Simulation of the circumnuclear disk

This is a simulation of the circumnuclear disk with the same parameters as last week, I only extended the final time by a factor of 2.5 (and worked on a different cluster that uses gcc instead of intel compilers).

So the first 40% of this simulation should look the same as last weeks simulation, but as you can see, there is a kind of wind/outflow from the bottom of the disk. The reason is that the initial conditions are not set properly as you can see in the second picture, where we see a contour plot of the disk at t=0 that shows a kind of patchy structure at one of the quarters.

I'm currently trying to find out what is causing this behaviour.

​Movie

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