Astronomy and Astrophysics – Astronomy
Scientific paper
May 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baicz..33...36b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin, vol. 33, no. 1, 1982, p. 36-46.
Astronomy and Astrophysics
Astronomy
5
Solar Activity, Solar Magnetic Field, Chromosphere, Photosphere, Solar Corona
Scientific paper
The evolution of the background magnetic field pattern is described. The complex needed only one or two rotations to reach its maximum evolutionary state and its whole duration was about 10 or 12 rotations. The studied active region appears during the early stages of a new impulse of activity, whose development is described along with that of the green coronal emission of which the complex of activity forms the center of gravity. Low resolution magnetic maps are used to describe the development of the complex of activity and high resolution maps are used to compare characteristic evolutionary features of the active region with photospheric and chromospheric development. It is concluded that the active region represents only a small part of a more general evolutionary process of the magnetic field.
Bumba Vaclav
Klvana Mirek
Pflug K.
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