Íàéäåíî äîêóìåíòîâ: 308224 (181 ñàéòîâ) ---- Âðåìÿ ïîèñêà: 0.58ñåê. |
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http://www.astronet.ru/db/varstars/msg/1160384.
http://www.astronet.ru/db/varstars/msg/1160384.
21. The Brightness of the Night Sky
The night sky brightness, together with number of clear nights, seeing, transparency, photometric stability and humidity, are some of the most important parameters that qualify a site for front-line ground--based astronomy. ... Night sky at ESO-Paranal (Chile). ... Night sky brightness data . ... UBVRI night sky brightness at ESO-Paranal during sunspot maximum (A 2003, PDF) . ... The Dancing Sky: six years of night sky observations at Cerro Paranal (Starlight 2007 conference proceedings, PDF) . ...
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Ññûëêè http://www.eso.org/~fpatat/science/skybright/index.html -- 6.1 Êá -- 22.04.2010
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>46641) - www.eso.org/ )
22. Phil Plait's Bad Astronomy: Bad News
... What's New? Bad Astronomy . ... News . ... The questions was: "During a flight, I saw a round rainbow shaped like a doughnut. ... However, she said that all rainbows are actually circles, and that she could not find a name for this phenomenon. ... One is that rainbows really aren't full circles. ... Basically, rainbows are due to light getting bent ("refracted") inside of raindrops. ... It's called a "glory", and is formed in a somewhat different way than rainbows. ... 2008 Phil Plait. ...
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Ññûëêè http://www.badastronomy.com/bad/news/marilyn3.html -- 20.6 Êá -- 09.04.2016
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>377) - www.badastronomy.com/ )
23. The International Olympiad of Euro-Asian Astronomical Society
Euro-Asian Astronomical Society . ... International Astronomy Olympiad . The First (Experimental) International Astronomy Olympiad was carried out by Euro-Asian Astronomical Society and took place at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) in North Caucasus on November 1-8, 1996. ... Why is it sometimes better to use a small telescope in orbit around the Earth than it is to use a large telescope on a mountain top? ... Grades 11-12 . ... Russia) . ...
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Ññûëêè http://www.issp.ac.ru/univer/astro/ioas96_e.html -- 15.3 Êá -- 11.04.2001
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24. http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/folk/g/galveston_flood
GALVESTON FLOOD It was a September evening when the sky was dark and grey Raging wind and water battled Hell in its sway The rich folk in the mansions and the poor ones in the dell Were swept into eternity the story left to tell Wasn't that a mighty time Wasn't that a mighty time that evening Wasn't that a mighty time When the storm winds struck our town The men left home that ...
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Ññûëêè http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/folk/g/galveston_flood -- 3.5 Êá -- 20.10.1992
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>3443) - crydee.sai.msu.ru/ )
25. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200111/Cal-Ops_Nov2001_NewerModes.pdf
... Three ` flavours'of binning and discard: · Discard 9 rows , readout 1 row, cut 10:1, resolution 1.75ms · Discard 90 rows , bin 10 rows , cut 10:1, resolution 2.76ms · Discard 95 rows , bin 5 rows , cut 20:1, resolution 2.76ms · Compared with normal timing : · 100 rows and readout, no cut, resolution 1.75ms Bin · Tested on XMM on Crab during rev 333 - 3 October 2001 Crab - rev 333 - Bright timing ... Counting mode and FIFO full errors. ... Crab - rev 333 - Bright timing mode ...
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Ññûëêè http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200111/Cal-Ops_Nov2001_NewerModes.pdf -- 426.1 Êá -- 14.05.2014
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>3006) - xmm.vilspa.esa.es/ )
26. Amateur Telescope Makers of Boston
... Telescopes . ... But regardless of where you observe from or whether or not you have a telescope, exploring the many aspects of astronomy can be an exciting hobby. It can be an activity shared with thousands of other amateurs all over the world. ... Or it might be pursued more actively by joining a local astronomy club like the Amateur Telescope Makers of Boston and learning by direct association with other amateurs. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
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Ññûëêè http://www.atmob.org/library/articles/gettingstarted.php -- 14.4 Êá -- 09.04.2016
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>385) - www.atmob.org/ )
27. First X-Rays From a Comet Discovered
A team of U.S. and German astrophysicists have made the first ever detection of X-rays coming from a comet. ... Following the initial detection, the team reported repeated X-ray emissions from the comet over the next 24 hours. ... One preliminary theory is that X-ray emission from the Sun was absorbed by a cloud of gaseous water molecules surrounding the nucleus of the comet, and then were re-emitted by the molecules in a process physicists call "fluorescence." ... Comets . ...
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Ññûëêè http://www.iki.rssi.ru/solar/eng/hyakutak.htm -- 5.3 Êá -- 15.10.1997
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>554) - www.iki.rssi.ru/ )
28. My activity
I recieved PhD in 1998 and now I'm a reseacher at the division of Relativistic Astrophysics at Sternberg Astronomical Institute of the Moscow State University. ... Isolated neutron stars and black holes. Their evolution, distribuion, accretion onto INSs and BHs . ... My 4th year work (B.S.): Accretion onto isolated neutron stars and accretion in X-ray pulsars. ... My diploma (M.S.): Binary evolution after the starformation burst at the Galactic Center, Moscow State University, 1995 January. ...
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Ññûëêè http://xray.sai.msu.ru/~polar/html/interest.html -- 8.7 Êá -- 03.05.2004
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>600) - xray.sai.msu.ru/ )
29. Àñòðîíîìèÿ, Çåìëÿ, Ñîëíöå, Ëóíà, Ìàðñ, Çâåçäû, Ãàëàêòèêè, Ôîòî êîñìîñà, Ñëîâàðü
... Ôàçà ëóíû = 9% . ... Ñîëíå÷íàÿ ñèñòåìà . ... Ëóíà . Ìàðñ . ... Ñðàâíåíèå ïëàíåò . ... Êàðòû ïîâåðõíîñòè ïëàíåò . ... Îá àñòðîíîìèè . ... Ãàëàêòèêè . ... Êîñìîñ . ... Íîâîñòè êîñìîñà . ... Ñîáûòèÿ â àñòðîíîìèè . ... Íóæíû ëè Âàì êíèãè ïî àñòðîíîìèè . ... Ôîòî êîñìîñà . ... Áèáëèîòåêà . ... Ëóíà ON-LINE . ... Êîñìîñ âèäåî . ... Õðîíîëîãèÿ àñòðîíîìèè . ... Ïåðèîäè÷åñêàÿ ñèñòåìà . ... ×àñòóøêè î êîñìîñå . ... Ôîòî äíÿ . ... Ñèìâîëû ïëàíåò . ...
30. Meade Instruments Corporation - Pictor Manual Parts 14 and 15
Home About Meade Product Information Dealer Locator Customer Support Investor Relations Dealer Support Employment Opportunities Site Map . Meade Instruments Corporation . ... Meade Pictor XT-Series CCD Autoguider/Imagers . ... The status bar provides tool tips for each menu item, communication status information, the current x and y coordinates of the mouse on the active image, and the temperature of the CCD chip. (left to right): . ... File Save: Saves the current active image. ... about meade | ...
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Ññûëêè http://www.meade.com/manuals/pictor/pictor14.html -- 12.6 Êá -- 01.02.2006
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31. Gravitational Lensing by Stars
This animation shows a binary star being lensed by a binary lens. ... The sharp changes in the size of the lensed images of the stars lead to sharp changes in the brightness of the stars, which can be analyzed to determine many parameters about the objects doing the lensing, even though they are not bright enough to be seen. ... The graph shown above gives the predicted and observed brightness of a star in the Small Magellanic Cloud being magnified by a binary lens. ... Tutorial : Part 1 | ...
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Ññûëêè http://www.sao.ru/cats/~satr/cosmo/microlensing.html -- 3.4 Êá -- 17.10.2000
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32. 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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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>229) - www.stecf.org/ )
33. Àñòðîíîìèÿ â ÃÀÈØ ÌÃÓ: ó÷åáíèêè ïî àñòðîíîìèè, ôèçèêå: ïåðåìåííûå çâåçäû, êóðñ
... ÈÑÒÎÐÈß ÃÀÈØ - õðîíèêà, ìóçåé, ïåðñîíàëèè, ìåìóàðû, ïåðèîäèêà . Ñàéò "HERITAGE - àñòðîíîìèÿ, àñòðîíîìè÷åñêîå îáðàçîâàíèå ñ ñîõðàíåíèåì òðàäèöèé" îðèåíòèðîâàí íà ñòóäåíòîâ 1 è 2-ãî êóðñîâ àñòðîíîìè÷åñêîãî îòäåëåíèÿ ôèçè÷åñêîãî ôàêóëüòåòà ÌÃÓ è îòðàæàåò ðàíåíèåì òðàäèöèé" îðèåíòèðîâàí íà ñòóäåíòîâ 1 è 2-ãî êóðñîâ àñòðîíîìè÷åñêîãî îòäåëåíèÿ ôèçè÷åñêîãî ôàêóëüòåòà ÌÃÓ è îòðàæàåò ðàáîòó, ïðîâîäèìóþ ñîòðóäíèêàìè ÃÀÈØ ÌÃÓ è ôèçè÷åñêîãî ôàêóëüòåòà ÌÃÓ ïî ðàñøèðåíèþ àñòðîíîìè÷åñêîãî îáðàçîâàíèÿ ñòóäåíòîâ. ...
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>9) - heritage.sai.msu.ru/ )
34. http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf
Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...
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Ññûëêè http://site2010.sai.msu.ru/static/doc/BSafonov_site2010.pdf -- 705.7 Êá -- 18.10.2010
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>222) - site2010.sai.msu.ru/ )
35. http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...
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Ññûëêè http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf -- 346.6 Êá -- 06.10.2008
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>134) - selena.sai.msu.ru/ )
36. Îáñåðâàòîðèÿ
... GRB060712 ( GCN5303 ) The first R image was at 2006-07-12 21:10:32 UT, 72 s after notice time and 212 s after the GRB time. ... HETE Alert 4006 ( GCN 4549 ) - MASTER promt optical limit time . ... GCN 4173 | ... GRB050410 ( GCN 3221 5 h after Swift GRB trigger time . ... GRB05017 ( GCN 2954 19m at between 2h and 4h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . GRB05017 ( GCN 2953 17m at 2h after Swift GRB trigger time (first Swift GRB with X-ray promt observation) . ...
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Ññûëêè http://observ.pereplet.ru/work.shtml -- 14.9 Êá -- 27.02.2014
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>37) - observ.pereplet.ru/ )
37. SAI Space Monitoring Laboratory
Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... All news ...
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Ññûëêè http://master.sai.msu.ru/en/news/?page=7 -- 11.7 Êá -- 09.04.2016
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Åùå â ðàçäåëå:
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38. Bojan Nikolic -- Memo on inference of phase correction coefficients
... Bojan Nikolic web pages home . ... Previous: Visiting ALMA Santiago office and the ALMA.. This is the second memo in the series. ... By observing bright and compact astronomical sources while also taking data with the 183 GHz Water Vapour Radiometers, ALMA will be able to measure the `empirical' relationship between fluctuations in the phase of the astronomical signal and the fluctuations of sky brightness around 183 GHz. ... Copyright 2012, Bojan Nikolic feedback welcome ...
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Ññûëêè http://www.mrao.cam.ac.uk/~bn204/blog/2009/08/memo-on-inference-of-phase-correction.html -- 5.1 Êá -- 22.11.2012
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Åùå â ðàçäåëå:
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39. merkurie
Mercury - is the nearest to the Sun. Ellusive planet. ... They had several names for this star: Set and Gor (ant. ... The same surface spot with many craters, some of which has the systems of light beams only dark spots, like the Moon seas were considerably less. ... Further was the period of intensive bombing Mercury by the remains of before planet’s swarm (planetozimalies), when the ponds were founded for example Colories (diameter - 1300km) as well as craters like Copernic crater in the Moon. ...
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Ññûëêè http://www.space.vsi.ru/merkurie.htm -- 7.8 Êá -- 14.10.2000
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40. http://www.astro-soc.odessa.ua/
... Astronomical Observatory, Shevchenko Park, Odessa, 65014, . ... The XVI -th G. Gamow's Odessa Astronomical Summer Ñînference-School, 14-20 August, 2016, Odessa, Ukraine . ... The XV -th G. Gamow's Odessa Astronomical Summer Ñînference-School, 16-23 August, 2015, Odessa, Ukraine . ... The XIV -th G. Gamow's Odessa Astronomical Summer Ñînference-School, 17-23 August, 2014, Odessa, Ukraine . ... The XIII -th G. Gamow's Odessa Astronomical Summer Ñînference-School, 19-25 August, 2013, Odessa, Ukraine . ...
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Ññûëêè http://www.astro-soc.odessa.ua/ -- 16.6 Êá -- 15.03.2016
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>16) - www.astro-soc.odessa.ua/ )
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