Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990baicz..41..253b&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 41, no. 4, July 1990, p. 253-262.
Astronomy and Astrophysics
Astronomy
12
Solar Activity, Solar Corona, Solar Cycles, Solar Magnetic Field, Solar Prominences, Annual Variations, Solar Oscillations, Spatial Distribution
Scientific paper
The latitudinal distribution of green corona emission maxima and the maximum frequency of prominence occurrence are presently related to the large-scale regularities in the latitudinal distribution of (1) magnetic fields, (2) polar faculae, and (3) sunspots. The existence of polar and equatorial main latitudinal zones in both solar hemispheres is demonstrated by observational data. The main magnetic patterns are underlined by the distribution of prominences and of green coronal emission maxima; the latter also seem to exhibit two different qualities in their latitudinal distribution, depending on the heliographic latitudes.
Bumba Vaclav
Rusin Vojtech
Rybansky Milan
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