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42. Radio astronomy and the origin of cosmic rays

Published online by Cambridge University Press:  14 August 2015

A. Unsöld
A. Unsöld*
Affiliation:
Director of the Institute for Theoretical Physics and of the Observatory, Kiel, Germany

Extract

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At present we can observe the origin of only the solar component of cosmic rays. The sun emits cosmic rays in connexion with flares and probably also continuously on a smaller scale. Thus the emission of cosmic rays appears to be connected much more closely with non-thermal radio emission than with thermal radiation of light and heat.

Type
Part III: Galactic Structure and Statistical Studies of Point Sources
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 238 - 240
Copyright
Copyright © Cambridge University Press 1957 

References

Kosmische Strahlung (ed. Heisenberg, W.) (Berlin-Göttingen-Heidelberg, 1953).Google Scholar
Pawsey, J. L. and Bracewell, R. N. Radio Astronomy (Oxford, 1955).Google Scholar
Proc. Internat. Cosmic ray conference (Guanajuato, 1955), to be published.Google Scholar
Unsöld, A. Physik der Sternatmosphären (2nd ed.) (Berlin-Göttingen-Heidelberg, 1955).CrossRefGoogle Scholar