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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.Google Scholar
3. Kiepenheuer, K. O., in Kuiper, G. P., The Sun , pp. 449ff., Chicago, 1953.Google Scholar
4. Chapman, S. and Ferraro, V. C. A. J. Terr. Magn. Atm. El. 36, 77, 1931; ibid. 37, 421, 1932; and ibid. 38, 79, 1933.Google Scholar
5. Babcock, H. W. and Babcock, H. D. Ap. J. 121, 349, 1955.Google Scholar
6. Wild, J. P., Roberts, J. A. and Murray, J. D. Nature , 173, 532, 1954.Google Scholar
7. Kiepenheuer, K. O. Report of the Cosmic Ray Conference, held at Guanajuato (Mexico) in September 1955, to be published.Google Scholar