Possible Radio Evidence of Magnetic Reconnection in Solar Flares

Physics – Plasma Physics

Scientific paper

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Scientific paper

We present possible radio evidence of magnetic reconnection in solar flares.We discuss one specific solar flare -an LDE event of GOES class M3.2 that was observed with the Nobeyama Radio Heliograph (NoRH) in Japan as well as with the Soft X-ray telescope aboard the satellite Yohkoh.The event was also observed in H-alpha and with metric dynamic spectrum analyzers.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 apparently intersecting flaring loops or as a loop-top source above the flaring loop.The bright microwave source is clearly nonthermal and its time profile is similar to that of the flaring foot point microwave sources; and in the late decay phase of the event the microwave source structure is similar to that of the corresponding SXR source. The event was accompanied by a Moreton wave (evidence of shock wave ) and a type II radio burst (a consequence of the shock).We discuss the observations in relation to a specific flare model that involves magnetic reconnection.

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