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NIRVANA MHD simulation of a magnetically collimated jet (magnetic field lines in red), which is driven from a circumplanetary accretion disk. The visualization shows a zoom-in of the global simulation, which covers the entire circumstellar disk. Adaptive grid refinement allows to resolve the flow (streamlines in white) around the embedded planet.
Dr. Udo Ziegler
You can find the NIRVANA code on Gitlab: https://gitlab.aip.de/ziegler/NIRVANA, including the Documentation.
Involved AIP sections and groups: