Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241l.113k&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 241, Oct. 15, 1980, p. L113-L116.
Astronomy and Astrophysics
Astrophysics
37
Solar Flares, Solar X-Rays, Type 3 Bursts, Correlation, High Energy Electrons, Solar Atmosphere, Solar Corona
Scientific paper
The first measurements of the spatial structure of a group of type III solar radio bursts associated with an impulsive hard X-ray burst are presented. At 169 MHz the radio source has been found to consist of two principal regions separated by about 300,000 km. The two regions together produced a total of four component bursts in good time correlation with spikes in the hard X-ray emission. The observations indicate that electron acceleration/injection occurs over a region which covers a wide range of magnetic field lines.
Kane Sharad R.
Pick Monique
Raoult Annie
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