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Paper: Coronal Hard X-Ray Source Related to a Plasma Ejection
Volume: 325, The Solar-B Mission and the Forefront of Solar Physics
Page: 341
Authors: Masuda, S.
Abstract: 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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