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65. On the mechanism of solar outbursts

Published online by Cambridge University Press:  14 August 2015

K. O. Kiepenheuer
K. O. Kiepenheuer*
Affiliation:
Fraunhofer Institute, Freiburg im Breisgau, Germany

Extract

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Today it is taken for granted that the solar outbursts are produced by plasma oscillations of coronal matter, excited by a corpuscular radiation originating in the inner corona (Pawsey and Smerd, 1953) [1]. A certain component of this corpuscular radiation is obviously identical with that generating geomagnetic storms.

Type
Part V: The Active Sun
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 345 - 353
Copyright
Copyright © Cambridge University Press 1957 

References

1. Pawsey, J. L. and Smerd, S. F. in Kuiper, G. P., The Sun , pp. 508ff., Chicago, 1953.Google Scholar
2. Davies, R. D. M.N.R.A.S. 114, 74, 1955.CrossRefGoogle Scholar
3. Kiepenheuer, K. O., in Kuiper, G. P., The Sun , pp. 449ff., Chicago, 1953.Google Scholar
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6. Wild, J. P., Roberts, J. A. and Murray, J. D. Nature , 173, 532, 1954.CrossRefGoogle Scholar
7. Kiepenheuer, K. O. Report of the Cosmic Ray Conference, held at Guanajuato (Mexico) in September 1955, to be published.Google Scholar