This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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• Formation, stability and decay of inhomogeneus plasma structures in a hot

... The first column has the name of the qualifier. ... name of AB (inherited from first raw file, with grouping tag read from <instr>_organisation.h) . ... root name of products (inherited from first raw file and grouping tag read from <instr>_organisation.h) . ... name and value of non-default parameter(s) required to execute the recipe (set by createAB; read from <instr>_association.h) . ... name of waitfor(s) for this AB (relevant for DRS=CON only; set by createAB; read from <instr>_association.h) ....

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• ESO - Thesis Topic: Properties of kinematically decoupled structures in
• ESO - Thesis Topic: The dawn of planets: structure and evolution of
• ESO - E-ELT Telescope Design

Note : v is the velocity of the Sun with respect to the centroids of stellar groups ; l and b are the Galactic longitude and latitude of the Solar apex; 1 , 2 and 3 are the major, mean , and minor emi-axes of the velocity allipsoid, which can be considered equal to the velocity dispersions u , v , and w , respectively; L 1 and B 1 are the longitude and latitude component of the vertex deviation; e is the mean eccentricity; Z max is the ... VERTICAL STRUCTURE OF THE GALACTIC DISK. ...

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... The International Conference "Mode Conversion, Coherent Structures and Turbulence" will be held in the Space Research Institute of RAS during the period from 23 up to 25 November 2009. ... The international conference MSS-09 is organized by Space Research Institute with participation of the Russian Academy of Sciences, the Dynasty Foundation, the Russian foundation of fundamental researches, the European Geosciences Union, the Education and the Scientific Council on Nonlinear Dynamics of RAS. ...

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• Coronal holes [Oulu]
• ULF waves [Oulu]
• TCV [Oulu]

... In this section, we develop a physical model of the secondary as a disk that is centrifugally supported in the radial direction and hydrostatically supported in the vertical direction. We assume that the disk is vertically isothermal and well mixed. ... where is the mean molecular mass of the gas, is the orbital period at the outer edge of the disk in years, and all of the mass of the secondary has been assumed to be concentrated near its center, so the Keplerian approximation is valid. ...

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• Doug Burke's Perl/S-Lang pages: Structure examples
• Martin Elvis' Research: Quasar Structure
• The AstroStat Slog Blog Archive my first AAS. III. ANOVA

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• Database of Optical Properties -- Level: subsubpage
• LPV and Wind structure of OB stars
• Database of Optical Properties -- Level: subpage

... Stotskii A. A. Path length fluctuations through the Earth troposphere: turbulent model and data of observations. The spatial and temporal structure functions of path length the Earth troposphere for the whole space and time ranges constructed on the base of turbulence theory are considered. These structure functions include three domains: a power law of 5/3 (three-dimensional turbulence), a power law of 2/3 (two-dimensional turbulence) and saturation. ...

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• Annotation_26

... Future seminars . P a s t seminars . Seminar council . Collective processes and structures in spiral galaxies " . ... A new approach to studying global structures in thin stellar disks, which allows to describe universally both bar and spiral modes, is presented. ... Study of line-of sight velocity maps of gaseous disk in spiral galaxies allows, under some conditions, to reconstruct 3 components of gas velocity in the galactic plane. ...

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• The Sun's Corona
• Scientific Programme

. Next: RGS_CLOCKPATTERNS Up: RGS_BADPIX Previous: References Contents . TEMPERAT= 1.63150000000000E+02 / [K] Temperature of CCDs OCB = 3 / On-chip binning factor . CCD_ID . NODE_ID . RAWX (pixel) . RAWY (pixel) . YLENGTH (pixel) . DESCRIPTION . TEMPERAT= 1.63150000000000E+02 / [K] Temperature of CCDs OCB = 1 / On-chip binning factor . CCD_ID . NODE_ID . RAWX (pixel) . RAWY (pixel) . YLENGTH (pixel) . DESCRIPTION . Michael Smith 2011-09-20

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• CAL_getRGAObscure
• EllipseT structure definition
• ODF Structure

Microsymposium 38, MS080, 2003 (A4 format) PHYSICAL AND MINERALOGY CHARACTERISTICS OF THE LUNAR REGOLITH IN THE AREAS OF THE THERMAL ANOMALIES. ... Comparison of the local cumulative number of particles N per 104 m2 and photometric roughness parameter I. In this report we research data of the IR thermal radiation, the rough structure of the lunar regolith and mineralogy characteristics upper layer of the surface. ... The spatial graphical function of the lunar-surface thermal radiation. ... Figure 3. ...

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• http://selena.sai.msu.ru/San/Publications/ms38/ms059.pdf
• Шевченко Владислав Владимирович

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• Astronomy HyperText Book: Stellar Evolution
• The Galaxy Gallery: Messier Objects
• Low Surface Brightness Galaxy Gallery

... Credit: DMR , COBE , NASA Explanation: These spots are the oldest, most distant structures known. They are seen on the above two images of the microwave sky, north and south of our galaxy's equator, based on four-year's worth of data from NASA's COsmic Background Explorer (COBE) satellite (1989-1993). ... Publications with keywords: COBE - hotspots - cosmic microwave background radiation . Publications with words: COBE - hotspots - cosmic microwave background radiation . ...

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• Астронет > Microwave Hotspots: The Oldest Structures Known
• Earths Richat Structure
• COBE Hotspots:The Oldest Structures Known

... 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. ...

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H I Self-Absorption (HISA) arises from cold H I gas in front of warmer H I emission at the same velocity. HISA is thus a unique probe of the velocity and temperature structure of the Galactic ISM, from sub-parsec scales within clouds up to multi-kiloparsec scales across the disk. ... To address this question, a series of simple H I radiative transfer models of the Galaxy will be presented. ...

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• Galactic Spiral Structure in H I Emission and Self-Absorption
• Spectral-Line Observing
• Multiscale Structure of Interstellar Matter

... 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. ...

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• Theoretical Astrophysics

... Laboratory of Real Structure of Crystals . ... Microscopic mechanisms of magnetization reversal of nanostructured magnetic materials (multilayers, spin valves, etc.) ... Dynamical properties of domain walls, Bloch lines and points in ferromagnetics. ... Nonlinear excitations of spin systems localized in domain walls as well as of soliton-like spin waves and their evolutions. Dynamical properties of domain walls in ferroelectrics. ... ISSP RAS © 2006 All rights reserved ...

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• Laboratory of spectroscopy of defect structures ISSP RAS
• Laboratory for Spectroscopy of Molecular Structures
• X-Ray Structural Analysis

... On the internal structure of a thin accretion disk . The internal structure of the thin accretion disk in the vicinity of a black hole inside the last stable orbit ( r<3r g ) is considered within the hydrodynamical version of the Grad-Shafranov equation. It is shown that in the vicinity of the sonic surface takes place a sharp diminishing of the disk thickness, so at any way up to the sonic surface the flow is not radial. ...

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• Structure of the Galaxy
• Accretion Mechanizsm of the Formation of the Large Structure
• ADS Abstract Service Results

... 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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• Origin of the internal structures in HL Tauri jet (HH 151)
• V1494
• Observatory structure

The subdirectory steppe contains the time series recorded at Zymlyanskaya steppe in Rostov-na-Donu region. The data recorded in Moscow are placed at subdirectory moscow . ... The first one is the horizontal wind velocity, the second one is vertical velocity. ... The first two digits of filename is an identification of recording, and the third digit (1-6) is the number of time series. The first number N in any file is the total number of the points, followed by the N data values. ...

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• APOD: 2000 October 29 - Microwave Hotspots: The Oldest Structures Known
• APOD: March 9, 1997 - COBE Hotspots:The Oldest Structures Known
• APOD: 2013 May 19 - Earths Richat Structure