ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:2112.001] pycelp: Python package for Coronal Emission Line Polarization

pyCELP (aka "pi-KELP") calculates Coronal Emission Line Polarization. It forward synthesizes the polarized emission of ionized atoms formed in the solar corona and calculates the atomic density matrix elements for a single ion under coronal equilibrium conditions and excited by a prescribed radiation field and thermal collisions. pyCELP solves a set of statistical equilibrium equations in the spherical statistical tensor representation for a multi-level atom for the no-coherence case. This approximation is useful in the case of forbidden line emission by visible and infrared lines, such as Fe XIII 1074.7 nm and Si X 3934 nm.

Code site:
https://github.com/tschad/pycelp
Used in:
https://ui.adsabs.harvard.edu/abs/2021SoPh..296..166S
Bibcode:
2021ascl.soft12001S
Preferred citation method:

https://ui.adsabs.harvard.edu/abs/2020SoPh..295...98S ; please see additional citation information here: https://github.com/tschad/pycelp#citing-pyclep


Views: 1981

ascl:2112.001
Add this shield to your page
Copy the above HTML to add this shield to your code's website.