Abstract
Simple bounds on the growth rates of magneto-atmospheric instabilities are derived, both for perturbations along and perpendicular to a horizontal magnetic field. The physical significance of a singular level for stable modes is briefly discussed.
References
Acheson, D. J.: 1972,J. Fluid Mech. 53, 401.
Acheson, D. J.: 1973,J. Fluid Mech. 58, 27.
Adam, J. A.: 1977a,Astrophys. Space Sci. (in press).
Adam, J. A.: 1977b,Quart. J. Mech. Appl. Math. (in press).
Adam, J. A.: 1977c,Astron. Astrophys. (in press).
Adam, J. A.: 1977d,Solar Physics (in press).
Yu, C. P.: 1965,Phys. Fluids 8, 650.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Adam, J.A. Maximum growth rates of magnetoatmospheric instabilities. Astrophys Space Sci 47, L5–L7 (1977). https://doi.org/10.1007/BF00651375
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00651375