... Proximity e#ects of com­ ponents (reflection of radiation and surface gravity darkening) are taken into account. ... As an example, we consider the Algol (# Persei) system, where an eclipsing pair (Algol A­B) is accompanied by the third component (Algol C). ... The surface temperature distribution for Algol A­B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation e#ect. ... We solve this equation by the iterative Newton­Raphson method. ...

. M. Prohorow, S. Kuranow . D. Kosenko stand . against background . of Donguz-Orun . At the mountain . Cheget . From the mountain . Cheget . Return from Azau . Walk with Darja Kosenko . along Cheget Slopes . Into Andyrchi to the . Ga-Ge-neutrino-detector . Scintillator-detector . W. Lukash, M. Prohorow, . D. Kompaneetc and i were . waiting for airplain . The day of waiting . for airplain . The Great Seven

Measurement of Sky Brightness at the Iranian National Observatory Davoud Afshari1 and Sadollah Nasiri1,2 1Physics Department, Zanjan University, Zanjan 45195-313, Iran; Institute for Advanced studies in Basic Science (IASBS), Zanjan 45195-1159, Iran; Measurement of light pollution 2 Introduction Among 34 candidate sites at the central part of the country, 5 sites namely Garkesh (in Kashan ), Kolahbarfi(in Kashan ), Deynava (in ... One of these is light pollution. ...

Stellarium 0.12.3 . ... FileљStructure . ... varstar Struct Reference . QStringљ . ... Magnitude at maximum brightness. ... Magnitude flag code. ... First minimum magnitude or amplitude. ... Second minimum magnitude or amplitude. ... The photometric system for magnitudes. ... Definition at line 41 of file StarMgr.hpp . ... QString varstar::photosys . ... QString varstar::stype . ... QString varstar::vtype . ... The documentation for this struct was generated from the following file: . ...

... OF ROCKET SPACE TECHNOLOGY DEVELOPMENT . OKB1 - TSKBEM - NPO ENERGIA - S.P.KOROLEV RSC ENERGIA . 1961-1968 . ... April 26, 1962 . Launch of the Zenith satellite to take pictures of the earth's surface. ... Launch of the Mars-1 unmanned interplanetary station that reached the Mars area on June 19, 1963. ... 1946 - 1949 1950 - 1957 1957 - 1959 1959 - 1961 1961 - 1963 1964 - 1966 1967 - 1969 1971 - 1977 1977 - 1982 1986 - 1987 1987 - 1990 1992 - 1998 1998 - 2000 2000 - 2001 2001 - 2008 . ...

. Начало | Зеркало | Реклама | Анекдоты | Имена | Отчества | Календарь | Новости | Фильмы | Стихи | Фото | Песни | Сайты | Альбомы | Архив . Искусство | Семья | Финансы | Медицина | Военные | Наука | Спорт | Государство | Бизнес | Техника . Регистрация . Вход . Поиск . Сегодня 9 Апреля Суббота a б в г д е ж з и й к л м н о п р с т у ф х ц ч ш щ э ю я a b c d e f g h i j k l m n o p q r s t u v w x y z . Биография . Фотографии [0] . Тройня в 55-летнем возрасте . Посетило:393 . Ливерпульская версия Памелы

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Possibilities of observing . ... Investigations of the SSRT 5.7 GHz radio maps in conjunction with images obtained in other emission ranges, suggested the following conclsions: . ... Solar images obtained in line H a ;(on the left, 16:11 UT, Big Bear observatory) and in the microwave emission (on the right, 04:04 UT, SSRT) 4 march 1997 . ...

... 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 . ...

... SB, Porb = 55.9212d. V0745 Cas| ... Component B of the double system observed brighter than in the Hipparcos Input Catalogue. ... The variability may be due to the fainter component. ... Type ELL: is also possible. pi Cas| ... Variability type and spectral type (F2/F3Ib/II) do not agree. ... Variability type and spectral type (F3/F5II) do not agree. ... Variability may be due to component B. VZ Pic| ... Variability may be due to component B. V1377 Ori| ... SB, Porb = 9.073d. V0421 Cep|105091| ...

... Now comes a remarkable opportunity for all AAAP members to learn more about our closest star-- straight from a leading figure in solar physics and expert on solar eclipses. Dr. Fred Espenak from the NASA Goddard Spaceflight Center will present Predicting and Chasing Solar Eclipses at a special lecture on March 30. ... Information about future solar eclipses visible from Princeton will be distributed at this event, at which the public is also welcome (bring your kids too!) ...

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... 12 Oct 02 2006 1.9 Jan 26 2006 8 CB,CS,R=F. R=G, SMALL, TIGHT, BRIGHT NGC 1912 M38 17mmAT 2012 M.M . Open Cluster 8.0 II 2 r CL,B,VL,VRI,IF,STL$S Mar 16 2012 18 Mar 01 2011 12 Mar 08 2010 12 Dec 16 2009 12 Mar 20 2009 16 Mar 17 2007 1.9 17mmAT M.M . 2011 - MANUAL SETTING CIRCLES M.M . 2010 MANUAL SETTING CIRCLES 26mm 20mmUW MESSIER MARATHON - 2009 26mm ...

University Satellites and . Space Science Education . ... SYSTEM OF MEASUREMENT OF THE CHARGE S/C Foton-M #2 . ... The charging of the space vehicles and their elements leads to failures of an electric equipment. ... The charging of S/C occurs as a result of influence on its surface of some the factors, in particular surrounding space plasma and solar electromagnetic radiation. ... Skobeltsyn Institute of Nuclear Physics, Moscow State University, 2005-2006 . ...

. Download Izmccd (~2.7 MB). Viewing of image. Use the following functions of the program for viewing an image: . 1) Increase/decrease of scale. For this purpose, press / on the toolbar; and click on any place of the frame. There will be a change of scale. Besides the image will be centred on this place. 2) Increase/decrease of brightness is made by buttons / , or through adjustment of values of a background and range. This is the  button. 3) Mode of a negative is . Previous Next . Main page

... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...

... Status of spherical tokamak Globus-M, Proc. International Congress on Plasma Physics and 25th European Physics Society Conf. ... Globus-M experiment at the final stage of preparation, Proc. 17th IAEA Fusion Energy Conf. ... Globus-M spherical tokamak, Techn. ... First plasma experiments on spherical tokamak Globus-M, Proc. of EPS-27 Conf. on Contr. ... Plasma Formation and First OH Experiments in Globus-M Tokamak, Proc. 18 IAEA conf on Fusion Energy, 4-10 October, 2000, Sorrento, Italy, EXP1/03 . ...

Электронная библиотека астронома-любителя. ... библиотека . архив RSN . ... Ru.Space.News: . Март 1998 . ... Дата: 11 марта 1998 (1998-03-11) От: Alexander Bondugin Тема: Ed Massey Named Voyager Manager Привет всем! ... Дата: 11 марта 1998 (1998-03-11) От: Alexander Bondugin Тема: Cassini Update - March 6, 1998 Привет всем! ... Дата: 11 марта 1998 (1998-03-11) От: Alexander Bondugin Тема: Sky Telescope News Bulletin - March 6, 1998 Привет всем! ... Clear skies! ...

... 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. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

... Shareable data center . ... Experimental research on ionospheric disturbances of natural and technogenic origin, and on the transionospheric propagation of decimetric radio waves, based on processing data from the global network of two-frequency receivers of the GPS-GLONASS navigation systems . ... Estimation of the sensitivity of the method of global integration at the detection of an ionospheric response to faint solar flares and disturbances of non-solar origin (supernova explosions). ...