Unusual series of type III-RS solar radio bursts

Details Unusual series of type III-RS solar radio bursts Unusual series of type III-RS solar radio bursts

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.258..693t&link_type=abstract

Nature, vol. 258, Dec. 25, 1975, p. 693, 694. Research supported by the Schweizerischer Nationalfonds zur Foerderung der Wissens

Physics

10

Frequency Shift, Magnetic Mirrors, Solar Magnetic Field, Solar Spectra, Type 3 Bursts, Drift Rate, Microwave Emission, Particle Acceleration, Radio Spectra, Spectroheliographs

Scientific paper

Results are reported for observations of about 30 type III-RS ('reverse slope') solar radio bursts in the approximate range from 200 to 420 MHz on August 12, 1975. It is shown that the distributions of drift rate and duration were similar to those of type III bursts, that two bursts were second branches of U bursts, and that four events contained a type III-RS burst followed immediately by a type III burst, in a Y-like configuration. It is assumed that all the bursts in this extended series are homologous, originating in the same general source region and from similar acceleration events. It is suggested that all type III-RS bursts are second branches of U bursts.

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