Shock-associated kilometric radio emission and solar metric type II bursts

Details Shock-associated kilometric radio emission and solar metric type II bursts Shock-associated kilometric radio emission and solar metric type II bursts

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..393k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 393-405.

Physics

16

Kilometric Waves, Shock Waves, Type 2 Bursts, Electron Acceleration, International Sun Earth Explorer 3, Solar Corona

Scientific paper

New criteria are used here to select and study the properties of shock-associated (SA) kilometric bursts. Nearly half of all intense metric type II bursts were temporally associated with 1980 kHz emission which was not attributable to metric type III bursts. A quarter of all intense type II bursts are not associated with any significant 1980 kHz emission and another quarter are accompanied by 1980 kHz emission presumed due to type II bursts. The SA bursts are generally not well correlated with microwave flux-density profiles but compare more closely with the most intense and structured parts of the profiles of metric type II bursts. These results imply that the SA emission is due primarily to energetic electrons accelerated at the associated shock.

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