Image: General relativistic magnetohydrodynamic simulation of black hole accretion
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Description: Density (left) and magnetic energy density (right, zoom-in) in a turbulent, radiatively inefficient black hole accretion disk simulation (spin parameter a=0.9375). The simulation is performed in cartesian Kerr-Schild coordinates using 8 levels of mesh refinement (black lines are grid-lines). Simulation with the open source black hole accretion code (www.bhac.science).
Title: General relativistic magnetohydrodynamic simulation of black hole accretion
Credit: Own work
Author: Oliver Porth
Usage Terms: Creative Commons Attribution-Share Alike 4.0
License: CC BY-SA 4.0
License Link: https://creativecommons.org/licenses/by-sa/4.0
Attribution Required?: Yes
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