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Some properties of the sources of slowly varying component and of bursts at 612 Mc/s∗

Published online by Cambridge University Press:  14 August 2015

G. Swarup ,
M. R. Kundu ,
V. K. Kapahi  and
J. D. Isloor
G. Swarup
Affiliation:
Tata Institute of Fundamental Research, Bombay 5, India
M. R. Kundu
Affiliation:
Tata Institute of Fundamental Research, Bombay 5, India
V. K. Kapahi
Affiliation:
Tata Institute of Fundamental Research, Bombay 5, India
J. D. Isloor
Affiliation:
Tata Institute of Fundamental Research, Bombay 5, India

Extract

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A high-resolution 24-element, E–W interferometer situated at Kalyan near Bombay has been used to study the sources of slowly varying component and of bursts at a frequency of 612 Mc/s. This interferometer has a half-power beamwidth of 2·8 min of arc, and the fan beams are located about a degree apart in the sky. Thus, a strip scan is obtained roughly every 4 min as the Sun drifts through the beams. About 20 slowly varying sources and 11 bursts were observed during the period June 1965 to February 1967 at 612 Mc/s.

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. 581 - 584
Copyright
Copyright © Reidel 1968