Kinematics of the May 1981 flare complex's magnetic field decrease (H. R. 17 644)

Details Kinematics of the May 1981 flare complex's magnetic field decrease (H. R. 17 644) Kinematics of the May 1981 flare complex's magnetic field decrease (H. R. 17 644)

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..219b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, July 1986, p. 219-226.

Astronomy and Astrophysics

Astronomy

1

Solar Flares, Solar Magnetic Field, Temporal Distribution, Kinematics, Magnetic Field Configurations, Magnetic Flux, Photosphere, Sunspots

Scientific paper

Characteristic details of the postmaximum dissolution process of magnetic and photospheric patterns of the May 1981 flare complex are studied over about one week of fine-scale observations. Magnetic-flux and area changes in the course of field-topology simplification are estimated. In the photosphere only five features with a more stable field configuration survived this evolutionary stage. Flare activity variations are related to the individual changes observed in the magnetic field topology and photospheric morphology, and some conclusions concerning the consumption of magnetic energy stored in the system of magnetic field lines above the photosphere are drawn.

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