On some peculiarities in the evolution of the McMath 16051 flare active region on 2-7 June, 1979

Details On some peculiarities in the evolution of the McMath 16051 flare active region on 2-7 June, 1979 On some peculiarities in the evolution of the McMath 16051 flare active region on 2-7 June, 1979

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..142...67g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 142, no. 1, p. 67-86.

Physics

3

Solar Flares, Solar Magnetic Field, Magnetic Signatures, Photosphere

Scientific paper

The active region McMath 16051 showed during 2-7 June, 1979 a complex multipolar magnetic configuration, in which separate bipolar systems interacted. The period of high flare activity of 3-5 June was characterized by a rapid change in magnetic flux imbalance with the rate of 1.65 x 10 exp 9 Wb/s, while the period of low flare activity was typified by a synchronous decrease of the N- and S-polarity fluxes, with balance between them remaining unchanged. The high flare activity period exhibited the following structural features of the photosphere in the sunspot group: thin, thread-like bright bridges in sunspot kernels and complex dynamic penumbral structure, with superimposition of two systems of fibrils.

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