spectral_rad_scat_pathSunsFirstOrder

Workspace.spectral_rad_scat_pathSunsFirstOrder(self, spectral_rad_scat_path: ArrayOfStokvecVector = self.spectral_rad_scat_path, ray_path: ArrayOfPropagationPathPoint = self.ray_path, ray_path_suns_path: ArrayOfArrayOfArrayOfPropagationPathPoint = self.ray_path_suns_path, suns: ArrayOfSun = self.suns, jac_targets: JacobianTargets = self.jac_targets, freq_grid: AscendingGrid = self.freq_grid, atm_field: AtmField = self.atm_field, surf_field: SurfaceField = self.surf_field, scat_species: ArrayOfScatteringSpecies = self.scat_species, spectral_propmat_and_atm_path_agenda: Agenda = self.spectral_propmat_and_atm_path_agenda, rte_option: TransmittanceOption = self.rte_option, hse_derivative: Index = 0) → None

Compute first-order solar scattering from scat_species along ray_path.

Unlike spectral_rad_scat_pathSunsFirstOrderRayleigh(), both the scattering coefficient and the polarized phase matrix come from scat_species. This supports gas, particulate, and mixed scattering species.

Author: Richard Larsson

Used by wrapper method

Parameters:
  • spectral_rad_scat_path (~pyarts3.arts.ArrayOfStokvecVector, optional) – Spectral radiance scattered into the propagation path. Defaults to self.spectral_rad_scat_path. [OUT]

  • ray_path (~pyarts3.arts.ArrayOfPropagationPathPoint, optional) – A list path points making up a propagation path. Defaults to self.ray_path. [IN]

  • ray_path_suns_path (~pyarts3.arts.ArrayOfArrayOfArrayOfPropagationPathPoint, optional) – A list of paths to the suns from the ray path. Defaults to self.ray_path_suns_path. [IN]

  • suns (~pyarts3.arts.ArrayOfSun, optional) – A list of Sun. Defaults to self.suns. [IN]

  • jac_targets (~pyarts3.arts.JacobianTargets, optional) – A list of targets for the Jacobian Matrix calculations. Defaults to self.jac_targets. [IN]

  • freq_grid (~pyarts3.arts.AscendingGrid, optional) – A frequency grid. Unit: Hz. Defaults to self.freq_grid. [IN]

  • atm_field (~pyarts3.arts.AtmField, optional) – An atmospheric field in ARTS, this is the main atmospheric data structure in ARTS. Defaults to self.atm_field. [IN]

  • surf_field (~pyarts3.arts.SurfaceField, optional) – The surface field. Defaults to self.surf_field. [IN]

  • scat_species (~pyarts3.arts.ArrayOfScatteringSpecies, optional) – The scattering species. Defaults to self.scat_species. [IN]

  • spectral_propmat_and_atm_path_agenda (~pyarts3.arts.Agenda, optional) – Computes several path parameters along the path. Defaults to self.spectral_propmat_and_atm_path_agenda. [IN]

  • rte_option (~pyarts3.arts.TransmittanceOption, optional) – The radiative transfer equation (RTE) option. Defaults to self.rte_option. [IN]

  • hse_derivative (~pyarts3.arts.Index, optional) – Flag to compute the hypsometric distance derivatives. Defaults to 0 [IN]