{ "info": { "author": "Michael Hirsch, Ph.D.", "author_email": "", "bugtrack_url": null, "classifiers": [ "Development Status :: 5 - Production/Stable", "Environment :: Console", "Intended Audience :: Science/Research", "Operating System :: OS Independent", "Programming Language :: Python :: 3.6", "Programming Language :: Python :: 3.7", "Topic :: Scientific/Engineering :: Atmospheric Science" ], "description": "[![image](https://zenodo.org/badge/36744963.svg)](https://zenodo.org/badge/latestdoi/36744963)\n[![image](https://travis-ci.org/scivision/gridaurora.svg?branch=master)](https://travis-ci.org/scivision/gridaurora)\n[![Coverage Status](https://coveralls.io/repos/github/scivision/gridaurora/badge.svg?branch=master)](https://coveralls.io/github/scivision/gridaurora?branch=master)\n[![image](https://ci.appveyor.com/api/projects/status/2jjhaq3rqjrw77vg?svg=true)](https://ci.appveyor.com/project/scivision/gridaurora)\n[![pypi versions](https://img.shields.io/pypi/pyversions/gridaurora.svg)](https://pypi.python.org/pypi/gridaurora)\n[![pypi format](https://img.shields.io/pypi/format/gridaurora.svg)](https://pypi.python.org/pypi/gridaurora)\n[![PyPi Download stats](http://pepy.tech/badge/gridaurora)](http://pepy.tech/project/gridaurora)\n[![Xarray badge](https://img.shields.io/badge/powered%20by-xarray-orange.svg?style=flat)](http://xarray.pydata.org/en/stable/why-xarray.html)\n\n# Grid for Auroral models\n\nDiscretizations of space (grids) and time conversions useful for aeronomy and auroral modeling.\n\n## Install\n\n python -m pip install -e .\n\nNote: you will need a Fortran compiler on your system for `f2py` modules.\nIt works on Linux, Mac, [Windows](https://scivision.co/f2py-running-fortran-code-in-python-on-windows/), etc.\n\n## Eigenprofiles\n\nCurrently GLOW and Rees-Sergienko-Ivanov are available (Transcar in future). \nYou can install these models with\n\n```sh\npip install -e .[models]\n```\n\nOnce installed, select model by:\n\n* `-M rees` Rees-Sergienko-Ivanov\n* `-M glow` Stan Solomon's GLOW model\n\n\n### Command Line Options\n\n-t time, format yyyy-mm-ddTHH:MM:SSZ where Z sets UTC time zone -c lat,\nlon WGS84 geodetic degrees -o output, hDF5 ends in .h5 -M model select\n(see table above) -z min,max altitude to plot [km]\n\n### Example Command\n\n python MakeIonoEigenprofile.py -t 2013-01-31T09:00:00Z -c 65 -148 -o out.h5 -M rees\n\nAuroral Data Files\n------------------\n\nThe functions in `gridaurora/calcemissions.py`, based on work by\nZettergren, computes per-wavelength volume emission rate along a flux\ntube as a function of altitude along the tube. Starting with quantities\nsuch as neutral densities computed by MSIS, differential number flux as\na function of energy and altitude along the tube (this is what TRANSCAR\ncomputes), excitation cross sections as a function of energy,\nFranck-Condon factors and Einstein coefficients, the *prompt* volume\nemission rate may be computed.\n\n### precompute/vjeinfc.h5\n\nThis file is compiled from tables in Vallance Jones *Aurora* 1974 and other sources\nby Matthew Zettergren, and corrected and put into HDF5 format by Michael Hirsch. \nThe information within concerns:\n\n* N2+1NG: N~2~^+^ first negative group\n* N2_1PG: N~2~ first positive group\n* N2_2PG: N~2~ second positive group\n* N2+Meinel: N~2~^+^ Meinel band\n* atomic: atomic oxygen\n* metastable: metastable O and O^+^\n\n#### Einstein coefficient matrix A\n\narranged A(\ud835\udf08',\ud835\udf08'') where:\n\n* \ud835\udf08' upper state vibrational levels, excited from ground state \ud835\udf08''' by particle impact\n* \ud835\udf08'' lower state vibrational levels, decayed into from the upper state\n\nas discussed in Appendix C of Zettergren PhD thesis, Eqn. (C.2), photon\nvolume emission rate follows the relation P~\ud835\udf08',\ud835\udf08''~ = A(\ud835\udf08',\ud835\udf08'')\nn~\ud835\udf08'~\n\n#### lamdba\n\nwavelength in nanometers corresponding to the Einstein coefficient\nmatrix `A` except `atomic` that uses the reaction rates directly.\n\n#### Franck-Condon factor fc\n\nas described in Zettergren thesis Appendix C, specifically for Eqn\n(C.6-C.8), the Franck-Condon factors modify the total upper state\nexcitation cross section multiplicitively.\n\n## Function Description\n\nfunction | description\n----------|----------------------------------------------------------------------------------------------------------------\nztanh.py | continuously varying grid using hyperbolic tangent. 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