Large-amplitude MHD waves are routinely observed in space plasmas. We suggest that dispersive focusing, previously proposed for the excitation of freak waves in the ocean, can be also responsible for the excitation of short-lived large-amplitude MHD waves in space plasmas. The DNLS equation describes MHD waves propagating in plasmas at moderate angles with respect to the equilibrium magnetic field. We obtained an analytical solution of the linearised DNLS equation governing the generation of large-amplitude MHD waves from small-amplitude wave trains due to the dispersive focusing. Our numerical solutions of the full DNLS equation confirm this result
MHD - magnetohydrodynamicsSIGLEAvailable from British Library Document Supply Centre-DSC:DXN006719 /...
Context. Transport of flare energy from the corona to the chromosphere has traditionally b...
On the basis of a numerical solution of dispersion equation we analyze characteristics of low-dampin...
Large-amplitude MHD waves are routinely observed in space plasmas. We suggest that dispersive focusi...
Generation of large-amplitude short-lived wave groups from small-amplitude initial perturbations in ...
The nonlinear coupling of MHD waves in a cold (beta = 0) compressible plasma with a smoothly inhomog...
Restricted Access.The exact nonlinear cylindrical solution for incompressible Hall magnetohydrodynam...
Context. Magnetohydrodynamic (MHD) waves are ubiquitous in the solar corona where the highly structu...
The one-dimensional oblique propagation of magnetohydrodynamic waves with arbitrary amplitudes in a ...
In this paper a numerical study of the propagation and dissipation properties of magnetohydro-dynami...
Aims. In the approximation of linear dissipative magnetohydrodynamics (MHD), it can be shown that dr...
Large amplitude magnetic field fluctuations often accompanied by density variations are frequently o...
We investigate the interaction of magnetohydrodynamic waves with plasma density inhomogeneities. Our...
Magnetohydrodynamic (MHD) waves play an important role in the solar atmosphere both directly (or int...
In this study, we numerically investigate the excitation of MHD waves in the interchange reconnectio...
MHD - magnetohydrodynamicsSIGLEAvailable from British Library Document Supply Centre-DSC:DXN006719 /...
Context. Transport of flare energy from the corona to the chromosphere has traditionally b...
On the basis of a numerical solution of dispersion equation we analyze characteristics of low-dampin...
Large-amplitude MHD waves are routinely observed in space plasmas. We suggest that dispersive focusi...
Generation of large-amplitude short-lived wave groups from small-amplitude initial perturbations in ...
The nonlinear coupling of MHD waves in a cold (beta = 0) compressible plasma with a smoothly inhomog...
Restricted Access.The exact nonlinear cylindrical solution for incompressible Hall magnetohydrodynam...
Context. Magnetohydrodynamic (MHD) waves are ubiquitous in the solar corona where the highly structu...
The one-dimensional oblique propagation of magnetohydrodynamic waves with arbitrary amplitudes in a ...
In this paper a numerical study of the propagation and dissipation properties of magnetohydro-dynami...
Aims. In the approximation of linear dissipative magnetohydrodynamics (MHD), it can be shown that dr...
Large amplitude magnetic field fluctuations often accompanied by density variations are frequently o...
We investigate the interaction of magnetohydrodynamic waves with plasma density inhomogeneities. Our...
Magnetohydrodynamic (MHD) waves play an important role in the solar atmosphere both directly (or int...
In this study, we numerically investigate the excitation of MHD waves in the interchange reconnectio...
MHD - magnetohydrodynamicsSIGLEAvailable from British Library Document Supply Centre-DSC:DXN006719 /...
Context. Transport of flare energy from the corona to the chromosphere has traditionally b...
On the basis of a numerical solution of dispersion equation we analyze characteristics of low-dampin...