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The origin of the slowly varying component

Published online by Cambridge University Press:  14 August 2015

W. N. Christiansen  and
D. S. Mathewson
W. N. Christiansen
Affiliation:
Radiophysics Laboratory, Commonwealth Scientific and Industrial Research Organization, Sydney, Australia
D. S. Mathewson
Affiliation:
Radiophysics Laboratory, Commonwealth Scientific and Industrial Research Organization, Sydney, Australia

Extract

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Two main mechanisms have been proposed to explain the origin of the slowly varying component [1] of the decimeter-wavelength radiation from the sun. Both theories [2, 3, 4] are based on the facts that (a) this component of the sun's radiation is relatively steady in output for periods of days; (b) it originates from active regions on the sun; and (c) its magnitude is closely related to the sunspot area in the region.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 108 - 117
Copyright
Copyright © Stanford University Press 1959 

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