Atmos. Meas. Tech., 12, 35–50, 2019 https://doi.org/10.5194/amt-12-35-2019 © Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License. Using a speed-dependent Voigt line shape to retrieve O2 from Total Carbon Column Observing Network solar spectra to improve measurements of XCO2 Joseph Mendonca1, Kimberly Strong1, Debra Wunch1, Geoffrey C. Toon2, David A. Long3, Joseph T. Hodges3, Vincent T. Sironneau3, and Jonathan E. Franklin4 1Department of Physics, University of Toronto, Toronto, ON, Canada 2Jet Propulsion Laboratory, Pasadena, CA, USA 3National Institute of Standards and Technology, Gaithersburg, MD, USA 4Harvard John A. Paulson School of Engineering and Applied Sciences, Cambridge, MA, USA Correspondence: Joseph Mendonca (
[email protected]) Received: 23 February 2018 – Discussion started: 3 April 2018 Revised: 23 August 2018 – Accepted: 17 September 2018 – Published: 3 January 2019 Abstract. High-resolution, laboratory, absorption spectra of infrared CO2 and O2 spectra to improve the accuracy of 1 3 − the a 1g X 6g oxygen (O2) band measured using cav- XCO2 measurements. ity ring-down spectroscopy were fitted using the Voigt and speed-dependent Voigt line shapes. We found that the speed- dependent Voigt line shape was better able to model the mea- sured absorption coefficients than the Voigt line shape. We 1 Introduction used these line shape models to calculate absorption coeffi- cients to retrieve atmospheric total columns abundances of Accurate remote sensing of greenhouse gases (GHGs) such O2 from ground-based spectra from four Fourier transform as CO2, in the Earth’s atmosphere is important for study- spectrometers that are a part of the Total Carbon Column Ob- ing the carbon cycle to better understand and predict cli- serving Network (TCCON).