Modulational instability of finite-amplitude, circularly polarized Alfven waves

Details Modulational instability of finite-amplitude, circularly polarized Alfven waves Modulational instability of finite-amplitude, circularly polarized Alfven waves

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...224.1013d&link_type=abstract

Astrophysical Journal, Part 1, vol. 224, Sept. 15, 1978, p. 1013-1016.

Computer Science

Sound

56

Circular Polarization, Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Plasma Decay, Solar Wind, Hydrodynamic Equations, Ion Acoustic Waves, Wave Propagation

Scientific paper

The simple theory of the decay instability of Alfven waves is strictly applicable only to a small-amplitude parent wave in a low-beta plasma, but, if the parent wave is circularly polarized, it is possible to analyze the situation without either of these restrictions. Results show that a large-amplitude circularly polarized wave is unstable with respect to decay into three waves, one longitudinal and one transverse wave propagating parallel to the parent wave and one transverse wave propagating antiparallel. The transverse decay products appear at frequencies which are the sum and difference of the frequencies of the parent wave and the longitudinal wave. The decay products are not familiar MHD modes except in the limit of small beta and small amplitude of the parent wave, in which case the decay products are a forward-propagating sound wave and a backward-propagating circularly polarized wave. In this limit the other transverse wave disappears. The effect of finite beta is to reduce the linear growth rate of the instability from the value suggested by the simple theory. Possible applications of these results to the theory of the solar wind are briefly touched upon.

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