stellar parameters. The intricate non-LTE conditions in stellar winds dictate the development of adequate sophisticated model atmosphere codes. The increase in both, the computational power and our understanding of physical processes in stellar atmospheres, led to an increasing complexity in the models. As a result, codes emerged that can tackle a wide range of stellar and wind parameters. After a brief address of the fundamentals of stellar atmosphere modeling, the current stage of clumped and line-blanketed model atmospheres will be discussed. Finally, the path for the next generation of stellar atmosphere models will be outlined. Apart from discussing multi-dimensional approaches, I will emphasize on the coupling of hydrodynamics with a sophisticated treatment of the radiative transfer. This next generation of models will be able to predict wind parameters from first principles, which could open new doors for our understanding of the various facets of massive star physics, evolution, and death.

  5. Proton Testing of Advanced Stellar Compass Digital Processing Unit

    DEFF Research Database (Denmark)

    Thuesen, Gøsta; Denver, Troelz; Jørgensen, Finn E

    1999-01-01

    The Advanced Stellar Compass Digital Processing Unit was radiation tested with 300 MeV protons at Proton Irradiation Facility (PIF), Paul Scherrer Institute, Switzerland.......The Advanced Stellar Compass Digital Processing Unit was radiation tested with 300 MeV protons at Proton Irradiation Facility (PIF), Paul Scherrer Institute, Switzerland....

  6. The Advanced Stellar Compass onboard the Oersted satellite

    DEFF Research Database (Denmark)

    Jørgensen, John Leif; Eisenman, Allan R.; Liebe, Carl Christian

    1997-01-01

    In 1997 the first Danish satellite will be launched. The primarily scientific objective of the satellite is to map the magnetic field of the Earth. The attitude of the satellite is determined by an advanced stellar compass (star tracker). An advanced stellar compass consists of a CCD camera...

  7. Variation of galactic cold gas reservoirs with stellar mass

    NARCIS (Netherlands)

    Maddox, Natasha; Hess, Kelley M.; Obreschkow, Danail; Blyth, S.-L.; Jarvis, Matt J.

    The stellar and neutral hydrogen (H I) mass functions at z ˜ 0 are fundamental benchmarks for current models of galaxy evolution. A natural extension of these benchmarks is the two-dimensional distribution of galaxies in the plane spanned by stellar and H I mass, which provides a more stringent test

  8. Stellar Relics from the Early Galaxy T. Sivarani

    Indian Academy of Sciences (India)

    metal-poor stars is used to study the chemical history of the galaxy. Apart from this,. 5 .... They fit a color-magnitude diagram in order to trace different stellar population and derived a ... distinctly different stellar population with a different origin.

  9. Is the Mercier criterion relevant to stellarator stability?

    International Nuclear Information System (INIS)

    Carreras, B.A.; Lynch, V.E.; Ichiguchi, K.; Wakatani, M.; Tatsuno, T.

    2001-01-01

    Local flattening of the pressure profile at the resonant surfaces may significantly change the stellarator stability properties. This flattening may be an intrinsic consequence of the three-dimensional nature of the equilibrium and may invalidate the local stability criteria often used in stellarator design. (author)

  10. Operations of a non-stellar object tracker in space

    DEFF Research Database (Denmark)

    Riis, Troels; Jørgensen, John Leif; Betto, Maurizio

    1999-01-01

    The ability to detect and track non-stellar objects by utilizing a star tracker may seem rather straight forward, as any bright object, not recognized as a star by the system is a non stellar object. However, several pitfalls and errors exist, if a reliable and robust detection is required. To te...

  11. La resistencia a las innovaciones. Informe de la academia de profesores de primera educación (1838

    Directory of Open Access Journals (Sweden)

    Federico GÓMEZ-R. DE CASTRO

    2010-03-01

    Full Text Available RESUMEN: 1837. La recién restituida Dirección General de Estudios elabora un informe sobre la enseñanza gratuita de las primeras letras en la Corte. Está en quiebra el principio de la gratuidad y alienta un criterio economista de sacar el rendimiento óptimo a las inversiones. Se subordinan organización y métodos a estos supuestos económicos. Y sobre ello se cantan las excelencias del método de enseñanza mutua, el viejo y querido juguete de constitucionalistas, liberales, aristócratas y militares. Detrás está en marcha el proceso de centralización de enseñanza pública. No obstante, con buenos modales democráticos —dinamos hoy— la Dirección General de Estudios presenta el resultado de su encuesta al Ayuntamiento constitucional de la Corte el día 13 de septiembre. El Ayuntamiento constitucional solicita un contrainforme de la Academia Literaria de Profesores de Primera Educación. El contrainforme está listo y se remite el día 4 de enero de 1838 firmado por el secretario de la Academia, Alejandro Palomino.

  12. Proyectos y ensayos en torno a la primera Exposición conjunta de Arte Normativo Español

    Directory of Open Access Journals (Sweden)

    Barreiro López, Paula

    2005-06-01

    Full Text Available The Primera Exposición Conjunta de Arte Normativo Español, held in the Athenaeum of Valencia in March 1960, was the result of a series of earlier projects which, since 1959, had been oriented toward the unification in a common front of Spanish constructivist tendencies. In this article the author studies the precedent projects and their transformation into this exhibition, and analyses the projects and debates brought about by the show, both within this collective and in the criticism of the period.

    La Primera Exposición Conjunta de Arte Normativo Español, realizada en el Ateneo de Valencia en marzo de 1960, fue el resultado de toda una serie de proyectos anteriores que, desde 1959, estaban encaminados a la unificación de las tendencias constructivistas españolas en un frente común. El objeto de este artículo es el estudio de dichos proyectos precedentes y de su transformación en la citada exposición, analizando, además, los planes y debates que suscitó la muestra, tanto dentro del colectivo, como en la crítica del momento

  13. Abdominoplastia y pexia de pubis: estandarización de medidas

    Directory of Open Access Journals (Sweden)

    O. Ballestas-Campo

    2014-06-01

    Full Text Available La abdominoplastia es el procedimiento de elección para corregir la flacidez abdominal, la lipodistrofia supra e infraumbilical y la diástasis de los rectos abdominales. Los nuevos métodos añaden liposucción para definir el contorno corporal. Presentamos una estandarización de medidas para lograr una cicatriz abdominal baja y pexia pubiana en casos de lipodistrofias tipo III y IV de Matarasso. Realizamos un estudio observacional, descriptivo y retrospectivo, evaluando las historias clínicas y las fotografías sobre 420 mujeres, con edades entre 18 y 63 años, intervenidas entre 2004 y 2011. Basamos la técnica quirúrgica en los siguientes principios: referencias anatómicas; medidas estandarizadas con la paciente de pie sobre zapatos de tacón alto para el trazado de una incisión suprapúbica baja, siguiendo diseño de los autores; pexia de pubis y región inguinal; cicatriz suprapúbica baja cubierta por un biquini estándar. El 70,95 % de los casos (298 pacientes correspondieron a abdomen grado IV de lipodistrofia, el 28,57 % (120 pacientes al grado III y el 0,47 % (2 pacientes al grado II según Matarasso. Las complicaciones más frecuentes fueron: seroma, (4,04 % , alteraciones cicatríciales (7,37 % , necrosis parcial y epidermolisis (2,38 % y estenosis umbilical (1,19 % . Como conclusión creemos que la estandarización de medidas para el diseño de la cicatriz en la abdominoplastia permite obtener resultados estéticos predecibles y funcionales buenos: cicatriz baja cubierta por un biquini o ropa interior estándar, cicatriz umbilical ovalada, pexia de pubis y excelente definición del contorno abdominal y corporal, con baja tasa de complicaciones.

  14. The economic emergency: an insufficient solution La emergencia económica: una medida inconclusa

    Directory of Open Access Journals (Sweden)

    Lorente Luis

    1997-06-01

    Full Text Available There are many reasons for the Colombian recession that began in 1995, but the disagreement between fiscal and monetary authorities is an outstanding one. Monetary measures against inflation promoted high interest rates, made real investment more risky, rocketed the exchange rate, attracted foreign capital and elevated public debt costs.
    Emergency measures announced early in the year were insufficient because the problem comes from old and needs long range measures. Balanced budget is a valid target, but along the economic cycle and not in each fiscal year. Reduction of public expenses or public debt must be applied in periods of growth and not when taxes go down because a recession has begun. Monetary policy must allow for anti-cyclical measures and can do it effectively by controlling the volume. of credit accessible to the Government, or to finance private construction of public works, or to those that will buy the facilities and services that get privatized.La fase recesiva de la economía colombiana que comenzó en 1995 tiene varias causas, en especial, el desacuerdo entre políticas fiscales y monetarias. Las medidas antiinflacionarias elevaron las tasas de interés y dificultaron la inversión, y provocaron la revaluación de la moneda, la promoción de la entrada masiva de capital externo y del encarecimiento del servicio de la deuda pública. Las medidas de emergencia anunciadas a comienzos de 1995 no fueron suficientes: se necesita una política con objetivos de largo plazo. Hay que buscar un balance fiscal a lo largo del ciclo económico y no en cada año fiscal; la contracción del gasto público debe aplicarse en las fases de auge económico y no cuando caen los recaudos porque ya comenzó una recesión. La política monetaria debe permitir medidas anticíclicas y puede contribuir a ellas si regula el volumen de crédito accesible al Estado, a sus contratistas y a quienes adquieren prvatizaciones.

  15. SERVIÇO SOCIAL, MEDIDAS SOCIOEDUCATIVAS E O ADOLESCENTE INFRATOR NO LIBERDADE ASSISTIDA

    Directory of Open Access Journals (Sweden)

    Cristiano Costa Carvalho

    2013-10-01

    Full Text Available RESUMO: A temática dos adolescentes em conflito com a Lei é uma questão que merece uma atenção especial, pois é significativa ao longo da trajetória pela conquista da mudança de paradigma na legislação em relação ao enfrentamento desta expressão da questão social, e porque mesmo diante desta mudança, as medidas em meio aberto são as que têm sido menos aplicadas. Deste modo, esta pesquisa permitiu conhecer e problematizar a atuação do profissional de Serviço Social dentro da política de atendimento aos adolescentes em conflito com a Lei e em destaque a medida socioeducativa no programa de Liberdade Assistida, devido a sua característica educativa que preserva o convívio social, familiar e comunitária.  O processo de preparação desta pesquisa consistiu em entrevistas semi-estruturadas, estudos bibliográficos, documentais, e acervos digitais. Foi analisado o potencial da atuação profissional em consonância com as diretrizes previstas pelo Estatuto da Criança e do Adolescente, Lei que garante aos mesmos um atendimento especial, e reconhece que são sujeitos em processo de formação. PALAVRAS-CHAVE: adolescentes, ato infracional, medidas socioeducativas ABSTRACT: The topic of minors in conflict with the Law is an issue that deserves special attention due to its representativeness in the course of attaining a paradigm shift in the legislation related to this social matter, and because even before this change takes place, it is the open regime measures that have been less applied. This research has therefore helped identify and discuss the role of the Social Worker in the assistance policy for juveniles in conflict with the Law, highlighting the socio-educational measure of the probation program “Liberdade Assistida”, which, due to its educational nature, preserves the social, family and community life. The process of preparing this research consisted of semi-structured interviews, bibliographical and documentary

  16. Improving 1D Stellar Models with 3D Atmospheres

    Science.gov (United States)

    Rørsted Mosumgaard, Jakob; Silva Aguirre, Víctor; Weiss, Achim; Christensen-Dalsgaard, Jørgen; Trampedach, Regner

    2017-10-01

    Stellar evolution codes play a major role in present-day astrophysics, yet they share common issues. In this work we seek to remedy some of those by the use of results from realistic and highly detailed 3D hydrodynamical simulations of stellar atmospheres. We have implemented a new temperature stratification extracted directly from the 3D simulations into the Garching Stellar Evolution Code to replace the simplified atmosphere normally used. Secondly, we have implemented the use of a variable mixing-length parameter, which changes as a function of the stellar surface gravity and temperature - also derived from the 3D simulations. Furthermore, to make our models consistent, we have calculated new opacity tables to match the atmospheric simulations. Here, we present the modified code and initial results on stellar evolution using it.

  17. Medida de la evapotranspiración real en coberturas vegetales semiáridas (Cuenca de Mula, Murcia), según las varicaciones de humedad del suelo medidas mediante el procedimiento (TDR)

    OpenAIRE

    Belmonte Serrato, Francisco; Romero Díaz, María Asunción

    2006-01-01

    En este trabajo se presenta un método de medida directa de la Evapotranspiración Real (ETR) bajo distintas coberturas vegetales, basado en las diferencias de humedad en el suelo medidas mediante el procedimiento TDR, en un intervalo temporal de 15 días y su comparación con los valores calculados mediante el método de Thornthwaite, que usa la temperatura media como parámetro fundamental. Los resultados demuestran la validez del método utilizado, habiendo obtenido valores de E...

  18. Equipo adiabático para medida del coeficiente de absorción específico de un material sometido a un campo magnético alterno y método para realizar dicha medida

    OpenAIRE

    Mediano, Arturo; Natividad, Eva; Palacio, Fernando; Castro, Miguel

    2007-01-01

    Equipo adiabático para medida del coeficiente de absorción específico de un material sometido a un campo magnético alterno y método para realizar dicha medida. En esta patente se describe un equipo que permite medir de forma adiabática el incremento de temperatura experimentado por aquellos materiales que presentan mecanismos activos de disipación de calor al someterlos a un campo magnético alterno. Conocida esta magnitud y el tiempo de aplicación del campo y, conocien...

  19. Spectrum of ballooning instabilities in a stellarator

    Energy Technology Data Exchange (ETDEWEB)

    Cooper, W A [Ecole Polytechnique Federale, Lausanne (Switzerland). Centre de Recherche en Physique des Plasma (CRPP); Singleton, D B [Australian National Univ., ANU Supercomputing Facility, Canberra (Australia); Dewar, R L [Australian National Univ., Canberra, ACT (Australia). Research School of Physical Sciences

    1995-08-01

    The recent revival of interest in the application of the `ballooning formalism` to low-frequency plasma instabilities has prompted a comparison of the Wentzel-Brillouin-Kramers (WKB) ballooning approximation with an (in principle) exact normal mode calculation for a three-dimensional plasma equilibrium. Semiclassical quantization, using the ideal magnetohydrodynamic (MHD) ballooning eigenvalue to provide a local dispersion relation, is applied to a ten-field period stellarator test case. Excellent qualitative agreement, and good quantitative agreement is found with predictions from the TERPSICHORE code for toroidal mode numbers from 1 to 14 and radial mode numbers from 0 to 2. The continuum bands predicted from three-dimensional WKB theory are too narrow to resolve. (author) 3 figs., 24 refs.

  20. Spectrum of ballooning instabilities in a stellarator

    International Nuclear Information System (INIS)

    Cooper, W.A.; Singleton, D.B.; Dewar, R.L.

    1995-08-01

    The recent revival of interest in the application of the 'ballooning formalism' to low-frequency plasma instabilities has prompted a comparison of the Wentzel-Brillouin-Kramers (WKB) ballooning approximation with an (in principle) exact normal mode calculation for a three-dimensional plasma equilibrium. Semiclassical quantization, using the ideal magnetohydrodynamic (MHD) ballooning eigenvalue to provide a local dispersion relation, is applied to a ten-field period stellarator test case. Excellent qualitative agreement, and good quantitative agreement is found with predictions from the TERPSICHORE code for toroidal mode numbers from 1 to 14 and radial mode numbers from 0 to 2. The continuum bands predicted from three-dimensional WKB theory are too narrow to resolve. (author) 3 figs., 24 refs

  1. Constraints on stellar evolution from pulsations

    International Nuclear Information System (INIS)

    Cox, A.N.

    1984-01-01

    Consideration of the many types of intrinsic variable stars, that is, those that pulsate, reveals that perhaps a dozen classes can indicate some constraints that affect the results of stellar evolution calculations, or some interpretations of observations. Many of these constraints are not very strong or may not even be well defined yet. The author discusses the case for six classes: classical Cepheids with their measured Wesselink radii, the observed surface effective temperatures of the known eleven double-mode Cepheids, the pulsation periods and measured surface effective temperatures of three R CrB variables, the delta Scuti variable VZ Cnc with a very large ratio of its two observed periods, the nonradial oscillations of the Sun, and the period ratios of the newly discovered double-mode RR Lyrae variables. (Auth.)

  2. Status of the US stellarator reactor study

    International Nuclear Information System (INIS)

    Lyon, J.F.; Gulec, K.; Miller, R.L.; El-Guebaly, L.

    1994-01-01

    Stellarators have significant operational advantages over tokamaks as ignited steady-state reactors. This scoping study, which uses an integrated cost-minimization code that incorporates costing and reactor component models self-consistently with a 1-D energy transport calculation, shows that a torsatron reactor could also be competitive with a tokamak reactor. The projected cost of electricity (COE) estimated using the ARIES costing algorithms is 62.5 mill/kW(e)h in constant 1992 dollars for a 1-GW(e) Compact Torsatron reactor reference case. The COE is relatively insensitive (< 10% variation) over a wide range of assumptions including variations in the maximum field allowed on the coils, the coil elongation, the shape of the density profile, the beta limit, the confinement multiplier, and the presence of a large loss region for alpha particles. The largest variations in the COE occur for variations in the electrical power output demanded and the plasma-coil separation ratio

  3. Quasiaxially symmetric stellarators with three field periods

    International Nuclear Information System (INIS)

    Garabedian, P.; Ku, L.

    1999-01-01

    Compact hybrid configurations with two field periods have been studied recently as candidates for a proof of principle experiment at the Princeton Plasma Physics Laboratory. This project has led us to the discovery of a family of quasiaxially symmetric stellarators with three field periods that have significant advantages, although their aspect ratios are a little larger. They have reversed shear and perform better in a local analysis of ballooning modes. Nonlinear equilibrium and stability calculations predict that the average beta limit will be at least as high as 4% if the bootstrap current turns out to be as big as that expected in comparable tokamaks. The concept relies on a combination of helical fields and bootstrap current to achieve adequate rotational transform at low aspect ratio. copyright 1999 American Institute of Physics

  4. Planck scale still safe from stellar images

    International Nuclear Information System (INIS)

    Coule, D H

    2003-01-01

    The recent paper of Lieu and Hillman (2003 Astrophys. J. Lett. 585 L77) suggesting that a possible (birefringence-like) phase difference ambiguity coming from Planck effects would alter stellar images of distant sources is questioned. Instead for division of wavefront interference and diffraction phenomena, initial (lateral) coherence is developed simply by propagation of rays (cf the van Cittert-Zernike theorem). This case is strongly immune to quantum gravity influences that could tend to reduce phase coherence. The phase ambiguity, if actually present, could reduce any underlying polarization of the light rays. However, we argue that, as expected since any inherent quantum discreteness of space should become increasingly negligible over larger distances, such a phase ambiguity is rapidly cancelled if a more realistic constantly fluctuating quantum 'buffeting' occurs

  5. Tutorial: Asteroseismic Stellar Modelling with AIMS

    Science.gov (United States)

    Lund, Mikkel N.; Reese, Daniel R.

    The goal of aims (Asteroseismic Inference on a Massive Scale) is to estimate stellar parameters and credible intervals/error bars in a Bayesian manner from a set of asteroseismic frequency data and so-called classical constraints. To achieve reliable parameter estimates and computational efficiency, it searches through a grid of pre-computed models using an MCMC algorithm—interpolation within the grid of models is performed by first tessellating the grid using a Delaunay triangulation and then doing a linear barycentric interpolation on matching simplexes. Inputs for the modelling consist of individual frequencies from peak-bagging, which can be complemented with classical spectroscopic constraints. aims is mostly written in Python with a modular structure to facilitate contributions from the community. Only a few computationally intensive parts have been rewritten in Fortran in order to speed up calculations.

  6. Recent progress in stellarator reactor conceptual design

    International Nuclear Information System (INIS)

    Miller, R.L.

    1985-01-01

    The Stellarator/Torsatron/Heliotron (S/T/H) class of toroidal magnetic fusion reactor designs continues to offer a distinct and in several ways superior approach to eventual commercial competitiveness. Although no major, integrated conceptual reactor design activity is presently underway, a number of international research efforts suggest avenues for the substantial improvement of the S/T/H reactor embodiment, which derive from recent experimental and theoretical progress and are responsive to current trends in fusion-reactor projection to set the stage for a third generation of designs. Recent S/T/H reactor design activity is reviewed and the impact of the changing technical and programmatic context on the direction of future S/T/H reactor design studies is outlined

  7. Energy balance in solar and stellar chromospheres

    Science.gov (United States)

    Avrett, E. H.

    1981-01-01

    Net radiative cooling rates for quiet and active regions of the solar chromosphere and for two stellar chromospheres are calculated from corresponding atmospheric models. Models of chromospheric temperature and microvelocity distributions are derived from observed spectra of a dark point within a cell, the average sun and a very bright network element on the quiet sun, a solar plage and flare, and the stars Alpha Boo and Lambda And. Net radiative cooling rates due to the transitions of various atoms and ions are then calculated from the models as a function of depth. Large values of the net radiative cooling rate are found at the base of the chromosphere-corona transition region which are due primarily to Lyman alpha emission, and a temperature plateau is obtained in the transition region itself. In the chromospheric regions, the calculated cooling rate is equal to the mechanical energy input as a function of height and thus provides a direct constraint on theories of chromospheric heating.

  8. Stellar pulsations in beyond Horndeski gravity theories

    Energy Technology Data Exchange (ETDEWEB)

    Sakstein, Jeremy [Center for Particle Cosmology, Department of Physics and Astronomy, University of Pennsylvania, 209 S. 33rd St., Philadelphia, PA 19104 (United States); Kenna-Allison, Michael; Koyama, Kazuya, E-mail: sakstein@physics.upenn.edu, E-mail: mka1g13@soton.ac.uk, E-mail: kazuya.koyama@port.ac.uk [Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX (United Kingdom)

    2017-03-01

    Theories of gravity in the beyond Horndeski class recover the predictions of general relativity in the solar system whilst admitting novel cosmologies, including late-time de Sitter solutions in the absence of a cosmological constant. Deviations from Newton's law are predicted inside astrophysical bodies, which allow for falsifiable, smoking-gun tests of the theory. In this work we study the pulsations of stars by deriving and solving the wave equation governing linear adiabatic oscillations to find the modified period of pulsation. Using both semi-analytic and numerical models, we perform a preliminary survey of the stellar zoo in an attempt to identify the best candidate objects for testing the theory. Brown dwarfs and Cepheid stars are found to be particularly sensitive objects and we discuss the possibility of using both to test the theory.

  9. Comparison between stellarator and tokamak divertor transport

    International Nuclear Information System (INIS)

    Feng, Y.; Lunt, T.; Kobayashi, M.; Reiter, D.

    2010-11-01

    The paper compares the essential divertor transport features of the poloidal divertor, which is well-developed for tokamaks, and the non-axisymmetric divertors currently investigated on helical devices. It aims at surveying the fundamental similarities and differences in divertor concept and geometry, and their consequences for how the divertor functions. In particular, the importance of various transport terms governing axisymmetric and helical scrape-off-layers (SOLs) is examined, with special attention being paid to energy, momentum and impurity transport. Tokamak and stellarator SOLs are compared by identifying key geometric parameters through which the governing physics can be illustrated by simple models and estimates. More quantitative assessments rely nevertheless on the modeling using EMC3-EIRENE code. Most of the theoretical results are discussed in conjunction with experimental observations. (author)

  10. Stellar pulsations in beyond Horndeski gravity theories

    Science.gov (United States)

    Sakstein, Jeremy; Kenna-Allison, Michael; Koyama, Kazuya

    2017-03-01

    Theories of gravity in the beyond Horndeski class recover the predictions of general relativity in the solar system whilst admitting novel cosmologies, including late-time de Sitter solutions in the absence of a cosmological constant. Deviations from Newton's law are predicted inside astrophysical bodies, which allow for falsifiable, smoking-gun tests of the theory. In this work we study the pulsations of stars by deriving and solving the wave equation governing linear adiabatic oscillations to find the modified period of pulsation. Using both semi-analytic and numerical models, we perform a preliminary survey of the stellar zoo in an attempt to identify the best candidate objects for testing the theory. Brown dwarfs and Cepheid stars are found to be particularly sensitive objects and we discuss the possibility of using both to test the theory.

  11. A new class of relativistic stellar models

    Science.gov (United States)

    Haggag, Salah

    1995-03-01

    Einstein field equations for a static and spherically symmetric perfect fluid are considered. A formulation given by Patino and Rago is used to obtain a class of nine solutions, two of them are Tolman solutions I, IV and the remaining seven are new. The solutions are the correct ones corresponding to expressions derived by Patino and Rago which have been shown by Knutsen to be incorrect. Similar to Tolan solution IV each of the new solutions satisfies energy conditions inside a sphere in some range of two independent parameters. Besides, each solution could be matched to the exterior Schwarzschild solution at a boundary where the pressure vanishes and thus the solutions constitute a class of new physically reasonable stellar models.

  12. Stellar parametrization from Gaia RVS spectra

    Science.gov (United States)

    Recio-Blanco, A.; de Laverny, P.; Allende Prieto, C.; Fustes, D.; Manteiga, M.; Arcay, B.; Bijaoui, A.; Dafonte, C.; Ordenovic, C.; Ordoñez Blanco, D.

    2016-01-01

    Context. Among the myriad of data collected by the ESA Gaia satellite, about 150 million spectra will be delivered by the Radial Velocity Spectrometer (RVS) for stars as faint as GRVS~ 16. A specific stellar parametrization will be performed on most of these RVS spectra, I.e. those with enough high signal-to-noise ratio (S/N), which should correspond to single stars that have a magnitude in the RVS band brighter than ~14.5. Some individual chemical abundances will also be estimated for the brightest targets. Aims: We describe the different parametrization codes that have been specifically developed or adapted for RVS spectra within the GSP-Spec working group of the analysis consortium. The tested codes are based on optimisation (FERRE and GAUGUIN), projection (MATISSE), or pattern-recognition methods (Artificial Neural Networks). We present and discuss each of their expected performances in the recovered stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity) for B- to K-type stars. The performances for determining of [α/Fe] ratios are also presented for cool stars. Methods: Each code has been homogeneously tested with a large grid of RVS simulated synthetic spectra of BAFGK-spectral types (dwarfs and giants), with metallicities varying from 10-2.5 to 10+ 0.5 the solar metallicity, and taking variations of ±0.4 dex in the composition of the α-elements into consideration. The tests were performed for S/N ranging from ten to 350. Results: For all the stellar types we considered, stars brighter than GRVS~ 12.5 are very efficiently parametrized by the GSP-Spec pipeline, including reliable estimations of [α/Fe]. Typical internal errors for FGK metal-rich and metal-intermediate stars are around 40 K in Teff, 0.10 dex in log(g), 0.04 dex in [M/H], and 0.03 dex in [α/Fe] at GRVS = 10.3. They degrade to 155 K in Teff, 0.15 dex in log(g), 0.10 dex in [M/H], and 0.1 dex in [α/Fe] at GRVS~ 12. Similar accuracies in Teff and [M/H] are

  13. STRESS - STEREO TRansiting Exoplanet and Stellar Survey

    Science.gov (United States)

    Sangaralingam, Vinothini; Stevens, Ian R.; Spreckley, Steve; Debosscher, Jonas

    2010-02-01

    The Heliospheric Imager (HI) instruments on board the two STEREO (Solar TErrestrial RElations Observatory) spacecraft provides an excellent opportunity for space based stellar photometry. The HI instruments provide a wide area coverage (20° × 20° for the two HI-1 instruments and 70° × 70° for the two HI-2 instruments) and long continuous periods of observations (20 days and 70 days respectively). Using HI-1A which has a pass band of 6500Å to 7500Å and a cadence of 40 minutes, we have gathered photometric information for more than a million stars brighter than 12th magnitude for a period of two years. Here we present some early results from this study on a range of variable stars and the future prospects for the data.

  14. Habitable zone dependence on stellar parameter uncertainties

    International Nuclear Information System (INIS)

    Kane, Stephen R.

    2014-01-01

    An important property of exoplanetary systems is the extent of the Habitable Zone (HZ), defined as that region where water can exist in a liquid state on the surface of a planet with sufficient atmospheric pressure. Both ground- and space-based observations have revealed a plethora of confirmed exoplanets and exoplanetary candidates, most notably from the Kepler mission using the transit detection technique. Many of these detected planets lie within the predicted HZ of their host star. However, as is the case with the derived properties of the planets themselves, the HZ boundaries depend on how well we understand the host star. Here we quantify the uncertainties of HZ boundaries on the parameter uncertainties of the host star. We examine the distribution of stellar parameter uncertainties from confirmed exoplanet hosts and Kepler candidate hosts and translate these into HZ boundary uncertainties. We apply this to several known systems with an HZ planet to determine the uncertainty in their HZ status.

  15. Habitable zone dependence on stellar parameter uncertainties

    Energy Technology Data Exchange (ETDEWEB)

    Kane, Stephen R., E-mail: skane@sfsu.edu [Department of Physics and Astronomy, San Francisco State University, 1600 Holloway Avenue, San Francisco, CA 94132 (United States)

    2014-02-20

    An important property of exoplanetary systems is the extent of the Habitable Zone (HZ), defined as that region where water can exist in a liquid state on the surface of a planet with sufficient atmospheric pressure. Both ground- and space-based observations have revealed a plethora of confirmed exoplanets and exoplanetary candidates, most notably from the Kepler mission using the transit detection technique. Many of these detected planets lie within the predicted HZ of their host star. However, as is the case with the derived properties of the planets themselves, the HZ boundaries depend on how well we understand the host star. Here we quantify the uncertainties of HZ boundaries on the parameter uncertainties of the host star. We examine the distribution of stellar parameter uncertainties from confirmed exoplanet hosts and Kepler candidate hosts and translate these into HZ boundary uncertainties. We apply this to several known systems with an HZ planet to determine the uncertainty in their HZ status.

  16. Physics issues of compact drift optimized stellarators

    International Nuclear Information System (INIS)

    Spong, D.A.; Hirshman, S.; Berry, L.A.

    2001-01-01

    Physics issues are discussed for compact stellarator configurations which achieve good confinement by the fact that the magnetic field modulus, vertical bar B vertical bar, in magnetic coordinates is dominated by poloidally symmetric components. Two distinct configuration types are considered: (1) those which achieve their drift optimization and rotational transform at low β and low bootstrap current by appropriate plasma shaping; and (2) those which have a greater reliance on plasma β and bootstrap currents for supplying the transform and obtaining quasi poloidal symmetry. Stability analysis of the latter group of devices against ballooning, kink and vertical displacement modes has indicated that stable 's on the order of 15% are possible. The first class of devices is being considered for a low β near-term experiment that could explore some of the confinement features of the high beta configurations. (author)

  17. Free-boundary stability of straight stellarators

    International Nuclear Information System (INIS)

    Barnes, D.C.; Cary, J.R.

    1984-02-01

    The sharp-boundary model is used to investigate the stability of straight stellarators to free-boundary, long-wavelength modes. To correctly analyze the heliac configuration, previous theory is generalized to the case of arbitrary helical aspect ratio (ratio of plasma radius to periodicity lengths). A simple low-β criterion involving the vacuum field and the normalized axial current is derived and used to investigate a large variety of configurations. The predictions of this low-β theory are verified by numerical minimization of deltaW at arbitrary β. The heliac configuration is found to be remarkably stable, with a critical β of over 15% determined by the lack of equilibrium rather than the onset of instability. In addition, other previously studied systems are found to be stabilized by net axial plasma current

  18. Retrieving cirrus microphysical properties from stellar aureoles

    Science.gov (United States)

    DeVore, J. G.; Kristl, J. A.; Rappaport, S. A.

    2013-06-01

    The aureoles around stars caused by thin cirrus limit nighttime measurement opportunities for ground-based astronomy, but can provide information on high-altitude ice crystals for climate research. In this paper we attempt to demonstrate quantitatively how this works. Aureole profiles can be followed out to ~0.2° from stars and ~0.5° from Jupiter. Interpretation of diffracted starlight is similar to that for sunlight, but emphasizes larger particles. Stellar diffraction profiles are very distinctive, typically being approximately flat out to a critical angle followed by gradually steepening power-law falloff with slope less steep than -3. Using the relationship between the phase function for diffraction and the average Fourier transform of the projected area of complex ice crystals, we show that defining particle size in terms of average projected area normal to the propagation direction of the starlight leads to a simple, analytic approximation representing large-particle diffraction that is nearly independent of crystal habit. A similar analytic approximation for the diffraction aureole allows it to be separated from the point spread function and the sky background. Multiple scattering is deconvolved using the Hankel transform leading to the diffraction phase function. Application of constrained numerical inversion to the phase function then yields a solution for the particle size distribution in the range between ~50 μm and ~400 μm. Stellar aureole measurements can provide one of the very few, as well as least expensive, methods for retrieving cirrus microphysical properties from ground-based observations.

  19. Stellar Interlopers Caught Speeding Through Space

    Science.gov (United States)

    2009-01-01

    [figure removed for brevity, see original site] [figure removed for brevity, see original site] [figure removed for brevity, see original site] [figure removed for brevity, see original site] Figure 1 Figure 2 Figure 3 Figure 4 Click on individual image for larger view Resembling comets streaking across the sky, these four speedy stars are plowing through regions of dense interstellar gas and creating brilliant arrowhead structures and trailing tails of glowing gas. These bright arrowheads, or bow shocks, can be seen in these four images taken with NASA's Hubble Space Telescope. The bow shocks form when the stars' powerful stellar winds, streams of matter flowing from the stars, slam into surrounding dense gas. The phenomenon is similar to that seen when a speeding boat pushes through water on a lake. The stars in these images are among 13 runaway stars spotted by Hubble's Advanced Camera for Surveys. The stars appear to be young, just millions of years old. Their ages are based on their colors and the presence of strong stellar winds, a signature of youthful stars. Depending on their distance from Earth, the bullet-nosed bow shocks could be 100 billion to a trillion miles wide (the equivalent of 17 to 170 solar system diameters, measured out to Neptune's orbit). The bow shocks indicate that the stars are moving fast, more than 180,000 kilometers an hour (more than 112,000 miles an hour) with respect to the dense gas they are plowing through. They are traveling roughly five times faster than typical young stars, relative to their surroundings. The high-speed stars have traveled far from their birth places. Assuming their youthful phase lasts only a million years and they are moving at roughly 180,000 kilometers an hour, the stars have journeyed 160 light-years. The Hubble observations were taken between October 2005 and July 2006.

  20. Rapid mass segregation in small stellar clusters

    Science.gov (United States)

    Spera, Mario; Capuzzo-Dolcetta, Roberto

    2017-12-01

    In this paper we focus our attention on small-to-intermediate N-body systems that are, initially, distributed uniformly in space and dynamically `cool' (virial ratios Q=2T/|Ω| below ˜0.3). In this work, we study the mass segregation that emerges after the initial violent dynamical evolution. At this scope, we ran a set of high precision N-body simulations of isolated clusters by means of HiGPUs, our direct summation N-body code. After the collapse, the system shows a clear mass segregation. This (quick) mass segregation occurs in two phases: the first shows up in clumps originated by sub-fragmentation before the deep overall collapse; this segregation is partly erased during the deep collapse to re-emerge, abruptly, during the second phase, that follows the first bounce of the system. In this second stage, the proper clock to measure the rate of segregation is the dynamical time after virialization, which (for cold and cool systems) may be significantly different from the crossing time evaluated from initial conditions. This result is obtained for isolated clusters composed of stars of two different masses (in the ratio mh/ml=2), at varying their number ratio, and is confirmed also in presence of a massive central object (simulating a black hole of stellar size). Actually, in stellar systems starting their dynamical evolution from cool conditions, the fast mass segregation adds to the following, slow, secular segregation which is collisionally induced. The violent mass segregation is an effect persistent over the whole range of N (128 ≤ N ≤1,024) investigated, and is an interesting feature on the astronomical-observational side, too. The semi-steady state reached after virialization corresponds to a mass segregated distribution function rather than that of equipartition of kinetic energy per unit mass as it should result from violent relaxation.

  1. Accretion onto stellar mass black holes

    Science.gov (United States)

    Deegan, Patrick

    2009-12-01

    I present work on the accretion onto stellar mass black holes in several scenarios. Due to dynamical friction stellar mass black holes are expected to form high density cusps in the inner parsec of our Galaxy. These compact remnants may be accreting cold dense gas present there, and give rise to potentially observable X-ray emission. I build a simple but detailed time-dependent model of such emission. Future observations of the distribution and orbits of the gas in the inner parsec of Sgr A* will put tighter constraints on the cusp of compact remnants. GRS 1915+105 is an LMXB, whose large orbital period implies a very large accretion disc and explains the extraordinary duration of its current outburst. I present smoothed particle hydrodynamic simulations of the accretion disc. The models includes the thermo-viscous instability, irradiation from the central object and wind loss. I find that the outburst of GRS 1915+105 should last a minimum of 20 years and up to ˜ 100 years if the irradiation is playing a significant role in this system. The predicted recurrence times are of the order of 104 years, making the duty cycle of GRS 1915+105 to be a few 0.1%. I present a simple analytical method to describe the observable behaviour of long period black hole LMXBs, similar to GRS 1915+105. Constructing two simple models for the surface density in the disc, outburst and quiescence times are calculated as a function of orbital period. LMXBs are an important constituent of the X-ray light function (XLF) of giant elliptical galaxies. I find that the duty cycle can vary considerably with orbital period, with implications for modelling the XLF.

  2. Exoplanet Transits of Stellar Active Regions

    Science.gov (United States)

    Giampapa, Mark S.; Andretta, Vincenzo; Covino, Elvira; Reiners, Ansgar; Esposito, Massimiliano

    2018-01-01

    We report preliminary results of a program to obtain high spectral- and temporal-resolution observations of the neutral helium triplet line at 1083.0 nm in transiting exoplanet systems. The principal objective of our program is to gain insight on the properties of active regions, analogous to solar plages, on late-type dwarfs by essentially using exoplanet transits as high spatial resolution probes of the stellar surface within the transit chord. The 1083 nm helium line is a particularly appropriate diagnostic of magnetized areas since it is weak in the quiet photosphere of solar-type stars but appears strongly in absorption in active regions. Therefore, during an exoplanet transit over the stellar surface, variations in its absorption equivalent width can arise that are functions of the intrinsic strength of the feature in the active region and the known relative size of the exoplanet. We utilized the Galileo Telescope and the GIANO-B near-IR echelle spectrograph to obtain 1083 nm spectra during transits in bright, well-known systems that include HD 189733, HD 209458, and HD 147506 (HAT-P-2). We also obtained simultaneous auxiliary data on the same telescope with the HARPS-N UV-Visible echelle spectrograph. We will present preliminary results from our analysis of the observed variability of the strength of the He I 1083 nm line during transits.Acknowledgements: Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. The NSO is operated by AURA under a cooperative agreement with the NSF.

  3. La Corte Constitucional colombiana ante las medidas de seguridad y defensa nacional del gobierno de Uribe

    Directory of Open Access Journals (Sweden)

    Miguel Revenga-Sánchez

    2010-03-01

    Full Text Available En este trabajo se describen las medidas de seguridad y defensa nacional impulsadas por el gobierno de Álvaro Uribe durante la vigencia del Estado de conmoción interior, así como el posicionamiento que la Corte Constitucional ha adoptado sobre estas, en ejercicio de su función de control de constitucionalidad. La negativa reiterada de la Alta Corte a dar su visto bueno a determinados preceptos restrictivos de los derechos fundamentales ha provocado que el Ejecutivo colombiano imponga el estatuto antiterrorista como parte del programa de seguridad democrática que lidera, mediante una reforma constitucional que es analizada en el presente artículo.

  4. IMPACTOS DE LAS CARRETERAS SOBRE LA FAUNA SILVESTRE Y SUS PRINCIPALES MEDIDAS DE MANEJO

    Directory of Open Access Journals (Sweden)

    María del Pilar Arroyave

    Full Text Available El objetivo de este artículo es presentar el impacto de los proyectos viales sobre la fauna silvestre y evaluar las medidas de manejo de estos efectos. Se revisó y analizó la información de diversos estudios realizados en el mundo, al igual que algunos estudios de impacto ambiental de carreteras que se han desarrollado en Antioquia. Se encontró que los principales impactos son el atropellamiento, el aislamiento de poblaciones y el cambio en los patrones reproductivos de la fauna; esto trae como consecuencia la disminución de las poblaciones de especies de fauna silvestre. También se plantean las estrategias comúnmente implementadas para el manejo de los impactos.

  5. Assessment of global stellarator confinement: Status of the international stellarator confinement scaling data base

    International Nuclear Information System (INIS)

    Dinklage, A.; Beidler, C.D.; Dose, V.; Geiger, J.; Kus, A.; Preuss, R.; Ascasibar, E.; Tribaldos, V.; Harris, J.H.; Murakami, S.; Sano, F.; Okamura, S.; Suzuki, Y.; Watanabe, K.Y.; Yamada, H.; Yokoyama, M.; Stroth, U.; Talmadge, J.

    2005-01-01

    Different stellarator/heliotron devices along with their respective flexibility cover a large magnetic configuration space. Since the ultimate goal of stellarator research aims at an alternative fusion reactor concept, the exploration of the most promising configurations requires a comparative assessment of the plasma performance and how different aspects of a 3D configuration influence it. Therefore, the International Stellarator Confinement Database (ISCDB) has been re- initiated in 2004 and the ISS95 database has been extended to roughly 3000 discharges from eight different devices. Further data-sets are continuously added. A revision of a data set restricted to comparable scenarios lead to the ISS04 scaling law which confirmed ISS95 but also revealed clearly the necessity to incorporate configuration descriptive parameters. In other words, an extension beyond the set of regression parameters used for ISS95/ISS04 appears to be necessary and candidates, such as the elongation are investigated. Since grouping of data is a key-issue for deriving ISS04, basic assumptions are revised, e.g. the dependence on the heating scheme. Moreover, an assessment of statistical approaches is investigated with respect to their impact on the scaling. A crucial issue is the weighting of data groups which is discussed in terms of error-in-variable techniques and Bayesian model comparison. The latter is employed for testing scaling ansatzes depending on scaling invariance principles hence allowing the assessment of applicability of theory-based scaling laws on stellarator confinement. 1. ISCDB resources are jointly hosted by NIFS and IPP, see http://iscdb.nifs.ac.jp and http://www.ipp.mpg.de/ISS. (author)

  6. Adaptacao transcultural e confiabilidade de medidas de caracteristicas autorreferidas de vizinhanca no ELSA-Brasil

    Directory of Open Access Journals (Sweden)

    Simone M Santos

    2013-06-01

    Full Text Available OBJETIVO: Descrever o processo de adaptação de escalas de medida de características de vizinhança para o português brasileiro. MÉTODOS: As dimensões abordadas foram coesão social, ambiente propício para atividade física, disponibilidade de alimentos saudáveis, segurança em relação a crimes, violência percebida e vitimização. No processo de adaptação foram avaliados aspectos de equivalência entre as escalas originais e respectivas versões para o português. A confiabilidade teste-reteste foi avaliada em submostra de 261 participantes do Estudo Longitudinal de Saúde do Adulto (ELSA-Brasil que responderam ao mesmo questionário em dois momentos distintos em um intervalo de tempo de sete a 14 dias entre as duas aplicações. RESULTADOS: Os aspectos de equivalência avaliados mostraram-se adequados. O coeficiente de correlação intraclasse variou entre 0,83 (IC95% 0,78;0,87 para Coesão Social e 0,90 (IC95% 0,87;0,92 para Ambiente para Atividade Física. As escalas apresentaram consistência interna (alfa de Cronbach que variaram entre 0,60 e 0,84. CONCLUSÕES: As medidas autorreferidas de características de vizinhança tiveram reprodutibilidade muito boa e boa consistência interna. Os resultados sugerem que essas escalas podem ser utilizadas em estudos com população brasileira que apresente características similares àquelas do ELSA-Brasil.

  7. Contribuciones tecnicas para la medida de la contaminacion electromagnetica de microondas. Estudio en diversas poblaciones

    Science.gov (United States)

    Segura Garcia, Jaume

    La contaminacion ambiental por campos electromagneticos ha resultado ser en estos ultimos anos uno de los problemas mas acuciantes del panorama tecnologico y de salud publica. En el primero de los casos porque las inversiones realizadas son enormes y en el segundo porque cada vez es mayor el numero de articulos, "technical reports" e informes medicos que afirman la existencia de una cierta causalidad, aunque sea debil, entre los campos electromagneticos y ciertos cuadros sintomatologicos. En nuestro caso, hemos dedicado bastantes esfuerzos a investigar el llamado "sindrome de radiofrecuencia / microondas", denominado asi en la literatura cientifica por presentarse en operarios de estaciones de radar y en trabajadores de potentes emisoras de radio y television. En esta memoria presentamos un resumen del trabajo realizado durante los ultimos anos en la medida de la contaminacion electromagnetica ambiental asociado a las comunicaciones inalambricas. En ella se recogen los fundamentos fisicos y propiedades de las ondas electromagneticas, la tecnologia empleada en los sistemas de telefonia celular y los antecedentes relativos a la investigacion de la interaccion de las ondas electromagneticas con organismos vivos. Se desarrolla un procedimiento de medida que ha conducido a la elaboracion de los primeros "mapas de radiofrecuencia" similares, en el aspecto descriptivo, a los mapas de ruido desarrollados en el area de la contaminacion acustica. Por ultimo, se analiza la respuesta subjetiva de los residentes, personas que viven en el entorno de cobertura de las estaciones base de telefonia movil y que se ven sometidos a determinados niveles de radiacion electromagnetica, con el fin de situar este fenomeno al nivel que le corresponde en el ambito de la respuesta subjetiva ciudadana.

  8. Sentidos da trajetória de vida para adolescentes em medida de liberdade assistida

    Directory of Open Access Journals (Sweden)

    Clara Costa Gomes

    2014-03-01

    Full Text Available O presente artigo trata de uma pesquisa que teve como objetivo compreender os sentidos atribuídos por adolescentes que cumpriam medida socioeducativa de liberdade assistida às trajetórias de vida e ao envolvimento com infrações à lei. Foram realizados sete sociodramas semanais com 21 adolescentes da comunidade, dos quais 18 eram do sexo masculino. As informações foram organizadas com base no modelo construtivo-interpretativo de González-Rey e analisadas à luz do aporte teórico da Psicossociologia. Da análise resultaram três zonas de sentido: 1 "Parecia uma vida fácil" - referente à sedução do mundo do crime; 2 "Minhas tábuas de salvação" - sobre as estratégias usadas ante os infortúnios da incursão infracional; 3 "A vida no crime não compensa" - concernente ao saldo das escolhas: dores, perdas e arrependimento. As discussões dos encontros desencadearam nos adolescentes relatos acerca do passado, presente e futuro e reflexões que conduzem à reconstrução de projetos de vida desvinculados de atos de infração. Concluiu-se que os métodos socionômico e de história de vida favoreceram a produção de sentidos pelos adolescentes a partir de sua proposta de ação e reflexão e forneceram informações relevantes para se compreender a trajetória infracional dos adolescentes, constituindo-se em poderosa ferramenta de pesquisa-intervenção junto a adolescentes em cumprimento de medidas socioeducativas.

  9. Direct UV/Optical Imaging of Stellar Surfaces: The Stellar Imager (SI) Vision Mission

    Science.gov (United States)

    Carpenter, Kenneth G.; Lyon, Richard G.; Schrijver, Carolus; Karovska, Margarita; Mozurkewich, David

    2007-01-01

    The Stellar Imager (SI) is a UV/optical, space-based interferometer designed to enable 0.1 milli-arcsecond (mas) spectral imaging of stellar surfaces and, via asteroseismology, stellar interiors and of the Universe in general. SI's science focuses on the role of magnetism in the Universe, particularly on magnetic activity on the surfaces of stars like the Sun. SI's prime goal is to enable long-term forecasting of solar activity and the space weather that it drives, in support of the Living with a Star program in the Exploration Era. SI will also revolutionize our understanding of the formation of planetary systems, of the habitability and climatology of distant planets, and of many magneto-hydrodynamically controlled processes in thc Universe. SI is a "Flagship and Landmark Discovery Mission" in the 2005 Sun Solar System Connection (SSSC) Roadmap and a candidate for a "Pathways to Life Observatory" in the Exploration of the Universe Division (EUD) Roadmap. We discuss herein the science goals of the SI Mission, a mission architecture that could meet those goals, and the technologies needed to enable this mission. Additional information on SI can be found at: http://hires.gsfc.nasa.gov/si/.

  10. Optimización de la medida de conductividad en membranas poliméricas para pilas de combustible

    OpenAIRE

    Espeso González, Iván

    2016-01-01

    El objetivo de este Trabajo de Fin de Grado se centra en la medida de conductividad iónica de membranas poliméricas de intercambio iónico en diferentes celdas de conductividad para poder optimizar este tipo de medidas y evaluar las ventajas e inconvenientes que presenta cada una de las celdas de conductividad utilizadas para poder ser utilizadas con otro tipo de membranas poliméricas utilizadas también como electrolitos sólidos en pilas de combustible. Se han utilizado co...

  11. Inferring probabilistic stellar rotation periods using Gaussian processes

    Science.gov (United States)

    Angus, Ruth; Morton, Timothy; Aigrain, Suzanne; Foreman-Mackey, Daniel; Rajpaul, Vinesh

    2018-02-01

    Variability in the light curves of spotted, rotating stars is often non-sinusoidal and quasi-periodic - spots move on the stellar surface and have finite lifetimes, causing stellar flux variations to slowly shift in phase. A strictly periodic sinusoid therefore cannot accurately model a rotationally modulated stellar light curve. Physical models of stellar surfaces have many drawbacks preventing effective inference, such as highly degenerate or high-dimensional parameter spaces. In this work, we test an appropriate effective model: a Gaussian Process with a quasi-periodic covariance kernel function. This highly flexible model allows sampling of the posterior probability density function of the periodic parameter, marginalizing over the other kernel hyperparameters using a Markov Chain Monte Carlo approach. To test the effectiveness of this method, we infer rotation periods from 333 simulated stellar light curves, demonstrating that the Gaussian process method produces periods that are more accurate than both a sine-fitting periodogram and an autocorrelation function method. We also demonstrate that it works well on real data, by inferring rotation periods for 275 Kepler stars with previously measured periods. We provide a table of rotation periods for these and many more, altogether 1102 Kepler objects of interest, and their posterior probability density function samples. Because this method delivers posterior probability density functions, it will enable hierarchical studies involving stellar rotation, particularly those involving population modelling, such as inferring stellar ages, obliquities in exoplanet systems, or characterizing star-planet interactions. The code used to implement this method is available online.

  12. Nuclear challenges and progress in designing stellarator fusion power plants

    International Nuclear Information System (INIS)

    El-Guebaly, L.A.; Wilson, P.; Henderson, D.; Sawan, M.; Sviatoslavsky, G.; Tautges, T.; Slaybaugh, R.; Kiedrowski, B.; Ibrahim, A.

    2008-01-01

    Over the past 5-6 decades, stellarator power plants have been studied in the US, Europe, and Japan as an alternate to the mainline magnetic fusion tokamaks, offering steady-state operation and eliminating the risk of plasma disruptions. The earlier 1980s studies suggested large-scale stellarator power plants with an average major radius exceeding 20 m. The most recent development of the compact stellarator concept delivered ARIES-CS - a compact stellarator with 7.75 m average major radius, approaching that of tokamaks. For stellarators, the most important engineering parameter that determines the machine size and cost is the minimum distance between the plasma boundary and mid-coil. Accommodating the breeding blanket and necessary shield within this distance to protect the ARIES-CS superconducting magnet represents a challenging task. Selecting the ARIES-CS nuclear and engineering parameters to produce an economic optimum, modeling the complex geometry for 3D nuclear analysis to confirm the key parameters, and minimizing the radwaste stream received considerable attention during the design process. These engineering design elements combined with advanced physics helped enable the compact stellarator to be a viable concept. This paper provides a brief historical overview of the progress in designing stellarator power plants and a perspective on the successful integration of the nuclear activity into the final ARIES-CS configuration

  13. Confinement and heating in modular and continuous coil stellarators

    International Nuclear Information System (INIS)

    Anderson, D.T.; Anderson, F.S.B.; Bonomo, R.L.

    1983-01-01

    Major efforts on the Proto-Cleo stellarator have focused on ICRH of a net current-free plasma, measurements of plasma secondary currents, RF heating by externally induced magnetic reconnection through the formation and destruction of an internal separatrix, and RF current drive experiments. Efforts on the Proto-Cleo torsatron have focused on electron heat conduction. A modular stellarator has been designed and is under fabrication at the University of Wisconsin. The Interchangeable Module Stellarator (IMS) is designed to approximate closely the magnetic properties of the existing Proto-Cleo stellarator as much as possible. Monte-Carlo transport calculations have been made in flux coordinates using model fields patterned after magnetic fields in Proto-Cleo and IMS. Plasma simulation techniques using a 2.5-dimensional particle-in-cell method have been utilized in a numerical search for the bootstrap current. A current is found which is proportional to temperature and density gradients but is independent of poloidal field. The behaviour of charged particles moving in a stellarator under the influence of a steady magnetic field is analysed in terms of the Hamiltonian of the moving particle and the technique of repeated canonical transformations to identify possible adiabatic invariants and drift motions. An improved theory of collisionless particle motion in stellarators has been developed for a family of stellarator configurations. The broad range of configurations encompassed by this family permits an understanding of the differences in numerically observed transport coefficients. Two procedures have been developed to calculate the bootstrap current in non-axisymmetric stellarators. In fully toroidal stellarators the flows and consequent bootstrap current are reduced from their axisymmetric values by a factor of order l slash-l/m in the Pfirsch-Schlueter regime. (author)

  14. Massive Black Hole Implicated in Stellar Destruction

    Science.gov (United States)

    2010-01-01

    New results from NASA's Chandra X-ray Observatory and the Magellan telescopes suggest that a dense stellar remnant has been ripped apart by a black hole a thousand times as massive as the Sun. If confirmed, this discovery would be a cosmic double play: it would be strong evidence for an intermediate mass black hole, which has been a hotly debated topic, and would mark the first time such a black hole has been caught tearing a star apart. This scenario is based on Chandra observations, which revealed an unusually luminous source of X-rays in a dense cluster of old stars, and optical observations that showed a peculiar mix of elements associated with the X-ray emission. Taken together, a case can be made that the X-ray emission is produced by debris from a disrupted white dwarf star that is heated as it falls towards a massive black hole. The optical emission comes from debris further out that is illuminated by these X-rays. The intensity of the X-ray emission places the source in the "ultraluminous X-ray source" or ULX category, meaning that it is more luminous than any known stellar X-ray source, but less luminous than the bright X-ray sources (active galactic nuclei) associated with supermassive black holes in the nuclei of galaxies. The nature of ULXs is a mystery, but one suggestion is that some ULXs are black holes with masses between about a hundred and several thousand times that of the Sun, a range intermediate between stellar-mass black holes and supermassive black holes located in the nuclei of galaxies. This ULX is in a globular cluster, a very old and crowded conglomeration of stars. Astronomers have suspected that globular clusters could contain intermediate-mass black holes, but conclusive evidence for this has been elusive. "Astronomers have made cases for stars being torn apart by supermassive black holes in the centers of galaxies before, but this is the first good evidence for such an event in a globular cluster," said Jimmy Irwin of the University

  15. CCFpams: Atmospheric stellar parameters from cross-correlation functions

    Science.gov (United States)

    Malavolta, Luca; Lovis, Christophe; Pepe, Francesco; Sneden, Christopher; Udry, Stephane

    2017-07-01

    CCFpams allows the measurement of stellar temperature, metallicity and gravity within a few seconds and in a completely automated fashion. Rather than performing comparisons with spectral libraries, the technique is based on the determination of several cross-correlation functions (CCFs) obtained by including spectral features with different sensitivity to the photospheric parameters. Literature stellar parameters of high signal-to-noise (SNR) and high-resolution HARPS spectra of FGK Main Sequence stars are used to calibrate the stellar parameters as a function of CCF areas.

  16. Young Stellar Objects from Soft to Hard X-rays

    Science.gov (United States)

    Güdel, Manuel

    2009-05-01

    Magnetically active stars are the sites of efficient particle acceleration and plasma heating, processes that have been studied in detail in the solar corona. Investigation of such processes in young stellar objects is much more challenging due to various absorption processes. There is, however, evidence for violent magnetic energy release in very young stellar objects. The impact on young stellar environments (e.g., circumstellar disk heating and ionization, operation of chemical networks, photoevaporation) may be substantial. Hard X-ray devices like those carried on Simbol-X will establish a basis for detailed studies of these processes.

  17. The Dark Energy Survey: Prospects for resolved stellar populations

    Energy Technology Data Exchange (ETDEWEB)

    Rossetto, Bruno M. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Santiago, Basílio X. [Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Instituto de Fisica, Porto Alegre (Brazil); Girardi, Léo [Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Osservatorio Astronomica di Padova-INAF, Padova (Italy); Camargo, Julio I. B. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Balbinot, Eduardo [Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Instituto de Fisica, Porto Alegre (Brazil); da Costa, Luiz N. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Yanny, Brian [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Maia, Marcio A. G. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Makler, Martin [Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro (Brazil); Ogando, Ricardo L. C. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Pellegrini, Paulo S. [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Ramos, Beatriz [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); de Simoni, Fernando [Observatorio Nacional, Rio de Janeiro (Brazil); Lab. Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro (Brazil); Armstrong, R. [Univ. of Illinois, Urbana, IL (United States); Bertin, E. [Univ. Pierre et Marie Curie, Paris (France); Desai, S. [Univ. of Illinois, Urbana, IL (United States); Kuropatkin, N. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lin, H. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Mohr, J. J. [Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany); Tucker, D. L. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

    2011-05-06

    Wide angle and deep surveys, regardless of their primary purpose, always sample a large number of stars in the Galaxy and in its satellite system. We here make a forecast of the expected stellar sample resulting from the Dark Energy Survey and the perspectives that it will open for studies of Galactic structure and resolved stellar populations in general. An estimated 1.2 x 108 stars will be sampled in DES grizY filters in the southern equatorial hemisphere. This roughly corresponds to 20% of all DES sources. Most of these stars belong to the stellar thick disk and halo of the Galaxy.

  18. The fluctuation theory of the stellar mass loss

    International Nuclear Information System (INIS)

    Andriesse, C.D.

    1981-01-01

    The idea that fluctuations in the mass flow are as significant as the very existence of the flow has led to the development of a fluctuation theory of the stellar mass loss. A general theory for fluctuations in non-equilibrium systems - and such are stellar atmospheres - was developed long ago. In developing the general theory to a specific stellar theory, however, the arguments have not come up in their logical order. The present sketch of this theory improves on that order and is offered as a framework for further study. (Auth.)

  19. La primera migración laboral en las poblaciones rurales del sur de Veracruz, México

    Directory of Open Access Journals (Sweden)

    Alberto DEL-REY-POVEDA

    2010-01-01

    Full Text Available El objetivo de este trabajo es analizar los determinantes que han afectado a la primera migración laboral de las poblaciones rurales situadas en el sur del estado de Veracruz. Utilizando la Encuesta sobre Movilidad y Reproducción Social en la Región del Sotavento (Moreso realizada en 1999 se ha aplicado un modelo de supervivencia en tiempo discreto a tres generaciones de hombres: nacidos antes de 1950, nacidos entre 1950 y 1969 y nacidos a partir de 1970. Los resultados señalan diferentes riesgos y determinantes para cada una de las generaciones como consecuencia del cambiante contexto laboral en la región y en particular, de la disponibilidad de tierra agrícola.

  20. Morfología de la primera zoea de los cangrejos marinos Petrolisthes haigae y P. nobilii (Decapoda: Porcellanidae

    Directory of Open Access Journals (Sweden)

    Gonzalo Hernández

    2007-12-01

    Full Text Available Los "cangrejos porcelana" Petrolisthes haigae Chace 1962 y P. nobilii Haig 1960, son especies de aguas poco profundas distribuidas a lo largo de las costas del Pacífico Este Tropical. Recolectamos larvas de ambas especies, de ocho y cuatro hembras, en las islas de Taboga y Naos, respectivamente. Las criamos en el laboratorio para describir e ilustrar los primeros estados de zoea de estas especies fueron, hasta ahora desconocidos. Las comparamos con los primeros estadios de zoea de otras especies del género en el oeste de Panamá y concluimos que las características de la primera zoea de ambas especies se asemejan a las del grupo 4 de larvas propuesto por Osawa en 2002.

  1. Redención de la virtud : la primera traducción castellana de "Arte della Guerra" de Maquiavelo

    Directory of Open Access Journals (Sweden)

    Eva Botella Ordinas

    2000-01-01

    Full Text Available La primera traducción al castellano del Arte della guerra de Maquiavelo, publicada en 1536, nunca fue prohibida por la inquisición. En este artículo se argumenta que la razón es que Diego de Salazar con su traducción realizó una conversión del lenguaje político del humanismo cívico al de derechos de matriz teológica.The first castillian translation of Machiavelli's Arte della guerra, published in 1536, was never prohibited by the inquisition. It will be shown along this paper how Diego de Salazar, the translator, made this possible by doing a transformation of the original civic humanism political language into a theological-based rights one.

  2. Historiografía latinoamericana de la Primera Guerra Mundial. Los casos de Argentina, México y Colombia

    Directory of Open Access Journals (Sweden)

    Renzo Ramírez Bacca

    2015-01-01

    Full Text Available El texto ofrece una revisión crítica sobre la historiografía latinoamericana en torno a la Primera Guerra Mundial. El autor se concentra en los casos de Argentina, México y Colombia para rendir cuenta de las líneas de trabajo, categorías de análisis y aportes recientes sobre la problemática. Tiene en cuenta de igual modo, el contexto historiográfico occidental, pone en discusión y dialoga con los estudios recientes, del mismo modo como advierte sobre sus limitaciones, y el porqué de los vacíos historiográficos señalados.

  3. COMPORTAMIENTO DE LOS PRECIOS DEL GANADO HEMBRA DE LEVANTE DE PRIMERA CLASE EN MONTERÍA Y SINCELEJO (COLOMBIA

    Directory of Open Access Journals (Sweden)

    OMAR ENRIQUE CASTILLO NUÑEZ

    2008-01-01

    precios del ganado hembra vivo de levante de primera calidad en las ciudades de Montería y Sincelejo, comercializado en las subastas. Para ello se acude al análisis de los precios durante el periodo 1997-2008 utilizando técnicas estadísticas y económetricas como la media móvil multiplicativa, la tasa de crecimiento sobre medias anuales y modelos generalizados auto-regresivos condicionales heterocedásticos, GARCH. Los resultados indican la presencia de estacionalidad y ciclos en los precios mensuales; en los precios semanales hay evidencias de volatilidad, lo cual genera riesgos para la inversión ganadera en el largo plazo y torna impredecibles su evolución.

  4. Los cambios socio-económicos y el medio ambiente: Cuba. Primera mitad del siglo XIX

    Directory of Open Access Journals (Sweden)

    Opatrný, Josef

    1996-08-01

    Full Text Available The explosive development of Cuba´s sugar industry in the 1 st half of the 19th century had a profound effect on the environment. First among the white creoles' concerns was the rapid deforestation. Many of them, however, also objected to the industry's growth on the grounds that it was causing a substantial increase of the black population on the island.

    El gran desarrollo de la industria azucarera en Cuba en la primera mitad del siglo XIX influyó de forma decisiva en el medio ambiente. La demanda acuciante de madera y de mano de obra esclava para los ingenios pasaron a ser el tema de preocupación entre algunos criollos de la élite. Ambos problemas aparecen unidos en sus peticiones para frenar la deforestación.

  5. Intergalactic stellar populations in intermediate redshift clusters

    Science.gov (United States)

    Melnick, J.; Giraud, E.; Toledo, I.; Selman, F.; Quintana, H.

    2012-11-01

    A substantial fraction of the total stellar mass in rich clusters of galaxies resides in a diffuse intergalactic component usually referred to as the intracluster light (ICL). Theoretical models indicate that these intergalactic stars originate mostly from the tidal interaction of the cluster galaxies during the assembly history of the cluster, and that a significant fraction of these stars could have formed in situ from the late infall of cold metal-poor gas clouds on to the cluster. However, these models also overpredict the fraction of stellar mass in the ICL by a substantial margin, something that is still not well understood. The models also make predictions about the age distribution of the ICL stars, which may provide additional observational constraints. Here we present population synthesis models for the ICL of an intermediate redshift (z = 0.29) X-ray cluster that we have extensively studied in previous papers. The advantage of observing intermediate redshift clusters rather than nearby ones is that the former fit the field of view of multi-object spectrographs in 8-m telescopes and therefore permit us to encompass most of the ICL with only a few well-placed slits. In this paper we show that by stacking spectra at different locations within the ICL it is possible to reach sufficiently high signal-to-noise ratios to fit population synthesis models and derive meaningful results. The models provide ages and metallicities for the dominant populations at several different locations within the ICL and the brightest cluster galaxies (BCG) halo, as well as measures of the kinematics of the stars as a function of distance from the BCG. We thus find that the ICL in our cluster is dominated by old metal-rich stars, at odds with what has been found in nearby clusters where the stars that dominate the ICL are old and metal poor. While we see weak evidence of a young, metal-poor component, if real, these young stars would amount to less than 1 per cent of the total ICL

  6. Ciencia y público en la ciudad de México en la primera mitad del siglo XIX

    Directory of Open Access Journals (Sweden)

    Azuela Bernal, Luz Fernanda

    2015-12-01

    Full Text Available In the first half of the Nineteenth Century a large diversity of scientific activities were performed in Mexico City, establishing the foundation of a scientific culture. This paper will analyze its features, revealing the numerous activities of rational entertainment and learned performances that were complemented by the scientific contents of many literary magazines published during that time. As a result, the contents and values of Nineteenth Century science were appropriated by men and women of the middle and upper classes, who extended them into the larger public.Entre 1821 y 1860 la Ciudad de México fue escenario de una gran diversidad de actividades de talante científico en las que participó un público heterogéneo que no estuvo restringido a las élites intelectuales y que estableció las bases de una cultura proclive a todo tipo de ciencias. En este trabajo se examinarán sus rasgos a través de la exposición de las diversas actividades científicas de entretenimiento racional y espectáculos cultos que se ofrecieron en el ámbito urbano y que tuvieron como complemento los contenidos de las ciencias difundidos en las numerosas revistas literarias de la primera mitad de la centuria. De esta manera, tanto hombres como mujeres con ciertos recursos económicos, tiempo libre, instrucción más allá de las primeras letras y hábitos de lectura, tuvieron la oportunidad de acceder a los contenidos y los valores de la ciencia de su tiempo, que ellos mismos extenderían a un público más amplio.

  7. Bayo Azteca, primera variedad mejorada de frijol con resistencia a Apion godmani Wagner Bayo Azteca, first improved bean variety with resistance to Apion godmani Wagner

    OpenAIRE

    Ramón Garza-García; Carmen Jacinto-Hernández; Dagoberto Garza-García

    2010-01-01

    Bayo Azteca, la primera variedad mejorada de frijol (Phaseolus vulgaris L.), con resistencia a una plaga insectil, ha sido obtenida por el programa de frijol del Campo Experimental Valle de México, del Instituto Nacional de Investigaciones Forestales, Agrícolas y Pecuarias por cruzas múltiples, esto involucró un largo proceso de mejora genética. Bayo Azteca es la primera variedad mejorada resistente al picudo del ejote (Apion godmani Wagner), un curculiónido que ataca al frijol en las zonas t...

  8. "Cosechando frutos de esperanza”: sistematización del proyecto sembrando esperanza por la primera infancia de Santa Lucía (Atlántico)

    OpenAIRE

    Vásquez Mejía, Olga Beatriz; Robayo Noreña, Sandra Milena

    2015-01-01

    Tesis (Maestría en Educación y Desarrollo Humano). Universidad de Manizales. Facultad de Ciencias Sociales y Humanas, 2014 Se realizó una sistematización de experiencias educativas a un exitoso proyecto educativo en primera infancia en la región caribe colombiana, identificando y generando comprensiones sobre los aprendizajes que fueron significativos, que transformaron y transformarán prácticas personales, organizacionales e institucionales en los ambientes educativos para la primera inf...

  9. Propuesta proyecto pedagógico de educación para la primera infancia con enfoque holístico transformador

    OpenAIRE

    Sandoval Castillo, Diana Patricia

    2013-01-01

    El proyecto pedagógico de educación para la primera infancia, se enfocó desde la perspectiva del modelo pedagógico holístico transformador. Se analizaron actividades pedagógicas planeadas por las maestras de los niveles, párvulos, prejardín y jardín, con el fin de proponer una estrategia pedagógica para la educación de la primera infancia teniendo en cuenta las dimensiones del desarrollo corporal cinético, personal social, cognitivo, comunicativo y artístico que transforman y determinan estil...

  10. Manual de atención psicológica a Equipos de primera respuesta especializados en Emergencias pre-hospitalarias, rescates y operaciones en desastres

    OpenAIRE

    Cortez Andrade, Gabriel Eduardo

    2007-01-01

    Los efectos de los desastres sobre la salud física y mental de un equipo de primera respuesta pretenden ser conocidas por medio de este manual, ya que existen secuelas a corto, mediano y largo plazo. Hasta hoy lamentablemente en el Ecuador, no siempre se reconoce los efectos sobre la salud mental en los equipos de primera respuesta, a pesar de haberse demostrado que, en situaciones de desastre y emergencias complejas, se produce un incremento de los signos de sufrimiento psicológico, como la...

  11. Medidas dinámicas de predictibilidad en el índice s&p 500 y sus determinantes

    Directory of Open Access Journals (Sweden)

    Javier Humberto Ospina Holguín

    2015-04-01

    Full Text Available El objeto de este estudio es medir la predictibilidad del índice accionario estadounidense S&P 500 y establecer posibles determinantes de esta predictibilidad. La predictibilidad se ha estudiado ampliamente, pero en pocos casos mediante medidas dinámicas y per se, como se hace aquí. Para establecer la predictibilidad se utilizan la medida eta del campo de las redes neuronales, el valor p del test de la razón de varianzas del campo de la econometría financiera y el análisis de fluctuación sin tendencia del campo de la econofísica. Se construye un algoritmo de inversión basado en las medidas dinámicas de predictibilidad que es mejor que la estrategia de comprar y mantenerse en el periodo estudiado. Para la medida más promisoria, se establece una relación empírica entre la predictibilidad y varios factores económicos y financieros. El panorama que arroja este estudio es el de un mercado que no es estáticamente predecible, sino cuya predictibilidad evoluciona dinámicamente en el tiempo, lo cual es compatible con la hipótesis del mercado adaptativo.

  12. Medidas Sanitarias y Fitosanitarias, ¿Barreras al Comercio?: el Caso Peruano en el Asia-Pacífico

    Directory of Open Access Journals (Sweden)

    Marcelo Alonso Valverde Arevalo

    2016-01-01

    Full Text Available Los aranceles han dejado de representar la principal barrera al comercio exterior, debido a la reducción constante de éstos en el ámbito multilateral o bilateral. Contrariamente, las medidas no arancelarias han ido en aumento, siendo la principal preocupación para las exportaciones mundiales. En este escenario, se presentan las medidas sanitarias y fitosanitarias, las cuales sirven para proteger la salud de las personas, animales y plantas en contra de riesgos asociados con enfermedades, pestes u otros; sin embargo, por la naturaleza de las mismas pueden distorsionar el comercio hasta ser utilizadas con fines proteccionistas en favor de las industrias nacionales de los países importadores. El presente artículo cuestiona si es que a pesar de contar con una serie de acuerdos comerciales internacionales, los cuales han disminuido progresivamente los aranceles, el Perú ha logrado un acceso real al mercado del Asia-Pacífico con productos agropecuarios y pesqueros. En ese sentido, se presentan casos históricos y pendientes en materia de acceso a mercados por medidas de carácter sanitario o fitosanitario, tal como el acceso de paltas a Japón. Asimismo, se analizan las disposiciones de los acuerdos comerciales en materia de medidas sanitarias y fitosanitarias y se presentan las potenciales oportunidades que se establecen en estos acuerdos, a fin de agilizar el acceso a mercados internacionales, y que no se han aprovechado.

  13. As Inundações e Memória Social: Algumas Medidas De Prevenção ...

    African Journals Online (AJOL)

    As Inundações e Memória Social: Algumas Medidas De Prevenção e Controlo da Biodegradação Dos Documentos e Arquivos (Floods and Social Memory: Some Measures for the Protection and Control of Biodegradation in Records and Archives)

  14. Medidas que puede tomar para prevenir el cáncer (Steps You Can Take to Prevent Cancer)

    Centers for Disease Control (CDC) Podcasts

    2012-02-02

    Este podcast habla de las principales medidas que las personas pueden tomar para reducir su riesgo de contraer cáncer.  Created: 2/2/2012 by National Center for Chronic Disease Prevention and Health Promotion (NCCDPHP).   Date Released: 3/13/2012.

  15. Impacto sonoro do aeroporto Santos Dumont/RJ: análise e medidas de controle

    Directory of Open Access Journals (Sweden)

    José R. de Lima Neto

    2014-09-01

    Full Text Available A poluição sonora é parte cotidiana da vida nas grandes cidades. Dentre as fontes sonoras relevantes no contexto das cidades, tais como o ruído viário, uma que oferece desafios particulares é a relacionada ao sobrevoo de aeronaves, sejam aviões comerciais, jatos particulares ou helicópteros. Por se tratar de fontes intensas de ruído e das características das suas trajetórias (extensas e acima das habitações, tanto a avaliação do incômodo gerado, como eventuais medidas de mitigação são complexas e de difícil implementação.Dessa forma, o desconforto acústico gerado nas comunidades próximas as rotas de pouso e decolagem de grandes aeroportos tornou-se alvo de grandes reclamações por parte dos moradores que tem seu conforto ameaçado, o que reforça a necessidade de enfrentar estes desafios e atacar este problema.Assim, nesse trabalho, buscamos avaliar o impacto sonoro das aeronaves que possuem como destino ou são oriundas do aeroporto Santos Dumont/RJ (SBRJ, através de simulação computacional de ruído, em uma região próxima ao aeroporto com área de aproximadamente 39 km². A partir da quantificação e determinação das áreas efetivamente afetadas pelo ruído aeronáutico, e da comparação dos valores obtidos com as normas da legislação brasileira, esse trabalho visa mapear possíveis regiões de conflito e fornecer informações que orientem possíveis medidas mitigadoras e de controle de ruído plausíveis para a realidade atual. Palavras-Chave: Acústica, Ruído aeronáutico, Impacto Sonoro de Aeroportos.

  16. Medidas de biossegurança adotadas por profissionais atuantes em audiologia

    Directory of Open Access Journals (Sweden)

    Ana Paula Ferreira Rocha

    2015-03-01

    Full Text Available OBJETIVO: explicitar as práticas de biossegurança adotadas por fonoaudiólogos atuantes na área de Audiologia e relacioná-las com a educação continuada e o tempo de formação dos profissionais. MÉTODOS: participaram deste estudo 70 fonoaudiólogos atuantes na área de Audiologia, nos municípios de Belo Horizonte e Contagem. Foi aplicado um questionário sobre biossegurança em Audiologia, com base na Norma Regulamentadora 32, composto por 27 perguntas fechadas, abordando os aspectos de higienização das mãos, equipamentos de proteção individual e organização e higienização dos artigos e do ambiente. RESULTADOS: a maioria dos fonoaudiólogos relatou que adota as seguintes medidas de biossegurança: higienização das mãos antes dos atendimentos (71%, uso de jaleco com mangas longas (74% e abotoado (91%, cabelos presos (79%, unhas limpas e cortadas (91%, separação e desinfecção dos artigos usados (83% e organização do ambiente (97%. No entanto somente 40% dos profissionais referiram higienizar as mãos entre os atendimentos e 9% referiram o uso de luvas na realização da meatoscopia. Observou-se que a destinação dos artigos para desinfecção é uma prática mais rotineira para profissionais com especialização (p< 0,05. Os profissionais com maior tempo de formação aderiram melhor à prática de higienização das mãos. CONCLUSÃO: higienizar as mãos antes dos atendimentos, vestir-se corretamente, destinar os artigos para desinfecção e organizar o ambiente de trabalho são práticas de biossegurança adotadas pela maioria dos fonoaudiólogos. Fatores como tempo de formação e educação continuada influenciam de maneira positiva na adoção de corretas medidas de biossegurança.

  17. Un criterio robusto para la medida del margen –coeficiente– de seguridad

    Directory of Open Access Journals (Sweden)

    Cervera, J.

    2010-06-01

    Full Text Available This paper offers a brief analysis of the drawbacks that can be found with the usual partial security coefficients, as loads multipliers, when employed for the measurement of the distance to the collapse condition in such structures, as masonry arches, that have important anisotropies or lacks tensile strength. To deal with such difficulties the paper presents a simple and robust security criterium based on a contraction of the yield surface. That criterium, that performs identically in isotropic structures to those usually employed, can however deal consistently with situations where former criteria fail. The criterium is applied to sections with double symmetry under axial load and unsymmetrical bending, in materials with and without tension resistance. It is also applied to the prism stability problem, showing the advantages in the caracterization of such problems.

    En este trabajo se analizan en primer lugar algunos inconvenientes de los habituales coeficientes parciales de seguridad —factores multiplicadores de las cargas— como medida del alejamiento a las condiciones de colapso en el caso de las estructuras con anisotropías importantes, como son especialmente aquellas sin resistencia a la tracción —los arcos de fábrica, como ejemplo paradigmático— Para superar dichas dificultades se propone un criterio sencillo y robusto basado en la contracción de la superficie límite, criterio que aporta una medida coincidente con la habitual para los casos isótropos, pero que permite medir igualmente de forma consistente el alejamiento a las condiciones del colapso para el resto de las situaciones. Se aplica finalmente el modelo a la determinación de los márgenes de seguridad en secciones de doble simetría sometidas a compresión esviada para materiales sin, y con resistencia a tracción, así como al problema de la estabilidad de un prisma frente al vuelco, mostrando las mejoras que aporta para caracterizar dichos problemas.

  18. TYCHO: Simulating Exoplanets Within Stellar Clusters

    Science.gov (United States)

    Glaser, Joseph Paul; Thornton, Jonathan; Geller, Aaron M.; McMillan, Stephen

    2018-01-01

    Recent surveys exploring nearby open clusters have yielded noticeable differences in the planetary population from that seen in the Field. This is surprising, as the two should be indistinguishable given currently accepted theories on how a majority of stars form within the Galaxy. Currently, the existence of this apparent deficit is not fully understood. While detection bias in previous observational surveys certainly contributes to this issue, the dynamical effects of star-star scattering must also be taken into account. However, this effect can only be investigated via computational simulations and current solutions of the multi-scale N-body problem are limited and drastically simplified.To remedy this, we aim to create a physically complete computational solution to explore the role of stellar close encounters and interplanetary interactions in producing the observed exoplanet populations for both open cluster stars and Field stars. To achieve this, TYCHO employs a variety of different computational techniques, including: multiple n-body integration methods; close-encounter handling; Monte Carlo scattering experiments; and a variety of observationally-backed initial condition generators. Herein, we discuss the current state of the code's implantation within the AMUSE framework and its applications towards present exoplanet surveys.

  19. Grain formation in cool stellar envelopes

    International Nuclear Information System (INIS)

    Deguchi, S.

    1980-01-01

    The nucleation and growth of dust grains in the stellar envelope are investigated for the case of oxygen-rich stars, where the mass loss occurs as a result of the radiation pressure on the dust grains. The number density of grains, the final grain sizes, and the final amount of metals remaining in gaseous states are calculated based on the grain-nucleation theory proposed by Yamamoto and Hasegawa and Draine and Salpeter. It is shown that, even if we base our calculations on the Lothe-Pound nucleation rate equation instead of the classical, homogeneous nucleation rate equation, the proposed theory gives a number density of grains quite similar to that based on the classical rate equation. The approximate solution of the flow, in this paper, brings physical insight to the problem of how the formation of grains couples the flow passing the sonic point. The metals in the outer envelope remain in gaseous state by the amount of 1--10% of the initial content for the mass-loss rate of 10 -5 M/sub sun/ yr -1 and by less than 1% for the massloss are less than 3 x 10 -6 M/sub sun/ yr -1 . Species of metals condensed onto the grains are also discussed

  20. A Bayesian method for detecting stellar flares

    Science.gov (United States)

    Pitkin, M.; Williams, D.; Fletcher, L.; Grant, S. D. T.

    2014-12-01

    We present a Bayesian-odds-ratio-based algorithm for detecting stellar flares in light-curve data. We assume flares are described by a model in which there is a rapid rise with a half-Gaussian profile, followed by an exponential decay. Our signal model also contains a polynomial background model required to fit underlying light-curve variations in the data, which could otherwise partially mimic a flare. We characterize the false alarm probability and efficiency of this method under the assumption that any unmodelled noise in the data is Gaussian, and compare it with a simpler thresholding method based on that used in Walkowicz et al. We find our method has a significant increase in detection efficiency for low signal-to-noise ratio (S/N) flares. For a conservative false alarm probability our method can detect 95 per cent of flares with S/N less than 20, as compared to S/N of 25 for the simpler method. We also test how well the assumption of Gaussian noise holds by applying the method to a selection of `quiet' Kepler stars. As an example we have applied our method to a selection of stars in Kepler Quarter 1 data. The method finds 687 flaring stars with a total of 1873 flares after vetos have been applied. For these flares we have made preliminary characterizations of their durations and and S/N.

  1. Massive stellar content of some Galactic supershells

    Science.gov (United States)

    Kaltcheva, Nadejda; Golev, Valeri

    2015-08-01

    The giant Galactic H II regions provide a unique opportunity to study the OB-star influence on the surrounding interstellar matter. In this contribution, several multi-wavelength surveys (Wisconsin H-α Mapper Northern Sky Survey, Southern H-α Sky Survey Atlas, MSX Mid-IR Galactic Plane Survey, WISE All-Sky Data Release, CO survey of the Milky Way, and the Southern Galactic Plane HI Survey) are combined with available intermediate-band uvbyβ photometry to attempt a precise spatial correlation between the OB-stars and the neutral and ionized material. Our study is focused on the H I supershell GSH 305+01-24 in Centaurus, the Car OB2 supershell, the Cygnus star-forming complex and the GSH 224-01+24 shell toward the GMN 39/Seagull nebula region. We refine the massive stellar content of these star-forming fields and study the energetics of its interaction with the shells’ material.

  2. MiniCNT - A Tabletop Stellarator

    Science.gov (United States)

    Dugan, Chris; Pedersen, Thomas; Berkery, John

    2006-10-01

    MiniCNT is a scaled down version of the Columbia Non-Neutral Torus, a stellarator built to study confinement of non-neutral plasmas on magnetic surfaces. MiniCNT is a glass vacuum chamber capable of holding pressures six orders of magnitude below atmospheric pressure. Unlike CNT, in which plasmas are invisible, MiniCNT allows some collisions with neutrals, causing it to glow. Using two twelve-volt car batteries to power four magnetic coils, MiniCNT generates a 0.02 Tesla magnetic field. While CNT, being larger, is obviously more accurate, there are multiple benefits in MiniCNT. First, it is more flexible and can be adjusted to fit many scenarios easily. The car batteries can be switched for other power sources, the coils can be realigned, and the chamber can be pumped to various pressures of various gases. Also, it is visually accessible; while CNT has glass viewing ports and its plasma is dark, MiniCNT is made of glass and its plasma glows, allowing visualization of the magnetic surfaces.

  3. Theoretical and observational studies of stellar activity

    International Nuclear Information System (INIS)

    Schmitt, J.H.M.M.

    1984-01-01

    In the theoretical part of this thesis, doubly-diffusive MHD instabilities are studied as a means of breaking up a diffuse magnetic field at the bottom of the solar convection zone. The analysis is linear and local, and assumes short meridional wavelengths; the effects of rotation and diffusion of vorticity, magnetic fields and heat are included. Results show that the instability depends sensitively on the temperature stratification, but rather insensitively on the assumed magnetic field configuration; instability time scales considerably less than the solar cycle period can be easily obtained. In the observational part of the thesis, results are reported of a survey of the x-ray emission of stars with shallow connection zones to study the onset of convection and dynamo activity along the main sequence. Complications arising from stellar multiplicity are discussed extensively; it is demonstrated that binaries have statistically higher x-ray luminosities; and it is shown that physical parameters can only be deduced from single stars. It is further shown that the x-ray luminosities of stars with spectral type in the color range 0.1 less than or equal to B. V less than or equal to 0.5 increase rapidly, whereas stars with B. V approx. 0.0 appear to have no intrinsic x-ray emission at presently detectable levels

  4. On neoclassical impurity transport in stellarator geometry

    International Nuclear Information System (INIS)

    García-Regaña, J M; Kleiber, R; Beidler, C D; Turkin, Y; Maaßberg, H; Helander, P

    2013-01-01

    The impurity dynamics in stellarators has become an issue of moderate concern due to the inherent tendency of the impurities to accumulate in the core when the neoclassical ambipolar radial electric field points radially inwards (ion root regime). This accumulation can lead to collapse of the plasma due to radiative losses, and thus limit high performance plasma discharges in non-axisymmetric devices. A quantitative description of the neoclassical impurity transport is complicated by the breakdown of the assumption of small E × B drift and trapping due to the electrostatic potential variation on a flux surface Φ-tilde compared with those due to the magnetic field gradient. This work examines the impact of this potential variation on neoclassical impurity transport in the Large Helical Device heliotron. It shows that the neoclassical impurity transport can be strongly affected by Φ-tilde . The central numerical tool used is the δf particle in cell Monte Carlo code EUTERPE. The Φ-tilde used in the calculations is provided by the neoclassical code GSRAKE. The possibility of obtaining a more general Φ-tilde self-consistently with EUTERPE is also addressed and a preliminary calculation is presented. (paper)

  5. Direct nuclear reaction experiments for stellar nucleosynthesis

    International Nuclear Information System (INIS)

    Cherubini, S.

    2016-01-01

    During the last two decades indirect methods where proposed and used in many experiments in order to measure nuclear cross sections between charged particles at stellar energies. These are among the lowest to be measured in nuclear physics. One of these methods, the Trojan Horse method, is based on the Quasi- Free reaction mechanism and has proved to be particularly flexible and reliable. It allowed for the measurement of the cross sections of various reactions of astrophysical interest using stable beams. The use and reliability of indirect methods become even more important when reactions induced by Radioactive Ion Beams are considered, given the much lower intensity generally available for these beams. The first Trojan Horse measurement of a process involving the use of a Radioactive Ion Beam dealt with the "1"8F(p,α)"1"5O process in Nova conditions. To obtain pieces of information on this process, in particular about its cross section at Nova energies, the Trojan Horse method was applied to the "1"8F(d,α "1"5O)n three body reaction. In order to establish the reliability of the Trojan Horse method approach, the Treiman-Yang criterion is an important test and it will be addressed briefly in this paper.

  6. Technological aspects of the Wega stellarator

    International Nuclear Information System (INIS)

    Fritsch, R.; Ohlendorf, W.; Pacher, G.W.; Pacher, H.D.; Wegrowe, J.G.; Lipa, M.; CEA Centre d'Etudes Nucleaires de Grenoble, 38

    1976-01-01

    Wega, an ohmically heated Stellarator at Grenoble for the study of R.F. heating at high power. On the vacuum vessel are mounted helical windings with periods l=2, m=5, designed to produce a rotational transform of 0.3 at a main field of 2.5T. Calculations to simulate the effect of the stray flux of the transformer yokes show that a vertical field variation of the same periodicity as the helical windings (five-fold symmetry) does not affect the magnetic surfaces. Accordingly five transformer yokes are used. To assemble internal R.F. structures, it was required that the two halves of the device be separable, therefore electrically and mechanically distinct. The 14 helical conductors of the 4 windings of each of the device are placed in series by means of end connections magnetically compensated. To facilitate further the separability of the two halves, one of them, weighing 5 tons (vacuum vessel, toroidal field coils, supporting structures) is supported at three points, and can be displaced horizontally by 3m using an air cushion system [fr

  7. On radiative density limits in stellarators

    International Nuclear Information System (INIS)

    Wobig, H.

    2001-01-01

    Density limits in stellarators are caused mainly by enhanced impurity radiation leading to a collapse of the temperature. A simple model can be established, which computes the temperature in the plasma with a fixed heating profile and a temperature-dependent radiation profile. If the temperature-dependent radiation function has one or several extrema, multiple solutions of the transport equation exist and radiative collapse occurs when the high temperature branch merges with the unstable temperature branch. At this bifurcation point the temperature decreases to a stable low temperature solution. The bifurcation point is a function of the heating power and the plasma density. Thus a density limit can be defined as the point where bifurcation occurs. It is shown that bifurcation and sudden temperature collapse does not occur below a power threshold. Anomalous thermal conductivity and the details of the impurity radiation, which in the present model is assumed to be in corona equilibrium, determine the scaling of the density limit. A model of the anomalous transport is developed, which leads to Gyro-Bohm scaling of the confinement time. The density limit based on this transport model is close to experimental findings in Wendelstein 7-AS. (author)

  8. Survival of planets around shrinking stellar binaries.

    Science.gov (United States)

    Muñoz, Diego J; Lai, Dong

    2015-07-28

    The discovery of transiting circumbinary planets by the Kepler mission suggests that planets can form efficiently around binary stars. None of the stellar binaries currently known to host planets has a period shorter than 7 d, despite the large number of eclipsing binaries found in the Kepler target list with periods shorter than a few days. These compact binaries are believed to have evolved from wider orbits into their current configurations via the so-called Lidov-Kozai migration mechanism, in which gravitational perturbations from a distant tertiary companion induce large-amplitude eccentricity oscillations in the binary, followed by orbital decay and circularization due to tidal dissipation in the stars. Here we explore the orbital evolution of planets around binaries undergoing orbital decay by this mechanism. We show that planets may survive and become misaligned from their host binary, or may develop erratic behavior in eccentricity, resulting in their consumption by the stars or ejection from the system as the binary decays. Our results suggest that circumbinary planets around compact binaries could still exist, and we offer predictions as to what their orbital configurations should be like.

  9. Secular instabilities of Keplerian stellar discs

    Science.gov (United States)

    Kaur, Karamveer; Kazandjian, Mher V.; Sridhar, S.; Touma, Jihad R.

    2018-05-01

    We present idealized models of a razor-thin, axisymmetric, Keplerian stellar disc around a massive black hole, and study non-axisymmetric secular instabilities in the absence of either counter-rotation or loss cones. These discs are prograde mono-energetic waterbags, whose phase-space distribution functions are constant for orbits within a range of eccentricities (e) and zero outside this range. The linear normal modes of waterbags are composed of sinusoidal disturbances of the edges of distribution function in phase space. Waterbags that include circular orbits (polarcaps) have one stable linear normal mode for each azimuthal wavenumber m. The m = 1 mode always has positive pattern speed and, for polarcaps consisting of orbits with e normal modes for each m, which can be stable or unstable. We derive analytical expressions for the instability condition, pattern speeds, growth rates, and normal mode structure. Narrow bands are unstable to modes with a wide range in m. Numerical simulations confirm linear theory and follow the non-linear evolution of instabilities. Long-time integration suggests that instabilities of different m grow, interact non-linearly, and relax collisionlessly to a coarse-grained equilibrium with a wide range of eccentricities.

  10. Stellar Atmospheric Parameterization Based on Deep Learning

    Science.gov (United States)

    Pan, Ru-yang; Li, Xiang-ru

    2017-07-01

    Deep learning is a typical learning method widely studied in the fields of machine learning, pattern recognition, and artificial intelligence. This work investigates the problem of stellar atmospheric parameterization by constructing a deep neural network with five layers, and the node number in each layer of the network is respectively 3821-500-100-50-1. The proposed scheme is verified on both the real spectra measured by the Sloan Digital Sky Survey (SDSS) and the theoretic spectra computed with the Kurucz's New Opacity Distribution Function (NEWODF) model, to make an automatic estimation for three physical parameters: the effective temperature (Teff), surface gravitational acceleration (lg g), and metallic abundance (Fe/H). The results show that the stacked autoencoder deep neural network has a better accuracy for the estimation. On the SDSS spectra, the mean absolute errors (MAEs) are 79.95 for Teff/K, 0.0058 for (lg Teff/K), 0.1706 for lg (g/(cm·s-2)), and 0.1294 dex for the [Fe/H], respectively; On the theoretic spectra, the MAEs are 15.34 for Teff/K, 0.0011 for lg (Teff/K), 0.0214 for lg(g/(cm · s-2)), and 0.0121 dex for [Fe/H], respectively.

  11. Second harmonic electron cyclotron breakdown in stellarators

    International Nuclear Information System (INIS)

    Carter, M.D.; Batchelor, D.B.; England, A.C.

    1987-01-01

    In linear wave-particle interaction models, the coupling between cold electrons and microwaves with frequency equal to twice the electron gyrofrequency is so weak that the ionization of a significant number of neutral hydrogen atoms would seem impossible in practical applications. However, the non-linear interaction of a cold electron with the wave is very large if the electron becomes trapped near resonance in a shallow, static magnetic well. A model has been developed to describe the breakdown of a neutral gas when these non-linear interactions are considered, and it is in reasonable agreement with the limited amount of available experimental data. For gas pressures that are too large, electron-neutral collisions inhibit the non-linear interaction and prevent breakdown. For gas pressures that are too low, the growth rate of the free electron population is limited because electrons capable of causing ionization are lost before suffering a collision with a neutral. Quantitative growth rate predictions are presented for stellarators, and formulae for rough estimates are given. (author)

  12. Stellar 'Incubators' Seen Cooking up Stars

    Science.gov (United States)

    2005-01-01

    [figure removed for brevity, see original site] Figure 1 [figure removed for brevity, see original site] [figure removed for brevity, see original site] Figure 2Figure 3Figure 4Figure 5 This image composite compares visible-light and infrared views from NASA's Spitzer Space Telescope of the glowing Trifid Nebula, a giant star-forming cloud of gas and dust located 5,400 light-years away in the constellation Sagittarius. Visible-light images of the Trifid taken with NASA's Hubble Space Telescope, Baltimore, Md. (inside left, figure 1) and the National Optical Astronomy Observatory, Tucson, Ariz., (outside left, figure 1) show a murky cloud lined with dark trails of dust. Data of this same region from the Institute for Radioastronomy millimeter telescope in Spain revealed four dense knots, or cores, of dust (outlined by yellow circles), which are 'incubators' for embryonic stars. Astronomers thought these cores were not yet ripe for stars, until Spitzer spotted the warmth of rapidly growing massive embryos tucked inside. These embryos are indicated with arrows in the false-color Spitzer picture (right, figure 1), taken by the telescope's infrared array camera. The same embryos cannot be seen in the visible-light pictures (left, figure 1). Spitzer found clusters of embryos in two of the cores and only single embryos in the other two. This is one of the first times that multiple embryos have been observed in individual cores at this early stage of stellar development.

  13. Cool WISPs for stellar cooling excesses

    Energy Technology Data Exchange (ETDEWEB)

    Giannotti, Maurizio [Physical Sciences, Barry University, 11300 NE 2nd Avenue, Miami Shores, FL 33161 (United States); Irastorza, Igor; Redondo, Javier [Departamento de Física Teórica, Universidad de Zaragoza, Pedro Cerbuna 12, E-50009, Zaragoza, España (Spain); Ringwald, Andreas, E-mail: mgiannotti@barry.edu, E-mail: igor.irastorza@cern.ch, E-mail: jredondo@unizar.es, E-mail: andreas.ringwald@desy.de [Theory group, Deutsches Elektronen-Synchrotron DESY, Notkestraße 85, D-22607 Hamburg (Germany)

    2016-05-01

    Several stellar systems (white dwarfs, red giants, horizontal branch stars and possibly the neutron star in the supernova remnant Cassiopeia A) show a mild preference for a non-standard cooling mechanism when compared with theoretical models. This exotic cooling could be provided by Weakly Interacting Slim Particles (WISPs), produced in the hot cores and abandoning the star unimpeded, contributing directly to the energy loss. Taken individually, these excesses do not show a strong statistical weight. However, if one mechanism could consistently explain several of them, the hint could be significant. We analyze the hints in terms of neutrino anomalous magnetic moments, minicharged particles, hidden photons and axion-like particles (ALPs). Among them, the ALP or a massless HP represent the best solution. Interestingly, the hinted ALP parameter space is accessible to the next generation proposed ALP searches, such as ALPS II and IAXO and the massless HP requires a multi TeV energy scale of new physics that might be accessible at the LHC.

  14. Cool WISPs for stellar cooling excesses

    International Nuclear Information System (INIS)

    Giannotti, Maurizio; Irastorza, Igor; Redondo, Javier; Ringwald, Andreas

    2016-01-01

    Several stellar systems (white dwarfs, red giants, horizontal branch stars and possibly the neutron star in the supernova remnant Cassiopeia A) show a mild preference for a non-standard cooling mechanism when compared with theoretical models. This exotic cooling could be provided by Weakly Interacting Slim Particles (WISPs), produced in the hot cores and abandoning the star unimpeded, contributing directly to the energy loss. Taken individually, these excesses do not show a strong statistical weight. However, if one mechanism could consistently explain several of them, the hint could be significant. We analyze the hints in terms of neutrino anomalous magnetic moments, minicharged particles, hidden photons and axion-like particles (ALPs). Among them, the ALP or a massless HP represent the best solution. Interestingly, the hinted ALP parameter space is accessible to the next generation proposed ALP searches, such as ALPS II and IAXO and the massless HP requires a multi TeV energy scale of new physics that might be accessible at the LHC.

  15. Constraints on stellar evolution from pulsations

    International Nuclear Information System (INIS)

    Cox, A.N.

    1983-01-01

    Consideration of the many types of intrinsic variable stars, that is, those that pulsate, reveals that perhaps a dozen classes can indicate some constraints that affect the results of stellar evolution calculations, or some interpretations of observations. Many of these constraints are not very strong or may not even be well defined yet. In this review we discuss only the case for six classes: classical Cepheids with their measured Wesselink radii, the observed surface effective temperatures of the known eleven double-mode Cepheids, the pulsation periods and measured surface effective temperatures of three R CrB variables, the delta Scuti variable VZ Cnc with a very large ratio of its two observed periods, the nonradial oscillations of our sun, and the period ratios of the newly discovered double-mode RR Lyrae variables. Unfortunately, the present state of knowledge about the exact compositions; mass loss and its dependence on the mass, radius, luminosity, and composition; ;and internal mixing processes, as well as sometimes the more basic parameters such as luminosities and surface effective temperatures prevent us from applying strong constraints for every case where currently the possibility exists

  16. Weak-interaction rates in stellar conditions

    Science.gov (United States)

    Sarriguren, Pedro

    2018-05-01

    Weak-interaction rates, including β-decay and electron captures, are studied in several mass regions at various densities and temperatures of astrophysical interest. In particular, we study odd-A nuclei in the pf-shell region, which are involved in presupernova formations. Weak rates are relevant to understand the late stages of the stellar evolution, as well as the nucleosynthesis of heavy nuclei. The nuclear structure involved in the weak processes is studied within a quasiparticle proton-neutron random-phase approximation with residual interactions in both particle-hole and particle-particle channels on top of a deformed Skyrme Hartree-Fock mean field with pairing correlations. First, the energy distributions of the Gamow-Teller strength are discussed and compared with the available experimental information, measured under terrestrial conditions from charge-exchange reactions. Then, the sensitivity of the weak-interaction rates to both astrophysical densities and temperatures is studied. Special attention is paid to the relative contribution to these rates of thermally populated excited states in the decaying nucleus and to the electron captures from the degenerate electron plasma.

  17. Gravitational wave generation by stellar core collapse

    International Nuclear Information System (INIS)

    Moore, T.A.

    1981-01-01

    Stars which have masses greater than 5 to 8 solar masses are thought to undergo a stage of catastrophic core collapse and subsequent supernova explosion at the end of their lives. If the core is not spherically symmetric, the bounce which halts its collapse at transnuclear densities will generate a pulse of gravitational waves. This thesis presents a fully relativistic model of core collapse which treats deviations from spherical symmetry as small perturbations on a spherical background. This model may be used to predict qualitative and quantitative features of the gravitational radiation emitted by stellar cores with odd-parity, axisymmetric fluid perturbations, and represents a first step in the application of perturbative methods to more general asymmetries. The first chapter reviews the present consensus on the physics of core collapse and outlines the important features, assumptions, and limitations of the model. A series of model runs are presented and discussed. Finally, several proposals for future research are presented. Subsequent chapters explore in detail the mathematical features of the present model and its realization on the computer

  18. Predicting gravitational lensing by stellar remnants

    Science.gov (United States)

    Harding, Alexander J.; Stefano, R. Di; Lépine, S.; Urama, J.; Pham, D.; Baker, C.

    2018-03-01

    Gravitational lensing provides a means to measure mass that does not rely on detecting and analysing light from the lens itself. Compact objects are ideal gravitational lenses, because they have relatively large masses and are dim. In this paper, we describe the prospects for predicting lensing events generated by the local population of compact objects, consisting of 250 neutron stars, five black holes, and ≈35 000 white dwarfs. By focusing on a population of nearby compact objects with measured proper motions and known distances from us, we can measure their masses by studying the characteristics of any lensing event they generate. Here, we concentrate on shifts in the position of a background source due to lensing by a foreground compact object. With Hubble Space Telescope, JWST, and Gaia, measurable centroid shifts caused by lensing are relatively frequent occurrences. We find that 30-50 detectable events per decade are expected for white dwarfs. Because relatively few neutron stars and black holes have measured distances and proper motions, it is more difficult to compute realistic rates for them. However, we show that at least one isolated neutron star has likely produced detectable events during the past several decades. This work is particularly relevant to the upcoming data releases by the Gaia mission and also to data that will be collected by JWST. Monitoring predicted microlensing events will not only help to determine the masses of compact objects, but will also potentially discover dim companions to these stellar remnants, including orbiting exoplanets.

  19. STELLAR ACTIVITY IN THE BROADBAND ULTRAVIOLET

    International Nuclear Information System (INIS)

    Findeisen, K.; Hillenbrand, L.; Soderblom, D.

    2011-01-01

    The completion of the GALEX All-Sky Survey in the ultraviolet allows activity measurements to be acquired for many more stars than is possible with the limited sensitivity of ROSAT or the limited sky coverage of Chandra, XMM, or spectroscopic surveys for line emission in the optical or ultraviolet. We have explored the use of GALEX photometry as an activity indicator, using stars within 50 pc as a calibration sample representing the field and in selected nearby associations representing the youngest stages of stellar evolution. We present preliminary relations between UV flux and the optical activity indicator R' HK and between UV flux and age. We demonstrate that far-UV (FUV, 1350-1780 A) excess flux is roughly proportional to R' HK . We also detect a correlation between near-UV (NUV, 1780-2830 A) flux and activity or age, but the effect is much more subtle, particularly for stars older than ∼0.5-1 Gyr. Both the FUV and NUV relations show large scatter, ∼0.2 mag when predicting UV flux, ∼0.18 dex when predicting R' HK , and ∼0.4 dex when predicting age. This scatter appears to be evenly split between observational errors in current state-of-the-art data and long-term activity variability in the sample stars.

  20. Recent Progress in MHD Stability Calculations of Compact Stellarators

    International Nuclear Information System (INIS)

    Fu, G.Y.; Ku, L.P.; Redi, M.H.; Kessel, C.; Monticello, D.A.; Reiman, A.; Cooper, W.A.; Nuehrenberg, C.; Sanchez, R.; Ware, A.; Hirshman, S.P.; Spong, D.A.

    2000-01-01

    A key issue for compact stellarators is the stability of beta-limiting MHD modes, such as external kink modes driven by bootstrap current and pressure gradient. We report here recent progress in MHD stability studies for low-aspect-ratio Quasi-Axisymmetric Stellarators (QAS) and Quasi-Omnigeneous Stellarators (QOS). We find that the N = 0 periodicity-preserving vertical mode is significantly more stable in stellarators than in tokamaks because of the externally generated rotational transform. It is shown that both low-n external kink modes and high-n ballooning modes can be stabilized at high beta by appropriate 3D shaping without a conducting wall. The stabilization mechanism for external kink modes in QAS appears to be an enhancement of local magnetic shear due to 3D shaping. The stabilization of ballooning mode in QOS is related to a shortening of the normal curvature connection length