Coronal Mass Ejections and Solar Radio Emissions (invited)

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2011Publisher:Austrian Academy of Sciences PressJournal:PLANETARY RADIO EMISSIONS VII

Authors: N. Gopalswamy;

doi: 10.1553/pre7s325

Coronal Mass Ejections and Solar Radio Emissions (invited)

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Abstract

Three types of low-frequency nonthermal radio bursts are associated with coronal mass ejections (CMEs): Type III bursts due to accelerated electrons propagating along open magnetic field lines, type II bursts due to electrons accelerated in shocks, and type IV bursts due to electrons trapped in post-eruption arcades behind CMEs. This paper presents a summary of results obtained during solar cycle 23 primarily using the white-light coronagraphic observations from the Solar Heliospheric Observatory (SOHO) and the WAVES experiment on board Wind.

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