... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...

... 2000 July 7 . Sirius, Sun, Moon, and Southern Cross . Credit: European Southern Observatory (ESO) . Explanation: From left to right are the enclosures of Yepun ( ye-poon ; Sirius ), Antu ( an-too ; Sun ), Kueyen ( qua-yen ; Moon ), and Melipal ( me-li-pal ; Southern Cross ), pictured here as night falls at Paranal Observatory in northern Chile. These are the four 8.2 meter wide telescope units of the European Southern Observatory's Very Large Telescope (VLT). ... About APOD | ...

... In a solar prominence, charged particles stream up from the Sun, spiraling around magnetic field structures poking out of the solar surface, and ultimately fall back along those structures into the Sun. ... As evolution would predict, animals' eyes sense the colors of light emitted most strongly by the Sun. ... The tiny Moon can completely cover the disk of the Sun, blocking most of the emitted visible light, and reveal the Sun's faint outer atmosphere called the corona...a mass of incandescent gas ...

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

... SAI CAS . ... Catalog Access Services . ... This site is about the Virtual Observatory project at the Sternberg Astronomical Institute, Moscow University ( SAI MSU ). We provide a public access to the growing set of astronomical services developed by the SAI RVO development team in accordance with the Virtual Observatory standards. ... We provide access (programmatic and interactive) to the all major and biggest astronomical catalogs (about 4 billions objects total) as well as other web-services. ...

... The evolution of magnetic fields in OB-type stars from the study of open clusters of different ages . ... Wade G. A. The MiMeS Project: Magnetism in Massive Stars . ... Polosukhina N., Shavrina T., Drake N., Kudryavtsev D. Smirnova M. New results of the spectral observations of CPstars in the Li I 6708? spectral region with BTA telescope of SAO RAS . ... Magnetic Stars-2010 . ... List of participants . List of reports . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

Optical Observatories . ... National Optical Astronomy Observatories . ... Adam Mickiewicz University - Astronomical Observatory . ... Astronomical Institute and National Observatory of Athens . ... Jagiellonian University Astronomical Observatory - Scientific research here comprises radio and extragalactic astronomy, solar radio emission, active galactic nuclei, interstellar matter, galaxies, cosmology, variable stars and comets. ... National Radio Astronomy Observatory Home Page . ...

The Chandra X-ray Observatory is the third of NASA's four " Great Observatories ", and is used by Astronomers to study some of the more extreme objects and events (in terms of temperature and mass) in the Universe. ... This page uses Javascript to show you the timeline for Chandra, NASA's X-ray Observatory. ... If you can not enable Javascript, much of the information is available at the Chandra X-ray Center . Further information on Chandra can be found at: . ... The Chandra X-ray Center . ...

. The XMM-Newton website has moved to the following location: . http://www.cosmos.esa.int/web/xmm-newton

CATS home ] [ Back to CATS list ] [ ftp ] . ... 117.1578Bock+ The Molonglo Observatory Synthesis Telescope, operating at 843 MHz with a 5 deg^2 field of view, is carrying out a radio imaging survey of the sky south of declination -30 deg. This survey (the Sydney University Molonglo Sky Survey, or SUMSS) produces images with a resolution of 43"x43" csc|delta| and an rms noise level of ~1 mJy beam^-1. ... See also MGPS2 Galactic plane survey. ...

... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...

The IAA RAS . ... View details . ... Observatories 'Svetloe' and 'Zelenchukskaya' participate in frequent VLBI-observation sessions organized by the International VLBI Service for Geodesy and Astrometry . ... As part of collaboration with the U. S. Naval observatory in the areas of EOP determination and analysis the USNO uses IAA RAS daily EOP data obtained from SLR and VLBI. ... The IAA RAS and the Centre National d'Etudes Spatiales carry out joint DORIS observations on the Badary observatory. ...

SAO is Russia's main centre for ground-based space research. ... The basic instruments of the Observatory are the optical telescope BTA (Big Alt-azimuth Telescope) with a main mirror diameter of 6 m and the radio telescope RATAN-600 with the antenna diameter 600 m. Study of the Universe as a whole, analysis of non-stationary energy release in galactic and extragalactic objects of various types, investigation of evolution and chemical composition of our Galaxy and the nature of solar activity. ...

Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 04 - 10.07.2011, Forecast on 11 - 18.07.2011, Carrington Rotations 2112 (03,01.07.2011) SOLAR SUNSPOT ACTIVITY OF THE LAST PERIOD KEPT CLOSE TO LOW AND MIDDLE LEVELS. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE VALUE. ... FLARE ACTIVITY WAS AT LOW ONLY JULY 7-8, AND AT A VERY LOW ON OTHER DAYS. ... NEXT WEEK GEOMAGNETIC CONDITIONS WILL MOST PROBABLY REMAIN QUIET TO UNSETTLED. ...

Главная Сотрудники Публикации Инструменты История Наблюдения . ссылки по теме "физика Солнца" . ... Патрульные наблюдения Солнца . на ГАС ГАО РАН . ... ИКИР ДВО РАН . ... Уссурийский район, . ... Уссурийская астрофизическая обсерватория ДВО РАН создана в 1953 г. (станция Службы Солнца) для регулярных наблюдений Солнца и солнечной активности. ... В составе обсерватории функционируют три научно-исследовательских лаборатории: . Лаборатория солнечной активности и солнечно-земных связей; . ...

. WIN-1251 . Agafonov B.I. major electronic engineer . Aleshkov V.M. major electronic engineer . Grigoriev V.A. electronic engineer . Zavorin A.V . head of observafory . Kraschuk P.A. electronic engineer . Lytkevich V.V. major electronic engineer . Pasechnik L.A. electronic engineer . Prihodjko N.A. major electronic engineer . Shenhorov N.D. electronic engineer . Mail: rp@iszf.irk.ru . WIN-1251

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Winer Observatory) was incorporated in 1983 as a 501(c)(3) non-profit public charity to perform basic research in astronomy, provide educational outreach programs, and provide site and maintenance services for small telescopes through cooperative agreements with other astronomical institutions. ... The picture at the top left of this page is of our facility near Sonoita, Arizona, approximately 50 miles southeast of Tucson, Arizona. ...

... Alexander Gusev, Sternberg Astronomical Institute . Andrei Tokovinin, National Optical Astronomy Observatory . ... Antonia M. Varela, Instituto de Astrofisica de Canarias . ... Behnam Javanmardi, Shiraz University-Biruni Observatory . Boris Safonov, Sternberg Astronomical Institute . ... Davoud Afshari, Zanjan University . ... Florian Kerber, European Southern Observatory . Gianluca Lombardi, European Southern Observatory . ... Hiroshi Matsuo, National Astronomical Observatory of Japan . ...

. Institute Structure . • Administration . • Research Divisions: . Superhigh energy particles . Space plasma physics . Aeronomy . • Center of information technology . • Stations: . Yakutsk Extensive Air Shower (EAS) Array . Polar Geocosmophysical Observatory (PGO) . Complex Geophysical Station (CGS) . Optical Station . Yakutsk Cosmic Ray Spectrograph . Magnetic Observatory . Ionospheric Station . Station for Receiving of Satellite Information .

. When a UHECR with energy above 10 19 eV hits Earth's atmosphere, it creates an "air shower" of particles. Here, red corresponds to muons, yellow to photons, and purple to electrons and positrons. This computer simulation overlays an image of the site of the Pierre Auger Observatory — a UHECR detector in Argentina. Cosmus at University of Chicago: Randy Landsberg, Dinoj Surendran, and Mark SubbaRao