Prominence activity during the ascending phase of solar cycle 22

Details Prominence activity during the ascending phase of solar cycle 22 Prominence activity during the ascending phase of solar cycle 22

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138..415d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, no. 2, April 1992, p. 415-418. Research supported by Ministry of Science and Education

Physics

H Alpha Line, Solar Activity Effects, Solar Corona, Solar Cycles, Solar Prominences, Solar Limb, Solar Magnetic Field, Sunspots

Scientific paper

Longitude-latitude and time-latitude distributions of the number and area of prominences observed at Lomnicky Stit coronal station in the years 1986-1990 are studied using the method of contour maps construction with different degree of smoothing. Special attention is paid to the bifurcation in the prominence distribution. Comparison with the ascending phase of solar cycle 21 is made.

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