Correlated observations of a spatially resolved type III solar radio burst group and the associated hard X-ray emission

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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