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Production of Different Non-Thermal Electron Groups in Small Solar Flares*

Published online by Cambridge University Press:  12 April 2016

S. R. Kane
S. R. Kane*
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, Calif. 94720, U.S.A.

Extract

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Using the measurements of impulsive solar X-rays made with the OGO-5 satellite to identify the flash phase electron acceleration in solar flares of Hα-importance ≲ 1, the satellite and ground based observations are analyzed to study the origin of the different groups of non-thermal electrons responsible for the impulsive X-ray, impulsive microwave, type III radio and interplanetary electron emission.

Type
Section V / The Solar Flare Plasma
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 822 - 823
Copyright
Copyright © Reidel 1972

Footnotes

*

Research supported by NASA under Contract NAS 5-9094.

References

Anderson, K. A., Kane, S. R., and Lin, R. P.: 1970, Fast Electrons from Solar Flares, Presented at the International Seminar on the Problem of Cosmic Ray Generation on the Sun, Leningrad, U.S.S.R., December 1970 (UC Space Sciences Lab, Series 12, Issue 7).Google Scholar
De Jager, C. and Kundu, M. R.: 1963, in Priester, W. (ed.), Space Res. 3, 836, North-Holland Publ. Co., Amsterdam.Google Scholar
Wild, J. P.: 1964, AAS-NASA Symposium on Solar Flares, NASA SP-50.Google Scholar