Skip to main content
Log in

Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields

  • Session I: Plasma Flows, Shocks and Turbulence
  • Published:
Space Science Reviews Aims and scope Submit manuscript

Abstract

This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Andrea Mignone.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Mignone, A., Massaglia, S. & Bodo, G. Relativistic MHD Simulations of Jets with Toroidal Magnetic Fields. Space Sci Rev 121, 21–31 (2005). https://doi.org/10.1007/s11214-006-3588-4

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11214-006-3588-4

Keywords

Navigation