Building Opacity Tables
From Planets
Revision as of 15:07, 31 March 2023 by Martin.turbet (talk | contribs) (→Adding continuum opacities)
This page describes the main steps required to build new opacity tables.
Calculation of high-resolution spectra
describe the tools we used :
- k-spectrum
- home-made scripts
Several important notes:
- The units of correlated-k tables is cm^2/molec.
- The format of correlated-k tables is (n_temperature, n_pressure, n_vmr, n_band, n_gauss)
Adding continuum opacities
Explain strategies to calculate continuum opacities
- Usually the continuum units used as input in the GCM is cm-1 amagat-2