pyarts.arts
Interface directly to the C++ types via python
Classes
Contains line-by-line absorption information for a number of related absorption lines |
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Single absorption line |
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Describes a set of function calls and variable definitions |
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Internal agenda record - do not use manually |
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Members: |
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Meta type for when methods can take any argument (avoid manual use) |
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A list of |
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List of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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List of |
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A list of |
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A list of |
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A list of |
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A list of |
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List of |
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A list of |
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List of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of retrieval quantitities |
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A list of |
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A list of |
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A list of |
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List of |
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List of |
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A list of species tags |
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A list of |
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A list of |
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A list of sun |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of |
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A list of cross-section records |
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A single block matrix |
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Members: |
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Used to inject custom code into |
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Contains information to compute collision induced absorption for a pair of species |
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The C++ standard clock type |
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Holds complex vector data. |
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A covariance matrix |
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Maps data based on energy levels |
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Type of energy level |
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Data for the error corrected sudden method of line mixing |
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An absorption lookup table |
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A 1 dimensional gridded set of |
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A 2 dimensional gridded set of |
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A 3 dimensional gridded set of |
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A 4 dimensional gridded set of |
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A 5 dimensional gridded set of |
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A 6 dimensional gridded set of |
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A position in a grid |
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Wraps data required to use Hitran line mixing |
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A 64 bit signed integer type |
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A single target of a partial derivative computation |
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Interpolation object |
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Class to compute the line shape |
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Multi-species line shape model |
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A temperature model calculator |
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Derived line shape parameters |
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Single species line shape model |
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A map of data required for computing the error-corrected-sudden relaxation matrix |
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A 2 dimensional array of |
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An antenna object used by |
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Method record for the workspace - do not use manually |
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Method record for |
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IEEE 754 binary64 floating point number |
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Describes a propagation path |
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Contains any data required for a predefined model |
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The propagation matrix data is help by this type |
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Members: |
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An ID for an absorption species state |
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A local state of quantum numbers |
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A single quantum number with a value |
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A list of unique |
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Contains the radiation vector as a function of frequency |
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A range, used to select parts of a matpack type |
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Holds a rational number as two |
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A retrieval quantity |
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Holds meta data about the scattering |
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Holds single scattering data |
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A sparse version of |
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Holds data required for a single species error corrected sudden method application |
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An isotopologue record entry |
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Contains a list of isotopologue ratios for all defined species |
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The tag of a single absorption species |
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An operator that turns a frequency and zenith angle into a spectral radiance profile |
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A stokes vector |
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Basic string type |
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A single sun. |
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A telsem atlas |
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A 3 dimensional array of |
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A 4 dimensional array of |
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A 5 dimensional array of |
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A 6 dimensional array of |
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A 7 dimensional array of |
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Data required by TESSEM to calculate surface emissivity |
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Represents a time stamp |
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Represents a clock |
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Custom class holding any value in token form inside ARTS - do not use manually |
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Contains the transmission matrix as a function of frequency |
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A 1 dimensional array of |
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Controls the screen, agenda, and file verbosity level (i.e. the level of information printed). |
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A wrapper around all workspace groups |
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A workspace variable record |
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A cross-section record. |
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A Zeeman model |
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Options for ZeemanPolarization |
Functions
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Compute the magnetic field according to IGRF |
pyarts.arts.constants
Contain copies of constants of Arts internals
Functions
Convert a string or number to a floating-point number, if possible. |
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Convert a string or number to a floating-point number, if possible. |
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Convert a string or number to a floating-point number, if possible. |
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Convert a string or number to a floating-point number, if possible. |
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Convert a string or number to a floating-point number, if possible. |
pyarts.arts.convert
Contains several unit conversion functions used in Arts
These all should work with any array-like type
Functions
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Converts from Frequency [Hz] to Kayser [cm-1] |
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Converts from Frequency [Hz] to Wavelenth [m] |
Converts from Spectral line intensity [Hz/m2] to CGS spectral line intensity [cm-1/cm-2] |
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Converts from Line shape parameter [Hz/Pa] to CGS line shape parameter [cm-1/atm] |
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Converts from Energy [J] to CGS Energy [cm-1] |
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Converts from Kayser [cm-1] to Frequency [Hz] |
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Converts from CGS Energy [cm-1] to Energy [J] |
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Converts from CGS line shape parameter [cm-1/atm] to Line shape parameter [Hz/Pa] |
Converts from CGS spectral line intensity [cm-1/cm-2] to Spectral line intensity [Hz/m2] |
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Converts from Pressure [Pa] to Torr [Torr] |
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Converts from Torr [Torr] to Pressure [Pa] |
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Converts from Wavelenth [m] to Frequency [Hz] |
pyarts.arts.docserver
Run the ARTS documentation server
Functions
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Run the ARTS documentation server |
pyarts.arts.globals
Classes
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Global workspace data golder - do not use manually |
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Access to static settings data |
Functions
Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a list of the global isotopologues |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get a copy of the global data variable |
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Get maximum number of OpenMP threads |
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Sets the maximum number of OpenMP threads |
pyarts.arts.hitran
Helpers to interface with HITRAN
Functions
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Get the Arts quantum identifier of the HITRAN molecule |
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Get the isotopologue ratio in HITRAN of HITRAN molecule |
pyarts.arts.math
Contains select mathematics from Arts internal functions
Functions
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Computes the Wigner 3J symbol using floating point approximation |
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Computes the Wigner 6J symbol using floating point approximation |
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Initialize a Wigner computation block for |
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Computes the Wigner 3J symbol |
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Computes the Wigner 6J symbol |
pyarts.arts.options
Various named options of Arts
Classes
Options for AbsorptionCutoffType |
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Options for AbsorptionMirroringType |
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Options for AbsorptionNormalizationType |
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Options for AbsorptionPopulationType |
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Options for dobatch_calc_agendaDefaultOptions |
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Options for doit_conv_test_agendaDefaultOptions |
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Options for doit_mono_agendaDefaultOptions |
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Options for doit_rte_agendaDefaultOptions |
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Options for doit_scat_field_agendaDefaultOptions |
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Options for forloop_agendaDefaultOptions |
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Options for g0_agendaDefaultOptions |
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Options for gas_scattering_agendaDefaultOptions |
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Options for inversion_iterate_agendaDefaultOptions |
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Options for iy_cloudbox_agendaDefaultOptions |
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Options for iy_independent_beam_approx_agendaDefaultOptions |
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Options for iy_loop_freqs_agendaDefaultOptions |
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Options for iy_main_agendaDefaultOptions |
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Options for iy_radar_agendaDefaultOptions |
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Options for iy_space_agendaDefaultOptions |
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Options for iy_surface_agendaDefaultOptions |
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Options for jacobian_agendaDefaultOptions |
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Options for JacobianAtm |
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Options for JacobianLine |
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Options for JacobianSensor |
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Options for JacobianSpecial |
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Options for JacobianType |
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Options for LineShapeTemperatureModel |
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Options for LineShapeType |
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Options for LineShapeVariable |
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Options for main_agendaDefaultOptions |
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Options for met_profile_calc_agendaDefaultOptions |
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Options for pha_mat_spt_agendaDefaultOptions |
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Options for planetDefaultOptions |
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Options for ppath_agendaDefaultOptions |
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Options for ppath_step_agendaDefaultOptions |
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Options for PredefinedModelDataKey |
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Options for propmat_clearsky_agendaDefaultOptions |
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Options for QuantumNumberType |
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Options for refr_index_air_agendaDefaultOptions |
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Options for sensor_response_agendaDefaultOptions |
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Options for SpeciesTagType |
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Options for spt_calc_agendaDefaultOptions |
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Options for surface_rtprop_agendaDefaultOptions |
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Options for test_agendaDefaultOptions |
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Options for water_p_eq_agendaDefaultOptions |
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Options for ybatch_calc_agendaDefaultOptions |
pyarts.arts.physics
Contains simple physics functions in arts
Functions
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Overloaded function. |
pyarts.arts.predef
Contains predefined absorption models
Classes
Water data representation for the MT CKD 4.0 model |
Functions
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Computes self absorption using MT CKD version 2.52 |
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Computes foreign absorption using MT CKD version 3.20 |
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Computes foreign absorption using MT CKD version 3.50 |
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Computes foreign absorption using MT CKD Hitran version |
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Computes foreign water absorption using Rosenkranz standard |
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Computes water absorption using MPM89 |
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Computes water absorption using PWR2021 |
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Computes water absorption using PWR2022 |
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Computes water absorption using PWR98 |
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Computes self water absorption using Rosenkranz standard |
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Computes N2 fun absorption using MT CKD version 2.52 |
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Computes nitrogen absorption using MPM93 |
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Computes nitrogen absorption using PWR2021 |
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Computes N2 rot absorption using MT CKD version 2.52 |
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Computes nitrogen absorption using Rosenkranz standard |
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Computes self absorption using MT CKD version 3.50 |
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Computes oxygen absorption using MPM89 |
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Computes oxygen absorption using PWR2021 |
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Computes oxygen absorption using PWR2022 |
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Computes oxygen absorption using PWR98 |
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Computes oxygen absorption using Rosenkranz standard |
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Computes oxygen absorption using TRE05 |
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Computes self absorption using MT CKD version 3.50 |
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Computes self absorption using MT CKD version 3.50 |
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Computes self absorption using MT CKD version 2.52 |
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Computes self absorption using MT CKD version 3.20 |
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Computes self absorption using MT CKD version 3.50 |
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Computes self absorption using MT CKD Hitran version |
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Computes water absorption using PWR98 |