Run a model with vertical hydrostatic equilibrium.
Note
this is an experimental function that is currently in development. Please use with care!
The hydrostatic equilibrium condition is only applied to the disk components. The following requirements must be met:
The dust properties for the model can be specified as dust or dust+gas densities as this does not have an impact on this calculation - however, the hydrostatic equilibrium is computed assuming an H2 + He mix of gas (i.e. mu=2.279). Note that this calculation also ignores the effects of self-gravity in the disk, which might be important for more massive disks.
Parameters : | prefix : str
model : ~hyperion.model.analytical_yso_model.AnalyticalYSOModel
n_iter : int, optional
mpi : bool, optional
n_processes : int, optional
overwrite : bool, optional
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Given a Model instance with a spherical polar coordinate grid, find the radius from which the optical depth to escape radially is a fixed value.
This only works for spherical polar grids, but works for 1-, 2-, and 3-d grids.
Parameters : | model : ~hyperion.model.Model instance tau : float
wav : float
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Returns : | r : np.ndarray
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