CND with outflow and magnetic field

This simulation includes the central outflow with the usual parameters, and an initially vertical magnetic field with a field strength of 10 microgauss. The first animation shows the density of the central 4 pc, the interaction of the outflow with the inner rim of the accretion disk causes a clumpy structure, as it does in the simulation without magnetic field that I have shown last week. The second animation shows the face-on beta parameter of the disk's inner region. As it is expected with such a weak magnetic field, the beta parameter is very high, so the dynamics are completely dominated by the gas and not by the magnetic field. The third animation shows the edge-on beta parameter, the outflow shapes the magnetic field into a more or less radial configuration.

Animation of the density, face-on, inner 4 pc of the disk

Animation of the beta-parameter, face-on, inner 4 pc of the disk, with streamlines of the magnetic Field

Animation of the beta-parameter, edge-on, with streamlines of the magnetic Field

Density, face-on, inner 4 pc of the disk:

Beta-parameter, face-on, inner 4 pc of the disk, with streamlines of the magnetic Field:

Beta-parameter, edge-on, with streamlines of the magnetic Field:

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