Seemingly intersecting flaring loops in microwaves: Possible radio evidence for reconnection

Details Seemingly intersecting flaring loops in microwaves: Possible radio evidence for reconnection Seemingly intersecting flaring loops in microwaves: Possible radio evidence for reconnection

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ep%26s...53..585k&link_type=abstract

Earth, Planets and Space, Volume 53, p. 585-591.

Physics

5

Scientific paper

We present possible radio evidence of magnetic reconnection in a solar flare -- an LDE event of GOES class M3.2 that was observed on 1999 February 16 on the disk. Our evidence is based upon the facts that we observed a bright microwave source-blob at 17 and 34 GHz near the intersection of two seemingly intersecting flaring loops or as a loop-top source above one flaring loop. The bright microwave source is clearly non-thermal and its time profile is similar to those of the flaring footpoint microwave sources; and in the late decay phase of the event the microwave source structure is similar to that of the corresponding SXR source.

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