Correlation of solar x-ray bursts with optical, radio and energetic particle phenomena. Final report, Aug 1973--Jul 1974
Technical Report
·
OSTI ID:7285812
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; this finding lends 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. (GRA)
- Research Organization:
- California Univ., San Diego, La Jolla (USA)
- OSTI ID:
- 7285812
- Report Number(s):
- AD-A-010039
- Country of Publication:
- United States
- Language:
- English
Similar Records
Hard x-ray bursts from flares behind the solar limb. Interim report
X-ray bursts from solar flares behind the limb
Energetic electrons, type III radio bursts, and impulsive solar flare X-rays
Technical Report
·
Thu Jun 19 00:00:00 EDT 1975
·
OSTI ID:7190144
X-ray bursts from solar flares behind the limb
Technical Report
·
Tue Dec 31 23:00:00 EST 1974
·
OSTI ID:4179209
Energetic electrons, type III radio bursts, and impulsive solar flare X-rays
Journal Article
·
Sat Aug 01 00:00:00 EDT 1981
· Astrophys. J.; (United States)
·
OSTI ID:5973595