Meeting Update 0801 - Jason and Ivan

So far we have done different runs:

Batch 1 (4 runs):
Constant parameters:
Central mass = .4 MSun
Disk mass = 10 M_Jupiter
Disk radius = 2e10 cm
Disk height = 2e9 cm
Disk temperature = 4000 K
Ambient density = 0.001 g/cc
Variable parameters:
Ambient temperature = 1e6K | 5e6K | 1e7K | 5e7K
Preview:​Batch1_preview

Batch 2 (4 runs):
Constant parameters:
Central mass = .4 MSun
Disk radius = 2e10 cm
Disk height = 2e9 cm
Disk temperature = 4000 K
Ambient density = 0.001 g/cc
Ambient temperature = 5e6 K
Variable parameters :
Disk Mass = .1 | .5 | 1 | 10 MJupiter
Preview: ​Batch2_preview

In all the cases the ambient is attracted towards the central object, this generates velocity and temperature, and a heat bubble embeds the disk. A new hydrostatic equilibrium module (the current one implements constant pressure, which is not appropriate in our case) is needed to prevent the ambient from generating heat.

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