Turbulence and transport in two-dimensional magnetized electron plasmas

Abstract

Electron plasmas confined by an external magnetic field exhibit variations in a two-dimensional plane orthogonal to the confining magnetic field. A nonlinear fluid simulation code to investigate the properties of 2-D electron plasma wave turbulence in a nonuniform magnetoplasma has been developed. It is found that the presence of the density gradient convection by mean electric fields considerably influence the characteristic nonlinear interaction processes, such as the energy cascades and the cross-field electron transport. The initial random turbulent state evolves towards an intermittent state where forward cascade of vorticity coexists with an inverse cascade of electric potential fluctuations. The latter lead to the formation of large scale entities in 2D electron plasmas and can be alternatively understood by seeking exact nonlinear coherent vortex solutions in the form of a dipolar-like configuration. The energy cascades are governed typically by the Kolmogorov-like $k^{-5/3}$ spectrum. In agreement with the experimental observations, we find that the electron transport is improved significantly by the application of an externally imposed electric field

Whistler Wave Turbulence in Solar Wind Plasma

“…We find from our 3D simulations that whistler wave turbulence in the kd e < 1 and kd e > 1 regimes exhibits respectively k −7/3 and k −5/3 (see Fig 1) spectra. The inertial range turbulent spectra obtained from our 3D simulations are further consistent with 2D work [11,21,22]. Interestingly, the wave effects dominate in the large scale, i.e.…”