This rep. contains the codes required to make a correlated-k distribution spectra which frees one from the hassle of tiresome and computationally intensive line-by-line computations for computing full/1D reflected flux. Adapted from the original version by Dr. D.M. Stam. Paper: "A fast method for simulating observations of polarized light emerging from the atmosphere applied to the oxygen-A band (2000)"
Dependencies:
- PyMieDAP: https://gitlab.com/loic.cg.rossi/pymiedap
- HAPI: https://hitran.org/hapi/
Parts of this code have been used to produce this work which is under review/in-prep: https://www.essoar.org/doi/abs/10.1002/essoar.10501491.1