... January . February . March . April . ... November . December . ... April ((April Fools)) . ... April (Star Party Reports) . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...

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• Automated Spectral Classification Using Neural Networks
• An Approach for Obtaining Polarization Information from COBE-DMR
• Substepping and its Application to HST Imaging

Statistics of sunspot activity . The sunspot indices . ... The solar regions . ... 1998 . ... September . ... September, 1998 . Visual indices of solar activity by author's observations . ... Average . ... 100 . ...

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• The Sunspot Observer - Average annual indices of solar activity NGDC -

What is a Handler . ... mod_actions . ... A "handler" is an internal Apache representation of the action to be performed when a file is called. Generally, files have implicit handlers, based on the file type. Normally, all files are simply served by the server, but certain file types are "handled" separately. Apache 1.1 adds the ability to use handlers explicitly. ... The following directives will enable the send-as-is handler, which is used for files which contain their own HTTP headers. ...

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• Starting Apache
• Module mod_cern_meta
• Apache module mod_auth_digest

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• XV-MULTI
• XV-IMAGE

June 1, 1998 . ... An example of the EUV chain revealed by the modified SOHO/EIT images. ... The chains on the 171 ( a) and 195 A (b) images are very similar, but there are some differences on the 284 A image (c) . ... A comparison of the large-scale chains and threads on the modified SOHO/EIT (195 A) image (inverted) and two He I (10830 A) images (normal). ... SOHO/EIT, 171 A, June 01-03, 1998 GIF Animation (670 KB) . SOHO/EIT, 195 A, June 01-03, 1998 GIF Animation (1.76 MB) . ...

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• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/971216.htm
• Large_Scale Emitting Chains

Supernova 2002dv and 2002eg in UGC 11486 . This page is devoted to information on Supernova 2002dv and Supernova 2002eg in UGC 11486 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . ... Ella Sanders discovered this one, the thrid double SN in four months, almost a stastical impossibility. ... SNWeb has a 2002dv page . ... Ella Sanders 2002eg images page 1 and 2002eg images page 2 . ... 2002/07/01.4 . ... Ella Sanders image . ...

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• Supernova 2006en in MCG +05-54-41
• Supernova 1999gq in NGC 4523
• Supernova 1998eg in UGC 12133

Hunger is a simple feeling: when your body needs some energy for normall and full functioning, our brains just senda few signals and we begin looking for something to eat.. The great majority of scientists say that the right way of eating is when you begin sating when you really want, and end this process when the feeling of hunger disappears. ... The problem is redoubled with the fact that some people try to suppress negative feelings with effective and easy method. ...

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Университет . ... Информация Руководство и преподаватели Гоголева Софья Юрьевна . ... Публикации . ... Самарский государственный аэрокосмический университет имени академика С.П. Королева . национальный исследовательский университет)" . ... Тел.: 846) 335-18-26 Факс: (846) 335-18-36 . ... Тел.: (846) 267-44-99 . e-mail: pr@ssau.ru . ... тел.: +7 (846) 267-48-21, . e-mail: tech@ssau.ru . Работа корпоративной сети университета: . ... СГАУ 2016 http://ssau.ru | http://сгау.рф | ...

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• Федина Мария Ефимовна. Публикации
• Федотов Юрий Аркадьевич. Публикации
• Завершинский Дмитрий Игоревич. Публикации

Прохождения БКП . через центральный меридиан Юпитера . в сентябре 2003г: . ... В указанные моменты времени вы увидите Большое Красное Пятно вблизи центра диска Юпитера. Это уникальное образование в атмосфере планеты легко доступно наблюдениям в пределах +/- полутора часов от указанного момента. ... Астрокалендарь | ...

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• Jupiter Red Spot September 2004

... Bad Astronomy . ... Mad Science . ... Site Info . ... Public Talks . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Who is this guy who calls himself "The Bad Astronomer?" ... First, yes, I am a real live astronomer (when people ask me what astronomers do, I tell them "They astronom !" ... These are emitted by powerful objects like black holes, exploding stars, and super-dense neutrons stars. ... Finally, am I really a bad astronomer? ... 2008 Phil Plait. ...

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• Phil Plait's Bad Astronomy: Mad Science
• Phil Plait's Bad Astronomy: Brains on Vacation
• Phil Plait's Bad Astronomy: Misconceptions: The Planet X Arguments in a...

. Prague, August 16, 2006 . Present classification : Suggested: . SN, SNI, SNII SN (to avoid introducing the current complex classification) AM AM (including XM from X-ray variables), DQ (intermediate polars) . UG, UGSS, UGZ UG, UGSS, UGZ UGSU UGSU, UGWZ (WZ Sge type, extremely long supercycles, large amplitudes), UG_ER (ER Uma type, short supercycles and normal cycles, small amplitudes; ideas of a better abbreviation are welcome) . CATACLYSMIC VARIABLES . AND OTHER STARS WITH OUTBURSTS (CONTINUED)

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... 2. ui , i- , : 5 ui = ( - sin cos i cosi - cos i sini T ), i (1) i ­ i- OYZ; i ­ i- OYZ, i = 225 - 90 i, i = 1,.. ... 6 max ( L1 , L2 ) nmax = min ( L1 , L2 ) ( nmax + 1) , nmax = min ( L1 , L2 ) max ( L1 , L2 ) - min ( L1 , L2 ) - . ... 3) D1min1 , D1min 2 7 mi n1min1 , n2 n1 , min 2 min 2 n1 , n2 , Dlast . ... 11) OX OXY : nxy = nijk - ( nijk , ez ) ez , (12) ex , ey , ez ­ . ... nxy , ex ) ( , ( nxy , ex ) < 0 -arccos nxy (13) OX OXZ : nxz = nijk - ( nijk , ey ) ey . ... 450 B2 (+225 ) B1 (-225 )...

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Unno, W. Line Formation of a Normal Zeeman Triplet http://adsabs.harvard.edu/abs/1956PASJ.. ... 108U Moe, Olav Kjeldseth A Generalized Theory for Line Formation in a Homogeneous Magnetic Field http://adsabs.harvard.edu/abs/1968SoPh.. ... 24S Landi Degl'Innocenti, Egidio; Landi Degl'Innocenti, Maurizio Quantum Theory of Line Formation in a Magnetic Field http://adsabs.harvard.edu/abs/1972SoPh.. ... 235H Sazonov, V. N. Polarization in Zeeman-split absorption lines http://adsabs.harvard.edu/abs/1975SvA.. ...

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