THE CENTENARY OF LEONID BOXAN: MOMENTS OF LIFE

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PILIPEȚCHII SERGHEI

2016-06-01

Full Text Available The article presents information about the famous Moldovan tenor, excellent vocal teacher — Leonid Boxan who would have been 100 years old in 2016. He died at the age of 96 leaving an immence heritage: well- trained vocalists and a number of scene characters performed on the srages of the Timişoara, Liviv and Chişinau Opera Theatres. Of special interest is the circle of personalities who were around him. In the first place should be mentioned the outstanding representatives of the national vocal school: his teachers, friends, colleagues, and pupils. The author also mentions the anniversary concert dedicated to his memory that was held on the stage of the Organ Hall in which the Master’s pupils and colleagues took part.

120th anniversary of the birth of Sergei Ivanovich Vavilov (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 30 March 2011)

Science.gov (United States)

2011-12-01

A scientific session of the Physical Sciences Division of the Russian Academy of Sciences (RAS) dedicated to the 120th anniversary of the birth of Sergei Ivanovich Vavilov was held in the Conference Hall of the P N Lebedev Physical Institute, RAS, on 30 March 2011. The following reports were put on the session's agenda posted on the web site www.gpad.ac.ru of the Physical Sciences Division, RAS: (1) Masalov A V (P N Lebedev Physical Institute, RAS, Moscow) "S I Vavilov and nonlinear optics"; (2) Basiev T T (Laser Materials and Technology Research Center, A M Prokhorov General Physics Institute, RAS, Moscow) "Luminescent nanophotonics and high-power lasers"; (3) Vitukhnovsky A G (P N Lebedev Physical Institute, RAS, Moscow) "Advances in luminescent light sources and displays"; (4) Aleksandrov E B (Ioffe Physical Technical Institute, RAS, St. Petersburg) "Sergei Ivanovich Vavilov and the special theory of relativity"; (5) Bolotovsky B M (P N Lebedev Physical Institute, RAS, Moscow) "Vavilov-Cherenkov effect"; (6) Vizgin V P (S I Vavilov Institute of the History of Natural Scienses and Technology, RAS, Moscow) "Sergei Ivanovich Vavilov as a historian of science"; (7) Ginzburg A S (Knowledge Society) "Academician S I Vavilov — a devotee of the enlightenment and the first president of the Knowledge Society of the USSR". The papers written on the basis of reports 1-4 and 6 are given below. The main contents of report 5 is reflected in the paper "Vavilov-Cherenkov radiation: its discovery and application" [Usp. Fiz. Nauk 179 1161 (2009); Phys. Usp. 52 1099 (2009)] published earlier by B M Bolotovsky. • S I Vavilov and nonlinear optics, A V Masalov, Z A Chizhikova Physics-Uspekhi, 2011, Volume 54, Number 12, Pages 1257-1262 • Luminescent nanophotonics, fluoride laser ceramics, and crystals, T T Basiev, I T Basieva, M E Doroshenko Physics-Uspekhi, 2011, Volume 54, Number 12, Pages 1262-1268 • Advances in light sources and displays, A G Vitukhnovsky Physics

Video and photographic spectroscopy of 1998 and 2001 Leonid persistent trains from 300 to 930 nm

Czech Academy of Sciences Publication Activity Database

Abe, S.; Ebizuka, N.; Murayama, H.; Ohtsuka, K.; Sugimoto, S.; Yamamoto, M.; Yano, H.; Watanabe, J.; Borovička, Jiří

2005-01-01

Roč. 95, 1-4 (2005), s. 265-277 ISSN 0167-9295. [Meteoroids 2004. London, Ontario, 16.08.2004-20.08.2004] Institutional research plan: CEZ:AV0Z1003909 Keywords : airglow * Leonid meteor * shower Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 0.975, year: 2005

Pavel Ivanovich Karpov (1873-1932?)--the Russian Prinzhorn: art of the insane in Russia.

Science.gov (United States)

Lerner, Vladimir; Podolsky, Grigory; Witztum, Eliezer

2016-03-01

The complicated relationship between the discipline of mental health and the arts has barely been studied systematically. Mental hospitals, shelters and prisons--institutions that accommodate the mentally ill--sometimes promote but often discourage and disrupt the patients' artistic creativity and the images created. In psychiatric circles, the recognition of patient art was a long, slow and frustrating process. Among the Western psychiatrists who studied the creative activity of the mentally ill, researchers usually mention such names as C. Lombroso, M. Shearing, V. Morgentaller, H. Prinzhorn and others, but rarely refer to their Russian colleagues and contemporaries. Pavel Ivanovich Karpov (1873-1932?), a Russian psychiatrist, was one of the most extensive researchers in the field of the art of the insane, but unfortunately his name is little known among modern psychiatrists. For his clinical and scientific contributions, he deserves to be remembered in the history of psychiatry. © The Author(s) 2016.

Russia - Africa. Klondike of Interaction. Interview with Leonid L. Fituni, Institute of African Studies

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Ol'ga Gerasimova

2016-12-01

Full Text Available Professor Leonid L. Fituni was born on the 27th of September 1953. He graduated from the Moscow State Institute of International Relations, MFA of the USSR in 1975. He is Deputy Director of the Institute for African Studies of the Russian Academy of Sciences. Concurrently, he heads the Center for Strategic and Global Studies there. He is the author of 18 books and about 300 articles, is fluent in English, French and Arabic. Interview with Doctor of Economics, Professor L.L. Fituni is devoted to the most topical issues of Russian-African relations, as well as key features of interaction in historical perspective. According to Leonid Leonidovich, at the moment we can not say that these relations are at their peak, however, there can be traced a certain rise in the past decade. Professor also touches upon Russian debt relief to African countries and the presence of Russian business on the African continent. L.L. Fituni in details describes the economic potential of African countries and the prospects for cooperation with Russia. Particular attention is paid to the world scientific schools of African research and training in this area, including the national school of African studies.

FeO "Orange Arc" Emission Detected in Optical Spectrum of Leonid Persistent Trains

Science.gov (United States)

Jenniskens, Peter; Lacey, Matt; Allan, Beverly J.; Self, Daniel E.; Plane, John M. C.; DeVincenzi, Donald L. (Technical Monitor)

2000-01-01

We report the detection of a broad continuum emission dominating the visual spectrum of a Leonid persistent train. A comparison with laboratory spectra of FeO 1 "orange arc" emission at I mbar shows a general agreement of the band position and shape. The detection of FeO confirms the classical mechanism of metal atom catalyzed recombination of ozone and oxygen atoms as the driving force behind optical emission from persistent trains. Sodium and iron atoms are now confirmed catalysts.

Implementing the Zone of Proximal Development: From the Pedagogical Experiment to the Developmental Education System of Leonid Zankov

Science.gov (United States)

Guseva, Liudmila G.; Solomonovich, Mark

2017-01-01

This article overviews the theoretical and applied works of the psychologist and pedagogue Leonid Zankov. Zankov's model of teaching is based on Vygotsky's theory that appropriate teaching methods stimulate cognitive development, whose core notion is the Zone of Proximal Development. This educational psychology research was verified by large scale…

Long time experience with deactivation and regeneration of DENOX catalysts and evaluation with the Internet database LEONID; Langzeiterfahrung mit der Deaktivierung und Regeneration von DENOX-Katalysatoren sowie Auswertung mit der Internet-Datenbank LEONID

Energy Technology Data Exchange (ETDEWEB)

Brandenstein, J.; Dieckmann, H.J.; Gutberlet, H. [E.ON Engineering GmbH, Gelsenkirchen (Germany)

2008-07-01

The paper gives an overview over the long-term catalyst deactivation and the main reasons for catalyst aging. The chemical composition of de-activated catalysts provides information on the optimum catalyst regeneration process. The long-term deactivation behaviour of regenerated catalysts is compared to new catalysts. All characteristic catalyst features are listed in an online 'LEONID'-database, developed by E.ON Engineering. The database provides the basis for long-term catalyst management of all connected SCR systems. (orig.)

H.E. Mr Leonid A. Skotnikov, Ambassador, Permanent Representative of the Russian Federation to the United Nations and other International Organisations in Geneva

CERN Multimedia

Patrice Loïez

2003-01-01

H.E. Mr Leonid A. Skotnikov, Ambassador of the Russian Federation to the United Nations and other International Organisations in Geneva (far right). On his right F. Grishaev, Adviser, Mission of the Russian Federation; opposite N. Koulberg and L. Maiani, CERN Director general

Observations on Stratospheric-Mesospheric-Thermospheric temperatures using Indian MST radar and co-located LIDAR during Leonid Meteor Shower (LMS

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R. Selvamurugan

2002-11-01

Full Text Available The temporal and height statistics of the occurrence of meteor trails during the Leonid meteor shower revealed the capability of the Indian MST radar to record large numbers of meteor trails. The distribution of radio meteor trails due to a Leonid meteor shower in space and time provided a unique opportunity to construct the height profiles of lower thermospheric temperatures and winds, with good time and height resolution. There was a four-fold increase in the meteor trails observed during the LMS compared to a typical non-shower day. The temperatures were found to be in excellent continuity with the temperature profiles below the radio meteor region derived from the co-located Nd-Yag LIDAR and the maximum height of the temperature profile was extended from the LIDAR to ~110 km. There are, how-ever, some significant differences between the observed profiles and the CIRA-86 model profiles. The first results on the meteor statistics and neutral temperature are presented and discussed below.  Key words. Atmospheric composition and structure (pres-sure, density, and temperature History of geophysics (at-mospheric sciences Meteorology and atmospheric dynamics (middle atmosphere dynamics

SOKOLSKY GRIGORY IVANOVICH: CONTRIBUTION TO THE DEVELOPMENT OF RUSSIAN AND INTERNATIONAL MEDICINE. ON THE OCCASION OF THE 210th ANNIVERSARY OF HIS BIRTH

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D. I. Abdulganieva

2018-01-01

Full Text Available The paper is devoted to the anniversary – the 210th anniversary of the birth of the outstanding scientist and clinician Grigory Ivanovich Sokolsky. G.I. Sokolsky made a huge contribution to the development of rheumatology, internal medicine, pathofisiology, and to the enhancement of disease diagnostic capabilities. He published many works in various branches of medicine. The surprising fact is that the young scientist published one or two large works every year in the second half of the 1830s. The scientist won international recognition for his work “On Rheumatism of Heart Muscle Tissue” (1836 that opened up a new understanding of the pathophysiology of rheumatism, by establishing a relationship of joint injuries to the heart. The clinical introduction and teaching of auscultation and percussion also became G.I. Sokolsky’s priceless merit to Russian medicine.

MSFC Stream Model Preliminary Results: Modeling Recent Leonid and Perseid Encounters

Science.gov (United States)

Cooke, William J.; Moser, Danielle E.

2004-01-01

The cometary meteoroid ejection model of Jones and Brown (1996b) was used to simulate ejection from comets 55P/Tempel-Tuttle during the last 12 revolutions, and the last 9 apparitions of 109P/Swift-Tuttle. Using cometary ephemerides generated by the Jet Propulsion Laboratory s (JPL) HORIZONS Solar System Data and Ephemeris Computation Service, two independent ejection schemes were simulated. In the first case, ejection was simulated in 1 hour time steps along the comet s orbit while it was within 2.5 AU of the Sun. In the second case, ejection was simulated to occur at the hour the comet reached perihelion. A 4th order variable step-size Runge-Kutta integrator was then used to integrate meteoroid position and velocity forward in time, accounting for the effects of radiation pressure, Poynting-Robertson drag, and the gravitational forces of the planets, which were computed using JPL s DE406 planetary ephemerides. An impact parameter was computed for each particle approaching the Earth to create a flux profile, and the results compared to observations of the 1998 and 1999 Leonid showers, and the 1993 and 2004 Perseids.

Buoyancy of the ''Y2K'' Persistent Train and the Trajectory of the 04:00:29 UT Leonid Fireball

Science.gov (United States)

Jenniskens, Peter; Rairden, Rick L.; DeVincenzi, Donald L. (Technical Monitor)

2000-01-01

The atmospheric trajectory is calculated of a particularly well studied fireball and train during the 1999 Leonid Multi-Instrument Aircraft Campaign. Less than a minute after the meteor's first appearance, the train curves into a '2'-shape, which persisted until at least 13 minutes after the fireball. We conclude that the shape results because of horizontal winds from gravity waves with a scale height of 8.3 km at 79-91 km altitude, as well as a westerly wind gradient with altitude. In addition, there is downward drift that affects the formation of loops in the train early on.

Buoyancy of the "Y2K" Persistent Train and the Trajectory of the 04:00:29 UT Leonid Fireball

Science.gov (United States)

Jenniskens, Peter; Rairden, Rick L.

The atmospheric trajectory is calculated of a particularly well studied fireball and train during the 1999 Leonid Multi-Instrument Aircraft Campaign. Less than a minute after the meteor's first appearance, the train curves into a "2"-shape, which persisted until at least 13 minutes after the fireball. We conclude that the shape results because of horizontal winds from gravity waves with a scale height of 8.3 km at 79-91 km altitude, as well as a westerly wind gradient with altitude. In addition, there is downward drift that affects the formation of loops in the train early on.

Implementing the Zone of Proximal Development: From the Pedagogical Experiment to the Developmental Education System of Leonid Zankov

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Liudmila G. GUSEVA

2017-06-01

Full Text Available This article overviews the theoretical and applied works of the psychologist and pedagogue Leonid Zankov. Zankov’s model of teaching is based on Vygotsky’s theory that appropriate teaching methods stimulate cognitive development, whose core notion is the Zone of Proximal Development. This educational psychology research was verified by large scale pedagogical experiments conducted in 1970s at public schools in Russia. Over several decades L.V. Zankov with co-workers and followers created the comprehensive system of developmental education for elementary school. The Zankov education system is used now at public schools in Russia. Its main principles and properties are described.

Implementing the zone of proximal development: From the pedagogical experiment to the developmental education system of Leonid Zankov

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Liudmila G. Guseva

2017-06-01

Full Text Available This article overviews the theoretical and applied works of the psychologist and pedagogue Leonid Zankov. Zankov’s model of teaching is based on Vygotsky’s theory that appropriate teaching methods stimulate cognitive development, whose core notion is the Zone of Proximal Development. This educational psychology research was verified by large scale pedagogical experiments conducted in 1970s at public schools in Russia. Over several decades L.V. Zankov with co-workers and followers created the comprehensive system of developmental education for elementary school. The Zankov education system is used now at public schools in Russia. Its main principles and properties are described.

MSFC Stream Model Preliminary Results: Modeling the 1998-2002 Leonid Encounters and the 1993,1994, and 2004 Perseid Encounters

Science.gov (United States)

Moser, D. E.; Cooke, W. J.

2004-01-01

The cometary meteoroid ejection models of Jones (1996) and Crifo (1997) were used to simulate ejection from comets 55P/Tempel-Tuttle during the last 12 revolutions, and the 1862, 1737, and 161 0 apparitions of 1 OSP/Swift-Tuttle. Using cometary ephemerides generated by the JPL HORIZONS Solar System Data and Ephemeris Computation Service, ejection was simulated in 1 hour time steps while the comet was within 2.5 AU of the Sun. Also simulated was ejection occurring at the hour of perihelion passage. An RK4 variable step integrator was then used to integrate meteoroid position and velocity forward in time, accounting for the effects of radiation pressure, Poynting-Robertson drag, and the gravitational forces of the planets, which were computed using JPL's DE406 planetary ephemerides. An impact parameter is computed for each particle approaching the Earth, and the results are compared to observations of the 1998-2002 Leonid showers, and the 1993-1 994 Perseids. A prediction for Earth's encounter with the Perseid stream in 2004 is also presented.

Sporadic-E associated with the Leonid meteor shower event of November 1998 over low and equatorial latitudes

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H. Chandra

2001-01-01

Full Text Available Rapid radio soundings were made over Ahmedabad, a low latitude station during the period 16–20 November 1998 to study the sporadic-E layer associated with the Leonid shower activity using the KEL Aerospace digital ionosonde. Hourly ionograms for the period 11 November to 24 November were also examined during the years from 1994 to 1998. A distinct increase in sporadic-E layer occurrence is noticed on 17, 18 and 19 November from 1996 to 1998. The diurnal variations  of  f0Es and fbEs also show significantly enhanced values for the morning hours of 18 and 19 November 1998. The ionograms clearly show strong sporadic-E reflections at times of peak shower activity with multiple traces in the altitude range of 100–140 km in few ionograms. Sporadic-E layers with multiple structures in altitude are also seen in some of the ionograms (quarter hourly at Thumba, situated near the magnetic equator. Few of ionograms recorded at Kodaikanal, another equatorial station, also show sporadic- E reflections in spite of the transmitter power being significantly lower. These new results highlighting the effect of intense meteor showers in the equatorial and low latitude E-region are presented.Key words. Ionosphere (equatorial ionosphere – Radio science (ionospheric physics

Love on the Final Slopes of Life: Fedor Ivanovich Tiutchev and “The Denis’eva Cycle”

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Lillian Jorunn Helle

2017-09-01

Full Text Available Old age represents a serious contemporary social issue. With the greater incidence of longevity also literary approaches to ageing have emerged, and “Ageing and literature” is now established among literary scholars as a critical perspective in its own right, with a perspective usually marked by an interdisciplinary stance. What insights can literature offer when it comes to old age that other kinds of knowledge cannot? As my article aims to show, literature is and remains (inter alia highly relevant as a unique access to individual ageing, enabling us to grasp the ambivalences and intricacies connected to growing old more distinctly then quantitative, statistical sociological studies and medical reports can do. And most notably, literature can investigate the domain of ageing senses and sensations and widen our understanding of how elderly people experience sensual attractions, love and desire. To concretize these assumptions, I will focus on the so called “Denisieva cycle”, by Feodor Ivanovich Tyutchev, one of the greatest poets in the classical Russian tradition. The cycle has an autobiographical context: it retells in lyrical verse how the married Tyutchev, at 50, an advanced age at that time, fell  in love with Elena Aleksandrovna Denisieva, a noblewoman of 22 and a school-friend of his daughters. While not divorcing, the poet kept up an illicit relationship with Denisieva for 15 years and she bore him three children. The affair ended in utmost tragedy, when Denisieva, ostracized by both family and former friends, died in 1865, followed closely by the death of two of their children. These events brought the elderly lover into a spiral of endless despair, but also resulted in a sublime body of poems which constitutes a remarkably testimony of the senescent subject in love, questioning, as I will demonstrate, a number of prevalent stereotypes about passions in the winter of a man’s life. Moreover, the manner in which Tyutchev

Sporadic-E associated with the Leonid meteor shower event of November 1998 over low and equatorial latitudes

Directory of Open Access Journals (Sweden)

H. Chandra

Full Text Available Rapid radio soundings were made over Ahmedabad, a low latitude station during the period 16–20 November 1998 to study the sporadic-E layer associated with the Leonid shower activity using the KEL Aerospace digital ionosonde. Hourly ionograms for the period 11 November to 24 November were also examined during the years from 1994 to 1998. A distinct increase in sporadic-E layer occurrence is noticed on 17, 18 and 19 November from 1996 to 1998. The diurnal variations 
of  f₀E_s and f_bE_s also show significantly enhanced values for the morning hours of 18 and 19 November 1998. The ionograms clearly show strong sporadic-E reflections at times of peak shower activity with multiple traces in the altitude range of 100–140 km in few ionograms. Sporadic-E layers with multiple structures in altitude are also seen in some of the ionograms (quarter hourly at Thumba, situated near the magnetic equator. Few of ionograms recorded at Kodaikanal, another equatorial station, also show sporadic- E reflections in spite of the transmitter power being significantly lower. These new results highlighting the effect of intense meteor showers in the equatorial and low latitude E-region are presented.

Key words. Ionosphere (equatorial ionosphere – Radio science (ionospheric physics

Kino o "barhatnõhh revoljutsijahh" / Valentin Sedov

Index Scriptorium Estoniae

Sedov, Valentin

2005-01-01

21. juulil esilinastub Venemaal poliitiline põnevik, mis kujutab, kuidas lääne miljardär Sors (George Soros?) organiseerib sametrevolutsioone SRÜ maades. Filmi tegemisele osutas igakülgset abi Venemaa valitsus

The tectonic and stratigraphic history of the Cardaño area, Cantabrian mountains, Northwest Spain

NARCIS (Netherlands)

Veen, van J.

1965-01-01

The Devonian and Carboniferous rock-sequence in the Cantabrian Mountains is developed in two different facies which are separated by an E-W tectonic line, the León Line, and called the Leonide and Palentian facies, respectively to the S and N. The Leonide facies is widely exposed throughout the

Moskovski desant / Galina Balashova

Index Scriptorium Estoniae

Balashova, Galina

2006-01-01

Tallinna Vene saatkonna galerii osalemisest Madridi ja Moskva kunstilaatadel. Moskva kunstiajakirjast "Iskusstvo" ja selle esitlusest peatoimetaja Leonid Lerneri poolt Tallinna Vene saatkonna galeriis. Samas toimuvast Vene kaasaegse kunsti näitusest "Moskva ja teised". Tööd on Moskva galerii Artgentum (direktor Leonid Lerner) kogust. Lähemalt Damir Muratovi, Ruslan Vashkevitshi ja Rinata Voligamsi loomingust

An improved method to experimentally determine temperature and pressure behind laser-induced shock waves at low Mach numbers

International Nuclear Information System (INIS)

Hendijanifard, Mohammad; Willis, David A

2011-01-01

Laser-matter interactions are frequently studied by measuring the propagation of shock waves caused by the rapid laser-induced material removal. An improved method for calculating the thermo-fluid parameters behind shock waves is introduced in this work. Shock waves in ambient air, induced by pulsed Nd : YAG laser ablation of aluminium films, are measured using a shadowgraph apparatus. Normal shock solutions are applied to experimental data for shock wave positions and used to calculate pressure, temperature, and velocity behind the shock wave. Non-dimensionalizing the pressure and temperature with respect to the ambient values, the dimensionless pressure and temperature are estimated to be as high as 90 and 16, respectively, at a time of 10 ns after the ablation pulse for a laser fluence of F = 14.5 J cm -2 . The results of the normal shock solution and the Taylor-Sedov similarity solution are compared to show that the Taylor-Sedov solution under-predicts pressure when the Mach number of the shock wave is small. At a fluence of 3.1 J cm -2 , the shock wave Mach number is less than 3, and the Taylor-Sedov solution under-predicts the non-dimensional pressure by as much as 45%.

The contribution of professor G. I. Turner in pediatric orthopedics and clinical surgery (160th anniversary of birth

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T. Sh Morgoshiya

2018-01-01

Full Text Available The article is devoted to the multifarious activities of Genrikh Ivanovich Turner (1858–1941. It is noted that originally G.I. Turner was interested in problems abstracted from orthopedics: acute purulent processes in the right iliac fossa, etc. In 1895, Turner was appointed Professor of  the Department of Desmurgy and Mechanics of  the Military Medical Academy. He revived the teaching of the subject and transmitted it into “broad practical soil”. Genrikh Ivanovich Turner became one of the founders of the Russian orthopedics, the organizer and the head (since 1900 of the first in Russia department and clinic of orthopedics. G.I. Turner gave a lot of power and energy to render assistance to sick children suffering from physical disabilities, restore the working capacity of children with disabilities. For many years he was in charge of the orphanage in St. Petersburg, which was transformed into the G.I. Turner Research Institute of Child Disability in 1932. This institution became an organizational and methodological center for combating child disability in  the Soviet Union. Genrikh Ivanovich was the first in Russia, who raised his voice in favor of  the disabled child, pointed out the need to provide systematic state assistance to disabled children with diseases of the musculoskeletal system.

Vladimir Ivanovich Lubowsky (1923–2017

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Basilova T.A.

2018-01-01

Full Text Available The article is dedicated to the memory of the famous in our country and abroad scientist in the field of special education, professor Vladimir Lubovsky, who died at November 9, 2017 at 93 years old. Describes the main stages of his professional biography. He was a Veteran of World War II. V.I. Lubowsky received an education of the psychologist in the Moscow State University in 1951, His supervisor in graduate school was the world-famous psychologist Alexander Luria. For 40 years he worked at the Institute of Defectology, then more than 20 years he was Professor at Moscow City University and Moscow State University of Psychology and Education. A list of his scientific works is more than 200 items.

On the way from logic to algebra

International Nuclear Information System (INIS)

Ershov, Yurii L

2011-01-01

In this paper, which is from a shorthand report of the author's plenary lecture at the international conference 'Malcev Meeting 2009' (Novosibirsk, 24-28 August 2009), the influence of three papers by Anatolii Ivanovich Malcev on the development of algebra and mathematical logic is discussed. Bibliography: 75 titles.

Dissipative quantum mechanics: The generalization of the canonical quantization and von Neumann equation

International Nuclear Information System (INIS)

Tarasov, V.E.

1994-07-01

Sedov variational principle, which is the generalization of the least actional principle for the dissipative processes is used to generalize the canonical quantization and von Neumann equation for dissipative systems (particles and strings). (author). 66 refs, 1 fig

Gorodskoje jaitso / Leonid Surkov

Index Scriptorium Estoniae

Surkov, Leonid

1998-01-01

Tallinna linna kaunistavatest ausammastest ja dekoratiivskulptuuridest ning Rävala pst-le Hoiupanga uue hoone ette planeeritud dekoratiivskulptuuri projektide konkursi võidutöödest : I koha sai Angela Orgussaare töö "Urban Egg", mis artikli autori arvates ei pääse antud kohal mõjule.

Creating cometary models using ancient Chinese data

Science.gov (United States)

Yeomans, D. K.

For more than two millennia, Chinese court astronomers maintained a rather comprehensive record of cometary sightings. Owing to the significance of comets as portents for the reigning emperor, early sky watchers from China (as well as their counterparts from Korea and Japan) carefully noted each cometary apparition for the purpose of astrological predictions. The dates and corresponding celestial locations and motions were usually recorded and in some cases, the colors, coma sizes, and tail lengths were also noted. These ancient observations represent the only source of information available for modeling the long-term behavior of periodic comets. For comets Halley and Swift-Tuttle, Chinese records have been identified as far back as 240 B.C. and 69 B.C. respectively and these data have been used to define their long-term motions. As a result, heliocentric and geocentric distances for each Chinese sighting of these two comets can be computed and estimates can be made for each comet's intrinsic brightness at various observed returns. Although the earliest identified apparition of comet Tempel-Tuttle is A.D. 1366, the associated Leonid meteor showers were noted back to at least A.D. 902. The Leonid meteor stream is young in the sense that outstanding meteor displays occur only near the time of the parent comet's perihelion passages. The ancient Chinese records of the Leonid meteor showers and storms have been used to map the particle distribution around the parent comet and this information was used to guide predictions for the 1998-1999 Leonid meteor showers.

Объявлены финалисты русского "Букера"

Index Scriptorium Estoniae

2003-01-01

Vene Bookeri ("Букер - Открытая Россия") finalistid: Natalja Galkina (romaan "Вилла Рено"), Ruben Gonzalez ("Белое на черном"), Leonid Zorin ("Юпитер"), Afanassi Mamedov ("Фрау Шрам"), Jelena Tšižova ("Лавра") ja Leonid Juzefovitš ("Казароза"). Ka intervjuust žürii esimehega Jakov Gordiniga

An Annotated Bibliography of the Open Literature on Deception.

Science.gov (United States)

1985-12-01

Potter, 1961, pp. 82, 102-103; ch. 8, "For Righteous or Sinners,", pp. 87-104. Arendt , Hannah , "Lying in Politics: Reflections on the Pentagon Papers...79 Ardamatskiy, Vasiliy Ivanovich............................. 103 Arendt , Hannah ...34 New York Review of Books, Vol. 17, No. 8, November 18, 1971, pp. 30-39; in H. Arendt , Lying in Politics. New York- Harcourt, Brace, Jovanovich

Adamkus tries hand at mediating in eye of Ukrainian maelstrom

Index Scriptorium Estoniae

2004-01-01

Leedu president Valdas Adamkus sõitis Leonid Kutshma kutsel Ukrainasse vahendamaks läbirääkimisi presidendikandidaatide - opositsiooniliider Viktor Jushtshenko ja peaminister Viktor Janukovitshi vahel

Poltora milliona za "Maugli" namerena polutshit naslednitsa odnogo iz sozdatelei multfilma

Index Scriptorium Estoniae

2004-01-01

Stsenarist Leonid Belokurovi abikaasa nõuab filmistuudio "Sojuzmultifilm" õigusjärgsetelt omanikelt kohtu kaudu poolteist miljonit rubla multifilmi "Mowgli" näitamise eest Venemaa eri telekanalitel

Tsena, ravnaja zhizni / Leonid Stolovitsh

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Stolovitš, Leonid, 1929-2013

2003-01-01

Saksa arhitektuuriteoreetikust ja graafikust Kurt Magritzist ja tema fashismivastase sisuga graafikast ja joonistustest aastatest 1933-1945. 1966. a. mais oli K. Magritzi graafika näitus Tartu Kunstimuuseumis

Дагерротип - фотография - фильм / Елена Скульская

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Скульская, Елена, 1950-

2009-01-01

ETV saatesarjast "Ela sajani", mille sisuks on portreefilmid tegusatest eesti vanemaealistest. Autor käsitleb Jaanis Valgu ja Viktoria Korpani filmi Leonid Gordejevist ning Leeni Linna filmi Ants Viiresest

Narvitjanin Andrei Ivanen napisal knigu o dramatitsheskoi sudbe tserkvi Stieglitza / Irina Tokareva

Index Scriptorium Estoniae

Tokareva, Irina

2004-01-01

Sankt-Peterburi kirjastuse "Kollo" väljaantud raamatu "Ivangorodskaja-Svjato-Troitskaja tserkov barona Aleksandra Stieglitza" saamisloost, kirikust (arhitekt Aleksandr Krakau, altarimaal Fjodor Bruni) ja selle taastamisest. Raamatu fotod: Leonid Lashkevitsh

Käsitlusi ingerisoomlaste kannatusteest / Taisto-Kalevi Raudalainen

Index Scriptorium Estoniae

Raudalainen, Taisto-Kalevi

2005-01-01

Rets. rmt.: Gildi, Leonid. Sudba "sotsialno opasnogo" naroda. Sankt-Peterburg, 2003 ; Sihvo, Jouko. Inkerin kansan 60 kohtalon vuotta. Helsinki, 2000 ; Konkka, Unelma. Oma maa omenakukka, vieras maa veripunainen. Petroskoi, 2003

"Spicy ice" ja klaveri talveuniversiteet / Toomas Velmet

Index Scriptorium Estoniae

Velmet, Toomas, 1942-

2011-01-01

25. veebruaril Pärnu kontserdimajas toimunud talveunversiteedi galakontserdist, kus esinesid pianistid Liidia Ilves (Eesti), Cäcilia Maria Weber (Austria) ja Nena Kozjek (Sloveenia) ja Pärnu Linnaorkester Leonid Grini dirigeerimisel

Namedni Ernst prigrozil Parjenovu dezha vju

Index Scriptorium Estoniae

2004-01-01

Vene telekanal NTV vallandas autorisaate "Namedni" juhi Leonid Parfjonovi. Telekanal ORT juht Konstantin Ernst peab saatejuhiga läbirääkimisi sarnase saate, nimega "Deja vu", tegemiseks nende kanalil

Nebolshaja sensatsija / Ilja Sundelevitsh

Index Scriptorium Estoniae

Sundelevitsh, Ilja

2001-01-01

Venemaa ei seo enam majandusliku koostöö arengut nii rangelt Eesti astumisega NATO-sse. Kommentaar Vene Riigiduuma rahvusvaheliste asjade komisjoni aseesimehelt Leonid Slutskilt. Lühiintervjuu A. Tarandiga. Parlamendisaadik (A. Tarand)

Из Таллинна в Париж / Антон Бакунцев

Index Scriptorium Estoniae

Бакунцев, Антон, 1973-

2013-01-01

Kahe 1930ndatel Tallinnast Pariisi saadetud kirja publikatsioonid: Pavel Irteli (1896-1979) kiri Pavel Miljukovile (dateeritud 21.03.1932) ja Aleksandr Šultsi (1884-?) kiri Leonid Zurovile (dateeritud 28.11.1935)

78 FR 60297 - Center for Scientific Review; Notice of Closed Meetings

Science.gov (United States)

2013-10-01

..., Rockville, MD 20852. Contact Person: Leonid V. Tsap, Ph.D., Scientific Review Officer, Center for Scientific...: Residence Inn Bethesda, 7335 Wisconsin Avenue, Bethesda, MD 20814. Contact Person: Patrick K Lai, Ph.D...

Hirm valitseb Marimaad / Jaak Prozes

Index Scriptorium Estoniae

Prozes, Jaak, 1965-

2005-01-01

Fenno-Ugria hõimukeskuse juhataja sõnul toimub Marimaal arveteõiendamine nendega, kes toetasid presidendivalimiste kampaanias Leonid Markelovi vastaskandidaati, samuti ei sallita neid, kelle arvamus presidendi omaga kokku ei lange. Vägivallajuhtumitest

Bagatellid : Maailm / Nele-Eva Steinfeld

Index Scriptorium Estoniae

Steinfeld, Nele-Eva

2009-01-01

Muusikasõnumeid maailmast: Sofya Gulyak võitis Leedsi rahvusvahelise pianistide konkursi. EMI plaadikompanii uus artist Vilde Frang. Lahkus Alicia de Larrocha. Moskva Suure Teatri juhiks sai Leonid Desjatnikov. Avastati maailma vanimad muusikainstrumendid

Ljubov nebessnaja i zemnaja / Anna Moleva

Index Scriptorium Estoniae

Moleva, Anna

2002-01-01

Venemaa teleseriaali "Vene amatsoonid" ("Russkije amazonki") võtteplatsil vastavad küsimustele režissöör Isaak Fridberg, näitlejad Leonid Jakubovitsh, Juozas Budraitis, Aleksei Krivtshenko ja Irina Rozanova

So zvjozdami na Lune / Adolf Käis

Index Scriptorium Estoniae

Käis, Adolf, 1946-2013

1999-01-01

Moskva "Teatr Lunõ" külalisetendused Tallinnas 15. ja 16. juunil Vene Draamateatris. Mängitakse Francis Scott Fitzgeraldi romaani "Sume on öö" instseneeringut. Instseneerija ja lavastaja Sergei Prohhanov, kunstnik Leonid Podossenov

Asambljazh v "Iskusstve"

Index Scriptorium Estoniae

2006-01-01

Vene saatkonna galeriis Tallinnas näitab töid oma kaasaegse kunsti kogust Moskva galerii Artgentum - fotograafia, maalikunst, graafika ja assamblaaž. Näituse avamisel esitles Artgentumi direktor Leonid Lerner Moskva kunstiajakirja "Iskusstvo"

Journal of Biosciences | Indian Academy of Sciences

Indian Academy of Sciences (India)

Mass distributions of a macromolecular assembly based on electrospray ionization mass spectrometric masses of the constituent subunits · Leonid Hanin Brian Green Franck Zal .... pinealocytes of the catfish pineal organ. pp 623-636 Review.

Dust Acoustic Mode Manifestations in Earth's Dusty Ionosphere

International Nuclear Information System (INIS)

Kopnin, S.I.; Popel, S.I.

2005-01-01

Dust acoustic mode manifestations in the dusty ionosphere are studied. The reason for an appearance of the low-frequency radio noises associated with such meteor fluxes as Perseids, Orionids, Leonids, and Gemenids is determined

Narvitjanin Andrei Ivanen napisal knigu o dramatitsheskoi sudbe tserkvi Shtiglitsa / Irina Tokareva

Index Scriptorium Estoniae

Tokareva, Irina

2004-01-01

Narva koduloolane Andrei Ivanen raamatu "Ivangorodskaja-Svjato-Troitskaja tserkov barona Aleksandra Stiglitsa" saamisloost. Arhitekt Aleksandr Krakau kavandatud Ivangorodi Püha Kolmainsuse kiriku hoonest ja selle taastamisest. Kiriku altarimaal on Fjodor Brunilt. Raamatu fotod Leonid Lashkevitshilt

Kolm ostumekat viskasid Tsingisseri kullaäri välja / Lauri Linnamäe

Index Scriptorium Estoniae

Linnamäe, Lauri

2008-01-01

Ilmunud ka: Postimees : na russkom jazõke 8. juuli 2008, lk. 4. Ekspoliitikust juveeliärimehe Leonid Tsingisseri kella- ja kullapoodide kett Wrist.net on välja visatud kolmest suurest kaubanduskeskusest. Lisa: Ekspoliitikust ärimees

Kapo hakkas siiski rahavahetuspaanika tagamaid uurima / Maria-Elisa Rannajõe

Index Scriptorium Estoniae

Rannajõe, Maria-Elisa

2007-01-01

Kaitsepolitsei pressiesindaja Olari Valtin selgitab, miks kaitsepolitsei hakkas siiski uurima massilise rahavahetuse juhtumit. ERL-i liige ja ärimees Leonid Tsingisser ütles Läti ajalehele, et kuigi olukord on stabiliseerunud, on krooni devalveerimine vältimatu

The view from Kiev

International Nuclear Information System (INIS)

Kiselyov, S.

1993-01-01

This article reports the observations of correspondents for the Bulletin (two Russian journalists, one based in Moscow, the other in Kiev) who investigated the status of the Soviet Union's Black Sea Fleet and Ukraine's status as a non-nuclear-weapons state. After two years of wrangling and two earlier failed settlements, Russian President Boris Yeltsin met with Ukrainian President Leonid Kravchuk at Massandra in Crimea. On September 3, the leaders announced that Russia would buy out Ukraine's interest in the fleet and lease the port at Sevastopol. The Massandra summit was also supposed to settle Ukraine's status as a non-nuclear-weapons state. Described here are the Kiev-based correspondent's views on the Massandra summit (and its major topics), which was to have been called off by the Russian foreign ministry when Ukrainian Prime Minister Leonid Kuchma resigned

Mõtteid tegevusetusdeliktist Riigikohtu praktika valguses. Riigikohtu kriminaalkolleegiumi otsus väärteoasjas 3-1-1-104-09 / Erkki Hirsnik

Index Scriptorium Estoniae

Hirsnik, Erkki, 1982-

2010-01-01

Riigikohtu lahendist 3-1-1-104-09: Edelaraudtee Infrastruktuuri AS kaitsja vandeadvokaat Leonid Tolstovi kassatsioon Pärnu Maakohtu 4. juuni 2009. a kohtuotsuse peale Edelaraudtee Infrastruktuuri AS väärteoasjas looduskaitseseaduse § 71 lg 2 järgi

Gamma-Ray Burst Dynamics and Afterglow Radiation from Adaptive Mesh Refinement, Special Relativistic Hydrodynamic Simulations

Science.gov (United States)

De Colle, Fabio; Granot, Jonathan; López-Cámara, Diego; Ramirez-Ruiz, Enrico

2012-02-01

We report on the development of Mezcal-SRHD, a new adaptive mesh refinement, special relativistic hydrodynamics (SRHD) code, developed with the aim of studying the highly relativistic flows in gamma-ray burst sources. The SRHD equations are solved using finite-volume conservative solvers, with second-order interpolation in space and time. The correct implementation of the algorithms is verified by one-dimensional (1D) and multi-dimensional tests. The code is then applied to study the propagation of 1D spherical impulsive blast waves expanding in a stratified medium with ρvpropr -k , bridging between the relativistic and Newtonian phases (which are described by the Blandford-McKee and Sedov-Taylor self-similar solutions, respectively), as well as to a two-dimensional (2D) cylindrically symmetric impulsive jet propagating in a constant density medium. It is shown that the deceleration to nonrelativistic speeds in one dimension occurs on scales significantly larger than the Sedov length. This transition is further delayed with respect to the Sedov length as the degree of stratification of the ambient medium is increased. This result, together with the scaling of position, Lorentz factor, and the shock velocity as a function of time and shock radius, is explained here using a simple analytical model based on energy conservation. The method used for calculating the afterglow radiation by post-processing the results of the simulations is described in detail. The light curves computed using the results of 1D numerical simulations during the relativistic stage correctly reproduce those calculated assuming the self-similar Blandford-McKee solution for the evolution of the flow. The jet dynamics from our 2D simulations and the resulting afterglow light curves, including the jet break, are in good agreement with those presented in previous works. Finally, we show how the details of the dynamics critically depend on properly resolving the structure of the relativistic flow.

GAMMA-RAY BURST DYNAMICS AND AFTERGLOW RADIATION FROM ADAPTIVE MESH REFINEMENT, SPECIAL RELATIVISTIC HYDRODYNAMIC SIMULATIONS

International Nuclear Information System (INIS)

De Colle, Fabio; Ramirez-Ruiz, Enrico; Granot, Jonathan; López-Cámara, Diego

2012-01-01

We report on the development of Mezcal-SRHD, a new adaptive mesh refinement, special relativistic hydrodynamics (SRHD) code, developed with the aim of studying the highly relativistic flows in gamma-ray burst sources. The SRHD equations are solved using finite-volume conservative solvers, with second-order interpolation in space and time. The correct implementation of the algorithms is verified by one-dimensional (1D) and multi-dimensional tests. The code is then applied to study the propagation of 1D spherical impulsive blast waves expanding in a stratified medium with ρ∝r –k , bridging between the relativistic and Newtonian phases (which are described by the Blandford-McKee and Sedov-Taylor self-similar solutions, respectively), as well as to a two-dimensional (2D) cylindrically symmetric impulsive jet propagating in a constant density medium. It is shown that the deceleration to nonrelativistic speeds in one dimension occurs on scales significantly larger than the Sedov length. This transition is further delayed with respect to the Sedov length as the degree of stratification of the ambient medium is increased. This result, together with the scaling of position, Lorentz factor, and the shock velocity as a function of time and shock radius, is explained here using a simple analytical model based on energy conservation. The method used for calculating the afterglow radiation by post-processing the results of the simulations is described in detail. The light curves computed using the results of 1D numerical simulations during the relativistic stage correctly reproduce those calculated assuming the self-similar Blandford-McKee solution for the evolution of the flow. The jet dynamics from our 2D simulations and the resulting afterglow light curves, including the jet break, are in good agreement with those presented in previous works. Finally, we show how the details of the dynamics critically depend on properly resolving the structure of the relativistic flow.

GAMMA-RAY BURST DYNAMICS AND AFTERGLOW RADIATION FROM ADAPTIVE MESH REFINEMENT, SPECIAL RELATIVISTIC HYDRODYNAMIC SIMULATIONS

Energy Technology Data Exchange (ETDEWEB)

De Colle, Fabio; Ramirez-Ruiz, Enrico [Astronomy and Astrophysics Department, University of California, Santa Cruz, CA 95064 (United States); Granot, Jonathan [Racah Institute of Physics, Hebrew University, Jerusalem 91904 (Israel); Lopez-Camara, Diego [Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Ap. 70-543, 04510 D.F. (Mexico)

2012-02-20

We report on the development of Mezcal-SRHD, a new adaptive mesh refinement, special relativistic hydrodynamics (SRHD) code, developed with the aim of studying the highly relativistic flows in gamma-ray burst sources. The SRHD equations are solved using finite-volume conservative solvers, with second-order interpolation in space and time. The correct implementation of the algorithms is verified by one-dimensional (1D) and multi-dimensional tests. The code is then applied to study the propagation of 1D spherical impulsive blast waves expanding in a stratified medium with {rho}{proportional_to}r{sup -k}, bridging between the relativistic and Newtonian phases (which are described by the Blandford-McKee and Sedov-Taylor self-similar solutions, respectively), as well as to a two-dimensional (2D) cylindrically symmetric impulsive jet propagating in a constant density medium. It is shown that the deceleration to nonrelativistic speeds in one dimension occurs on scales significantly larger than the Sedov length. This transition is further delayed with respect to the Sedov length as the degree of stratification of the ambient medium is increased. This result, together with the scaling of position, Lorentz factor, and the shock velocity as a function of time and shock radius, is explained here using a simple analytical model based on energy conservation. The method used for calculating the afterglow radiation by post-processing the results of the simulations is described in detail. The light curves computed using the results of 1D numerical simulations during the relativistic stage correctly reproduce those calculated assuming the self-similar Blandford-McKee solution for the evolution of the flow. The jet dynamics from our 2D simulations and the resulting afterglow light curves, including the jet break, are in good agreement with those presented in previous works. Finally, we show how the details of the dynamics critically depend on properly resolving the structure of the

Vnuk Brezhneva podajot v sud na rezhissjora / Jevgeni Tshazov

Index Scriptorium Estoniae

Tshazov, Jevgeni

2005-01-01

Vene televisiooni jaoks valminud 4-seerialise ajaloolise filmi Leonid Brezhnevist "Brezhnev" : stsenarist Valentin Tshernõhh : režissöör Sergei Snezhkin, teemadel. Brezhnevi sugulased ei ole rahul filmiga. Ära on toodud nimekiri faktidest, mis ei vastavat tegelikkusele

Raul Meel ja Ülo Sooster ajakirjas Zimmerli Journal

Index Scriptorium Estoniae

2007-01-01

Ajakirjas Zimmerli Journal, Fall, 2006, lk. 88-103 Jeremy Canwelli artikkel "System, Terminus and Time : The Mystical Art of Raul Meel" ja lk. 118-125 Leonid Lammi mälestused "Ülo Sooster : an Artist, a Friend and his Time"

Tanzania Journal of Science - Vol 40, No 1 (2014)

African Journals Online (AJOL)

Determination of radioactivity in maize and mung beans grown in the neighborhood of Minjingu phosphate mine, Tanzania · EMAIL FREE FULL TEXT EMAIL FREE FULL TEXT DOWNLOAD FULL TEXT DOWNLOAD FULL TEXT. Leonid L Nkuba, Najat K Mohammed, 51-59 ...

Väga kuldne trio / Ilona Martson

Index Scriptorium Estoniae

Martson, Ilona, 1970-

2008-01-01

Leonid Gaidai 60ndatel loodud filmid "Koer Barboss ja ebatavaline kross", "Kaukaasia vang", "Operatsioon Õ", kus osaleb kuulus vene koomikute trio Nikulin-Vitsõn-Morgunov. Režissöörist, näitlejatest ja nende filmide sünniloost

Metamaterials for Miniaturization of Optical Components

Science.gov (United States)

2014-09-24

elementary EM fields are exactly the Maxwell equations with proper conserved currents; (iii) a free charge moves uniformly preserving up to the...Disordered Systems -- A Conference in Honor of Leonid Pastur , Hagen, Germany, Some Mathematical Problems in a Neoclassical Theory of Electric Charges

ANATOLY I. KITOV: PERSONALITY THROUGH THE PRISM OF DOCUMENTS

Directory of Open Access Journals (Sweden)

Vladimir A. Kitov

2016-01-01

Full Text Available The paper for the first time discusses nine formal characteristics and certifications of the outstanding Russian scientist Anatoly Ivanovich Kitov related to the military and the first postwar years (1944–1950. Their analysis allows detecting the manifestations of the properties of the personality and character of the young combat officer, and then of a student of the military Academy, which later became the basis of his scientific achievements, but also determined the conflict with the administrative-command system.

MegaFoni-diplomaatia : oligarh sõdib Putini liitlasega / Stephen Fidler, Arkady Ostrovsky, Neil Buckley

Index Scriptorium Estoniae

Fidler, Stephen

2006-01-01

Vene firma Alfa väitel kasutatakse firmat Ipoc rahapesuks ja selle telekomiinvesteeringute tegelik omanik on telekommunikatsiooniminister Leonid Reiman. Reimani väitel ei ole talle kunagi kuulunud Ipoci osakuid, ta pole kunagi olnud selle otsene või kaudne omanik. Ipoc on uurimise all Bermudal

"Andke vene kunstnikele vaid toetuspunkt..." : intervjuu Moskva Riikliku Kaasaegse Kunsti Keskuse teaduri Irina Gorlovaga / Irina Gorlova ; interv. Reet Varblane

Index Scriptorium Estoniae

Gorlova, Irina

2002-01-01

Irina Gorlova ja Leonid Bazhanovi kureeritud vene kunstnike Dmitri Gutovi, Sergei Shutovi ja Vadim Zahharovi näitusest "Ristumised" Hansapanga galeriis. I. Gorlova suhtumisest 1960ndate avangardistide põlvkonda, Ülo Soosterist, Ilja Kabakovist, sürrealismist ja praegusest vene kunstist, Oleg Kulikust, Aleksandr Brenerist, Aleksandr Ponomarjovist

Euroopa Inimõiguste Kohtusse avalduse esitamise tingimused ja seda piiravad asjaolud. Eesti Vabariigi vastu Euroopa Inimõiguste Kohtusse esitatud kaebused : [bakalaureusetöö] / Merit Ulvik ; Tartu Ülikool, õigusteaduskond ; juhendaja: Juhani Ko

Index Scriptorium Estoniae

Ulvik, Merit

2003-01-01

Kaebeõigusest üldiselt, avalduse vastuvõtmise kriteeriumid, reservatsiooni tegemise õigus, Eesti Vabariigi vastu esitatud kaebused (vastuvõetamatuks või osaliselt vastuvõetamatuks tunnistatud kaebused - Arnold Treiali ja Leonid Šestjorkini kaebused ; kaebused, mis said lahendi kohtuotsusega - Vitali Slavgorodski, Enno Tammeri, Tiit Veeberi ja Tõnu Mõtsniku kaebused)

Exploring the Diffuse X-ray Emission of Supernova Remnant Kesteven 69 with XMM-Newton

Directory of Open Access Journals (Sweden)

Kyoung-Ae Seo

2013-06-01

Full Text Available We have investigated the X-ray emission from the shock-heated plasma of the Galactic supernova remnant Kesteven 69 with XMM-Newton. Assuming the plasma is at collisional ionization equilibrium, a plasma temperature and a column absorption are found to be kT ~ 0.62 keV and NH ~ 2.85 ×1022 cm-2 respectively by imaging spectroscopy. Together with the deduced emission measure, we place constraints on its Sedov parameters.

Calibration-free quantitative elemental analysis of meteor plasma using reference laser-induced breakdown spectroscopy of meteorite samples

Science.gov (United States)

Ferus, Martin; Koukal, Jakub; Lenža, Libor; Srba, Jiří; Kubelík, Petr; Laitl, Vojtěch; Zanozina, Ekaterina M.; Váňa, Pavel; Kaiserová, Tereza; Knížek, Antonín; Rimmer, Paul; Chatzitheodoridis, Elias; Civiš, Svatopluk

2018-03-01

Aims: We aim to analyse real-time Perseid and Leonid meteor spectra using a novel calibration-free (CF) method, which is usually applied in the laboratory for laser-induced breakdown spectroscopic (LIBS) chemical analysis. Methods: Reference laser ablation spectra of specimens of chondritic meteorites were measured in situ simultaneously with a high-resolution laboratory echelle spectrograph and a spectral camera for meteor observation. Laboratory data were subsequently evaluated via the CF method and compared with real meteor emission spectra. Additionally, spectral features related to airglow plasma were compared with the spectra of laser-induced breakdown and electric discharge in the air. Results: We show that this method can be applied in the evaluation of meteor spectral data observed in real time. Specifically, CF analysis can be used to determine the chemical composition of meteor plasma, which, in the case of the Perseid and Leonid meteors analysed in this study, corresponds to that of the C-group of chondrites.

Mendeleiev, el que pudo haber sido y no fue

OpenAIRE

Bascuñán Blaset, Aníbal

2008-01-01

The life of Dimitri Ivanovich Mendeleiev is revisited in this paper. After studying based on the support of his mother, he managed to receive a fellowship to make work with the best European chemists of that time: Bunsen, Dumas, Kirchhoff, Liebig, Würtz and Erlenmeyer. Dimitri attended the Karlsruhe Conference in 1860, fact that he afterwards revealed as key to the proposal of his Periodic Table in 1869, when he was as young as 35 years old, and he proposed a whole set of predictions about un...

Королевские игры / Тамара Унанова

Index Scriptorium Estoniae

Унанова, Тамара 1951-

2009-01-01

19. nov. Tallinnas Nokia kontserdimajas etendunud rahvusvahelisest balletiprogrammist "Tantsukuningad - Kings of Dance maailmatuur 2009". Käesoleva tuuri eripäraks on uus programm, millesse kuuluvad Nacho Duato, Jose Limoni, Frederick Ashtoni, Gabriel Faure, Christopher Wheeldoni, Roland Petit, Leonid Jakobsoni, Boris Eifmani tööd. Produtsent Sergei Daniljan

[Deutschland, Russland und das Baltikum] / Bogus̮aw Dyba{250}

Index Scriptorium Estoniae

Dyba{250}, Bogus̮aw

2006-01-01

Rets. rmt.: Deutschland, Russland und das Baltikum. Beiträge zu einer Geschichte wechselvoller Beziehungen. Festschrift zum 85. Geburtstag von Peter Krupnikow, hrsg. v. Florian Anton und Leonid Luks (=Schriften des Zentralinstituts für Mittel- und Osteuropastudien. Bd.7), Böhlau Verlag, Köln-Weimar-Wien, 2005

The Pulkovo Observatory in the last 50 years through the eyes of its Learned Secretary Yu. I. Vitinsky.

Science.gov (United States)

Zhukov, V. Yu.; Soboleva, T. V.

A solar physicist, a Pulkovo astronomer, Yury Ivanovich Vitinsky (1926-2003) was the author of 210 scientific papers known in both Russia and abroad. He worked in the Observatory for about half a century (1953-2002) and held the office of the Learned Secretary of the Russian Academy of Sciences Main Astronomical Observatory for 35 years (1965-2000). In the last years of his life, Vitinsky brought his recollections that he titled "My Pulkovo" to the Main Astronomical Observatory Archive. His memoirs narrate about problems of the astronomical science, staff members and deeds of Pulkovo, things he thought of an events he was through. This is the half-a-century history of the Pulkovo Observatory in biographies of persons. The writer of the Recollections mentions the names of fifty persons most of whom are the Main Astronomical Observatory staff members that he worked with side by side. The memoirs provide accurate descriptions that are brief yet rather capacious of the author's Pulkovo colleagues, as well as other astronomers. The language of Vitinsky's recollection is good and clear. His memoirs contain moderate balanced views of people and events and provide objective and trustworthy data. "My Pulkovo" is an indispensable biographical source for the historian of the astronomical science, the Pulkovo Observatory and its scholarly staff members of the most recent decades. It is also just an interesting human document. In 2006, Yury Ivanovich would have been eighty.

The beginning heights and light curves of high-altitude meteors

Czech Academy of Sciences Publication Activity Database

Koten, Pavel; Spurný, Pavel; Borovička, Jiří; Evans, S.; Elliott, A.; Betlem, H.; Štork, Rostislav; Jobse, K.

2006-01-01

Roč. 41, č. 9 (2006), s. 1305-1320 ISSN 1086-9379 R&D Projects: GA ČR GP205/02/P038 Institutional research plan: CEZ:AV0Z10030501 Keywords : bright Leonid meteors * atmospheric trajectories Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 2.524, year: 2006

The Politics of Drug Trafficking in Mexican and Mexico-Related Narconovelas

Science.gov (United States)

Palaversich, Diana

2006-01-01

This essay traces the emergence of the Mexican and Mexico-related narconovela. It examines perspectives on drug trafficking and traffickers expressed in novels by Elmer Mendoza, Leonides Alfaro, Gerardo Cornejo, Homero Aridjis, Arturo Perez-Reverte, and Paul Flores. The variety of positions taken refutes the tendency of the Mexican mainstream…

Interaction of Supernova Blast Waves with Wind-Driven Shells: Formation of "Jets", "Bullets", "Ears", Etc.

Science.gov (United States)

Gvaramadze, V. V.

Most of middle-aged supernova remnants (SNRs) have a distorted and complicated appearance which cannot be explained in the framework of the Sedov-Taylor model. We consider three typical examples of such SNRs (Vela SNR, MSH15-52, G309.2-00.6) and show that their structure could be explained as a result of interaction of a supernova (SN) blast wave with the ambient medium preprocessed by the action of the SN progenitor's wind and ionized emission.

Periodismo ruso en el exilio: Alexánder Ivánovich Herzen (1812-1870

Directory of Open Access Journals (Sweden)

Miguel Vázquez Liñán

2006-01-01

Full Text Available El siguiente artículo se interesa por la actividad periodística de Alexánder Ivánovich Herzen (Moscú, 1812 – París, 1870 y reproduce un texto suyo de 1857, que sirvió como presentación de una de sus publicaciones más representativas: Kólokol (La Campana.The following article analyses the journalistic work of Alexander Ivanovich Herzen,and reproduce one of his articles of 1857, specifically the introducction to Kolokol (The Bell, one of his most representative publications.

Tshto v imeni tebe mojom? / Leonid Surkov

Index Scriptorium Estoniae

Surkov, Leonid

1998-01-01

Liivi sõjas langenud Mustpeadele püstitatud mälestusmärgist Tallinnas Marta tänava ääres ja epitaafist Kiek in de Kökis, autoriks Tallinna meister Lambert Glandorf. Asula ja Magdaleena tänavatest Tallinnas : hoonetest

Elemental Abundances in Leonid and Perseid Meteoroids

Czech Academy of Sciences Publication Activity Database

Borovička, Jiří

2005-01-01

Roč. 95, 1-4 (2005), s. 245-253 ISSN 0167-9295. [Meteoroids 2004. London, Ontario, 16.08.2004-20.08.2004] R&D Projects: GA ČR GA205/02/0982 Institutional research plan: CEZ:AV0Z1003909 Keywords : meteors * meteoroids * spectroscopy Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 0.975, year: 2005

Video Observation of the Leonids 2001 Activity

Czech Academy of Sciences Publication Activity Database

Lin, C.L.; Abe, S.; Koten, Pavel; Yang, I.-Ch.

2012-01-01

Roč. 64, č. 1 (2012), 6/1-6/6 ISSN 0004-6264 Institutional research plan: CEZ:AV0Z10030501 Keywords : comet 55P/Tempel-Tuttle * interplanetary medium * meteors Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 2.439, year: 2012

KGB, Stasi ja Eesti luureajalugu / Ivo Juurvee

Index Scriptorium Estoniae

Juurvee, Ivo, 1979-

2008-01-01

Väidetest Saksa luure koostöö kohta Balti riikidega 1930ndatel aastatel. Nende väidete algallikatest ja paikapidavusest. Nimetatud väidete teaduskäibesse toojast Leonid Barkovist ja Barkovi väidete levitajatest ajalookirjanduses Edgar Siegfried Meosest ning Julius Maderist. Paljukorratud väidete usaldusväärseiks pidamise ohust

Perspectivas Pedagogicas. Documentos-Ponencias Y Ensayos Proyecto Teacher Corps, Ciclo XII (Pedagogical Perspectives. Documents, Papers and Essays, Teacher Corps Project, Cycle XII).

Science.gov (United States)

Albino, Isidra, Ed.; Davila, Sonia, Ed.

The purpose of this book is to stimulate ideas leading to a sharing of approaches, strategies, and methodologies applicable to the education of Puerto Ricans. Following introductory material, 18 papers are presented, the first 10 of which are in Spanish. Titles and authors are: (1) "El maestro que Puerto Rico necesita," Leonides Santos…

Mechanism design: theory and application to welfare-to-work programs

NARCIS (Netherlands)

Onderstal, S.

2008-01-01

In October 2007, Leonid Hurwicz , Eric Maskin, and Roger Myerson won the Nobel Prize in Economic Sciences "for having laid the foundations of mechanism design theory". My aim is to give you a flavor of what mechanism design theory is and how we can apply it in practice. More in particular, I will

Pantvangidraama Põhja-Osseetia keskkoolis / Kalev Vilgats

Index Scriptorium Estoniae

Vilgats, Kalev

2004-01-01

Põhja-Osseetia piirilinnas Beslanis võeti koolimaja koos õpilaste, õpetajate ja lapsevanematega pantvangi, hõivajad nõudsid läbirääkimistele Põhja-Osseetia presidenti Aleksandr Dzassohhovit, Inguššia presidenti Murat Zjazikovi ja doktor Leonid Roshali, et nende kaudu esitada nõudmised Inguššia võimude poolt vangistatud sisside vabastamiseks. Kaart: Põhja-Osseetia

2nd February 2011 - EPFL Vice President, Academic Affairs, P. Gillet signing the guest book with Director-General R. Heuer.

CERN Multimedia

Jean-Claude Gadmer

2011-01-01

On photograph 16: form left to right: Nicolas Guérin, Willy Zwaenepoel, Bastien Confino, Frédérick Bordry (CERN), Philippe Gillet, Benoît Deveaud-Plédran, Dominique Bonvin, Gérard Escher, Jacques Giovanola, Tatsuya Nakada, Stéphane Decoutère, Ambrogio Fasoli, Demetri Psaltis, Olivier Schneider, Aurelio Bay and Leonid Rivkin.

STS-96 Crew Training

Science.gov (United States)

1999-01-01

The training for the crew members of the STS-96 Discovery Shuttle is presented. Crew members are Kent Rominger, Commander; Rick Husband, Pilot; Mission Specialists, Tamara Jernigan, Ellen Ochoa, and Daniel Barry; Julie Payette, Mission Specialist (CSA); and Valery Ivanovich Tokarev, Mission Specialist (RSA). Scenes show the crew sitting and talking about the Electrical Power System; actively taking part in virtual training in the EVA Training VR (Virtual Reality) Lab; using the Orbit Space Vision Training System; being dropped in water as a part of the Bail-Out Training Program; and taking part in the crew photo session.

Elevated PYY is associated with energy deficiency and indices of subclinical disordered eating in exercising women with hypothalamic amenorrhea.

Science.gov (United States)

Scheid, Jennifer L; Williams, Nancy I; West, Sarah L; VanHeest, Jaci L; De Souza, Mary Jane

2009-02-01

The purpose of this study was twofold: (1) to determine if gastrointestinal hormones, associated with energy intake and energy balance, are altered in exercising women with hypothalamic amenorrhea and (2) to assess the association between gastrointestinal hormones and behavioural indicators of subclinical disordered eating in exercising women with hypothalamic amenorrhea. This cross-sectional study analyzed serum ghrelin, peptide YY (PYY), glucagon-like peptide-1 (GLP-1), menstrual status (by E1G and PdG), resting energy expenditure (REE), and subclinical eating behaviours in sedentary ovulatory (SedOv), exercising ovulatory (ExOv), and exercising amenorrheic (ExAmen) women. Groups were similar with respect to age (23.8+/-0.6 years) and BMI (21.4+/-0.3 kg/m(2)). The ratio of REE to predicted REE (REE:predicted REE) was 0.94+/-0.02, 0.94+/-0.02, and 0.88+/-0.02 in the SedOv, ExOv, and ExAmen groups, respectively. The REE:predicted REE in the ExAmen group was consistent with an energy deficiency. LogPYY, ghrelin, dietary cognitive restraint, and drive for thinness were elevated in the ExAmen group compared to other groups. GLP-1 concentrations were similar among groups. LogPYY correlated with drive for thinness and REE/FFM. In conclusion, fasting PYY and ghrelin concentrations are elevated in exercising women with FHA and both gastrointestinal peptides may serve as a proxy indicator of energy deficiency in this population.

Sadamaala konkurss : Tallinna kesklinnaga piirneva mereäärse ala parima linnaehitusliku kontseptsiooni saamiseks korraldatud arhitektuurivõistlus / Andres Alver, Margus Koot, Arvo Rikkinen...[jt.] ; interv. Triin Ojari

Index Scriptorium Estoniae

2000-01-01

Zürii liikmed konkursist, premeeritud töödest. Preemiad: I - Villem Tomiste, Veronika Valk; II - Illimar Truverk, Indrek Järve, Mattias Agabus, Tiit Sild, Karri Tiigisoon ning Toomas Paaver, Lauri Saar; III - Ivar Lubjak, Maria Pukk; ostud: Ott Kadarik, Rene Valner ning Siiri Vallner, Indrek Peil; täiendav ost (Muinsuskaitseamaet): Nikolai Serebrjakov, Leonid Tozil, Sergei Sevtsenko, Sulev Roosmaa. 6 illustratsiooni

Robert J. Aumann - matemaatikust Nobeli preemia laureaat / Peeter Puusemp

Index Scriptorium Estoniae

Puusemp, Peeter, 1947-

2006-01-01

2005. a. Nobeli preemia majanduse alal silmapaistva panuse eest mänguteooria ülesannete lahendamisse saanud Robert J. Aumannist ja D. Saari loetelu matemaatikutest - Nobeli preemia laureaatidest: John Nash'ist, Herbert Hauptman'ist, John Pople'ist, Bertrand Arthur William Russell'ist, Kenneth Joseph Arrow'ist, Gerard Debreu'ist, Leonid Vitaljevitš Kantorovitš'ist, Reinhard Selten'ist, Jan Tinbergen'ist

Projekt "Baltenet - The Baltic Technology Network" / Leonid Pai

Index Scriptorium Estoniae

Pai, Leonid

2005-01-01

Baltenet - The Baltic Technology Network on projekt, mille alusel teevad koostööd tehniliste erialade koolituse arendamiseks Baltimere äärsetes riikides neli kutseõppeasutust Soomest, Rootsist, Lätis ja Eestist. Projekti rahastab Euroopa Liidu Leonardo da Vinci programm

Kuidas sünnib pealkiri? / Pärt Lias

Index Scriptorium Estoniae

Lias, Pärt

2003-01-01

Eesti kirjanikud vastavad Pärt Liase küsimusele oma teoste pealkirjade saamisloo kohta: Doris Kareva, Ilona Laaman, Eha Lättemäe, Priidu Beier, Oskar Kruus, Jaan Kruusvall, Paul-Eerik Rummo ja Andres Vanapa (1); Triin Soomets, Priit Aimla, Aarne Puu, Einar Sander, Jüri Tuulik ja Ülo Tuulik (2); Nikolai Baturin, Leo Metsar, Toomas Vint, Leonid Stolovitš ja Pärt Lias (3)

Evaluation of Available Software for Reconstruction of a Structure from its Imagery

Science.gov (United States)

2017-04-01

scene and signature generation for ladar and imaging sensors, in Proc. SPIE 9071 Infrared Imaging System : Design , Analysis , Modeling, and Testing XXV...UNCLASSIFIED Evaluation of Available Software for Reconstruction of a Structure from its Imagery Leonid K Antanovskii Weapons and Combat Systems ...project. The Computer Vision System toolbox of MATLAB R© and the Visual Structure from Motion (VisualSFM) software are evaluated on three datasets of

Paradoxies and axioms of science in the creativity of Clim Ivanovich Churyumov

Science.gov (United States)

Steklov, A. F.; Vidmachenko, A. P.; Zhilyaev, B. E.; Dashkiev, G. N.; Svyatogorov, O. A.

2017-09-01

Key ideas of K.I. Churyumov and authors of the article on the development of astronomical research in Ukraine, creation of Ukrainian Institute for Advanced Studies; concerning special directions of interaction of astronomical observatories and the Armed Forces of Ukraine during the period of hybrid wars and methods of solving certain tasks of astrobiology, life of people on the planet Earth taking into account monthly rhythms and climatic seasons.

Nikolay Ivanovich Pirogov (1810-1881): A pioneering Russian surgeon and medical scientist.

Science.gov (United States)

Hendriks, Inge F; Bovill, James G; van Luijt, Peter A; Hogendoorn, Pancras Cw

2018-02-01

Nikolay Pirogov qualified as a physician from Moscow University in 1828 and then studied surgery and anatomy at University of Dorpat. He developed new surgical techniques, including the eponymous osteoplastic foot amputation. His application of scientifically based techniques extended surgery from a craft to a science. During the Crimean War he initiated the deployment of women as nurses and used triage for dealing with mass casualties. His textbook on field surgery became the standard reference on the subject and his principles remained virtually unchanged until the Second World War. Pirogov died on 5 December 1881 at his estate in Vishnya.

Review of advanced catheter technologies in radiation oncology brachytherapy procedures

OpenAIRE

Zhou J; Zamdborg L; Sebastian E

2015-01-01

Jun Zhou,1,2 Leonid Zamdborg,1 Evelyn Sebastian1 1Department of Radiation Oncology, Beaumont Health System, 2Oakland University William Beaumont School of Medicine, Royal Oak, MI, USA Abstract: The development of new catheter and applicator technologies in recent years has significantly improved treatment accuracy, efficiency, and outcomes in brachytherapy. In this paper, we review these advances, focusing on the performance of catheter imaging and reconstruction techniques in brachytherapy ...

The effect of SNR structure on non-equilibrium X-ray spectra

International Nuclear Information System (INIS)

Hamilton, A.J.S.; Sarazin, C.L.

1983-01-01

A technique is presented for characterizing the ionization structure and consequent thermal X-ray emission of a SNR when non-equilibrium ionization effects are important. The technique allows different theoretical SNR models to be compared and contrasted rapidly in advance of detailed numerical computations. In particular it is shown that the spectrum of a Sedov remnant can probably be applied satisfactorily in a variety of SNR structures, including the reverse shock model advocated by Chevalier (1982) for Type I SN, the isothermal similarity solution of Solinger, Rappaport and Buff (1975), and various inhomogenous or 'messy' structures. (Auth.)

The Composition of the Y2K Meteor

Science.gov (United States)

Coulson, S. G.

During the Leonid meteor shower of November 1999 a very bright meteor train, subsequently called the Y2K meteor, was observed. Analysis of the trajectory of the meteor suggests that it was composed of two distinct materials. The bulk of the meteor was composed of a comet-like material, while a much smaller fraction was of a denser carbonaceous material. A simple model is used to analytically determine the mass of the meteor fragments.

Что мешает развитию малого бизнеса: мнения предпринимателей

OpenAIRE

Веревкин, Леонид

2003-01-01

Leonid Verevkin in his commentary "Obstacles to the Small Business Development: Opinion of the Businessmen" states, "To assess the prospects for the development of small business in Russia, the Center for Social Forecasts held the all-Russia study in February-March 2003 in Moscow, St. Petersburg, Northern, Central, Central Chernozemny, Volgo-Vyatsky, North Caucasus, Urals, Western Siberian and Eastern Siberian territorial economic districts. The polls covered 1,200 experts — heads of small bu...

Some theoretic elements about vocational guidance in the specialty Carpintería

Directory of Open Access Journals (Sweden)

Odelmi Miló García

2016-03-01

Full Text Available Presently article the methodological conceptual theoretical bases are presented that sustain in an essential way the cultural historical theory, The objective of the same one is to elaborate a methodological strategy for the development of the professional orientation toward the specialty carpentry in students of the first year of the Polytechnic Leonides Blanco González, being given the problem that the students are not motivated by the specialty.

The impact of the form of the Euler equations for radial flow in cylindrical and spherical coordinates on numerical conservation and accuracy

Science.gov (United States)

Crittenden, P. E.; Balachandar, S.

2018-03-01

The radial one-dimensional Euler equations are often rewritten in what is known as the geometric source form. The differential operator is identical to the Cartesian case, but source terms result. Since the theory and numerical methods for the Cartesian case are well-developed, they are often applied without modification to cylindrical and spherical geometries. However, numerical conservation is lost. In this article, AUSM^+ -up is applied to a numerically conservative (discrete) form of the Euler equations labeled the geometric form, a nearly conservative variation termed the geometric flux form, and the geometric source form. The resulting numerical methods are compared analytically and numerically through three types of test problems: subsonic, smooth, steady-state solutions, Sedov's similarity solution for point or line-source explosions, and shock tube problems. Numerical conservation is analyzed for all three forms in both spherical and cylindrical coordinates. All three forms result in constant enthalpy for steady flows. The spatial truncation errors have essentially the same order of convergence, but the rate constants are superior for the geometric and geometric flux forms for the steady-state solutions. Only the geometric form produces the correct shock location for Sedov's solution, and a direct connection between the errors in the shock locations and energy conservation is found. The shock tube problems are evaluated with respect to feature location using an approximation with a very fine discretization as the benchmark. Extensions to second order appropriate for cylindrical and spherical coordinates are also presented and analyzed numerically. Conclusions are drawn, and recommendations are made. A derivation of the steady-state solution is given in the Appendix.

Dissipative quantum dynamics and nonlinear sigma-model

International Nuclear Information System (INIS)

Tarasov, V.E.

1992-01-01

Sedov variational principle which is the generalization of the least action principle for the dissipative and irreversible processes and the classical dissipative mechanics in the phase space is considered. Quantum dynamics for the dissipative and irreversible processes is constructed. As an example of the dissipative quantum theory the nonlinear two-dimensional sigma-model is considered. The conformal anomaly of the energy momentum tensor trace for closed bosonic string on the affine-metric manifold is investigated. The two-loop metric beta-function for nonlinear dissipative sigma-model was calculated. The results are compared with the ultraviolet two-loop conterterms for affine-metric sigma model. 71 refs

International Conference on Mathematical Methods in Electromagnetic Theory (MMET 2000), Volume 1 Held in Kharkov, Ukraine on September 12-15, 2000

Science.gov (United States)

2000-09-01

Proceedings 21 DECOMPOSITION APPROACH TO MULTILAYER CIRCUITS ELECTROMAGNETIC MODELING Anatoly Kirilenko1 , Protap Pramanick 2, Leonid Rud’, and Vladimir...number of zero elements. On the one hand , it leads to a more laborious algorithm and to greater time consumption. On the other hand , the determinants being...spectrum of TEM-modes much easier. At the real choice of dimensions of the "end steps", one should take into account two factors. On the one hand , it is

Gailit protesteerib : [August Gailiti kiri Valev Uibopuule 14. okt. 1956] / August Gailit

Index Scriptorium Estoniae

Gailit, August, 1891-1960

1998-01-01

Leonid Treti mälestuste käsikirjast 'A. H. Tammsaare, nagu teda tundsin'. Vastukajad: Siimisker, Leenu. Kultuuri, enam tekstikriitilist kultuuri // Sirp (1998) 13. märts, lk. 18-19 ; Treier, Elem. Klassiku teenimise kibe leib // Sirp (1998) 17. apr., lk. 14 ; Rebane, Hilve. Isikuloolisi lisandusi A. H. Tammsaare tundmisesse // Keel ja Kirjandus (1998) nr. 5, lk. 343-345 ; Kronberg, Janika. Kaanonid ja apokrüüfid // Keel ja Kirjandus (1998) nr. 8, lk. 563-564

Chilly Senate gives Carter a hard time

International Nuclear Information System (INIS)

Anon.

1979-01-01

Is the United States Senate about to deliver the final coup de grace to President Jimmy Carter Initial reaction from the Senate to Carter's Salt II agreement with Soviet Premier Leonid Brezhnev certainly points that way. The Salt II agreement still has to be submitted to a Senate that is as yet decidedly undecided about whether to ratify it. Washington sources indicate that 70 of the 100 senators are uncommitted, and 67 members must support the treaty if it is to be ratified

Translations on USSR Science and Technology Biomedical and Behavioral Sciences No. 47.

Science.gov (United States)

1978-10-27

problem is allowed to be simplified,, then the basic contents of the ergonomic section may be castrated ; if it is complicated, then the document will be...demands of agriculture. The rise of livestock farming does not mean only an increase in cattle stock, but also an increase in the productivity of... cattle and poultry. Leonid Il’yich Brezhnev stressed atthe July Plenum: "All that we want to have rom the animal husbandry is more meat, milk, and other

Dynamics and stability of relativistic gamma-ray-bursts blast waves

Science.gov (United States)

Meliani, Z.; Keppens, R.

2010-09-01

Aims: In gamma-ray-bursts (GRBs), ultra-relativistic blast waves are ejected into the circumburst medium. We analyse in unprecedented detail the deceleration of a self-similar Blandford-McKee blast wave from a Lorentz factor 25 to the nonrelativistic Sedov phase. Our goal is to determine the stability properties of its frontal shock. Methods: We carried out a grid-adaptive relativistic 2D hydro-simulation at extreme resolving power, following the GRB jet during the entire afterglow phase. We investigate the effect of the finite initial jet opening angle on the deceleration of the blast wave, and identify the growth of various instabilities throughout the coasting shock front. Results: We find that during the relativistic phase, the blast wave is subject to pressure-ram pressure instabilities that ripple and fragment the frontal shock. These instabilities manifest themselves in the ultra-relativistic phase alone, remain in full agreement with causality arguments, and decay slowly to finally disappear in the near-Newtonian phase as the shell Lorentz factor drops below 3. From then on, the compression rate decreases to levels predicted to be stable by a linear analysis of the Sedov phase. Our simulations confirm previous findings that the shell also spreads laterally because a rarefaction wave slowly propagates to the jet axis, inducing a clear shell deformation from its initial spherical shape. The blast front becomes meridionally stratified, with decreasing speed from axis to jet edge. In the wings of the jetted flow, Kelvin-Helmholtz instabilities occur, which are of negligible importance from the energetic viewpoint. Conclusions: Relativistic blast waves are subject to hydrodynamical instabilities that can significantly affect their deceleration properties. Future work will quantify their effect on the afterglow light curves.

Professional technical plantar ability in students of 1er year of the Agricultural specialty

Directory of Open Access Journals (Sweden)

Yonel Areces Mireles

2015-09-01

Full Text Available The present article which approaches on the problems as to the development of professional technical plantar ability in the Agricultural Specialty Polytechnic Leonides Blanco González. Splitting of a dialectic materialistic focus various methods were utilized and techniques: Theorists and empiricists, the ones that permitted going into the background and conception assumed for the treatment of professional technical ability like formation of the personality of the future agricultural worker, as well as determining the needs of developmental students of technical plantar ability.

Modeling of the Atmospheric Response to the Leonid Meteor Showers

National Research Council Canada - National Science Library

McNeil, William

1998-01-01

... showers of recent years. The model allows for ablation, deposition, diffusion and chemical dynamics, thereby permitting the computation of the modifications in the layers due to the showers in a self-consistent manner, based...

Activity of the Leonid meteor shower on 2009 November 17

Czech Academy of Sciences Publication Activity Database

Koten, Pavel; Borovička, Jiří; Kokhirova, G.I.

2011-01-01

Roč. 528, April (2011), A94/1-A94/4 ISSN 0004-6361 R&D Projects: GA ČR GA205/09/1302 Institutional research plan: CEZ:AV0Z10030501 Keywords : meteorites * meteors * meteoroids Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 4.587, year: 2011

Significance of Pirogov`s scientific ideas for modern organization of Public Health

Directory of Open Access Journals (Sweden)

Semenova L.S.

2015-03-01

Full Text Available This article is about Nikolay Ivanovich Pirogov, a surgeon and anatomist, prominent scientist and educator, founder of field surgery. He was the first to learn field surgery and military administration in practice. He was the first to use famous triage (the wounded were sorted according to the severity of injuries. N.I.Pirogov considered that well organized triage at dressing stations and temporary military hospitals is the main tool to provide proper care and to prevent harmful consequences. He organized training of medical nurses to help the wounded. He also published the work on the problems of pedagogy in which he proposed reforms of education system. The authors of the article have analyzed N.I.Pirogov`s works and showed their significance for modern social medicine and organization of Public Health.

The professional orientation to the masonry specialty: a system of activities

Directory of Open Access Journals (Sweden)

Jóse Andrés Gómez Torres

2018-03-01

Full Text Available The specialty Masonry in Technical and Vocational Education is of great importance given the mission that has to train workers who have to use the most efficient and updated techniques and technologies for the construction of buildings and other construction works. In the pedagogical practice manifested a contradiction expressed in the need to raise the quality of the professional training of the workers in the specialty Masonry, however, there were inadequacies in the work of professional guidance with students who attend the first year in the Polytechnical center "Leonides Blanco", reflected in the insufficient inclination towards the study profile, which led to the failure of a percentage of students. The objective of the work was to elaborate a system of activities that perfected the process of professional orientation towards the specialty Albañilería the first year at the "Leonides Blanco" PolytechnicCenter. In the investigative process, the dialectical-materialist method was assumed as the general method, which supported the theoretical methods, the application of statistical techniques that made possible the study and systematization of the theoretical and methodological foundations of the process under investigation. The practical significance is expressed in a system of activities that contributed to the professional orientation of the first-year students of the specialty Masonry, which guarantees a relevant initial training process, depending on the demands of the professional model and the needs educational and social

On the determination of the carbon balance of continents (Vladimir Ivanovich Vernadsky Medal Lecture)

Science.gov (United States)

Dolman, Albertus J. Han

2013-04-01

The carbon balance of regions, the size of continents, can be determined, albeit with significant uncertainty, by combining several bottom up and top down methods. The bottom up methods use eddy covariance techniques, biometric inventory measurements and modeling, while the top down methods use atmospheric observations and inverse models. There has been considerable progress in the last few years in determining these balances through more or less standard protocols, as highlighted for instance by studies of the REgional Carbon Cycle Assessment and Processes (RECAPP) project of the Global Carbon Project. Important areas where uncertainty creeps in are the scaling of point measurements in the bottom up methods, the sparseness of the observation network and the role of model and other errors in the inversion methods. Typically these balances hold for periods of several years. They therefore do not resolve the impact of anomalies in weather and climate directly. The role of management in these balances also differs for different continents. For instance in Europe management plays a strong role in the carbon balance, whereas for the Russian continent this is less important. Management in the European carbon balance may potentially override climatically driven variability. In contrast, for Russia, the importance of the role of forest is paramount, but there the vulnerability of the Arctic regions and permafrost is a key uncertainty for future behaviour. I hope to show the importance of these different aspects of the terrestrial carbon balance by comparing the two continents, and also discuss the significant uncertainty we still face in determining the carbon budgets of large areas. I will argue that we need to get a clearer picture of the role of management in these budgets, but also of the time variability of the budgets to be able to determine the impact of anomalous weather and the vulnerability in a future climate.

Gas crisis today and yesterday

International Nuclear Information System (INIS)

Anon

2009-01-01

Problem with natural gas prices and its transport from the Ukrainian territory to Europe have been occurring on regular basis. It all started soon after decline of the Soviet Union in 1992. In September 1992 a former Prime Minister Vitold Fodkin announced that the Ukraine would collect fees for goods (gas) transition in convertible currencies. According to him, the Ukraine needed a foreign currency, not roubles. Leonid Kravchuk, a former Ukrainian President President indicated that if the raw material prices increase, Kiev might complicate sale of pipes for gas and oil pipelines. (author)

Supernova blast wave within a stellar cluster outflow

Science.gov (United States)

Rodríguez-Ramírez, J. C.; Raga, A. C.; Velázquez, P. F.; Rodríguez-González, A.; Toledo-Roy, J. C.

2014-11-01

In this paper, we develop a semi-analytic model of a supernova which goes off in the centre of a stellar cluster. The supernova remnant interacts with a stratified, pre-existent outflow produced by the winds of the cluster stars. We compare our semi-analytic model with numerical simulations using the spherically symmetric Euler equations with appropriate mass and energy source terms. We find good agreement between these two approaches, and we find that for typical parameters the blast wave is likely to reach the Taylor-Sedov regime outside the cluster radius. We also calculate the predicted X-ray luminosity of the flow as a function of time, and we obtain its dependence on the outer radius and the number of stars of the cluster.

Observations of the 2009 Leonid activity by the Tajikistan fireball network

Czech Academy of Sciences Publication Activity Database

Kokhirova, G.I.; Borovička, Jiří

2011-01-01

Roč. 533, - (2011), A115/1-A115/6 ISSN 0004-6361 R&D Projects: GA ČR(CZ) GAP209/11/1382 Institutional research plan: CEZ:AV0Z10030501 Keywords : meteorites * meteors * meteoroids Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 4.587, year: 2011

Spetsoperatsija "Rossija". Rasklad sil / Kirill Kabanov, Mihhail Krasnov, Leonid Nikitinski...[jt.

Index Scriptorium Estoniae

2003-01-01

Bürokraatia Venemaal on oma kontrolli alla võtnud poliitika põhifunktsiooni - riigi arengustrateegia kujundamise. Riik, kus eksisteerib ainult üks poliitik, ei saa olla demokraatlik. Korruptsioon Venemaal. Eliiti ei ole ajalugu õpetanud, riigipöörded Venemaal ei lõpe vandenõulaste võidu, vaid kogu riigi kaotusega. Tulevikustsenaariumid

New type of radiation of bright Leonid meteors above 130 km

Czech Academy of Sciences Publication Activity Database

Spurný, Pavel; Betlem, H.; Jobse, K.; Koten, Pavel; van't Leven, J.

2000-01-01

Roč. 35, č. 5 (2000), s. 1109-1115 ISSN 0026-1114 R&D Projects: GA ČR GA205/00/1727; GA ČR GA205/99/0146; GA AV ČR KSK1003601 Institutional research plan: CEZ:AV0Z1003909 Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 3.168, year: 2000

The wave of the future - Searching for gravity waves

International Nuclear Information System (INIS)

Goldsmith, D.

1991-01-01

Research on gravity waves conducted by such scientists as Gamov, Wheeler, Weber and Zel'dovich is discussed. Particular attention is given to current trends in the theoretical analysis of gravity waves carried out by theorists Kip Thorne and Leonid Grishchuk. The problems discussed include the search for gravity waves; calculation of the types of gravity waves; the possibility of detecting gravity waves from localized sources, e.g., from the collision of two black holes in a distant galaxy or the collapse of a star, through the Laser Interferometer Gravitational Wave Observatory; and detection primordial gravity waves from the big bang

Psychosocial aspects of Mammary carcinoma

Directory of Open Access Journals (Sweden)

C. Searle

1980-09-01

Full Text Available Malignant neoplastic diseases in man are as old as mankind itself. The Hindu epic, Ramayana, dating back to c 2500 B C, described tumours and their treatment. Since then Hippocrates (c 460 - 375 B C, Celsus (c 30 B C - A D 38, Galen (c 130 - 200 A D and Leonides of Alexandria (c 180 A D, and numerous other scientists have studied and recorded these phenomena. Heller from the National Cancer Institute stressed that “Man’s attempt to understand cancer and to find ways of preventing, controlling and curing it began in ancient times”. (Heller, I960

Conjoined twins: scientific cinema and Pavlovian physiology.

Science.gov (United States)

Krementsov, Nikolai

2015-01-01

Through the lens of a 1957 documentary film, "Neural and humoral factors in the regulation of bodily functions (research on conjoined twins)," produced by the USSR Academy of Medical Sciences, this essay traces the entwined histories of Soviet physiology, studies of conjoined twins and scientific cinema. It examines the role of Ivan Pavlov and his students, including Leonid Voskresenkii, Dmitrii Fursikov and Petr Anokhin, in the development of "scientific film" as a particular cinematographic genre in Soviet Russia and explores numerous puzzles hidden behind the film's striking visuals. Crown Copyright © 2015. Published by Elsevier Ltd. All rights reserved.

THE TOMSK SCIENTIFIC SCHOOL OF NEUROLOGISTS. TO THE 120TH ANNIVERSARY OF THE DEPARTMENT OF NEUROLOGY AND NEUROSURGERY OF SIBERIAN STATE MEDICAL UNIVERSITY

Directory of Open Access Journals (Sweden)

V. M. Alifirova

2013-01-01

Full Text Available The history of the development of the Tomsk Scientific School Neurologists and the past and current events in the Department of Neurology and Neurosurgery of Siberian State Medical University are described. The Department of Neurology was established in 1881–1882. At a different times the department was headed by many great Russian physicians such as Michail G. Kurlov, Leonid I. Omorokov, Nikolay V. Schubin, Nikolay I. Komandenko. In addition to the academic work the department leads research in many fields of neurology, including movement disorders, cerebrovascular diseases, demyelinating and paroxysmal diseases. 

Diffuse remnants of supernova explosions of moving massive stars

Science.gov (United States)

Gvaramadze, V. V.

The modification of the ambient interstellar medium by the wind of massive stars (the progenitors of most of supernovae) results in that the structure and evolution of diffuse supernova remnants (SNRs) significantly deviate from those derived from standard models of SNRs based of the Sedov-Taylor solution. The stellar proper motion and the regular interstellar magnetic field affect the symmetry of the processed medium and cause the SNR to be non-spherically-symmetric. We show that taking into account these effects allows us to explain the diverse morphologies of the known SNRs (the particular attention is paid to the elongated axisymmetric SNRs and the SNRs consisting of two partially overlapping shells) and to infer the ``true" supernova explosion sites in some peculiar SNRs (therefore to search for new neutron stars associated with them).

Zadonshchina, Ryazan, and the Moscow Princely Family

Directory of Open Access Journals (Sweden)

Alexander V. Lavrentyev

2015-12-01

Full Text Available This paper is devoted to the history and controversies surrounding the outstanding representative of Russian medieval literature from the late 14th century, the famous Zadonshchina. This work glorifies the military victory of the united forces of the Russian troops, led by Grand Prince Dmitry Donskoy, over the Tatar army on 8 September 1380, at Kulikovo Field near the Don River. This article presents arguments in favor of a Ryazan origin of the Zadonshchina text; furthermore, the article offers an explanation of the presence in the text of two “protagonists,” Grand Prince Dmitry Ivanovich and his cousin, Vladimir Andreyevich the Bold, Prince of Serpukhov. The joint rule of the “brothers” was a result of deaths caused by the plague in the Moscow ruling house, which took the dynasty to the brink of extinction. This feature of the political situation is reflected in the Zadonshchina text.

Ancient Chinese Observations and Modern Cometary Models

Science.gov (United States)

Yeomans, D. K.

1995-12-01

Ancient astronomical observations by Chinese, Japanese, and Korean observers represent the only data source for discerning the long-term behavior of comets. The primary source material is derived from Chinese astrologers who kept a vigilant celestial watch in an effort to issue up-to-date astrological forecasts for the reigning emperors. Surprisingly accurate records were kept on cometary apparitions with careful notes being made of an object's position, motion, size, color, and tail length. For comets Halley, Swift-Tuttle, and Tempel-Tuttle, Chinese observations have been used to model their motions over two millennia and to infer their photometric histories. One general result is that active comets must achieve an apparent magnitude of 3.5 or brighter before they become obvious naked-eye objects. For both comets Halley and Swift-Tuttle, their absolute magnitudes and hence their outgassing rates, have remained relatively constant for two millennia. Comet Halley's rocket-like outgassing has consistently delayed the comet's return to perihelion by 4 days so that the comet's spin axis must have remained stable for at least two millennia. Although its outgassing is at nearly the same rate as Halley's, comet Swift-Tuttle's motion has been unaffected by outgassing forces; this comet is likely to be ten times more massive than Halley and hence far more difficult for rocket-like forces to push it around. Although the earliest definite observations of comet Tempel-Tuttle were in 1366, the associated Leonid meteor showers have been identified as early as A.D. 902. The circumstance for each historical meteor shower and storm have been used to guide predictions for the upcoming 1998-1999 Leonid meteor displays.

Exosat observations of the Kepler supernova remnant

International Nuclear Information System (INIS)

Smith, A.; Peacock, A.; Arnaud, M.; Ballet, J.; Rothenflug, R.

1989-01-01

The medium-energy experiment on board Exosat was used to measure the X-ray spectrum of the Kepler supernova remnant over the range 1.5-10 keV. An Fe emission line was clearly resolved with an energy of about 6.5 keV and equivalent width of about 1.8 keV. This was superposed on a continuum with a temperature of 5.0(+3.8, -1.9) keV. The medium-energy spectrum is shown to be consistent with a model in which the Kepler SNR is presently in a Sedov phase of evolution, the 5 keV continuum arises from the shocked interstellar/circumstellar medium, and thermal (but not ionization) equilibrium exists between electrons and ions behind the primary shock front. However, in this case, an overabundance of iron by more than 6 times cosmic is required. 28 refs

Leonid Brezhnev in Moldavia, 1950-52: the making of a GenSek?

Directory of Open Access Journals (Sweden)

Sandle, Mark

2016-12-01

Full Text Available This is the first article dealing specifically with Brezhnev in Soviet Moldavia. The article draws mainly on recently disclosed files from the Archive of the Social-Political Organizations of the Republic of Moldova, the former archive of the Central Committee of Communist Party of Moldavia. The authors are trying to understand the importance of the period when Brezhnev served as First Secretary of Central Committee of Moldavia from 1950 to 1952 for his subsequent career. In order to understand better the results of Brezhnev’s rule in Moldavian SSR and the impact on his leadership style, the authors discuss the previous career of Brezhnev as well as the activity of the previous First Secretaries in Soviet Moldavia. One of the main results of Brezhnev period in Moldavia was the consolidation of kolkhozes. In a broader sense, since this period at least, Brezhnev favoured quantity over quality.

STS-96 Crew Training, Mission Animation, Crew Interviews, STARSHINE, Discovery Rollout and Repair of Hail Damage

Science.gov (United States)

1999-01-01

Live footage shows the crewmembers of STS-96, Commander Kent V. Rominger, Pilot Rick D. Husband, Mission Specialists Ellen Ochoa, Tamara E. Jernigan, Daniel T. Barry, Julie Payette and Valery Ivanovich Tokarev during various training activities. Scenes include astronaut suit-up, EVA training in the Virtual Reality Lab, Orbiter space vision training, bailout training, and crew photo session. Footage also shows individual crew interviews, repair activities to the external fuel tank, and Discovery's return to the launch pad. The engineers are seen sanding, bending, and painting the foam used in repairing the tank. An animation of the deployment of the STARSHINE satellite, International Space Station, and the STS-96 Mission is presented. Footage shows the students from Edgar Allen Poe Middle School sanding, polishing, and inspecting the mirrors for the STARSHINE satellite. Live footage also includes students from St. Michael the Archangel School wearing bunny suits and entering the clean room at Goddard Space Flight Center.

Near-Earth Object (NEO) Hazard Background

Science.gov (United States)

Mazanek, Daniel D.

2005-01-01

The fundamental problem regarding NEO hazards is that the Earth and other planets, as well as their moons, share the solar system with a vast number of small planetary bodies and orbiting debris. Objects of substantial size are typically classified as either comets or asteroids. Although the solar system is quite expansive, the planets and moons (as well as the Sun) are occasionally impacted by these objects. We live in a cosmic shooting gallery where collisions with Earth occur on a regular basis. Because the number of smaller comets and asteroids is believed to be much greater than larger objects, the frequency of impacts is significantly higher. Fortunately, the smaller objects, which are much more numerous, are usually neutralized by the Earth's protective atmosphere. It is estimated that between 1000 and 10,000 tons of debris fall to Earth each year, most of it in the form of dust particles and extremely small meteorites. With no atmosphere, the Moon's surface is continuously impacted with dust and small debris. On November 17 and 18, 1999, during the annual Leonid meteor shower, several lunar surface impacts were observed by amateur astronomers in North America. The Leonids result from the Earth's passage each year through the debris ejected from Comet Tempel-Tuttle. These annual showers provide a periodic reminder of the possibility of a much more consequential cosmic collision, and the heavily cratered lunar surface acts a constant testimony to the impact threat. The impact problem and those planetary bodies that are a threat have been discussed in great depth in a wide range of publications and books, such as The Spaceguard Survey , Hazards Due to Comets and Asteroids, and Cosmic Catastrophes. This paper gives a brief overview on the background of this problem and address some limitations of ground-based surveys for detection of small and/or faint near-Earth objects.

The breast: from Ancient Greek myths to Hippocrates and Galen.

Science.gov (United States)

Iavazzo, C R; Trompoukis, C; Siempos, I I; Falagas, M E

2009-01-01

This is a historical article about Ancient Greek literature from mythological times until the first centuries AD with regard to the female breast. We endeavoured to collect several elegant narratives on the topic as well as to explore the knowledge of Ancient Greek doctors on the role, physiology and pathology of breast and the treatment of its diseases. We identified such descriptions in myths regarding Amazons, Hercules, Zeus, Hera and Amaltheia. Furthermore, descriptions on the topic were also found in the work of Hippocrates, Aristoteles, Soranos, Alexander of Aphrodisias, Celsus, Archigenis, Leonides, Galen and Oribasius. We may conclude that some of today's medical knowledge or practice regarding the breast was also known in the historical period.

Observational study of ion-electron equilibration and of cloud evaporation in supernova remnants under the HEAO-2 guest investigator program. Final project report, 1 June 1985-30 September 1986

International Nuclear Information System (INIS)

Teske, R.G.

1986-09-01

Observations of three selected supernovae remnants (Cygnus Loop, IC 443, and Puppis A) were made in the forbidden coronal iron lines (Fe X) lambda 6374 and (Fe XIV) lambda 5303. The resulting data was compared quantitatively with Einstein images of the same objects, and an attempt was made to determine (a) the process by which ion and electron energies are equilibrated behind the shock front in the ISM and (b) whether cloud evaporation occurs within the hot remnant interiors. Spatially-resolved x-ray emission were modeled for Sedov-Taylor blast wave models of supernovae remnants (SNR) under conditions of non-equlibrium ionization. The computations are intended to provide results that can be directly compared with Einstein high resolution image (HRI) and imaging proportional counter (IPS) data. The computer program for predicting the spatial distribution of HRI and IPS counting rates was completed, and final testing of it had begun

DISCOVERY OF X-RAY EMISSION FROM AND DISTANCE TO THE SUPERNOVA REMNANT G84.2-0.8

Energy Technology Data Exchange (ETDEWEB)

Leahy, Denis A.; Green, Kaylie S., E-mail: leahy@ucalgary.ca, E-mail: ksgreen@ucalgary.ca [Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, T2N 1N4 (Canada)

2012-11-20

We analyze X-ray and radio observations of the supernova remnant G84.2-0.8. 1420 MHz atomic hydrogen (H I) line and radio continuum data yield H I absorption spectra and a new H I absorption distance of 5.8-6.2 kpc. Archival X-ray observations from ROSAT and Chandra which cover the area including G84.2-0.8 are analyzed to show extended X-ray emission from G84.2-0.8. Fits to X-ray spectra from Chandra, with the new H I distance of 5.8-6.2 kpc, are used to determine the Sedov parameters of the supernova remnant. G84.2-0.8 is large (16-18 pc radius), middle aged ({approx}9000 yr), expanding in low-density interstellar medium (0.02 cm{sup -3}), and consistent with a low explosion energy (0.8-6.5 Multiplication-Sign 10{sup 50} erg).

Obituary: Kenneth L. Franklin, 1923-2007

Science.gov (United States)

Rao, Joe; Degrasse Tyson, Neil

2007-12-01

Renowned astronomer and astronomy popularizer Kenneth L. Franklin died early Monday morning, June 18, 2007, in Boulder, Colorado, two weeks after undergoing heart surgery. He was 84 years old. Kenneth Linn Franklin, the only child of Myles and Ruth (Houston) Franklin, was born March 25, 1923 in Alemeda, California. Ken obtained his Ph.D. in astronomy in 1953 at the University of California, Berkeley. From 1954 to 1956 he was a research fellow in radio astronomy at the Department of Terrestrial Magnetism, Carnegie Institution of Washington, DC. While there, he and Bernard F. Burke discovered radio emissions from the planet Jupiter. They announced their find on April 6, 1955, at a meeting of the American Astronomical Society (AAS). In 1956 Ken joined the staff of the American Museum-Hayden Planetarium, where he later served as chairman and chief scientist. Over the course of thirty years he wrote and/or presented innumerable sky shows for the planetarium sky theater, taught popular and technical courses in astronomy, and answered questions from the public. Ken was frequently consulted by local industries engaged in the space program, as well as by the news media and publishers. He was often interviewed on local and national radio and television, especially when a celestial event of special interest was due to occur. On the first page of the November 1966 issue of Sky & Telescope, in comments about the upcoming Leonid meteor shower, Franklin stuck his neck out. Based on some calculations that he'd made, he said he felt we were going to be in for a "interesting display." His was one of the few forecasts that suggested the '66 Leonids might be memorable. As it turned out, he was right — that year observers experienced the now-legendary Leonid meteor storm. From 1973 to 1979, Ken was the AAS's public-affairs officer. For two decades he also served in the society's Harlow Shapley Visiting Lecturer Program, speaking at one or two colleges each year. Ken was an active

Detection of the N2+ first negative system in a bright Leonid fireball

Czech Academy of Sciences Publication Activity Database

Abe, S.; Ebizuka, N.; Yano, H.; Watanabe, J.; Borovička, Jiří

2005-01-01

Roč. 618, č. 2 (2005), L141-L144 ISSN 0004-637X Institutional research plan: CEZ:AV0Z1003909 Keywords : meteors * molecular process * astrobiology Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 6.308, year: 2005

A method based on a separation of variables in magnetohydrodynamics (MHD); Une methode de separation des variables en magnetohydrodynamique

Energy Technology Data Exchange (ETDEWEB)

Cessenat, M.; Genta, P.

1996-12-31

We use a method based on a separation of variables for solving a system of first order partial differential equations, in a very simple modelling of MHD. The method consists in introducing three unknown variables {phi}1, {phi}2, {phi}3 in addition of the time variable {tau} and then searching a solution which is separated with respect to {phi}1 and {tau} only. This is allowed by a very simple relation, called a `metric separation equation`, which governs the type of solutions with respect to time. The families of solutions for the system of equations thus obtained, correspond to a radial evolution of the fluid. Solving the MHD equations is then reduced to find the transverse component H{sub {Sigma}} of the magnetic field on the unit sphere {Sigma} by solving a non linear partial differential equation on {Sigma}. Thus we generalize ideas due to Courant-Friedrichs and to Sedov on dimensional analysis and self-similar solutions. (authors).

A method based on a separation of variables in magnetohydrodynamics (MHD)

International Nuclear Information System (INIS)

Cessenat, M.; Genta, P.

1996-01-01

We use a method based on a separation of variables for solving a system of first order partial differential equations, in a very simple modelling of MHD. The method consists in introducing three unknown variables φ1, φ2, φ3 in addition of the time variable τ and then searching a solution which is separated with respect to φ1 and τ only. This is allowed by a very simple relation, called a 'metric separation equation', which governs the type of solutions with respect to time. The families of solutions for the system of equations thus obtained, correspond to a radial evolution of the fluid. Solving the MHD equations is then reduced to find the transverse component H Σ of the magnetic field on the unit sphere Σ by solving a non linear partial differential equation on Σ. Thus we generalize ideas due to Courant-Friedrichs and to Sedov on dimensional analysis and self-similar solutions. (authors)

Influence of the laser parameters on the space and time characteristics of an aluminum laser-induced plasma

International Nuclear Information System (INIS)

Barthelemy, O.; Margot, J.; Chaker, M.; Sabsabi, M.; Vidal, F.; Johnston, T.W.; Laville, S.; Le Drogoff, B.

2005-01-01

In this work, an aluminum laser plasma produced in ambient air at atmospheric pressure by laser pulses at a fluence of 10 J/cm 2 is characterized by time- and space-resolved measurements of electron density and temperature. Varying the laser pulse duration from 6 ns to 80 fs and the laser wavelength from ultraviolet to infrared only slightly influences the plasma properties. The temperature exhibits a slight decrease both at the plasma edge and close to the target surface. The electron density is found to be spatially homogeneous in the ablation plume during the first microsecond. Finally, the plasma expansion is in good agreement with the Sedov's model during the first 500 ns and it becomes subsonic, with respect to the velocity of sound in air, typically 1 μs after the plasma creation. The physical interpretation of the experimental results is also discussed to the light of a one-dimensional fluid model which provides a good qualitative agreement with measurements

Improved optical spectrophotometry of supernova remnants in M33

Science.gov (United States)

Blair, W. P.; Kirshner, R. P.

1985-01-01

Optical spectra of SNRs in M33 have been used to investigate abundance gradients and SNR evolution in this galaxy. Abundances of O, N, and S are derived from the spectra using new shock models by Dopita et al. (1984). The results for N and S show abundance gradients similar to those in NGC 300 and the Galaxy. The O abundances may be affected by possible contamination from H II regions and low-velocity shocks. Electron densities derived from the forbidden S II 6717 A/6731 A line ratio are used with a pressure equilibrium argument to estimate the initial explosion energy for each SNR. Evolutionary models for the remnants are investigated, and the distribution of the number of remnants with diameter is found to be consistent with free expansion of the SNRs to diameters of about 26 pc. The results may also be consistent with Sedov evolution if the ranges of initial supernova energies and surrounding interstellar medium densities are large enough.

Three-dimensional simulations of supernovae dominated interstellar media in disk galaxies

International Nuclear Information System (INIS)

Cioffi, D.F.

1985-01-01

Evolution of the interstellar media of spiral galaxies was studied, assuming that their dynamical and thermal properties are dominated by supernova remnants (SNRs). To do this, a computer simulation was developed that uses standard SNR evolutionary solutions (Sedov-Taylor, pressure-modified snowplow) to redistribute mass and energy throughout a rectangular, three-level grid which models the interstellar medium (ISM). This comprehensive treatment includes bremsstrahlung or metal cooling, the creation and evaporation of clouds, mass injection and return from a galactic halo, multiple SNRs, and internally determined SNR lifetimes. The importance of spatially correlating supernovae sites, which can increase the global evolution rate of the (ISM), is confirmed. The simulations of primeval (zero metal abundance) galaxies revealed that the enhancement ability of bremsstrahlung-cooled SNR to transport mass can continually agitate the ISM, preventing the establishment of long-lived tunnel networks (i.e., hot rarefied volumes). This demonstrated the inadequacy of porosity theory for predicting the topology of the ISM, because it does not account for mass transport

Dynamics of ionizing shock waves on adiabatic motions of gases

International Nuclear Information System (INIS)

Zorev, N.N.; Sklizkov, G.V.; Shikanov, A.S.

1982-01-01

Results are presented of an experimental investigation of free (adiabatic) motion of a spherical ionizing wave in deuterium produced by an expanding laser plasma. It is shown that the discrepancy between the free movement of shock waves (which lead to total ionization of the gas) and the Sedov-Taylor model of a spontaneous point explosion is not related to variations in the adiabat exponent γ and the motion occurs for a constant γ=5/3. The effect is ascribed to the influence of the shock wave front structure on the dynamics of its propagation. An analytic expression for the motion of symmetric ionizing shock waves is found which has an accuracy of better than 1%. As a result the adiabat exponent was determined experimentally. A method for determining the energy of a shock wave on the basis of its dynamics of motion is developed which has an accuracy of approximately 5% [ru

A Lagrangian meshfree method applied to linear and nonlinear elasticity.

Science.gov (United States)

Walker, Wade A

2017-01-01

The repeated replacement method (RRM) is a Lagrangian meshfree method which we have previously applied to the Euler equations for compressible fluid flow. In this paper we present new enhancements to RRM, and we apply the enhanced method to both linear and nonlinear elasticity. We compare the results of ten test problems to those of analytic solvers, to demonstrate that RRM can successfully simulate these elastic systems without many of the requirements of traditional numerical methods such as numerical derivatives, equation system solvers, or Riemann solvers. We also show the relationship between error and computational effort for RRM on these systems, and compare RRM to other methods to highlight its strengths and weaknesses. And to further explain the two elastic equations used in the paper, we demonstrate the mathematical procedure used to create Riemann and Sedov-Taylor solvers for them, and detail the numerical techniques needed to embody those solvers in code.

Conference on the structure and model of the first cell. The Alexander Ivanovich Oparin 100th Anniversary Conference

International Nuclear Information System (INIS)

1994-08-01

The report includes 17 summaries of the papers presented at the Third Trieste Conference on Chemical Evolution concerning the structure and model of the first cell which was the central theme of the conference. A separate indexing is provided for each summary. Refs and figs

Leonid Apananski müüs AB Grupi maa oma firmale / Silva Männik

Index Scriptorium Estoniae

Männik, Silva, 1974-

1999-01-01

Ilmunud ka: Den za Dnjom Nov/26 lk. 8. Apananski müüs AB Kindlustuse Grupile kuulunud Maakri tänava kinnistu. Skeem: AB Grupist on välja viidud ligikaudu 70 milj. krooni. Ilmunud ka: Den za Dnjom 23. nov. lk. 3

Mother as Donor, Hero or Villain: New Sides of the Mother's Image in Sergey Sedov's "Fairy Tales about Mums"

Science.gov (United States)

Gubaidullina, Anastasia N.; Gorenintseva, Valentina N.

2017-01-01

A new model of society in post-Soviet Russia introduced novel family patterns to everyday life as well as to children's literature, with traditional parent and children's functions becoming subject to rethinking. The tendency to reconsider parental functions can be observed in texts from different genres, but it appears most overtly in modern…

Statistical relationship between the succeeding solar flares detected by the RHESSI satellite

Science.gov (United States)

Balázs, L. G.; Gyenge, N.; Korsós, M. B.; Baranyi, T.; Forgács-Dajka, E.; Ballai, I.

2014-06-01

The Reuven Ramaty High Energy Solar Spectroscopic Imager has observed more than 80 000 solar energetic events since its launch on 2002 February 12. Using this large sample of observed flares, we studied the spatiotemporal relationship between succeeding flares. Our results show that the statistical relationship between the temporal and spatial differences of succeeding flares can be described as a power law of the form R(t) ˜ tp with p = 0.327 ± 0.007. We discuss the possible interpretations of this result as a characteristic function of a supposed underlying physics. Different scenarios are considered to explain this relation, including the case where the connectivity between succeeding events is realized through a shock wave in the post Sedov-Taylor phase or where the spatial and temporal relationship between flares is supposed to be provided by an expanding flare area in the sub-diffusive regime. Furthermore, we cannot exclude the possibility that the physical process behind the statistical relationship is the reordering of the magnetic field by the flare or it is due to some unknown processes.

Revised Distances to 21 Supernova Remnants

Science.gov (United States)

Ranasinghe, S.; Leahy, D. A.

2018-05-01

We carry out a comprehensive study of H I 21 cm line observations and 13CO line observations of 21 supernova remnants (SNRs). The aim of the study is to search for H I absorption features to obtain kinematic distances in a consistent manner. The 21 SNRs are in the region of sky covered by the Very Large Array Galactic Plane Survey (H I 21 cm observations) and Galactic Ring Survey (13CO line observations). We obtain revised distances for 10 SNRs based on new evidence in the H I and 13CO observations. We revise distances for the other 11 SNRs based on an updated rotation curve and new error analysis. The mean change in distance for the 21 SNRs is ≃25%, i.e., a change of 1.5 kpc compared to a mean distance for the sample of 6.4 kpc. This has a significant impact on interpretation of the physical state of these SNRs. For example, using a Sedov model, age and explosion energy scale as the square of distance, and inferred ISM density scales as distance.

Irreversible Aspects of Continuum Mechanics and Transfer of Physical Characteristics in Moving Fluids : Symposia

CERN Document Server

Sedov, L

1968-01-01

At its meeting on April 23, 1965 in Paris the Bureau of IUTAM decided to have a Symposium on the Irreversible Aspects of Continaum Mechanics held in June 1966 in Vienna. In addition, a Symposium on the Transfer of Physical Characteristics in Moving Fluids which, orig­ inally, had been scheduled to take place in Stockholm was rescheduled to be held in Vienna immediately following the Symposium on the Irre­ versible Aspects of Continuum Mechanics. It was felt that the subjects of the two symposia were so closely related that participants should be given an opportunity to attend both. Both decisions were unanimously approved by the members of the General Assembly of IUTAM. Prof. H. PARKUS, Vienna, was appointed Chairman of the Symposium on the Irreversible Aspects, and Prof. L. I. SEDOV, Moscow, was appointed Chairman of the Symposium on the Transfer of Physical Characteristics, with Prof. P ARKUS being re­ sponsible for the local organization of both symposia. In accordance with the policy set forth by IUTAM...

On the generation of a bubbly universe - A quantitative assessment of the CfA slice

Science.gov (United States)

Ostriker, J. P.; Strassler, M. J.

1989-01-01

A first attempt is made to calculate the properties of the matter distribution in a universe filled with overlapping bubbles produced by multiple explosions. Each spherical shell follows the cosmological Sedov-Taylor solution until it encounters another shell. Thereafter, mergers are allowed to occur in pairs on the basis of N-body results. At the final epoch, the matrix of overlapping shells is populated with 'galaxies' and the properties of slices through the numerically constructed cube compare well with CfA survey results for specified initial conditions. A statistic is found which measures the distance distribution from uniformly distributed points to the nearest galaxies on the projected plane which appears to provide a good measure of the bubbly character of the galaxy distribution. In a quantitative analysis of the CfA 'slice of the universe', a very good match is found between simulation and the real data for final average bubble radii of (13.5 + or - 1.5)/h Mpc with formal filling factor 1.0-1.5 or actual filling factor of 65-80 percent.

Generation of a bubbly universe - a quantitative assessment of the CfA slice

International Nuclear Information System (INIS)

Ostriker, J.P.; Strassler, M.J.

1989-01-01

A first attempt is made to calculate the properties of the matter distribution in a universe filled with overlapping bubbles produced by multiple explosions. Each spherical shell follows the cosmological Sedov-Taylor solution until it encounters another shell. Thereafter, mergers are allowed to occur in pairs on the basis of N-body results. At the final epoch, the matrix of overlapping shells is populated with 'galaxies' and the properties of slices through the numerically constructed cube compare well with CfA survey results for specified initial conditions. A statistic is found which measures the distance distribution from uniformly distributed points to the nearest galaxies on the projected plane which appears to provide a good measure of the bubbly character of the galaxy distribution. In a quantitative analysis of the CfA 'slice of the universe', a very good match is found between simulation and the real data for final average bubble radii of (13.5 + or - 1.5)/h Mpc with formal filling factor 1.0-1.5 or actual filling factor of 65-80 percent. 25 references

Time-resolved dynamics of nanosecond laser-induced phase explosion

International Nuclear Information System (INIS)

Porneala, Cristian; Willis, David A

2009-01-01

Visualization of Nd : YAG laser ablation of aluminium targets was performed by a shadowgraph apparatus capable of imaging the dynamics of ablation with nanosecond time resolution. Direct observations of vaporization, explosive phase change and shock waves were obtained. The influence of vaporization and phase explosion on shock wave velocity was directly measured. A significant increase in the shock wave velocity was observed at the onset of phase explosion. However, the shock wave behaviour followed the form of a Taylor-Sedov spherical shock below and above the explosive phase change threshold. The jump in the shock wave velocity above phase explosion threshold is attributed to the release of stored enthalpy in the superheated liquid surface. The energy released during phase explosion was estimated by fitting the transient shock wave position to the Taylor scaling rules. Results of temperature calculations indicate that the vapour temperature at the phase explosion threshold is slightly higher than the critical temperature at the early stages of the shock wave formation. The shock wave pressure nearly doubled when transitioning from normal vaporization to phase explosion.

Qualitative and quantitative analysis of arsenic and mercury in human remains of the XVI-XVII centuries from the Moscow Kremlin necropolises by neutron activation analysis at the IREN facility and the IBR-2 reactor of FLNP, JINR

International Nuclear Information System (INIS)

Panova, T.D.; Dmitriev, A.Yu.; Borzakov, S.B.; Khramko, K.

2017-01-01

The neutron activation analysis (NAA) of three samples of human remains of the XVI-XVII centuries from the necropolises of the Moscow Kremlin has been carried out at FLNP JINR. The samples were irradiated at two facilities: at the IREN source of resonance neutrons and at the IBR-2 reactor. Spectra of induced activity of the irradiated samples were measured by using the automatic measurement system developed at FLNP JINR. This system consists of a high-purity germanium detector with spectrometric electronics, a sample changer, and a control software. Mass fractions of arsenic, mercury and other elements were calculated by relative and absolute NAA methods. The obtained values confirmed the fact of an acute mercury poisoning of the first wife of Tsar Ivan Vasilievich the Terrible - Tsarina Anastasia Romanovna. Increased mercury content was detected in the bone remains of the son of Tsar Ivan the Terrible, Tsarevich Ivan Ivanovich, and Prince M. V. Skopin-Shuisky. The obtained results allow us to introduce into scientific circulation the exact values of mass fraction of mercury, arsenic and some other elements in the samples from the graves of Russian historical figures of the second half of XVI - early XVII centuries. [ru

Reaching for Success: Picasso’s Rise in the Market (The First Two Decades

Directory of Open Access Journals (Sweden)

Enrique Mallen

2017-04-01

Full Text Available This article explores the exhibitions of Picasso’s works in the first two decades of his artistic career, as well as the dealers and collectors who came into contact with them. It describes the relationship between Picasso and his first dealers, Pere Manyach, Berthe Weill, Clovis Sagot, Père Soulier, Ambroise Vollard, Daniel-Henry Kahnweiler, Georg Caspari, L. W. Guthier, Hans Goltz, Heinrich Thannhauser, Otto Feldmann, Alfred Flechtheim, Emil Richter, Gottfried Tanner, Michael Brenner, R. J. Coady, Léonce Rosenberg, Paul Rosenberg, etc.; as well as his first collectors, Leo and Gertrude Stein, Olivier Sainsère, Joachim Gasquet, Wilhelm Uhde, Herman Rupf, Vincenc Kramář, Frank Stoop, Hugo Perls, Edwin Suermondt, Dr. Paul Ferdinand Schmidt, Princess Mechtilde Lichnowsky, Henry Simms, Ludwig and Rosy Fischer, Professor Wilhelm Kreis, Adolf Erblösch, Justin K. Thannhauser, Sergei Ivanovich Shchukin, Ivan A. Morosov, etc. It also identifies all important Picasso expositions in this time period and how those dealers and collectors were involved in their arrangement. The information provided here has been excerpted from an exhaustive study of the critical literature on Pablo Picasso, as well as from published exhibition catalogues.

Üldohtlik viis, kahe või enama isiku tapmine ja omakasu motiiv kui mõrva tunnused. Riigikohtu kriminaalkolleegiumi otsus asjas 3-1-1-36-09 / Elina Elkind

Index Scriptorium Estoniae

Elkind, Elina, 1982-

2009-01-01

Riigikohtu lahendist 3-1-1-36-09: Nikolai Galkovski kaitsja vandeadvokaat Anatoli Jaroslavski, Andrei Grišini kaitsja vandeadvokaat Leonid Olovjanišnikovi, Aleksandr Semjonovi kaitsja vandeadvokaat Oleg Nišajevi ja Dmitri Štšerbakovi kaitsja vandeadvokaat Toomas Alpi kassatsioonid Tallinna Ringkonnakohtu 24. novembri 2008. a kohtuotsuse peale kriminaalasjas Andrei Grišini süüdistuses KarS § 114 p-de 2, 3 ja 5 ja § 22 lg-te 2 ja 3, Dmitri Štšerbakovi süüdistuses KarS § 114 p-de 2, 3 ja 5, Aleksandr Semjonovi süüdistuses KarS § 114 p-de 2, 3 ja 5 ning Nikolai Galkovski süüdistuses KarS § 257, § 114 p-de 2, 3 ja 5 ja § 22 lg 3 järgi

HISTORY OF FORMATION AND PROSPECTS FOR DEVELOPMENT OF BELARUSIAN SCIENTIFIC CHEMICAL ANT THERMAL TREATMENT SCHOOL

Directory of Open Access Journals (Sweden)

N. I. Ivanitsky

2007-01-01

Full Text Available History of the «Material Science in Mechanical Engineering»” accounts for more than 40 years and by right it can be called a history of the Belarusian School of Metal Science Specialists. One of the founders of the Scientific School of Belarusian Metal Science Specialists has been Professor Leonid Grigorievich Voroshnine, double N.A. Minkevich prize-winner, Doctor of Technical Sciences, Head of the Department. Under his leadership and as a result of his personal participation more than 100 new diffusion coatings of multi- and special purposes such as heat-resistant, wear-resistant, anti-corrosive, cavitation- resistant have been developed. The papers written by the Department scientists are well known and they are generally recognized as classical books on chemical and thermal treatment. Nowadays the Scientific School created by Professor Voroshnine L.G is successfully working.

Ground-based multi-station spectroscopic imaging with ALIS. - Scientific highlights, project status and future prospects

Science.gov (United States)

Brändström; Gustavsson, Björn; Pellinen-Wannberg, Asta; Sandahl, Ingrid; Sergienko, Tima; Steen, Ake

2005-08-01

The Auroral Large Imaging System (ALIS) was first proposed at the ESA-PAC meeting in Lahnstein 1989. The first spectroscopic imaging station was operational in 1994, and since then up to six stations have been in simultaneous operation. Each station has a scientific-grade CCD-detector and a filter-wheel for narrow-band interference-filters with six positions. The field-of-view is around 70°. Each imager is mounted in a positioning system, enabling imaging of a common volume from several sites. This enables triangulation and tomography. Raw data from ALIS is freely available at ("http://alis.irf.se") and ALIS is open for scientific colaboration. ALIS made the first unambiguous observations of Radio-induced optical emissions at high latitudes, and the detection of water in a Leonid meteor-trail. Both rockets and satellite coordination are considered for future observations with ALIS.

Budapesti memorandumid julgeolekutagatiste kohta, 1994 / Leonid Kutšma, Boriss Jeltsin, John Major, William Clinton

Index Scriptorium Estoniae

2014-01-01

Ukraina, Venemaa ja Ameerika Ühendriikide president ning Ühendkuningriigi peaminister allkirjastasid 5. detsembril 1994 seoses Ukraina ühinemisega tuumarelvade tõkestamise lepinguga kolm memorandumit. Väljavõte

The 1996 Leonid shower as studied with a potassium lidar: Observations and inferred meteoroid sizes

Science.gov (United States)

Höffner, Josef; von Zahn, Ulf; McNeil, William J.; Murad, Edmond

1999-02-01

We report on the observation and analysis of meteor trails that are detected by ground-based lidar tuned to the D1 fine structure line of K. The lidar is located at Kühlungsborn, Germany. The echo profiles are analyzed with a temporal resolution of about 1 s and altitude resolution of 200 m. Identification of meteor trails in the large archive of raw data is performed with help of an automated computer search code. During the peak of the Lenoid meteor shower on the morning of November 17, 1996, we observed seven meteor trails between 0245 and 0445 UT. Their mean altitude was 89.0 km. The duration of observation of individual trails ranges from 3 s to ~30 min. We model the probability of observing a meteor trail by ground-based lidar as a function of both altitude distribution and duration of the trails. These distributions depend on the mass distribution, entry velocity, and entry angle of the meteoroids, on the altitude-dependent chemical and dynamical lifetimes of the released K atom, and on the absolute detection sensitivity of our lidar experiment. From the modeling, we derive the statistical likelihood of detection of trails from meteoroids of a particular size. These bracket quite well the observed trails. The model also gives estimates of the probable size of the meteoroids based on characteristics of individual trails.

Grafica de carte din RSS Moldovenească în perioada de instaurare a realismului socialist (1940–1953

Directory of Open Access Journals (Sweden)

Victoria Rocaciuc

2016-10-01

Full Text Available Initially, the publishing processes in the MASSR and Bessarabia of the interwar period developed completely differently in the aesthetic and ideological scope. Their unification is observed after 1940. In the art of book graphics of the Moldavian Soviet Socialist Republic, the transition to socialist realism was characterized by documentation and the domination of illustration characteristics, accumulation of professional skills, formation of creative manners and the author’s styles of illustrators. Evgheni Merega was among the first graphic artists involved in these processes who cooperated with: Tiraspol State Printing House, the State Publishing House (Chisinau, „Shkoala sovetica” and „Uchpedgiz”. Boris Nesvedov and Valentina Neceaev started in the interwar period. In the period 1940–1953, Leonid Grigoraşenco, Ilia Bogdesco, Boris Şirocorad, Iacob Averbuh, Ioachim Postolachi, Aleksandr Neforosov etc. made a name for themselves in the field of book graphics.

ExactPack Documentation

Energy Technology Data Exchange (ETDEWEB)

Singleton, Robert Jr. [Los Alamos National Laboratory; Israel, Daniel M. [Los Alamos National Laboratory; Doebling, Scott William [Los Alamos National Laboratory; Woods, Charles Nathan [Los Alamos National Laboratory; Kaul, Ann [Los Alamos National Laboratory; Walter, John William Jr [Los Alamos National Laboratory; Rogers, Michael Lloyd [Los Alamos National Laboratory

2016-05-09

For code verification, one compares the code output against known exact solutions. There are many standard test problems used in this capacity, such as the Noh and Sedov problems. ExactPack is a utility that integrates many of these exact solution codes into a common API (application program interface), and can be used as a stand-alone code or as a python package. ExactPack consists of python driver scripts that access a library of exact solutions written in Fortran or Python. The spatial profiles of the relevant physical quantities, such as the density, fluid velocity, sound speed, or internal energy, are returned at a time specified by the user. The solution profiles can be viewed and examined by a command line interface or a graphical user interface, and a number of analysis tools and unit tests are also provided. We have documented the physics of each problem in the solution library, and provided complete documentation on how to extend the library to include additional exact solutions. ExactPack’s code architecture makes it easy to extend the solution-code library to include additional exact solutions in a robust, reliable, and maintainable manner.

1st Lunar International Laboratory (LIL) Symposium Research in Geosciences and Astronomy : Organized by the International Academy of Astronautics at the XVIth International Astronautical Congress Athens, 16 September, 1965 and Dedicated to the Twentieth Anniversary of UNESCO

CERN Document Server

1966-01-01

The Lunar International Laboratory (LIL) project of the International Academy of Astronautics was begun upon the proposal of the editor at the First Special Meeting of the Academy at Stockholm on 16 August 1960. The late THEODORE VON KARMAN, first President of the Academy, appointed the following members of the LIL Committee: Prof. N. BoNEFF (Bulgaria), Prof. M. FLoRKIN (Belgium), Mr. A. G. HALEY (U. S. A. ), Prof. Sir BERNARD LovELL (U. K. ) (Vice­ Chairman), Prof. L. MALAVARD (France), Dr. F. J. MALINA (U. S. A. ) (Chairman), Prof. H. 0BERTH (German Federal Republic), Dr. W. H. PicKERING (U. S. A. ), Prof. E. SANGER (German Federal Republic), Prof. L. I. SEDOV (U. S. S. R. ), Prof. L. SPITZER, JR. (U. S. A. ), Dr. H. STRUGHOLD (U. S. A. ), Prof. H. C. UREY (U. S. A. ) and himself. Since 1960 the following additional members were appointed to the Committee: Mr. A. C. CLARKE (U. K. ), Prof. A. DoLLFUS (France), Prof. Z. KoPAL (U. K. ), Dr. S. F. SINGER (U. S. A. ), Prof. N. M. SISSAKIAN (U. S. S. R. ) and Pr...

Interferometric and schlieren characterization of the plasmas and shock wave dynamics during laser-triggered discharge in atmospheric air

Energy Technology Data Exchange (ETDEWEB)

Wei, Wenfu; Li, Xingwen, E-mail: xwli@mail.xjtu.edu.cn; Wu, Jian; Yang, Zefeng; Jia, Shenli; Qiu, Aici [State Key Laboratory of Electrical Insulation and Power Equipment, Xi' an Jiaotong University, Shaanxi 710049 (China)

2014-08-15

This paper describes our efforts to reveal the underlying physics of laser-triggered discharges in atmospheric air using a Mach-Zehnder interferometer and schlieren photography. Unlike the hemispherical shock waves that are produced by laser ablation, bell-like morphologies are observed during laser-triggered discharges. Phase shifts are recovered from the interferograms at a time of 1000 ns by the 2D fast Fourier transform method, and then the values of the refractive index are deduced using the Abel inversion. An abundance of free electrons is expected near the cathode surface. The schlieren photographs visualize the formation of stagnation layers at ∼600 ns in the interaction zones of the laser- and discharge-produced plasmas. Multiple reflected waves are observed at later times with the development of shock wave propagations. Estimations using the Taylor-Sedov self-similar solution indicated that approximately 45.8% and 51.9% of the laser and electrical energies are transferred into the gas flow motions, respectively. Finally, numerical simulations were performed, which successfully reproduced the main features of the experimental observations, and provided valuable insights into the plasma and shock wave dynamics during the laser-triggered discharge.

Charles Olivier and the rise of meteor science

CERN Document Server

Taibi, Richard

2017-01-01

This fascinating portrait of an amateur astronomy movement tells the story of how Charles Olivier recruited a hard-working cadre of citizen scientists to rehabilitate the study of meteors. By 1936, Olivier and members of his American Meteor Society had succeeded in disproving an erroneous idea about meteor showers. Using careful observations, they restored the public’s trust in predictions about periodic showers and renewed respect for meteor astronomy among professional astronomers in the United States. Charles Olivier and his society of observers who were passionate about watching for meteors in the night sky left a major impact on the field. In addition to describing Olivier’s career and describing his struggles with competitive colleagues in a hostile scientific climate, the author provides biographies of some of the scores of women and men of all ages who aided Olivier in making shower observations, from the Leonids and Perseids and others. Half of these amateur volunteers were from 13 to 25 years of...

The Concept of Beneficial Owner in Application of the Ukrainian Double Taxation Treaties / Leonid Tymchenko, Pavlo Selezen

Index Scriptorium Estoniae

Tymchenko, Leonid

2016-01-01

Tegelikult kasusaava omaniku kontseptsioonist Ukraina topeltmaksustamise lepingutes. Tegelikult kasusaava omaniku mõistest Ukraina seadusandluses ja Ukraina maksuseadusest. Sisaldab asjakohast kohtupraktikat

The agricultural sector of Ukraine in the era of Leonid Kuchma’s presidency: state and development trends

Directory of Open Access Journals (Sweden)

M. M. Ignatenko

2017-01-01

All in all, during the 1994-2004 years was created original version of state capitalism, in which elements of the free market were accompanied by extremely close cooperation of its members with government bureaucratic structures.

Russia's Approach to Revisiting the European Security Architecture and its Implications for the Common Neighbourhood / Leonid Karabeshkin

Index Scriptorium Estoniae

Karabeškin, Leonid

2011-01-01

Venemaa strateegilised ettepanekud praegusel kujul ei vasta endiste NSV Liidu vabariikide rahvuslikele huvidele ja välispoliitika suunistele, kuid nende toetamine võib tuua endistele vabariikidele poliitilist ja majanduslikku kasu. Euroopa Liit on huvitatud SRÜ maade kaasamisest Euroopa julgeolekut käsitlevasse diskussiooni

Analysis of arsenic and mercury content in human remains of the 16th and 17th centuries from Moscow Kremlin necropolises by neutron activation analysis at the IREN facility and the IBR-2 reactor FLNP JINR

Science.gov (United States)

Panova, T. D.; Dmitriev, A. Yu.; Borzakov, S. B.; Hramco, C.

2018-01-01

A neutron activation analysis (NAA) of three samples of human remains of the 16th and 17th centuries from the necropolises of the Moscow Kremlin has been carried out at FLNP JINR. The samples were irradiated at two facilities: the IREN source of resonance neutrons and the IBR-2 reactor. Spectra of the induced activity of the irradiated samples were measured by using the automatic measurement system developed at the Frank Laboratory of Neutron Physics (FLNP) of the Joint Institute for Nuclear Research (JINR). This system consists of a high-purity germanium detector with spectrometric electronics, a sample changer, and control software. Mass fraction of arsenic, mercury, and some other elements were calculated using two NAA methods—relative and absolute. The obtained values confirm the fact of acute mercury poisoning of Anastasia Romanovna, the first wife of Tsar Ivan Vasil'evich the Terrible, the first Russian Tsarina (died in 1560). High levels of mercury were detected in the bone remains of Tsarevich Ivan Ivanovich (died in 1581), the son of Tsar Ivan the Terrible, and Prince Mikhail Vasil'evich Skopin-Shuiskii (died in 1610). The results provide an opportunity to introduce into scientific circulation the exact values of mass fraction of mercury, arsenic, and other elements in the samples taken from the burials of the Russian historical figures of the second half of 16th-early 17th century.

3rd International Conference on X-ray Technique

Science.gov (United States)

Potrakhov, N. N.; Gryaznov, A. Yu; Lisenkov, A. A.; Kostrin, D. K.

2017-02-01

In this preface a brief history, modern aspects and future tendencies in development of the X-ray technique as seen from the 3rd International Conference on X-ray Technique that was held on 24-25 November 2016 in Saint Petersburg, Russia are described On 24-25 November 2016 in Saint Petersburg on the basis of Saint Petersburg State Electrotechnical University “LETI” n. a. V. I. Ulyanov (Lenin) was held the 3rd International Conference on X-ray Technique. The tradition to hold a similar conference in our country was laid in Soviet times. The last of them, the All-Union Conference on the Prospects of X-ray Tubes and Equipment was organized and held more than a quarter century ago - on 21-23 November 1999, at the initiative and under the leadership of the chief engineer of the Leningrad association of electronic industry “Svetlana” Borovsky Alexander Ivanovich and the chief of special design bureau of X-ray devices of “Svetlana” Shchukin Gennady Anatolievich. The most active part in the organization and work of the conference played members of the department of X-ray and electron beam instruments of Leningrad Electrotechnical Institute “LETI” (the former name of Saint Petersburg State Electrotechnical University “LETI”), represented by head of the department professor Ivanov Stanislav Alekseevich.

Analytical Solution for Interface Flow to a Sink With an Upconed Saline Water Lens: Strack's Regimes Revisited

Science.gov (United States)

Kacimov, A. R.; Obnosov, Y. V.

2018-01-01

A study is made of a steady, two-dimensional groundwater flow with a horizontal well (drain), which pumps out freshwater from an aquifer sandwiched between a horizontal bedrock and ponded soil surface, and containing a lens-shaped static volume of a heavier saline water (DNAPL-dense nonaqueous phase liquid) as a free surface. For flow toward a line sink, an explicit analytical solution is obtained by a conformal mapping of the hexagon in the complex potential plane onto a reference plane and the Keldysh-Sedov integral representation of a mixed boundary-value problem for a complex physical coordinate. The interface is found as a function of the pumping rate, the well locus, the ratio of liquid densities, and the hydraulic heads at the soil surface and in the well. The shape with two inflexion points and fronts varies from a small-thickness bedrock-spread pancake to a critical curvilinear triangle, which cusps toward the sink. The problem is mathematically solvable in a relatively narrow band of geometric and hydraulic parameters. A similar analytic solution for a static heavy bubble confined by a closed-curve interface (no contact with the bedrock) is outlined as an illustration of the method to solve a mixed boundary-value problem.

Blast-Wave Generation and Propagation in Rapidly Heated Laser-Irradiated Targets

Science.gov (United States)

Ivancic, S. T.; Stillman, C. R.; Nilson, P. M.; Solodov, A. A.; Froula, D. H.

2017-10-01

Time-resolved extreme ultraviolet (XUV) spectroscopy was used to study the creation and propagation of a >100-Mbar blast wave in a target irradiated by an intense (>1018WWcm2 cm2) laser pulse. Blast waves provide a platform to generate immense pressures in the laboratory. A temporal double flash of XUV radiation was observed when viewing the rear side of the target, which is attributed to the emergence of a blast wave following rapid heating by a fast-electron beam generated from the laser pulse. The time-history of XUV emission in the photon energy range of 50 to 200 eV was recorded with an x-ray streak camera with 7-ps temporal resolution. The heating and expansion of the target was simulated with an electron transport code coupled to 1-D radiation-hydrodynamics simulations. The temporal delay between the two flashes measured in a systematic study of target thickness and composition was found to evolve in good agreement with a Sedov-Taylor blast-wave solution. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0001944 and Department of Energy Office of Science Award Number DE-SC-0012317.

INJECTION TO RAPID DIFFUSIVE SHOCK ACCELERATION AT PERPENDICULAR SHOCKS IN PARTIALLY IONIZED PLASMAS

Energy Technology Data Exchange (ETDEWEB)

Ohira, Yutaka, E-mail: ohira@phys.aoyama.ac.jp [Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara 252-5258 (Japan)

2016-08-10

We present a three-dimensional hybrid simulation of a collisionless perpendicular shock in a partially ionized plasma for the first time. In this simulation, the shock velocity and upstream ionization fraction are v {sub sh} ≈ 1333 km s{sup −1} and f {sub i} ∼ 0.5, which are typical values for isolated young supernova remnants (SNRs) in the interstellar medium. We confirm previous two-dimensional simulation results showing that downstream hydrogen atoms leak into the upstream region and are accelerated by the pickup process in the upstream region, and large magnetic field fluctuations are generated both in the upstream and downstream regions. In addition, we find that the magnetic field fluctuations have three-dimensional structures and the leaking hydrogen atoms are injected into the diffusive shock acceleration (DSA) at the perpendicular shock after the pickup process. The observed DSA can be interpreted as shock drift acceleration with scattering. In this simulation, particles are accelerated to v ∼ 100 v {sub sh} ∼ 0.3 c within ∼100 gyroperiods. The acceleration timescale is faster than that of DSA in parallel shocks. Our simulation results suggest that SNRs can accelerate cosmic rays to 10{sup 15.5} eV (the knee) during the Sedov phase.

25th anniversary of the Lenin nuclear icebreaker

International Nuclear Information System (INIS)

Khlopkin, N.S.; Mitenkov, F.M.; Movshevich, Z.M.; Pologikh, B.G.; Sledzyuk, A.K.

1984-01-01

The main results of operation and prospects of further development of nuclear ships in the USSR are considered. The main characteristics and the data on the most important stages of operation of nuclear-powered ice-breakers ''Lenin'', ''Leonid Brezhnev'' and ''Sibir''' are presented. Advantages of nuclear-powered ice-breakers as compared with diesel electric ice-breakers are analyzed. In the course of operation of nuclear-powered ice-breakers high reliability of water-pressurized reactors, installed in the ships, the crew and environment safety, and economic advisability of nuclear power on big ships durably worbing far from bases have been proved. The exploitation of nuclear-powered ice-breakers permitted considerably increase the periods of navigation to have made it all-theMyear-round in the western sector of the Arctic. The speed of steering the ships has increased 1.5-2 times. Presently shallow-draught nuclear ice-breakers are developed for the Siberian rivers. An ice-breaker transport lighter-carrier is now being built, that can take on board 74 lighters 370 t each

From the "Modern Synthesis" to cybernetics: Ivan Ivanovich Schmalhausen (1884-1963) and his research program for a synthesis of evolutionary and developmental biology.

Science.gov (United States)

Levit, Georgy S; Hossfeld, Uwe; Olsson, Lennart

2006-03-15

Ivan I. Schmalhausen was one of the central figures in the Russian development of the "Modern Synthesis" in evolutionary biology. He is widely cited internationally even today. Schmalhausen developed the main principles of his theory facing the danger of death in the totalitarian Soviet Union. His great services to evolutionary and theoretical biology are indisputable. However, the received view of Schmalhausen's contributions to evolutionary biology makes an unbiased reading of his texts difficult. Here we show that taking all of his works into consideration (including those only available in Russian) paints a much more dynamic and exciting picture of what he tried to achieve. Schmalhausen pioneered the integration of a developmental perspective into evolutionary thinking. A main tool for achieving this was his approach to living objects as complex multi-level self-regulating systems. Schmalhausen put enormous effort into bringing this idea into fruition during the final stages of his career by combining evolutionary theory with cybernetics. His results and ideas remain thought-provoking, and his texts are of more than just historical interest. Copyright 2006 Wiley-Liss, Inc.

The Growth, Polarization, and Motion of the Radio Afterglow from the Giant Flare from SGR 1806-20

Energy Technology Data Exchange (ETDEWEB)

Taylor, G

2005-04-20

The extraordinary giant flare (GF) of 2004 December 27 from the soft gamma repeater (SGR) 1806-20 was followed by a bright radio afterglow. We present an analysis of VLA observations of this radio afterglow from SGR1806-20, consisting of previously reported 8.5 GHz data covering days 7 to 20 after the GF, plus new observations at 8.5 and 22 GHz from day 24 to 81. For a symmetric outflow, we find a deceleration in the expansion, from {approx}4.5 mas/day to <2.5 mas/day. The time of deceleration is roughly coincident with the rebrightening in the radio light curve, as expected to result when the ejecta from the GF sweeps up enough of the external medium, and transitions from a coasting phase to the Sedov-Taylor regime. The radio afterglow is elongated and maintains a 2:1 axis ratio with an average position angle of -40{sup o} (north through east), oriented perpendicular to the average intrinsic linear polarization angle. We also report on the discovery of motion in the flux centroid of the afterglow, at an average velocity of 0.26 {+-} 0.03 c (assuming a distance of 15 kpc) at a position angle of -45{sup o}. This motion, in combination with the growth and polarization measurements, suggests an initially asymmetric outflow, mainly from one side of the magnetar.

Impaired vascular function in physically active premenopausal women with functional hypothalamic amenorrhea is associated with low shear stress and increased vascular tone.

Science.gov (United States)

O'Donnell, Emma; Goodman, Jack M; Mak, Susanna; Harvey, Paula J

2014-05-01

Exercise-trained hypoestrogenic premenopausal women with functional hypothalamic amenorrhea (ExFHA) exhibit impaired endothelial function. The vascular effects of an acute bout of exercise, a potent nitric oxide stimulus, in these women are unknown. Three groups were studied: recreationally active ExFHA women (n = 12; 24.2 ± 1.2 years of age; mean ± SEM), and recreationally active (ExOv; n = 14; 23.5 ± 1.2 years of age) and sedentary (SedOv; n = 15; 23.1 ± 0.5 years of age) ovulatory eumenorrheic women. Calf blood flow (CBF) and brachial artery flow-mediated dilation (FMD) were evaluated using plethysmographic and ultrasound techniques, respectively, both before and 1 hour after 45 minutes of moderate-intensity exercise. Endothelium-independent dilation was assessed at baseline using glyceryl trinitrate. Calf vascular resistance (CVR) and brachial peak shear rate, as determined by the area under the curve (SRAUCpk), were also calculated. FMD and glyceryl trinitrate responses were lower (P .05) the findings. CBF was lower (P .05) between the groups. CBF in ExFHA was increased (P < .05) and CVR decreased (P < .05) to levels observed in ovulatory women. Acute dynamic exercise improves vascular function in ExFHA women. Although the role of estrogen deficiency per se is unclear, our findings suggest that low shear rate and increased vasoconstrictor tone may play a role in impaired basal vascular function in these women.

A deep Suzaku observation of the Galactic Ia supernova remnant G306.3-0.9

Science.gov (United States)

Tachibana, K.; Sawada, M.; Uchida, H.; Ito, Y.; Matsumura, H.; Bamba, A.; Tsuru, T.; Tanaka, T.

2017-10-01

The supernova remnant (SNR) G306.3-0.9 was discovered by Swift in 2011. Its relatively small size confirmed by Chandra implies the SNR is young (Reynolds et al. 2013). XMM-Newton (Combi et al. 2016) and Suzaku (Sezer et al. 2017) discovered strong Fe-Kα, and established a type-Ia origin of the SNR. Recent studies of young Ia SNRs have revealed Fe has lower ionization state than intermediate mass elements (IME) . This implies they maintain a stratified ejecta structure. However, previous studies of G306.3-0.9 assumed Fe and IME have a common ionization timescale. We reanalyzed the Suzaku data with the latest calibration database to study the nature of Fe ejecta and to estimate the age. Spectrum analysis showed the Fe-Kα centroid is 6.47±0.01 keV (O-like), which results in higher electron temperature (>3 keV) and lower ionization state (˜1.5×10^{10} s cm^{3}) for Fe than IME. The Hydrogen absorption column density is (1.2-1.3)× 10^{22} cm^{-2}, leading to the conclusion that the distance of the SNR is ˜ 20 kpc and the age is ˜ 8.5 kyr. The SNR is the first example of still stratified ejecta in the late Sedov phase.

Optical Pattern Recognition

Science.gov (United States)

Yu, Francis T. S.; Jutamulia, Suganda

2008-10-01

Contributors; Preface; 1. Pattern recognition with optics Francis T. S. Yu and Don A. Gregory; 2. Hybrid neural networks for nonlinear pattern recognition Taiwei Lu; 3. Wavelets, optics, and pattern recognition Yao Li and Yunglong Sheng; 4. Applications of the fractional Fourier transform to optical pattern recognition David Mendlovic, Zeev Zalesky and Haldum M. Oxaktas; 5. Optical implementation of mathematical morphology Tien-Hsin Chao; 6. Nonlinear optical correlators with improved discrimination capability for object location and recognition Leonid P. Yaroslavsky; 7. Distortion-invariant quadratic filters Gregory Gheen; 8. Composite filter synthesis as applied to pattern recognition Shizhou Yin and Guowen Lu; 9. Iterative procedures in electro-optical pattern recognition Joseph Shamir; 10. Optoelectronic hybrid system for three-dimensional object pattern recognition Guoguang Mu, Mingzhe Lu and Ying Sun; 11. Applications of photrefractive devices in optical pattern recognition Ziangyang Yang; 12. Optical pattern recognition with microlasers Eung-Gi Paek; 13. Optical properties and applications of bacteriorhodopsin Q. Wang Song and Yu-He Zhang; 14. Liquid-crystal spatial light modulators Aris Tanone and Suganda Jutamulia; 15. Representations of fully complex functions on real-time spatial light modulators Robert W. Cohn and Laurence G. Hassbrook; Index.

Compoziţia tematică în grafica de şevalet. Anii 1980-1990

Directory of Open Access Journals (Sweden)

Tatiana Raşchitor

2016-10-01

Full Text Available The evolution of thematic composition in the MSSR arts was hampered in terms of style and themes by the social and cultural context of the time. Therefore, most of the compositions created during the Soviet decades reflected pre-established models. However, a more detailed examination of thematic compositions created during the 1980s convince us of the beginning of democratization within artistic environment, emerged in the background of collapse of the old ideology. We notice new visions in the compositions signed by Victor Cuzmenco, Igor Liberman, Nina Danilenco etc. Their works have the unique artistic approach infused with dreaminess, melancholy, symbolism and transcendence, or present new topics by appealing to different artistic manners. With the collapse of the communist paradigm, artistic space has acquired a heterogeneous and eclectic character, receptive to contemporary art trends. Anthropocentric and sacred perspective represented by the works signed by Emil Childescu and Leonid Grigoraşenco in the easel graphic of the 1990s coexist in relative proximity in to inherent mental models of contemporary time represented by the works of Gheorghe Diaconu, Simion Zamsa, Elena Karacenţev etc.

Photometric Calibration of Consumer Video Cameras

Science.gov (United States)

Suggs, Robert; Swift, Wesley, Jr.

2007-01-01

Equipment and techniques have been developed to implement a method of photometric calibration of consumer video cameras for imaging of objects that are sufficiently narrow or sufficiently distant to be optically equivalent to point or line sources. Heretofore, it has been difficult to calibrate consumer video cameras, especially in cases of image saturation, because they exhibit nonlinear responses with dynamic ranges much smaller than those of scientific-grade video cameras. The present method not only takes this difficulty in stride but also makes it possible to extend effective dynamic ranges to several powers of ten beyond saturation levels. The method will likely be primarily useful in astronomical photometry. There are also potential commercial applications in medical and industrial imaging of point or line sources in the presence of saturation.This development was prompted by the need to measure brightnesses of debris in amateur video images of the breakup of the Space Shuttle Columbia. The purpose of these measurements is to use the brightness values to estimate relative masses of debris objects. In most of the images, the brightness of the main body of Columbia was found to exceed the dynamic ranges of the cameras. A similar problem arose a few years ago in the analysis of video images of Leonid meteors. The present method is a refined version of the calibration method developed to solve the Leonid calibration problem. In this method, one performs an endto- end calibration of the entire imaging system, including not only the imaging optics and imaging photodetector array but also analog tape recording and playback equipment (if used) and any frame grabber or other analog-to-digital converter (if used). To automatically incorporate the effects of nonlinearity and any other distortions into the calibration, the calibration images are processed in precisely the same manner as are the images of meteors, space-shuttle debris, or other objects that one seeks to

Radio Evolution of Supernova Remnants Including Nonlinear Particle Acceleration: Insights from Hydrodynamic Simulations

Science.gov (United States)

Pavlović, Marko Z.; Urošević, Dejan; Arbutina, Bojan; Orlando, Salvatore; Maxted, Nigel; Filipović, Miroslav D.

2018-01-01

We present a model for the radio evolution of supernova remnants (SNRs) obtained by using three-dimensional hydrodynamic simulations coupled with nonlinear kinetic theory of cosmic-ray (CR) acceleration in SNRs. We model the radio evolution of SNRs on a global level by performing simulations for a wide range of the relevant physical parameters, such as the ambient density, supernova (SN) explosion energy, acceleration efficiency, and magnetic field amplification (MFA) efficiency. We attribute the observed spread of radio surface brightnesses for corresponding SNR diameters to the spread of these parameters. In addition to our simulations of Type Ia SNRs, we also considered SNR radio evolution in denser, nonuniform circumstellar environments modified by the progenitor star wind. These simulations start with the mass of the ejecta substantially higher than in the case of a Type Ia SN and presumably lower shock speed. The magnetic field is understandably seen as very important for the radio evolution of SNRs. In terms of MFA, we include both resonant and nonresonant modes in our large-scale simulations by implementing models obtained from first-principles, particle-in-cell simulations and nonlinear magnetohydrodynamical simulations. We test the quality and reliability of our models on a sample consisting of Galactic and extragalactic SNRs. Our simulations give Σ ‑ D slopes between ‑4 and ‑6 for the full Sedov regime. Recent empirical slopes obtained for the Galactic samples are around ‑5, while those for the extragalactic samples are around ‑4.

Conversion of piston-driven shocks from powerful solar flares to blast wave shocks in the solar wind

International Nuclear Information System (INIS)

Pinter, S.

1990-01-01

It was suggested by Smart and Shea (1985) that the time of arrival of solar-flare-generated shock waves at any point in space may be predicted by assuming that they are first driven from the Sun after which they decay into blast shocks. Their study was extended by using the duration of the Type IV radio emission as a phenomenological symptom of the piston-driven phase of these shocks. Using a sample of 39 cases of combined Type II/Type IV observations from 1972 to 1982 solar flares, it was found that the average predicted times-of-arrival of these shocks to Earth (and elsewhere) deviate from the actual times by 1.40 hr with a standard deviation of 1.25 hr. On the average, a representative shock from this sample is emitted from a powerful flare with a velocity of 1,560 km sec -1 ; moves at a constant inertial velocity to a distance of 0.12 AU after which it begins to decelerate as a classical (Sedov-type) blast shock that is convected by the ambient solar wind as suggested by Smart and Shea; and arrives to Earth 45.8 hr after its initiation in the Sun. Shocks that appear to deviate from this phenomenological scenario by virtue of lack of detection on Earth are assumed to decay into fast mode MHD waves. (author). 7 figs., 1 tab., 53 refs

3D staggered Lagrangian hydrodynamics scheme with cell-centered Riemann solver-based artificial viscosity

International Nuclear Information System (INIS)

Loubere, Raphael; Maire, Pierre-Henri; Vachal, Pavel

2013-01-01

The aim of the present work is the 3D extension of a general formalism to derive a staggered discretization for Lagrangian hydrodynamics on unstructured grids. The classical compatible discretization is used; namely, momentum equation is discretized using the fundamental concept of subcell forces. Specific internal energy equation is obtained using total energy conservation. The subcell force is derived by invoking the Galilean invariance and thermodynamic consistency. A general form of the subcell force is provided so that a cell entropy inequality is satisfied. The subcell force consists of a classical pressure term plus a tensorial viscous contribution proportional to the difference between the node velocity and the cell-centered velocity. This cell-centered velocity is an extra degree of freedom solved with a cell-centered approximate Riemann solver. The second law of thermodynamics is satisfied by construction of the local positive definite subcell tensor involved in the viscous term. A particular expression of this tensor is proposed. A more accurate extension of this discretization both in time and space is also provided using a piecewise linear reconstruction of the velocity field and a predictor-corrector time discretization. Numerical tests are presented in order to assess the efficiency of this approach in 3D. Sanity checks show that the 3D extension of the 2D approach reproduces 1D and 2D results. Finally, 3D problems such as Sedov, Noh, and Saltzman are simulated. (authors)

Catalogue of Meteor Showers and Storms in Korean History

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Sang-Hyeon Ahn

2004-03-01

Full Text Available We present a more complete and accurate catalogue of astronomical records for meteor showers and meteor storms appeared in primary official Korean history books, such as Samguk-sagi, Koryo-sa, Seungjeongwon-ilgi, and Choson-Wangjo-Sillok. So far the catalogue made by Imoto and Hasegawa in 1958 has been widely used in the international astronomical society. The catalogue is based on a report by Sekiguchi in 1917 that is mainly based on secondary history books. We observed that the catalogue has a number of errors in either dates or sources of the records. We have thoroughly checked the primary official history books, instead of the secondary ones, in order to make a corrected and extended catalogue. The catalogue contains 25 records of meteor storms, four records of intense meteor-showers, and five records of usual showers in Korean history. We also find that some of those records seem to correspond to some presently active meteor showers such as the Leonids, the Perseids, and the ¥ç-Aquarids-Orionids pair. However, a large number of those records do not correspond to such present showers. This catalogue we obtained can be useful for various astrophysical studies in the future.

Grafica de carte din RSS Moldovenească în anii 1953–1960

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Victoria Rocaciuc

2017-10-01

Full Text Available The years of 1953–1960 entered in national history of book graphics as a stage marked by increases in professionalism. Considerable revival of all processes of art becomes more pronounced towards 1957 and 1960, marked by several important events (First All-Union Congress of Union of Artists Formation, Union Jubilee Exhibition dedicated to 40 years anniversary of the Great October, the participation of young artists from the Soviet Union in the VIth World Festival of Youth and Students in Moscow, the Decade of Moldovan Literature and Art in Moscow etc.. More pronounced will became the trend of Moldovan national school to specify the ethnic character. At that time, spiritual processes coincided with the broadening of spheres of knowledge. Given promoting of innovation in the editorial process, the elements of narrative and documentary, were enriched with new forms of conventional treatment of fine art images. The remarkable masters of the book graphics at this time where Leonid Grigoraşenco, Ilia Bogdesco, Boris Nesvedov. After 1953, the Moldovan Soviet art of book graphics, was additioned by already established masters, which have started working young as Igor Vieru, Boris Nesvedov, Iacob Averbuh, Ghennadi Zikov, Vasili Ţehmister, Filimon Hămuraru, Nikolai Makarenko etc.

VERNADSKY'S V.I. THEORY OF NOOSPHERE AS THE BASIS FOR SUSTAINABLE DEVELOPMENT

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V. A. Grachev

2015-01-01

Full Text Available Aim. To implement Vladimir Ivanovich Vernadsky's teachings of noospheric outlook as the basis for sustainable development of the world community.Discussion. The theory of noosphere has become the philosophical basis of the concept for sustainable development of society, a strategy for balanced economic development and natural resource management, and continues to have great influence on modern environmental awareness and as often happens with great scientists, that walk ahead of their time, Vernadsky’s scientific legacy will still be comprehended and creatively developed by the next generations. Vernadsky suggested the change of attitudes and ideological principles, i.e. noospheric thinking, as the solution for environmental problems. Therefore, today, Vernadsky's teachings of biosphere-noosphere transition is of particular relevance that could be the basis for fundamental research of environmental issues and practical search for their resolution. According to Vernadsky, the basic prerequisites for the development of the noosphere are the following: humanity should be united; means of communication and exchange should be transformed; the discovery of new energy sources; the rise of well-being, equality of all people; conflict-free society.Conclusion. The knowledge of the development of the biosphere is the key to rational nature management. Vernadsky concludes that humanity, in the course of its development, is transformed into a powerful new geological force, and with thought and action it changes the face of the planet. Accordingly, for the purpose of its preservation, the humanity will have to take responsibility for the development of the biosphere turning into noosphere, and it will require a certain social organization and new environmental and humanistic ethics at the same time.

NEAR-IR STUDIES OF RECURRENT NOVA V745 SCORPII DURING ITS 2014 OUTBURST

International Nuclear Information System (INIS)

Banerjee, D. P. K.; Joshi, Vishal; Venkataraman, V.; Ashok, N. M.; Raj, A.; Marion, G. H.; Hsiao, E. Y.

2014-01-01

The recurrent nova V745 Scorpii underwent its third known outburst on 2014 February 6. Infrared monitoring of the eruption on an almost daily basis, starting from 1.3 days after discovery, shows the emergence of a powerful blast wave generated by the high velocity nova ejecta exceeding 4000 km s –1 plowing into its surrounding environment. The temperature of the shocked gas is raised to a high value exceeding 10 8 K immediately after outburst commencement. The energetics of the outburst clearly surpass those of similar symbiotic systems like RS Oph and V407 Cyg which have giant secondaries. The shock does not show a free-expansion stage but rather shows a decelerative Sedov-Taylor phase from the beginning. Such strong shock fronts are known to be sites for γ-ray generation. V745 Sco is the latest nova, apart from five other known novae, to show γ-ray emission. It may be an important testbed to resolve the crucial question of whether or not all novae are generically γ-ray emitters by virtue of having a circumbinary reservoir of material that is shocked by the ejecta rather than γ-ray generation being restricted to only symbiotic systems with a shocked red giant (RG) wind. The lack of a free-expansion stage favors V745 Sco to have a density enhancement around the white dwarf (WD), above that contributed by a RG wind. Our analysis also suggests that the WD in V745 Sco is very massive and a potential progenitor for a future SN Ia explosion

PHYSICS OF A PARTIALLY IONIZED GAS RELEVANT TO GALAXY FORMATION SIMULATIONS—THE IONIZATION POTENTIAL ENERGY RESERVOIR

International Nuclear Information System (INIS)

Vandenbroucke, B.; De Rijcke, S.; Schroyen, J.; Jachowicz, N.

2013-01-01

Simulation codes for galaxy formation and evolution take on board as many physical processes as possible beyond the standard gravitational and hydrodynamical physics. Most of this extra physics takes place below the resolution level of the simulations and is added in a ''sub-grid'' fashion. However, these sub-grid processes affect the macroscopic hydrodynamical properties of the gas and thus couple to the ''on-grid'' physics that is explicitly integrated during the simulation. In this paper, we focus on the link between partial ionization and the hydrodynamical equations. We show that the energy stored in ions and free electrons constitutes a potential energy term which breaks the linear dependence of the internal energy on temperature. Correctly taking into account ionization hence requires modifying both the equation of state and the energy-temperature relation. We implemented these changes in the cosmological simulation code GADGET2. As an example of the effects of these changes, we study the propagation of Sedov-Taylor shock waves through an ionizing medium. This serves as a proxy for the absorption of supernova feedback energy by the interstellar medium. Depending on the density and temperature of the surrounding gas, we find that up to 50% of the feedback energy is spent ionizing the gas rather than heating it. Thus, it can be expected that properly taking into account ionization effects in galaxy evolution simulations will drastically reduce the effects of thermal feedback. To the best of our knowledge, this potential energy term is not used in current simulations of galaxy formation and evolution.

RESOLUTION OF THE COMPACT RADIO CONTINUUM SOURCES IN Arp220

International Nuclear Information System (INIS)

Batejat, Fabien; Conway, John E.; Hurley, Rossa; Parra, Rodrigo; Diamond, Philip J.; Lonsdale, Colin J.; Lonsdale, Carol J.

2011-01-01

We present 2 cm and 3.6 cm wavelength very long baseline interferometry images of the compact radio continuum sources in the nearby ultra-luminous infrared galaxy Arp220. Based on their radio spectra and variability properties, we confirm these sources to be a mixture of supernovae (SNe) and supernova remnants (SNRs). Of the 17 detected sources we resolve 7 at both wavelengths. The SNe generally only have upper size limits. In contrast all the SNRs are resolved with diameters ≥0.27 pc. This size limit is consistent with them having just entered their Sedov phase while embedded in an interstellar medium (ISM) of density 10 4 cm -3 . These objects lie on the diameter-luminosity correlation for SNRs (and so also on the diameter-surface brightness relation) and extend these correlations to very small sources. The data are consistent with the relation L∝D -9/4 . Revised equipartition arguments adjusted to a magnetic field to a relativistic particle energy density ratio of 1% combined with a reasonable synchrotron-emitting volume filling factor of 10% give estimated magnetic field strengths in the SNR shells of ∼15-50 mG. The SNR shell magnetic fields are unlikely to come from compression of ambient ISM fields and must instead be internally generated. We set an upper limit of 7 mG for the ISM magnetic field. The estimated energy in relativistic particles, 2%-20% of the explosion kinetic energy, is consistent with estimates from models that fit the IR-radio correlation in compact starburst galaxies.

Converging shock flows for a Mie-Grüneisen equation of state

Science.gov (United States)

Ramsey, Scott D.; Schmidt, Emma M.; Boyd, Zachary M.; Lilieholm, Jennifer F.; Baty, Roy S.

2018-04-01

Previous work has shown that the one-dimensional (1D) inviscid compressible flow (Euler) equations admit a wide variety of scale-invariant solutions (including the famous Noh, Sedov, and Guderley shock solutions) when the included equation of state (EOS) closure model assumes a certain scale-invariant form. However, this scale-invariant EOS class does not include even simple models used for shock compression of crystalline solids, including many broadly applicable representations of Mie-Grüneisen EOS. Intuitively, this incompatibility naturally arises from the presence of multiple dimensional scales in the Mie-Grüneisen EOS, which are otherwise absent from scale-invariant models that feature only dimensionless parameters (such as the adiabatic index in the ideal gas EOS). The current work extends previous efforts intended to rectify this inconsistency, by using a scale-invariant EOS model to approximate a Mie-Grüneisen EOS form. To this end, the adiabatic bulk modulus for the Mie-Grüneisen EOS is constructed, and its key features are used to motivate the selection of a scale-invariant approximation form. The remaining surrogate model parameters are selected through enforcement of the Rankine-Hugoniot jump conditions for an infinitely strong shock in a Mie-Grüneisen material. Finally, the approximate EOS is used in conjunction with the 1D inviscid Euler equations to calculate a semi-analytical Guderley-like imploding shock solution in a metal sphere and to determine if and when the solution may be valid for the underlying Mie-Grüneisen EOS.

Sound wave generation by a spherically symmetric outburst and AGN feedback in galaxy clusters

Science.gov (United States)

Tang, Xiaping; Churazov, Eugene

2017-07-01

We consider the evolution of an outburst in a uniform medium under spherical symmetry, having in mind active galactic nucleus feedback in the intracluster medium. For a given density and pressure of the medium, the spatial structure and energy partition at a given time tage (since the onset of the outburst) are fully determined by the total injected energy Einj and the duration tb of the outburst. We are particularly interested in the late phase evolution when the strong shock transforms into a sound wave. We studied the energy partition during such transition with different combinations of Einj and tb. For an instantaneous outburst with tb → 0, which corresponds to the extension of classic Sedov-Taylor solution with counter-pressure, the fraction of energy that can be carried away by sound waves is ≲12 per cent of Einj. As tb increases, the solution approaches the 'slow piston' limit, with the fraction of energy in sound waves approaching zero. We then repeat the simulations using radial density and temperature profiles measured in Perseus and M87/Virgo clusters. We find that the results with a uniform medium broadly reproduce an outburst in more realistic conditions once proper scaling is applied. We also develop techniques to map intrinsic properties of an outburst (Einj, tb and tage) to the observables like the Mach number of the shock and radii of the shock and ejecta. For the Perseus cluster and M87, the estimated (Einj, tb and tage) agree with numerical simulations tailored for these objects with 20-30 per cent accuracy.

Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics

Science.gov (United States)

Smith, Matthew C.; Sijacki, Debora; Shen, Sijing

2018-04-01

While feedback from massive stars exploding as supernovae (SNe) is thought to be one of the key ingredients regulating galaxy formation, theoretically it is still unclear how the available energy couples to the interstellar medium and how galactic scale outflows are launched. We present a novel implementation of six sub-grid SN feedback schemes in the moving-mesh code AREPO, including injections of thermal and/or kinetic energy, two parametrizations of delayed cooling feedback and a `mechanical' feedback scheme that injects the correct amount of momentum depending on the relevant scale of the SN remnant resolved. All schemes make use of individually time-resolved SN events. Adopting isolated disk galaxy setups at different resolutions, with the highest resolution runs reasonably resolving the Sedov-Taylor phase of the SN, we aim to find a physically motivated scheme with as few tunable parameters as possible. As expected, simple injections of energy overcool at all but the highest resolution. Our delayed cooling schemes result in overstrong feedback, destroying the disk. The mechanical feedback scheme is efficient at suppressing star formation, agrees well with the Kennicutt-Schmidt relation and leads to converged star formation rates and galaxy morphologies with increasing resolution without fine tuning any parameters. However, we find it difficult to produce outflows with high enough mass loading factors at all but the highest resolution, indicating either that we have oversimplified the evolution of unresolved SN remnants, require other stellar feedback processes to be included, require a better star formation prescription or most likely some combination of these issues.

Waiting for the new Nobel laureate(s in economic sciences

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Pantelić Svetlana

2016-01-01

Full Text Available Since the start in 1901, with the exception of the war years, the Nobel Prizes have always been awarded on the 10th of December, to mark the day of Alfred Nobel's demise. The exception is the prize for achievements in economic sciences which only started to be awarded in 1969. Since 1995 the Prize in Economic Sciences has been defined as the Prize in Social Sciences, so that the other recognized scientists in these fields, such as political sciences, psychology and sociology, could be awarded. Moreover, it was established that the Prize can be divided among no more than three winners. The Prize in Economic Sciences has been awarded to the total of 76 scientists, most of which, i.e. 52 of them, were the citizens of the USA. The largest number of laureates, i.e. twelve, came from the University of Chicago, six of them from Princeton, and five from Berkley. It was only once, in 2009, that the Nobel Prize in Economics was awarded to a woman - Elinor Ostrom (1933-2012 from the USA, together with Oliver Williamson. The average age of the Nobel Prize winners is about 60 years. The oldest laureate to have ever won the prize was Leonid Hurwicz, who received the Nobel Prize in Economic Sciences in 2007 at the age of 90.

HIV Pathogenesis: Abstracts from the March 2017 Cleveland Immunopathogenesis Consortium Meeting

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Michael M. Lederman

2017-06-01

Full Text Available The Cleveland Immunopathogenesis Consortium (CLIC was launched in March 2004 by a small group of investigators (Ron Bosch, Jason Brenchley,  Steven Deeks, Danny Douek, Zvi Grossman, Robert Kalayjian, Clifford Harding, Michael Lederman, Leonid Margolis, Miguel Quinones, Benigno Rodriguez, Rafick Sekaly, Scott Sieg, and Guido Silvestri who were increasingly persuaded that immune activation was an important driver of HIV pathogenesis. We met around a chalk board and scribbled our models of pathogenesis, designed some experiments then went back home to do them. We met again soon to review our new and unpublished findings that refined and shaped these models. The data presentations were short, informal and heavy on discussion. The model worked well, the consortium was productive and the meetings catalyzed numerous collaborations and scores of high impact papers. The CLIC (less formally, the Bad Boys of Cleveland [1] has been meeting regularly since then. Consortium membership has expanded to include other investigators (some are listed in the presentations below. Whether the goal is to prevent the morbid complications of HIV infection, to understand the determinants of HIV persistence or the factors that protect from acquisition of infection, a more clear understanding of HIV immunopathogenesis is central. Here in this issue of Pathogens and Immunity is a brief summary of the most recent CLIC//BBC meeting held in Cleveland in March 2017.

The Fourth Way in Finland

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Vesa Iitti

2008-01-01

Full Text Available This article focuses on the general history of the Fourth Way in Finland. The Fourth Way, or simply ‘the Work’, began as a Greco-Armenian man named Georges Ivanovich Gurdjieff (1866?–1949 gathered groups of pupils in St Petersburg and Moscow in 1912. To these groups, Gurdjieff started to teach what he had learned and synthesized between ca 1896 and 1912 during his travels on spiritual search of Egypt, Crete, Sumeria, Assyria, the Holy Land, Mecca, Ethiopia, Sudan, India, Afghanistan, the northern valleys of Siberia, and Tibet. Neither Gurdjieff nor any of his disciples called themselves a church, a sect, or anything alike, but referred to themselves simply as ‘the Work’, or as ‘the Fourth Way’. The name ‘the Fourth Way’ originates in a Gurdjieffian view that there are essentially three traditional ways of spiritual work: those of a monk, a fakir, and a yogi. These ways do not literally refer to the activities of a monk, a fakir, and a yogi, but to similar types of spiritual work emphasizing exercise of emotion, body, or mind. Gurdjieff’s teaching is a blend of various influences that include Suf­ism, orthodox Christianity, Buddhism, Kabbalah, and general elem­ents of various occult teachings of both the East and the West. Gurdjieff’s teaching is a blend of various influences that include Suf­ism, orthodox Christianity, Buddhism, Kabbalah, and general elem­ents of various occult teachings of both the East and the West. It is a unique combination of cosmology, psychology, theory of evolution, and overall theory and practise aiming to help individ­uals in their efforts towards what is called ‘self-remembering’.

TO 135TH ANNIVERSARY FROM THE DATE OF BIRTH OF ZHEGALOV S.I. – AN ESTABLISHER OF NATIONAL SCHOOL FOR BREEDING AND SEED INDUSTRY OF VEGETABLE CROPS

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V. F. Pivovarov

2016-01-01

Full Text Available On the second of October, in 1881, Sergey Ivanovich Zhegalov, an establisher of national breeding and seed production of vegetable crops was born in a little village Vasilkovo of Vyazemskogo uezda. He was a founder and a first director of Gribovskaya Vegetable Breeding Station. This year marked by 135th anniversary from the date of birth of the outstanding scientist. All the time at All-Russian Research Institute of Vegetable Breeding and Seed Production (VNIISSOK, its scientific leader and mastermind is honored and remembered for his heritage that is still preserved andaugmented. This scientist was at the beginning of plant breeding science and became the first who brought scientifically proved methods into agricultural plant science. The process of newplant- form-producing and development of new more qualified breeding forms through distant crossing, hybridization, heterosis effect, are the problems which interested the mind of Zhegalov and always were the sense of his life. These problems still remain in these days, where his ideas are embodied in scientific program of the institute covering theoretical researches for development of innovation method needed for creation of new highly qualified breeding plant material regarded as a source for nearest breeding practice and seed production. At VNIISSOK the richest plant collection with important genes and donor genotypes of productivity, fast ripening, high quality, resistance to biotic and abiotic stresses is created in Cucurbitaceae, Solanaceae,Alliaceae, Fabaceae, root vegetables, Brassicas, leafy crops, aromatic and medicinal crops and ornamental crops. Core plant collection is substantially extending by means of introduction of new crops and non-traditional ones as well. The specialist-breeders of VNIISSOK have developed over 800 cultivars and hybrids F1 of vegetables, melons and gourds, aromatic plants, ornamental plants, non-traditional. 546 accessions out of 118 crops have been included

A multifrequency study of the radio structure of 3C10, the remnant of Tycho's supernova

International Nuclear Information System (INIS)

Duin, R.M.; Strom, R.G.

1975-01-01

Synthesis observations of 3C10 have been made at 6 cm and 50 cm using the Westerbork telescope. Combining these results with earlier 21 cm Westerbork maps, we have made detailed comparisons between the three wavelengths. The total intensity maps are remarkably similar: we find no evidence for changes in the spectral index of small scale features around the rim of the shell-like remnant. On the large scale, however, there appears to be a significant steepening of the spectrum near the center of 3C10. We believe this to be related to the fact that the integrated radio spectrum steepens at low frequencies, and suggest that particles presently near the outer boundary may be accelerated with a relatively flat energy spectrum. Although no linear polarization exceeding about 1% of the total intensity could be detected at 50 cm, at 6 cm the polarized emission is quite smooth, being typically 10% of the total intensity. The position angle distribution of the linear polarization is also smooth, confirming our earlier conclusion that 3C10 is surrounded by an irregular Faraday screen. By comparing our 6 cm map with 2.8 cm and 10.4 cm results we are able to construct a rotation measure map, and confirm that the intrinsic position angles are tangentially aligned, with an average rotation measure of -249 rad m -2 . We conclude that the ordered component of the magnetic field is radially directed, and suggest that the mechanism for producing such a configuration can be found in the Sedov solution for shock waves in a fluid medium. (orig.) [de

Modeling for Stellar Feedback in Galaxy Formation Simulations

Science.gov (United States)

Núñez, Alejandro; Ostriker, Jeremiah P.; Naab, Thorsten; Oser, Ludwig; Hu, Chia-Yu; Choi, Ena

2017-02-01

Various heuristic approaches to model unresolved supernova (SN) feedback in galaxy formation simulations exist to reproduce the formation of spiral galaxies and the overall inefficient conversion of gas into stars. Some models, however, require resolution-dependent scalings. We present a subresolution model representing the three major phases of supernova blast wave evolution—free expansion, energy-conserving Sedov-Taylor, and momentum-conserving snowplow—with energy scalings adopted from high-resolution interstellar-medium simulations in both uniform and multiphase media. We allow for the effects of significantly enhanced SN remnant propagation in a multiphase medium with the cooling radius scaling with the hot volume fraction, {f}{hot}, as {(1-{f}{hot})}-4/5. We also include winds from young massive stars and AGB stars, Strömgren sphere gas heating by massive stars, and a mechanism that limits gas cooling that is driven by radiative recombination of dense H II regions. We present initial tests for isolated Milky Way-like systems simulated with the Gadget-based code SPHgal with improved SPH prescription. Compared to pure thermal SN input, the model significantly suppresses star formation at early epochs, with star formation extended both in time and space in better accord with observations. Compared to models with pure thermal SN feedback, the age at which half the stellar mass is assembled increases by a factor of 2.4, and the mass-loading parameter and gas outflow rate from the galactic disk increase by a factor of 2. Simulation results are converged for a variation of two orders of magnitude in particle mass in the range (1.3-130) × 104 solar masses.

PHYSICS OF A PARTIALLY IONIZED GAS RELEVANT TO GALAXY FORMATION SIMULATIONS-THE IONIZATION POTENTIAL ENERGY RESERVOIR

Energy Technology Data Exchange (ETDEWEB)

Vandenbroucke, B.; De Rijcke, S.; Schroyen, J. [Department of Physics and Astronomy, Ghent University, Krijgslaan 281, S9, B-9000 Gent (Belgium); Jachowicz, N. [Department of Physics and Astronomy, Ghent University, Proeftuinstraat 86, B-9000 Gent (Belgium)

2013-07-01

Simulation codes for galaxy formation and evolution take on board as many physical processes as possible beyond the standard gravitational and hydrodynamical physics. Most of this extra physics takes place below the resolution level of the simulations and is added in a ''sub-grid'' fashion. However, these sub-grid processes affect the macroscopic hydrodynamical properties of the gas and thus couple to the ''on-grid'' physics that is explicitly integrated during the simulation. In this paper, we focus on the link between partial ionization and the hydrodynamical equations. We show that the energy stored in ions and free electrons constitutes a potential energy term which breaks the linear dependence of the internal energy on temperature. Correctly taking into account ionization hence requires modifying both the equation of state and the energy-temperature relation. We implemented these changes in the cosmological simulation code GADGET2. As an example of the effects of these changes, we study the propagation of Sedov-Taylor shock waves through an ionizing medium. This serves as a proxy for the absorption of supernova feedback energy by the interstellar medium. Depending on the density and temperature of the surrounding gas, we find that up to 50% of the feedback energy is spent ionizing the gas rather than heating it. Thus, it can be expected that properly taking into account ionization effects in galaxy evolution simulations will drastically reduce the effects of thermal feedback. To the best of our knowledge, this potential energy term is not used in current simulations of galaxy formation and evolution.

The work of the couple Brailowsky in the mirror of Serbian critiques

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Mosusova Nadežda

2003-01-01

Full Text Available Leonid (1867-1937 and Rimma (1877-1959 Brailowsky brought to Belgrade National theatre (together with other Russian emigrated stage and costume designers the spirit of the World of Art (Mir Iskusstva, making décor and costumes for 18 performances during the period of 1921-1924. Les romanesques by Edmond Rostand, Le malade imaginaire by Molière, Shakespeare's Richard III, Merchant of Venice and King Lear and two Serbian dramas, Offenbach's Hoffmann's Tales, Faust by Gounod, Smetana's Bartered Bride, Bizet's Carmen Onegin and Queen of Spades by Tchaikovsky, Massenet's Manon, The Tsar's Bride by Rimsky-Korsakov, The Wedding of Miloš by Petar Konjović, the Serbian opera composer, two ballets, Sheherazade and Nutcracker. The artists, husband and wife, were praised for their modernization of the Belgrade scene, for their vivid realization of sets and costumes, for their novelties, especially in Serbian historical dramas by Branislav Nušić and Milutin Bojić, and Shakespeare as well. In operas and ballets they were also respected in some extent, but the pictorial, sometimes independent value of their scenic work, although inspired by music, arouse opposing questions among the musical critics, who could not accept their too bright colors which once conquered Paris in the scenic interpretation of Leon Bakst or Nikolai Roerich. To avoid resistance of Belgrade critics the couple decided to leave Yugoslav capital for Italy where they continued successfully their artistic career.

Integral Field Spectroscopy of Balmer-dominated Shocks in the Magellanic Cloud Supernova Remnant N103B

Energy Technology Data Exchange (ETDEWEB)

Ghavamian, Parviz [Department of Physics, Astronomy and Geosciences, Towson University, Towson, MD 21252 (United States); Seitenzahl, Ivo R.; Dopita, M. A. [Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611 (Australia); Vogt, Frédéric P. A. [European Southern Observatory, Av. Alonso de Córdova 3107, 763 0355 Vitacura, Santiago (Chile); Terry, Jason P. [Department of Physics and Astronomy, University of Georgia (United States); Williams, Brian J. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Winkler, P. Frank, E-mail: pghavamian@towson.edu [Department of Physics, Middlebury College, Middlebury, VT 05753 (United States)

2017-10-01

We present results of integral field spectroscopy of Balmer-dominated shocks in the LMC supernova remnant (SNR) N103B, carried out using the Wide Field Integral Spectrograph (WiFeS ) on the 2.3 m telescope at the Siding Spring Observatory in Australia. Existing X-ray studies of N103B have indicated an SN Ia origin. Radiative shock emission from clumpy material surrounding the SNR may result from interaction of the forward shock with relic stellar wind material, possibly implicating a thermonuclear explosion in a single-degenerate binary system. The recently discovered Balmer-dominated shocks mark the impact of the forward shock with low density, partially neutral CSM gas, and form a partial shell encircling clumps of material exhibiting radiative shocks. The WiFeS spectra of N103B reveal broad H α emission having a width as high as 2350 km s{sup −1} along the northern rim, and both H α and H β broad profiles having widths around 1300 km s{sup −1} along the southern rim. Fits to the H α line profiles indicate that in addition to the usual broad and narrow emission components, a third component of intermediate width exists in these Balmer-dominated shocks, ranging from around 125 km s{sup −1} up to 225 km s{sup −1} in width. This is consistent with predictions of recent Balmer-dominated shock models, which predict that an intermediate-width component will be generated in a fast neutral precursor. We derive a Sedov age of approximately 685 ± 20 years for N103B from the Balmer-dominated spectra, consistent with the young age of 380–860 years estimated from light echo studies.

Do the TTBT and JVE provide a framework for 'effective' verification?

International Nuclear Information System (INIS)

Vergino, E.S.

1998-01-01

The Threshold Test Ban Treaty (TTBT) was signed in 1974 by Richard Nixon and Leonid Brezhnev with both the US and USSR agreeing to adhere to the 150 kt limit of the treaty as of March 31, 1976. Yet the treaty remained non ratified for more than twelve years and during this time during the height of the Cold War, the US and USSR continued to accuse one another of violating the treaty. During late 1987, during the Nuclear Testing Talks in Geneva the Joint Verification Experiment (JVE) was discussed and then was formally announced at the Shultz/Shevardnadze meeting in December, 1987. In the course of arranging JVE Information and data for five Soviet and five US nuclear tests, were exchanged. JVE activity culminated with Kearsarge, detonated on August 17, 1988 and Shagan, detonated on September 14, 1988. JVE provided a unique opportunity for US and USSR technical experts to work together to demonstrate that effective verification of the TTBT could be achieved. The TTBT was the first treaty in which the US pursued a series of complex protocols involving additional, intrusive verification measures. These required extensive collaboration between scientific and political communities, a collaboration necessary to address the balance between the technical capabilities and requirements and the political drivers and needs. During this talk the author discusses this balance, how the balance changed with time, the drivers for change and the lessons learned, and weather there are lessons to be learned that are applicable to the development of other, future, arms control agreements

РУССКИЕ МАСТЕРА БАЛЕТА НА БЕЛГРАДСКОЙ СЦЕНЕ В XX – НАЧАЛЕ XXI ВВ.

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Viktor Ivanovich Kosik

2017-02-01

Full Text Available The main goal of the article is to outline significant contribution to the history of Belgrade ballet of those Russian dancers who came to the Kingdom of Serbia after leaving Russia in 1917, and to monitor the contribution of the next generations of Russian masters who came to Belgrade, the capital of the Kingdom of Yugoslavia, later the Socialistic Federative Republic of Yugoslavia. They have invested a lot of their effort, talent, and time, laid the foundations and provided very fast development of Belgrade ballet so that it caught up step with European ballet scene. The article, based on numerous sources and literature, including unpublished memoirs, confirmed that dancers who came after Bolshevik revolution contributed to the establishment of the national ballet center at the Belgrade National Theater and the ballet school where the first dancers of the Serbian origin were formed under the tutelage of Elena Poljakova, Nina Kirsanova, Xenia Grundt-Dumet. Celebrated ballerinas Anna Pavlova and Tamara Karsavina performed at the Belgrade stage in the twenties of the last century. In addition, unlike previously common approaches to this subject limited to the role and activity of the Russian emigration in the interwar period, the article is extended from the period during and after the Second World War to the present days. Accordingly, the paper includes the renowned Soviet masters such as Leonid Lavrovsky, Maya Plisetskaya, Natalia Dudinskaya, and those who have played important role in the contemporary ballet life in Serbia, to name Hmela, Pilipenko, Kasatkin, Logunov, and Kostjukov.

Gynaecomastia and scrotal rhacosis: two aesthetic surgical operations for men in Byzantine times.

Science.gov (United States)

Papadakis, Marios; Manios, Andreas; de Bree, Eelco; Trompoukis, Constantinos; Tsiftsis, Dimitris D

2010-08-01

Nowadays, as in the past, much attention is paid to aesthetic operations in women, while only infrequently have such operations been referred to in males. Generally, male aesthetic surgery was introduced to surgical practise during the 19th century. In this study, we analysed the practise of such operations in Byzantine times and in other ancient cultures with surgical knowledge, i.e. ancient India and China The sixth book of Paul of Aegina's "Epitome of Medicine" was studied for description of aesthetic operations in males in the Byzantine period, since this book is completely devoted to surgery and is generally considered to be the most important reference for surgery in Byzantine times. The original text and its excellent translation by Francis Adams were used. References concerning aesthetic operations for males were identified. Accordingly, historical work and reviews on plastic surgery in ancient India and China were studied. Mainly, two aesthetic surgical procedures for males in the Byzantine period were identified. These two procedures comprise gynaecomastia and rhacosis (scrotal relaxation). Two different techniques were reported for the surgical management of gynaecomastia, through sub-mammary or supra-mammary access. Two procedures were noted for rhacosis, for which Paul of Aegina reproduced the respective chapters from Leonides' and Antyllus' works. Evidence supporting male aesthetic surgery in ancient India and China or elsewhere was not found. Despite the dubious aesthetic result, the existence of different aesthetic surgical techniques in males substantiate the advanced level of surgery achieved by physicians in the Byzantine period. Copyright 2010 British Association of Plastic, Reconstructive and Aesthetic Surgeons. Published by Elsevier Ltd. All rights reserved.

«Odessa branch of «the True Orthodox Church» 1935: Tragic Scenario of the Soviet Secret Service

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Nikolay I. Mikhaylutsa

2012-12-01

Full Text Available The article is concerned with the bolshevists’ violence against adepts of “the True Orthodox Church” in Odessa in the middle 30s of the XX century. The article is focused on the case, framed up in January, 1935 by local authorities of NKVD (People's Commissariat for Internal Affairs against “Odessa branch of “the True Orthodox Church”. Investigator chose monk-pilgrim Leonid Vasilevich Salkov as the founder and ideological instigator of the branch. Besides, F.S. Pospelov, V.I. Ivanov, G.I. Balukhatin and S.Ya. Kokh were arrested in January, 1935 pursuant to the decrees by Odessa Oblast Authority of NKVD and Odessa Oblast Attorney Office. Investigation didn’t manage to collect any material evidence, but almost all the interrogated, pressed by the NKVD investigators confessed the participation in illegal branch of “the True Orthodox Church”, except former secretary of Odessa Diocesan Authority F.S. Pospelov. Yet, L. Salkov was sentenced to 5 years in labour camps, V. Ivanov and G. Balakhutin to 3 years in labour camps and S. Kokh and F. Pospelov to 3 years of exile by the decision of the special council of NKVD of the USSR d.d. 13 September, 1935.The article considers the factors, which were crucial in framing up of “the True Orthodox Church case”, shows the geography of Odessa branch relationship with other regions of the country, methods and techniques, used by officers of NKVD authorities to frame up the cases of the investigated persons, gravamen and consequences of the repressions of “Odessa branch of “the True Orthodox Church” participants.

Langton's flies

International Nuclear Information System (INIS)

Dorbec, P; Gajardo, A

2008-01-01

Langton's ant is an automaton defined over a two-dimensional grid. Its movement is governed by the environment in a very simple way: it turns to the left over white vertices and to the right over black vertices. This definition only applies on a two-dimensional space. We look for generalizations of this automaton to n-dimensional lattices. Remembering the different ways through which the ant was originally defined, we consider two approaches: the first comes from physics (lattice gas) and the second from artificial life (virtual ants). Two generalizations are proposed defining two families of dynamical systems. From the physics point of view, the ant is seen as a particle and hence it has no internal state other than its velocity. From the artificial life point of view, the ant is viewed as an insect, and it has an orientation in space which we represent by an orthogonal basis. This constitutes the ant's internal state. This formulation allows us to define the ant's behaviour without drawing upon any information relative to the global system of external coordinates. Each model yields different sets of rules with distinctive behaviours. We characterize all the possible rules satisfying some basic restrictions. We found that many rules produce trajectories which are restricted to a diagonal plane and are equivalent to a version of Langton's ant over a two-dimensional grid, squared or hexagonal. In the particle model, only two of them use the whole space, and it is shown that such rules do not admit periodical trajectories. This result reinforces a previous one reported by Leonid Bunimovich, who states that 'the skeleton of any bounded trajectory cannot contain any three-dimensional polyhedron'

A DETAILED X-RAY INVESTIGATION OF PSR J2021+4026 AND THE γ-CYGNI SUPERNOVA REMNANT

Energy Technology Data Exchange (ETDEWEB)

Hui, C. Y.; Seo, K. A. [Department of Astronomy and Space Science, Chungnam National University, Daejeon (Korea, Republic of); Lin, L. C. C.; Huang, R. H. H.; Wu, J. H. K.; Kong, A. K. H. [Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan (China); Hu, C. P.; Chou, Y. [Graduate Institute of Astronomy, National Central University, Jhongli 32001, Taiwan (China); Trepl, L. [Astrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, Schillergäßchen 2-3, D-07745 Jena (Germany); Takata, J.; Wang, Y.; Cheng, K. S., E-mail: cyhui@cnu.ac.kr [Department of Physics, University of Hong Kong, Pokfulam Road (Hong Kong)

2015-01-20

We have investigated the field around the radio-quiet γ-ray pulsar, PSR J2021+4026, with a ∼140 ks XMM-Newton observation and ∼56 ks archival Chandra data. Through analyzing the pulsed spectrum, we show that the X-ray pulsation is purely thermal in nature, which suggests that the pulsation originated from a hot polar cap with T ∼ 3 × 10{sup 6} K on the surface of a rotating neutron star. On the other hand, the power-law (PL) component that dominates the pulsar emission in the hard band is originated from off-pulse phases, which possibly comes from a pulsar wind nebula. In re-analyzing the Chandra data, we have confirmed the presence of a bow-shock nebula that extends from the pulsar to the west by ∼10 arcsec. The orientation of this nebular feature suggests that the pulsar is probably moving eastward, which is consistent with the speculated proper motion by extrapolating from the nominal geometrical center of the supernova remnant (SNR) G78.2+2.1 to the current pulsar position. For G78.2+2.1, our deep XMM-Newton observation also enables a study of the central region and part of the southeastern region with superior photon statistics. The column absorption derived for the SNR is comparable to that for PSR J2021+4026, which supports their association. The remnant emission in both of the examined regions is in a non-equilibrium ionization state. Also, the elapsed time of both regions after shock-heating is apparently shorter than the Sedov age of G78.2+2.1. This might suggest that the reverse shock has reached the center not long ago. Apart from PSR J2021+4026 and G78.2+2.1, we have also serendipitously detected an X-ray flash-like event, XMM J202154.7+402855, from this XMM-Newton observation.

On the cosmic ray spectrum from type II Supernovae expanding in their red giant presupernova wind

Science.gov (United States)

Cardillo, Martina

2015-12-01

While from the energetic point of view SNRs are viable sources of Galactic CRs, the issue of whether they can accelerate protons up to PeV remains unsolved. Here we discuss particle acceleration at the forward shock of SN and discuss the possibility that the escaping particle current may excite a non-resonant instability that in turn leads to the formation of resonant modes confining particles close to the shock and increasing the maximum energy. This mechanism works throughout the expansion of the SN explosion, from the ejecta dominated (ED) to the Sedov-Taylor (ST) phase. Because of their higher explosion rate,we focus on type II SNae expanding in the slow, dense red supergiant wind. When the explosion occurs in such winds, the transition between the ED and the ST phase is likely to take place within a few tens of years. As a result, the spectrum of accelerated particles shows a break in the slope, at the maximum energy (EM) achieved at the beginning of the ST phase. Above this energy, the spectrum becomes steeper but remains a power law than developing an exponential cutoff. We show that for type II SNae typical parameters, proton EM can easily reach PeV energies, confirming that type II SNRs are the best candidate sources for CRs at the knee. We have tried to fit KASCADE-Grande, ARGO -YBJ and YAC1-Tibet Array data with our model but we could not find any parameter combination that could explain all data sets. Indeed the recent measurement of the proton and helium spectra in the knee region, with the ARGO-YBJ and YAC1-Tibet Array, has made the situation very confused. These measurements suggest that the knee in the light component is at 650 TeV, appreciably below the overall spectrum knee. This finding would resolve the problem of reaching very high energies in SNae, but, on the other hand, it would open a critical issue in the transition region between Galactic and extragalactic CRs.

High-order shock-fitted detonation propagation in high explosives

Science.gov (United States)

Romick, Christopher M.; Aslam, Tariq D.

2017-03-01

A highly accurate numerical shock and material interface fitting scheme composed of fifth-order spatial and third- or fifth-order temporal discretizations is applied to the two-dimensional reactive Euler equations in both slab and axisymmetric geometries. High rates of convergence are not typically possible with shock-capturing methods as the Taylor series analysis breaks down in the vicinity of discontinuities. Furthermore, for typical high explosive (HE) simulations, the effects of material interfaces at the charge boundary can also cause significant computational errors. Fitting a computational boundary to both the shock front and material interface (i.e. streamline) alleviates the computational errors associated with captured shocks and thus opens up the possibility of high rates of convergence for multi-dimensional shock and detonation flows. Several verification tests, including a Sedov blast wave, a Zel'dovich-von Neumann-Döring (ZND) detonation wave, and Taylor-Maccoll supersonic flow over a cone, are utilized to demonstrate high rates of convergence to nontrivial shock and reaction flows. Comparisons to previously published shock-capturing multi-dimensional detonations in a polytropic fluid with a constant adiabatic exponent (PF-CAE) are made, demonstrating significantly lower computational error for the present shock and material interface fitting method. For an error on the order of 10 m /s, which is similar to that observed in experiments, shock-fitting offers a computational savings on the order of 1000. In addition, the behavior of the detonation phase speed is examined for several slab widths to evaluate the detonation performance of PBX 9501 while utilizing the Wescott-Stewart-Davis (WSD) model, which is commonly used in HE modeling. It is found that the thickness effect curve resulting from this equation of state and reaction model using published values is dramatically more steep than observed in recent experiments. Utilizing the present fitting

Laser light scattering in a laser-induced argon plasma: Investigations of the shock wave

Energy Technology Data Exchange (ETDEWEB)

Pokrzywka, B. [Obserwatorium Astronomiczne na Suhorze, Uniwersytet Pedagogiczny, ulica Podchorazych 2, 30-084 Krakow (Poland); Mendys, A., E-mail: agata.mendys@uj.edu.pl [Instytut Fizyki im. M. Smoluchowskiego, Uniwersytet Jagiellonski, ulica Reymonta 4, 30-059 Krakow (Poland); Dzierzega, K.; Grabiec, M. [Instytut Fizyki im. M. Smoluchowskiego, Uniwersytet Jagiellonski, ulica Reymonta 4, 30-059 Krakow (Poland); Pellerin, S. [GREMI, site de Bourges, Universite d' Orleans, CNRS, rue Gaston Berger BP 4043, 18028 Bourges (France)

2012-08-15

Shock wave produced by a laser induced spark in argon at atmospheric pressure was examined using Rayleigh and Thomson scattering. The spark was generated by focusing a laser pulse from the second harmonic ({lambda} = 532 nm) of a nanosecond Nd:YAG laser using an 80 mm focal length lens, with a fluence of 2 kJ{center_dot}cm{sup -2}. Images of the spark emission were recorded for times between 30 ns and 100 {mu}s after the laser pulse in order to characterize its spatial evolution. The position of the shock wave at several instants of its evolution and for several plasma regions was determined from the Rayleigh-scattered light of another nanosecond Nd:YAG laser (532 nm, 40 J{center_dot}cm{sup -2} fluence). Simultaneously, Thomson scattering technique was applied to determine the electron density and temperature in the hot plasma core. Attempts were made to describe the temporal evolution of the shock wave within a self-similar model, both by the simple Sedov-Taylor formula as well as its extension deduced by de Izarra. The temporal radial evolution of the shock position is similar to that obtained within theory taking into account the counter pressure of the ambient gas. Density profiles just behind the shock front are in qualitative agreement with those obtained by numerically solving the Euler equations for instantaneous explosion at a point with counter pressure. - Highlights: Black-Right-Pointing-Pointer We investigated shock wave evolution by Rayleigh scattering method. Black-Right-Pointing-Pointer 2D map of shockwave position for several times after plasma generation is presented. Black-Right-Pointing-Pointer Shock wave evolution is not satisfactorily described within self-similar models. Black-Right-Pointing-Pointer Evolution of shock position similar to theory taking into account counter pressure. Black-Right-Pointing-Pointer Density profile behind the shock similar to numerical solution of Euler equations.

From the Editor

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Željko Hutinski

2012-07-01

Full Text Available All the papers in this issue of the JIOS Journal may fit into the Science as Usual categoryand are therefore not going to be dealt with in detail in the introduction. However, for oneof the papers included an exception has been provided, namely the paper Sigma-notationand the equivalence of P and NP classes by Miron Ivanovich Telpiz. The circumstancesleading to its publication in this issue of JIOS are presented by the editors in this preface.It is generally acknowledged that, ever since it was defined by S. Cook over thirty yearsago, P = NP has presented one of the major open problems in computing science andinformation science in general. Whereas, on one hand, this problem presents a formidablechallenge to any scientist dealing with it, its solution, especially in case it should turn out tobe a positive one considering that current technology tends to evolve in a practicaldirection and its overall functioning is conducted implicitly under the assumption of anegative solution would have a major impact on the development of informationtechnology as well as the wider context of human society as a whole. Apart from being putforward in conferences, both positive and negative “solutions” to P = NP problem can beoccasionally found in press, scientific and professional journals. The web page titled “Pversus-NP Page” (see http://www.win.tue.nl/~gwoegi/P-versus-NP.htm provides anexcellent source for this issue. It contains links to papers stating that P = NP, as well asthose contradicting the opposite, i.e., stating that P NP. Furthermore, references are givento Oded Goldreich's rationale behind his decision not to review papers proposing solutionsto P = NP problem and related difficult problems because, in his own words, they “alsoattract the attention of non-experts, and one annoying consequence is a flood of falseclaims of resolutions of these problems” (see http://www.wisdom.weizmann.ac.il/~oded/faq.html. Dr. Goldreich a recognised

Processing of low-quality bauxite feedstock by thermochemistry-Bayer method

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О. А. Дубовиков

2016-11-01

Full Text Available The modern production of aluminum which by its global output ranks first among the non-ferrous metals includes three main stages: ore extraction, its processing into alumina and, finally, the production of primary aluminum. Alumina production from bauxites,  being the  primary raw material in the  alumina industry,  is based  on two main methods: the Bayer method and the sintering method developed in Russia under the lead of an academician Nikolay Semenovich Kurnakov. Alumina production by the Bayer’s method is more cost effective,  but  has  higher  requirements to the  quality of the bauxite feedstock.  A great deal  of research has  been carried  out on low quality bauxites focusing firstly on finding ways to enrich the feedstock, secondly on improving the combined sequential Bayer-sintering method and thirdly on developing new hydrometallurgical ways for bauxites processing. Mechanical methods of bauxite enrichment have not yet brought any positive outcome, and a development of new hydrometallurgical high alkaline  autoclave process  faced  significant hardware  difficulties not addressed so far. For efficient processing of such low quality bauxite feedstock it is suggested to use a universal thermochemistry-Bayer method, which was developed in St. Petersburg Mining University under  the lead  of  Nikolay Ivanovich Eremin, allows to process different substandard bauxite feedstock and has a competitive costing as compared to the sintering method and combined methods. The main stages of thermochemistry-Bayer method are thermal activation of feedstock, its further desiliconization with the alkaline solution and leaching of the resultant bauxite product  under Bayer’s method. Despite high energy consumption at  the baking stage,  it  allows to condition the  low quality bauxite feedstock by neutralizing a variety of technologically harmful impurities such as organic matter, sulfide sulfur, carbonates, and at the

http://periodical.pstgu.ru/en/pdf/article/2425

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A. AVDEEV

2014-02-01

Full Text Available In the paper considered gravestones with epitaphs of the end of the 15 th—16th century from Kashin (modern Tver region, which are an important source of medieval Kashin’s topography. In this regard the paper looks into the question Kashin city structure history and the directions of its development in the 15th — the end of the 16th century. On the basis of the sources along with epigraphical monuments are put in the sources published so far and among them — annales, lives of sacred from Kashin, acts from monastic archives, Census book of church lands of Kashin of 1621, and also the results of archaeological researches which report about the earliest elements of Kashin’s city building of — ostrog, churches and monasteries which existed in the last third of 14th — the beginning of the 17th century. From them the most ancient are city ostrog (built anew in 1392/93 and the Uspensky monastery (the first mention — 1368. The subscriptions gravestones connected with ancient necropolises, add to the list the first mentions of the Dimitrovsky monastery (1491, list churches st. Forty martyrs of Sevasty (1537, st. Ioakim and Anna (1594 and the Signs of the Mother of God (1594. Data of sources shows that in the last third of 14th — the end of the 16th century Kashin’s territory developed from the downtown in four directions. The northern, the east and the southern directions are obviously synchronous to each other. The southwest direction which, probably, developed less intensively is less documented by sources. The remained sources show an asynchronical emergence of separate sites of the city building and disprove the idea spread in local history literature, of the existance of Kashin “sacral plan“, which is allegedly was prêt as a platform for the building planning of the city. In the paper periods of active city planning connected with the activity of Princes of Kaschin Vasily Mikhaylovich (1319-1349/50 and Yury Ivanovich (1504

Effects and safety profile of betahistine in patients in the Russian contingent of OSVaLD, an open-label observational study in vestibular vertigo

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Morozova SV

2015-01-01

Full Text Available Svetlana Vyacheslavovna Morozova,1 Natalia Stepanovna Alekseeva,2 Sergey Vasilyevich Lilenko,3 Eduard Ivanovich Matsnev,4 Oleg Anatol'evich Melnikov51Department of Ear, Nose, and Throat, State Budgetary Educational Institution of Higher Professional Training, IM Sechenov First Moscow State Medical University of the Ministry of Healthcare and Social Development of the Russian Federation, Moscow, 2Federal State Budgetary Institution, Scientific Neurology Center of the Russian Academy of Medical Sciences, Moscow, 3St Petersburg Research Institute of Ear, Throat, Nose and Speech, St Petersburg, 4Department of Physiology and Pathology of Auditory and Vestibular Systems, Federal Scientific Center (FSC, Institute for Biomedical Problems, Russian Academy of Sciences (RAS, Moscow, 5ANO Guta Clinic, Moscow, Russian Federation Background: We report here data from the >200 patients recruited in Russia to take part in OSVaLD, a 12-week, open-label, post-marketing surveillance study of the response to betahistine 48 mg/day in vertigo of peripheral vestibular origin carried out in a total of 13 countries.Methods: The primary efficacy endpoint was change in the Dizziness Handicap Inventory (DHI; 100-point scale. Changes in Hospital Anxiety and Depression Scale (HADS and Medical Outcomes Study Short-Form 36, version 2 (SF-36v2® scores were a priori secondary Outcomes.Results: Total DHI score improved by 43 points during betahistine treatment. This aggregate improvement was equally distributed across the three domains of the DHI (physical, emotional, and functional; P<0.0001 for main and subscore changes from baseline. Statistically significant improvements versus baseline were also observed in mean HADS scores for anxiety and depression (both P<0.0001, and in the Physical Component Summary and Mental Component Summary scores of the SF-36v2 (both P<0.0001 versus baseline. Only one suspected adverse drug reaction was recorded in the Russian safety population (n

SURVEYING THE DYNAMIC RADIO SKY WITH THE LONG WAVELENGTH DEMONSTRATOR ARRAY

International Nuclear Information System (INIS)

Lazio, T. Joseph W.; Clarke, Tracy E.; Lane, W. M.; Gross, C.; Kassim, N. E.; Hicks, B.; Polisensky, E.; Stewart, K.; Ray, P. S.; Wood, D.; York, J. A.; Kerkhoff, A.; Dalal, N. Paravastu; Cohen, A. S.; Erickson, W. C.

2010-01-01

This paper presents a search for radio transients at a frequency of 73.8 MHz (4 m wavelength) using the all-sky imaging capabilities of the Long Wavelength Demonstrator Array (LWDA). The LWDA was a 16-dipole phased array telescope, located on the site of the Very Large Array in New Mexico. The field of view of the individual dipoles was essentially the entire sky, and the number of dipoles was sufficiently small that a simple software correlator could be used to make all-sky images. From 2006 October to 2007 February, we conducted an all-sky transient search program, acquiring a total of 106 hr of data; the time sampling varied, being 5 minutes at the start of the program and improving to 2 minutes by the end of the program. We were able to detect solar flares, and in a special-purpose mode, radio reflections from ionized meteor trails during the 2006 Leonid meteor shower. We detected no transients originating outside of the solar system above a flux density limit of 500 Jy, equivalent to a limit of no more than about 10 -2 events yr -1 deg -2 , having a pulse energy density ∼>1.5 x 10 -20 J m -2 Hz -1 at 73.8 MHz for pulse widths of about 300 s. This event rate is comparable to that determined from previous all-sky transient searches, but at a lower frequency than most previous all-sky searches. We believe that the LWDA illustrates how an all-sky imaging mode could be a useful operational model for low-frequency instruments such as the Low Frequency Array, the Long Wavelength Array station, the low-frequency component of the Square Kilometre Array, and potentially the Lunar Radio Array.

"Aparat" čy "dyspozytyv"? Notatky pro vyrobnyctvo obrazu i vyrobnyctvo sub''jekta v kino

Directory of Open Access Journals (Sweden)

Ol'ha Briukhovets'ka

2015-09-01

Während der Begriff "Apparatus" in der Filmtheorie gut etabliert ist, ging sein Pendant und zugleich korrelatives Double "Dispositiv" (ebenfalls in die Filmtheorie von Jean-Louis Baudry in den 1970er Jahren eingeführt, bei der Übersetzung aus dem Französischen ins Englische verloren. So verschwand auch der nuancierte Bedeutungsunterschied zwischen den beiden Begriffen, und damit die Unterscheidung von zwei Prozessen – einem, der sich auf die Bildproduktion bzw. die Figuration bezieht, und einem anderen, bei dem es um die Subjektproduktion bzw. die Subjektwerdung geht. Der Begriff "Dispositiv" tauchte in der Filmtheorie gelegentlich als Ersatz für den Begriff oder die Theorie des "Apparatus" auf. Der Beitrag beabsichtigt, die ursprüngliche Unterscheidung zwischen den beiden Begriffen wieder herzustellen und ein mögliches Vorgehen nicht nur für die Filmtheorie, sondern auch für die Analyse bestimmter Filme aufzuzeigen. Am Beispiel von zwei Filmen, Tini zabutich predkiv / Schatten der vergessenen Vorfahren (Sergij Paradžanov, 1965, Sowjetunion und Bol’šaja žizn’. Vtoraja čast’ / Das große Leben. Zweiter Teil  (Leonid Lukov, 1946, Sowjetunion wird gezeigt, wie die beiden Begriffe "Apparatus" und "Dispositiv" in konkreten filmischen Texten angewandt werden könnten. Schatten der vergessenen Vorfahren wurde mit proto-faschistischen Bergfilmen verglichen, wenn auch nur auf der Ebene des "Produktionsdramas",  um zu zeigen, wie durch das optische Unbewusste des Apparatus, der Bildproduktion und der Figuration das ethnisch Andere zurückgewiesen wird. Die Dezentrierung des Bildes, welche die grundlegenden, ungeschriebenen Regel des Anthropozentrismus verletzt, entblößt am Ende von Das große Leben. Zweiter Teil ein stalinistisches Dispositiv, seine spezifische Generierung des Subjekts und dessen Interpellation.

GRADSPMHD: A parallel MHD code based on the SPH formalism

Science.gov (United States)

Vanaverbeke, S.; Keppens, R.; Poedts, S.

2014-03-01

Sedov test including 15625 particles on a single CPU. Classification: 12. Nature of problem: Evolution of a plasma in the ideal MHD approximation. Solution method: The equations of magnetohydrodynamics are solved using the SPH method. Running time: The test provided takes approximately 20 min using 4 processors.

GTPases and the origin of the ribosome

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Smith Temple F

2010-05-01

Full Text Available Abstract Background This paper is an attempt to trace the evolution of the ribosome through the evolution of the universal P-loop GTPases that are involved with the ribosome in translation and with the attachment of the ribosome to the membrane. The GTPases involved in translation in Bacteria/Archaea are the elongation factors EFTu/EF1, the initiation factors IF2/aeIF5b + aeIF2, and the elongation factors EFG/EF2. All of these GTPases also contain the OB fold also found in the non GTPase IF1 involved in initiation. The GTPase involved in the signal recognition particle in most Bacteria and Archaea is SRP54. Results 1 The Elongation Factors of the Archaea based on structural considerations of the domains have the following evolutionary path: EF1→ aeIF2 → EF2. The evolution of the aeIF5b was a later event; 2 the Elongation Factors of the Bacteria based on the topological considerations of the GTPase domain have a similar evolutionary path: EFTu→ IF→2→EFG. These evolutionary sequences reflect the evolution of the LSU followed by the SSU to form the ribosome; 3 the OB-fold IF1 is a mimic of an ancient tRNA minihelix. Conclusion The evolution of translational GTPases of both the Archaea and Bacteria point to the evolution of the ribosome. The elongation factors, EFTu/EF1, began as a Ras-like GTPase bringing the activated minihelix tRNA to the Large Subunit Unit. The initiation factors and elongation factor would then have evolved from the EFTu/EF1 as the small subunit was added to the evolving ribosome. The SRP has an SRP54 GTPase and a specific RNA fold in its RNA component similar to the PTC. We consider the SRP to be a remnant of an ancient form of an LSU bound to a membrane. Reviewers This article was reviewed by George Fox, Leonid Mirny and Chris Sander.

18th International Conference PhysicA.SPb

International Nuclear Information System (INIS)

2016-01-01

Institute), Dr. Mikhail Dunaevskii (Ioffe Institute), Dr. Alexandra Kalashnikova (Ioffe Institute), Dr. Leonid Lutsev (Ioffe Institute). The Editors: Nikita S. Averkiev, Sergey A. Poniaev and Grigorii S. Sokolovskii (paper)

Shooting Stars over China

Science.gov (United States)

Hodges, John

International cultural exchange and education in the sciences and arts is one of the chief aims of the British Council (BC). The 1998 Leonids Meteor Shower was recognised by the BC in China as an event that would offer an opportunity, both to promote the public understanding of space science at an international level, and to encourage on-going cultural links between the United Kingdom and China. Predictions suggested that the 1998 shower, which was likely to be the most intense for more than three decades, would be best viewed in north-east Asia. The BC contracted the Orbital Mechanics Educational Network, an independent organisation that promotes space education amongst young people, to organise several activities aimed particularly at teenagers. The culmination of the project was a visit to Beijing by a party of British teenagers, to take part in meteor observation at China's Mi Yun Observatory. The paper focusses on the practicalities of organising and running such a project and reports on the achievements and shortcomings of the overall venture. It also reports on the observations and findings that were made by the UK group and their Chinese student partners, all of whom were observing a meteor shower for the first time. It reports on the techniques of observing that were tried, the observations themselves and the findings that were made by the group. It also offers advice to those who might wish to set up similar bi-lateral ventures, particularly with China and the UK, and outlines plans to continue and improve the relationships that have been established. (Please note: I realise this is topic not directly covered by the Conference, but how the subject of the meteor phenomenon in particular and, for that matter, science in general is conveyed to the " man in the street" should be important to all scientists, not least because they depend on external funding and public goodwill! Perhaps a suitable slot can be made for this presentation on Tuesday, which is the

Fuel cells science and engineering. Materials, processes, systems and technology. Vol. 1

Energy Technology Data Exchange (ETDEWEB)

Stolten, Detlef; Emonts, Bernd (eds.) [Forschungszentrum Juelich GmbH (DE). Inst. fuer Energieforschung (IEF), Brennstoffzellen (IEF-3)

2012-07-01

The first volume is divided in four parts and 22 chapters. It is structured as follows: PART I: Technology. Chapter 1: Technical Advancement of Fuel-Cell Research and Development (Dr. Bernd Emonts, Ludger Blum, Thomas Grube, Werner Lehnert, Juergen Mergel, Martin Mueller and Ralf Peters); 2: Single-Chamber Fuel Cells (Teko W. Napporn and Melanie Kuhn); 3: Technology and Applications of Molten Carbonate Fuel Cells (Barbara Bosio, Elisabetta Arato and Paolo Greppi); 4: Alkaline Fuel Cells (Erich Guelzow); 5: Micro Fuel Cells (Ulf Groos and Dietmar Gerteisen); 6: Principles and Technology of Microbial Fuel Cells (Jan B. A. Arends, Joachim Desloover, Sebastia Puig and Willy Verstraete); 7: Micro-Reactors for Fuel Processing (Gunther Kolb); 8: Regenerative Fuel Cells (Martin Mueller). PART II: Materials and Production Processes. Chapter 9: Advances in Solid Oxide Fuel Cell Development between 1995 and 2010 at Forschungszentrum Juelich GmbH, Germany (Vincent Haanappel); 10: Solid Oxide Fuel Cell Electrode Fabrication by Infiltration (Evren Gunen); 11: Sealing Technology for Solid Oxide Fuel Cells (K. Scott Weil); 12: Phosphoric Acid, an Electrolyte for Fuel Cells - Temperature and Composition Dependence of Vapor Pressure and Proton Conductivity (Carsten Korte); 13: Materials and Coatings for Metallic Bipolar Plates in Polymer Electrolyte Membrane Fuel Cells (Heli Wang and John A. Turner); 14: Nanostructured Materials for Fuel Cells (John F. Elter); 15: Catalysis in Low-Temperature Fuel Cells - An Overview (Sabine Schimpf and Michael Bron). PART III: Analytics and Diagnostics. Chapter 16: Impedance Spectroscopy for High-Temperature Fuel Cells (Ellen Ivers-Tiffee, Andre Leonide, Helge Schichlein, Volker Sonn and Andre Weber); 17: Post-Test Characterization of Solid Oxide Fuel-Cell Stacks (Norbert H. Menzler and Peter Batfalsky); 18: In Situ Imaging at Large-Scale Facilities (Christian Toetzke, Ingo Manke and Werner Lehnert); 19: Analytics of Physical Properties of Low

Is the shaman indeed risen in post-Soviet Siberia?

Directory of Open Access Journals (Sweden)

Olle Sundström

2012-01-01

Full Text Available In his exhaustive study of ‘shamanism’ among the Altaic peoples in Southern Siberia, the renowned Soviet ethnographer Leonid P. Potapov contends that ‘under the present conditions there are no remnants or survivals of Shamanism as such left in Altai’. What remains are legends and reminiscences, but these can no longer be told by people with personal experiences of Altaic ‘shamans’ and their rituals. According to Potapov, modern socialist culture has changed the minds of the Altaic peoples to the degree that they are now a materialistically thinking people, and ‘shamanism’ has completely disappeared. In addition, he contends that there are no prospects of its return after the deathblow dealt by Soviet anti-religious repression in the 1930s ‘shamanic’ rituals were forbidden and ritual paraphernalia such as drums and costumes were expropriated by the authorities. Considering that Potapov in his study follows Altaic ‘shamanism’ through 1500 years, depicting it as a ‘religion’ and ‘theology’ which stayed more or less intact over the centuries, his statement seems more like a pious hope based on the Soviet vision of a society liberated from superstition, religion, and spiritual exploitation. Potapov himself delineates Altaic ‘shamanism’s’ development from a ‘state religion’to a ‘folk religion’. From this perspective it might seem remarkable that ‘shamanism’ should not have survived 70 years of atheist repression, missionary work and the Soviet transformation of society. Already by the time Potapov’s book was published, during the very last months of the existence of the Soviet Union, there had, in fact, appeared a number of persons claiming to be ‘shamans’, with an ancestry dating from the time of ‘shamans’ of the first half of the twentieth century. These individuals were also part of organisations and movements promoting the revival of ‘shamanism’ in the autonomous Altai Republic. In

Light-element nucleosynthesis in a molecular cloud interacting with a supernova remnant and the origin of beryllium-10 in the protosolar nebula

International Nuclear Information System (INIS)

Tatischeff, Vincent; Duprat, Jean; De Séréville, Nicolas

2014-01-01

The presence of short-lived radionuclides (t 1/2 < 10 Myr) in the early solar system provides important information about the astrophysical environment in which the solar system formed. The discovery of now extinct 10 Be (t 1/2 = 1.4 Myr) in calcium-aluminum-rich inclusions (CAIs) with Fractionation and Unidentified Nuclear isotope anomalies (FUN-CAIs) suggests that a baseline concentration of 10 Be in the early solar system was inherited from the protosolar molecular cloud. In this paper, we investigate various astrophysical contexts for the nonthermal nucleosynthesis of 10 Be by cosmic-ray-induced reactions. We first show that the 10 Be recorded in FUN-CAIs cannot have been produced in situ by irradiation of the FUN-CAIs themselves. We then show that trapping of Galactic cosmic rays (GCRs) in the collapsing presolar cloud core induced a negligible 10 Be contamination of the protosolar nebula, the inferred 10 Be/ 9 Be ratio being at least 40 times lower than that recorded in FUN-CAIs ( 10 Be/ 9 Be ∼ 3 × 10 –4 ). Irradiation of the presolar molecular cloud by background GCRs produced a steady-state 10 Be/ 9 Be ratio ≲ 1.3 × 10 –4 at the time of the solar system formation, which suggests that the presolar cloud was irradiated by an additional source of CRs. Considering a detailed model for CR acceleration in a supernova remnant (SNR), we find that the 10 Be abundance recorded in FUN-CAIs can be explained within two alternative scenarios: (1) the irradiation of a giant molecular cloud by CRs produced by ≳ 50 supernovae exploding in a superbubble of hot gas generated by a large star cluster of at least 20,000 members, and (2) the irradiation of the presolar molecular cloud by freshly accelerated CRs escaped from an isolated SNR at the end of the Sedov-Taylor phase. In the second picture, the SNR resulted from the explosion of a massive star that ran away from its parent OB association, expanded during most of its adiabatic phase in an intercloud medium of

Handbook of RF, Microwave, and Millimeter-Wave Components. Edited by Leonid A. Belov, Sergey M. Smolskiy and Victor N. Kochemasov, Artech House, 2012; 504 pages. Price: £119.00, ISBN 978-1-60807-209-5

Directory of Open Access Journals (Sweden)

Shu-Kun Lin

2013-01-01

Full Text Available This unique and comprehensive resource offers you a detailed treatment of the operations principles, key parameters, and specific characteristics of active and passive RF, microwave, and millimeter-wave components. The book covers both linear and nonlinear components that are used in a wide range of application areas, from communications and information sciences, to avionics, space, and military engineering.

Z Kaliningradu na Кёнигсберг – zapotrzebowanie społeczne czy marzenie nielicznych? Społeczna inicjatywa zmiany nazwy miasta

Directory of Open Access Journals (Sweden)

Miłosz J. Zieliński

2015-04-01

Full Text Available Kaliningrad into Кёнигсберг – a social need or a dream of a few? Societal initiative for a change of the city’s name Kaliningrad Oblast of the Russian Federation has been subject to manifold social processes due to its specific history, geographic conditions and other factors. Some of the former resulted in rejecting numerous elements of the Soviet past by a part of the local population. This included the very name of Kaliningrad, as a tribute paid to Mikhail Ivanovich Kalinin who has been considered one of the state and party officials responsible for mass purges in the 1930s and 1940s. the purpose of the article is to analyse the initiative put forward by a group of social activists to change the name ‘Kaliningrad’ into ‘Кёнигсберг’ (Königsberg, that is to return to the pre-war name of the city. As authors of the petition refer to previous attempts of changing the name and use them as an important part of their reasoning, the history of the notion has also been outlined with emphasis on the December 1988 discussion noted by Alexander Nikolaevich Yakovlev, then a Communist Party official. In the article, a brief introduction of the petition is followed by main arguments used by its supporters and the discussion which the document triggered among the local administration and in the media, in particular the Internet. The discussion concentrated on two aspects of the petition. First, controversies around procedural handling of the petition by Kaliningrad Duma. Secondly, fierce debates about phrases used in the document and their political significance in the context of the contemporary identity of Kaliningrad Oblast. Results of the debate and the impact the petition had on broader public opinion, both in Kaliningrad Oblast and the whole of Russia, turned out to be meagre. Only 400 signatures were collected across the country to support the idea. No decisive measures were taken on the administrative level such as

Impact of recipient-related factors on structural dysfunction of xenoaortic bioprosthetic heart valves

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Barbarash O

2015-03-01

Full Text Available Olga Barbarash, Natalya Rutkovskaya, Oksana Hryachkova, Olga Gruzdeva, Evgenya Uchasova, Anastasia Ponasenko, Natalya Kondyukova, Yuri Odarenko, Leonid Barbarash Federal State Budgetary Scientific Institution Research Institute for Complex Issues of Cardiovascular Diseases, Kemerovo, Russia Objective: To analyze the influence of recipient-related metabolic factors on the rate of structural dysfunction caused by the calcification of xenoaortic bioprostheses. Materials and methods: We retrospectively analyzed clinical status, calcium–phosphorus metabolism, and nonspecific markers of inflammatory response in bioprosthetic mitral valve recipients with calcific degeneration confirmed by histological and electron microscopic studies (group 1, n=22, and in those without degeneration (group 2, n=48. Results: Patients with confirmed calcification of bioprostheses were more likely to have a severe clinical state (functional class IV in 36% in group 1 versus 15% in group 2, P=0.03 and a longer cardiopulmonary bypass period (112.8±18.8 minutes in group 1 versus 97.2±23.6 minutes in group 2, P=0.02 during primary surgery. Patients in group 1 demonstrated moderate hypovitaminosis D (median 34.0, interquartile range [21.0; 49.4] vs 40 [27.2; 54.0] pmol/L, P>0.05, osteoprotegerin deficiency (82.5 [44.2; 115.4] vs 113.5 [65.7; 191.3] pg/mL, P>0.05 and osteopontin deficiency (4.5 [3.3; 7.7] vs 5.2 [4.1; 7.2] ng/mL, P>0.05, and significantly reduced bone-specific alkaline phosphatase isoenzyme (17.1 [12.2; 21.4] vs 22.3 [15.5; 30.5] U/L, P=0.01 and interleukin-8 levels (9.74 [9.19; 10.09] pg/mL vs 13.17 [9.72; 23.1] pg/mL, P=0.045 compared with group 2, with an overall increase in serum levels of proinflammatory markers. Conclusion: Possible predictors of the rate of calcific degeneration of bioprostheses include the degree of decompensated heart failure, the duration and invasiveness of surgery, and the characteristics of calcium–phosphorus homeostasis in

D. I. BLOKHINTSEV – SCIENTIST AND TEACHER. THE SPIRITUAL FOUNDATIONS OF SCIENTIFIC WORK

Directory of Open Access Journals (Sweden)

V. N. Pervushin

2016-01-01

Full Text Available The aim of the publication is to state the creative principles of activity of the outstanding scientist and teacher Dmitry Ivanovich Blokhintsev (1/10/1908 – 1/29/1979 – the organizer and the first director of the Joint Institute for Nuclear Researches in Dubna in 1956–1965, one of the pioneers of Nuclear Science and Atomics, the corresponding member of the Academy of Sciences of the USSR.The author of the article shares memories about the teacher and the research supervisor, and gives a peculiar report on realization of ideas of D. I. Blokhintsev. D. I. Blokhintsev had the special, original point of view on spiritual bases of scientific creativity that was directly reflected in his research and pedagogical activity.There are two fundamental aspects of pedagogics. On the one hand, it is the science possessing own specific laws and methods. On the other hand, the pedagogics is an art which methods, unlike scientific methodologies, can’t be acquired by formal and logical schemes. They are broadcast from one personality to another in direct communication. Thus possibly the «correspondence» assimilation of methods of outstanding teachers is inefficient as a rule. Not enough attention in the press is paid to this informal aspect of pedagogics in the view of difficulty of its description and analysis. The discussed D. I. Blokhintsev’s heritage is valuable from positions of the characteristic of pedagogics as arts of creative skill transfer. At first sight, it can seem paradoxical that this part of pedagogics is considered in connection with work in the field of the Quantum Field Theory and Cosmology – one of the most formalized fields of Theoretical Physics. However, the science, as well as pedagogics, considering it from top-level creativity, is becoming some kind of art too.One more important direction of work of D. I. Blokhintsev continued by the author of the publication in the book «Principles of the Quantum Universe» is

Limits on efficient computation in the physical world

Science.gov (United States)

Aaronson, Scott Joel

More than a speculative technology, quantum computing seems to challenge our most basic intuitions about how the physical world should behave. In this thesis I show that, while some intuitions from classical computer science must be jettisoned in the light of modern physics, many others emerge nearly unscathed; and I use powerful tools from computational complexity theory to help determine which are which. In the first part of the thesis, I attack the common belief that quantum computing resembles classical exponential parallelism, by showing that quantum computers would face serious limitations on a wider range of problems than was previously known. In particular, any quantum algorithm that solves the collision problem---that of deciding whether a sequence of n integers is one-to-one or two-to-one---must query the sequence O (n1/5) times. This resolves a question that was open for years; previously no lower bound better than constant was known. A corollary is that there is no "black-box" quantum algorithm to break cryptographic hash functions or solve the Graph Isomorphism problem in polynomial time. I also show that relative to an oracle, quantum computers could not solve NP-complete problems in polynomial time, even with the help of nonuniform "quantum advice states"; and that any quantum algorithm needs O (2n/4/n) queries to find a local minimum of a black-box function on the n-dimensional hypercube. Surprisingly, the latter result also leads to new classical lower bounds for the local search problem. Finally, I give new lower bounds on quantum one-way communication complexity, and on the quantum query complexity of total Boolean functions and recursive Fourier sampling. The second part of the thesis studies the relationship of the quantum computing model to physical reality. I first examine the arguments of Leonid Levin, Stephen Wolfram, and others who believe quantum computing to be fundamentally impossible. I find their arguments unconvincing without a "Sure

A Chandra Study of Supernova Remnants in the Large and Small Magellanic Clouds

Science.gov (United States)

Schenck, Andrew Corey

2017-08-01

distance from the SNR center than the previous estimate (˜6 pc). Based on our estimated larger size of the CD, we suggest that the significant effect from the presence of a Fe-Ni bubble at the SNR center (as proposed by the previous work) may not be required to describe the overall dynamics of this SNR. Applying the Sedov-Taylor similarity solutions, we estimate the dynamical age of ˜17,000 yr and an explosion energy of E0 ˜ 1:7 x 1051 erg for B0049-73.6. We place a stringent upper limit of LX ˜ 6:0 x 1032 erg s-1 on the 0.3-7.0 keV band luminosity for the embedded compact stellar remnant at the center of B0049-73.6. Our tight estimate for the X-ray luminosity upper limit suggests that the compact stellar remnant of this SNR may be a similar object to those in a peculiar class of low-luminosity neutron stars (e.g., the so-called Dim Isolated neutron stars) or may possibly be a black hole. Finally, we demonstrate our adaptive mesh grid method for the analysis of the rich SNR data. We developed our own computer software to implement this technique which is useful for an efficient spatially-resolved spectroscopic study of high-quality datasets of SNRs. As part of this software we also implement automated spectral model fits for all individual spectra extracted from our adaptively defined small sub- regions. We illustrate the utility of this technique with an example study of SNR N63A in the LMC.

NEW TYPE OF ELASTIC ROTATIONAL WAVES IN GEO-MEDIUM AND VORTEX GEODYNAMICS

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Alexander V. Vikulin

2010-01-01

Full Text Available Natural-science concepts of rotational movements and the ‘lumpy’ structure of medium are reviewed with a focus on key aspects. Through using torsional traps for hunting and «implementing» mechanical torque for ignition, Homo sapiens developed to man. Vortex movements «impregnated» in spiral structures of shells and torsional movements of toothy whales and fish were intuitively perceived by man as major stable movements of the environment. Based on the above, the ancient philosophy established the concept of the uniform world represented by atomic («noncuttable» structure of medium and vortex movements of ether. Based on conclusive arguments stated by R. Dekart, H. Helmgolz, Lord Kelvin and others within the framework of classical physics and in the first half of the 20th century by scientists in quantum physics and cosmogony, both «quantum structure» («lumpiness» and rotation («vorticity» are integral features of matter – space – time throughout the whole range from elementary particles to galaxies and galactic clusters.Nowadays researchers in natural sciences, particularly in the Earth sciences, call attention again to the problem of structure of matter and its movements. In the 1920s, Chinese geologist Li Siguang established fundamentals of vortex geodynamics. In the second half of the 20th century, Li Siguan’s concepts were developed by geologists O.I. Slenzak and I.V. Melekestsev. Geologist A.V. Peive, mechanic L.I. Sedov and physicist M.A. Sadovsky put forward a concept of block structure of the geo-medium (geological and geophysical medium and proposed a justified assumption that such blocks can move by own torque. This method of movement is confirmed by results of geological and tectonophysical studies, as well as instrumental geophysical measurements obtained from a variety of stations and focal zones of strong earthquakes. Many researchers, including W. Elsasser and V.N. Nikolaevsky, develop fundamentals of

Ethnic Motives in Russian Mass Consciousness

Directory of Open Access Journals (Sweden)

Natalija Pliskevič

2000-12-01

nation, which fuels nationalism. Yet Russian nationalism has not yet assumed a massive level, although the mass awareness of Russians is marked by a form of traditionalism, which manifests itself not so much in adherence to traditions, as in preventing the penetration of universal (foreign values. The author (N.P. further summarised some results on the level of anti-Semitism in Russia. In this regard she presents the conclusions of the American researcher, R. Brim, who found that after the 1998 devaluation of the ruble attitudes towards Jews were divided, but with a preponderance of the negative stance. Brim concluded that political factors and leaders had the most effect on the fate of Jews in Russia. At more stable times, as Gudkov claimed, the Russian attitude towards Jews was either positive or neutral, no different then the relationship to other ethnic groups and less negative than the attitudes of non-Russians, especially in the autonomous entities, to minorities (including Jews. All in all, one researcher (Zdravomyslov estimated that ethnic nationalism in Russian society effected no more than 10% of the population. The author (N.P. also summarises the results of some comparative analyses between Russia and other former Soviet republics. First, the image of the CIS as a threat to Russia has fallen in recent years and the great majority of Russians favour peaceful methods in regard to protecting the rights of Russian minorities in the former Soviet republics (Sedov. Comparative research in the Russia, the Baltic states and the Ukraine, shows that Russians and Estonians have similar attitudes to state paternalism and a similarly divided opinion on reforms and socialism (however state paternalism has more support in Russia and reforms are slightly more favoured in Estonian public opinion. As to social fears, comparative study of public opinion in Lithuania, Russia and the Ukraine showed that respondents in Lithuania felt relatively the least social fears, while those

The Biological Big Bang model for the major transitions in evolution

Directory of Open Access Journals (Sweden)

Koonin Eugene V

2007-08-01

-pattern cladogenesis. Reviewers This article was reviewed by William Martin, Sergei Maslov, and Leonid Mirny.

Methodological basis for formation of uniterruptible education content for future specialists of atomic-nuclear complex

International Nuclear Information System (INIS)

Burtebayev, N.; Burtebayeva, J.T.; Basharuly, R.; Altynsarin, Y.

2009-01-01

content for future specialists of atomic-nuclear complex at the particular science methodological level. It should be highlighted that the so called 'methods system' of teaching is the inseparable link of its subsequent backbone elements: aim, content, forms, methods and techniques of teaching. The creation of such methods system, consisting of above five elements assures the functional adequacy of specialists teaching, including nuclear profile personnel. Thereby, as the system methodological analysis shows, the determination of the content of uninterrupted education for nuclear profile specialists is only one of the tasks of united teaching methods system formation. Consequently, the development of other its backbone elements is the vital task of the training of atomic-nuclear complex specialists. These are the main approaches in general of theoretical-methodological provision of the training for future competitive capable specialists of nuclear profile in the national system of uninterrupted education in the Republic of Kazakhstan. Reference: 1. Basharuly R. Methodology of poly-cultural education development in Kazakhstan. Almaty: G ylym , 2002, p. 236.; 2. Sedov E.A. Again dialectics: truth and myths. // Pedagogic, 1993, No.3, pp.113-117.; 3. Lednev V.S. Education content. M.: High school. 1989, p.362. (authors)

7. Lasers and plasmas forum - ILP 2015 Forum. Book of abstracts

International Nuclear Information System (INIS)

Mora, P.; Le Marec, A.; Ferri, S.; Corde, S.; Ceccotti, T.; Dozieres, M.; Pariente, G.; Azamoum, Y.; Cheriaux, G.; Baccou, C.; Romagnani, L.; Ravasio, A.; Masson-Laborde, P.E.; Laffite, S.; Neuville, C.; Casner, A.; Debayle, A.; Lobet, M.; Cosse, P.; Falize, E.; Taieb, R.; Rozmus, W.; Colaitis, A.; Boutoux, G.; Llor Aisa, E.; Ducret, J.E.; Le Pennec, M.; Barbrel, B.; Rouan, D.; Smets, R.; Seisson, G.; Boyer, S.; Massacrier, G.; Harmand, M.; Jacquemot, S.; Adam, J.C.; Boutoux, G.; Busquet, M.; Bychenkov, V. Yu.; Castan, A.; Chatagnier, A.; Chiaramello, M.; Debayle, A.; Deschaud, Basil; Do, A.; Fedeli, L.; Ferri, J.; Gangolf, T.; Gilles, D.; Vallet, A.; D'Humieres, E.; Khiar, B.; Grassi, A.; Hadj-Bachir, M.; Lee, P.; Lobet, M.; Loiseau, P.; Maitrallain, A.; Masson-Laborde, P.E.; Mollica, F.; Moreau, J.G.; Nicolas, Loic; Pain, J.-C.; Penninckx, D.; Riconda, C.; Ruyer, C.; Soleilhac, A.; Van Box Som, L.

2015-06-01

List of oral presentation abstracts: Effect of XUV lasers partial coherence on the characterization of their spectral properties; Study of ionization potential lowering and other statistical properties of coupled plasmas using numerical simulation and classical molecular dynamics; Plasma acceleration by particle beam; Electron acceleration by surface wave resonant excitation in relativistic regime; Optimization of a laser-generated X Ka source (Ti:Sa 10 TW - 100 Hz); Apollon 10 PW: description and status; The future of the research federation and of power laser facilities; Inertial confinement fusion and operation of 'rugby'-shape hohlraums; Chronometry and efficiency of direct attack implosion at OMEGA facility; Laser-plasma interaction physics in beam crossing configuration; NIF Discovery Science experiments for the study of the strongly nonlinear regime of the ablative Rayleigh-Taylor instability; X opacity measurements in mid-Z dense plasmas with a new target design of indirect heating; Photoionization dynamics: Transition and scattering delays; Ion acceleration induced by laser-produced electrostatic shocks; Electron Transport and Related Non-equilibrium Distribution Functions in Hot Large Scale ICF Plasmas; Rate optimization of neutron-less fusion reactions initiated by laser-accelerated protons; Nonlinear laser-plasma interactions modeling at hydrodynamic scales: application to beam crossing energy exchange; Evolution of a Sedov-Taylor blast-wave: radiative, nonlocal heat transport and field effects; Measuring ultra-intense laser beams in space time; A few applications of the radiative and quantum electrodynamics effects in future extreme-intensity laser-matter experiments; X-rays imaging diagnostics for PETAL; Laboratory Astrophysics with High Power Lasers; Femto-second electron dynamics in the Warm dense Matter; The extra-solar planets; Study of HEDP magnetic reconnection; Opacity of solar-type stars inside: what (un)certainties?; Validation of solar

EDITORIAL: Focus on Carbon Nanotubes

Science.gov (United States)

2003-09-01

The study of carbon nanotubes, since their discovery by Iijima in 1991, has become a full research field with significant contributions from all areas of research in solid-state and molecular physics and also from chemistry. This Focus Issue in New Journal of Physics reflects this active research, and presents articles detailing significant advances in the production of carbon nanotubes, the study of their mechanical and vibrational properties, electronic properties and optical transitions, and electrical and transport properties. Fundamental research, both theoretical and experimental, represents part of this progress. The potential applications of nanotubes will rely on the progress made in understanding their fundamental physics and chemistry, as presented here. We believe this Focus Issue will be an excellent guide for both beginners and experts in the research field of carbon nanotubes. It has been a great pleasure to edit the many excellent contributions from Europe, Japan, and the US, as well from a number of other countries, and to witness the remarkable effort put into the manuscripts by the contributors. We thank all the authors and referees involved in the process. In particular, we would like to express our gratitude to Alexander Bradshaw, who invited us put together this Focus Issue, and to Tim Smith and the New Journal of Physics staff for their extremely efficient handling of the manuscripts. Focus on Carbon Nanotubes Contents Transport theory of carbon nanotube Y junctions R Egger, B Trauzettel, S Chen and F Siano The tubular conical helix of graphitic boron nitride F F Xu, Y Bando and D Golberg Formation pathways for single-wall carbon nanotube multiterminal junctions Inna Ponomareva, Leonid A Chernozatonskii, Antonis N Andriotis and Madhu Menon Synthesis and manipulation of carbon nanotubes J W Seo, E Couteau, P Umek, K Hernadi, P Marcoux, B Lukic, Cs Mikó, M Milas, R Gaál and L Forró Transitional behaviour in the transformation from active end

EDITORIAL: Message from the Editor Message from the Editor

Science.gov (United States)

Thomas, Paul

2012-01-01

Board Members, Guest Editors of special editions and those referees who were already listed in the last years. The following people have been selected: Marina Becoulet, CEA Cadarache, France Russell Doerner, University of California - San Diego, USA Emiliano Fable, Max-Planck-Institut fuer Plasmaphysik, Germany Akihide Fujisawa, Kyushi University, Japan Gerardo Giruzzi, CEA Cadarache, France Grigory Kagan, LANL, USA Morten Lennholm, CCFE, UK Akinobu Matsuyama, NIFS, Japan Peter Stangeby, University of Toronto, Canada Leonid Zakharov, PPPL, USA In addition, there is a group of several hundred referees who have helped us in the past year to maintain the high scientific standard of Nuclear Fusion. At the end of this issue we give the full list of all referees for 2011. Our thanks to them! Authors The winner of the 2011 Nuclear Fusion Award is H. Urano, for the paper 'Dimensionless parameter dependence of H-mode pedestal width using hydrogen and deuterium plasmas in JT-60U' (Nucl. Fusion 48 045008). The award was presented at the Plasma Conference 2011 (Joint meeting of 28th JSPF Annual Meeting, The 29th Symposium on Plasma Processing, and Division of Plasma Physics, 2011 Autumn Meeting of The Physical Society of Japan). This is the sixth year that the International Atomic Energy Agency (IAEA) has awarded an annual prize to honour exceptional work published in Nuclear Fusion. IOP Publishing has generously made a contribution of $2500 to the award. The Nuclear Fusion Electronic Archive The journal's electronic archive has been online since the beginning of the year. The archive has been a roaring success and has contributed to the nearly 300 000 downloads of journal papers in 2011. The archive can be accessed via http://iopscience.iop.org/0029-5515/page/Archive. It has direct links to 16 landmark papers, from authors such as Artsimovich and Mercier. The Nuclear Fusion office and IOP Publishing Just as the journal depends on the authors and referees, so its success is also

ІСТОРІЯ КАФЕДРИ МЕДИЦИНИ КАТАСТРОФ ТА ВІЙСЬКОВОЇ МЕДИЦИНИ БУКОВИНСЬКОГО ДЕРЖАВНОГО МЕДИЧНОГО УНІВЕРСИТЕТУ / THE HISTORY OF THE DEPARTMENT OF DISASTER AND MILITARY MEDICINE OF BUKOVINIAN STATE MEDICAL UNIVERSITY

Directory of Open Access Journals (Sweden)

Бірюк Ігор

2017-06-01

Full Text Available Бирюк Игорь, Цыркот Ігорь, Куковськая Ирина, Стефанчук Василий, Мойсюк Владимир, Стефак Ярослав, Юрчук Леонид История кафедры медицины катастроф и военной медицины Буковинского государственного медицинского университета. Резюме. Отражена история кафедры медицины катастроф и военной медицины Высшего государственного учебного заведения Украины "Буковинский государственный медицинский университет". Раскрыты основные этапы становления и направления деятельности кафедры, а также указано весь руководящий состав за период с 1944 по 2017 годы. Ключевые слова: кафедра, история, создание, медицина катастроф, военная медицина Biryuk Igor, Tsyrkot Igor, Kukovska Iryna, Stefanchuk Vasil, Moysyuk Vladimir, Stefak Jaroslav, Yurchuk Leonid The history of the department of disaster and military medicine of Bukovinian state medical university Abstract. The article is devoted to the history of the Department of Disaster Medicine and Military Medicine of the Supreme State educational institution of Ukraine "Bukovinіan State Medical University." Characterizing the main stages of the formation of the department, the direction of its activities from the period of creation of the Chernivtsi State Medical Institute (our time "Bukovinian State Medical University" our days. Set management team of the department for the entire period of its operation from 1944 to 2017 It is shown that the organization of educational process of military training of students

PREFACE: Semiconducting oxides Semiconducting oxides

Science.gov (United States)

Catlow, Richard; Walsh, Aron

2011-08-01

their help in producing this special section. We hope that it conveys some of the excitement and significance of the field. Semiconducting oxides contents Chemical bonding in copper-based transparent conducting oxides: CuMO2 (M = In, Ga, Sc) K G Godinho, B J Morgan, J P Allen, D O Scanlon and G W Watson Electrical properties of (Ba, Sr)TiO3 thin films with Pt and ITO electrodes: dielectric and rectifying behaviourShunyi Li, Cosmina Ghinea, Thorsten J M Bayer, Markus Motzko, Robert Schafranek and Andreas Klein Orientation dependent ionization potential of In2O3: a natural source for inhomogeneous barrier formation at electrode interfaces in organic electronicsMareike V Hohmann, Péter Ágoston, André Wachau, Thorsten J M Bayer, Joachim Brötz, Karsten Albe and Andreas Klein Cathodoluminescence studies of electron irradiation effects in n-type ZnOCasey Schwarz, Yuqing Lin, Max Shathkin, Elena Flitsiyan and Leonid Chernyak Resonant Raman scattering in ZnO:Mn and ZnO:Mn:Al thin films grown by RF sputteringM F Cerqueira, M I Vasilevskiy, F Oliveira, A G Rolo, T Viseu, J Ayres de Campos, E Alves and R Correia Structure and electrical properties of nanoparticulate tungsten oxide prepared by microwave plasma synthesisM Sagmeister, M Postl, U Brossmann, E J W List, A Klug, I Letofsky-Papst, D V Szabó and R Würschum Charge compensation in trivalent cation doped bulk rutile TiO2Anna Iwaszuk and Michael Nolan Deep level transient spectroscopy studies of n-type ZnO single crystals grown by different techniquesL Scheffler, Vl Kolkovsky, E V Lavrov and J Weber Microstructural and conductivity changes induced by annealing of ZnO:B thin films deposited by chemical vapour depositionC David, T Girardeau, F Paumier, D Eyidi, B Lacroix, N Papathanasiou, B P Tinkham, P Guérin and M Marteau Multi-component transparent conducting oxides: progress in materials modellingAron Walsh, Juarez L F Da Silva and Su-Huai Wei Thickness dependence of the strain, band gap and transport properties of

Meteorites, Bolides and Comets: A Tale of Inconsistency

Science.gov (United States)

Jakes, P.; Padevet, V.

1992-07-01

Inhomogeneity of cometary nuclei has been established through the observed disruptions of comets [1] and through the determination of dust particle composition during the encounter of the Vega and Giotto satellites with comet Halley [2,3,4]. The raisin bread model of cometary nuclei [5,6] assumes the presence of solid (rock) and dust particle material set in the volatile rich, ice- cemented material. Rock material may contribute to the formation of dust particles. Gombosi and Houpis [5] argued that only the composition of dust particles derived from the icy, volatile component of the comet were analyzed and implied thus that the third cometary component present (raisins/rocks) has not been examined. The compositions of the cometary (Halley) dust and the interplanetary dust particles (IDPs) are "chondritic" (Blanford et al., 1988). It is difficult, therefore to estimate the proportion of cometary to asteroid-derived dust in near Earth space, e.g., among the IDPs [7] unless other criteria are available. Bolide multistation photographic tracking allows the determination of the orbital preencounter parameters of solid bodies (0.01-100,000 kg in mass) with the Earth, and allows us to classify them according to their ablation coefficient (tau), penetration depth into the atmosphere (PE), theoretical densities (sigma), and terminal velocities (V(sub)E). Four groups are recognized (Table 1). Three of the type I bolides were recovered as ordinary chondrites (Pribram, Lost City, and Innisfree). Ceplecha [8] has shown that 38% of bolides (fireballs) come from cometary orbits (11% from highly eccentric orbits typical of new comets), but most of the bolides (62%) originate at asteroidal orbits. Seven of the 14 known meteoric showers could be attributed to known comets: N,S Taurids to 1970 P/Encke, Lyrids to 1861 I Thatcher-Beaker, Perseids to 1862 III Swift-Tuttle- Simons, Orionids to 1835 III P/Halley, Draconids to 1946 V P/Giacobini-Zinner, Leonids to 1966 I Tempel

Editorial: Focus on Atom Optics and its Applications

Science.gov (United States)

Schmidt-Kaler, F.; Pfau, T.; Schmelcher, P.; Schleich, W.

2010-06-01

Couvert, B Georgeot and D Guéry-Odelin Analysis of the entanglement between two individual atoms using global Raman rotations A Gaëtan, C Evellin, J Wolters, P Grangier, T Wilk and A Browaeys Spin polarization transfer in ground and metastable helium atom collisions D Vrinceanu and H R Sadeghpour A fiber Fabry-Perot cavity with high finesse D Hunger, T Steinmetz, Y Colombe, C Deutsch, T W Hänsch and J Reichel Atomic wave packets in amplitude-modulated vertical optical lattices A Alberti, G Ferrari, V V Ivanov, M L Chiofalo and G M Tino Atom interferometry with trapped Bose-Einstein condensates: impact of atom-atom interactions Julian Grond, Ulrich Hohenester, Igor Mazets and Jörg Schmiedmayer Storage of protonated water clusters in a biplanar multipole rf trap C Greve, M Kröner, S Trippel, P Woias, R Wester and M Weidemüller Single-atom detection on a chip: from realization to application A Stibor, H Bender, S Kühnhold, J Fortágh, C Zimmermann and A Günther Ultracold atoms as a target: absolute scattering cross-section measurements P Würtz, T Gericke, A Vogler and H Ott Entanglement-assisted atomic clock beyond the projection noise limit Anne Louchet-Chauvet, Jürgen Appel, Jelmer J Renema, Daniel Oblak, Niels Kjaergaard and Eugene S Polzik Towards the realization of atom trap trace analysis for 39Ar J Welte, F Ritterbusch, I Steinke, M Henrich, W Aeschbach-Hertig and M K Oberthaler Resonant superfluidity in an optical lattice I Titvinidze, M Snoek and W Hofstetter Interference of interacting matter waves Mattias Gustavsson, Elmar Haller, Manfred J Mark, Johann G Danzl, Russell Hart, Andrew J Daley and Hanns-Christoph Nägerl Magnetic trapping of NH molecules with 20 s lifetimes E Tsikata, W C Campbell, M T Hummon, H-I Lu and J M Doyle Imprinting patterns of neutral atoms in an optical lattice using magnetic resonance techniques Michal Karski, Leonid Förster, Jai-Min Choi, Andreas Steffen, Noomen Belmechri, Wolfgang Alt, Dieter Meschede and Artur Widera

Obituary: Thomas C. Van Flandern (1940-2009)

Science.gov (United States)

Dunham, David; Slabinski, Victor

2011-12-01

planetary formation. The Bulletin claimed mainstream scientists preferred making ad hoc corrections to the theories rather than acknowledge fundamental difficulties that might jeopardize their funding. Tom Van Flandern's advocacy of an artificial origin for the "face on Mars," especially after higher-resolution images were taken in 2001, antagonized many. His questioning of the speed of gravity, first published in a 1998 paper in Physics Letters A, provoked additional attacks from relativists. He showed the same persistence with these controversies that had enabled him to solve complex programming and celestial mechanics problems. Tom Van Flandern did not reject General Relativity as some have asserted, but rather rejected its geometrical interpretation. He said: "General relativity has a geometric and a field interpretation. If angular momentum conservation is invoked in the geometric interpretation to explain experiments, the causality principle is violated. The field interpretation avoids this problem by allowing faster-than-light propagation in forward time." For more, see http://www.metaresearch.org/cosmology/gravity/speed_limit.asp. Tom Van Flandern strongly attacked some alternative theories, such as Velikovsky's ideas of recent planetary close approaches, turning one of Velikovsky's supporters, C. L. Ellenberger, into a strong critic. If not for these antagonisms, the "mainstream" part of Tom Van Flandern's work in later years might be better acknowledged, including his "Eclipse Edge" company that organized expeditions to several solar eclipses, and his work with E. Lyytinen on the passage of Earth through cometary debris trails. Their prediction was closest to the observed time of the Leonid storm maximum of November 2001. Tom Van Flandern held memberships in the International Astronomical Union, the American Astronomical Society (and in its Divisions on Dynamical Astronomy and Planetary Sciences), and several other scientific organizations. He received second

EDITORIAL: From reciprocal space to real space in surface science From reciprocal space to real space in surface science

Science.gov (United States)

Bartels, Ludwig; Ernst, Karl-Heinz

2012-09-01

Triest.let's finish—aus basta Some move atoms around to hear how they sound.Karl-Heinz Rieder, Erice, 6 April 1998 From reciprocal space to real space in surface science contents From reciprocal space to real space in surface scienceLudwig Bartels and Karl-Heinz Ernst Karl-Heinz Reider: the quiet pioneerGiorgio Benedek Scattering of CO and N2 molecules by a graphite surfaceJunepyo Oh, Takahiro Kondo, Keitaro Arakawa, Yoshihiko Saito, Junji Nakamura, W W Hayes and J R Manson Helium, neon and argon diffraction from Ru(0001)M Minniti, C Díaz, J L Fernández Cuñado, A Politano, D Maccariello, F Martín, D Farías and R Miranda Enhanced charge transfer in a monolayer of the organic charge transfer complex TTF-TNAP on Au(111)T R Umbach, I Fernandez-Torrente, J N Ladenthin, J I Pascual and K J Franke Extended pattern recognition scheme for self-learning kinetic Monte Carlo simulationsSyed Islamuddin Shah, Giridhar Nandipati, Abdelkader Kara and Talat S Rahman Acetylene on Cu(111): imaging a molecular surface arrangement with a constantly rearranging tipYeming Zhu, Jonathan Wyrick, Kamelia D Cohen, Katie Marie Magnone, Connor Holzke, Daniel Salib, Quan Ma, Dezheng Sun and Ludwig Bartels Coulomb attraction during the carpet growth mode of NaClFriederike Matthaei, Sarah Heidorn, Konrad Boom, Cord Bertram, Ali Safiei, Jörg Henzl and Karina Morgenstern Molecular self-assembly on an insulating surface: interplay between substrate templating and intermolecular interactionsMarkus Kittelmann, Philipp Rahe and Angelika Kühnle Vertical manipulation of native adatoms on the InAs(111)A surfaceJ Yang, C Nacci, J Martínez-Blanco, K Kanisawa and S Fölsch Charge transfer between isomer domains on n+-doped Si(111)-2 × 1: energetic stabilizationR M Feenstra, G Bussetti, B Bonanni, A Violante, C Goletti, P Chiaradia, M G Betti and C Mariani Probing the properties of metal-oxide interfaces: silica films on Mo and Ru supportsLeonid Lichtenstein, Markus Heyde, Stefan Ulrich, Niklas Nilius

International Conference on Gravitation Cosmology and Continuum Mechanics (dedicated to the centenary of Kirill Petrovich Staniukovich)

International Nuclear Information System (INIS)

2016-01-01

International Conference - Gravitation, Cosmology and Mechanics of Continuous Environments (devoted to the 100th anniversary K.P. Stanyukovich's birth) was held in Bauman Moscow State Technical University on the 3th and 4th of March. More than 100 papers were presented by K.P. Stanyukovich's students, faculty, various universities staff and representatives of the Russian Academy of Sciences. Kirill Petrovich Stanyukovich (3 March, 1916 - 4 June, 1989) - an outstanding physicist, mathematician and engineer made a significant contribution to the development of various fields of science: gas dynamics, physics of explosion, magnetic hydrodynamics, astronomy. He developed a hydrodynamic model of gravity, the theory of gravity with a variation of the effective gravitational constant, with a variable number of particles, he offered one of the first Universe evolution scenarios from the initial vacuum stage. Kirill Petrovich was the author of a number of inventions and of 330 scientific and popular-science works. He came from an old noble family - the Stanyukovich. (The famous writer and marine painter Konstantin Stanyukovich was his granduncle). Not yet having finished school, K.P. Stanyukovich got seriously interested in astronomy and became a member of the observers’ team of the Moscow Society of Astronomy Fanciers (MSAF) where he met Leonid Alekseevich Kulik, the famous Tunguska meteorite investigator and one of the national meteoritics founders. In 1932 the first K.P. Stanyukovich's research article on meteor astronomy (in co-authorship with I.E. Vasilyev) “Lyrids in 1930” was published in the 'Bulletin of MSAF Observers. In 1931 K.P. Stanyukovich took part in the MSAF meteors observation expedition on the Karadag scientific station in the Crimea, and in 1932 proposed a new method for estimating the meteor extinction height, based on an empirical relationship between meteor brightness and path length. In the same year he was involved in the processing of bright

Последнее крымское нашествие на Москву в изображении русских публицистов конца XVI — первой трети XVII веков / The last Crimean invasion of Moscow in the works by Russian essayists of the late XVI — first third of the XVII centuries

Directory of Open Access Journals (Sweden)

Ya. G. Solodkin

2016-12-01

�остойным наследником. Иван Тимофеев же, писавший по собственным воспоминаниям спустя два десятилетия, если не позднее, о быстром бегстве татар из окрестностей «царствующего града», представил Годунова (в том числе под впечатлением Серпуховского похода 1598 г. «лжехрабрым» военачальником, а главную роль в разгроме хана отвел мольбам подобного святым самодержца, в конце жизни которого с Крымом установились мирные отношения. / The Crimean Tatar invasion of Moscow in the summer of 1591 was the last in the long history of bilateral relations, and it is reflected along with chronicle writings in the Russian journalism on the eve of the Time of Troubles and the 1620s. Mention (not very accurate about the failed attempt by Gazi Giray II to master the Russian capital, rising to some brief chronicler, available in the second edition of the Chronograph. The Tale of Tsar Fyodor Ivanovich, written by the patriarch Iov, and Annals clerk Ivan Timofeev we encounter lengthy stories devoted to battles near Moscow, between the Tatars and the army, which was the de facto commander of Boris Godunov. Using chronicle source (probably the one that V. N. Tatischev called “History of the Destruction of Russia”, Iov tendentiously portrayed ruler Boris as an outstanding military leader and stressed the importance of prayers for the intercession addressed to God and the Virgin Mary by “saint” Tsar Fedor. By the way, the victory won over the Crimeans at the walls of Moscow, under the pen of “humility” of the patriarch did childless brother in law of the sovereign of his worthy successor. Ivan Timofeev also, writing on his own memoirs after two decades

Granitoid magmatism of Alarmaut granite-metamorphic dome, West Chukotka, NE Russia

Science.gov (United States)

Luchitskaya, M. V.; Sokolov, S. D.; Bondarenko, G. E.; Katkov, S. M.

2009-04-01

-metamorphic domes at Russian North-East. Paper 2. Magmatism, metamorphism and migmatization in Late Mesozoic domes // Pacific geology. 1996. V. 15. № 1. P. 84-93. (in Russian) 13. Bering Strait Geologic Field Party, Koolen metamorphic complex, NE Russia: implications for the tectonic evolution of the Bering Strait region // Tectonics, vol. 16, no. 5, p. 713-729 14. Bondarenko G.E., Luchitskaya M.V. Mesozoic tectonic evolution of Alarmaut rise // Byul. MOIP. Otd. Geol. V. 78. Is. 3. P. 25-38. (in Russian) 15. Katkov S.M., Strikland A., Miller E.L. Age of granite batholiths in the Anyui-Chukotka Foldbelt // Doklady. Earth Sciences. 2007. Vol. 414. № 4. P. 515-518. 16. Amato J.M., Wright J.E. Potassic mafic magtism in the Kigluaik gneiss dome, northern Alaska: a geochemical study of arc magmatism in an extensional tectonic setting // J. Geophys. Res. 1997. Vol.102. N B4. P.8065-8084 17. Tikhomirov P.L., Luchitskaya M.V., Kravchenko-Berezhnoy I.R. Comparison of Cretaceous granitoids of the Chaun tectonic zone to those of the Taigonos Peninsula, NE Asia: rock chemistry, composition of rock forming minerals, and conditions of formation // Stephan Mueller series. Geology and Tectonic Origins of Northeast Russia: A Tribute to Leonid Parfenov (in press) 28. Velikoslavinsky S.D. Geochemical typification of acid magmatic rocks of leading geodynamic settings // Petrology. 2003. V. 11. № 4. P.363-380. (in Russian) 19. Pearce J.A. Sources and settings of granitic rocks // Episodes. 1996. V. 19. N. 4. P. 120-125

PREFACE: 13th International Conference on Liquid and Amorphous Metals

Science.gov (United States)

Popel, Pjotr; Gelchinskii, Boris; Sidorov, Valeriy; Son, Leonid; Sabirzjanov, Alexandre

2007-06-01

Dupuy, M Silbert, F Sommer, W C Pilgrim, W Freyland, K Lu, J Brmejo and F Hensel. We dedicate the LAM13 conference to the 80-year jubilee of Professor Nikolay Vatolin who is the leader of Russian investigations in the field of liquid and amorphous metals and who managed twelve(!) similar conferences in our country. One of us (PP) commemorates his father, Professor Stanislav Popel, who was a known specialist in high temperature capillarity and left us half a year before the event. Pjotr Popel, Boris Gelchinskii, Valeriy Sidorov, Leonid Son, Alexandre Sabirzjanov Ekaterinburg, January 14 2008

Catching a Falling Star

Science.gov (United States)

2004-07-01

. Comets are another important source of meteoroids and perhaps the most spectacular. After many visits near the Sun, a comet "dirty-snowball" nucleus of ice and dust decays and fragments, leaving a trail of meteoroids along its orbit. Some "meteoroid streams" cross the earth's orbit and when our planet passes through them, some of these particles will enter the atmosphere. The outcome is a meteor shower - the most famous being the "Perseids" in the month of August [2] and the "Leonids" in November. Thus, although meteors are referred to as "shooting" or "falling stars" in many languages, they are of a very different nature. More information The research presented in this paper is published in the journal Meteoritics and Planetary Science, Vol. 39, Nr. 4, p. 1, 2004 ("Spectroscopic anatomy of a meteor trail cross section with the ESO Very Large Telescope", by P. Jenniskens et al.). Notes [1] The team is composed of Peter Jenniskens (SETI Institute, USA), Emmanuël Jehin (ESO), Remi Cabanac (Pontificia Universidad Catolica de Chile), Christophe Laux (Ecole Centrale de Paris, France), and Iain Boyd (University of Michigan, USA). [2] The maximum of the Perseids is expected on August 12 after sunset and should be easily seen.