General_relativistic_magnetohydrodynamic_simulation_of_black_hole_accretion.jpg
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Summary
| Description |
English:
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).
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| Date | |
| Source | Own work |
| Author | Oliver Porth |
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