Distribution of Radio-Frequency Brightness across the Solar Disk and the Derivation of a Model Corona

Details Distribution of Radio-Frequency Brightness across the Solar Disk and the Derivation of a Model Corona Distribution of Radio-Frequency Brightness across the Solar Disk and the Derivation of a Model Corona

Jan 1954

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954natur.173..219o&link_type=abstract

Nature, Volume 173, Issue 4396, pp. 219 (1954).

Physics

3

Scientific paper

DETERMINATIONS of the distribution of radio-frequency brightness across the solar disk have been made by Stanier1 at a wave-length of 60 cm. and by Machin2 at a wave-length of 3.7 metres. A series of similar observations has been carried out by one of us3 at wave-lengths of 1.4, 3.7 and 7.9 metres during the period July 1951-July 1952. In this communication we describe the results of an attempt to derive a model of the corona which is consistent with these observations4.

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