Abstract
Full-spectrum k-distributions (or absorption-line blackbody distribution functions) have been calculated for CO 2 from the new HITEMP database for a large number of gas temperatures, and an approximate mathematical correlation is presented. This correlation supersedes the older one by Denison and Webb, which was based on the HITRAN92 database. Comparison between the correlations shows that, although giving excellent results for temperatures below 1000 K, the older correlation seriously underpredicts radiative losses at high temperatures
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