๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Association between gradual hard X-Ray emission and metric continua during large flares

โœ Scribed by L. Klein; K. Anderson; M. Pick; G. Trottet; N. Vilmer; S. Kane

Publisher
Springer
Year
1983
Tongue
English
Weight
723 KB
Volume
84
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

X-ray radiation is used to study coronal phenomena in conjunction with meter wave observations during some large solar flares. It is found that metric flare continua and moving type IV bursts are associated with gradual and long lasting (a few tens of minutes) microwave and hard X-ray emissions. The detailed temporal analysis reveals that although metric and hard X-ray sources are located at very different heights, both kinds of emission result from a common and continuous/repetitive injection of electrons in the corona. The late part of the metric event (stationary type IV burst) is only associated with soft X-ray radiation. This indicates that the mean energy of the radiating electrons is lower during stationary type IV bursts than during the earlier parts of the event.

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