Physics
Scientific paper
Apr 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...84..295k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 84, April 1983, p. 295-310.
Physics
26
Solar Flares, Solar X-Rays, Type 4 Bursts, Continuous Radiation, Flux Density, Spectroheliographs, Temporal Distribution, Type 3 Bursts, Ultrahigh Frequencies, Very High Frequencies
Scientific paper
X-ray radiation is used to study coronal phenomena in conjunction with meter wave observations during some large solar flares. It is found that metric flare continua and moving type IV bursts are associated with gradual and long lasting (a few tens of minutes) microwave and hard X-ray emissions. The detailed temporal analysis reveals that although metric and hard X-ray sources are located at very different heights, both kinds of emission result from a common and continuous/repetitive injection of electrons in the corona. The late part of the metric event (stationary type IV burst) is only associated wih soft X-ray radiation. This indicates that the mean energy of the radiating electrons is lower during stationary type IV bursts than during the earlier parts of the event.
Anderson Kenneth
Kane Sean
Klein Lior
Pick Monique
Trottet Gerard
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