Energy Transport Mechanisms and the Event of 16th December 1991

Physics

Scientific paper

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Scientific paper

The flare of 16th December 1991 had relatively simple structure, which has made it useful for studing the energetics of chromospheric evaporation. Energy balance calculations for this flare support an electron beam energy deposition hypothesis for this event. The creation of `super-hot' plasma is also investigated, using YOHKOH Hard X-ray Telescope images. Contrary to previously reported events, the `super-hot' plasma in the 16th December flare is generated, and remains close to the chromospheric footpoints, with a decay time consistent with saturated thermal conduction to the chromosphere.

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