Damping of nonlinear magneto-acoustic waves
Abstract
Nonlinear magneto-acoustic waves in a turbulent plasma are simulated by collisional MHD equations. Damping of these waves due to electrical conductivity arising from micro-instabilities and collisional viscosity are analyzed. Numerical investigation of competing effects due to non-linearity and dissipation has been carried out. It is found that finite amplitude perturbation leads to the formation of a shock in both the slow and the fast mode propagation. Collisional viscosity plays an important role in the damping of nonlinear magneto-acoustic waves in the astrophysical and space plasmas.
- Publication:
-
Journal of Plasma Physics
- Pub Date:
- August 1978
- DOI:
- Bibcode:
- 1978JPlPh..20..125K
- Keywords:
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- Cosmic Plasma;
- Elastic Damping;
- Magnetoacoustic Waves;
- Plasma Turbulence;
- Plasma Waves;
- Wave Attenuation;
- Burger Equation;
- Electrical Resistivity;
- Propagation Modes;
- Shock Wave Propagation;
- Solar Corona;
- Viscosity;
- Plasma Physics