Simulating Magnetized Jets

Details Simulating Magnetized Jets Simulating Magnetized Jets

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.293..217k&link_type=abstract

Astrophysics and Space Science, v. 293, Issue 1, p. 217-224 (2004).

Astronomy and Astrophysics

Astrophysics

Jets, Mhd, Numerical

Scientific paper

A suitable model for the macroscopic behavior of accretion disk-jet systems is provided by the equations of MagnetoHydroDynamics (MHD). These equations allow us to perform scale-encompassing numerical simulations of multidimensional nonlinear magnetized plasma flows. For that purpose, we continue the development and exploitation of the Versatile Advection Code (VAC) along with its recent extension which employs dynamically controlled grid adaptation. In the adaptive mesh refinement AMRVAC code, modules for simulating any-dimensional special relativistic hydro- and magnetohydrodynamic problems are currently operational.

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