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Dissipation of hydromagnetic waves in viscous polytropic zone of solar wind including FLR corrections, Ohmic diffusion and Hall effect
In the polytropic zone of the solar wind, we have used the generalized polytrope pressure laws to investigate the dissipation of hydromagnetic waves and pressure anisotropy driven fluid instabilities in magnetized viscous plasmas including finite Larmor radius (FLR) corrections and non-ideal magnetohydrodynamic (MHD) effects. The modified dispersion properties have been analyzed in the MHD and Chew-Goldberger-Low (CGL) limits for typical conditions of solar wind and corona. The theoretical results are found to be in good agr ...
Prajapati, Ram; Desta, Ephrem; Fok, Mei-Ching; Eritro, Tigistu;
Published by: \mnras Published on: jun
YEAR: 2022   DOI: 10.1093/mnras/stac1743
plasmas; MHD; waves; instabilities; Solar wind; Solar corona; magnetic fields