The objects of research in this work are evanescent wave modes in a gravitationally
stratified atmosphere and their associated pseudo-modes. Whereas the former, according to …

In this theoretical exploration, the stabilizing or destabilizing impacts of the rotation, electron
inertia, and electrical resistivity on the Kelvin–Helmholtz stability in two-superimposed …

The boundary stability problem is solved for a dipole magnetosphere wrapped by an
azimuthal solar wind flow. A simplified equation is obtained describing small‐scale fast …

The spatial structure of ultra‐low‐frequency (ULF) fast magnetosonic (FMS) waves is
calculated in the dayside magnetosphere. A balanced model is developed of a dipole …

Recent observations support the propagation of a number of magnetohydrodynamic (MHD)
modes which, under some conditions, can become unstable and the developing instability is …

Описаны математические и теоретические методы исследования продольных и косых
МГД-мод, генерируемых солнечным ветром и локализованных вблизи границы …

The main attention is paid to the construction of a mathematical model and the description of
methods for studying magnetic hydrodynamic (MHD) waves propagating in the" tail" of the …

В настоящей работе изучаются магнитогидродинамические (МГД) волны в системе
«неподвижный плоский плазменный слой–внешняя движущаяся плазма». Такая задача …