Contributions of argon, nitrogen, and oxygen to air broadening in the oxygen A-band
Abstract
The oxygen (O2) A-band is used to determine the airmass in ground- and space-based remote sensing measurements because O2 is well-mixed in the Earth’s atmosphere and its column-integrated amount fraction on a dry-gas basis is nearly constant. Because biases in the retrieved airmass propagate to measurements of target species, low-uncertainty spectroscopic parameters are essential for increasingly precise and accurate greenhouse gas measurements. However, laboratory measurements and atmospheric retrievals of this O2 band typically neglect the line-shape effects caused by collisions with argon (Ar), which comprises 0.934 % by volume of the Earth’s atmosphere. To quantify the contribution of Ar to O2 A-band air-broadening line-shape parameters, we measured pressure broadening and shifting parameters for ten high J lines in the P-branch of this band. These data were acquired in the laboratory over a range of pressures and nitrogen (N2), O2, and Ar amount fractions using cavity ring-down spectroscopy. Respective line-shape parameters for these collisional partners were determined with a multi-spectrum fitting algorithm. These results were combined with literature data to provide an empirical model for the rotational dependencies of the broadening and shifting parameters by each collisional partner. Incorporating these results into analyses of atmospheric column-integrated solar absorption spectra in the O2 A-band shows that the neglect of Ar can lead to a small but potentially relevant systematic bias in surface pressure retrievals and a slight increase in the fit residuals of atmospheric spectra.
Copyright and License
Published by Elsevier Ltd.
Acknowledgement
EMA and JTH acknowledge funding from the NIST Greenhouse Gas and Climate Science Program and the National Aeronautics and Space Administration (NASA) [contract NNH20ZDA0001NOCOT(NIST)]. LES acknowledges support of a National Science Foundation Graduate Research Fellowship under Grant No 2139433. Work at Caltech (MO and LES) was funded by NASA Grant Numbers 80NSSC21K1331 and 80NSSC24K0746. A portion of this research was carried out at the Jet Propulsion Laboratory (JPL), California Institute of Technology, under a contract with NASA (80NM0018D0004). Government sponsorship is acknowledged. JLL and the operation of the Park Falls TCCON site were supported by NASA funding through grant 80NSSC22K1066. The authors would like to thank Adam J. Fleisher (NIST) and Sean M. Bresler (NIST) for commenting on the manuscript.
Supplemental Material
Appendix. Supplementary materials: 1-s2.0-S0022407325001426-mmc1.docx
Additional Information
HITRAN 2024: HITRAN special issue to celebrate the scientific contributions of Dr. Laurence Rothman
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Additional details
- National Science Foundation
- Graduate Research Fellowship 2139433
- National Aeronautics and Space Administration
- NNH20ZDA0001N-OCOT(NIST)
- National Institute of Standards and Technology
- Greenhouse Gas and Climate Science Program -
- National Aeronautics and Space Administration
- 80NSSC21K1331
- National Aeronautics and Space Administration
- 80NSSC24K0746
- National Aeronautics and Space Administration
- 80NM0018D0004
- National Aeronautics and Space Administration
- TCCON 80NSSC22K1066
- Accepted
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2025-04-15Accepted
- Available
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2025-04-16Published online
- Available
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2025-04-25Version of record
- Caltech groups
- Division of Chemistry and Chemical Engineering (CCE), Total Carbon Column Observing Network
- Publication Status
- Published