Difference between revisions of "Building Opacity Tables"
From Planets
(→Building correlated-k tables) |
(→Building correlated-k tables) |
||
| Line 5: | Line 5: | ||
== Building correlated-k tables == | == Building correlated-k tables == | ||
| − | + | ||
| + | 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 == | == Adding continuum opacities == | ||
Revision as of 13:50, 31 March 2023
This page describes the main steps required to build new opacity tables.
Calculation of high-resolution spectra
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)
