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Hydromagnetic-gravity wave critical levels in the solar atmosphere

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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.

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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

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  • DOI: https://doi.org/10.1007/BF00160100

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