On the regimes of heating during solar flares

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We suggest a new differential method whereby we have detected the separation of a long-duration flare into intervals characterized by different regimes of plasma heating and cooling based on soft X-ray data. The rise phase of the flare is shown to consist of accelerated and decelerated heating regimes compared to an exponential law. Accelerated cooling takes place at the beginning of the decay phase, which is followed by decelerated one. The final part of the flare is a prolonged process of cooling according to a nearly exponential law.

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