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Scattering of Radio Waves in the Solar Corona

Published online by Cambridge University Press:  25 April 2016

R. D. Robinson
R. D. Robinson*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Radiation generated in the solar corona can be drastically altered by refraction and scattering as it escapes. This is especially true for sources having a frequency near the local plasma frequency, where the index of refraction approaches zero. Early investigations of the problem (e.g. Fokker 1965; Steinberg et al. 1971; Riddle 1972, 1974) have shown that the size, shape, location, intensity and time profile for the observed source can all be influenced.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 208 - 211
Copyright
Copyright © Astronomical Society of Australia 1983

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References

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