Hard X-ray Imaging Observations of Footpoint Sources in Impulsive Solar Flares

Details Hard X-ray Imaging Observations of Footpoint Sources in Impulsive Solar Flares Hard X-ray Imaging Observations of Footpoint Sources in Impulsive Solar Flares

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..169s&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.169-172.

Physics

11

Scientific paper

Hard X-ray imaging observations of intense impulsive flares with the Yohkoh Hard X-ray Telescope have revealed that the hard X-ray emission in an energy range above 30 keV originates most frequently from double sources, suggesting that bulk of hard X-rays is emitted from footpoints of flaring magnetic loops. Temporal and spectral behaviors of the double sources are described and their physical implications discussed.

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