Meeting Update 07917 - Jason and Ivan

HSE, stage 1:

  • Astrobear now calculates the pressure needed for HSE using a discrete method (cell by cell)
  • HSE code does not need to be changed for new density profiles
  • Custom density based on star models needs to be loaded (that's where we are at now ..)


HSE movie example:

  • Very low velocities
  • Reflected boundaries
  • Very small or no change in pressure profile, over a timescale of 4 disk rotations (the disk we used to have in the previous simulations)
  • Not a final demonstration of HSE since density profile is not consistent with a star model
  • It's simply a test

​HSE-test

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