English

Oscillatory disintegration of a trans-Alfvenic shock: A magnetohydrodynamic simulation

Plasma Physics 2009-10-31 v1 Space Physics

Abstract

Nonlinear evolution of a trans-Alfvenic shock wave (TASW), at which the flow velocity passes over the Alfven velocity, is computed in a magnetohydrodynamic approximation. The analytical theory suggests that an infinitesimal perturbation of a TASW results in its disintegration, i.e., finite variation of the flow, or transformation into some other unsteady configuration. In the present paper, this result is confirmed by numerical simulations. It is shown that the disintegration time is close to its minimum value equal to the shock thickness divided by a relative velocity of the emerging secondary structures. The secondary TASW that appears after the disintegration is again unstable with respect to disintegration. When the perturbation has a cyclic nature, the TASW undergoes oscillatory disintegration, during which it repeatedly transforms into another TASW. This process manifests itself as a train of shock and rarefaction waves, which consecutively emerge at one edge of the train and merge at the other edge.

Keywords

Cite

@article{arxiv.physics/9904011,
  title  = {Oscillatory disintegration of a trans-Alfvenic shock: A magnetohydrodynamic simulation},
  author = {S. A. Markovskii and S. L. Skorokhodov},
  journal= {arXiv preprint arXiv:physics/9904011},
  year   = {2009}
}

Comments

REVTEX, 8 pages, 13 PostScript figures, uses epsfig.sty

R2 v1 2026-07-22T19:18:56.603Z