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Testing

2 AMR level. 0.1 AU the finest resolution.

The radial velocity at the boundary varies as v=v_{piston}\cos{2\pi t/P} where P= 1\ yr.

Dust form at fixed radii, the radius is calculated by R=\sqrt{\frac{L \xi}{4 \pi \sigma T_{df}^4}} where \xi=0.5 is the dust absorption coefficient and T_{df}=1500\ K is the dust formation temperature.

AstroBEARAGBproperties1.pdf

AstroBEAR_single_AGB001.gif

AstroBEAR_single_AGB002.gif

AstroBEAR_single_AGB003.gif

Posted: 9 years ago (Updated: 9 years ago)
Author: Zhuo Chen
Categories: (none)

Attachments (4)

AstroBEAR_single_AGB001.gif (11.5 MB) - added by Zhuo Chen 9 years ago.
AstroBEAR_single_AGB002.gif (11.2 MB) - added by Zhuo Chen 9 years ago.
AstroBEAR_singleAGB003.gif (11.3 MB) - added by Zhuo Chen 9 years ago.
AstroBEARAGBproperties1.pdf (27.0 KB) - added by Zhuo Chen 9 years ago.

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