... 2258 DAYS IN SOLARROTATION INTERVAL 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 1999 Jan 1 5 8 Jan 2259 Jan 2260 Feb 2261 Mar 2262 Mar 2263 Apr 2264 May 2265 Jun 2266 Jul 2267 Aug 2268 Sep 2269 Oct 2270 Nov 2271 Nov 2272 Dec ...
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Ссылки http://www.wdcb.ru/stp/data/mag-scan_dupl/Ars/ARS1999/musi1999.pdf -- 242.3 Кб -- 18.01.2010 Похожие документы
... solar rotational pole through the center of the solar disk as viewed from Earth (central meridian).The Carrington longitude (L) is the heliographic longitude of a solar feature in the coordinate system that rotates with the Sun (Solar Geophysical Data PRF ...
... solar rotational pole through the center of the solar disk as viewed from Earth (central meridian).The Carrington longitude (L) is the heliographic longitude of a solar feature in the coordinate system that rotates with the Sun (Solar Geophisical Data PRF ...
... solar rotational pole through the center of the solar disk as viewed from Earth (central meridian).The Carrington longitude (L) is the heliographic longitude of a solar feature in the coordinate system that rotates with the Sun (Solar Geophysical Data PRF ...
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Ссылки http://www.wdcb.ru/stp/data/Solar_Flare_Events/Fl_XXIVo.pdf -- 250.3 Кб -- 04.03.2015 Похожие документы
... solar rotational pole through the center of the solar disk as viewed from Earth (central meridian).The Carrington longitude (L) is the heliographic longitude of a solar feature in the coordinate system that rotates with the Sun (Solar Geophisical Data PRF ...
... Moreover, the use of Earth as a platform from which to record these numbers contributes to their varia- bility, too, because the sun rotates and the evolving spot groups are distrib- uted unevenly across solar longitudes. ...