Íàéäåíî äîêóìåíòîâ: 279205 (181 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.93ñåê. |
Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150413.en.txt.
http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150413.en.txt.
21. http://www.iki.rssi.ru/apetruko/forecast/data/RSGA.txt
Product: Report of Solar-Geophysical Activity :Issued: 2016 Apr 08 2200 UTC # Prepared jointly by the U.S. Dept. of Commerce, NOAA, # Space Weather Prediction Center and the U.S. Air Force. ... Analysis of Solar Active Regions and Activity from 07/2100Z to 08/2100Z: Solar activity has been at low levels for the past 24 hours. ... Geophysical Activity Summary 07/2100Z to 08/2100Z: The geomagnetic field has been at quiet to minor storm levels for the past 24 hours. ...
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Ññûëêè http://www.iki.rssi.ru/apetruko/forecast/data/RSGA.txt -- 2.9 Êá -- 08.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.cosmos.ru/forecast/data/RSGA.txt -- 2.9 Êá -- 08.04.2016
Ïîõîæèå äîêóìåíòû
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.cosmos.ru/forecast/data/RSGA.txt -- 2.9 Êá -- 08.04.2016
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1424) - www.cosmos.ru/ )
22. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2006/ptcspn51.pdf
Precision Telescope Control System PTCS Project Note 51.1 A Preliminary Analysis of the Correlation Scales of Wavefront Errors of the GBT Using the Moon Bojan Nikolic, Dana S. Balser & Richard M. Prestage 27 June 2006 GBT Archive: PR063 File: PROJECTS Keys: PTCS, OOF Abstract Observations of the GBT error beam are performed using the Moon to explore the spatial scales in the aperture plane over which the dominant wavefront errors are correlated. ... The expected observed scan is shown in Figure 7. ...
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Ññûëêè http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2006/ptcspn51.pdf -- 159.4 Êá -- 25.11.2009
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Åùå â ðàçäåëå:
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23. http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf
... N. Kardashev and M. Popov informed the participants on the current IOC results. ... Kovalev). ... Agenda of the RadioAstron teleconference November 16, 2011 Corrections to the Agenda 1 2 3 4 5 6 IOC status and results Single Dish observation with RA VLBA observations to find best fringe search candidates Fringe search plan Early science program plan Tracking stations outside Russia N.Kardashev N. Kardashev / M.Popov V. Kostenko E.Fomalont M.Popov Y.Y. Kovalev / M.Popov /A.Alakoz ...
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Ññûëêè http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf -- 24.6 Êá -- 13.12.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>150) - www.asc.rssi.ru/ )
24. Bob Berman's strange universe: Expect a surprise | Astronomy.com
... Tonight's Sky . ... Observing . ... Bob Berman . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... Dave's Universe . ... Bob Berman's Strange Universe . Bob Berman's strange universe: Expect a surprise . ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...
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Ññûëêè http://www.astronomy.com/magazine/bob-berman/2005/07/bob-bermans-strange-universe-expect-a-surprise -- 63.3 Êá -- 10.04.2016
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25. Description
... efftplot (efftplot-2.17) [xmmsas_20070708_1801-7.1.0] . ... The parameters of powspec are computed from the parameters of efftplot , such that for each energy band, only one time-averaged PDS is computed. Then for each energy band, efftplot reads the PDS into the FITS file produced by powspec , and plots it with the PGPLOT library. ... 1 : PDS is normalized such that the (white) noise level expected corresponds to a power value of 2. ... 2 : as =2, but the expected white noise level is subtracted. ...
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Ññûëêè http://xmm.vilspa.esa.es/sas/7.1.0/doc/efftplot/node3.html -- 8.8 Êá -- 08.07.2007
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>29812) - xmm.vilspa.esa.es/ )
26. Limiting Magnitude Table
DISCLAIMER: The larger the aperture, the more light a telescope will gather and the fainter the object you can see. Here is a range of magnitudes you might expect to see. Given excellent sky conditions and good optics, a well trained eye can sometimes add up to 0.8 magnitude to these values. Limiting Magnitude depends on much more than the instruments aperture. ... One formula is for aperture in inches the other is for aperture in millimeters. ... Aperture (inches) . ... 15.2 . ...
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Ññûëêè http://www.wro.org/ras/matto/limiting_magnitude_table.htm -- 9.6 Êá -- 18.08.2005
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Åùå â ðàçäåëå:
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27. Discussion and conclusions
... We compare our results with the GRANAT X-ray observations of the Galactic center (Churazov et al. ... It is instructive to compare our results for the Galactic center starburst with what might be expected for a continuous star formation, with the average rate characteristic for the whole Galaxy. For this continuous star formation model, we would expect to observe in the region of around the Galactic center about 10% of the total number of X-ray sources in the Galaxy. ...
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Ññûëêè http://xray.sai.msu.ru/~polar/html/publications/apj/node10.html -- 10.8 Êá -- 21.06.1996
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>603) - xray.sai.msu.ru/ )
28. http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf
... Several attempts to discover the FICN signal in VLBI nutation series made during last years failed. ... We investigated several VLBI CPO series by means of spectral and wavelet analysis. It has been shown that there are several periodic signals with close amplitude around the expected FICN period without any prevailing one that can be reliably associated with the FICN. ... DATA ANALYSIS We analyzed several CPO series obtained in IVS analysis centers by means of spectral and wavelet analysis. ...
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Ññûëêè http://www.gao.spb.ru/english/personal/malkin/publ/zm135.pdf -- 144.9 Êá -- 02.01.2015
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29. http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf
TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...
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Ññûëêè http://www.ssau.ru/files/science/conferences/itnt2015/itnt_2015_70.pdf -- 161.6 Êá -- 04.08.2015
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>657) - www.ssau.ru/ )
30. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz
... The CoAddition Technique Applied to Images of Galaxy Cores W. W. Zeilinger Institut f˜ur Astronomie, University of Vienna, T˜urkenschanzstraúe 17, A1180 Wien, Austria P. Crane, P. GrosbÜl and A. Renzini European Southern Observatory, KarlSchwarzschild Straúe 2, D85748 Garching, Germany Abstract. ... One may therefore take full advantage of the high resolution FOC images by coadding them with (high signaltonoise) ground based data. ... References Crane, P. et al. ...
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Ññûëêè http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz -- 76.9 Êá -- 12.06.2006
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>262) - www.stecf.org/ )
31. http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p366.pdf
Magnetic Stars, 2011, pp. 366 373 Sp ectral Variability of the Be Star HD 152478: Evidence for Magnetized Wind? ... Notable variations of line profiles have been found for a number of elements (H I, He I, Fe II, etc.) ... In this report we consider the largescale profile variability, observed in the opticallythick H and H lines, and in several opticallythin Fe II lines. ... Figure 2: The same as in Fig. 1 but for H line