The investigation of instabilities adopting the point of view of inhomogeneous mass flow, physically corresponds to consideration of stability of the perturbations whose wavelengths in the direction of plasma inhomogeneities are much larger than the characteristic plasma scale length. The dissipation of hydromagnetic-waves and instabilities takes place due to the inhomogeneous plasma flow. Both the velocity and plasma density vary in the direction perpendicular to the magnetic field. It is found that the Alfvén wave branch and magnetosonic branch may be driven unstable by the velocity shear. Instability, oscillatory modes, marginal instability and overstability are worked out.
This is a preview of subscription content, log in to check access.
Buy single article
Instant access to the full article PDF.
Price includes VAT for USA
Braginskii, S. I.: 1965, in M. A. Leontovich (ed.),Review of Plasma Physics, Vol. 1, Academic Press, New York, p. 217.
D'Angelo, N.: 1965,Phys. Fluids 8, 1948.
Dobrowlny, M. and D'Angelo, N.: 1972, in K. Schindler (ed.),Cosmic Plasma Physics, Plenum Press, New York, p. 149.
Fejev, J. A.: 1965,Phys. Fluids 7, 499.
Hung, R. J. and Barnes, A.: 1973a,Astrophys. J. 180, 253.
Hung, R. J. and Barnes, A.: 1973b,Astrophys. J. 180, 271.
Hung, R. J. and Barnes, A.: 1973c,Astrophys. J. 181, 183.
Jokipii, J. R. and Davis, L.: 1969,Astrophys. J. 156, 1101.
Parker, E. N.: 1964,Astrophys. J. 139, 690.
Smith, C. G. and Von Goeler, S.: 1968,Phys. Fluids 11, 2665.
Srivastava, K. M. and Singh, R.: 1981,Astrophys. Space Sci. 79, 37.
About this article
Cite this article
Singh, R., Srivastava, K.M. Dissipation of MHD waves in an inhomogeneous streaming plasma. Astrophys Space Sci 90, 3–18 (1983). https://doi.org/10.1007/BF00651543
- Magnetic Field
- Mass Flow
- Plasma Density
- Plasma Flow
- Oscillatory Mode