Paper
8 December 2011 Infrared radiant spectrum calculation of the gas in the atmosphere based on physical model
Juan Wang, Licheng Xu, Fang Wang
Author Affiliations +
Proceedings Volume 8002, MIPPR 2011: Multispectral Image Acquisition, Processing, and Analysis; 80020C (2011) https://doi.org/10.1117/12.901895
Event: Seventh International Symposium on Multispectral Image Processing and Pattern Recognition (MIPPR2011), 2011, Guilin, China
Abstract
This paper proposes a theoretical method based on physical model to calculate infrared (IR) radiation spectrum. IR physics establishes that emission abilities of objects are measured by emissivity, while the emissivity of objects is based on the emissivity of a blackbody. Planck formula shows how to calculate the spectral energy density of a blackbody, and IR radiation spectrum of a sample can be easily obtained if its emissivity is known. Kirchhoff's law shows the emissivity of an object is equal to its absorptance at the same conditions. By calculating the absorption coefficient using line-by-line model, the absorptance can be achieved through the relationship between them. The performance data of the technique is from public databases.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Juan Wang, Licheng Xu, and Fang Wang "Infrared radiant spectrum calculation of the gas in the atmosphere based on physical model", Proc. SPIE 8002, MIPPR 2011: Multispectral Image Acquisition, Processing, and Analysis, 80020C (8 December 2011); https://doi.org/10.1117/12.901895
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KEYWORDS
Absorption

Infrared radiation

Atmospheric modeling

Databases

Molecules

Black bodies

Doppler effect

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