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Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
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 |
sun's ionization structure |