International audienceNew results provided by numerical simulations of the weak instability of a warm electron beam in a collisionless plasma are presented. The theoretical model considers the self-consistent resonant interactions of beam particles with wave packets of broad spectra; it is derived using some of the initial approximations of the standard derivation of the quasilinear diffusion equation in the weak turbulence approach, without, however, the assumption of randomly phased waves. A huge number of particle trajectories calculated over long times by a symplectic code are analyzed using various statistical algorithms. The dynamics of the beam relaxation and the saturation of the wave spectrum are studied and compared with the analy...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceNew results provided by numerical simulations of the weak instability of a war...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceParticle diffusion in velocity space is studied on the basis of 1D simulations...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...