... 8, ``Celestial Mechanics'', 2002 The ephemerides server of the Institut de m'ecanique c'eleste et de calcul des 'eph'em'erides N. Baron, J. E. Arlot Institut de m'ecanique c'eleste et de calcul des 'eph'em'erides, Paris, France The Institut de m'ecanique c'eleste et de calcul des 'eph'em'erides (IMCCE), formerly known as Bureau des longitudes, produces, since its creation (1795), the French ephemerides for most of the bodies of the solar system. ... The code of several theoretical models is provided...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/ZAMAR.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/FOMINOV.PS
• Keywords_189

Next: Polarization efficiency: size/shape/orientation effects Up: Optical properties of cosmic Previous: The 2175? feature . To model the interstellar polarization one needs to calculate the forward-transmitted radiation for an ensemble of non-spherical aligned dust grains. ... Let non-polarized stellar radiation passes through a dusty cloud with a homogeneous magnetic field. ... The angle between the line of sight and the magnetic field is ( ). ... where the angle is connected with and ( ). ...

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• Linear polarization: wavelength dependence
• Database of Optical Properties -- Level: subpage
• Amorphous magnesium silicate

Multiple Supernovae in the same galaxy . ... When looking at these images, you should note just how big these galaxies are. ... SN 2009as and sn2009gb images sub-page . ... LOTOSS discovered 2003hl , and a few weeks later JM Llapasset was taking an image of it, and he noticed a new star . ... Supernovae 2002cv and 2002bo in NGC 3190 2002cv was discovered by Campo Imperatore Observatory while observing 2002bo in IR. 2002cv was only visible in IR must likly due to it being behind a dust lane. ...

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• Supernova 1998eg in UGC 12133
• Supernova 2002hh in NGC 6946

Date: Mon, 1 Jul 1996 16:03:06 -0700 (PDT) From: Alexei Kosut <akosut@organic.com> To: Apache Group Subject: Re: keepalive and windoze Good news and good news (of a sort).. I was able to snag a Windows 95 machine here at Organic, and tried out some things: 1) On Netscape 3.0b4, I was able to reproduce the bug, each and every time. ... Alexei Kosut <akosut@organic.com> The Apache HTTP Server http://www.nueva.pvt.k12.ca.us/~akosut/ http://www.apache.org/ . ...

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• Custom error responses

... In the Sun-Earth system these are the impulses of the solar activity and the processes in the Earth atmosphere. ... However only recently we succeeded to prove that the weather anomalies and even that of climate are noticeably connected with the variety and diversity of the solar activity. ... All these particularities are specific for the convection zone and extremely important for the whole “life” of the Sun because they are the main causes of the Solar Activity . ... What is the Solar Activity? ...

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• Y.Kupryakov, SAI, MSU
• jg0043
• Список публикаций Пасынка С.Л.

Journal of the Amateur Astronomers Association of New York March 2010 Volume 58 Number 3, ISSN 0146-7662 EYEPIECE will save significant weight. ... The JWST will be a very large space telescope. ... March 28 Moon at perigee, 224,859 miles from Earth, 12:59 a.m. March 29 Moon lies near Saturn; full Moon at 10:25 p.m. 2 Mars and Moon Shone Bright By Joseph A. Fedrick During the nights of January and the first half of February, Mars and the Moon shone bright, although the frost was cruel. ...

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• http://www.aaa.org/EyepieceFiles/aaa/2008_04_April_Eyepiece.pdf
• Amateur Astronomers Association of New York ? Amateur Astronomers Association

Общая Астрономическая Конференция > Практика > Астрономические наблюдения > Полярное сияние! Взгляды на небо! ... Просмотр полной версии : Полярное сияние! ... Только что мне позвонил Стас Короткий и сказал, что над Москвой наблюдается полярное сияние, и притом разноцветное. ... В Питере с 18-го по 31-ое марта стояли ясные ночи (и какие ночи - сказка!), а ночь 31.03/01.04 как раз зятянуло напрочь http://www.starlab.ru/ubb/frown.gif Думается, и над нами могло бы быть. ...

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• Новая серия телескопов от целестрона!! [Архив] - Общая Астрономическая
• Полярное сияние! Взгляды на небо! - Общая Астрономическая Конференция

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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... Using the CFBDSIR wide field survey for brown dwarfs, we identified CFBDSIRJ214947.2-040308.9, a late T dwarf with atypically red J-Ks colour. ... SN 2009ip in NGC 7259 Electronic Telegram No. ... 7.09, [19.0; 2009 Aug. ... Accepted for publication in MNRAS Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) The jet opening angle theta_jet and the bulk Lorentz factor Gamma_0 are crucial parameters for the computation of the energetics of Gamma Ray Bursts (GRBs). ...

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• http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf

Report on the work done in 2015. ... Namely, it concerns a result from 2006 that was my first work on cyclic homology in positive characteristic -- a proof of Kontsevich-Soibelman Degeneration Conjecture. The conjecture asserts that for a smooth and proper DG algebra over a field of characteristic 0 , the non-commutative Hodge-tode Rham spectral sequence degenerates (if the DG algebra is Morita-equivalent to an algebraic variety, this is the standard Hodge-to-de Rham degeneration). ...

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• Conference "Flows on surfaces, symbolic dynamics and dynamics in moduli spaces"
• Books (Latin j), sorted by title
• IUM10 conference: A.Gorodentsev

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA ETC - Exposure Time Calculator
• Use of the (UK) VISTA Data Flow System

MICROSCOPES . ... In the last three to five years, LOMO has developed new lines of products, including new families of biological, fluorescent, and polarizing microscopes, night vision devices, consumer Maksutov telescopes, etc. ... 1939 Company introduces its first student and biological microscopes. as well as its first manual movie camera . ... 1956 LOMO produces its first wide-screen-format movie projector and introduces its first fluorescent microscope for chemical structure analysis. ...

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• Professional Telescopes
• OEM Optical Components

To the Deputy Head of the Administration of Russian Federation President Mr. A.V.Ogarev . ... First the international space station (ISS) Alpha, which is under construction now, will compare to the OS Mir on the amount of information only in 5-7 years. ... Thirdly, the participation of Russian Federation in the international space projects, including work on the international space station (ISS) Alpha, is to be aimed first of all at the providing of Russian interests. ...

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• News of Cosmonautics - August, 2002 | Russian Space News | CosmoWorld.ru
• News of Cosmonautics - May, 2002 | Russian Space News | CosmoWorld.ru
• Carrying out of the experiments on the orbital station MIR

... Solanki S. K. Small-scale solar magnetic fields: An overview // Space Sky . ... Fe I 5247,1 5250,2 е, Fe I 6301,5 6302,5 е. ), . ... Lvm 5250 , 6301 ­ . ... k, rv- (rvw), rv- - (rvf). , rvo = rvf + k* rvw, rvo ­ . ... 2 , Lvm, [6] е 5247 40,5 5250 58,5 6301 67 6302 73 Lvm, [5] 40,8 40,8 64,8 58 Lvm, k=0,8 40,8 53,2 65,5 65 Lvm, k=-0,8 39 61,2 69,5 80 Lvm, k=3,0 40,8 44,8 65 61 Lvm, k=-3,0 27,2 53,5 65,2 49,5 80 86 If*f, rvo = (rvf + k*rvw)/ [1 + (1-f)/f *Ip/If], k = (Ip*p)/(If*f) = 0,72p/f (3) (2) ....

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... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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• Katsova Livshits poster paper on CS-11
• Elena Seifina
• Nikolay Bochkarev

... Рябов Б.И., Максимов В.П. О возможности обнаружения особенностей структуры коронального магнитного поля// Труды Международной конференции по физике Солнца 'Структура и динамика солнечной короны/' 4-8 октября 1999г, Троицк: ИЗМИРАН, 1999, с. 137-143. ... Международная конференция по физике Солнца 'Структура и динамика солнечной короны', 4-8 октября 1999г., г. Троицк, с.290-294. ... Международной конференции по физике Солнца 'Структура и динамика солнечной короны', 4-8 октября 1999 г., г. Троицк, 1999...

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• Radioastrophysical Observatory ISTP RAS SB

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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• Mid Scales Role

... In the course of the BURAN orbiter development, suborbital and orbital launches of BOR-4 and BOR-5 flight vehicles have been produced for aerodynamic analysis and working capacity of thermal protection structures verification. ... The flights of the SPIRAL prototype and BOR-4 and BOR-5 flying vehicles have allowed not only to speed up the BURAN orbiter development, but also to justify the choice of the aerodynamic scheme of the orbital stage of the advanced MAKS aerospace system. ... Buran Orbiter ....

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• Molniya-1 Triplane Aircraft

... This is usually defined as the direction pointing toward the center of the primary body. ... NODE: The place where the plane of one orbit crosses the plane of another. ... ORBITAL PLANE: The flat surface that would result if every point on the orbit of a body was connected to the center of its primary. ... PENUMBRA: The edge of the primary body's shadow. ... PERIOD : The time required for one body to orbit the primary body. ... PROBE: A vessel designed to pass and observe an astronomical object. ...

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• Surface Features of Earth's Moon and Mars
• Astronomical Glossary - J thru M
• RAS Glossary A to C

MUON METHOD FOR A MATTER STUDYING Yu. ... З МТЪУflВВ , ВПfl ПУММњИ ПВЪУ Оfl ЩЛБЛНЛ Л iЛПЛЛ НУМВМТЛУ,ММњi Л ,,БУУћ БМњi ЩБ ЛПВВЪ ЪНУВ КВ БМ~ВМЛВ, НН ПВЪУ flВ МУ,,У П,,МЛЪМУ,,У ВБУММТ ЛОЛ ПfiТТћЫУ,ТНfl ,,ПП-ТФВНЪ УТНУФЛfl. ы. е. ЕЦгймлйЗ, З. и. леагЙД еУТНУ,ТНЛИ ЩЛБЛНУ-ЪВiМЛ~ВТНЛИ ЛМТЪЛЪЫЪ, СУО,,УФ ЫМњИ еУТНУ,ТНУИ УћО. ЗЗЦСЦзаЦ 76 ї ЕВОУЫТУ, ы.е., лПЛО,, З.и., 1999 : ( ), , , чSR-, , . чSR . ... ЕЦгймлйЗ ы.е., леагЙД З.и. унй нДдйЦ еыйззхв еЦнйС аллгЦСйЗДзаь ЗЦфЦлнЗД 77 M mr. : . ... 3) : cos | ...