Large solar flares and coronal mass ejections: Their manifestations in the chromosphere

A phenomenological model of a united (solar flare-coronal mass ejection (CME)) event is briefly described. The model is based on the analysis of the images of the development of some events in various spectral ranges. A modified classification of the chomospheric manifestations of the event is propo...

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Bibliographic Details
Published in:	Geomagnetism and Aeronomy Vol. 49; no. 8; pp. 1076 - 1079
Main Authors:	Sidorov, V. I., Yazev, S. A.
Format:	Journal Article
Language:	English
Published:	Dordrecht SP MAIK Nauka/Interperiodica 01-12-2009 Springer Nature B.V
Subjects:	Astrophysics Corona Earth and Environmental Science Earth Sciences Geophysics/Geodesy Scientific imaging Solar flares Coronal Mass Ejection Current Layer Coronal Magnetic Field Flare Solar Flare
Online Access:	Get full text
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Summary:	A phenomenological model of a united (solar flare-coronal mass ejection (CME)) event is briefly described. The model is based on the analysis of the images of the development of some events in various spectral ranges. A modified classification of the chomospheric manifestations of the event is proposed. A phenomenological model describing phenomena in the process of the development of intense solar flare-CME events in the activity complexes on the Sun is briefly presented. The model is based on the analysis of the observation data for some major flares (May 16, 1981, October 19, 2001, July 23, 2002).
Bibliography:	ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23
ISSN:	0016-7932 1555-645X 0016-7940
DOI:	10.1134/S0016793209080039