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21. Galaxy sector, archive 1994
... 1994: . Deep CCD images of the bright gamma-ray bursts GRB790418 and GRB790613 localization regions were obtained for the first time. In both cases, a faint blue star-like object (V = 24.5 m , BV m ) was detected within the region of localization of gamma-ray bursts. ... Based on sixty daily instantaneous spectra of the object SS433, obtained on the RATAN-600 in April-May 1994, we traced its variability in four very powerful flares at five frequencies. ... Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res1994.html -- 6.6 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_galaxy/res1994.html -- 6.6 Кб -- 10.04.2016
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22. PS_obj.html
... Shematovich, V.I . ... Shematovich, V. I. ; Bisikalo, D. V.; Marov , M. Ya . ... Shematovich, V.I., Bisikalo, D.V., and Gerard J.-C. Superthermal particles in the planetary atmosphere. ... Shematovich, V.I., Bisikalo, D.V., and Gerard, J.-C. The thermospheric odd nitrogen photochemistry : role of non-thermal N(4S) atoms (abstract) . ... Geophys ., ... Gerard, J.C., Shematovich, V.I., and Bisikalo, D.V. Effect of hot N( 4S) atoms on the NO solar cycle variation in the lower thermosphere (abstract) . ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~shematov/HotAtoms.html -- 71.4 Кб -- 06.04.2010
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23. Internal Structure of Stars
... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/vnutr_bud_zir_e.html -- 6.6 Кб -- 23.02.2005
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24. ASP: What Have We Learned About Halley's Comet?
... What Have We Learned About Halley's Comet? ... Until the Russian VEGA and the European Giotto spacecraft flew by Halley's core, people had never really seen the heart of a comet! ... showed that the comet's nucleus was about 15 kilometers long and 8 kilometers wide. ... The Giotto spacecraft came within 600 km of the comet's nucleus, surviving the great gas and dust storms of the inner coma. ... Comet Halley's dark icy nucleus (center) and bright "jets'' of gas and dust as photographed by "Giotto''....
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/06/06.html -- 16.6 Кб -- 02.10.2012
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25. http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf
Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...
[ Текст ]  Ссылки http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf -- 1659.8 Кб -- 24.09.2008
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26. Eddington's Temperature of Space
... In the first page of this chapter, Eddington computes an effective temperature of 3.18 K, but this has nothing to do with the 2.725 K blackbody spectrum of the Cosmic Microwave Background (CMB) . Here is a quote of what Eddington actually said: . ... We shall first calculate the energy density of this radiation. ... It is clear that Eddington's model fits the optical data, but that Eddington did not anticipate either the CMB (red curve) or the interstellar dust (ISD, green curve). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~satr/cosmo/Eddington-T0.html -- 7.3 Кб -- 16.10.2000
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27. Seminars
The seminar is supported by the grant of Federal Programm "Integration" . annotation of talk . Karnaukhov A.V. (ICB RAS) . Greenhouse catastrophe. ... An analysis of a casual-consecutive model of processes determining the greenhouse catastrophe development is presented. The whole geobiophysical system is considered, which includes atmosphere, hydrosphere, litosphere, biosphere, and noosphere. ... Some possible measures to low the rate of the greenhouse catastrophe are considered. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/sciwork/archive/64/eannot1.html -- 2.0 Кб -- 16.06.2000
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28. ESO Top 10 Astronomical Discoveries | ESO
... Video News Releases . ... Press Releases . ... ESO Top 10 Astronomical Discoveries . ... Here is our list of ESO€‡s Top 10 astronomical discoveries so far. ... Read more in the ESO Press Release eso0226 , eso0846 , eso1151 , eso1332 and eso1512 . ... Read more in the ESO Press Release eso0425 and in the ESO Press Release eso0106 . ... Read more in the ESO Press Release eso1047 and in the ESO Press Release eso1002 . ... Read more in the ESO Press Release eso0318 and in the ESO Press Release eso0533 ....
[ Сохраненная копия ]  Ссылки http://www.eso.org/public/science/top10/ -- 101.5 Кб -- 10.04.2016
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29. The basic stages in the Earth's pre-geological development
... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...
[ Сохраненная копия ]  Ссылки http://www.lermus.ru/users/trunaev/part2.htm -- 22.6 Кб -- 04.12.2001
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30. Atmospheric influence on the different radioengineering systems functioning.
Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/atm/correction.html -- 19.8 Кб -- 18.10.2011
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31. http://astro.uni-altai.ru/AFgalleries.html
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/AFgalleries.html -- 1.1 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://astroclub.ru/ -- 1.2 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://astronomy.tomsk.ru/google.php -- 1.3 Кб -- 01.10.2012
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32. WORKSHOP "STELLAR ATMOSPHERES" "THE CHEMICAL AND DYNAMIC EVOLUTION OF STARS AND
... WORKSHOP "STELLAR ATMOSPHERES" . THE CHEMICAL AND DYNAMIC EVOLUTION OF STARS AND GALAXIES" . ... Chernomorka , Odessa , Ukraine . ... Modeling and interpretation of the stellar spectra of the usual and peculiar stars. Elemental abundances in the stars of different types and populations of the Galaxy. Chemical evolution of the stars and galaxies. ... Andrievsky S.M. (OAO ONU, Odessa, Ukraine) . ... CHEMICAL and DYNAMIC EVOLUTION STARS and GALAXIES" . ... Odessa mailto:astro@paco.odessa.ua . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/EAAS/rus/doc/25_08_08.htm -- 19.1 Кб -- 06.11.2007
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33. http://www.izmiran.rssi.ru/~obridko/papers/31.pdf
ON THE ENERGY DISSIPATION RELEASE IN THE BY MAGNETIC FIELD SOLAR ATMOSPHERE M. KOPECKY and V. OBRIDKO* Astronomical Institute of the Czechoslovak Academy of Sciences, Ond(ejov (Received 18 April, 1968) Abstract. ... 1) The calculations of the conductivity for the case of fully ionized gas gave very great values for all layers in the solar atmosphere. ... 2) What is the value of the energy released by magnetic-field dissipation, and how large is the heating of atmospheric layers by this process? ...
[ Текст ]  Ссылки http://www.izmiran.rssi.ru/~obridko/papers/31.pdf -- 245.5 Кб -- 22.03.2011
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34. Stellarium: Atmosphere Class Reference
Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Atmosphere Class Reference . ... More... #include < Atmosphere.hpp > . voidљ . computeColor (double JD, Vec3d _sunPos, Vec3d moonPos, float moonPhase, StelCore *core, float eclipseFac, float latitude=45.f, float altitude=200.f, float temperature=15.f, float relativeHumidity=40.f) . ... Get fade in/out duration in seconds. ... getFlagShow () const . ... getFadeIntensity (void) const . ... Definition at line 40 of file Atmosphere.hpp . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classAtmosphere.html -- 21.2 Кб -- 28.02.2014
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35. http://www.aaa.org/s932/images/09fallclass3.pdf
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System Characteristics Formation Exosolar Planets Class 3 Stars The S un Stellar Evolution of Low and High Mass Stars Deaths of Stars Exotic Stars Class 4 Galaxies Galaxy Classification Formation of Galaxies Galactic ... Low mass stars live and die differently than high mass stars. ...
[ Текст ]  Ссылки http://www.aaa.org/s932/images/09fallclass3.pdf -- 1260.6 Кб -- 07.09.2011
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36. http://master.sai.msu.ru/media/presentations/2014/20140208_Shibata.pdf
... 8 February , 2014 SAI seminar (Ryde et al 2010) 5 Thermal emission from GRB jet progenitor observer photon jet Photosphere (=1) · · · · Photons are not produced at the photosphere We have to calculate radiative transfer We need to know where the photons are produced We construct the expression for effective optical depth in relativistic flow considering random walk process in relativistic flow SAI seminar 6 8 ... 8 February, 2014 SAI seminar 28 ...
[ Текст ]  Ссылки http://master.sai.msu.ru/media/presentations/2014/20140208_Shibata.pdf -- 1131.7 Кб -- 07.02.2014
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37. http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,391.pdf
... Numerical Modeling of RadioAstron SRT Temperature Deformations M. Yu. Arkhipov, I. S. Vinogradov, S. B. Novikov, and S. D. Fedorchuk Astro Space Center, Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia e mail: rusengineer@mail.ru Received December 16, 2013 Abstract--The results of modeling the thermal deformations of a space radio telescope's reflecting surface are presented in the paper. ...
[ Текст ]  Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,391.pdf -- 437.2 Кб -- 07.10.2014
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38. http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Kuznetsov/JASR2006-S-06-01000.pdf
Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...
[ Текст ]  Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Kuznetsov/JASR2006-S-06-01000.pdf -- 253.7 Кб -- 15.04.2011
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39. Astronaut Bio: Leland D. Melvin (3/2014)
National Aeronautics and Space Administration . ... Leland D. Melvin . ... NASA EXPERIENCE: б  Selected by NASA JSC in June 1998, Mr. Melvin reported for training in August 1998.б  Astronaut Candidate Training included orientation briefings and tours, numerous scientific and technical briefings, intensive instruction in Shuttle and International Space Station systems, physiological training and ground school to prepare for T-38 flight training, as well as learning water and wilderness ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/Bios/htmlbios/melvin.html -- 8.6 Кб -- 07.07.2015
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40. Hydrogenated amorphous carbon
... Amorphous carbonaceous materials can show a great diversity of optical properties due to the variability in their microstructure. ... The differently pyrolized celluloses are representative for a suit of carbonaceous material ranging from strongly disordered (insulating) to graphitized (conducting) material. Figure: Complex refractive index of hydrogenated amorphous carbon prepared by pyrolysis (annealing) of cellulose at different temperatures. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/5-OPTC/JPDOC2/node10.html -- 8.0 Кб -- 19.11.2010
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