Spectral Characteristics of Type II Solar Radio Bursts

Details Spectral Characteristics of Type II Solar Radio Bursts Spectral Characteristics of Type II Solar Radio Bursts

Oct 1961

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1961natur.192...58s&link_type=abstract

Nature, Volume 192, Issue 4797, pp. 58 (1961).

Computer Science

18

Scientific paper

IT has been, recognized for some time that Type II solar radio bursts are due to the excitation of plasma oscillations in the solar corona by some exciting agency which moves through the corona. Roberts1, in reviewing observations and theories of these phenomena, leaves unexplained two salient characteristics: (1) the appearance of radiation at the fundamental and second harmonic at comparable powers and the lack of radiation at all higher harmonics; (2) the frequent splitting of each of these two `lines' into a pair of lines, the fractional splitting of each of these two pairs being the same, typically a few per cent.

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