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Uncertainties in the magnetized plasma viscosity remain as an obstacle to unambiguous tests of the results in the case of real plasmas.
Relativistic effects are known to be important in magnetized thermal plasmas near perpendicular propagation, even when they would otherwise be considered weak.
A comparatively small number of dust particles can thus drastically alter the behavior of the nonlinear structures in magnetized plasmas.
It was shown that the considered effects must be taken into account if the electrons are magnetized.
We consider the parameter regime in which the ions and electrons are strongly magnetized, while the charged dust is unmagnetized.
Thus, the ions and electrons are magnetized but the dust is unmagnetized.
It is assumed that the magnetic field strength is such that the ions and electrons are magnetized, while the dust is unmagnetized.
The electrons and ions are magnetized, while the dust is unmagnetized.
These results provide useful information on the self-gravitational effects and magnetic field effects on the surface dust-ion-acoustic mode in semi-bounded self-gravitating magnetized dusty plasmas.
The transitions and the self-gravitational effects on the surface dust-ionacoustic mode are investigated in semi-bounded magnetized dusty plasmas.
The equations are then used to investigate decay and modulational instabilities in magnetized dusty plasmas.
As will be seen below, this has profound effects on the nonlinear dynamics of magnetized dusty plasmas.
We derive the dielectric tensor for multicomponent magnetized dusty plasmas, including the effect of capture of plasma electrons and ions by the dust particles.
We initially input turbulent velocity into the magnetized plate-shaped cloud which is in hydrostatic equilibrium between thermal pressure and self-gravity.
Using the somewhat inaccessible result of the general theory, we deduce the explicit expressions for the coupling coefficients of a cold magnetized two-component plasma.
