Special Issue: Magnetic Reconnection in Space and Laboratory Plasmas
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Seemingly intersecting flaring loops in microwaves: Possible radio evidence for reconnection
Earth, Planets and Space volume 53, pages 585–591 (2001)
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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Kundu, M.R., Grechnev, V.V. Seemingly intersecting flaring loops in microwaves: Possible radio evidence for reconnection. Earth Planet Sp 53, 585–591 (2001). https://doi.org/10.1186/BF03353275
- Current Sheet
- Magnetic Reconnection
- Decay Phase
- Impulsive Phase
- Microwave Source