In the calculations I used
an absorption wavenumber of 650 cm - 1 and tuned the optical depth to reach saturation.
Not exact matches
We derive the spatial variations of dust continuum emission at different
wavenumbers, which are compared with those of the [O III] 88 micron (113 cm ^ -1) emission and the OH 119 micron (84 cm ^ -1)
absorption.
Click on Spectral Database Browser — then Atmosphere Browser — set the
wavenumber to 0 to 3,000 which covers the majority of the visible and far infrared spectrum and you can compare the
absorption bands of all the various gases.
CO2 has a main
absorption band near 15 um (about
wavenumber 667) that includes a strong
absorption line at that wavelength with correspondingly weaker lines as one moves into the «wings» toward either 13 or 17 um.
The standard tables for
absorption of photons by CO2 show that at STP, 50 % of photons are absorbed within 25m and 50m for
wavenumbers 650, and 700 respectively.
Phil says: «Where do you get your value of 0.2 emissivity from, what range of
wavenumber is it for, why haven't you accounted for the variation of energy over the
wavenumber range or the different
absorption bands of H2O and CO2?»
The radiation spectrum for temperatures between 300 k and 250 k only includes a single
absorption window for CO2 centred on 14.77 microns wavelength (677 cm ^ -1
wavenumber).