To Do List

Simulations in order of priority:

1. Higher resolution around planet (do I need to adjust the buffer in the problem module?) - Had to add data point at center of object to Parker wind profile.

2. Increase density and decrease temp (for constant pressure) in center of planet - Does not do much

3. Raise ambient temperature to planet temperature - No more pressure protections (immediately, anyway)

Movies:

• Smallest non-pressure protecting simulation - rho with magnetic field, beta with magnetic field

JC - Another option is to increase the transition radius for the magnetic field from r_p/2 to closer to r_p. This will take a little calculus to make sure it is done correctly… see ​https://astrobear.pas.rochester.edu/trac/blog/johannjc06302015 for the equations currently implemented in the problem module. In terms of increasing the resolution - you may be able to just add additional levels of AMR - would need to see plots of the mesh (sliced through the midplane) with density overlayed to see how it is currently refined.

I believe just increasing the resolution should be ok - higher resolution is forced out to about 4R_p, and it doesn't seem to want to resolve a ton outside of that, so shouldn't increase computational time more than necessary. Here's a slice near the midplane, zoomed in a bit: