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- W102902455 abstract "A common form of wave propagation in the highly structured magnetic fields and density profiles of the solar atmosphere should be magnetohydrodynamic surface waves, i.e. waves with magnetic and velocity fields concentrated at an interface of two regions of plasma of differing properties. For example, local concentrations of equilibrium magnetic fields forming flux tubes will support these waves on their surfaces, in addition to the more commonly considered ‘body waves’ that are supported by an isolated flux tube, waves with an oscillatory radial dependence inside the tube. Mhd surface waves have recently been identified in a laboratory plasma at Sydney University (Collins, Cramer and Donnelly 1983)." @default.
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- W102902455 date "1983-01-01" @default.
- W102902455 modified "2023-09-25" @default.
- W102902455 title "Resonant Alfvén Wave Absorption in Solar Magnetic Fields" @default.
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- W102902455 doi "https://doi.org/10.1017/s1323358000016842" @default.
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