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Measuring the Whole-Sun Intensity at Decimetre Wavelengths
Published online by Cambridge University Press: 25 April 2016
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