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61. http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/README
... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/Model2000/AtmModel/UV/README -- 7.8 Кб -- 26.03.2000
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62. Fotogallery
. The Planet's Parade . The Hale-Bopp Comet . The Ikeya-Zhang Comet. Sergey Nazarov's Foto . Ursa Major . The Young Moon . The Moon. Andrew Zolotukhin' s Foto . 2003 May 07: Transit of Mercury . Home | My Telescope | Introduction | Links .
[ Сохраненная копия ]  Ссылки http://southsky.chat.ru/English/Fotogallery_Eng.html -- 6.0 Кб -- 09.04.2016
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63. Report on Cosmic Call 1999
... Report on Cosmic Call 1999 . ... Cosmic Call Sessions . ... This Report outlines methodology, hard- and software, which were developed to transmit first public Interstellar messages from Evpatoria Deep Space Center (EDSC), and describes four Cosmic Call Sessions, which were fulfilled in EDSC on May 24 and June 30 - July 1, 1999. ... Each Cosmic Call consists of two parts. ... Dutil Message, . ... The software for gathering all messages and creating the Cosmic Call stream, was written on C language. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/ra&sr/irm/report-1999.html -- 56.9 Кб -- 30.11.2002
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64. Lunar Eclipse of August 28, 2007
These images were taken at Moore Observatory in Louisville, Kentucky, and at Mt. Kent Observatory in Queensland, Australia, with Nikon D200 digital SLR cameras. ... 2:10 EDT (Full moon) . 3:19 EDT (Penumbral eclipse underway) . ... 5:22 EDT (Totality 30 minutes away) . ... 5:53 EDT (Totality) . ... Kent Observatory are Copyright 2007 by the University of Southern Queensland and Rhodes Hart. Images from Moore Observatory are Copyright 2007 by John Kielkopf , University of Louisville. ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/gallery/eclipse/index.html -- 3.5 Кб -- 11.05.2010
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65. Scientific.ru Альтернативный форум
Альтернативный форум . Scientific.ru Все форумы . ... Time (@) - 13.04.2007 09:15 . Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results . x203a; x203a; x203a; в ответ на: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич . ... Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич, 13.04.2007 13:37 . ...
[ Сохраненная копия ]  Ссылки http://www.scientific.ru/dforum/altern/1176441340 -- 10.0 Кб -- 12.04.2016
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66. http://www.asc.rssi.ru/RadioAstron/meetings/RA&RISC/2013/risc2013_summary.pdf
... The early science program has been very successful with about 600 separate segments observed of which about 92% were successful. ... In response to AO-1, thirteen Key Science proposals were received from ~200 authors for 1800 hours and were evaluated by the RPEC. ... The RISC strongly urged that the results of the ESP and AO-1 need to be made available (published in refereed journals) as soon as possible which will give credibility to AO-2 proposals. ...
[ Текст ]  Ссылки http://www.asc.rssi.ru/RadioAstron/meetings/RA&RISC/2013/risc2013_summary.pdf -- 27.4 Кб -- 10.07.2013
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67. http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf
... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf -- 100.3 Кб -- 21.05.2007
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68. SPUTNIK home page
. Dedicated to 40th anniversary of the . first artificial Earth satellite launch . Russian (Win) .
[ Сохраненная копия ]  Ссылки http://sputnik.infospace.ru/ -- 7.9 Кб -- 22.10.2003
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69. http://www.ssau.ru/files/education/metod_1/gavrilov_sozdanie_program.pdf
... 1.4 OSGi Java. ... Solver, package sample; import org.slavery.basic.Solver; import org.xdp.commons.SessionID; import org.xdp.commons.URI; public class SampleSolver extends Solver { public SampleSolver(SessionID sid, String name) { super(sid, name); } @Override public void perform() { double d = (Double) storage.load( new URI(getName() + "/initdata"), getSessionID()); double r = Math.sin(d); storage.save(new URI(getName() + "/resdata"), r, getSessionID()); } 41 } load() storage, Solver. , save(). , ,...
[ Текст ]  Ссылки http://www.ssau.ru/files/education/metod_1/gavrilov_sozdanie_program.pdf -- 1267.7 Кб -- 09.12.2014
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70. What is Redshift? (2dF QSO Redshift Survey - 2QZ)
... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...
[ Сохраненная копия ]  Ссылки http://www.2dfquasar.org/restframe.html -- 10.2 Кб -- 07.05.2008
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71. http://comet.sai.msu.ru/~gmr/AC/AC1573.pdf
ASTRONOMICHESKII TSIRKULYAR No.1573, 2010 April 12 1995 2009 . A Comparison of the Latitudinal Variations of the Methane Absorption Bands on Saturn's Disk at Equinoxes 1995 and 2009 Abstract. The observations of Saturn at last equinox 2009 have detected significant differences of the latitudinal variations of the methane absorption from observed at 1995 equinox . ... 1995 . 2008- 2009 , ­ . ... 4 ( 580-880 ) , (.1) , 2008-2009 . ... 2 , 4 725 1995 2009 . ... 1995 2009 15 , 1980 1995 . ...
[ Текст ]  Ссылки http://comet.sai.msu.ru/~gmr/AC/AC1573.pdf -- 236.4 Кб -- 06.03.2012
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72. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
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73. Observing with VISTA
Home . ... Observing . Exposure Time Calculator (ETC) . Survey processing . ... ESO - Public Surveys . near IR surveys . ... Exposure Time Calculator . ... Survey Area Definition Tool . Recommended values for Detector Integration Time (DIT) . ... Detector Properties . ... Filter properties . ... ESO ][ VISTA Home ] ...
[ Сохраненная копия ]  Ссылки http://www.vista.ac.uk/observing/index.html -- 8.0 Кб -- 24.10.2012
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74. Catalogue of acient and medieval eclipses
. This page uses frames, but your browser doesn't support them.
[ Сохраненная копия ]  Ссылки http://www.pereplet.ru/gorm/atext/ginzele.htm -- 2.0 Кб -- 01.03.2014
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75. 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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76. http://solarwind.cosmos.ru/txt/egs2010list.doc
... Anomalous magnetosheath dynamics: magnetosheath crossings by spacecraft in few minutes and flow balancing by plasma jets Sergey Savin, Ermanno Amata, Lev Zelenyi, Viacheslav Budaev, David Sibeck, Natalia Borodkova, Vassilis Angelopoulos, Jean-Lous Rauch, Eugene Panov, and Jan Blecki Comparison of Two Successive Substorms Observed on August 1, 1998 Natalia Borodkova, Vladimir Parkhomov, and Georgy Zastenker ...
[ Текст ]  Ссылки http://solarwind.cosmos.ru/txt/egs2010list.doc -- 29.5 Кб -- 24.05.2010
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77. http://site2010.sai.msu.ru/static/doc/WHongshuai_site2010.pdf
Cloud cover and water vapor observed at Oma site,Tibet W ang Hong-shuai (National Astronomical Observatories of China) Kislovodsk 8.10.2010 Wang Hongshuai ­ Kislovodsk ­ Oct.2010 2 2008.11 Oma Site 40 m CT 2 tow er 4.5 m antenna Satellite communication w eather station 10m tow er SBIG seeing m onitor DIMM seeing dome MIR cloud m onitor R en ew al p o w er supply Wang Hongshuai ­ Kislovodsk ­ Oct.2010 3 PWV<0.5 5 .0 % 1 0 .1 % 8 .1 % Percent. ... 05 8.3% Percent . ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/WHongshuai_site2010.pdf -- 1237.0 Кб -- 20.10.2010
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78. The Sunspot Observer - Visual indices of solar activity
Statistics of sunspot activity . The sunspot indices . ... Visual indices of solar activity . ... n - number of spot groups . A - Waldmeier class of unipolar spot groups without penumbra . B - class of bipolar spot groups without penumbra . C - class of bipolar spot groups with one penumbra pole . D - class of small bipolar spot groups with two penumbra poles . E - class of middle bipolar spot groups with two penumbra poles . ... H - class of unipolar penumbrated spot groups . ...
[ Сохраненная копия ]  Ссылки http://www.alexeyryback.ru/en/sunspot_indices.htm -- 5.5 Кб -- 03.02.2016
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79. http://www.sai.msu.su/gcvs/gcvs/iii/vartype.txt
GCVS Variability Types and Distribution Statistics of Designated Variable Stars According to their Types of Variability ======================================================================== I. GCVS Variability Types. ... Amplitudes usually do not exceed 0.1 mag. ... RR Variables of the RR Lyrae type, which are radially-pulsating giant A-F stars having amplitudes from 0.2 to 2 mag in V. Cases of variable light-curve shapes as well as variable periods are known. ... RV Variables of the RV Tauri type. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/gcvs/gcvs/iii/vartype.txt -- 54.3 Кб -- 25.09.2012
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80. Pulkovo databases: photometric observation
... mag . ... arcsec . ... deg . ... 2014-11-19 03:02:03 . ... Observation . ... Pulkovo . ... mag(j4+j3)-mag(j2) . ... Izmailov I.S. processed by . Izmailov I.S. ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/photometry/phemu2014-2015/?oid=1 -- 4.1 Кб -- 09.04.2016
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