... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

... Version # 5 from Aug-01-1999 c********************************************************** nt=nvers; call fildsph(&ni,&nj,&nk,&nc,&nm,namef) 10 call cdirsph ! ... Next step stop; end function funcrat(ff) c************************************************************ c Calculation of the right hand function c ff(15) - dimension of parameters : c (ff(1),ff(2),ff(3)) = (r,q,f) - point coordinats; c ff(4) - Ph (pressure); ff(5) - Pz (phase); c ff(6) - Th (themperature ... Th)*(1.+0.*rx) return; end...

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. ...

... 16, EGU2014-5683, 2014 EGU General Assembly 2014 © Author(s) 2014. ... Common oscillations in Global Earth Temperature , Sea Level , and Earth rotation Leonid Zotov (1), Christian Bizouard (2), and Nikolay Sidorenkov (3) (1) Sternberg Astronomical Institute of Lomonosov Moscow State University, Russia (wolftempus@gmail.com), (2) Paris Observatory, Service de la Rotation de la Terre, France, (3) Hydro-Meteorological Center of Russia, ...

... 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. ...

... core . ... 54 љ void forward ( const Vec3d *altAzPos, float *mag, const int num=1) const ; . 55 љ void forward ( const Vec3f *altAzPos, float *mag, const int num=1) const ; . ... 57 љ void forward ( const float *sinAlt, float *mag, const int num) const ; . ... 59 љ void forward ( const float *sinAlt, float *mag) const ; . ... 68 љ void backward ( const float *sinAlt, float *mag, const int num=1) const ; . ... 89 љ static float SUBHORIZONTAL_AIRMASS; . ... 168 љ // static const QString source( . ...

... October 6, 09:00 09:40 . Jorge Melnick (ESO) . ... We present a statistical and temporal analysis of the ground meteorological properties recorded at the five selected sites for hosting the European Extremely Large Telescope (EELT). ... Marc Sarazin (ESO) . The organization and development of the E-ELT site testing campaign by ESO are described. ... The E-ELT Site Testing activities in northern Chile and Argentina are reviewed, and pioneering explorative campaigns are illustrated. ...

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... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

... Program of the Course of Radio Astronomy . Moscow State University , Physics Department , Astronomy Division , 4 th year, 60 hours in total) . ... Molecular maser emission. ... The emission of the interstellar neutral hydrogen. ... Pacholczyk, A. G. Radio Astrophysics, W. H. Freeman & Co., ... Frontiers of Astrophysics, Avrett, E. H., ed., Harvard University Press, Cambridge, Mass., ... Kaplan, S. A., Pikelner, S. B. The Interstellar Medium, Harvard University Press, Cambridge, Mass., ...

... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...