An idea of flare dynamo mechanism

Details An idea of flare dynamo mechanism An idea of flare dynamo mechanism

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acasn..23..226z&link_type=abstract

Acta Astronomica Sinica, vol. 23, Sept. 1982, p. 226-231. In Chinese, with abstract in English.

Physics

Dynamo Theory, Solar Flares, Solar Magnetic Field, Solar Physics, Sunspots, Convective Flow, Energy Sources, Kinetic Energy, Magnetic Flux, Solar Atmosphere

Scientific paper

It is suggested that a solar-active region with a bipolar sunspot is formed when the magnetic flux ring of the sunspot rises to the solar surface from the depths of the solar convection zone. Conditions for the formation of two-ribbon flares are investigated. It is shown that the required flare energy of 10 to the 29th to 10 to the 33rd ergs can be produced as long as the perpendicular velocity is 0.3-3 km/s and the magnetic field strength is 10-100 gauss.

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