Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-28T07:34:31.901Z Has data issue: false hasContentIssue false

Propagation of hydromagnetic waves in a perfectly conducting non-isothermal atmosphere in the presence of rotation and a variable magnetic field

Published online by Cambridge University Press:  19 April 2006

N. Rudraiah
Affiliation:
Department of Mathematics, Central College, Bangalore University, Bangalore-560001, India
M. Venkatachalappa
Affiliation:
Department of Mathematics, Central College, Bangalore University, Bangalore-560001, India

Abstract

The propagation of internal Alfvén-inertio-acoustic gravity waves in a perfectly electrically conducting, stratified, inviscid, non-isothermal, rotating atmosphere permeated by a non-uniform magnetic field is investigated. These waves exhibit singular properties at the critical levels at which the magnetic field and the sound velocity are such that \[ (\omega^2 - S^2)\{(c^2+V^2)\omega^2-c^2S^2\}-(c^2+V^2)\overline{R}^2=0, \] where ω is the frequency of the waves, $S = kV_x + lV_y,\overline{R} = 2\Omega_z\omega$, Vx and Vy are the x and y components of the Alfvén velocity, k and l are the corresponding wavenumbers and c is the sonic velocity. These levels act like valves which permit waves to penetrate them from one side only and absorb them when they propagate from the other side. In contrast to the incompressible results of Acheson (1972), we show that the valve effect in compressible flow no longer requires the presence of non-zero components of rotation in the plane normal to the direction in which the medium varies. We find that the compressibility increases the probability of a valve effect and so increases the capacity of a hydromagnetic wave to propagate across a field line, rather than being absorbed at some critical level.

Type
Research Article
Copyright
© 1978 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Acheson, D. J. 1972 J. Fluid Mech. 53, 401.
Acheson, D. J. & Hide, R. 1973 Rep. Prog. Phys. 36, 159.
Booker, J. R. & Bretherton, F. P. 1967 J. Fluid Mech. 27, 513.
Bretherton, F. P. 1966 Quart. J. Roy. Met. Soc. 92, 466.
Eltayeb, I. A. 1977 Phil. Trans. Roy. Soc. A 285, 607.
Grimshaw, R. 1975 J. Fluid Mech. 70, 287.
Gossard, E. E. & Hooke, W. H. 1975 Waves in the Atmosphere. Elsevier.
Hines, C. O. 1968 J. Atmos. Terr. Phys. 30, 837.
Hines, C. O. 1974 The Upper Atmosphere in Motion. Washington: Am. Geophys. Un.
Jones, W. L. 1967 J. Fluid Mech. 30, 439.
Mckenzie, J. F. 1973 J. Fluid Mech. 58, 709.
Rudraiah, N. & Venkatachalappa, M. 1972a J. Fluid Mech. 52, 1093.
Rudraiah, N. & Venkatachalappa, M. 1972b J. Fluid Mech. 54, 209.
Rudraiah, N. & Venkatachalappa, M. 1972c J. Fluid Mech. 54, 217.
Rudraiah, N. & Venkatachalappa, M. 1974 J. Fluid Mech. 62, 705.
Rudraiah, N., Venkatachalappa, M. & Kandaswamy, P. 1976 J. Fluid Mech. 73, 125.
Rudraiah, N., Venkatachalappa, M. & Kandaswamy, P. 1977 J. Fluid Mech. 80, 223.