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Properties of sources of the slowly varying component of 2 cm solar radio emission

Published online by Cambridge University Press:  14 August 2015

V. G. Nagnibeda
V. G. Nagnibeda*
Affiliation:
Astronomical Observatory of Leningrad University, Leningrad V-178, U.S.S.R.

Extract

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To study the nature of the local sources of solar radio emission connected with active regions, it is important to investigate the structure of such sources and their emission spectra. These problems are being investigated in detail by a group of workers of the Radio Astronomy Department of the Pulkovo Observatory led by G.B. Gelfreikh. The Pulkovo large radio telescope used for the observations allows them to investigate the solar radio sources at the whole cm-wavelength range with a high resolution reaching 40 sec of arc at the 2-cm wave. Observations are taken at 2·0, 3·2, 4·4, 6·6, and 9-cm waves. The author observes at the 2-cm wave.

Type
Part VIII: Radio Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 575 - 580
Copyright
Copyright © Reidel 1968 

References

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