Physics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...49..297p&link_type=abstract
Solar Physics, vol. 49, Aug. 1976, p. 297-313.
Physics
11
Centimeter Waves, High Resolution, Microwave Emission, Solar Flares, Solar Radio Bursts, Spatial Distribution, X Ray Spectra, H Alpha Line, Radio Interferometers, Skylab Program, Solar Spectra, Spaceborne Telescopes, Stellar Models, Time Dependence
Scientific paper
High-resolution images of the decay phase of a soft X-ray flare observed by the S-054 experiment on Skylab are compared with interferometric scans of the radio burst obtained simultaneously at 2.8 cm. The spatial resolution of the radio instrument in one direction, although lower than the X-ray telescope resolution, is high enough for a detailed comparison. The comparison clarifies the relationship between the sources of soft X-ray and thermal radio emission in solar flares. The X-ray emission is localized in a looplike structure which appears spatially coincident with the rapidly varying component of the radio burst. The more stable components of the radio source, which do not appear to contribute substantially to X-ray emission, are found to be spatially associated with the extremes of the X-ray loop. A model of plasma-filled loops is suggested which accounts for the emissions in both spectral ranges and for their spatial location and temporal development.
Pallavicini Roberto
Vaiana Giuseppe S.
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