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

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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• ON THE STRUCTURE OF 3.11.94 ECLIPSE CORONA

To understand the impact of low metallicities on giant molecular cloud (GMC) structure, we compare far-infrared dust emission, CO emission, and dynamics in the star-forming complex N83 in the Wing of the Small Magellanic Cloud (SMC). ... This allows us to resolve the relative structures of H2, dust, and CO within a GMC complex, one of the first times such a measurement has been made in a low-metallicity galaxy. ... ADS Citation Query . citations = 59 . citations vs. year [year,citations] . ...

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• The DIRTY Model. II. Self-consistent Treatment of Dust Heating and Emission in
• The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
• Star formation rates from young-star counts and the structure of the ISM across

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. ...

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• Internal Structure of Stars
• Methods of Radio-Astronomy

... Archives . ... Magnitude [Eqn] . ... Differential Emission Measures (DEMs) are a summary of the temperature structure of the outer atmospheres (aka coronae) of stars, and are usually derived from a select subset of line fluxes. ... is called the Differential Emission Measure and is a very useful summary of the temperature structure of stellar coronae. ... Tags: DEM , Differential Emission Measure , EotW , Equation , Equation of the Week , stellar coronae . ... Comment ( RSS ) | ... Chandra Blog . ...

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• Vertical Structure of the Secondary: Hydrostatic Model
• The AstroStat Slog Differential Emission Measure
• A Structure for Quasars

A Tunable 350-780 GHz CW Solid State Oscillator of Intrinsic Josephson Junctions in a high-Tc Superconductor H. B. Wang#,*, M. Y. Li#,*, J. Yuan#, N. Kinevy, J. Li#, B. Grossz, S. Guenonz, A. Ishii# ... Quantum Phenomena in LISA+, Universitaet Tuebingen, D-72076 Tuebingen, Germany Email: hbwang1000@gmail.com Abstract--We report on THz emission measurements and low temperature scanning laser imaging of Bi2Sr2CaCu2O8 intrinsic ...

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• Project 5 - State Program "Condenced Matter Physics"
• Kotel'nikov IRE RAS, LASLDS
• Project 1 - SfP - Ovsyannikov, Supersensitive high-Tc superconducting

... 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
• Structure in N63A
• Астронет > Structure in N63A

... DLTS . ... Deep Level Transient Spectroscopy ( DLTS ) is a unique and powerful tool for the study of electrically active defects (known as traps) in semiconductors. DLTS can be used in one of two modes of operation; with Schottky diodes or with p-n junctions. ... The capacitance transient is measured as a function of temperature (usually in the range from liquid nitrogen temperature to room temperature 300K or above). ...

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• Laboratory of Real Structure of Crystals ISSP RAS
• Lead tungstate PbWO4
• Laboratory for Spectroscopy of Molecular Structures

... The spatially resolved structure near the hydrogen emission H line was found in the spectrum taken with the BTA/SCORPIO in June, 2013. ... The fragment of the Nova V1494 Aql spectrum is shown in Fig.1. ... The Nova V1494 Aql has passed the stage of the supersoft X-ray source (SSS) in the period between 218 and 516 days after the visible light maximum (Schwarz et al., ... The spectrum of Nova V1494 Aql taken on 2013 June 9 with BTA/SCORPIO . ... The vertical lines are the lines of night sky emission....

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• Origin of the internal structures in HL Tauri jet (HH 151)
• Detection of polarized radiation sources with unusual spectral characteristics
• Solar system sector, archive 1997

MULTIґFREQUENCY OBSERVATIONS OF THE POLAR RADIO STRUCTURES A. Riehokainen 1 , A.G. Tlatov 2 1 Tuorla Observatory 21500, Piikkio, Finland; 2 Pulkovo Astronomical Observatory, St. Petersburg, Russia alerie@utu.fi In this work we present a comparison of the enhanced temperature regions (ETRs) in the radio emission of the Sun with other manifestations of solar polar structures over some days in 2003ґ2005. ... We compared our radio data with di#erent SOHO/EIT and SOHO/MDI images for the same periods. ...

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• "Structure" publications in 1998 year
• "Structure" publications in 1999 year
• "Structure" publications in 2001 year

. 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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• EllipseT structure definition
• ODF Structure

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . Figure 1: Dynamic spectrum of Jovian radio emission recorded by Cassini on October 21, 2000 (courtesy of W.S. Kurth, Cassini RPWS Team, University of Iowa). ... We investigate the formation of zebra-like fine spectral structures (consisting of several parallel bands in the dynamic spectrum) in the Jovian broadband kilometric radiation; such radio bursts were observed by Cassini in 2000/2001. ...

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• PhD Thesis abstract
• Jorick Vink
• Organizational Structure

The neutral hydrogen structure at high galactic latitude . ... Angular structure of the interstellar HI emission at 21 cm was investigated on the declinations of +5 degree, +16 dg., +27.5 dg., +39 dg. and +50 dg. in the R.A. range of 10 h to 16 h (galactic latitudes from 45 dg to 90 dg) with the help of RATAN-600 radio telescope with mean angular resolution 2.0'x 20'. ... Angular power spectrum of interstellar HI emission was computed with standard FFT code and smoothed over 1 h along R.A. (figure 1). ...

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• RESEARCH PROBLEMS of the LRS
• Structure and properties of IRC+10216
• Cosmological Gene project

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters ? and dwarf irregular satellites of the Galaxy. ...

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• Frequency distribution of galactic binaries
• Accretion Mechanizsm of the Formation of the Large Structure
• Seminars

... 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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• Radiation Dominance in the Early Universe
• Structure of Atomic Nuclei
• Cosmological Issues for Theorists

The Neutral Atmosphere H20 O 2 Water Vapour Radiometry Bob Sault O 2 H20 1 2 Microwave Radiometry Water Its dipolar structure means that its melting and boiling points are much higher than other simple molecules (e.g. CO2, O2, N2). ... Water vapour introduces 50-300cm of excess path. ... 5 6 Water vapour radiometry Continuum vs Line systems "Continuum" water vapour radiometers measure fluctuations far from water lines Line systems work near either of the two water lines: 22.3 GHz or 183 GHz. ...

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• The giant HII region NGC 3603
• Inhomogeneous Disk Structure
• Research

. Graca Rocha - Research . For a summary I'm interested in the study of the Cosmic Microwave Background Radiation Temperature and Polarization Anisotropies, non-Gaussianity, Topology of the Universe, Varying Fundamental Constants Theories, Weak Lensing, Large Scale Structure, etc.. Last updated: 2005 June. home .

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• PPT Slide
• PPEUC Programme - Cosmic Microwave Background Workshop
• OptInt PmWiki : Wiki 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: 2004 January 1 - Structure in N63A
• APOD: 2000 October 29 - Microwave Hotspots: The Oldest Structures Known
• APOD: March 9, 1997 - COBE Hotspots:The Oldest Structures Known

... 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 sґ1 cmґ2] 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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• Future of the Galaxy