Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...44..135f&link_type=abstract
Solar Physics, vol. 44, Sept. 1975, p. 135-147.
Astronomy and Astrophysics
Astronomy
6
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.
Felli Marcello
Pallavicini Roberto
Tofani Gianni
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