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The Third Harmonic in Solar Radio Bursts
Published online by Cambridge University Press: 25 May 2016
Abstract
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
- Information
- Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 289 - 290
- Copyright
- Copyright © Reidel 1974
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