Difference between revisions of "Building Opacity Tables"
From Planets
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(→Calculation of high-resolution spectra) |
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== Calculation of high-resolution spectra == | == Calculation of high-resolution spectra == | ||
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| + | describe the tools we used : | ||
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| + | - k-spectrum | ||
| + | - home-made scripts | ||
== Building correlated-k tables == | == Building correlated-k tables == | ||
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)
