Solar flares - The gradual phase

Details Solar flares - The gradual phase Solar flares - The gradual phase

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..399s&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

35

Energy Transfer, Solar Flares, Solar Physics, Coronal Loops, H Alpha Line, Magnetic Field Reconnection, Stellar Models

Scientific paper

There are two kinds of the gradual phase of flares: (1) flares in which all the energy is released within the impulsive phase, and the gradual phase is simply the cooling of the heated flare plasma (confined flares) and (2) flares in which the energy release continues during the gradual phase (dynamic flares). The simplest case of the former, the single-loop flare, and the associated phenomena of coronal 'tongues', flaring arches, and bright surges are briefly addressed. Dynamic flares are discussed in more detail, including the Kopp and Pneuman (1976) model of these flares, subsequent modifications of the model, loop shrinking, giant postflare X-ray arches, radio type IV events and noise storms, complex structures of dynamic flares, and small dynamic flares. Flare hybrids are briefly addressed.

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