Abstract
It is shown that the discontinuous jump in the vertical wave energy flux of slow hydromagnetic-gravity waves, occurring at a critical level, which is accompanied by wave absorption, and the existence of a reflection point imply that slow waves are trapped in the solar atmosphere. Thus such a system behaves as a leaky wave guide.
Similar content being viewed by others
References
Adam, J. A.: 1977, Solar Phys. 52, 293.
Booker, J. R. and Bretherton, F. P.: 1967, J. Fluid Mech. 27, 513.
Eltayeb, I. A. and McKenzie, J. F.: 1977, J. Fluid Mech. 81, 1.
Lighthill, M. J.: 1967, IAU Symp. 28, 429.
McKenzie, J. F.: 1973, J. Fluid Mech. 58, 709.
Miles, J. W.: 1961, J. Fluid Mech. 10, 496.
Nye, A. H. and Thomas, J. H.: 1974, Solar Phys. 38, 399.
Nye, A. H. and Thomas, J. H.: 1976, Astrophys. J. 204, 582.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
El Mekki, O., Eltayeb, I.A. & McKenzie, J.F. Hydromagnetic-gravity wave critical levels in the solar atmosphere. Sol Phys 57, 261–266 (1978). https://doi.org/10.1007/BF00160100
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00160100