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http://www.cplire.ru/html/lab234/Tarasov/reprints/sust4_5_062.pdf.
http://www.cplire.ru/html/lab234/Tarasov/reprints/sust4_5_062.pdf.
21. CHIANTI atomic database
The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... For consistency with Griffin et al 2000, who adapted their atomic structure calculation to a set of observed energies identical to the NIST one, we use the NIST v.2 level ordering. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E.Landi - Nov 2004 . ...
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Ссылки http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/fe/fe_8.html -- 6.2 Кб -- 15.09.2005
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22. Special Year in Multiscale Mathematical Modeling in Biology and Medicine
The multiscale analysis of heterogeneous structures is actually an important and effective tool of mathematical modeling in physics, technique and biology. ... The special year will extend the existing cooperation between French and Russian researchers in the multiscale analysis and in mathematical modeling in hemodynamics, taking into consideration the mass transport, coagulation, fluid-structure interaction and other aspects. ...
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Ссылки http://www.mccme.ru/lifr/medicine.htm -- 3.1 Кб -- 10.09.2014
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23. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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24. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . ... History of flights . ... Investigation of impact of space factors on the state of the "microorganisms - substrates" system as applied to the problem of ecological safety of space technology and planetary quarantine. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
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Ссылки http://www.energia.ru/en/iss/researches/biology/all.html -- 29.2 Кб -- 10.04.2016
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25. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...
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Ссылки http://rp.iszf.irk.ru/esceir/isr/ismodelen.htm -- 5.9 Кб -- 04.06.2001
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26. astro-ph
... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...
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Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=Jr -- 12.6 Кб -- 06.02.2013
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27. New data on the cpmplex field structure of chemically peculiar stars
... As a result of BTA observations of 23 chemically peculiar stars with strong magnetic fields, it was found that in 22 of them the longitudinal magnetic field, measured from the hydrogen line cores are considerably lower (by about 1/3) than the value measured from metal lines in the same spectra. ... New approaches need to be developed in order to interpret the data. ... The Zeeman spectrum of a star with a strong magnetic field, 53 Cam. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Roman/ -- 5.4 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Roman/ -- 5.4 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Roman/ -- 5.4 Кб -- 02.10.2012
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28. cat5
. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.
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Ссылки http://www.wdcb.ru/stp/cat5MOD.html -- 2.2 Кб -- 18.01.2010
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29. http://www.mso.anu.edu.au/~raquel/Salmeron_Madrid.pdf
... Because of the low conductivity, the magnetic coupling is weak and depends critically on density, temperature, ionisation rate and charged species. ... Implications When the Hall regime dominates near the midplane and ambipolar diffusion is dominant closer to the surface, a thicker layer of the disc is unstable to MRI perturbations and modes grow faster than under the ambipolar diffusion approximation. ... Right panel: For weak coupling, Hall limit perturbations grow until vA/cs ~ 2.9. ...
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Ссылки http://www.mso.anu.edu.au/~raquel/Salmeron_Madrid.pdf -- 466.0 Кб -- 21.11.2006
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30. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
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Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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31. Theoretical Astrophysics Department
. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:
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Ссылки http://www.asc.rssi.ru/mdiv/tad/tad.htm -- 1.8 Кб -- 04.12.1997
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32. APOD: March 9, 1997 - COBE Hotspots:The Oldest Structures Known
... March 9, 1997 . COBE Hotspots: The Oldest Structures Known . Credit: DMR , COBE , NASA , Four-Year Sky Map . ... These spots are the oldest, most distant structures known. ... By studying the size and distribution of the spots found with COBE and future missions , astronomers hope to learn what matter and processes caused the spots to form - and hence determine the composition , density, and future of our Universe. ... About APOD > . ...
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Ссылки http://www.sai.msu.su/apod/ap970309.html -- 4.9 Кб -- 02.10.2012
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33. http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_125.pdf
MODERN APPROACHES TO CALCULATION OF THE PROPERTIES OF MATERIALS FOR ENERGY STORAGE A. Kabanov Samara State University The modern technologies demands to compact and effective rechargeable systems of energy storage. ... In this work we investigated the activation energies of one promising compound Li2CoPO4F using combination of two methods ab-initio and geometrical calculations. ... The nudged elastic band (NEB) method is adopted to find the kinetic energy barrier along diffusion pathways. ...
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Ссылки http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_125.pdf -- 294.6 Кб -- 04.08.2015
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34. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB53F2F00-06F4-43C9-AE69-0696A2821461%7D
An example of galaxy that shows a double-component structure in the HST/ACS image. North is up and east is left. ... The thumbnails of the HST/ACS I band (effective wavelength = 814 nm), the Subaru Telescope/Suprime-Cam NB711 and i'- and z'-bands are shown from left to right. Note that the NB711 image, which captures the Lyman-alpha line emitted by neutral hydrogen, shows spatially extended gas which is ionized by ultraviolet (UV) radiation from many massive stars. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB53F2F00-06F4-43C9-AE69-0696A2821461%7D -- 4.3 Кб -- 10.04.2016
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35. sune
The Star called the Sun. The Sun as the star . ... The visible star value . ... Spectrum class . ... 149 597 870 km . ... The Solar energy sourse is the core transformation of the Sun, where temperature is 15 000 000 K. The energy from inside is carried by irradiation and then in the external layer with 0,2 Ra of thikness - by convection. ... The Earth, situating far from the Sun (149 mil km), receives about 2.1017 W of the Solar beam energy (see item "The Solar constant" ). ...
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Ссылки http://www.space.vsi.ru/sune.htm -- 6.1 Кб -- 14.10.2000
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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 ...
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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.inasan.rssi.ru/~akimkin/presentations/UVUniverse2010.pdf
... It is reasonable to expect that UV part of the irradiating spectrum is most influenced by the grain evolution (growth and sedimentation ) which marks the very initial stage of planet formation. 2 log J [erg s1 cm2] 1 0 -1 -2 -3 1000 BB 40 0 0 (A5 ) BB 20 0 00 (A5) Drai ne (A5 ) BP Ta u (A5) BB 40 0 0 (GS) BB 20 0 00 (GS) Drai ne (GS) BP Ta u (GS) Disk Model Density distribution is based on a 1+1D disk ... Green lines are used for a model with dust growth and sedimentation. ...
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Ссылки http://www.inasan.rssi.ru/~akimkin/presentations/UVUniverse2010.pdf -- 256.1 Кб -- 12.03.2013
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38. Корпус экспертов
. Корпус экспертов . Ключевые слова . физика магнитных явлений . магнитный резонанс . магнитоупорядоченные структуры . Специализация по классификатору . 71. Electronic structure of bulk materials . 73. Electronic structure and electrical properties of surfaces, interfaces, thin films, and low-dimensional structures . 75. Magnetic properties and materials . 76. Magnetic resonances and relaxations in condensed matter, Mossbauer effect .
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Ссылки http://www.scientific.ru/expertise/petrakov.html -- 6.1 Кб -- 10.03.2011
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39. Geomagnetic Indices Kp, ap, Ap, Cp and C9
This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/index.html -- 13.1 Кб -- 14.10.2001
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40. Stellarium: StelViewportEffect Class Reference
Stellarium 0.12.3 . ... Classes . ... Renderer . FileљStructure . ... StelViewportEffect Class Reference abstract . Allow to apply visual effects on the whole Stellarium viewport. More... #include < StelViewportEffect.hpp > . virtual QStringљ . ... drawToViewport (class StelRenderer *renderer)=0 . ... distortXY (float &x, float &y) const . ... Definition at line 35 of file StelViewportEffect.hpp . virtual void StelViewportEffect::distortXY . ... core/ StelViewportEffect.hpp . ...
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Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelViewportEffect.html -- 8.8 Кб -- 28.02.2014
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