The Timing of Radio Emission in Flares and CMEs

Details The Timing of Radio Emission in Flares and CMEs The Timing of Radio Emission in Flares and CMEs

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh31c..06w&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH31C-06

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7513 Coronal Mass Ejections, 7534 Radio Emissions

Scientific paper

Radio observations are very sensitive to emission by electrons accelerated in the solar corona. This talk will review evidence for acceleration in flares and coronal mass ejections from the radio perspective, focussing on the timing of radio emission in relation to other high-energy phenomena. Amongst other topics, the relationship of coronal type II radio bursts and coronal mass ejections will be discussed in the light of Zhang et al's LASCO data, and recent results on radio emission from CMEs by Bastian et al will be reviewed.

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