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Line strengths and self-broadening coefficients of carbon dioxide isotopologues (CO2 and OCO) near 2.04 μm for the in situ laser sensing of the Martian atmosphere
Authors:T. Le Barbu,V. Zé  ninari,B. Parvitte,G. Durry
Affiliation:a Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039, 51687 Reims, Cedex 2, France
b Institut Pierre Simon Laplace (IPSL), Service d’Aéronomie, UMR 7620, CNRS-Réduit de Verrières, B.P. 3, 91371 Verrières-le-Buisson Cedex, France
Abstract:A diode laser spectrometer was used in the laboratory to study 13CO2 and 18O12C16O line intensities and self-broadening coefficients near 2.04 μm. The spectral region ranging from 4896 to 4903 cm1, which is suitable for in situ laser sensing of both isotopologues in the lower Martian atmosphere, was investigated using a distributed feedback GaInSb diode laser. Five lines of the (2 00 1)II←(0 0 0) band of 13CO2 and seven lines of the (2 00 1)II←(0 0 0) band of 18O12C16O were carefully revisited. The measured intensities and self-broadening coefficients were thoroughly compared with relevant molecular databases.
Keywords:07.57T   07.87
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