Difference between revisions of "Building Opacity Tables"
From Planets
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== Adding continuum opacities == | == Adding continuum opacities == | ||
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Revision as of 15:06, 31 March 2023
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
