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