Radioheliograph and white-light coronagraph studies of a coronal mass ejection event

Details Radioheliograph and white-light coronagraph studies of a coronal mass ejection event Radioheliograph and white-light coronagraph studies of a coronal mass ejection event

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..122..145g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 122, no. 1, 1989, p. 145-173.

Physics

17

Coronagraphs, Solar Radio Bursts, Spectroheliographs, Stellar Mass Ejection, Coronal Loops, Plasma Radiation, Type 2 Bursts, Type 3 Bursts

Scientific paper

The radioheliograph and SMM-C/P observations of November 3, 1986 mass ejection event are analyzed. The metric radio emissions are the only detected activity associated with the mass ejection, but are adequate to study the evolution of the event. The start time of the ejection seems to precede a possible flare behind the limb indicated by the early type III bursts. The physical relation between various types of bursts and the CME is studied, interpreting moving type IV bursts as a plasma emission process. It is also shown using white-light coronagraph data that the density in the source region of the moving type IV is sufficient to support second-harmonic plasma emission at the observed frequency of 50 MHz.

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