In the partially ionized solar chromosphere, viscosity can dominate magnetic diffusion and, together with Hall and gyroviscous effects, can destabilize waves in shear flows.
A., Ma\'rquez I., S\'anchez J
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Viscous Heating and Instabilities in the Partially Ionized Solar Atmosphere
In the partially ionized solar chromosphere, viscosity can dominate magnetic diffusion and, together with Hall and gyroviscous effects, can destabilize waves in shear flows.