Soft X-Ray Enhancement During Flares

Details Soft X-Ray Enhancement During Flares Soft X-Ray Enhancement During Flares

Aug 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970soph...13..462d&link_type=abstract

Solar Physics, Volume 13, Issue 2, pp.462-466

Physics

2

Scientific paper

The estimates of quiescent and flare time temperatures of soft X-ray emitting regions on the Sun are obtained for flares observed during March August 1967 from X-ray observations in two soft X-ray bands, 2 12 Å (Explorer-33 data) and 8 12 Å (OSO-3 data). It is concluded that hot coronal condensation, originally at 2 3 × 106 K, is raised to the temperature of about 4 5 × 106 K and is responsible for soft X-ray enhancement.

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