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The Response of Microwave Emission to the Development of Active Regions

Published online by Cambridge University Press:  30 March 2016

G. Ya. Smolkov
G. Ya. Smolkov*
Affiliation:
SibIZMIR, USSR Academy of Sciences, P.O.Box 4, 664033 Irkutsk, USSR

Extract

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As is known from eclipse observations, the microwave emission of an active region consists of three main components: floccular, inter-spot (halo) and spot components which differ in intensity, the degree of polarization, and in structure and sizes /1/. A possibility of identifying the finer spatial and temporal structure in the active region (AR) emission has existed since RATAN, the VLA and WSRT became operational. The construction of the SSRT permitted the initiation of a systematic study of spatio-temporal properties of the development of active regions /2, 3/.

The majority of the properties in the AR development are reflected in detail and rapidly in the microwave emission characteristics /4, 6/.

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 755 - 757
Copyright
Copyright © Reidel 1986

References

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