Astrophysics and Space Science

, Volume 292, Issue 1–4, pp 261–265

Drag Instability

  • Pin-Gao Gu
  • Douglas N.C. Lin
  • Ethan T. Vishniac
Article

DOI: 10.1023/B:ASTR.0000045025.13684.ae

Cite this article as:
Gu, PG., Lin, D.N. & Vishniac, E.T. Astrophysics and Space Science (2004) 292: 261. doi:10.1023/B:ASTR.0000045025.13684.ae
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Abstract

With the ionization rate of neutral particles caused by cosmic rays and balanced by the recombination rate of ions for a cold, weakly ionized fluid threaded by stressed magnetic fields, we show that a local perturbation can evolve to a traveling wave with its perturbed quantities growing with time so long as the drift velocity between neutrals and ions is comparable to the Alfven speed of the fluid. Since the large drift velocity is one of the key assumptions to drive this instability, we name it the “drag instability”. We suggest that the drag instability might occur in the regions where magnetic fields are highly stressed such as a C-shock front or a collapsing proto-stellar cloud.

ambipolar drift ionization equilibrium fluid instability 

Copyright information

© Kluwer Academic Publishers 2004

Authors and Affiliations

  • Pin-Gao Gu
    • 1
  • Douglas N.C. Lin
    • 2
  • Ethan T. Vishniac
    • 3
  1. 1.Institute of Astronomy and Astrophysics, Academia SinicaTaipeiTaiwan, R.O.C
  2. 2.UCO/Lick ObservatoryUniversity of CaliforniaSanta CruzU.S.A
  3. 3.Department of Physics and AstronomyJohns Hopkins UniversityBaltimoreU.S.A

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