Rapid processes in solar prominences - A parallel between cycles No. 20 and 21

Details Rapid processes in solar prominences - A parallel between cycles No. 20 and 21 Rapid processes in solar prominences - A parallel between cycles No. 20 and 21

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..145..129d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 145, no. 1, p. 129-135.

Physics

Solar Cycles, Solar Prominences, Asymmetry, Maxima, Minima, Solar Longitude, Surges

Scientific paper

The study presents some statistical aspects of three types of rapid processes (surges, activations, and eruptions) in solar prominences during cycle No. 20 and compares them with those of cycle No. 21. Emphasis is placed on the distribution of the events over the cycles, the active longitude intervals each year within a solar cycle, and the north-south asymmetry. It is found that during both cycles, as far as active longitudes and north-south asymmetry are concerned, eruptive prominences have quite a different behavior from surges or prominence activations.

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