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Measuring the Whole-Sun Intensity at Decimetre Wavelengths

Published online by Cambridge University Press:  25 April 2016

T. L. Landecker
T. L. Landecker*
Affiliation:
School of Electrical Engineerings, University of Sydney
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Extract

The study of the sources of the slowly varying component at decimetre and centimetre wavelengths has been a major preoccupation of solar radio astronomers. Grating interferometers and other high-resolution aerial systems have enabled the separation of the S-component from the Sun’s total emission, and the study of individual sources. Nevertheless much of value remains to be derived from whole-sun intensity measurements—the most basic solar radio observation.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 2 , November 1967 , pp. 61 - 62
Copyright
Copyright © Astronomical Society of Australia 1967

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References

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