Solar Radio Asymmetry at 4-Metres Wave-length

Details Solar Radio Asymmetry at 4-Metres Wave-length Solar Radio Asymmetry at 4-Metres Wave-length

Apr 1954

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954natur.173..771h&link_type=abstract

Nature, Volume 173, Issue 4408, pp. 771 (1954).

Physics

2

Scientific paper

IN 1948, Hey, Parsons and Phillips1 reported that at 4.1-metres wave-length bursts of radio emission, usually of a few minutes duration, occurred more often in association with flares on the eastern half of the sun's disk than on the western half. Subsequent observations have confirmed this conclusion. In a recent analysis of radio emissions at 1.5-metres wavelength, Dodson, Hedeman and Owren2 could find no evidence of this asymmetry. The following reasons may explain why they failed to observe the effect.

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