Formation of the May 1981 solar flare complex and the global magnetic field of the sun (H. R. 17 644)

Details Formation of the May 1981 solar flare complex and the global magnetic field of the sun (H. R. 17 644) Formation of the May 1981 solar flare complex and the global magnetic field of the sun (H. R. 17 644)

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..210b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, July 1986, p. 210-218.

Mathematics

Logic

8

Magnetic Effects, Solar Flares, Solar Magnetic Field, Astronomical Maps, Coronal Holes, H Alpha Line, Solar Longitude

Scientific paper

The degree to which the development of the May 1981 flare complex is related to the global changes of the solar background magnetic fields is studied. It is connected with the action of magnetic active longitudes, it lasts about 10 rotations, and in its last phase it forms a coronal hole. Its fields play a role in forming two sectors in the equatorial background fields and are involved in the fast global field redistribution into regular morphological patterns. All regularities found require physical interpretation.

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