English

Nonhelical turbulent dynamos: shocks and shear

Astrophysics 2007-05-23 v1

Abstract

Small scale turbulent dynamo action in compressible transonic turbulence is discussed. It is shown that the critical value of the magnetic Reynolds number displays a bimodal behavior and changes from a typical value of 35 for small Mach numbers to about 80 for larger Mach numbers. The transition between the two regimes is relatively sharp. The direct simulations are then compared with simulations where shocks are captured using a shock viscosity that becomes large at locations where there are shocks. In the presence of shear it is shown that large scale dynamo action is possible.

Keywords

Cite

@article{arxiv.astro-ph/0501006,
  title  = {Nonhelical turbulent dynamos: shocks and shear},
  author = {A. Brandenburg and N. E. L. Haugen and A. J. Mee},
  journal= {arXiv preprint arXiv:astro-ph/0501006},
  year   = {2007}
}

Comments

8 pages, 6 pictures, to appear in: The Magnetized Plasma in Galaxy Evolution, Eds. K.T. Chyzy, R.-J. Dettmar, K. Otmianowska-Mazur and M. Soida

R2 v1 2026-07-22T08:47:01.092Z