4.2 Article

High-sensitivity CW-cavity ringdown spectroscopy of 12CO2 near 1.5 μm

Journal

JOURNAL OF MOLECULAR SPECTROSCOPY
Volume 230, Issue 1, Pages 1-21

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.jms.2004.09.011

Keywords

CW-CRDS; carbon dioxide; (CO2)-C-12; atmospheric window; effective Hamiltonian

Ask authors/readers for more resources

The absorption spectrum of carbon dioxide in natural isotopic abundance has been recorded by CW-cavity ringdown spectroscopy with a setup based on fibered DFB lasers. By using a series of 31 DFB lasers, the CO, spectrum could be recorded in the 61326747 cm(-1) region with a typical sensitivity of 5 x 10(-10) cm(-1). More than 3300 line positions were measured and assigned to the (CO2)-C-12-O-16 species while only 1159 (generally calculated) line positions are provided by the HITRAN database. Altogether, the band-by-band analysis has led to the determination of the rovibrational parameters of 53, 5, and 9 bands for the (CO2)-C-12-O-16, (OCO)-O-16-C-12-O-17, and (OCO)-O-16-C-12-O-18 isotopologues, respectively. For the three studied isotopologues, the majority of the observed line positions show an agreement close to the experimental uncertainty (3 x 10(-3) cm(-1)) with the predictions of their respective effective Hamiltonian models. Maximum deviations of the order of 0.03, 0.05, and 0.04 cm(-1) were, however, evidenced for (CO2)-C-12-O-16, (OCO)-O-16-C-12-O-17, and (OCO)-O-16-C-12-O-18, respectively. As some observed line positions show significant deviations from the predictions of the effective Hamiltonian model and as the observed data set has been recently enlarged by newly reported measurements, the observed line positions were gathered with all the data available in the literature in order to refine the set of effective Hamiltonian parameters of the (CO2)-C-12-O-16 isotopic species. The refined set of 130 effective Hamiltonian parameters reproduces more than 29000 observed line positions of (CO2)-C-12-O-16 with an RMS = 0.002 cm(-1). The comparison of our line positions values with those published earlier and with the line list provided by HITRAN is discussed. (C) 2004 Elsevier Inc. All rights reserved.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.2
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available