Copyright 2017 Monika Moscibrodzka and Charles F. Gammie

ipole  version 2.0  (released April, 2020)

The files in this directory are part of ipole.  

ipole is a program that solves the equations of polarized radiative transfer
in covariant form, using ray tracing.   It produces images in Stokes I,Q,U,V
at the location of a "camera."   

This version is configured to use data from a harm3d run, which use modified
Kerr-Schild coordinates, and assumes synchrotron emission and absorption
along with faraday rotation.

You are morally obligated to cite the following papera in any
scientific literature that results from use of any part of ipole:

[1] Moscibrodzka, Monika, and Gammie, Charles F., Monthly Notices of 
    the Royal Astronomical Society, Volume 475, Issue 1, p.43-54
	https://ui.adsabs.harvard.edu/abs/2018MNRAS.475...43M/abstract

[2] Noble, Scott C.; Leung, Po Kin; Gammie, Charles F.; Book, Laura G. 
    Classical and Quantum Gravity, Volume 24, Issue 12, pp. S259-S274 (2007)
    http://adsabs.harvard.edu/abs/2007CQGra..24S.259N

Further, we strongly encourage you to obtain the latest version of 
ipole directly from github,
https://github.com/moscibrodzka/ipole

ipole is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.