Fakultät für Physik und Astronomie
STEPHEN PHILLIPS hostreviews.co.uk / UNSPLASH

Implementation of magnetic resistivity in GR-MHD simulation

Qian Qian , MPIA

Turbulent magnetic diffusivity plays an important role for accretion disks and the launching of disk winds. We have implemented magnetic diffusivity, respective resistivity in the general relativistic MHD code HARM. This colloquium describes the theoretical background of our implementation, its numerical realization, tests and preliminary applications under astronomical context.

ITA "blackboard" Colloquium
19 Dec 2016, 11:15
Philosophenweg, 12, R106

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