Abstract
Alfvénic drift Kelvin-Helmholtz instability is discussed in the presence of equilibrium electric and magnetic fields which are perpendicular to each other. A dispersion relation is achieved with the help of WKB approximation and the instability criterion is established. A comparison is made with the previous studies and it is shown that the electric field has a stabilizing or destabilizing effect on the system according to the conditions discussed in the text.
Similar content being viewed by others
References
Bavassano, B., Dobrowolny, M., and Moreno, G.: 1978,Solar Phys. 57, 445.
Catto, P. J., Rosenbluth, M. N., and Liu, C. S.: 1973,Phys. Fluids 16, 1719.
D'Angelo, N.: 1973,J. Geophys. Res. 78, 1206.
Dobrowolny, M.: 1972,Phys. Fluids 15, 2263.
Mikhailovskii, A. B.: 1982,J. Plasma Phys 28, 1.
Mikhailovskii, A. B. and Klimenko, V. A.: 1980,J. Plasma Phys. 24, 385.
Sharma, A. C. and Srivastava, K. M.: 1992 (submitted).
Stix, T. H.: 1973,Phys. Fluids 16, 1922.
Vyas, D. N., Singh, R., and Srivastava, K. M.: 1983,Astrophys. Space Sci. 90, 351.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Sharma, A.C., Srivastava, K.M. Alfvénic drift Kelvin-Helmholtz instability in the presence of an equilibrium electric field. Astrophys Space Sci 197, 145–151 (1992). https://doi.org/10.1007/BF00645078
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00645078