Occurrence of radio bursts in the decametre range during solar cycle No. 20

Details Occurrence of radio bursts in the decametre range during solar cycle No. 20 Occurrence of radio bursts in the decametre range during solar cycle No. 20

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..324k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, no. 5, 1988, p. 324-326.

Astronomy and Astrophysics

Astronomy

Decametric Waves, Solar Cycles, Solar Flares, Solar Radio Bursts, Sunspots, Periodic Variations, Solar Atmosphere, Solar Corona

Scientific paper

The number of radio bursts on 23 and 29.5 MHz was evaluated in half-year intervals. The bursts were classified and processed in terms of their duration. The resultant changes in the occurrence of bursts during the solar cycle were compared with sunspot number and flare activity curves. The highest occurrence frequency was observed in the year 1967 (before the years of sunspot number maximum), which agrees with the occurrence frequency of flares: The occurrence of bursts of the long-duration type exhibits a roughly two-year fluctuation in the course of the whole cycle.

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