Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38..351b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 38, no.6, 1987, p. 351-355.
Astronomy and Astrophysics
Astronomy
1
Gyromagnetism, Solar Flares, Solar Magnetic Field, Solar Rotation, Chromosphere, Interplanetary Magnetic Fields, Solar Activity
Scientific paper
In the present continuation of their study of processes related to the development of the white-light flare region of April 1984, the authors pay greater attention to the problem of rotation rates of certain components of the background magnetic field, constituting the main patterns of the weak as well as strong fields, from three points of view: as they are demonstrated by the distribution of chromospheric filaments, from point of view of the existence of so-called "pivot points" (Mouradian et al., 1987) and of the rotation of the strongest magnetic flux sources.
Bumba Vaclav
Gesztelyi L.
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