H-alpha observations of the August 12, 1975 Type III-RS bursts

Details H-alpha observations of the August 12, 1975 Type III-RS bursts H-alpha observations of the August 12, 1975 Type III-RS bursts

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..201l&link_type=abstract

Solar Physics, vol. 50, Sept.-Oct. 1976, p. 201-211.

Physics

4

H Alpha Line, Solar Radio Emission, Type 3 Bursts, Filtergrams, Solar Corona, Solar Flares, Stellar Models, Time Response

Scientific paper

We present H-alpha filtergram observations of a number of the Type III-RS (reverse slope) bursts that occurred on August 12, 1975. Solar radio emission was peculiar on that date in that a large number, and proportion, of the usually rare reverse slope bursts were observed (Tarnstrom and Zehntner, 1975). We show that the radio bursts coincide in time with a homologous set of H-alpha flares located at the limbward edge of spot group Mt. Wilson 19598. We propose a model in which the reverse slope bursts are the downward branches of U bursts, whose upward branches are hidden behind the coronal density enhancement over the spot group.

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