Solar Radio-Frequency Noise Fluctuations and Chromospheric Flares

Details Solar Radio-Frequency Noise Fluctuations and Chromospheric Flares Solar Radio-Frequency Noise Fluctuations and Chromospheric Flares

Nov 1947

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1947natur.160..708w&link_type=abstract

Nature, Volume 160, Issue 4073, pp. 708-709 (1947).

Physics

1

Scientific paper

Martyn1 and Shklovsky2 have suggested that plasma
oscillations in the corona may provide a source of radio-frequency
radiation. It has also been shown that radiation of a few metres
wave-length must originate at heights above the chromosphere of the
order of a solar radius.

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