Abstract
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.
Publisher
Cambridge University Press (CUP)
Reference4 articles.
1. Pawsey J. L. and Bracewell R. N. Radio Astronomy (Oxford, 1955).
2. Kosmische Strahlung (ed. Heisenberg W. ) (Berlin-Göttingen-Heidelberg, 1953).
3. Proc. Internat. Cosmic ray conference (Guanajuato, 1955), to be published.
4. Unsöld A. Physik der Sternatmosphären (2nd ed.) (Berlin-Göttingen-Heidelberg, 1955).
Cited by
1 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献