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Observation of theS-component of the solar radio emission by an eight element grating interferometer at 17 Gc/s

✍ Scribed by Atsushi Tsuchiya; Kiyoshi Nagane


Book ID
104643278
Publisher
Springer
Year
1967
Tongue
English
Weight
213 KB
Volume
1
Category
Article
ISSN
0038-0938

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✦ Synopsis


The slowly varying components (S-components) of the solar radio emission were observed by a 17 Gc/s grating interferometer. In combination with 4 Gc/s data, it is deduced that the source of the 17 Gc/s S-component is optically thin.