Simultaneous multi-frequency imaging observations of solar microwave bursts

Details Simultaneous multi-frequency imaging observations of solar microwave bursts Simultaneous multi-frequency imaging observations of solar microwave bursts

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..153k&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

13

Centimeter Waves, Microwave Emission, Solar Radio Bursts, Stellar Flares, Astronomical Maps, Flux Quantization, Solar Flares, Very Large Array (Vla)

Scientific paper

The results of simultaneous two-frequency imaging observations of solar microwave bursts with the Very Large Array are reviewed. Simultaneous 2 and 6 cm observations have been made of bursts which are optically thin at both frequencies, or optically thick at the lower frequency. In the latter case, the source structure may differ at the two frequencies, but the two sources usually seem to be related. However, this is not always true of simultaneous 6 and 20 cm observations. The results have implications for the analysis of nonimaging radio data of solar and stellar flares.

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