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http://www.stsci.edu/stsci/meetings/space_detectors/paper.htm.

1. Heliophysics, Internal structure and seismology
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 . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ -- 5.6 Кб -- 21.03.2012
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2. http://www.stsci.edu/stsci/meetings/space_detectors/pdf/paper.pdf
... When integrated with antennas or horn feeds, such superconducting quantum wells could well be used as detectors for Tera hertz radiation for both photometric and spectroscopic applications. At a normal-superconductor interface electrons undergo a charge conversion process called Andreev reflection that transforms single electrons in the normal phase into Cooper pairs in the superconducting phase1. ... Andreev bound states are formed in such a superconducting quantum well. ... A. F. Andreev, Zh. ...
[ Текст ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/pdf/paper.pdf -- 33.4 Кб -- 22.08.2001
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3. HISA Radiative Transfer as a Probe of Galactic Structure
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. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/cv/igps06.html -- 2.1 Кб -- 11.05.2006
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4. Formation, stability and decay of inhomogeneus plasma structures in a hot
. 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 .
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/ionosphere/satellite_inv/str.shtml -- 8.3 Кб -- 09.04.2016
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5. Vertical Structure of the Secondary: Hydrostatic Model
... 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. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node89.html -- 10.7 Кб -- 01.10.2012
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6. Microwave Hotspots: The Oldest Structures Known
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1162396 -- 15.3 Кб -- 18.12.2000
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7. http://www.cplire.ru/html/lab234/pubs/2014_05.pdf
... 2*1018 /1/2, , 0.1 , 1.6 , 1 350 , 100 , 5*10 20 - 3. 10-100 10-100 , . ... Integrated structures comprising cold electron bolometers and twin-slot antennas have been studied in the temperature range 0.06-3 K. Dynamic resistance ratio and optical response was measured for 2-15 K black body radiation temperature. ... 12000 290 10000 RR Te 280 Electron temperature, mK 270 Resistance ratio, Rd/Rn 8000 260 250 6000 240 4000 230 220 210 0 50 100 150 200 250 300 2000 Phonon temperature, mK 3. ... 0.1 . ...
[ Текст ]  Ссылки http://www.cplire.ru/html/lab234/pubs/2014_05.pdf -- 1059.3 Кб -- 21.03.2016
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8. Internal Structure of Stars
... 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. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/vnutr_bud_zir_e.html -- 6.6 Кб -- 23.02.2005
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9. SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS SUPPLEMENTARY PROGRAM
... CONDENSED MATTER PHYSICS SUPPLEMENTARY PROGRAM . ... Relationship between symmetry of crystal structure, point symmetry and symmetry of physical properties of crystals. ... Crystal lattice energy, Structural types. ... Typical structures of metal and semiconductor phases. ... Wave diffraction in crystals and basic methods of investigation of crystal structures, their principles, potentialities and specifics. ... Crystal optics. ... Principal methods of investigation phase transitions in solids. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/engl/postgraduate/31-condensed-matter-physics-supplementary-program -- 23.3 Кб -- 10.04.2016
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10. CCF Structure
. 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
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node806.html -- 4.6 Кб -- 20.09.2011
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11. The Arcetri Spectral Code file format
Radiative losses have been determined by using the Arcetri Code line emissivities for each element calculated adopting a plasma electron density of 10 10 cm -3 . Each emissivity line is structured using the following format: An example from the Mg file (Phot cm 3 s -1 ) is given below: . ... Mail comments regarding interface to landi@poppeo.nrl.navy.mil Mail comments regarding spectrum data to mlandini@arcetri.astro.it, landi@poppeo.nrl.navy.mil ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/spettro/elements.html -- 2.4 Кб -- 15.03.2002
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12. Electron bombarded sensors-reliability
Electron-Bombarded, Back-Illuminated CCD Sensors . For Low-Light-Level Imaging Applications . ... Damage to the gate structure oxide layers from keV level X-rays will likely result in increased dark current and decreased full-well capacity. ... Figure 14 shows the increase in dark current