Relative Potency of Greenhouse Molecules
Abstract
The forcings due to changing concentrations of Earth's five most important, naturally occurring greenhouse gases, HO, CO, O, NO and CH as well as CF and SF were evaluated for the case of a cloud-free atmosphere. The calculation used over 1.5 million lines having strengths as low as cm. For a hypothetical, optically thin atmosphere, where there is negligible saturation of the absorption bands, or interference of one type of greenhouse gas with others, the per-molecule forcings are of order Watts for HO, CO, O, NO and CH and of order Watts for CF and SF. For current atmospheric concentrations, the per-molecule forcings of the abundant greenhouse gases HO and CO are suppressed by four orders of magnitude. The forcings of the less abundant greenhouse gases, O, NO and CH, are also suppressed, but much less so. For CF and SF, the suppression is less than an order of magnitude because the concentrations of these gases is very low. For current concentrations, the per-molecule forcings are two to four orders of magnitude greater for O, NO, CH, CF and SF than those of HO or CO. Doubling the current concentrations of CO, NO or CH increases the forcings by a few per cent. A concentration increase of either CF or SF by a factor of 100 yields a forcing nearly an order of magnitude smaller than that obtained by doubling CO. Important insight was obtained using a harmonic oscillator model to estimate the power radiated per molecule. Unlike the most intense bands of the 5 naturally occurring greenhouse gases, the frequency-integrated cross sections of CF and SF were found to noticeably depend on temperature.
Keywords
Cite
@article{arxiv.2103.16465,
title = {Relative Potency of Greenhouse Molecules},
author = {W. A. van Wijngaarden and W. Happer},
journal= {arXiv preprint arXiv:2103.16465},
year = {2021}
}
Comments
29 pages, 10 figures. arXiv admin note: substantial text overlap with arXiv:2006.03098