Review of some non-LTE high-altitude CO2 4.3-micrometer background effects: a ten-year update

John B. Kumer

doi:10.1117/12.48736

1 December 1991 Review of some non-LTE high-altitude CO₂ 4.3-micrometer background effects: a ten-year update

John B. Kumer

Author Affiliations +

Proceedings Volume 1540, Infrared Technology XVII; (1991) https://doi.org/10.1117/12.48736
Event: San Diego, '91, 1991, San Diego, CA, United States

Abstract

Progress in the ten years since the previous SPIE publication (Kumer, 1981) on the subject of modeling high-altitude non-LTE CO2 4.3 micron phenomena is summarized. Several models have been developed in these years. These models implement improvements in radiation transport, spectral characterization, rate constants, atmospheric models, and numerics. Applications of these models to the three distinct cases of daytime, ambient night time, and aurora are discussed, and compared with applications of the older model. Several new data bases have just become, or will soon become available. The obvious applications of the models to these data will be discussed.

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John B. Kumer "Review of some non-LTE high-altitude CO₂ 4.3-micrometer background effects: a ten-year update", Proc. SPIE 1540, Infrared Technology XVII, (1 December 1991); https://doi.org/10.1117/12.48736

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