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http://xmm.vilspa.esa.es/sas/8.0.0/doc/implot/node15.html.

21. UCAC2 Bright Star Supplement для Cartes du Ciel - Астрософт
... Астрософт (Модератор: tlgleonid ) > . UCAC2 Bright Star Supplement для Cartes du Ciel . ... Астрософт . ... Cartes du Ciel - Sky Charts . ... 08 Август 2008, 14:04:19 ? Также готов каталог I/294 The UCAC2 Bright Star Supplement (Urban+, 2004), являющийся северным дополнением к каталогу I/289 The UCAC2 Catalogue(Zacharias+ 2003). ... Ответ #1 : 08 Август 2008, 14:41:20 ? ... Самая слабая звезда в каталоге UCAC2 Bright Star Supplement - это 2UCA 50406212 Vmag: 15.19 в Малой Медведице. ...
[ Сохраненная копия ]  Ссылки http://www.astroclub.kiev.ua/forum/index.php?topic=6731.0 -- 62.7 Кб -- 09.04.2016
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22. The Brightest Moon
... Since moonshine is really reflected sunlight, the full Moon is on the average slightly brighter in mid-winter, when Earth is closest to the Sun. In addition, the distance of the full Moon also varies, due to the ellipticity ("eccentricity") of the Moon's orbit. On 22 December, 1999, the two effects combined to produce the brightest full Moon of the century. ... This year will be the first full moon to occur on the winter solstice, Dec. 22nd, commonly called the first day of winter. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/stargaze/Smoon3.htm -- 4.9 Кб -- 13.04.2005
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/stargaze/Smoon3.htm -- 4.9 Кб -- 22.12.2007
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23. ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group
ALMA | ... Phase Correction Algorithms | ... On this page, we describe what the phase correction algorithms set out to do and the framework we have developed to optimally use all of the available information. ... We are developing a Bayesian framework to combine all the information we have about the current and future meterological conditions (which are naturally accommodated as priors in a Bayesian scheme) with detailed physical models of the atmosphere. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/alma/fp6/algorithms.html -- 6.6 Кб -- 29.03.2012
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24. Brightest Pleiads Table
... More Cel no -- 16 Tauri 23288 5.46 B7 IV variable Yes data Electra -- 17 Tauri 23302 3.70 B6 IIIe emiss . line Yes data -- -- 18 Tauri 23324 5.64 B8 V Yes data Taygeta -- 19 Tauri 23338 4.30 B6 IV variable Yes data Maia -- 20 Tauri 23408 3.87 B8 III variable Yes data Asterope 1 -- 21 Tauri 23432 5.80 B8 V variable Yes ... No data -- -- -- 24802 6.19 K0 No data . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/pleiades/pleiades_stars.html -- 4.2 Кб -- 20.11.2005
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25. Classification of Objects in the Guide Star Catalog
... Next: Object Detection Using Up: Object Detection and Previous: Automated Classification of . ... A status report of the The GSC Object Classifier (GOC) project is presented. ... The GSC contains multiple entries for some objects due to plate overlap. It classifies objects as stars, non-stars, galaxies, blends and potential artifacts; the latter three classifications are rare, and only exist in GSC version 1.1, to which they were added manually. ... star, . ... non-star, . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/malkovo1.html -- 10.6 Кб -- 03.11.2000
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26. Procedures for Observations
... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/proc_ob.html -- 7.9 Кб -- 16.02.2000
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27. The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS
... The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS sources with PSPC countrate CR > 0.2 s -1 . ... 1S We present a summary of an identification program of the more than 2000 X-ray sources detected during the ROSAT All-Sky Survey (Voges et al. 1999) at high galactic latitude, |b| > 30degr , with countrate above 0.2 s -1 . This program, termed the ROSAT Bright Survey RBS, is to more than 99.5% complete. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2000_AN_321.html -- 14.9 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2000_AN_321.html -- 14.9 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2000_AN_321.html -- 14.9 Кб -- 02.10.2012
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28. Tilt and Sag Coefficients: 14 Apr 2000
On April 14, 2000 UT a series of Shack-Hartmann measurements were made at varying altitudes. ... The tilts and sags shown are those given by the normal Shack-Hartmann analysis. ... Without this feedback, off-telescope tests showed positioning errors on the order of 10 arcseconds in the secondary mirror position. ... Tilt M2 Bk by X" . ... The coefficients m1 through m3 need to be added to those that are currently in the TCC to correct for the secondary translation with respect to the primary. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/users/morgan/APO/SH_measurements/altitude.sweeps/apr.14.00.init_meas/report.html -- 9.8 Кб -- 29.03.2003
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29. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... Bad Astronomy: The North Star, Polaris, is a very bright star. Good Astronomy: Polaris is a middling-bright star, easily missed. ... He said it was close to Polaris, the North Star, but he also said it was in the East. ... It's natural, I suppose, to think that such an important star should be bright, but really, that's a conceit, like thinking that the Earth is at the center of the Universe. If more people knew just why Polaris is the North Star, this Bad Idea would stop. ...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/bad/misc/badpole.html -- 23.8 Кб -- 09.04.2016
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30. http://hea.iki.rssi.ru/Z-90/arc/24/derishev.pdf
... Particle distribution: dN d - with =1- ln pcn ln g Electron-photon conversion e + _ + _ electron _ e e electron/ positron high- energy photon e+ positron -25 cm cross-section, 10 8 6 4 2 0.5 1.0 center-of-momentum energy , MeV (log scale) 2 e + _ Proton-neutron conversion cm cross-section, 10 proton u +2/3 2 -28 d -1/3 6 u +2/3 4 resonance _ u d d+1/3 -1/3 d u+2/3 +2/3 -1/3 2 150 340 center-of-momentum ... Does the peak (cut-off) energy decrease with observation angle? Not always. ...
[ Текст ]  Ссылки http://hea.iki.rssi.ru/Z-90/arc/24/derishev.pdf -- 232.2 Кб -- 27.12.2004
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31. 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). ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf -- 346.6 Кб -- 06.10.2008
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32. Comet Center of SAI
. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/comet/ -- 2.7 Кб -- 17.06.2012
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33. http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/i/inxs/keep_the_peace
Hey y'all... these are the lyrics to "Keep the Peace," the INXS song off the Beverly Hills Cop III Soundtrack. ... Dancing in the light, Shadows fall from you, Learn to watch your step - You come falling In my arms again, in my heart again, You will break like a butterfly Keep the peace for what you're talking, Keep the Peace , Keep the Peace Walk of fame is where you're walking, Keep the Peace , Keep the Peace Keep a hold of what you're taking, Even though the ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/i/inxs/keep_the_peace -- 2.6 Кб -- 01.12.1994
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34. 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 . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/hyakutak.htm -- 5.3 Кб -- 15.10.1997
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35. SAI Space Monitoring Laboratory
Lab . Main page News People . ASA . Master . Master net Homepage . ... MASTER . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... 10.08.2011 . ... All news ...
[ Сохраненная копия ]  Ссылки http://master.sai.msu.ru/en/news/?page=10 -- 11.4 Кб -- 09.04.2016
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36. Digistar 4 Planetarium Projection System in Action | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium is leading the way in the digital theatre world with the installation of our brand new Digistar 4 Theatre System .€а This marks the first installation of the worldтАЩs most advanced star theatre system in the UK, enabling audiences to see the Cosmos like never before. ... Armagh Planetarium was the first in the world to use video projectors to show moving images on the dome. ... тАЬDigistar 4 Planetarium Projection System in Action | ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/digistar-4-comes-to-armagh.html -- 46.7 Кб -- 09.04.2016
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37. http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/921030.htm
October 30-31, 1992 . ... Modified images of the October 30-31, 1992 event. (a) - This NRH image is adapted to show a very bright loop-like source over AR 7321 near the SW-limb identified with the X1.7 soft X-ray LDE event peaked on 30d at 17:30 UT (see the GOES-7 soft X-ray plot also at the upper right corner). ... Here and hereafter, the white features are radio filaments. (c) - This modified NRH image shows some large scale microwave blob chains and structures. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/921030.htm -- 3.3 Кб -- 02.04.1999
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38. Other Useful Functions
. Next: *tprint* - Reading a Up: *imexamine* - General analysis Previous: Contour Plot . Some other useful functions which also give graphical results are: . r gives radial plot of surface brightness. c (column) gives brightness in a vertical slice through the cursor. l (line) gives brightness in a horizontal slice through the cursor. rsdc@cfa.harvard.edu . 1998-06-10
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node98.html -- 3.3 Кб -- 01.10.2012
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39. http://www.gao.spb.ru/database/csa/corona/cor_fmt_e.txt
Solar corona data format (up to June 1957) 1-4 Year 6-7 Month 9-13 Day (with fractional part) Data in line 5303 Angstroem : 15-17 Latitude of the radiation center ( 999 =no data ) 18 Limb (E= east , W=west) 20-21 Basis of the luminous zone, in degrees (99=no data ) 23 Brightness in 6-grade scale, or 0 ( brightness is below threshold), or 9 (no data ) Data in line 6374 Angstroem : 25-27 ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/database/csa/corona/cor_fmt_e.txt -- 1.7 Кб -- 21.05.2007
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40. Общая Астрономическая Конференция - Показать сообщение отдельно - Хвостатые
Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Хвостатые гостьи .. ... после того, как ISON приплыл мимо нас, земля находится на орбитальной траектории, которая пройдет через след частицы кометы (тот, который ISON оставил позади, когда это приближалось к солнцу и это случайно встретит или вокруг 12 января - 15, 2014 . ... лучшее время наблюдения 22:00 LDT (Northern hemisphere 45њ North) .. - радиант расположен вблизи Al'dzhabkhakh (30-Eta Leonis, ? ...
[ Сохраненная копия ]  Ссылки http://www.starlab.ru/showpost.php?p=135258&postcount=25 -- 21.6 Кб -- 12.04.2016
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