Physics
Scientific paper
Feb 1957
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1957natur.179..371k&link_type=abstract
Nature, Volume 179, Issue 4555, pp. 371 (1957).
Physics
Scientific paper
THREE of the most important solar disturbances observed during 1956 were the great eruptive prominence of February 10 and the large flares of May 17 and August 31. For a week or two after each of these events, a sequence of phenomena involving Venus, the Earth and the Moon were observed with a radio telescope operating on a wave-length of 11 m.1, these events appearing to be related to the preceding solar disturbance. In one case strong signals of apparent Venusian origin were observed a number of days after the solar disturbance, and a few days later a phenomenon was observed which, presumably, was caused by the presence of a large ion cloud near the Moon. Such a sequence of events suggests that a stream of particles ejected by the Sun and travelling earthward first encountered the planet Venus, resulting directly or indirectly in the production of strong 11-m. radio signals from Venus. Drifting farther out, the particles reached the vicinity of the Earth, with some of the particles forming a cloud near the Moon.
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