Statistics of sunspot activity . The sunspot indices . ... NGDC's observations . The solar regions . ... Average annual indices . ... November . ... November, 1997 . Visual indices of solar activity by National Geophysical Data Center . ... Average . ...
Dynamic Shack-Hartmann System RAPID V. G. Orlov, V. V. Voitsekhovich Instituto de AstronomМa, UNAM, MИxico CONACYT project E9507-1020P UNAM PAPIIT IN104910 Telescopes OAN OAN- SPM 2.1m telescope 1.5m telescope 0.84m telescope 2.1m telescope OAN-Tonanzintla 1m telescope Astronomical site SPM Observing statistics 1982-2002 (Tapia+ 2007 ) Photometric nights : 64.1% Spectroscopic ... Rapid - Dynamic Shack-Hartmann All modern telescopes demand installation of adaptive system. ...
... Piotrovich Main Astronomical Observatory, Pulkovo, St. Petersburg, Russia Received May 24, 2006; in final form, July 7, 2006 Abstract--We have used two astrometric methods developed at the Main Astronomical Observatory of the Russian Academy of Sciences--the method of apparent-motion parameters (AMP) and a direct geometrical method (DGM)--to derive the orbit of the star S2 around the Galactic center, and thereby the mass of the supermassive black hole at the Galactic center. ... Relative positions. ...
... Fakerat Software in the International Interferometric RadioAstron Project with Very Long GroundSpace Bases V. I. Zhuravlev Astro Space Center of the Lebedev Physical Institute, Russian Academy of Sciences (FIAN ASC), Leninskii pr. ... The results of sched uled observations using the Fakerat package, carried out during the first two years after launching the space radio telescope (SRT) in the spaceground interferometer mode, are reported in the paper. ... Figure 4 shows, in the (, observations. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2015,53,216.pdf -- 497.5 Кб -- 09.06.2015 Похожие документы
... 4 .D.Dolgov (INFN, Ferrara, Italy) STOCHASTIC BACKGROUND GRAVITATIONAL WAVES FORM PRIMORDIAL BLACK HOLES OF G.Tsarevsky (PRAO ASC LPI) PROJECT "RADIOASTRON" AND THE FUTURE OF SPACE RADIOASTRONOMY V.N.Melnikov (VNIIMS, Moscow) SCALAR FIELDS AND MULTIDIMENSIONAL MODELS IN GRAVITY AND COSMOLOGY Wednesday, 24.08.2011 Cosmology, Gravitation and High Energy Physics Conference hall "Sovinyon" 09.00 ? ... 8 Section 2. Astrophysics University Recreation Centre "Chernomorka" (2 ) Tuesday, 23.08.2011 14.30 ? ...
Rep ort by the ESA-ESO Working Group on Galactic p opulations, chemistry and dynamics Abstract Between the early 40s, when Baade showed the first evidence for the existence of two distinct stellar populations, and today, with our Galaxy surprising us with new substructures discovered almost on a monthly basis, it is clear that a remarkable progress has been achieved in our understanding of the Galaxy, of its structure and stellar populations, and of its chemical and dynamical signatures. Yet, some questions
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Ссылки http://www.stecf.org/coordination/esa_eso/galpops/report.pdf -- 2038.4 Кб -- 04.09.2008 Похожие документы
The Ministry of Education and Science of the Russian Federation Samara State Aerospace University (National Research University) N. M. BORGEST ONTOLOGY OF DESIGNING Electronic Textbook Part 1 Concepts and Principles SAMARA 2011 004.9(075) 32.97 Author: Borgest Nikolay M. Translated by: Borgest Diana N. Borgest, N. M. Ontology [Electronic resource] : Elect Education and Science of University. - Electronic text ROM. of Designing = ronic Textbook / N. M. the Russian Federation, and graphic data (3Mb). Borgest;
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Ссылки http://www.ssau.ru/files/education/uch_posob/Ontology%20of%20Designing.%20Pt.1-Borgest%20NM.pdf -- 1716.5 Кб -- 09.12.2014 Похожие документы
No. Name R.A.,Decl., 2000.0 Max Min Type Ref. Epoch Period M-m Spectrum h m s o ' " m m JD200000+ d 780001 V956 Cas 00 05 05.4 +59 39 01. 14.2 17.2 B IS: 001 002 780002 CD Scl 00 06 20.8 -35 17 13. 12.7 14.2 V RRAB 130 004 52068.835 0.57769 20 A0 780003 V439 And 00 06 36.8 +29 01 17. 6.13 ( 0.04 ) V BY 005 DM K0Ve 780004 V957 Cas 00 09 45.7 +50 30 39. 11.6 12.8 * SR: 006 USNO 780005 V958 Cas 00 10 48.5 +57 29 27. 8.8 9.8 * SR: 006 GSC 780006 V959 Cas 00 12 02.7 +55 05 19. 12.0 12.6 * EW 006 GSC 040
RT And * CB EA RS 8.97 0.41 0.31 V 0.6289 v 170 000 170 000 F8V+K1 a 231110.1 +530133 SY And SA * EA 10.70 1.50 V 34.9085 060 027 A0+K1 001316.4 +434241 TT And * SA EA 11.50 1.50 0.10 V 2.7651 v 140 000 A+G7IV 231322.9 +460851 TW And * SA EA 8.98 2.06 0.15 V 4.1228 v 130 020 F0V+K0 000318.2 +325045 UU And SA EA 11.20 3.00 0.20 V 1.4863 v 170 000 A8IV/V 004345.1 +305620 WW And * SA EA 10.92 0.67 0.16 V 23.2852 050 000 000 A0:+G5-K0III 234453.5 +454112 WX And SA * EA 12.10 1.70 V 3.0011 d 120 030 F5IV