Origin of Radio Emissions from the Disturbed Sun

Details Origin of Radio Emissions from the Disturbed Sun Origin of Radio Emissions from the Disturbed Sun

Jan 1947

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1947natur.159...26m&link_type=abstract

Nature, Volume 159, Issue 4027, pp. 26-27 (1947).

Physics

17

Scientific paper

IN a recent communication1 it was pointed out that thermal radiation from the solar corona should be detectable at wave-lengths as long as one or two metres. This source cannot account, however, for the much stronger emissions which are correlated with sunspots2,3,4. It has been shown5,6 that the latter emissions probably come from the immediate vicinity of active sunspots, and would require impossibly high source temperatures of about 109 degrees for explanation in terms of thermal radiation.

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