Workspace functions associated wih the surface and its properties. More...

#include <cmath>
#include "arts.h"
#include "auto_md.h"
#include "check_input.h"
#include "complex.h"
#include "geodetic.h"
#include "math_funcs.h"
#include "messages.h"
#include "special_interp.h"
#include "interpolation.h"
#include "physics_funcs.h"
#include "rte.h"
#include "surface.h"

Include dependency graph for m_surface.cc:

Go to the source code of this file.

Functions
void	InterpSurfaceFieldToPosition (Numeric &outvalue, const Index &atmosphere_dim, const Vector &lat_grid, const Vector &lon_grid, const Vector &rtp_pos, const Matrix &z_surface, const Matrix &field, const Verbosity &verbosity)
	WORKSPACE METHOD: InterpSurfaceFieldToPosition. More...

void	iySurfaceRtpropAgenda (Workspace &ws, Matrix &iy, ArrayOfTensor3 &diy_dx, const Tensor3 &iy_transmission, const Index &jacobian_do, const Index &atmosphere_dim, const Tensor3 &t_field, const Tensor3 &z_field, const Tensor4 &vmr_field, const Index &cloudbox_on, const Index &stokes_dim, const Vector &f_grid, const Vector &rtp_pos, const Vector &rtp_los, const Vector &rte_pos2, const Agenda &iy_main_agenda, const Agenda &surface_rtprop_agenda, const Verbosity &)
	WORKSPACE METHOD: iySurfaceRtpropAgenda. More...

void	specular_losCalc (Vector &specular_los, Vector &surface_normal, const Vector &rtp_pos, const Vector &rtp_los, const Index &atmosphere_dim, const Vector &lat_grid, const Vector &lon_grid, const Vector &refellipsoid, const Matrix &z_surface, const Verbosity &)
	WORKSPACE METHOD: specular_losCalc. More...

void	surfaceBlackbody (Workspace &ws, Matrix &surface_los, Tensor4 &surface_rmatrix, Matrix &surface_emission, const Vector &f_grid, const Index &stokes_dim, const Numeric &surface_skin_t, const Agenda &blackbody_radiation_agenda, const Verbosity &verbosity)
	WORKSPACE METHOD: surfaceBlackbody. More...

void	surfaceFlatRefractiveIndex (Workspace &ws, Matrix &surface_los, Tensor4 &surface_rmatrix, Matrix &surface_emission, const Vector &f_grid, const Index &stokes_dim, const Index &atmosphere_dim, const Vector &rtp_los, const Vector &specular_los, const Numeric &surface_skin_t, const GriddedField3 &surface_complex_refr_index, const Agenda &blackbody_radiation_agenda, const Verbosity &verbosity)
	WORKSPACE METHOD: surfaceFlatRefractiveIndex. More...

void	surfaceFlatReflectivity (Workspace &ws, Matrix &surface_los, Tensor4 &surface_rmatrix, Matrix &surface_emission, const Vector &f_grid, const Index &stokes_dim, const Index &atmosphere_dim, const Vector &specular_los, const Numeric &surface_skin_t, const Tensor3 &surface_reflectivity, const Agenda &blackbody_radiation_agenda, const Verbosity &verbosity)
	WORKSPACE METHOD: surfaceFlatReflectivity. More...

void	surfaceFlatScalarReflectivity (Workspace &ws, Matrix &surface_los, Tensor4 &surface_rmatrix, Matrix &surface_emission, const Vector &f_grid, const Index &stokes_dim, const Index &atmosphere_dim, const Vector &specular_los, const Numeric &surface_skin_t, const Vector &surface_scalar_reflectivity, const Agenda &blackbody_radiation_agenda, const Verbosity &verbosity)
	WORKSPACE METHOD: surfaceFlatScalarReflectivity. More...

void	surfaceLambertianSimple (Workspace &ws, Matrix &surface_los, Tensor4 &surface_rmatrix, Matrix &surface_emission, const Vector &f_grid, const Index &stokes_dim, const Index &atmosphere_dim, const Vector &rtp_los, const Numeric &surface_skin_t, const Vector &surface_scalar_reflectivity, const Index &lambertian_nza, const Agenda &blackbody_radiation_agenda, const Numeric &za_pos, const Verbosity &)
	WORKSPACE METHOD: surfaceLambertianSimple. More...

void	surface_complex_refr_indexFromGriddedField5 (GriddedField3 &surface_complex_refr_index, const Index &atmosphere_dim, const Vector &lat_grid, const Vector &lat_true, const Vector &lon_true, const Vector &rtp_pos, const GriddedField5 &complex_n_field, const Verbosity &)
	WORKSPACE METHOD: surface_complex_refr_indexFromGriddedField5. More...

void	surface_reflectivityFromGriddedField6 (Tensor3 &surface_reflectivity, const Index &stokes_dim, const Vector &f_grid, const Index &atmosphere_dim, const Vector &lat_grid, const Vector &lat_true, const Vector &lon_true, const Vector &rtp_pos, const Vector &rtp_los, const GriddedField6 &r_field, const Verbosity &)
	WORKSPACE METHOD: surface_reflectivityFromGriddedField6. More...

void	surface_scalar_reflectivityFromGriddedField4 (Vector &surface_scalar_reflectivity, const Index &stokes_dim, const Vector &f_grid, const Index &atmosphere_dim, const Vector &lat_grid, const Vector &lat_true, const Vector &lon_true, const Vector &rtp_pos, const Vector &rtp_los, const GriddedField4 &r_field, const Verbosity &)
	WORKSPACE METHOD: surface_scalar_reflectivityFromGriddedField4. More...

Variables
const Numeric	DEG2RAD

Detailed Description

Workspace functions associated wih the surface and its properties.

Author: Patrick Eriksson Patri.nosp@m.ck.E.nosp@m.rikss.nosp@m.on@c.nosp@m.halme.nosp@m.rs.s.nosp@m.e

Date: 2008-09-17

These functions are listed in the doxygen documentation as entries of the file auto_md.h.

Definition in file m_surface.cc.

Function Documentation

◆ InterpSurfaceFieldToPosition()

void InterpSurfaceFieldToPosition	(	Numeric &	out,
		const Index &	atmosphere_dim,
		const Vector &	lat_grid,
		const Vector &	lon_grid,
		const Vector &	rtp_pos,
		const Matrix &	z_surface,
		const Matrix &	field,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: InterpSurfaceFieldToPosition.

Point interpolation of surface fields.

The default way to specify the position is by rtp_pos.

Linear interpolation is applied.

The interpolation is done for the latitude and longitude in rtp_pos*, while the altitude in rtp_pos is not part of the calculations. However, it is checked that the altitude of rtp_pos is inside the range covered by z_surface with a 1 m margin, to give a warning when the specified position is not consistent with the surface altitudes.

Author: Patrick Eriksson

Parameters

[out]	out	Generic output
[in]	atmosphere_dim	WS Input
[in]	lat_grid	WS Input
[in]	lon_grid	WS Input
[in]	rtp_pos	WS Input
[in]	z_surface	WS Input
[in]	field	Generic Input

Definition at line 68 of file m_surface.cc.

References chk_atm_grids(), chk_atm_surface(), chk_interpolation_grids(), chk_rte_pos(), CREATE_OUT3, gridpos(), interp_atmsurface_by_gp(), max, and min.

Referenced by InterpSurfaceFieldToPosition_g().

◆ iySurfaceRtpropAgenda()

void iySurfaceRtpropAgenda	(	Workspace &	ws,
		Matrix &	iy,
		ArrayOfTensor3 &	diy_dx,
		const Tensor3 &	iy_transmission,
		const Index &	jacobian_do,
		const Index &	atmosphere_dim,
		const Tensor3 &	t_field,
		const Tensor3 &	z_field,
		const Tensor4 &	vmr_field,
		const Index &	cloudbox_on,
		const Index &	stokes_dim,
		const Vector &	f_grid,
		const Vector &	rtp_pos,
		const Vector &	rtp_los,
		const Vector &	rte_pos2,
		const Agenda &	iy_main_agenda,
		const Agenda &	surface_rtprop_agenda,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: iySurfaceRtpropAgenda.

Interface to surface_rtprop_agenda for iy_surface_agenda.

This method is designed to be part of iy_surface_agenda. It determines the radiative properties of the surface by surface_rtprop_agenda* and calculates the downwelling radiation by iy_main_agenda, and sums up the terms as described in AUG. That is, this WSM uses the output from surface_rtprop_agenda in a straightforward fashion.

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	iy	WS Output
[out]	diy_dx	WS Output
[in]	iy_transmission	WS Input
[in]	jacobian_do	WS Input
[in]	atmosphere_dim	WS Input
[in]	t_field	WS Input
[in]	z_field	WS Input
[in]	vmr_field	WS Input
[in]	cloudbox_on	WS Input
[in]	stokes_dim	WS Input
[in]	f_grid	WS Input
[in]	rtp_pos	WS Input
[in]	rtp_los	WS Input
[in]	rte_pos2	WS Input
[in]	iy_main_agenda	WS Input
[in]	surface_rtprop_agenda	WS Input

Definition at line 124 of file m_surface.cc.

References chk_if_in_range(), chk_rte_los(), chk_rte_pos(), iy_main_agendaExecute(), iy_transmission_mult(), joker, Agenda::name(), ConstTensor4View::nbooks(), ConstTensor4View::ncols(), ConstMatrixView::ncols(), ConstVectorView::nelem(), ConstTensor3View::npages(), ConstTensor4View::npages(), ConstTensor4View::nrows(), ConstMatrixView::nrows(), surface_calc(), and surface_rtprop_agendaExecute().

Referenced by iySurfaceRtpropAgenda_g().

◆ specular_losCalc()

void specular_losCalc	(	Vector &	specular_los,
		Vector &	surface_normal,
		const Vector &	rtp_pos,
		const Vector &	rtp_los,
		const Index &	atmosphere_dim,
		const Vector &	lat_grid,
		const Vector &	lon_grid,
		const Vector &	refellipsoid,
		const Matrix &	z_surface,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: specular_losCalc.

Calculates the specular direction for intersections with the surface.

A help method to set up the surface properties. This method calculates specular_los, that is required in several methods to convert zenith angles to incidence angles.

The method also returns the line-of-sight for the surface normal.

Author: Patrick Eriksson

Parameters

[out]	specular_los	WS Output
[out]	surface_normal	WS Output
[in]	rtp_pos	WS Input
[in]	rtp_los	WS Input
[in]	atmosphere_dim	WS Input
[in]	lat_grid	WS Input
[in]	lon_grid	WS Input
[in]	refellipsoid	WS Input
[in]	z_surface	WS Input

Definition at line 243 of file m_surface.cc.

References cart2zaaa(), chk_interpolation_grids(), cross3(), fac(), gridpos(), interp(), interpweights(), joker, max, plevel_angletilt(), plevel_slope_2d(), plevel_slope_3d(), refell2d(), Vector::resize(), sign(), and zaaa2cart().

Referenced by specular_losCalc_g().

◆ surface_complex_refr_indexFromGriddedField5()

void surface_complex_refr_indexFromGriddedField5	(	GriddedField3 &	surface_complex_refr_index,
		const Index &	atmosphere_dim,
		const Vector &	lat_grid,
		const Vector &	lat_true,
		const Vector &	lon_true,
		const Vector &	rtp_pos,
		const GriddedField5 &	complex_refr_index_field,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surface_complex_refr_indexFromGriddedField5.

Extracts complex refractive index from a field of such data.

The method allows to obtain surface_complex_refr_index by interpolation of a geographical field of such data. The position for which refraction shall be extracted is given by rtp_pos. The refractive index field is expected to be stored as: GriddedField5: Vector f_grid[N_f] Vector T_grid[N_T] ArrayOfString Complex[2] Vector "Latitude" [N_lat] Vector "Longitude" [N_lon] Tensor5 data[N_f][N_T][2][N_lat][N_lon]

Definition and treatment of the three first dimensions follows complex_refr_index*, e.g. the temperature grid is allowed to have length 1. The grids for latitude and longitude must have a length of >= 2 (ie. no automatic expansion).

Hence, this method performs an interpolation only in the lat and lon dimensions, to a single point. The remaining GriddedField3 is simply returned as surface_complex_refr_index.

Author: Patrick Eriksson

Parameters

[out]	surface_complex_refr_index	WS Output
[in]	atmosphere_dim	WS Input
[in]	lat_grid	WS Input
[in]	lat_true	WS Input
[in]	lon_true	WS Input
[in]	rtp_pos	WS Input
[in]	complex_refr_index_field	Generic Input

Definition at line 693 of file m_surface.cc.

References GriddedField5::checksize_strict(), chk_griddedfield_gridname(), chk_if_in_range(), chk_latlon_true(), chk_rte_pos(), GriddedField3::data, GriddedField5::data, GriddedField::get_numeric_grid(), gridpos(), interp(), interpweights(), joker, lon_shiftgrid(), ConstTensor5View::nbooks(), ConstTensor5View::ncols(), ConstTensor5View::npages(), ConstTensor5View::nrows(), ConstTensor5View::nshelves(), pos2true_latlon(), GriddedField3::resize(), GriddedField::set_grid(), and GriddedField::set_grid_name().

Referenced by surface_complex_refr_indexFromGriddedField5_g().

◆ surface_reflectivityFromGriddedField6()

void surface_reflectivityFromGriddedField6	(	Tensor3 &	surface_reflectivity,
		const Index &	stokes_dim,
		const Vector &	f_grid,
		const Index &	atmosphere_dim,
		const Vector &	lat_grid,
		const Vector &	lat_true,
		const Vector &	lon_true,
		const Vector &	rtp_pos,
		const Vector &	rtp_los,
		const GriddedField6 &	r_field,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surface_reflectivityFromGriddedField6.

Extracts surface reflectivities from a field of such data.

This method allows to specify a field of surface reflectivity for automatic interpolation to points of interest. The position and direction for which the reflectivity shall be extracted are given by rtp_pos and rtp_los. The reflectivity field is expected to be stored as: GriddedField6: Vector "Frequency" [N_f] Vector "Stokes element" [N_s1] Vector "Stokes_element" [N_s2] Vector "Incidence angle" [N_ia] Vector "Latitude" [N_lat] Vector "Longitude" [N_lon] Tensor6 data[N_f][N_s1][N_s2][N_ia][N_lat][N_lon]

Grids for incidence angle, latitude and longitude must have a length of >= 2 (ie. no automatic expansion). If the frequency grid has length 1, this is taken as that the reflectivity is constant, following the definition of surface_scalar_reflectivity. The data can cover higher Stokes dimensionalities than set by stokes_dim*. Data for non-used Stokes elements are just cropped. The order between the two Stokes dimensions is the same as in surface_reflectivity* and surface_rmatrix*.

The interpolation is done in steps: 1: Linear interpolation for lat and lon (std. extrapolation). 2: Interpolation in incidence angle (std. extrapolation). If the grid has a length of >= 4, cubic interpolation is applied. Otherwise linear interpolation. 3. Linear interpolation in frequency (if input data have more than one frequency).

Author: Patrick Eriksson

Parameters

[out]	surface_reflectivity	WS Output
[in]	stokes_dim	WS Input
[in]	f_grid	WS Input
[in]	atmosphere_dim	WS Input
[in]	lat_grid	WS Input
[in]	lat_true	WS Input
[in]	lon_true	WS Input
[in]	rtp_pos	WS Input
[in]	rtp_los	WS Input
[in]	r_field	Generic Input

Definition at line 796 of file m_surface.cc.

References GriddedField6::checksize_strict(), chk_griddedfield_gridname(), chk_if_in_range(), chk_interpolation_grids(), chk_latlon_true(), chk_rte_los(), chk_rte_pos(), GriddedField6::data, GriddedField::get_numeric_grid(), gridpos(), gridpos_poly(), interp(), interpweights(), joker, lon_shiftgrid(), ConstTensor6View::nbooks(), ConstTensor6View::ncols(), ConstVectorView::nelem(), ConstTensor6View::npages(), ConstTensor6View::nrows(), ConstTensor6View::nshelves(), ConstTensor6View::nvitrines(), pos2true_latlon(), and Tensor3::resize().

Referenced by surface_reflectivityFromGriddedField6_g().

◆ surface_scalar_reflectivityFromGriddedField4()

void surface_scalar_reflectivityFromGriddedField4	(	Vector &	surface_scalar_reflectivity,
		const Index &	stokes_dim,
		const Vector &	f_grid,
		const Index &	atmosphere_dim,
		const Vector &	lat_grid,
		const Vector &	lat_true,
		const Vector &	lon_true,
		const Vector &	rtp_pos,
		const Vector &	rtp_los,
		const GriddedField4 &	r_field,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surface_scalar_reflectivityFromGriddedField4.

Extracts scalar surface reflectivities from a field of such data.

This method allows to specify a field of surface reflectivity for automatic interpolation to points of interest. The position and direction for which the reflectivity shall be extracted are given by rtp_pos and rtp_los. The reflectivity field is expected to be stored as: GriddedField4: Vector "Frequency" [N_f] Vector "Incidence angle" [N_ia] Vector "Latitude" [N_lat] Vector "Longitude" [N_lon] Tensor4 data[N_f][N_ia][N_lat][N_lon]

Grids for incidence angle, latitude and longitude must have a length of >= 2 (ie. no automatic expansion). If the frequency grid has length 1, this is taken as the reflectivity is constant, following the definition of surface_scalar_reflectivity.

The interpolation is done in steps: 1: Linear interpolation for lat and lon (std. extrapolation). 2: Interpolation in incidence angle (std. extrapolation). If the grid has a length of >= 4, cubic interpolation is applied. Otherwise linear interpolation. 3. Linear interpolation if frequency (if input data have more than one frequency).

Author: Patrick Eriksson

Parameters

[out]	surface_scalar_reflectivity	WS Output
[in]	stokes_dim	WS Input
[in]	f_grid	WS Input
[in]	atmosphere_dim	WS Input
[in]	lat_grid	WS Input
[in]	lat_true	WS Input
[in]	lon_true	WS Input
[in]	rtp_pos	WS Input
[in]	rtp_los	WS Input
[in]	r_field	Generic Input

Definition at line 933 of file m_surface.cc.

References GriddedField4::checksize_strict(), chk_griddedfield_gridname(), chk_if_in_range(), chk_interpolation_grids(), chk_latlon_true(), chk_rte_los(), chk_rte_pos(), GriddedField4::data, GriddedField::get_numeric_grid(), gridpos(), gridpos_poly(), interp(), interpweights(), joker, lon_shiftgrid(), ConstTensor4View::nbooks(), ConstTensor4View::ncols(), ConstVectorView::nelem(), ConstTensor4View::npages(), ConstTensor4View::nrows(), pos2true_latlon(), and Vector::resize().

Referenced by surface_scalar_reflectivityFromGriddedField4_g().

◆ surfaceBlackbody()

void surfaceBlackbody	(	Workspace &	ws,
		Matrix &	surface_los,
		Tensor4 &	surface_rmatrix,
		Matrix &	surface_emission,
		const Vector &	f_grid,
		const Index &	stokes_dim,
		const Numeric &	surface_skin_t,
		const Agenda &	blackbody_radiation_agenda,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surfaceBlackbody.

Creates variables to mimic a blackbody surface.

This method sets up surface_los, surface_rmatrix and surface_emission* for surface_rtprop_agenda. Here, surface_los and surface_rmatrix are set to be empty, and surface_emission to hold blackbody radiation for a temperature of surface_skin_t.

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	surface_los	WS Output
[out]	surface_rmatrix	WS Output
[out]	surface_emission	WS Output
[in]	f_grid	WS Input
[in]	stokes_dim	WS Input
[in]	surface_skin_t	WS Input
[in]	blackbody_radiation_agenda	WS Input

Definition at line 324 of file m_surface.cc.

References blackbody_radiation_agendaExecute(), chk_if_in_range(), chk_not_negative(), CREATE_OUT2, ConstVectorView::nelem(), Tensor4::resize(), and Matrix::resize().

Referenced by surfaceBlackbody_g().

◆ surfaceFlatReflectivity()

void surfaceFlatReflectivity	(	Workspace &	ws,
		Matrix &	surface_los,
		Tensor4 &	surface_rmatrix,
		Matrix &	surface_emission,
		const Vector &	f_grid,
		const Index &	stokes_dim,
		const Index &	atmosphere_dim,
		const Vector &	specular_los,
		const Numeric &	surface_skin_t,
		const Tensor3 &	surface_reflectivity,
		const Agenda &	blackbody_radiation_agenda,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surfaceFlatReflectivity.

Creates variables to mimic specular reflection by a (flat) surface where surface_reflectivity is specified.

Works basically as surfaceFlatScalarReflectivity but is more general as also vector radiative transfer is handled. See the ARTS theory document (ATD) for details around how surface_emission* is determined. In the nomenclature of ATD, surface_reflectivity* gives R.

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	surface_los	WS Output
[out]	surface_rmatrix	WS Output
[out]	surface_emission	WS Output
[in]	f_grid	WS Input
[in]	stokes_dim	WS Input
[in]	atmosphere_dim	WS Input
[in]	specular_los	WS Input
[in]	surface_skin_t	WS Input
[in]	surface_reflectivity	WS Input
[in]	blackbody_radiation_agenda	WS Input

Definition at line 431 of file m_surface.cc.

References blackbody_radiation_agendaExecute(), chk_if_in_range(), chk_not_negative(), CREATE_OUT2, joker, mult(), ConstTensor3View::ncols(), ConstVectorView::nelem(), ConstTensor3View::npages(), ConstTensor3View::nrows(), Tensor4::resize(), and Matrix::resize().

Referenced by surfaceFlatReflectivity_g().

◆ surfaceFlatRefractiveIndex()

void surfaceFlatRefractiveIndex	(	Workspace &	ws,
		Matrix &	surface_los,
		Tensor4 &	surface_rmatrix,
		Matrix &	surface_emission,
		const Vector &	f_grid,
		const Index &	stokes_dim,
		const Index &	atmosphere_dim,
		const Vector &	rtp_los,
		const Vector &	specular_los,
		const Numeric &	surface_skin_t,
		const GriddedField3 &	surface_complex_refr_index,
		const Agenda &	blackbody_radiation_agenda,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surfaceFlatRefractiveIndex.

Creates variables to mimic specular reflection by a (flat) surface where the complex refractive index is specified.

The dielectric properties of the surface are described by surface_complex_refr_index*. The Fresnel equations are used to calculate amplitude reflection coefficients. The method can thus result in that the reflection properties differ between frequencies and polarisations.

Local thermodynamic equilibrium is assumed, which corresponds to that the reflection and emission coefficients add up to 1.

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	surface_los	WS Output
[out]	surface_rmatrix	WS Output
[out]	surface_emission	WS Output
[in]	f_grid	WS Input
[in]	stokes_dim	WS Input
[in]	atmosphere_dim	WS Input
[in]	rtp_los	WS Input
[in]	specular_los	WS Input
[in]	surface_skin_t	WS Input
[in]	surface_complex_refr_index	WS Input
[in]	blackbody_radiation_agenda	WS Input

Definition at line 364 of file m_surface.cc.

References calc_incang(), chk_if_in_range(), chk_not_negative(), complex_n_interp(), CREATE_OUT2, CREATE_OUT3, fresnel(), joker, ConstVectorView::nelem(), Tensor4::resize(), Matrix::resize(), and surface_specular_R_and_b().

Referenced by surfaceFlatRefractiveIndex_g().

◆ surfaceFlatScalarReflectivity()

void surfaceFlatScalarReflectivity	(	Workspace &	ws,
		Matrix &	surface_los,
		Tensor4 &	surface_rmatrix,
		Matrix &	surface_emission,
		const Vector &	f_grid,
		const Index &	stokes_dim,
		const Index &	atmosphere_dim,
		const Vector &	specular_los,
		const Numeric &	surface_skin_t,
		const Vector &	surface_scalar_reflectivity,
		const Agenda &	blackbody_radiation_agenda,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surfaceFlatScalarReflectivity.

Creates variables to mimic specular reflection by a (flat) surface where surface_scalar_reflectivity is specified.

The method can only be used for stokes_dim equal to 1. Local thermodynamic equilibrium is assumed, which corresponds to that reflectivity and emissivity add up to 1.

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	surface_los	WS Output
[out]	surface_rmatrix	WS Output
[out]	surface_emission	WS Output
[in]	f_grid	WS Input
[in]	stokes_dim	WS Input
[in]	atmosphere_dim	WS Input
[in]	specular_los	WS Input
[in]	surface_skin_t	WS Input
[in]	surface_scalar_reflectivity	WS Input
[in]	blackbody_radiation_agenda	WS Input

Definition at line 523 of file m_surface.cc.

References blackbody_radiation_agendaExecute(), chk_if_in_range(), chk_not_negative(), CREATE_OUT2, CREATE_OUT3, joker, max, min, ConstVectorView::nelem(), Tensor4::resize(), and Matrix::resize().

Referenced by surfaceFlatScalarReflectivity_g().

◆ surfaceLambertianSimple()

void surfaceLambertianSimple	(	Workspace &	ws,
		Matrix &	surface_los,
		Tensor4 &	surface_rmatrix,
		Matrix &	surface_emission,
		const Vector &	f_grid,
		const Index &	stokes_dim,
		const Index &	atmosphere_dim,
		const Vector &	rtp_los,
		const Numeric &	surface_skin_t,
		const Vector &	surface_scalar_reflectivity,
		const Index &	lambertian_nza,
		const Agenda &	blackbody_radiation_agenda,
		const Numeric &	za_pos,
		const Verbosity &	verbosity
	)

WORKSPACE METHOD: surfaceLambertianSimple.

Creates variables to mimic a Lambertian surface.

The method can only be used for 1D calculations.

A Lambertian surface can be characterised solely by its reflectivity, here taken from surface_scalar_reflectivity.

The down-welling radiation field is estimated by making calculations for lambertian_nza directions. The range of zenith angles ([0,90]) is divided in an equidistant manner. The values for surface_rmatrix are assuming a constant radiance over each zenith angle range. See AUG.

Default is to select the zenith angles for sensor_los to be placed centrally in the grid ranges. For example, if lambertian_nza is set to 9, down-welling radiation will be calculated for zenith angles = 5, 15, ..., 85. The position of these angles can be shifted by za_pos*. This variable specifies the fractional distance inside the ranges. For example, a za_pos of 0.7 (np still 9) gives the angles 7, 17, ..., 87.

Only upper-left diagonal element of the surface_rmatrix-es is non-zero. That is, the upwelling radiation is always unpolarised.

Local thermodynamic equilibrium is assumed, which corresponds to that the reflection and emission coefficients "add up to 1".

Author: Patrick Eriksson

Parameters

[in,out]	ws	Workspace
[out]	surface_los	WS Output
[out]	surface_rmatrix	WS Output
[out]	surface_emission	WS Output
[in]	f_grid	WS Input
[in]	stokes_dim	WS Input
[in]	atmosphere_dim	WS Input
[in]	rtp_los	WS Input
[in]	surface_skin_t	WS Input
[in]	surface_scalar_reflectivity	WS Input
[in]	lambertian_nza	WS Input
[in]	blackbody_radiation_agenda	WS Input
[in]	za_pos	Generic Input (Default: "0.5")

Definition at line 594 of file m_surface.cc.

References blackbody_radiation_agendaExecute(), chk_if_in_range(), chk_not_negative(), DEG2RAD, max, min, ConstVectorView::nelem(), Tensor4::resize(), Matrix::resize(), and w().

Referenced by surfaceLambertianSimple_g().

Variable Documentation

◆ DEG2RAD

const Numeric DEG2RAD

Referenced by surfaceLambertianSimple().

Functions

Variables

Detailed Description

Function Documentation

◆ InterpSurfaceFieldToPosition()

◆ iySurfaceRtpropAgenda()

◆ specular_losCalc()

◆ surface_complex_refr_indexFromGriddedField5()

◆ surface_reflectivityFromGriddedField6()

◆ surface_scalar_reflectivityFromGriddedField4()

◆ surfaceBlackbody()

◆ surfaceFlatReflectivity()

◆ surfaceFlatRefractiveIndex()

◆ surfaceFlatScalarReflectivity()

◆ surfaceLambertianSimple()

Variable Documentation

◆ DEG2RAD