Small-scale structure in solar flare radio emission

Details Small-scale structure in solar flare radio emission Small-scale structure in solar flare radio emission

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.275..105b&link_type=abstract

In ESA, Proceedings of the 21st ESLAB Symposium on Small Scale Plasma Processes in the Solar Chromosphere/Corona, Interplanetary

Physics

1

Fragmentation, Solar Flares, Solar Spectrometers, Type 3 Bursts, Ion Injection, Particle Acceleration, Solar Spectra, Spectral Emission

Scientific paper

High resolution radio observations of type 3 solar flares and spike bursts are presented. Considerable fragmentation appears in time and spectrum, indicating that many, small sources are involved. The structure in type 3 emission requires more than 100 distinct injections or acceleration events in a flare studied. There are suggestions of orders of magnitude higher fragmentation in the acceleration process from type 3 bursts and spikes. Small scale structures in flares may control the energy release and its time scale.

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