Parametric instabilities in shallow water magnetohydrodynamics of astrophysical plasma in external magnetic field
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文摘

Revised magnetohydrodynamic shallow water equations in external vertical magnetic field

Principal three-dimensionality of the magnetic field vector in revised magnetohydrodynamic shallow water equations

Prediction of three-wave interactions and parametric instabilities in rotating MHD thin layer of astrophysical plasma

New avenues of research in neutron stars atmospheres, in solar physics, in atmospheres of tidally locked exoplanets

The vertical magnetic field essentially changes the wave dynamics compared to plasma layer in a toroidal magnetic field

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