A type IV burst associated with a coronal streamer disruption event

Details A type IV burst associated with a coronal streamer disruption event A type IV burst associated with a coronal streamer disruption event

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111...53k&link_type=abstract

(Observatoire de Paris, CNRS, CNES, et al., CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, 2nd, Aubigny-s

Physics

5

Coronal Loops, Solar Flares, Solar Prominences, Type 4 Bursts, Electron Plasma, Goes Satellites, Solar X-Rays, Type 2 Bursts

Scientific paper

A type IV burst was observed on February 17, 1985 with the Clark Lake Radio Observatory multifrequency radioheliograph operating in the frequency range 20 - 125 MHz. This burst was associated with a coronal streamer disruption event. From two-dimensional images produced at 50 MHz, evidence is shown of a type II burst and a slow moving type IV burst. The observations of the moving type IV burst suggests that a plasmoid containing energetic electrons can result from the disruption of a coronal streamer.

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