Dissipative thermal models for impulsive microwave burst delays

Details Dissipative thermal models for impulsive microwave burst delays Dissipative thermal models for impulsive microwave burst delays

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..227b&link_type=abstract

Solar Physics, Volume 86, Issue 1-2, pp. 227-230

Physics

1

Scientific paper

Microwave emission is analysed for a source heated by magnetic dissipation. As the temperature rises and the field falls, the resulting variation in microwave optical depth results in time delays between emission features at different frequencies. A single such source can, however, only explain events exhibiting small delays (˜-1sec) and with lower frequencies peaking later. Continuous production of many such heated regions (multiple kernel model) can, however, explain long delays and produce either advancement or retardation of lower frequencies.

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