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http://mavr.sao.ru/hq/ssl/maryeva/Rhodes_poster1.pdf.

21. 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.
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/cat5MOD.html -- 2.2 Кб -- 18.01.2010
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22. http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf -- 2427.5 Кб -- 30.11.2014
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23. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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24. POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/polimodel.help.html -- 6.1 Кб -- 06.06.2006
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25. The magnetosphere models
The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Solar wind (SW) - the region outside BS; . ... Auroral field lines (AUR) region - the funnel-shape cavity restricted by the geocentric distance of the order of 6 RE, between surfaces formed by magnetic field lines emerged from the polar and equatorial OVAL borders; . ... Fairfield D.H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/msphere.htm -- 5.8 Кб -- 18.01.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/msphere.htm -- 5.8 Кб -- 18.01.1999
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26. Future of the Galaxy
... Line radiative transfer in C 18 O, HCO + , and CS lines is considered in a spherically symmetric chemo-dynamical model of a starless core, evolution of which is driven by the ambipolar diffusion. Theoretical line profiles are compared to observational data on the well-known L1544 core, which is one of possible candidates for collapsing protostellar clouds. ... Comparison between modelled and observed spectra suggests that L1544 has flattened structure and is observed at some inclination. ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/lines.html -- 2.2 Кб -- 27.09.2012
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27. http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c15-0.pdf
... Chapter 15. 15.0 Introduction Modeling of Data Given a set of observations, one often wants to condense and summarize the data by fitting it to a "model" that depends on adjustable parameters. Sometimes the model is simply a convenient class of functions, such as polynomials or Gaussians, and the fit supplies the appropriate coefficients. ... The parameters of the model are then adjusted to achieve a minimum in the merit function, yielding best-fit parameters. ... Data are generally not exact. ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c15-0.pdf -- 48.2 Кб -- 23.03.2000
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28. NASA JSC Cost Estimating and Models Web Site
Cost Estimating Web Site . ... 2005 NASA Cost Analysis Symposium Databases . ... World , European Communities , Other European Countries , Americas , Asia , Africa , General US , US Federal Government , US Department of Defense , Aerospace Industry , NASA , Science & Engineering Handbooks . NASA Cost Estimating Handbook 2004 , Parametric Estimating Handbook .. ... Consumer Price Index , Employment Cost Index , GDP Deflator , Import Price Index , NASA New Start Index , Producer Price Index . ...
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/bu2/ -- 15.7 Кб -- 26.11.2004
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29. Description of the RadioAstron project, english version
Status of the RadioAstron project development . The engineering model of the Space Radio Telescope (SRT) was assembled in Lavochkin Association (LA) in the configuration consisting of 10-m parabolic radio astronomical antenna made of carbon-fiber, F ocal and Device cabins of the scientific payload and on-board and ground complex of high data rate up-down radio link (VIRK). ... Then,radio astronomical tests were conducted using real radio sources. ... Space Radio Telescope . ... Data Processing . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/status_eng.htm -- 7.2 Кб -- 10.05.2008
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31. Theoretical Astrophysics
Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/teor_astroph_e.html -- 8.7 Кб -- 23.02.2005
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32. A Kernel Model for Precision Timekeeping
The technical memorandum: A Kernel Model for Precision Timekeeping (PostScript) describes an engineering model which implements a precision time-of-day function for a generic operating system. ... The model changes the way the system clock is adjusted in time and frequency, as well as provides mechanisms to discipline its time and frequency to an external precision timing source, such as a pulse-per-second (PPS) signal. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/kern.html -- 4.0 Кб -- 21.12.2007
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33. http://www.cplire.ru/rus/InformChaosLab/papers/iccsc04dek.pdf
MODELLING MICROWAVE TRANSISTOR CHAOS GENERATORS Alexander S.Dmitriev (member IEEE), Elena V.Efremova and Alexander D.Khilinsky Institute of RadioEngineering and Electronics, Russian Academy of Sciences, Mokhovaya St. 11-7, 101999, Moscow, Russia, E-mail: chaos@mail.cplire.ru Abstract н Microwave chaotic generators based on three-point circuit are analyzed. Principles of design of modelbased generator from low to microwave frequency range are discussed. ... Fig. ... Three-point scheme of generator. ...
[ Текст ]  Ссылки http://www.cplire.ru/rus/InformChaosLab/papers/iccsc04dek.pdf -- 331.3 Кб -- 14.01.2005
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34. http://www.iki.rssi.ru/galeev/astro2007/barkov2007.pdf
... Models of central engines (1) Potential of disk accretion onto stellar mass black holes: disk binding energy: thin disk life time: - accreted mass - disk outer radius - gravitational radius - Shakura­Sunyaev parameter Ultra-dense Hyper-Eddington neutrino cooled disks !! ... 1989); Neutron star + Neutron star Neutron star + Black hole White dwarf + Black hole Black hole + compact disk Burst duration: 0.1s ­ 1.0s Released binding energy: (1.2) Collapsars­ origin of long duration GRBs? ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/galeev/astro2007/barkov2007.pdf -- 2039.4 Кб -- 27.02.2008
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35. IUM (Spring 2015)
... Gaussian model selection by unbiased risk estimation (SURE) . ... Model selection for linear smoothers . Sieve model selection and uniform Wilks expansion . ... Bootstrap parameter tuning 16.02 19:20 - 20:50 ауд.310 . 17.02 19:20 - 20:50 ауд.401 . ... Курс может вызвать несколько больший интерес, чем в прошлые годы, поскольку летом 2015 на факультете компьютерных наук НИУ ВШЭ открывается магистерская программа "Математические методы оптимизации и стохастики" под его руководством. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ium/s15/s15-spokoinyii.html -- 2.7 Кб -- 18.02.2015
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36. Area of scientific investigations
... Research of an atmosphere of the Earth and other planets of Solar system by optical methods . ... The long-term experience of study of atmospheres of planets of Solar system in a department of physics of planets has defined directions and methods of researches spent for laboratory . ... The tasks of laboratory are researches by optical methods of structure of a Terrestrial atmosphere, namely study of spectra of absorption of its compound radiation of natural and artificial sources. ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/lao/investigations_eng.html -- 16.3 Кб -- 12.01.2010
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37. Vladimir Marsakov Publication List
Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/conf/paper1/conf1_1.htm -- 9.3 Кб -- 02.02.2007
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38. http://comet.sai.msu.ru/~dmbiz/abst/88-a
EVOLUTION OF GALACTIC DISCS: TWO MODES OF STAR FORMATION ABSTRACT We develop the model of the evolution of surface gas density, stellar density, star formation rates and chemical composition of galactic disc taking into account the gravitational instability of rotating gaseous layer in the scales of several kpc. ... In the model we took into account the gas return from evolved stars, a radial movement of the gas in a spiral arms and accretion of the gas into the galactic disc. ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~dmbiz/abst/88-a -- 2.3 Кб -- 14.01.1997
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39. The Ekpyrotic [string] Models And The Standard Guth Model. - an Astronomy Net
Bigbang Forum Message . Forums: . ... Discussion Forums | ... The Ekpyrotic [string] Models And The Standard Guth Model. Forum List | ... Post Message | ... Could you outline the differences between the Ekpyrotic [string] models and the standard Guth model? ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/bigbang/messages/859.shtml -- 13.9 Кб -- 09.04.2016
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40. Astronomical Catalogues
Astronomical Data Center . ... You can access the files described here in three ways: . ... Use CDS' VizieR Service at ADC to explore the data files. ... Get the data files via anonymous FTP. ... 1981) -------------------------------------------------------------------------------- Byte-per-byte Description of file : table1a Byte-per-byte Description of file : table1b -------------------------------------------------------------------------------- Bytes Format Units Label Explanations ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/source.htm -- 9.4 Кб -- 01.04.2000
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