spectral_radianceSurfaceBlackbody

Workspace.spectral_radianceSurfaceBlackbody(self, spectral_radiance: pyarts3.arts.StokvecVector | None = None, spectral_radiance_jacobian: pyarts3.arts.StokvecMatrix | None = None, frequency_grid: pyarts3.arts.AscendingGrid | None = None, surface_field: pyarts3.arts.SurfaceField | None = None, jacobian_targets: pyarts3.arts.JacobianTargets | None = None, ray_path_point: pyarts3.arts.PropagationPathPoint | None = None) None

Set surface spectral radiance from Planck function of the surface temperature.

\[\begin{split}\vec{I} = \left[ \begin{array}{c} \frac{2h\vec{\nu}^3}{c^2} \frac{1}{e^{\frac{h\vec{\nu}}{kT_s}} - 1} \\ 0 \\ 0 \\ 0 \end{array}\right],\end{split}\]

where \(T_s\) is the surface temperature extracted at the input ray_path_point. \(\nu\) is the frequency grid.

Author: Richard Larsson

Parameters: