Functions to solve radiative transfer tasks. More...

#include <cmath>
#include <stdexcept>
#include "auto_md.h"
#include "check_input.h"
#include "logic.h"
#include "math_funcs.h"
#include "montecarlo.h"
#include "physics_funcs.h"
#include "ppath.h"
#include "rte.h"
#include "special_interp.h"
#include "lin_alg.h"

Functions
void	apply_y_unit (MatrixView iy, const String &y_unit, ConstVectorView f_grid, const ArrayOfIndex &i_pol)
	apply_y_unit More...

void	apply_y_unit2 (Tensor3View J, ConstMatrixView iy, const String &y_unit, ConstVectorView f_grid, const ArrayOfIndex &i_pol)
	apply_y_unit2 More...

void	ext2trans (MatrixView trans_mat, ConstMatrixView ext_mat_av, const Numeric &l_step)
	ext2trans More...

void	get_ppath_atmvars (Vector &ppath_p, Vector &ppath_t, Matrix &ppath_vmr, Vector &ppath_wind_u, Vector &ppath_wind_v, Vector &ppath_wind_w, const Ppath &ppath, const Index &atmosphere_dim, ConstVectorView p_grid, ConstTensor3View t_field, ConstTensor4View vmr_field, ConstTensor3View wind_u_field, ConstTensor3View wind_v_field, ConstTensor3View wind_w_field)
	get_ppath_atmvars More...

void	get_ppath_pnd (Matrix &ppath_pnd, const Ppath &ppath, const Index &atmosphere_dim, const ArrayOfIndex &cloudbox_limits, ConstTensor4View pnd_field)
	get_ppath_pnd More...

void	get_ppath_rtvars (Workspace &ws, Tensor3 &ppath_abs_scalar, Matrix &ppath_tau, Vector &total_tau, Matrix &ppath_emission, const Agenda &abs_scalar_gas_agenda, const Agenda &emission_agenda, const Ppath &ppath, ConstVectorView ppath_p, ConstVectorView ppath_t, ConstMatrixView ppath_vmr, ConstVectorView ppath_wind_u, ConstVectorView ppath_wind_v, ConstVectorView ppath_wind_w, ConstVectorView f_grid, const Index &atmosphere_dim, const Index &emission_do)
	get_ppath_rtvars More...

void	get_ppath_cloudrtvars (Workspace &ws, Tensor3 &ppath_asp_abs_vec, Tensor4 &ppath_asp_ext_mat, Tensor3 &ppath_pnd_abs_vec, Tensor4 &ppath_pnd_ext_mat, Tensor4 &ppath_transmission, Tensor3 &total_transmission, Matrix &ppath_emission, Array< ArrayOfSingleScatteringData > &scat_data, const Agenda &abs_scalar_gas_agenda, const Agenda &emission_agenda, const Agenda &opt_prop_gas_agenda, const Ppath &ppath, ConstVectorView ppath_p, ConstVectorView ppath_t, ConstMatrixView ppath_vmr, ConstVectorView ppath_wind_u, ConstVectorView ppath_wind_v, ConstVectorView ppath_wind_w, ConstMatrixView ppath_pnd, const Index &use_mean_scat_data, const ArrayOfSingleScatteringData &scat_data_raw, const Index &stokes_dim, ConstVectorView f_grid, const Index &atmosphere_dim, const Index &emission_do, const Verbosity &verbosity)
	get_ppath_cloudrtvars More...

Range	get_rowindex_for_mblock (const Sparse &sensor_response, const Index &imblock)
	get_rowindex_for_mblock More...

void	iy_transmission_for_scalar_tau (Tensor3 &iy_transmission, const Index &stokes_dim, ConstVectorView tau)
	iy_transmission_for_scalar_tau More...

void	iy_transmission_mult (Tensor3 &iy_trans_new, ConstTensor3View iy_transmission, ConstTensor3View trans)
	iy_transmission_mult More...

void	iy_transmission_mult_scalar_tau (Tensor3 &iy_trans_new, ConstTensor3View iy_transmission, ConstVectorView tau)
	iy_transmission_mult_scalar_tau More...

void	mirror_los (Vector &los_mirrored, ConstVectorView los, const Index &atmosphere_dim)
	mirror_los More...

void	rte_step_std (VectorView stokes_vec, MatrixView trans_mat, ConstMatrixView ext_mat_av, ConstVectorView abs_vec_av, ConstVectorView sca_vec_av, const Numeric &l_step, const Numeric &rte_planck_value)
	rte_step_std More...

void	surface_calc (Matrix &iy, const Tensor3 &I, const Matrix &surface_los, const Tensor4 &surface_rmatrix, const Matrix &surface_emission)
	surface_calc More...

void	trans_step_std (VectorView stokes_vec, MatrixView trans_mat, ConstMatrixView ext_mat_av, const Numeric &l_step)
	trans_step_std More...

Variables
const Numeric	BOLTZMAN_CONST

const Numeric	PLANCK_CONST

const Numeric	SPEED_OF_LIGHT

const Numeric	PI

const Numeric	DEG2RAD

const Numeric	RAD2DEG

Detailed Description

Functions to solve radiative transfer tasks.

Author: Patrick Eriksson Patri.nosp@m.ck.E.nosp@m.rikss.nosp@m.on@r.nosp@m.ss.ch.nosp@m.alme.nosp@m.rs.se

Date: 2002-05-29

Definition in file rte.cc.

Function Documentation

◆ apply_y_unit()

void apply_y_unit	(	MatrixView	iy,
		const String &	y_unit,
		ConstVectorView	f_grid,
		const ArrayOfIndex &	i_pol
	)

apply_y_unit

Performs conversion from radiance to other units.

Use apply_y_unit_jac for conversion of jacobian data.

Parameters

iy	In/Out: Tensor3 with data to be converted, where column dimension corresponds to Stokes dimensionality and row dimension corresponds to frequency.
y_unit	As the WSV.
f_grid	As the WSV.
i_pol	Polarisation indexes. See documentation of y_pol.

Author: Patrick Eriksson

Date: 2010-04-07

Definition at line 82 of file rte.cc.

References invplanck(), invrayjean(), ConstMatrixView::ncols(), Array< base >::nelem(), ConstVectorView::nelem(), ConstMatrixView::nrows(), ns, and SPEED_OF_LIGHT.

Referenced by iyb_calc(), and y_unitApply().

◆ apply_y_unit2()

void apply_y_unit2	(	Tensor3View	J,
		ConstMatrixView	iy,
		const String &	y_unit,
		ConstVectorView	f_grid,
		const ArrayOfIndex &	i_pol
	)

apply_y_unit2

Largely as apply_y_unit but operates on jacobian data.

The associated spectrum data iy must be in radiance. That is, the spectrum can only be converted to Tb after the jacobian data.

iy* must be a single spectrum, and is accordingly here a matrix (and not a Tensor3 as for apply_y_unit).

Parameters

J	In/Out: Tensor3 with data to be converted, where column dimension corresponds to Stokes dimensionality and row dimension corresponds to frequency.
iy	Associated radiance data.
y_unit	As the WSV.
f_grid	As the WSV.

Author: Patrick Eriksson

Date: 2010-04-10

Definition at line 184 of file rte.cc.

References dinvplanckdI(), invrayjean(), ConstMatrixView::ncols(), ConstTensor3View::ncols(), Array< base >::nelem(), ConstVectorView::nelem(), ConstTensor3View::npages(), ConstMatrixView::nrows(), ConstTensor3View::nrows(), ns, and SPEED_OF_LIGHT.

Referenced by iyb_calc(), and y_unitApply().

◆ ext2trans()

void ext2trans	(	MatrixView	trans_mat,
		ConstMatrixView	ext_mat_av,
		const Numeric &	l_step
	)

ext2trans

Converts an extinction matrix to a transmission matrix

The function performs the calculations differently depending on the conditions to improve the speed. There are three cases:

Scalar absorption.
The matrix ext_mat_av is diagonal.
The total general case.

Parameters

trans_mat	Input/Output: Transmission matrix of slab.
ext_mat	Input: Averaged extinction matrix.
l_step	Input: The length of the RTE step.

Author: Claudia Emde and Patrick Eriksson,

Date: 2010-10-15

Definition at line 301 of file rte.cc.

References is_diagonal(), is_singular(), is_size(), matrix_exp(), ConstMatrixView::nrows(), and q.

Referenced by get_ppath_cloudrtvars(), and trans_step_std().

◆ get_ppath_atmvars()

void get_ppath_atmvars	(	Vector &	ppath_p,
		Vector &	ppath_t,
		Matrix &	ppath_vmr,
		Vector &	ppath_wind_u,
		Vector &	ppath_wind_v,
		Vector &	ppath_wind_w,
		const Ppath &	ppath,
		const Index &	atmosphere_dim,
		ConstVectorView	p_grid,
		ConstTensor3View	t_field,
		ConstTensor4View	vmr_field,
		ConstTensor3View	wind_u_field,
		ConstTensor3View	wind_v_field,
		ConstTensor3View	wind_w_field
	)

get_ppath_atmvars

Determines pressure, temperature, VMR and winds for each propgataion path point.

The output variables are sized inside the function. For VMR the dimensions are [ species, propagation path point ].

Parameters

ppath_p	Out: Pressure for each ppath point.
ppath_t	Out: Temperature for each ppath point.
ppath_vmr	Out: VMR values for each ppath point.
ppath_wind_u	Out: U-wind for each ppath point.
ppath_wind_v	Out: V-wind for each ppath point.
ppath_wind_w	Out: W-wind for each ppath point.
ppath	As the WSV.
atmosphere_dim	As the WSV.
p_grid	As the WSV.
lat_grid	As the WSV.
lon_grid	As the WSV.
t_field	As the WSV.
vmr_field	As the WSV.
wind_u_field	As the WSV.
wind_v_field	As the WSV.
wind_w_field	As the WSV.

Author: Patrick Eriksson

Date: 2009-10-05

Definition at line 383 of file rte.cc.

References Ppath::gp_lat, Ppath::gp_lon, Ppath::gp_p, interp_atmfield_by_itw(), interp_atmfield_gp2itw(), interpweights(), itw2p(), joker, ConstTensor4View::nbooks(), Ppath::np, ConstTensor3View::npages(), ns, Vector::resize(), and Matrix::resize().

Referenced by iyBeerLambertStandardClearsky(), iyBeerLambertStandardCloudbox(), iyEmissionStandardClearsky(), iyEmissionStandardClearskyBasic(), and iyFOS().

◆ get_ppath_cloudrtvars()

void get_ppath_cloudrtvars	(	Workspace &	ws,
		Tensor3 &	ppath_asp_abs_vec,
		Tensor4 &	ppath_asp_ext_mat,
		Tensor3 &	ppath_pnd_abs_vec,
		Tensor4 &	ppath_pnd_ext_mat,
		Tensor4 &	ppath_transmission,
		Tensor3 &	total_transmission,
		Matrix &	ppath_emission,
		Array< ArrayOfSingleScatteringData > &	scat_data,
		const Agenda &	abs_scalar_gas_agenda,
		const Agenda &	emission_agenda,
		const Agenda &	opt_prop_gas_agenda,
		const Ppath &	ppath,
		ConstVectorView	ppath_p,
		ConstVectorView	ppath_t,
		ConstMatrixView	ppath_vmr,
		ConstVectorView	ppath_wind_u,
		ConstVectorView	ppath_wind_v,
		ConstVectorView	ppath_wind_w,
		ConstMatrixView	ppath_pnd,
		const Index &	use_mean_scat_data,
		const ArrayOfSingleScatteringData &	scat_data_raw,
		const Index &	stokes_dim,
		ConstVectorView	f_grid,
		const Index &	atmosphere_dim,
		const Index &	emission_do,
		const Verbosity &	verbosity
	)

get_ppath_cloudrtvars

Determines variables for each step of "standard" RT integration

See code for details about dimensions etc.

Parameters

ws	Out: The workspace
ppath_asp_abs_vec	Out: Absorption vectors for absorption species
ppath_asp_ext_vec	Out: Extinction matrices for absorption species
ppath_pnd_abs_vec	Out: Absorption vectors for particles
ppath_pnd_ext_vec	Out: Extinction matrices for particles
ppath_transmission	Out: Transmissions of each ppath step
total_transmission	Out: Total transmission of path
ppath_emission	Out: Emission source term at each ppath point
scat_data	Out: Extracted scattering data. Length of array affected by use_mean_scat_data.
abs_scalar_gas_agenda	As the WSV.
emission_agenda	As the WSV.
opt_prop_gas_agenda	As the WSV.
ppath_p	Pressure for each ppath point.
ppath_t	Temperature for each ppath point.
ppath_vmr	VMR values for each ppath point.
ppath_wind_u	U-wind for each ppath point.
ppath_wind_v	V-wind for each ppath point.
ppath_wind_w	W-wind for each ppath point.
ppath_pnd	Particle number densities for each ppath point.
use_mean_scat_data	As the WSV.
scat_data_raw	As the WSV.
stokes_dim	As the WSV.
f_grid	As the WSV.
atmosphere_dim	As the WSV.
emission_do	Flag for calculation of emission. Should be set to 0 for pure transmission calculations.

Author: Patrick Eriksson

Date: 2011-07-14

Definition at line 672 of file rte.cc.

References abs_scalar_gas_agendaExecute(), emission_agendaExecute(), ext2trans(), id_mat(), joker, Ppath::l_step, Ppath::los, mirror_los(), mult(), ConstVectorView::nelem(), Ppath::np, opt_prop_gas_agendaExecute(), opt_propCalc(), Tensor4::resize(), Tensor3::resize(), Matrix::resize(), and scat_data_monoCalc().

Referenced by iyBeerLambertStandardCloudbox(), and iyFOS().

◆ get_ppath_pnd()

void get_ppath_pnd	(	Matrix &	ppath_pnd,
		const Ppath &	ppath,
		const Index &	atmosphere_dim,
		const ArrayOfIndex &	cloudbox_limits,
		ConstTensor4View	pnd_field
	)

get_ppath_pnd

Determines particle number densities for each propgataion path point.

The output variable is sized inside the function as [ particle type, propagation path point ].

Parameters

ppath_pnd	Out: PND for each ppath point.
ppath	As the WSV.
atmosphere_dim	As the WSV.
pnd_field	As the WSV.

Author: Patrick Eriksson

Date: 2011-07-14

Definition at line 479 of file rte.cc.

References Ppath::gp_lat, Ppath::gp_lon, Ppath::gp_p, interp_atmfield_by_itw(), interp_cloudfield_gp2itw(), joker, ConstTensor4View::nbooks(), Ppath::np, and Matrix::resize().

Referenced by iyBeerLambertStandardCloudbox(), and iyFOS().

◆ get_ppath_rtvars()

void get_ppath_rtvars	(	Workspace &	ws,
		Tensor3 &	ppath_abs_scalar,
		Matrix &	ppath_tau,
		Vector &	total_tau,
		Matrix &	ppath_emission,
		const Agenda &	abs_scalar_gas_agenda,
		const Agenda &	emission_agenda,
		const Ppath &	ppath,
		ConstVectorView	ppath_p,
		ConstVectorView	ppath_t,
		ConstMatrixView	ppath_vmr,
		ConstVectorView	ppath_wind_u,
		ConstVectorView	ppath_wind_v,
		ConstVectorView	ppath_wind_w,
		ConstVectorView	f_grid,
		const Index &	atmosphere_dim,
		const Index &	emission_do
	)

get_ppath_rtvars

Determines variables for each step of "standard" RT integration

The output variables are sized inside the function. The dimension order is [ frequency, absorption species, ppath point ]

Parameters

ws	Out: The workspace
ppath_abs_sclar	Out: Absorption coefficients at each ppath point
ppath_tau	Out: Optical thickness of each ppath step
total_tau	Out: Total optical thickness of path
ppath_emission	Out: Emission source term at each ppath point
abs_scalar_gas_agenda	As the WSV.
emission_agenda	As the WSV.
ppath_p	Pressure for each ppath point.
ppath_t	Temperature for each ppath point.
ppath_vmr	VMR values for each ppath point.
ppath_wind_u	U-wind for each ppath point.
ppath_wind_v	V-wind for each ppath point.
ppath_wind_w	W-wind for each ppath point.
f_grid	As the WSV.
atmosphere_dim	As the WSV.
emission_do	Flag for calculation of emission. Should be set to 0 for pure transmission calculations.

Author: Patrick Eriksson

Date: 2009-10-06

Definition at line 531 of file rte.cc.

References abs_scalar_gas_agendaExecute(), DEG2RAD, emission_agendaExecute(), joker, Ppath::l_step, Ppath::los, ConstVectorView::nelem(), Ppath::np, ConstMatrixView::nrows(), PI, Vector::resize(), Tensor3::resize(), Matrix::resize(), and SPEED_OF_LIGHT.

Referenced by iyBeerLambertStandardClearsky(), iyEmissionStandardClearsky(), and iyEmissionStandardClearskyBasic().

◆ get_rowindex_for_mblock()

Range get_rowindex_for_mblock	(	const Sparse &	sensor_response,
		const Index &	imblock
	)

get_rowindex_for_mblock

Returns the "range" of y corresponding to a measurement block

Returns: The range.

Parameters

sensor_response	As the WSV.
imblock	Index of the measurement block.

Author: Patrick Eriksson

Date: 2009-10-16

Definition at line 861 of file rte.cc.

References Sparse::nrows().

Referenced by jacobianCalcAbsSpeciesPerturbations(), jacobianCalcFreqShiftAndStretchInterp(), jacobianCalcPointingZaInterp(), jacobianCalcPointingZaRecalc(), jacobianCalcPolyfit(), jacobianCalcTemperaturePerturbations(), and yCalc().

◆ iy_transmission_for_scalar_tau()

void iy_transmission_for_scalar_tau	(	Tensor3 &	iy_transmission,
		const Index &	stokes_dim,
		ConstVectorView	tau
	)

iy_transmission_for_scalar_tau

Sets iy_transmission to match scalar optical thicknesses.

iy_transmission* is sized by the function.

Parameters

iy_transmission	Out: As the WSV.
stokes_dim	As the WSV.
tau	Vector with the optical thickness for each frequency.

Author: Patrick Eriksson

Date: 2009-10-06

Definition at line 885 of file rte.cc.

References ConstVectorView::nelem(), and Tensor3::resize().

Referenced by iyBeerLambertStandardClearsky(), and iyEmissionStandardClearsky().

◆ iy_transmission_mult()

void iy_transmission_mult	(	Tensor3 &	iy_trans_new,
		ConstTensor3View	iy_transmission,
		ConstTensor3View	trans
	)

iy_transmission_mult

Multiplicates iy_transmission with (vector) transmissions.

That is, a multiplication of iy_transmission with another variable having same structure and holding transmission values.

The "new path" is assumed to be further away from the sensor than the propagtion path already included in iy_transmission. That is, the operation can be written as:

Ttotal = Told * Tnew

where Told is the transmission corresponding to iy_transmission and Tnew corresponds to tau.

iy_trans_new* is sized by the function.

Parameters

iy_trans_new	Out: Updated version of iy_transmission
iy_transmission	As the WSV.
trans	A variable matching *iy_transmission.

Author: Patrick Eriksson

Date: 2009-10-06

Definition at line 929 of file rte.cc.

References joker, mult(), ConstTensor3View::ncols(), ConstTensor3View::npages(), ConstTensor3View::nrows(), ns, and Tensor3::resize().

Referenced by get_iy_of_background(), iyBeerLambertStandardCloudbox(), and iyFOS().

◆ iy_transmission_mult_scalar_tau()

void iy_transmission_mult_scalar_tau	(	Tensor3 &	iy_trans_new,
		ConstTensor3View	iy_transmission,
		ConstVectorView	tau
	)

iy_transmission_mult_scalar_tau

Multiplicates iy_transmission with scalar optical thicknesses.

The functions can incorporate the transmission of a clear-sky path. That is, the transmission can be described by a single value The transmission of this path is gives as the optical depth for each frequency.

The "new path" is assumed to be further away from the sensor than the propagtion path already included in iy_transmission. That is, the operation can be written as:

Ttotal = Told * Tnew

where Told is the transmission corresponding to iy_transmission and Tnew corresponds to tau.

iy_trans_new* is sized by the function.

Parameters

iy_trans_new	Out: Updated version of iy_transmission
iy_transmission	As the WSV.
tau	Vector with the optical thickness for each frequency.

Author: Patrick Eriksson

Date: 2009-10-06

Definition at line 981 of file rte.cc.

References joker, ConstTensor3View::ncols(), ConstVectorView::nelem(), ConstTensor3View::npages(), and ConstTensor3View::nrows().

Referenced by iyBeerLambertStandardClearsky(), and iyEmissionStandardClearsky().

◆ mirror_los()

void mirror_los	(	Vector &	los_mirrored,
		ConstVectorView	los,
		const Index &	atmosphere_dim
	)

mirror_los

Determines the backward direction for a given line-of-sight.

This function can be used to get the LOS to apply for extracting single scattering properties, if the propagation path LOS is given.

A viewing direction of aa=0 is assumed for 1D. This corresponds to positive za for 2D.

Parameters

los_mirrored	Out: The line-of-sight for reversed direction.
los	A line-of-sight
atmosphere_dim	As the WSV.

Author: Patrick Eriksson

Date: 2011-07-15

Definition at line 1016 of file rte.cc.

References Vector::resize().

Referenced by get_ppath_cloudrtvars(), and iyFOS().

◆ rte_step_std()

void rte_step_std	(	VectorView	stokes_vec,
		MatrixView	trans_mat,
		ConstMatrixView	ext_mat_av,
		ConstVectorView	abs_vec_av,
		ConstVectorView	sca_vec_av,
		const Numeric &	l_step,
		const Numeric &	rte_planck_value
	)

rte_step_std

Solves monochromatic VRTE for an atmospheric slab with constant conditions.

The function can be used for clearsky and cloudbox calculations.

The function is best explained by considering a homogenous layer. That is, the physical conditions inside the layer are constant. In reality they are not constant, so in practical all coefficients have to be averaged before calling this function. Total extinction and absorption inside the layer are described by ext_mat_av* and abs_vec_av respectively, the blackbdody radiation of the layer is given by rte_planck_value and the propagation path length through the layer is l_step.

There is an additional scattering source term in the VRTE, the scattering integral term. For this function a constant scattering term is assumed. The radiative transfer step is only a part the iterative solution of the scattering problem, for more information consider AUG. In the clearsky case this variable has to be set to 0.

When calling the function, the vector stokes_vec shall contain the Stokes vector for the incoming radiation. The function returns this vector, then containing the outgoing radiation on the other side of the layer.

The function performs the calculations differently depending on the conditions to improve the speed. There are three cases:

Scalar absorption (stokes_dim = 1).
The matrix ext_mat_gas is diagonal (unpolarised absorption).
The total general case.

Parameters

stokes_vec	Input/Output: A Stokes vector.
trans_mat	Input/Output: Transmission matrix of slab.
ext_mat_av	Input: Averaged extinction matrix.
abs_vec_av	Input: Averaged absorption vector.
sca_vec_av	Input: averaged scattering vector.
l_step	Input: The length of the RTE step.
rte_planck_value	Input: Blackbody radiation.

Author: Claudia Emde and Patrick Eriksson,

Date: 2002-11-22

Definition at line 1092 of file rte.cc.

References id_mat(), is_diagonal(), is_singular(), is_size(), lubacksub(), ludcmp(), matrix_exp(), mult(), ConstVectorView::nelem(), and q.

Referenced by cloud_ppath_update1D_planeparallel(), cloud_RT_no_background(), and iyFOS().

◆ surface_calc()

void surface_calc	(	Matrix &	iy,
		const Tensor3 &	I,
		const Matrix &	surface_los,
		const Tensor4 &	surface_rmatrix,
		const Matrix &	surface_emission
	)

surface_calc

Weights together downwelling radiation and surface emission.

iy* must have correct size when function is called.

Parameters

iy	In/Out: Radiation matrix, amtching the WSV with the same name.
I	Input: Downwelling radiation, with dimensions matching: (surface_los, f_grid, stokes_dim)
surface_los	Input: As the WSV with the same name.
surface_rmatrix	Input: As the WSV with the same name.
surface_emission	Input: As the WSV with the same name.

Author: Patrick Eriksson

Date: 2005-04-07

Definition at line 1245 of file rte.cc.

References joker, mult(), ConstTensor3View::ncols(), ConstMatrixView::nrows(), and ConstTensor3View::nrows().

Referenced by get_iy_of_background().

◆ trans_step_std()

void trans_step_std	(	VectorView	stokes_vec,
		MatrixView	trans_mat,
		ConstMatrixView	ext_mat_av,
		const Numeric &	l_step
	)

trans_step_std

Solves monochromatic (vector) Beer-Lambert for one step

The function can be used for clearsky and cloudbox calculations.

(As rte_step_std, but without emission and scattering source term)

When calling the function, the vector stokes_vec shall contain the Stokes vector for the incoming radiation. The function returns this vector, then containing the outgoing radiation on the other side of the layer.

Transmission calculated by ext2trans.

Parameters

stokes_vec	Input/Output: A Stokes vector.
trans_mat	Input/Output: Transmission matrix of slab.
ext_mat	Input: Averaged extinction matrix.
l_step	Input: The length of the RTE step.

Author: Claudia Emde and Patrick Eriksson,

Date: 2010-10-15

Definition at line 1300 of file rte.cc.

References ext2trans(), and mult().

Variable Documentation

◆ BOLTZMAN_CONST

const Numeric BOLTZMAN_CONST

extern

◆ DEG2RAD

const Numeric DEG2RAD

extern

Referenced by get_ppath_rtvars().

◆ PI

const Numeric PI

extern

Referenced by get_ppath_rtvars().

◆ PLANCK_CONST

const Numeric PLANCK_CONST

extern

◆ RAD2DEG

const Numeric RAD2DEG

extern

◆ SPEED_OF_LIGHT

const Numeric SPEED_OF_LIGHT

extern

Referenced by apply_y_unit(), apply_y_unit2(), and get_ppath_rtvars().

Functions

Variables

Detailed Description

Function Documentation

◆ apply_y_unit()

◆ apply_y_unit2()

◆ ext2trans()

◆ get_ppath_atmvars()

◆ get_ppath_cloudrtvars()

◆ get_ppath_pnd()

◆ get_ppath_rtvars()

◆ get_rowindex_for_mblock()

◆ iy_transmission_for_scalar_tau()

◆ iy_transmission_mult()

◆ iy_transmission_mult_scalar_tau()

◆ mirror_los()

◆ rte_step_std()

◆ surface_calc()

◆ trans_step_std()

Variable Documentation

◆ BOLTZMAN_CONST

◆ DEG2RAD

◆ PI

◆ PLANCK_CONST

◆ RAD2DEG

◆ SPEED_OF_LIGHT