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Observation of a Coronal Impulsive X-ray Burst and its Implications Regarding the Associated Microwave Source
Published online by Cambridge University Press: 14 August 2015
Summary
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Radial structure of impulsive hard X-ray and microwave sources in solar flares is not well known at the present time. Measurements of near-the-limb flares with a high spatial and temporal resolution is, of course, the best way to determine the radial structure of these sources. In absence of such measurements, particularly for the hard X-ray emission, behind-the-limb flares provide (through occultation) a means of observing the coronal part of the impulsive source. Here we summarize the characteristics of the impulsive coronal X-ray source deduced from multi-spacecraft observations of a behind-the-limb flare and their implications with respect to impulsive microwave source.
- Type
- Session VII - Solar Bursts - Radio, White Light and X-ray Observations
- Information
- Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 443 - 444
- Copyright
- Copyright © Reidel 1980
References
Kane, S. R., 1973, in Ramaty, R. R. and Stone, R. G. (eds.), High Energy Phenomena on the Sun, NASA SP-342, p. 55.Google Scholar
Kane, S. R., 1974, in Newkirk, G. Jr. (ed.), Coronal Disturbances, IAU Symp. 57, D. Reidel Publ. Co., Holland, p. 105.Google Scholar
Kane, S. R., Anderson, K. A., Evans, W. D., Klebesadel, R. W., and Laros, J., 1979, Astrophys. J. Letters, (in press).Google Scholar
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