Conductivity of an ion-acoustically turbulent plasma

Details Conductivity of an ion-acoustically turbulent plasma Conductivity of an ion-acoustically turbulent plasma

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...59...29k&link_type=abstract

Solar Physics, vol. 59, Sept. 1978, p. 29-42.

Physics

2

Ion Acoustic Waves, Plasma Conductivity, Plasma Turbulence, Solar Physics, Acoustic Scattering, Damping, Density Wave Model, Magnetohydrodynamic Stability, Plasma-Particle Interactions, Saturation, Skylab Program, Solar Flares, Wave Interaction

Scientific paper

Three possible mechanisms for nonlinear saturation of ion-acoustic instability are discussed: (1) wave mediated wave-particle interaction; (2) scattering of ion-acoustic waves by steady state density fluctuations; and (3) resonant wave-modified particle interaction. Values of anomalous plasma conductivity obtained in the study are used to estimate the magnitude of magnetic field gradients in the magnetically neutral sheet of the solar corona. Results are compared with Skylab data.

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