Meeting Update 07/08/2013

Did some runs of the HS disk with a de-resolved center. The red line is the accretion rate for the disk in HS equilibrium with an ambient. The other lines are the accretion rates but when the density of the ambient is an order of magnitude less then the previous line. The red curve has an accretion rate of about .0019 solar masses/yr and the green one has .00748 solar masses/yr, both of these are taken from the 40th cycle and onward.

Densities go down by an order of magnitude

There are also a few videos (mpeg) attached showing the density and radial flux during a run.

I've also did a small run with the wind driven disk on bluehive, but need to increase the bounds of it to be able to see anything.

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