... 284 A) that are sensitive to coronal plasma at temperatures of (1.22.0) в 106 K, as well as in soft Xrays, corresponding to temperatures > 2.5 в 106 K. Therefore, dimmings can be interpreted as a result of the complete or partial opening of the magnetic ...
... m + h -l(R /Rs )l -1 c1 , B = - Plm (cos ) (glm cos m + h +(R /Rs )l -1 cl , lm lm ... cos m - glm sin m) (R0 /R )l +2 + (3) Here, 0 m l < N (conventionally N = 9), cl ... Konakh, M. M., and Mansurov, G. S.: 1986, Geomagn. Aeron. 26, 313. ...
... and the ionosphere coupling V.M. Sorokin , V.M. Chmyrev, A.K. Yaschenko Institute of ... m, the atmosphere conductivity (0)=2в10-14 S= m near the Earth surface and the low ... 46 47. Sorokin, V.M., Chmyrev, V.M., Hayakawa, M., 2000. ...
[
Текст
]
Ссылки http://www.izmiran.rssi.ru/~sova/Copies/jastp01-63-1681.pdf -- 185.7 Кб -- 28.06.2005 Похожие документы
... За время полной фазы затмения (106 сек) было получено 430 фотографий короны в поляризованном свете. ... A.K. Kishonkov and M.M. Molodensky 'Precise determination of the Orientation of the Plane of Polarization in the Solar Corona'. ...
... 5 --------------------------------------------------------------------------- Weekly ... SUNSPOT GROUP AR11429 (N18L299, Sp=700 m.v.h. on 4.02) ALREADY OCCURENCED ONE LARGE ...