The structure and intensity evolution of a solar burst at 2.8 CM and the relation with the soft X-ray emitting region

Astronomy and Astrophysics – Astronomy

Scientific paper

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Microwaves, Solar Radio Bursts, Solar X-Rays, X Ray Astronomy, Electron Density (Concentration), Electron Energy, Emission Spectra, Solar Magnetic Field

Scientific paper

The decay phase of a microwave burst was observed with a one-dimensional angular resolution of 16 sec at 2.8 cm. The structure was found to be composed of several bursting regions with different evolution. The event was also observed in soft X-rays by full-disk detectors. Joint analysis of these data suggests that the complete event had a thermal origin and that the soft X-ray emission was associated with the rapidly varying component of the radio structure. From these results, the average values of electron temperatures and densities were computed for each component.

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