International audienceThe interaction of the electron beam propagating in a nonuniform solar wind plasma with Langmuir waves is considered. Plasma waves are described one dimensional system of Zakharov equations, the beam dynamics is modeled using particles moving in the total electric field of the Langmuir waves. The role of external plasma density fluctuations, which are known to be present in the solar wind, is taking into account. It is shown that at low density fluctuations delta n /n₀ delta n /n₀ >3k(2) L_d(2) , plasma inhomogeneity has a decisive influence on the relaxation process. First, the growth of waves on the linear stage becomes localized, thereby clearly identifiable wave packets or clumps dominate the wave spectrum. This ef...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
Non-thermal electron populations are observed throughout the heliosphere. The relaxation of an elect...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceThe interaction of the electron beam propagating in a nonuniform solar wind pl...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
International audienceObservations performed in the solar wind by different satellites show that ele...
Non-thermal electron populations are observed throughout the heliosphere. The relaxation of an elect...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceLangmuir turbulence excited by electron flows in solar wind plasmas is studied...
International audienceThe interaction of a beam propagating in a inhomogeneous solar wind plasma is ...