A numerical implementation of MHD in divergence form

Details A numerical implementation of MHD in divergence form A numerical implementation of MHD in divergence form

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jcoph.105..339v&link_type=abstract

Journal of Computational Physics (ISSN 0021-9991), vol. 105, no. 2, p. 339-353.

Statistics

Computation

24

Cosmic Plasma, Magnetic Field Configurations, Magnetohydrodynamic Flow, Shock Heating, Cauchy Problem, Computational Astrophysics, Divergence

Scientific paper

Shock computations are presently undertaken by a numerical implementation of fully relativistic MHD in divergence form, as illustrated by pseudospectral-method computations for the coplanar Riemann MHD problem. Compound waves are noted to persist in relativistic MHD. Attention is given to two limiting cases: (1) where the velocities become nonrelativistic, and (2) where the longitudinal magnetic field becomes zero. Comparisons are made with results for both the singular case of zero longitudinal magnetic field, and nonrelativistic MHD.

Affiliated with

Also associated with

No associations

Rating

A numerical implementation of MHD in divergence form does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A numerical implementation of MHD in divergence form, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A numerical implementation of MHD in divergence form will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1372547