Published May 30, 2023 | Version Published
Journal Article Open

Inferring the vertical distribution of CO and CO₂ from TCCON total column values using the TARDISS algorithm

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Jet Propulsion Lab
  • 3. ROR icon University of Toronto
  • 4. ROR icon Ames Research Center
  • 5. ROR icon Cooperative Institute for Research in Environmental Sciences
  • 6. ROR icon National Oceanic and Atmospheric Administration

Abstract

We describe an approach for determining limited information about the vertical distribution of carbon monoxide (CO) and carbon dioxide (CO2) from total column ground-based Total Carbon Column Observation Network (TCCON) observations. For CO and CO2, it has been difficult to retrieve information about their vertical distribution from spectral line shapes because of the errors in the spectroscopy and the atmospheric temperature profile that mask the effects of variations in their mixing ratio with altitude. For CO2 the challenge is especially difficult given that these variations are typically 2 % or less. Nevertheless, if sufficient accuracy can be obtained, such information would be highly valuable for evaluation of retrievals from satellites and more generally for improving the estimate of surface sources and sinks of these trace gases.

We present here the Temporal Atmospheric Retrieval Determining Information from Secondary Scaling (TARDISS) retrieval algorithm. TARDISS uses several simultaneously obtained total column observations of the same gas from different absorption bands with distinctly different vertical averaging kernels. The different total column retrievals are combined in TARDISS using a Bayesian approach where the weights and temporal covariance applied to the different retrievals include additional constraints on the diurnal variation in the vertical distribution for these gases. We assume that the near-surface part of the column varies rapidly over the course of a day (from surface sources and sinks, for example) and that the upper part of the column has a larger temporal covariance over the course of a day.

Using measurements from the five North American TCCON sites, we find that the retrieved lower partial column (between the surface and  800 hPa) of the CO and CO2 dry mole fractions (DMFs) have slopes of 0.999 ± 0.002 and 1.001 ± 0.003 with respect to lower column DMF from integrated in situ data measured directly from aircraft and in AirCores. The average error for our lower column CO retrieval is 1.51 ppb ( 2 %) while the average error for our CO2 retrieval is 5.09 ppm ( 1.25 %). Compared with classical line-shape-derived vertical profile retrievals, our algorithm reduces the influence of forward model errors such as imprecision in spectroscopy (line shapes and intensities) and in the instrument line shape. In addition, because TARDISS uses the existing retrieved column abundances from TCCON (which themselves are computationally much less intensive than profile retrieval algorithms), it is very fast and processes years of data in minutes. We anticipate that this approach will find broad application for use in carbon cycle science.

Copyright and License

© Author(s) 2023. This work is distributed under the Creative Commons Attribution 4.0 License. Published by Copernicus Publications on behalf of the European Geosciences Union.

Acknowledgement

The authors thank the ObsPack team and data providers for the in situ profile data used for validation. The data were downloaded from https://gml.noaa.gov/ccgg/obspack/data.php?id=obspack_co2_1_GLOBALVIEWplus_v5.0_2019-08-12 (last access: 2 September 2022). In particular, we thank the NASA LaRC AVOCET and DACOM groups for the KORUS-AQ CO2 and CO data, respectively; NASA Goddard for the Picarro CO2 data at the Armstrong AFB; the SEAC4RS and ATom groups for the CO2 data; and the NOAA Global Monitoring Laboratory for the AirCore CO2 and CO data and the long-term aircraft CO2 and CO at the SGP and ETL sites.

Funding

This work was funded via grant no. 80NSSC22K1066 for supporting the retrievals from the TCCON stations. A portion of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (grant no. 80NM0018D0004). Bianca C. Baier is supported by NASA (grant no. 80NSSC18K0898).

Data Availability

The data used in this study are made up of TARDISS retrieval products from five TCCON stations. The retrieval data are publicly available through CaltechDATA (https://doi.org/10.22002/pn9de-cry27, Parker et al., 2022), and the data input into the retrieval are publicly available via https://tccondata.org/ (last access: 28 April 2023; TCCON, 2023). The retrieval code is also available through CaltechDATA (https://doi.org/10.22002/dakd7-cdp29, Parker et al., 2023).

Supplemental Material

The supplement related to this article is available online at: https://doi.org/10.5194/amt-16-2601-2023-supplement.

Additional Information

This paper was edited by Thomas von Clarmann and reviewed by two anonymous referees.

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Additional details

Related works

Is new version of
Discussion Paper: 10.5194/amt-2022-322 (DOI)
Is supplemented by
Supplemental Material: 10.5194/amt-16-2601-2023-supplement (DOI)

Funding

National Aeronautics and Space Administration
80NSSC22K1066
National Aeronautics and Space Administration
80NM0018D0004
National Aeronautics and Space Administration
80NSSC18K0898

Dates

Accepted
2023-04-21

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