A recent study of solar gradual hard X-ray bursts is summarized. The data are interpreted in terms of a model involving the acceleration and trapping of electrons in post flare loop systems following coronal mass ejections. A controversy about the classification of the metric continuum that typically accompanies gradual hard X-ray events is addressed.
Solar gradual hard X-ray bursts - Observations and an interpretation
Advances in Space Research ; 6 , 6 19
1986-01-01
Miscellaneous
No indication
English
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