Secondary peaks in solar microwave outbursts

Details Secondary peaks in solar microwave outbursts Secondary peaks in solar microwave outbursts

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...84..347c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 84, April 1983, p. 347-359.

Physics

26

Continuous Radiation, Decametric Waves, Microwave Emission, Solar Flares, Solar Radio Bursts, Frequency Response, H Alpha Line, Lines Of Force, Stellar Models

Scientific paper

Observations are presented for several large solar flares in which a timing association is observed between late (approximately equal to or greater than 30 min after the flash phase) microwave peaks and late stationary decametric continua. It is suggested that the late microwave peaks are a phenomenon of the post flare loop (relaxation) stage of large flares and are caused by field line reconnections occurring above the H-alpha and soft X-ray emitting loops. A simple model to account for the association between the secondary radio peaks observed at discrete frequencies and the late decametric continua is proposed.

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