Linear stability and MHD wave propagation in plasmas with solar abundances

Details Linear stability and MHD wave propagation in plasmas with solar abundances Linear stability and MHD wave propagation in plasmas with solar abundances

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311...41i&link_type=abstract

In ESA, Plasma Astrophysics p 41-44 (SEE N91-15046 06-90)

Physics

Linearity, Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Wave Equations, Wave Propagation, Critical Point, Damping, Magnetoacoustic Waves, Plasmas (Physics), Solar Activity, Wave Amplification

Scientific paper

The local stability and the MHD (magnetohydrodynamic) propagation of linear waves in optically thin plasmas are analyzed. From Hurwitz's criteria the critical wave numbers for unstable disturbances are found. For the wave driven case, a dispersion relation for propagation of thermal and magnetosonic waves were obtained. Analytical conditions for amplification and damping are given for several asymptotic cases.

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