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Some remarks on the polarization of 200-Mc/s solar radio emission

Published online by Cambridge University Press:  14 August 2015

M. H. Cohen  and
A. D. Fokker
M. H. Cohen
Affiliation:
Cornell University, Ithaca, New York, U.S.A.
A. D. Fokker
Affiliation:
Ionosphere and Radio Astronomy Section, Netherlands Postal and Telecommunications Services The Hague, The Netherlands

Extract

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Detecting a weak linearly polarized component in an isolated solar burst is very difficult. It is a unique event and it is not possible to make a series of observations to reduce the error. Interference and reflections confuse the result and it is extremely difficult to determine the equipment parameters precisely, especially those pertaining to the antenna.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 252 - 258
Copyright
Copyright © Stanford University Press 1959 

References

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