Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..363b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, no. 6, Dec. 1988, p. 363-371.
Astronomy and Astrophysics
Astronomy
2
Magnetic Field Configurations, Solar Activity, Solar Magnetic Field, H Alpha Line, Solar Cycles, Spatial Distribution
Scientific paper
From the comparison of several modes of time development of the latitudinal distribution of solar magnetic fields, obtained by different authors using different basic observational material and different methods, the authors have obtained the following results: at high solar latitudes (|φ| ⪆ 40°) all distributions agree irrespective of the method of construction. In zones of activity around the solar equator, there is a qualitatively good but quantitatively poor agreement of the integrated, directly observed fields (from Mt. Wilson Observatory) and of the highly integrated fields derived from Hα synoptic charts. The areas covered by the positive and negative polarities on the whole Sun during the investigated one and half solar cycles (No. 20 and 21) are practically equal.
Bumba Vaclav
Hejna Ladislav
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