Workspace
- class pyarts3.workspace.Workspace(*args, **kwargs)[source]
The workspace object containing all ARTS variables and methods
Overview
Method
Ignore a workspace variable.
Method
Inversion by the so called optimal estimation method (OEM).
Method
Reads split catalog data from a folder structure similar to
arts-cat-data
Method
Reads a workspace variable from an XML file.
Method
As
ReadXML()
, but reads indexed file names.Method
Sets an atmospheric target.
Method
Set a measurement error to polynomial fit.
Method
Set magnetic field derivative.
Method
Set magnetic field derivative for overlapping fields.
Method
Set wind field derivative for overlapping fields.
Method
Set pressure derivative.
Method
Set sensor frequency derivative to use polynomial fitting offset
Method
Set isotopologue ratio derivative
Method
Set volume mixing ratio derivative.
Method
Sets a subsurface target
Method
Sets a surface target
Method
Set temperature derivative.
Method
Set wind field derivative.
Method
Finalize the retrieval setup.
Method
Initialize the retrieval setup.
Method
Integrate Disort spectral radiance.
Method
As
Ignore()
but for agenda output.Method
Update state of the model in preparation for a forward model run
Method
Initialize the Wigner tables
Method
Unloads the Wigner tables from static data (see
WignerInit()
)Method
Writes all the builtin partition functions to file.
Method
Writes a workspace variable to an XML file.
Method
As
WriteXML()
, but creates indexed file names.Method
Sets
absorption_bands
to the state of the model.Method
Keeps first band of ID
Method
Adapts select band to use ordered Line mixing coefficients.
Method
Reads HITRAN data from a file.
Method
Same as
absorption_bandsReadSpeciesSplitCatalog()
but for reading the old ARTSCAT format.Method
Reads all species in
absorption_species
from a basenameMethod
Saves all bands in
absorption_bands
to a directoryMethod
Remove first band of with a matching ID
Method
Saves all bands fin
absorption_bands
to a directoryMethod
Remove all bands whose lines all strictly falls outside a frequency range
Method
Remove all lines that strictly falls outside a frequency range
Method
Set all bands to use non-LTE calculations.
Method
Set the Zeeman splitting for lines within the frequency range
Method
Takes CIARecord as input and appends the results in the appropriate place.
Method
Read data from a CIA data file for all CIA molecules defined
Method
Read data from a CIA XML file and check that all CIA tags defined
Method
Reads a species split CIA dataset.
Method
Get
absorption_lookup_table
from available data.Method
Compute the lookup table for all species in
absorption_bands
.Method
Initialize an empty lookup table.
Method
Precompute the lookup table for a single species, adding it to the map.
Method
Compute the lookup table for all species in
absorption_bands
.Method
Set up a simple wide lookup table for all species in
absorption_bands
.Method
Sets the data for MT CKD 4.0 Water model
Method
Initialize the predefined model data
Method
Reads
absorption_predefined_model_data
catalog but only forabsorption_species
Method
Sets
absorption_species
[i][0] to all species in ARTSMethod
Set
absorption_species
to the named species.Method
Reads HITRAN Crosssection coefficients
Method
Set the magnetic field to use the magnitude field functional.
Method
Set the wind field to use the magnitude field functional.
Method
Append data to the atmospheric field based all absorption data
Method
Append base data to the atmospheric field
Method
Append species data to the atmospheric field based on collision-induced data data
Method
Append isotopologue data to the atmospheric field based on line data
Method
Append NLTE data to the atmospheric field based on line data
Method
Append species data to the atmospheric field based on line data
Method
Append species data to the atmospheric field based on lookup data
Method
Append species data to the atmospheric field based on predefined model data
Method
Append species data to the atmospheric field based on species data
Method
Append species data to the atmospheric field based on cross-section data
Method
Fits non-LTE atmospheric field values
Method
Sets
atmospheric_field
to the state of the model.Method
Sets the atmospheric field to be the 1D atmospheric profile.
Method
Add the hydrostatic pressure to the atmospheric field
Method
Use IGRF to compute the magnetic field at each point.
Method
Initialize the atmospheric field with some altitude and isotopologue ratios
Method
Initialize the non-LTE atmospheric field from the LTE temperature field.
Method
Read atmospheric data files from a directory
Method
Regrid the input atmospheric field parameter to a new grid.
Method
Regrid all parameters of the input atmospheric field to a new grid
Method
For forward calculations, this should be similar to
atmospheric_fieldIGRF()
.Method
Initialize an atmospheric point with some isotopologue ratios
Method
Extends the atmospheric profile in pressure.
Method
Extract an atmospheric profile from the atmospheric field.
Method
Fits non-LTE distributions to the level data.
Method
Extract an atmospheric profile and its grids.
Method
Space radiation into Disort is isotropic cosmic background radiation.
Method
Perform Disort calculations for spectral flux.
Method
Same as
disort_settingsLayerThermalEmissionLinearInTau()
but considers non-LTEMethod
Use a source function that changes linearly in optical thickness.
Method
Sets the legendre coefficients from the path-variable.
Method
Turns off fractional scattering in Disort calculations.
Method
Turns off source radiation in Disort calculations.
Method
Turns off Legendre coefficients in Disort calculations.
Method
Turns off single albedo scattering in Disort calculations.
Method
Turns off boundary condition from space for Disort calculations.
Method
Turns off solar radiation in Disort calculations.
Method
Turns boundary condition from surface for Disort calculations.
Method
Turns off BDRF in Disort calculations.
Method
Get optical thickness from path.
Method
Uses Set the FOV to the sun input for Disort calculations.
Method
Sets the single scattering albedo from the path-variable.
Method
Surface radiation into Disort is isotropic from surface temperature.
Method
Sets the surface to Lambertian.
Method
Executes
disort_settings_agenda
, see it for more detailsMethod
Executes an operator emulating
disort_settings_agenda
, see it, and alsodisort_settings_agendaOperator
, for more detailsMethod
Set
disort_settings_agenda
to exclusively use provided external operator. Seedisort_settings_agendaOperator
for more details.Method
Setup for Disort standard calculations.
Method
Perform Disort calculations for spectral flux.
Method
Use Disort for clearsky calculations of spectral flux field
Method
Extract a 1D path through the atmospheric field and calculate spectral flux using Disort
Method
Perform Disort calculations for spectral radiance.
Method
Perform CDisort calculations for spectral radiance.
Method
Use the disort settings agenda to calculate spectral radiance
Method
Use the disort settings agenda to calculate spectral radiance
Method
Extract a 1D path through the atmospheric field and calculate spectral radiance using Disort
Method
Extract a 1D path through the atmospheric field and calculate spectral radiance using Disort
Method
Sets the O2-66 microwave band data for ECS.
Method
Sets ECS data for air from other data if available.
Method
Sets the CO2-626, CO2-628, and CO2-636 band data for ECS.
Method
Sets the CO2-626, CO2-628, and CO2-636 band data for ECS.
Method
Resets/initializes the ECS data.
Method
Computes the spectral flux
Method
Frequency grid useful for
atmospheric_profileFitNonLTE()
.Method
Applies wind shift to the
frequency_grid
for the local frequency grid.Method
Gets the value of the variable with the given name.
Method
Sets a gravity operator from the gravitational constant and the mass of the planet
Method
Checks if the workspace contains the variable.
Method
Overloaded function.
Method
Executes
inversion_iterate_agenda
, see it for more detailsMethod
Executes an operator emulating
inversion_iterate_agenda
, see it, and alsoinversion_iterate_agendaOperator
, for more detailsMethod
Set
inversion_iterate_agenda
to a specific predefined optionMethod
Set
inversion_iterate_agenda
to exclusively use provided external operator. Seeinversion_iterate_agendaOperator
for more details.Method
Sets an atmospheric target.
Method
Set a measurement error to polynomial fit.
Method
Set magnetic field derivative.
Method
Set magnetic field derivative for overlapping fields.
Method
Set wind field derivative for overlapping fields.
Method
Set pressure derivative.
Method
Set sensor frequency derivative to use polynomial fitting offset
Method
Set isotopologue ratio derivative
Method
Set volume mixing ratio derivative.
Method
Sets a subsurface target
Method
Sets a surface target
Method
Set temperature derivative.
Method
Set wind field derivative.
Method
Clears
jacobian_targets
ifdo_jacobian
evaluates false.Method
Finalize
jacobian_targets
.Method
Initialize or reset the
jacobian_targets
.Method
Turns off
jacobian_targets
Method
Toggles logarithmic/relative or absolute retrievals.
Method
Toggles logarithmic/relative or absolute retrievals.
Method
Toggles logarithmic/relative or absolute retrievals.
Method
Toggles logarithmic or absolute retrievals.
Method
Toggles logarithmic or absolute retrievals.
Method
Toggles logarithmic or absolute retrievals.
Method
Toggles relative or absolute retrievals.
Method
Toggles relative humidity or absolute retrievals.
Method
Toggles relative or absolute retrievals.
Method
Toggles relative or absolute retrievals.
Method
Sets
legendre_degree
todisort_settings
legendre_polynomial_dimension
Method
Calculate the averaging kernel matrix.
Method
Executes
measurement_inversion_agenda
, see it for more detailsMethod
Executes an operator emulating
measurement_inversion_agenda
, see it, and alsomeasurement_inversion_agendaOperator
, for more detailsMethod
Set
measurement_inversion_agenda
to a specific predefined optionMethod
Set
measurement_inversion_agenda
to exclusively use provided external operator. Seemeasurement_inversion_agendaOperator
for more details.Method
Applies transformations to the atmospheric state Jacobian
Method
Applies transformations to the line-by-line state Jacobian
Method
Applies transformations to the measurement sensor state Jacobian
Method
Applies transformations to the subsurface state Jacobian
Method
Applies transformations to the surface state Jacobian
Method
Apply all transformations to the Jacobian related to states in
model_state_vectorFromData()
Method
Adds sensor elements from a raw perturbation of the sensor
Method
Adds a sensor with a dirac channel opening around the frequency grid.
Method
Adds a sensor with a Gaussian channel opening around the frequency grid.
Method
Adds a sensor with a Gaussian channel opening around the frequency grid.
Method
Update
measurement_sensor
frommodel_state_vector
.Method
Initialize
measurement_sensor
to empty.Method
Make the
measurement_sensor
excluive.Method
Creates a single simple dirac-opening sensor
Method
Creates a single simple Gaussian-opening sensor
Method
Creates a single simple Gaussian-opening sensor
Method
Add the measurement error to the measurement. Conditionally, also to the Jacobian.
Method
Sets measurement vector by looping over all sensor elements
Method
Sets measurement vector by looping over all sensor elements
Method
Set the error and its Jacobian from the state of the model.
Method
Sets a constant measurement vector error covariance matrix.
Method
measurement_vector_error_covariance_matrix_observation_systemCalc()
Calculates the covariance matrix describing the error due to uncertainties in the observation system.
Method
Sets the fitted measurement vector to the current measurement vector.
Method
Set a species model state covariance matrix element.
Method
Initialises the model state covariance matrix to the identity matrix.
Method
Calculates the covariance matrix describing the error due to smoothing.
Method
Sets
model_state_vector
’s atmospheric part.Method
Sets
model_state_vector
’s absorption line part.Method
Get
model_state_vector
from available dataMethod
Sets
model_state_vector
’s sensor part.Method
Sets
model_state_vector
’s subsurface part.Method
Sets
model_state_vector
’s surface part.Method
Sets
model_state_vector
to the sizejacobian_targets
demand.Method
Get
model_state_vector_apriori
from available dataMethod
Sets the a priori state of the model state vector to the current state.
Method
Integrate the spectral flux profile to get the line non-LTE flux
Method
Add absorption coefficients for HITRAN collision induced absorption (CIA).
Method
Calculates absorption matrix describing Faraday rotation.
Method
Line-by-line calculations.
Method
Lookup calculations.
Method
Adds all of the predefined models in
absorption_species
to the propagation_matrixMethod
Calculate absorption cross sections per tag group for HITRAN xsec species.
Method
Initialize
propagation_matrix
,propagation_matrix_source_vector_nonlte
, and their derivatives to zeroes.Method
Sets the
propagation_matrix_agenda
automatically from absorption data and species tag meta information.Method
Executes
propagation_matrix_agenda
, see it for more detailsMethod
Executes an operator emulating
propagation_matrix_agenda
, see it, and alsopropagation_matrix_agendaOperator
, for more detailsMethod
Set
propagation_matrix_agenda
to a specific predefined optionMethod
Set
propagation_matrix_agenda
to exclusively use provided external operator. Seepropagation_matrix_agendaOperator
for more details.Method
Fix for the wind field derivative.
Method
propagation_matrix_scatteringAddSpectralScatteringSpeciesTRO()
Adds
scattering_species
results for totally random oriented spectral calculations toMethod
Add simple air to
propagation_matrix_scattering
.Method
Initialize
propagation_matrix_scattering
to zeroes.Method
Initialize
propagation_matrix_scattering
and co to zeroes.Method
Executes
propagation_matrix_scattering_agenda
, see it for more detailsMethod
Executes an operator emulating
propagation_matrix_scattering_agenda
, see it, and alsopropagation_matrix_scattering_agendaOperator
, for more detailsMethod
Set
propagation_matrix_scattering_agenda
to a specific predefined optionMethod
Set
propagation_matrix_scattering_agenda
to exclusively use provided external operator. Seepropagation_matrix_scattering_agendaOperator
for more details.Method
Executes
propagation_matrix_scattering_spectral_agenda
, see it for more detailsMethod
propagation_matrix_scattering_spectral_agendaExecuteOperator()
Executes an operator emulating
propagation_matrix_scattering_spectral_agenda
, see it, and alsopropagation_matrix_scattering_spectral_agendaOperator
, for more detailsMethod
Set
propagation_matrix_scattering_spectral_agenda
to a specific predefined optionMethod
Set
propagation_matrix_scattering_spectral_agenda
to exclusively use provided external operator. Seepropagation_matrix_scattering_spectral_agendaOperator
for more details.Method
Fill the path with with points that crosses the grid of the atmspheric field.
Method
Add the limb point to the ray path
Method
Fill the path with geometric step points.
Method
Fill the path with geometric step points.
Method
Fix azimuth angle errors that can occur for 180 and 0 degrees zenith.
Method
Get a geometric radiation path
Method
Wraps
ray_pathGeometric()
for straight downlooking paths from the top-of-the-atmosphere altitudeMethod
Wraps
ray_pathGeometric()
for straight uplooking paths from the surface altitude at the positionMethod
Initialize the ray path with a single point.
Method
Remove points that are too close to each other.
Method
Remove non-atmospheric points to the ray path
Method
Remove all non-geometric grid crossings from the ray path.
Method
Add the geometric extremes to the ray path.
Method
Gets the atmospheric points along the path.
Method
Set
ray_path_atmospheric_point = atmospheric_profile
.Method
Adds observers that covers all zenith angles for each altitude point.
Method
Create a ray path field from a set of observers.
Method
Gets the frequency grids along the path.
Method
Executes
ray_path_observer_agenda
, see it for more detailsMethod
Executes an operator emulating
ray_path_observer_agenda
, see it, and alsoray_path_observer_agendaOperator
, for more detailsMethod
Set
ray_path_observer_agenda
from programmable geometric settings.Method
Set
ray_path_observer_agenda
to exclusively use provided external operator. Seeray_path_observer_agendaOperator
for more details.Method
Get a list of observer positions and line of sights to represent observing all angles of a profile.
Method
Add \(n\) observers per altitude point.
Method
Sets
ray_path_point
to the expected background point ofray_path
Method
Sets
ray_path_point
to the expected foreground point ofray_path
Method
Sets
ray_path_point
to the highest altitude point ofray_path
.Method
Sets
ray_path_point
to the lowest altitude point ofray_path
.Method
Adds the scattering part of the propagation matrix to the rest along the path.
Method
Gets the propagation matrix and non-LTE source term along the path.
Method
Gets the propagation matrix for scattering along the path.
Method
Compute
ray_path_propagation_matrix_scattering
and co for a path.Method
As
ray_path_propagation_matrixFromPath()
but the output is split between the species in theMethod
ray_path_spectral_radiance_scatteringSunsFirstOrderRayleigh()
Method
Adds the scattering part of the propagation matrix to the rest along the path.
Method
Gets the source term along the path.
Method
Wraps
sun_pathFromObserverAgenda()
for all paths to all suns.Method
Gets the transmission matrix in layers along the path.
Method
Sets
ray_path_transmission_matrix_cumulative
by forward iteration ofray_path_transmission_matrix
Method
Sets a path of Zeeman effect magnetic field properties.
Method
Read variable from file
Method
Saves variable to file
Method
Initialize scattering species.
Method
Selects all main absorbers from the absorption data.
Method
Set the variable to the new value.
Method
Get the sorting of the bands by first quantum identifier then some
criteria
Method
Computes the spectral flux from a field of paths.
Method
Computes the spectral flux. The input field must be a profile.
Method
Computes the spectral flux profile using pseudo-2D geometry
Method
Helper to call
spectral_radianceApplyUnit()
when you do not havespectral_radiance_jacobian
.Method
Applies a unit to
spectral_radiance
, returning a new fieldMethod
Helper method for calling
spectral_radianceApplyUnit()
.Method
Computes clearsky transmission of spectral radiances
Method
Computes clearsky emission of spectral radiances
Method
Computes clearsky emission of spectral radiances with solar Rayleigh scattering
Method
Computes clearsky transmission of spectral radiances
Method
Gets the spectral radiance from the path transmission.
Method
Sets default
spectral_radiance
andspectral_radiance_jacobian
for transmission.Method
Set surface spectral radiance from Planck function of the surface temperature and the reflectance of incoming radiation
Method
Integrate Disort spectral radiance.
Method
Gets the spectral radiance from the path.
Method
Get the spectral radiance of a sun or of the cosmic background if the sun is not hit.
Method
Get the spectral radiance of a sun or of the cosmic background if no sun is hit.
Method
Set surface spectral radiance from Planck function of the surface temperature
Method
Background spectral radiance is from a uniform cosmic background temperature.
Method
Computes the background radiation.
Method
Computes the spectral radiance field using
ray_path_observer_agenda
.Method
Computes the spectral radiance field assuming planar geometric paths
Method
Computes the spectral radiance field assuming a profile and a pseudo-2D path.
Method
Adds the propagation variables to
spectral_radiance_jacobian
Method
Adds sensor properties to the
spectral_radiance_jacobian
.Method
Set the cosmic background radiation derivative to empty.
Method
Sets
spectral_radiance_jacobian
from the background valuesMethod
Executes
spectral_radiance_observer_agenda
, see it for more detailsMethod
Executes an operator emulating
spectral_radiance_observer_agenda
, see it, and alsospectral_radiance_observer_agendaOperator
, for more detailsMethod
Set
spectral_radiance_observer_agenda
to a specific predefined optionMethod
Set
spectral_radiance_observer_agenda
to exclusively use provided external operator. Seespectral_radiance_observer_agendaOperator
for more details.Method
Set up a 1D spectral radiance operator
Method
Executes
spectral_radiance_space_agenda
, see it for more detailsMethod
Executes an operator emulating
spectral_radiance_space_agenda
, see it, and alsospectral_radiance_space_agendaOperator
, for more detailsMethod
Set
spectral_radiance_space_agenda
to a specific predefined optionMethod
Set
spectral_radiance_space_agenda
to exclusively use provided external operator. Seespectral_radiance_space_agendaOperator
for more details.Method
Executes
spectral_radiance_surface_agenda
, see it for more detailsMethod
Executes an operator emulating
spectral_radiance_surface_agenda
, see it, and alsospectral_radiance_surface_agendaOperator
, for more detailsMethod
Set
spectral_radiance_surface_agenda
to a specific predefined optionMethod
Set
spectral_radiance_surface_agenda
to exclusively use provided external operator. Seespectral_radiance_surface_agendaOperator
for more details.Method
Creates a
SpectralRadianceTransformOperator
from aSpectralRadianceUnitType
.Method
Sets
subsurface_field
to the state of the model.Method
Set
sun
to blackbody.Method
Extracts a sun spectrum from a field of such data.
Method
Find a path that hits the sun if possible
Method
Method
Earth reference ellipsoids.
Method
Europa reference ellipsoids.
Method
Sets
surface_field
to the state of the model.Method
Ganymede reference ellipsoids.
Method
Manual setting of the reference ellipsoid.
Method
Io reference ellipsoids.
Method
Jupiter reference ellipsoids.
Method
Mars reference ellipsoids.
Method
Moon reference ellipsoids.
Method
Initialize the surface field with the ellipsoid of a planet.
Method
Venus reference ellipsoids.
Method
Swap the workspace for andother.
Method
Sets
transmission_matrix_background
to back ofray_path_transmission_matrix_cumulative
.Method
Sets
transmission_matrix_background
to front ofray_path_transmission_matrix_cumulative
.Method
Sets an operator to compute the water equivalent pressure according to Murphy and Koop, 2005.
Method
A custom zenith grid for
spectral_radiance_fieldProfilePseudo2D()
Attribute
Bands of absorption lines for line-by-line (LBL) calculations.
Attribute
HITRAN Collision-Induced Absorption (CIA) Data.
Attribute
Absorption lookup table for scalar gas absorption coefficients.
Attribute
This contains predefined model data.
Attribute
Tag groups for gas absorption.
Attribute
The absorption vector of totally random orientation particles at a single point along a path using spectral representation
Attribute
Fitting model coefficients for cross section species.
Attribute
A single altitude in the atmosphere.
Attribute
An ascending list of
altitude
. Often related to a field or a profile.Attribute
An atmospheric field in ARTS.
Attribute
An atmospheric point in ARTS.
Attribute
An atmospheric profile in ARTS.
Attribute
A helper map for setting the covariance matrix.
Attribute
The number of Fourier modes for Disort.
Attribute
The number of input Legendre polynimials for Disort.
Attribute
The quadrature angles for Disort with accompying weights.
Attribute
The quadrature size for Disort.
Attribute
Contains the full settings of spectral Disort calculations.
Attribute
An agenda for setting up Disort.
Attribute
The spectral flux field from Disort.
Attribute
The spectral radiance field from Disort.
Attribute
A boolean calculations related to the
measurement_jacobian
should be ignored.Attribute
Error corrected sudden data
Attribute
A single frequency grid.
Attribute
The frequency grid wind shift Jacobian.
Attribute
The gravity operator.
Attribute
Work in progress …
Attribute
A counter for the inversion iterate agenda.
Attribute
A list of targets for the Jacobian Matrix calculations.
Attribute
A single latitude.
Attribute
An ascending list of
latitude
. Often related to a field or a profile.Attribute
The degree of a Legendre polynimial.
Attribute
A single longitude.
Attribute
An ascending list of
longitude
. Often related to a field or a profile.Attribute
Averaging kernel matrix.
Attribute
Contribution function (or gain) matrix.
Attribute
This is a helper
Agenda
intended for use withininversion_iterate_agenda
.Attribute
The first order partial derivatives of the
measurement_vector
.Attribute
The partial derivatives of the
measurement_vector_error
.Attribute
A list of sensor elements.
Attribute
The measurment vector for, e.g., a sensor.
Attribute
The model measurment vector error for, e.g., a sensor.
Attribute
Covariance matrix for observation uncertainties.
Attribute
As
measurement_vector
, but fitted to the model.Attribute
Covariance matrix of a priori distribution.
Attribute
A state vector of the model.
Attribute
An apriori state vector of the model.
Attribute
A per-line flux profile.
Attribute
The spectral phase matrix of totally random orientation particles at a single point along a path using spectral representation
Attribute
This contains the fully polarized propagation matrix for the current path point.
Attribute
Compute the propagation matrix, the non-LTE source vector, and their derivatives.
Attribute
Partial derivative of the
propagation_matrix
with regards tojacobian_targets
.Attribute
The propgation matrix of totally random orientation particles at a single point along a path using spectral representation
Attribute
Compute the part of the propagation matrix that relates to scattering.
Attribute
Get the scattering propagation matrix, the scattering absorption vector, and the scattering spectral phase matrix.
Attribute
The part of the source vector that is due to non-LTE.
Attribute
Partial derivative of the
propagation_matrix_source_vector_nonlte
with regards tojacobian_targets
.Attribute
A list path points making up a propagation path.
Attribute
The absorption vector of totally random orientation particles along the propagation path using spectral representation
Attribute
Atmospheric points along the propagation path.
Attribute
A list of
ray_path
intended to build up a field of observations.Attribute
All
frequency_grid
along the propagation path.Attribute
A list of
frequency_grid_wind_shift_jacobian
for a ray path.Attribute
Get the propagation path as it is obeserved.
Attribute
A list path points making up the observers of a propagation path.
Attribute
The spectral phase matrix of totally random orientation particles along the propagation path using spectral representation
Attribute
A single path point.
Attribute
Propagation matrices along the propagation path
Attribute
Propagation derivative matrices along the propagation path
Attribute
Propagation matrices along the propagation path for scattering
Attribute
Additional non-LTE along the propagation path
Attribute
Additional non-LTE derivative along the propagation path
Attribute
Spectral radiance derivative along the propagation path
Attribute
Spectral radiance scattered into the propagation path
Attribute
Source vectors along the propagation path
Attribute
Source derivative vectors along the propagation path
Attribute
A list of paths to the suns from the ray path.
Attribute
Transmission matrices along the propagation path.
Attribute
Cumulative transmission matrices along the propagation path
Attribute
Transmission derivative matrices along the propagation path.
Attribute
The scattering species
Attribute
Species selection.
Attribute
Species selection.
Attribute
An altitude profile of spectral flux.
Attribute
A spectral radiance vector.
Attribute
Spectral radiance from the background
Attribute
Spectral radiance derivative from the background
Attribute
The spectral radiance field.
Attribute
Jacobian of
spectral_radiance
with respect tojacobian_targets
.Attribute
Spectral radiance as seen from the input position and environment
Attribute
The line-of-sight of the observer of spectral radiance.
Attribute
The position of an observer of spectral radiance.
Attribute
The spectral radiance operator.
Attribute
Spectral radiance as seen of space.
Attribute
Spectral radiance as seen of the surface.
Attribute
The spectral radiance transform operator
Attribute
The sub0surface field describes the sub-surface properties.
Attribute
A sun.
Attribute
A path to a sun if it is visible.
Attribute
A list of
Sun
.Attribute
The surface field describes the surface properties.
Attribute
Transmittance from the background
Attribute
The water equivalent pressure operator.
Attribute
A single zenith angle grid.
Static Data
pyarts3.workspace.Workspace.fromxml
<function Workspace.fromxml at 0x7f80ce6fb560> (
function
)Operator
Return self==value.
Operator
__format__(self, arg: str, /) -> str
Operator
Return self>=value.
Operator
Operator
Return self>value.
Operator
Return hash(self).
Operator
__init__(self, with_defaults: bool = True) -> None
Operator
Allows iter(self)
Operator
Return self<=value.
Operator
Return self<value.
Operator
Return self!=value.
Operator
__repr__(self) -> str
Operator
Operator
__str__(self) -> str
Constructors