3-D General Relativistic MHD Simulations of Generating Jets

Details 3-D General Relativistic MHD Simulations of Generating Jets 3-D General Relativistic MHD Simulations of Generating Jets

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.7317n&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #73.17; Bulletin of the American Astronomical Society, Vol. 31, p.952

Astronomy and Astrophysics

Astronomy

Scientific paper

Koide et al have investigated the dynamics of an accretion disk initially threaded by a uniform poloidal magnetic field in a non-rotating corona (either in a steady-state infalling state or in hydrostatic equilibrium) around a non-rotating black hole using a 3-D GRMHD with the ``axisymmetry'' along the z-direction. Magnetic field is tightly twisted by the rotation of the disk, and plasmas in the shocked region of the disk are accelerated by J x B force to form bipolar relativistic jets. In order to investigate variabilities of generated relativistic jets and magnetic field structure inside jets, we have performed calculations using the 3-D GRMHD code on a full 3-dimensional system. We will investigate how the third dimension affects the global disk dynamics. 3-D RMHD simulations wil be also performed to investigate the dynamics of a jet with a helical mangetic field in it.

Affiliated with

Also associated with

No associations

Rating

3-D General Relativistic MHD Simulations of Generating Jets 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 3-D General Relativistic MHD Simulations of Generating Jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 3-D General Relativistic MHD Simulations of Generating Jets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1121480