Abstract
Observations are described of the spectrum
of outbursts of solar radio-frequency radiation in the frequency range 70-130
Mc/s. In accordance with Part I of this series, an " outburst " is
defined as a burst having a particular type of " dynamic " spectrum,
characterized by a drift of spectral features, with time, towards the lower
frequencies at a rate of the order of � Mc/s. per second. The observed
outbursts are shown to have a close connexion with solar flares and their
geophysical accompaniments.
�� The
spectra are tentatively interpreted in terms of the motion of a physical agency
in the solar atmosphere. The possible identification of the agency with "
surge " prominences and the corpuscular streams that cause a type of
terrestrial magnetic storm is discussed. It is shown that the evidence is quite
consistent with the hypothesis that the agency corresponds to the magnetic
storm particles.
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