First results from the Clark Lake Multifrequency Radioheliograph

Details First results from the Clark Lake Multifrequency Radioheliograph First results from the Clark Lake Multifrequency Radioheliograph

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...83..385k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 83, March 1983, p. 385-389.

Astronomy and Astrophysics

Astronomy

23

Radio Astronomy, Solar Corona, Solar Radio Emission, Spectroheliographs, Astronomical Maps, Decametric Waves, Photomapping, Plasma Diagnostics, Temporal Resolution, Very High Frequencies

Scientific paper

The characteristics of the Clark Lake Multifrequency Radioheliograph, which is presently being used for solar research in the frequency range 20-125 MHz, are examined and several solar maps obtained with this instrument are presented. Two-dimensional images of the sun's corona at several frequencies within this range are examined, which were obtained with time resolution as good as 1.28 s. It is found that the shape of the sun's outer corona as observed at meter-decameter wavelengths appears to change in time periods as short as a few seconds.

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