spectral_radiance_fieldClearskyPlaneParallel

Workspace.spectral_radiance_fieldClearskyPlaneParallel(self: pyarts.arts._Workspace, spectral_radiance_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor7]] = self.spectral_radiance_field, trans_field: Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3], propmat_clearsky_agenda: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Agenda]] = self.propmat_clearsky_agenda, water_p_eq_agenda: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Agenda]] = self.water_p_eq_agenda, iy_space_agenda: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Agenda]] = self.iy_space_agenda, iy_surface_agenda: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Agenda]] = self.iy_surface_agenda, iy_cloudbox_agenda: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Agenda]] = self.iy_cloudbox_agenda, stokes_dim: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Index]] = self.stokes_dim, f_grid: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Vector]] = self.f_grid, atmosphere_dim: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Index]] = self.atmosphere_dim, p_grid: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Vector]] = self.p_grid, z_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.z_field, t_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.t_field, nlte_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.EnergyLevelMap]] = self.nlte_field, vmr_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor4]] = self.vmr_field, abs_species: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.ArrayOfArrayOfSpeciesTag]] = self.abs_species, wind_u_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.wind_u_field, wind_v_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.wind_v_field, wind_w_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.wind_w_field, mag_u_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.mag_u_field, mag_v_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.mag_v_field, mag_w_field: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.mag_w_field, z_surface: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Matrix]] = self.z_surface, ppath_lmax: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Numeric]] = self.ppath_lmax, rte_alonglos_v: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Numeric]] = self.rte_alonglos_v, rt_integration_option: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.String]] = self.rt_integration_option, surface_props_data: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Tensor3]] = self.surface_props_data, za_grid: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Vector]] = self.za_grid, use_parallel_za: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Index]] = 1, verbosity: Optional[Union[pyarts.arts.WorkspaceVariable, pyarts.arts.Verbosity]] = self.verbosity) None

Clear-sky radiance field of a plane parallel atmosphere.

The method assumes a 1D flat planet. Radiances along each direction given by za_grid are calculated using ppathPlaneParallel() and iyEmissionStandard().

Surface properties are defined by iy_surface_agenda, i.e. there is no restriction to e.g. specular surfaces.

Note that the variable ppath_lmax is considered, and that it can be critical for the accuracy for zenith angles close to 90 degrees. That is, using ppath_lmax=-1 is not recommended for this function.

Information on transmittance is also provided by the GOUT trans_field. For up-welling radiation (scat_za > 90), this variable holds the transmittance to space, for considered position and propagation direction. For down-welling radiation, trans_field holds instead the transmittance down to the surface.

Author(s): Patrick Eriksson

Parameters:
  • spectral_radiance_field (Tensor7, optional) – Spectral radiance field. See spectral_radiance_field, defaults to self.spectral_radiance_field [OUT]

  • trans_field (Tensor3) – Dimensions: [f_grid,p_grid,za_grid]. See further above. [OUT]

  • propmat_clearsky_agenda (Agenda, optional) – Calculate the absorption coefficient matrix. See propmat_clearsky_agenda, defaults to self.propmat_clearsky_agenda [IN]

  • water_p_eq_agenda (Agenda, optional) – Calculation of the saturation pressure of water. See water_p_eq_agenda, defaults to self.water_p_eq_agenda [IN]

  • iy_space_agenda (Agenda, optional) – Downwelling radiation at the top of the atmosphere. See iy_space_agenda, defaults to self.iy_space_agenda [IN]

  • iy_surface_agenda (Agenda, optional) – Upwelling radiation from the surface. See iy_surface_agenda, defaults to self.iy_surface_agenda [IN]

  • iy_cloudbox_agenda (Agenda, optional) – Intensity at boundary or interior of the cloudbox. See iy_cloudbox_agenda, defaults to self.iy_cloudbox_agenda [IN]

  • stokes_dim (Index, optional) – The dimensionality of the Stokes vector (1-4). See stokes_dim, defaults to self.stokes_dim [IN]

  • f_grid (Vector, optional) – The frequency grid for monochromatic pencil beam calculations. See f_grid, defaults to self.f_grid [IN]

  • atmosphere_dim (Index, optional) – The atmospheric dimensionality (1-3). See atmosphere_dim, defaults to self.atmosphere_dim [IN]

  • p_grid (Vector, optional) – The pressure grid. See p_grid, defaults to self.p_grid [IN]

  • z_field (Tensor3, optional) – The field of geometrical altitudes. See z_field, defaults to self.z_field [IN]

  • t_field (Tensor3, optional) – The field of atmospheric temperatures. See t_field, defaults to self.t_field [IN]

  • nlte_field (EnergyLevelMap, optional) – The field of NLTE temperatures and/or ratios. See nlte_field, defaults to self.nlte_field [IN]

  • vmr_field (Tensor4, optional) – VMR field. See vmr_field, defaults to self.vmr_field [IN]

  • abs_species (ArrayOfArrayOfSpeciesTag, optional) – Tag groups for gas absorption. See abs_species, defaults to self.abs_species [IN]

  • wind_u_field (Tensor3, optional) – Zonal component of the wind field. See wind_u_field, defaults to self.wind_u_field [IN]

  • wind_v_field (Tensor3, optional) – Meridional component of the magnetic field. See wind_v_field, defaults to self.wind_v_field [IN]

  • wind_w_field (Tensor3, optional) – Vertical wind component field. See wind_w_field, defaults to self.wind_w_field [IN]

  • mag_u_field (Tensor3, optional) – Zonal component of the magnetic field. See mag_u_field, defaults to self.mag_u_field [IN]

  • mag_v_field (Tensor3, optional) – Meridional component of the magnetic field. See mag_v_field, defaults to self.mag_v_field [IN]

  • mag_w_field (Tensor3, optional) – Vertical component of the magnetic field. See mag_w_field, defaults to self.mag_w_field [IN]

  • z_surface (Matrix, optional) – The surface altitude. See z_surface, defaults to self.z_surface [IN]

  • ppath_lmax (Numeric, optional) – Maximum length between points describing propagation paths. See ppath_lmax, defaults to self.ppath_lmax [IN]

  • rte_alonglos_v (Numeric, optional) – Velocity along the line-of-sight to consider for a RT calculation. See rte_alonglos_v, defaults to self.rte_alonglos_v [IN]

  • rt_integration_option (String, optional) – Switch between integration approaches for radiative transfer steps. See rt_integration_option, defaults to self.rt_integration_option [IN]

  • surface_props_data (Tensor3, optional) – Various surface properties. See surface_props_data, defaults to self.surface_props_data [IN]

  • za_grid (Vector, optional) – Zenith angle grid. See za_grid, defaults to self.za_grid [IN]

  • use_parallel_za (Index, optional) – Flag to select parallelization over zenith angles. Defaults to 1 [IN]

  • verbosity (Verbosity) – ARTS verbosity. See verbosity, defaults to self.verbosity [IN]