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Synchrotron radiation and solar radio outbursts at microwave frequencies

Published online by Cambridge University Press:  14 August 2015

T. Takakura
T. Takakura*
Affiliation:
The Observatory, University of Michigan, Ann Arbor, Michigan, U.S.A.

Extract

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The characteristics and the generation mechanisms of solar radio outbursts seem to be distinct at the frequencies above and below a certain cross-over frequency somewhere between 300 and 600 Mc/s (see Table I).

Type
Part VI: Mechanisms of Solar and Cosmic Emission
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 562 - 570
Copyright
Copyright © Stanford University Press 1959 

References

1. Schwinger, J. Phys. Rev. 75, 1912, 1949.Google Scholar
2. Tanaka, H., and Kakinuma, T. Meeting of Astronomical Society of Japan. 1957.Google Scholar