Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-06T06:18:29.577Z Has data issue: false hasContentIssue false
  • English
  • Français

The determination of the energy distribution of relativistic electrons by the frequency distribution of their “synchrotron radiation”

Published online by Cambridge University Press:  14 August 2015

G. Wallis
G. Wallis*
Affiliation:
Heinrich Hertz-Institute, Berlin-Adlershof, Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Relativistic electrons moving in a homogeneous magnetic field H emit “synchrotron radiation” with a frequency distribution which may be written in the following form.

Type
Part VI: Mechanisms of Solar and Cosmic Emission
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 595 - 597
Copyright
Copyright © Stanford University Press 1959 

References

1. Ivanenko, D., and Sokolov, A. Dokl. Akad. Nauk S.S.S.R. 59, 1551, 1948.Google Scholar
2. Schwinger, J. Phys. Rev. 75, 1912, 1949.Google Scholar