Parametric interactions between a sonic pump wave and a weak Alfven wave are studied. It is shown that if the Alfven-wave velocity V_A is small relative to the sonic-wave velocity V_s there is a time-growing instability leading to the increase of the Alfven wave at the expense of the sonic wave. This phenomenon can be of importance in solar and stellar physics. For V_A large relative to V_s, the interaction is of the stop-band type
The authors acknowledge the International Space Science Institute (Switzerland) for funding the prog...
International audienceWe review our recent results of global one-dimensional (1-D) MHD simulations f...
We present a comprehensive model of the global properties of Alfven waves in the solar atmosphere an...
The weakly nonlinear interaction of sound and linearly polarised Alfven waves propagating in the sam...
The weakly nonlinear interaction of sound and linearly polarized Alfven waves propagating along an a...
The nonlinear interaction between two Alfvén waves and a sound wave is studied, using the normal-mod...
Our solar system contains more activity and complexity than can be seen through a telescope. One suc...
International audienceAlfvén waves, discontinuities, proton perpendicular acceleration and magnetic ...
Nonlinear coupling between 3-minute oscillations and Alfven waves in the solar lower atmosphere is s...
Alfven wave phase mixing is an extensively studied mechanism for dissipating wave energy in an inhom...
Final report for DOE Plasma Physics Junior Faculty Development award DOE-FG02-02ER54688. Reports on ...
International audienceThe terrestrial foreshock is characterised by the existence of large amplitude...
Alfven waves are an important energy transport modality in the collisionless plasmas that dominate E...
Some of the issues associated with a more complete treatment of Alfven transport in cosmic ray shock...
International audienceAs a continuation of our earlier paper, we consider here the case of the excit...
The authors acknowledge the International Space Science Institute (Switzerland) for funding the prog...
International audienceWe review our recent results of global one-dimensional (1-D) MHD simulations f...
We present a comprehensive model of the global properties of Alfven waves in the solar atmosphere an...
The weakly nonlinear interaction of sound and linearly polarised Alfven waves propagating in the sam...
The weakly nonlinear interaction of sound and linearly polarized Alfven waves propagating along an a...
The nonlinear interaction between two Alfvén waves and a sound wave is studied, using the normal-mod...
Our solar system contains more activity and complexity than can be seen through a telescope. One suc...
International audienceAlfvén waves, discontinuities, proton perpendicular acceleration and magnetic ...
Nonlinear coupling between 3-minute oscillations and Alfven waves in the solar lower atmosphere is s...
Alfven wave phase mixing is an extensively studied mechanism for dissipating wave energy in an inhom...
Final report for DOE Plasma Physics Junior Faculty Development award DOE-FG02-02ER54688. Reports on ...
International audienceThe terrestrial foreshock is characterised by the existence of large amplitude...
Alfven waves are an important energy transport modality in the collisionless plasmas that dominate E...
Some of the issues associated with a more complete treatment of Alfven transport in cosmic ray shock...
International audienceAs a continuation of our earlier paper, we consider here the case of the excit...
The authors acknowledge the International Space Science Institute (Switzerland) for funding the prog...
International audienceWe review our recent results of global one-dimensional (1-D) MHD simulations f...
We present a comprehensive model of the global properties of Alfven waves in the solar atmosphere an...