Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253..975c&link_type=abstract
Astrophysical Journal, Part 1, vol. 253, Feb. 15, 1982, p. 975-982.
Astronomy and Astrophysics
Astrophysics
4
Solar Flares, Solar Radio Bursts, Solar Radio Emission, Solar X-Rays, Energy Spectra, Microwave Emission, Solar Spectra, X Ray Spectra
Scientific paper
The gradual soft X-ray emissions associated with a homogeneous set of solar flares have been investigated in the context of a thermal model proposed to explain the impulsive components. The parametric techniques which successfully characterized the hard X-ray and microwave observations are employed in an event-by-event analysis to test for quantitative and correlative relationships between the impulsive and gradual emissions. The results of this investigation are consistent with the hypothesis that the hard X-ray and microwave emissions are produced by bulk heating of a common thermal source. The quantitative relationships require an additional source to explain the soft X-ray observations, consistent with previous results. Correlations between the energetics of the impulsive and gradual emissions, identified in the present work, provide the first clear evidence that their energizing mechanisms are related.
Crannell Carol J.
Karpen Judith T.
Thomas Robert J.
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