4.7 Article

NONRELATIVISTIC COLLISIONLESS SHOCKS IN WEAKLY MAGNETIZED ELECTRON-ION PLASMAS: TWO-DIMENSIONAL PARTICLE-IN-CELL SIMULATION OF PERPENDICULAR SHOCK

Journal

ASTROPHYSICAL JOURNAL
Volume 721, Issue 1, Pages 828-842

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/721/1/828

Keywords

instabilities; ISM: supernova remnants; magnetic fields; plasmas; shock waves

Funding

  1. Ministry of Education, Culture, Sports, Science and Technology (MEXT) [20740136, 22740164]
  2. National Science Foundation [NSF PHY05-51164]
  3. Grants-in-Aid for Scientific Research [22740164, 20740136] Funding Source: KAKEN

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A two-dimensional particle-in-cell simulation is performed to investigate weakly magnetized perpendicular shocks with a magnetization parameter of sigma = 6 x 10(-5), which is equivalent to a high Alfven Mach number M(A) of similar to 130. It is shown that current filaments form in the foot region of the shock due to the ion-beam-Weibel instability (or the ion filamentation instability) and that they generate a strong magnetic field there. In the downstream region, these current filaments also generate a tangled magnetic field that is typically 15 times stronger than the upstream magnetic field. The thermal energies of electrons and ions in the downstream region are not in equipartition and their temperature ratio is T(e)/T(i) similar to 0.3-0.4. Efficient electron acceleration was not observed in our simulation, although a fraction of the ions are accelerated slightly on reflection at the shock. The simulation results agree very well with the Rankine-Hugoniot relations. It is also shown that electrons and ions are heated in the foot region by the Buneman instability (for electrons) and the ion-acoustic instability (for both electrons and ions). However, the growth rate of the Buneman instability is significantly reduced due to the relatively high temperature of the reflected ions. For the same reason, ion-ion streaming instability does not grow in the foot region.

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