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A non-equilibrium Radiative Solver for HITRAN-like database species

Project description

.. image:: https://img.shields.io/pypi/v/radis.svg

:target: https://pypi.python.org/pypi/radis

:alt: PyPI



.. image:: https://img.shields.io/travis/radis/radis.svg

:target: https://travis-ci.org/radis/radis

:alt: Continuous Integration



.. image:: https://codecov.io/gh/radis/radis/branch/master/graph/badge.svg

:target: https://codecov.io/gh/radis/radis



.. image:: https://readthedocs.org/projects/climt/badge/

:target: https://radis.readthedocs.io/en/latest/?badge=latest

:alt: Documentation Status



=====

RADIS

=====



A code to simulate infrared spectra of molecules.



RADIS is nonequilibrium emission and absorption line-by-line code, for use

by infrared spectroscopic that want to compare line databases, or experimentalist

that want to fit their experimental line-of-sight spectra.



- Docs: http://radis.readthedocs.io/

- Source: https://github.com/radis

- PyPi: https://pypi.python.org/pypi/radis



.. warning::

Deployment is still in progress, not all modules are available yet. The

documentation will be updated as more modules are included.



Description

-----------



Written as a general purpose radiative solver, the code is built around the HITRAN,

HITEMP and CDSD databases for molecules in their electronic ground state. Energy

levels are read from tabulated databases or calculated from Dunham developments.

Boltzmann, Treanor, and state specific vibrational distributions can be generated.

A modular architecture makes it possible to add new species without modifications

to the core code. Thus far, |CO2|, CO are featured for non-equilibrium calculations,

and all species present in the HITRAN database are featured for equilibrium

calculations. To fit experimental spectra, RADIS includes a line survey tool, an

interface with a look-up database to improve fitting convergence times, and a

multi-slab module with a radiative transfer equation solver to reproduce line-of-sight

experiments. Validation cases against existing spectral codes and experimental

results from various plasma sources are included.



The code will soon be fully available on this repository under

`GNU LESSER GENERAL PUBLIC LICENSE (v3) <./LICENSE>`_





.. |CO2| replace:: CO\ :sub:`2`


Platform: any
Classifier: Development Status :: 4 - Beta
Classifier: Intended Audience :: Science/Research
Classifier: License :: OSI Approved :: GNU Lesser General Public License v3 (LGPLv3)
Classifier: Topic :: Scientific/Engineering
Classifier: Programming Language :: Python
Classifier: Programming Language :: Python :: 2.7
Classifier: Programming Language :: Python :: 3.4
Classifier: Programming Language :: Python :: 3.6
Classifier: Operating System :: OS Independent

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