Physical conditions in photospheric layers of the McMath 15526 active region at the stage of flare activity.

Details Physical conditions in photospheric layers of the McMath 15526 active region at the stage of flare activity. Physical conditions in photospheric layers of the McMath 15526 active region at the stage of flare activity.

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold...7...93a&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/7, p. 93 - 98

Mathematics

Solar Photosphere: Solar Flares, Solar Flares: Magnetic Fields

Scientific paper

Temperature, gaseous pressure and magnetic field strength are determined for two levels of the photosphere before and during flares in the McMath 15526 active region. During a flare heating up to 50K takes place at both levels, while in a subflare only the upper level is heated. The magnetic field strength at the lower level is 2200 Gs in a flare 1 n and 1800 Gs in a subflare, i.e. it decreases with height. Prior to flares it is smaller, than during flares by 300 - 600 Gs.

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