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Solar Radio Emission

  • A. D. Fokker
Part of the Astrophysics and Space Science Library book series (ASSL, volume 69)

Abstract

Outside active regions the Sun produces radio emission that is due entirely to bremsstrahlung from thermal electrons — the quiet-Sun radio emission. Radiation of frequency f originates at and above the level where f = f p (= plasma frequency), i.e. meter wavelengths in the corona, decimeter wavelengths in the transition region and centimeter wavelengths in the chromosphere. The spectrum is shown in Figure 11.1.

Keywords

Solar Phys Radio Emission Plasma Wave Solar Radio Spike Burst 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1977

Authors and Affiliations

  • A. D. Fokker

There are no affiliations available

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