Large resistivity in numerical simulations of radially self-similar outflows

Details Large resistivity in numerical simulations of radially self-similar outflows Large resistivity in numerical simulations of radially self-similar outflows

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..271..371c&link_type=abstract

Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 271,

Astronomy and Astrophysics

Astrophysics

Magnetic Fields (Magnetohydrodynamics): Mhd, Methods: Numerical, Stars: Winds, Outflows

Scientific paper

We investigate conditions in a radially self-similar outflow in the regime of large resistivity. Using the PLUTO code, we performed simulations with proper choice of boundary conditions, relaxed at the footpoints of critical surfaces in the flow. We investigate outflow propagation in a high-resistive disk corona, and compare it to the results with small or vanishing resistivity.

Affiliated with

Also associated with

No associations

Rating

Large resistivity in numerical simulations of radially self-similar outflows 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 Large resistivity in numerical simulations of radially self-similar outflows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Large resistivity in numerical simulations of radially self-similar outflows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1677519