Simulation of Turbulent Dynamo (IMAGE)

University of Chicago

Simulation of Turbulent Dynamo

Caption

This is a 3-D radiation magneto-hydrodynamic FLASH simulation of the experiment, performed on the Mira supercomputer at Argonne National Laboratory. The values demonstrate strong amplification of the seed magnetic fields by turbulent dynamo.

Credit

Petros Tzeferacos/University of Chicago

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