Thermal Runaway as the Solar Flare Trigger Mechanism

Details Thermal Runaway as the Solar Flare Trigger Mechanism Thermal Runaway as the Solar Flare Trigger Mechanism

Oct 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970soph...14..372k&link_type=abstract

Solar Physics, Volume 14, Issue 2, pp.372-383

Physics

8

Scientific paper

It is postulated that the solar flare ‘trigger’ mechanism is a thermal runaway which occurs in the inner corona. This runaway is the result of a radiative power function which decreases with increasing temperature. Relationships of the onsets of Hα flares, hard X-ray, soft X-ray and centimeter radio bursts are consistent with the model. Flares are shown to be common solar phenomena which occur preferentially in hot and dense active regions.

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