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• W2049442980 abstract "The effects, hitherto not treated, of the temperature and the number density gradients, both in the parallel and the perpendicular direction to the magnetic field, of O VI ions, on the MHD wave propagation characteristics in the solar North Polar Coronal Hole are investigated. We investigate the magnetosonic wave propagation in a resistive MHD regime where only the thermal conduction is taken into account. Heat conduction across the magnetic field is treated in a non-classical approach wherein the heat is assumed to be conducted by the plasma waves emitted by ions and absorbed at a distance from the source by other ions. Anisotropic temperature and the number density distributions of O VI ions revealed the chaotic nature of MHD standing wave, especially near the plume/interplume lane borders. Attenuation length scales of the fast mode is shown not to be smoothly varying function of the radial distance from the Sun (© 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
• W2049442980 created "2016-06-24" @default.
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• W2049442980 creator A5062886393 @default.
• W2049442980 date "2010-07-21" @default.
• W2049442980 modified "2023-09-25" @default.
• W2049442980 title "MHD waves in the solar north polar coronal hole" @default.
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• W2049442980 doi "https://doi.org/10.1002/asna.200911359" @default.
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