Origin of Solar Radiation in the 1 6 Metre Radio Wave-lenght Band

Details Origin of Solar Radiation in the 1 6 Metre Radio Wave-lenght Band Origin of Solar Radiation in the 1 6 Metre Radio Wave-lenght Band

Sep 1946

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1946natur.158..340k&link_type=abstract

Nature, Volume 158, Issue 4010, pp. 340 (1946).

Physics

8

Scientific paper

THE intensity of the solar radiation in the wave-length region of a few metres sometimes deviates extraordinarily from that for a black body at 6000°. The observed departures show a clear correlation with sunspots and their heliographic positions, and become extremely high during the appearance of chromospheric eruptions1. As can be shown, even the intensity of the corona, which will radiate in this spectral region nearly like a black body at 106 degrees, falls short of the observed values.

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