Distinctive spatial configuration of a class of microwave flaring sources

Details Distinctive spatial configuration of a class of microwave flaring sources Distinctive spatial configuration of a class of microwave flaring sources

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..319k&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun, Flares

Scientific paper

We discuss a particular spatial configuration of a class of microwave flaring regions in which the primary energy release results from the interaction between emerging magnetic flux and an existing overlying region. Such events typically exhibit radio and X-ray emission at the main flare site (the site of interaction) and in addition radio emission at a remote site up to 1×105 km away in another active region. We have identified and studied more than a dozen microwave flares in this class, in order to arrive at some general conclusions on reconnection and energy release in such solar flares.

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