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Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
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The code contained in
public_atmos.tbz
implements a simple stellar atmosphere model. It
assumes a one-dimensional slab in hydrostatic and local thermodynamic
equilibrium with gray rosseland mean opacities. Still, it can be
useful as a quick diagnostic of a stellar atmosphere, or for checking
the effects of a piece of local physics (e.g.,ionization).
sun's temperature structure
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sun's ionization structure
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