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The Third Harmonic in Solar Radio Bursts

Published online by Cambridge University Press:  25 May 2016

V. V. Zheleznyakov
Affiliation:
Radiophysical Research Institute, Gorkii, U.S.S.R.
E. Ya. Zlotnik
Affiliation:
Radiophysical Research Institute, Gorkii, U.S.S.R.

Abstract

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Generation of third harmonic plasma emission by coalescence of second harmonic radiation with a plasma wave is more favourable than by direct coalescence of three plasma waves. The predicted ratio of the intensities at the third (III) and second (II) harmonics is IIIIω/IIIω ~ ωLWlL/Nmc3, where ωL is the plasma frequency, Wl is the energy density in plasma waves, L the linear dimensions of the source and N the ambient electron number density. The intensity at the second harmonic is where LN(∼1010 cm at ωL ∼ 2π × 108 s−1) is the typical dimension of coronal inhomogeneities.

Type
Part II The Flash Phase of Solar Flares
Copyright
Copyright © Reidel 1974