作者: A. Goldman , D. G. Murcray , F. J. Murcray , A. Barbe , C. Secroun
DOI: 10.1007/978-94-009-5313-0_89
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摘要: Long path high resolution (0.02 cm-1) atmospheric infrared solar spectra show numerous new absorption features of ozone and other trace constituents. Spectroscopic analysis several bands from these spectra, coupled with laboratory intensity measurements, generated line parameters compilation for the ν1, ν3 ν2, 2ν2 -ν2 ν1 + ν2+ bands. These provide improved quantification as well constituents spectral overlapping ozone. Laboratory at 0.02 cm-3 assist in identification Higher (0.004 measurements are progress.