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http://www.sao.ru/cats/~satr/RFSymp/abs/28_Riehokainen.ps.
http://www.sao.ru/cats/~satr/RFSymp/abs/28_Riehokainen.ps.
1. http://www.sao.ru/cats/~satr/RFSymp/abs/28_Riehokainen.pdf
MULTI-FREQUENCY OBSERVATIONS OF THE POLAR RADIO STRUCTURES A. Riehokainen1 , A.G. Tlatov 1 2 2 Tuorla Observatory 21500, Piikkio, Finland; Pulkovo Astronomical Observatory, St. Petersburg, Russia alerie@utu.fi In this work we present a comparison of the enhanced temp erature regions (ETRs) in the radio emission of the Sun with other manifestations of solar p olar structures over some days in 2003-2005. ... We compared our radio data with different SOHO/EIT and SOHO/MDI images for the same p erio ds. ...
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Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/28_Riehokainen.pdf -- 17.6 Кб -- 09.10.2006
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2. Pulkovo Observatory
. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.
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3. National Astronomy and Ionosphere Center (Arecibo Observatory)
. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."
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4. Bright prospects: Comparing the H Survey with large-scale radio continuum
... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Australia Telescope 20GHz Survey . ... Bright prospects: Comparing the H Survey with large-scale radio continuum emission . ... Prospects for comparisons between the AAO/UKST H \ survey and large-scale radio continuum emission are considered, with particular reference to the recently completed Parkes 2.4-GHz survey of the southern Galactic Plane. ...
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Ссылки http://www.atnf.csiro.au/pasa/15_1/duncan/paper/index.html -- 52.4 Кб -- 08.04.2016
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5. Sternberg Astronomical Institute
SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...
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6. Astronomical Society
... Donate to Support Science Literacy . ... 2016 Annual Awards . The ASP is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach. ... Shop the AstroShop . ... The Astronomical Society of the Pacific (ASP) is accepting nominations for the organizationтАЩs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach.. ...
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Ссылки http://www.astrosociety.org/ -- 49.2 Кб -- 09.04.2016
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7. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... A sketch for the active region model on ultracool dwarfs. ... An active region model was built, based on the rotation of the UCD and the ECMI mechanism. ... The active region model is applied to the radio emission from TVLM 513-46546, in which the ECMI mechanism is responsible for the radio bursts from the magnetic tubes and the rotation of the dwarf can modulate the integral of flux with respect to time. ...
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Ссылки http://star.arm.ac.uk/highlights/2010/567.html -- 6.8 Кб -- 08.09.2010
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9. The Brightness of the Night Sky
The night sky brightness, together with number of clear nights, seeing, transparency, photometric stability and humidity, are some of the most important parameters that qualify a site for front-line ground--based astronomy. ... Night sky at ESO-Paranal (Chile). ... Night sky brightness data . ... UBVRI night sky brightness at ESO-Paranal during sunspot maximum (A 2003, PDF) . ... The Dancing Sky: six years of night sky observations at Cerro Paranal (Starlight 2007 conference proceedings, PDF) . ...
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Ссылки http://www.eso.org/~fpatat/science/skybright/index.html -- 6.1 Кб -- 22.04.2010
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10. ADASS 2003 Conference Proceedings
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Ссылки http://www.adass.org/adass/proceedings/adass03/P6-2/ -- 12.7 Кб -- 27.08.2004
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11. Results of recent and ongoing site programs
... Liyong Liu (NAOC) . Site testing on seeing conditions of the astronomical observatories over China are briefly reviewed, including Xionglong station of NAOC, Gaomeigu station of Yunnan Observatory, Delingha station of Purple Mountain Observatory. ... PDF [3.0€аMB] October 8, 09:55 10:20 . ... In this paper, we will review the site survey activities in the past years, and present the site-testing results on the Oma site, including cloud cover, seeing, water vapor, transparency and sky brightness. ...
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Ссылки http://site2010.sai.msu.ru/section/5 -- 6.7 Кб -- 09.04.2016
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12. Observatory structure
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Ссылки http://www.sao.ru/Doc-en/Divisions/ -- 7.6 Кб -- 09.04.2016
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13. Bright Planets at McMath Pierce Solar Telescope
... Bright Planets at McMath Pierce Solar Telescope . ... Wisconsin-Madison ), Ron Oliversen ( NASA-GSFC ) Explanation: Bright planets Venus and Jupiter are framed by the National Solar Observatory's McMath-Pierce Solar Telescope in this very astronomical scene. The photo was taken at Kitt Peak National Observatory on March 9. ... The angular McMath-Pierce was commissioned 50 years ago to study the Sun , but has also made many observations of these two bright planets. ... March . ... March 2012 . ...
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Ссылки http://www.astronet.ru/db/xware/msg/apod/2012-03-16 -- 15.4 Кб -- 16.03.2012
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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Receiving systems . The SSRT has two independent receiving systems for recording solar observational data, and several ancillary receivers for checking, setting up and adjusting the instrument. The base receiving systen is a multichannel filter receiver for a simultaneous recording in 180 channels with the 500 kHz band each, adjusted at steps of about 600 kHz. ... Channel's band . ...
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15. Science Innovations
. Сайт временно не работает.
16. THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE
... The bright supernova (hereafter SN) in the galaxy NGC 4527 was first sighted by S. Knight (USA) on April 13.17UT at magnitude ~14.0v. The report of the sighting was subsequently forwarded by phone to the AAVSO. ... SN 1991T. The galaxy NGC 4527 is an Sb(s)II type galaxy with an apparent Blue magnitude of 11.32 (Shapley-Ames, 1981). ... An analysis of this event utilizing visual observations by amateurs, plus a light curve is presented.. ... THE LIGHT CURVE: . ... ISN SN 1991T web page . ...
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17. SAI Virtual Observatory Project
... 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. ...
18. Y.Kupryakov, SAI, MSU
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19. VLBI observations of the quasar 3C380
... There are result from two global VLBI observations at 3.6 cm spaced about 2 years. ... The analysis of the apparent motion, indication of the jet flow trajectory and the other implications for the CSS quasars are discussed. ... The quasar 3C380 ( ; thus 1 arcsec corresponds to 4 kpc for , ) is one of the most powerful radio sources (its radio luminosity at 2.7 GHz is ) ( Wilkinson et al. ... 3C380 is a member of the class of Compact Steep Spectrum (CSS) sources. ...
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Ссылки http://www.mrao.cam.ac.uk/yerac/owsianik/owsianik.html -- 11.9 Кб -- 08.12.2003
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20. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kregel05
... 2004) Printed 26 March 2007 A (MN L TEX style file v2.2) Structure and kinematics of edge-on galaxy discs V. The dynamics of the stellar discs. ... The sample covers a substantial range in maximum rotation velocity and depro jected face-on surface brightness, and contains seven spirals with either a boxyor peanut-shaped bulge. ... From the photometry we find that intrinsically more flattened discs tend to have a lower face-on central surface brightness and a larger dynamical mass-to-light ratio. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kregel05 -- 45.8 Кб -- 26.03.2007
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