Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39....1b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, Jan. 1988, p. 1-7.
Astronomy and Astrophysics
Astronomy
11
Coronal Holes, Magnetic Anomalies, Solar Atmosphere, Solar Flares, Solar Longitude, Solar Magnetic Field, Solar Activity, Solar Cycles, Solar Limb, Southern Hemisphere, Sunspots
Scientific paper
In investigating the large-scale distribution changes of solar background magnetic field during a wide time interval around the formation of this very complex region, it is demonstrated that this development must be taken as part of a global process in the solar atmosphere. Complete reorganizations are seen in the magnetic active longitude patterns and the solar magnetic-field sector structure, clearly related to its maximum stage. It is also shown that, at the same time, restructuralization of coronal holes took place. The relation of large-scale cellularlike structures to this development is also studied. It is concluded that the formation of this strong white-light flare region was casually related to the rebuilding of the global solar magnetic field.
Bumba Vaclav
Gesztelyi L.
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