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

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

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ge%26ae..49.1076s&link_type=abstract

Geomagnetism and Aeronomy, Volume 49, Issue 8, pp.1076-1079

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Scientific paper

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).

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