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A simple model of dust settling and mixing in disks

C.P. Dullemond

General description

Dust sedimentation plays a major role in determining how protoplanetary disks appear to an observer. Here is a simple code for computing stationary and time-dependent 1-D vertical settling and mixing of dust grains in disks, in a way that allows direct insertion into radiative transfer codes or codes that compute disk chemistry.

The code is very simplistic, and I do not feel responsible for how it is used. Use it at your own risk!

Download version 2, of date 25.07.2010

Verantwortlich: Cornelis Petrus Dullemond, letzte Änderung am 15.03.2011 14:06 CET
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