WriteMolTau
- Workspace.WriteMolTau(self: pyarts.arts._Workspace, f_grid: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Vector]] = self.f_grid, z_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.z_field, propmat_clearsky_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor7]] = self.propmat_clearsky_field, atmosphere_dim: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Index]] = self.atmosphere_dim, filename: Union[pyarts.arts.WorkspaceVariable, pyarts.arts.String], verbosity: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Verbosity]] = self.verbosity) None
Writes a ‘molecular_tau_file’ as required for libRadtran.
The libRadtran (www.libradtran.org) radiative transfer package is a comprehensive package for various applications, it can be used to compute radiances, irradiances, actinic fluxes, … for the solar and the thermal spectral ranges. Absorption is usually treated using k-distributions or other parameterizations. For calculations with high spectral resolution it requires absorption coefficients from an external line-by-line model. Using this method, arts generates a file that can be used by libRadtran (option molecular_tau_file).
Author(s): Claudia Emde
- Parameters:
f_grid (Vector, optional) – The frequency grid for monochromatic pencil beam calculations. See
f_grid
, defaults toself.f_grid
[IN]z_field (Tensor3, optional) – The field of geometrical altitudes. See
z_field
, defaults toself.z_field
[IN]propmat_clearsky_field (Tensor7, optional) – Gas absorption field. See
propmat_clearsky_field
, defaults toself.propmat_clearsky_field
[IN]atmosphere_dim (Index, optional) – The atmospheric dimensionality (1-3). See
atmosphere_dim
, defaults toself.atmosphere_dim
[IN]filename (String) – Name of the
molecular_tau_file
. [IN]verbosity (Verbosity) – ARTS verbosity. See
verbosity
, defaults toself.verbosity
[IN]