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1. Calculating the Position and Velocity Components of HST
... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/aket.html -- 12.3 Кб -- 03.11.2000
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2. Inference of Coefficients for Use in Phase Correction
... OOF software . ... Memos . ... Raw data . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Please note that the files"COPYING" in each of the distribution packages have GPL listed but it is in fact LGPL which applies. ... This is the raw data from the SMA used in the analysis shown in Section 4 of the memo. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/alma/memo-infer.html -- 14.3 Кб -- 25.11.2009
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3. Parameters of the 41 Dra system components
Find Similar Abstracts (with default settings below ) . ... Also-Read Articles . ... Parameters of the 41 Dra system components . ... 00/2001 . ... Stars: Binaries, Binaries: Fundamental Parameters, Binaries: Individual . ... 61B Based on spectral and speckle-interferometric observations of the system 41 Dra, model atmosphere parameters of the system components have been derived: component Aa - T eff = 6500K, lg g = 3.99, R = 1.87 R solar , component Ab - T eff = 6500K, lg g = 4.11, R = 1.61 R solar . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/bal_1_2003.html -- 9.3 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/bal_1_2003.html -- 9.3 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/bal_1_2003.html -- 9.3 Кб -- 02.10.2012
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4. Abstract 206
. Polar spots in Doppler Imaging maps of rapidly rotating late-type stars, especially the active components of RS CVn binaries, represent a major break with the solar paradigm, within which spots are only found at low latitudes. I examine critically the evidence for polar spots and point out that they are particularly sensitive to a number of systematic effects relating to determining reference ``zero-points''.
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract206.html -- 1.7 Кб -- 15.08.1996
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5. System Controlled Functions
... Some of the functions that go into designing a tower have been left for SNEAKERS to handle. ... A connector can only be placed on top of a support. ... The supports are placed on top of each other at various angles. ... The system determines the ideal angle from the end of the last support to the designed top of that leg of the tower. ... The maximum angle allowed is , so that the tower will continue to be designed toward the goal at the top. Connectors are always placed on top of supports. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~rdouglas/publications/thesis/section2_7_6.html -- 5.5 Кб -- 13.05.1997
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6. LPCBC: Abstract 2_35
... Electronic Raman scattering in Tl 2 Ba 2 CuO 6+ d : Symmetry of the order parameter, oxygen doping effects, and normal-state scattering. Abstract: . Single crystals of the optimally doped, moderately and strongly overdoped high-temperature superconductor Tl 2 Ba 2 CuO 6+ d (Tl-2201) with T c = 80, 56, and 30 K, respectively, have been investigated by polarized Raman scattering. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lpcbc/ABST/2_35.html -- 3.7 Кб -- 24.12.1999
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7. http://www.atnf.csiro.au/pub/people/jreynold/joint97/dickey.txt
Abstract for an Oral Presentation at the ATNF/AAO Joint Symposium Author : John Dickey, ATNF Title : Measuring the Distance to the Galactic Polarized Continuum using 21-cm Absorptio n Abstract : Using the Compact Array in 210m and 750m configurations, I have detected the polarized component of the Galactic synchrotron background radiation at 18 and 21 cm wavelength in the region of strong linear polarization at (l,b) = (326 - 333, 0 - +3) studied by Duncan et al. 1997). ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/jreynold/joint97/dickey.txt -- 1.8 Кб -- 24.02.1997
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8. Theoretical Astrophysics Department
. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/mdiv/tad/tad.htm -- 1.8 Кб -- 04.12.1997
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9. AstroStatistics Workshop @ HEAD 2004
... Abstract (txt) . ... Xiao-li Meng (Harvard U) . ... presentation (pdf) . ... web page: astrostatistics.psu.edu/stat05.html . ... H. Kang (Department of Statistics, Harvard University), D. van Dyk (Department of Statistics, University of California at Irvine), V. Kashyap (Harvard-Smithsonian Center for Astrophysics), A. Connors (Eureka Scientific) . ... Poster (ps) . Poster (pdf) . ... Y. Yu, X.L. Meng (Dept. of Statistics, Harvard Univ.) ... Y. Yu (Dept. of Statistics, Harvard Univ.) ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/ -- 10.3 Кб -- 01.10.2012
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10. Vladimir Marsakov Abstracts
. Authors: V.A. Marsakov , Yu.G. Shevelev , . Journal: Bull. Inform. CDS, 1988, № 35, p.129-130. љљљљљThe values of [Fe/H], the distancec, the componets of the space velocities and orbital parameters are calculated for 1304 non-evolved F -stars with homogeneous data and proper motions.
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/abs/abst18.htm -- 2.0 Кб -- 02.02.2007
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11. A fast-scan extragalactic source survey at 4.755 GHz
... 88, Jan. 1983, p. 1-15. l. A survey of extragalactic radio sources made using driven declination scans is reported covering an area of about 0.07 sr to a limiting flux density of 35 mJy. The fast-scan survey was carried out at a galactic latitude greater than 17 deg with the NRAO 91-m telescope operating at 4.755 GHz, and the 480 sources detected were reobserved at 1.4 GHz with the National Astronomy and Ionosphere Center 305-m telescope at Arecibo. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/SRC_Owen.html -- 5.2 Кб -- 18.03.2015
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12. EPIC Related CCF Components
Next: EMOS_ADUCONV Up: CCF Components Previous: Generation from In-Orbit Data Contents . ... Description . Generation from Ground Calibration Data . Generation from In-Orbit Data . ... Generation from ground data . Generation from in-flight data . ... Generation from Ground Data . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node668.html -- 11.0 Кб -- 20.09.2011
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13. Marc White - Astrophysicist - The Australian National University
Marc White . ... Turbulent entrainment processes may play an important role in the outflows from young stellar objects at all stages of their evolution. In particular, lateral entrainment of ambient material by high-velocity, well-collimated protostellar jets may be the cause of the multiple emission-line velocity components observed in the microjet-scale outflows driven by classical T Tauri stars. ... University of Amsterdam; STARPLAN, Copenhagen, Jul 2013 . ... E marc.white@anu.edu.au . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/publications.php -- 12.6 Кб -- 09.04.2016
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14. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p458.pdf
... 458 ­ 461 Magnetic Variability of the Ap Star HD 9996 Bychkov V. D.1 , Bychkova L. V.1 , Madej J.2 , Shatilov A. V.1 1 2 Special Astrophysical Observatory, Nizhny Arkhyz, Russia Warsaw University Observatory, Poland Abstract. ... Its phase magnetic curve exhibits two components. ... 1 Long­Perio d Magnetic Phase Curve Compilation of early photometric measurements of HD 9996 allowed us to constrain the corresponding period P in the range of 7750 < Pph < 8550 days (Pyper & Adelman, 1986). ...
[ Текст ]  Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p458.pdf -- 122.8 Кб -- 11.08.2011
[ Текст ]  Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p458.pdf -- 122.8 Кб -- 11.08.2011
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15. Kholtygin et al., "Stochastic Data in Astronomy. II.", Astrophysics (2007)
Kholtygin A.F., Shneiwais A.B., Burlakova T.E., Milanova Yu.V. Stochastic Data in Astronomy. ... Fourier Analasis of Strongly Unevaen Time Series . Astrophysics, 50 , 225-2387 ( 2007 ) Original Russian Text published in Zhurnal Astrofizika , 50 , pp. 281-297 ( 2007 ) . ... It is supposed that analysed time series consist of harmonic components with amplitude $A$ and a period larger than the longest segment of the time series and the noise component with variance $N^2$. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2007/Fourier2007abstr.html -- 2.8 Кб -- 19.11.2010
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16. Stellar Astrophysics Department
... The department was founded in late sixties by Prof. D.Ya.Martynov, who for many years was also the director of Sternberg Astronomical Institute. At present time, the head of the department is Prof. A.M.Cherepashchuk, a pupil of D.Ya.Martynov and his successor as the director of SAI. Since Prof. Martynov, the scientific activity of the department was primarily related to binary stars. ... The department consists of 15 members most of which have Ph.D. in Astrophysics. ...
[ Сохраненная копия ]  Ссылки http://uranus.sai.msu.ru/ -- 2.3 Кб -- 08.06.2010
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17. ADS Abstract Service Results
Find Similar Abstracts . ... Creation of particles in cosmology . Authors: . ... 00/1974 . ... COSMOLOGY, GRAVITATIONAL FIELDS, PARTICLE PRODUCTION, QUANTUM MECHANICS, EINSTEIN EQUATIONS, FIELD THEORY (PHYSICS), SINGULARITY (MATHEMATICS), SPACE-TIME FUNCTIONS, STRESS TENSORS, VISCOSITY . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/html/Z/biblio/74.4.html -- 6.0 Кб -- 29.05.1996
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18. Астронет > Англо-Русский Словарь
... Астронет | ... Термин "component" . ... компонента . ... составляющие [компоненты] радиоизлучения Солнца . ... составляющие [компоненты] солнечного радиоизлучения . ... основная компонента (радиоизлучения Солнца) . ... составляющая (радиоизлучения всплесков IV типа) в сантиметровом диапазоне (радиоизлучения Солнца) . ... жесткий компонент (напр. корпускулярного излучения) . ... спорадическая [быстрая] компонента (радиоизлучения Солнца) . ... составляющие [компоненты] радиоизлучения (напр. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/dict/show_term.html?base=component -- 28.3 Кб -- 16.02.2011
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19. Circular Polarization
Abstract -- The strengths of magnetic fields in interstellar gas clouds are obtained through observations of the circular polarization of spectral line radiation. ... To infer information about these irregularities from the observational data, we develop statistical relationships between the rms values of the irregular component of the magnetic field and spatial variations in the circular polarization of the spectral line radiation. ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/circular.html -- 2.8 Кб -- 27.09.2012
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20. Additional Parts of Theoretical Astrophysics
Stationary Shock Waves. ... Influence of Medium Ionization on Shock Wave Propagation. Shock Waves with Decays. ... Results of Classic Theory of Radiation of the Electron Moving in Ion Field. ... Classification and Physical Features of Galaxies. X-Radiation of Coronae of Elliptical Galaxies and Clusters of Galaxies. ... Methods of Obtaining of Information about Physical Conditions and Components of Interstellar Medium. ... Ionization Fronts and Shock Waves in the Interstellar Medium. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/dod_rozd_teor_astroph_e.html -- 5.3 Кб -- 23.02.2005
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