Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10...60l&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal, vol. 10, p. 60 (1984)
Astronomy and Astrophysics
Astronomy
Scientific paper
A possible plasma wave spectrum of a solar type III radio burst source
is pointed out which permits to explain weak nonlinear wave scattering
by ions in the frame of the quasi-linear generation model. The proposed
model permits to single out the range of characteristic velocity of the
burst agent propagation in the corona.
Lerner A. M.
Levin B. N.
Rapoport V. O.
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