Shocks in unmagnetized plasma with a shear flow: Stability and magnetic field generation

نویسندگان

  • Mark Eric Dieckmann
  • Alexander Bock
  • Hamad Ahmed
  • Domenico Doria
  • Gianluca Sarri
  • Anders Ynnerman
  • Marco Borghesi
  • M. E. Dieckmann
  • A. Bock
  • H. Ahmed
  • D. Doria
  • G. Sarri
  • A. Ynnerman
  • M. Borghesi
چکیده

Convective radial energy flux due to resonant magnetic perturbations and magnetic curvature at the tokamak plasma edge Modification of the formation of high-Mach number electrostatic shock-like structures by the ion acoustic instability Phys. Generation of magnetic field and electrostatic shock wave driven by counterstreaming pair plasmas A pair of curved shocks in a collisionless plasma is examined with a two-dimensional particle-in-cell simulation. The shocks are created by the collision of two electron-ion clouds at a speed that exceeds everywhere the threshold speed for shock formation. A variation of the collision speed along the initially planar collision boundary, which is comparable to the ion acoustic speed, yields a curvature of the shock that increases with time. The spatially varying Mach number of the shocks results in a variation of the downstream density in the direction along the shock boundary. This variation is eventually equilibrated by the thermal diffusion of ions. The pair of shocks is stable for tens of inverse ion plasma frequencies. The angle between the mean flow velocity vector of the inflowing upstream plasma and the shock's electrostatic field increases steadily during this time. The disalignment of both vectors gives rise to a rotational electron flow, which yields the growth of magnetic field patches that are coherent over tens of electron skin depths. V C 2015 AIP Publishing LLC.

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تاریخ انتشار 2015