Coronal Hard X-Ray Source Related to a Plasma Ejection

Details Coronal Hard X-Ray Source Related to a Plasma Ejection Coronal Hard X-Ray Source Related to a Plasma Ejection

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..341m&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

1

Scientific paper

It is found in an X-class impulsive flare that a hard X-ray (above 20 keV) source exists almost at the same location as a soft X-ray ejected feature. This hard X-ray source is related to reconnection upward flow and/or electrons accelerated upward near the reconnection site. The characteristics of this source are summarized and possible scenarios are discussed.

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