Correlation of solar X-ray bursts with optical, radio and energetic particle phenomena

Details Correlation of solar X-ray bursts with optical, radio and energetic particle phenomena Correlation of solar X-ray bursts with optical, radio and energetic particle phenomena

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ucsd.rept.....h&link_type=abstract

Final Report, Aug. 1973 - Jul. 1974 California Univ., La Jolla.

Other

Solar Flares, Solar X-Rays, Brightness, Oso-7, Particle Emission, Spectrum Analysis

Scientific paper

The OSO-7 data on solar X-ray bursts have been used in several studies of solar flares. These studies have emphasized the correlation between X-ray emissions and phenomena observed at other wavelengths. A study of flares occurring beyond the solar limb has helped to determine the vertical extent of flare X-ray emission. This investigation also showed that the hot X-ray plasma cools predominantly by conduction, lending support to theories in which H alpha and other optical emissions obtain energy in this fashion. Another study determined the basic parameters of hard X-ray spectra as a support for detailed comparison with solar microwave emission.

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