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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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