Preprints
https://doi.org/10.5194/egusphere-2023-1057
https://doi.org/10.5194/egusphere-2023-1057
05 Jun 2023
 | 05 Jun 2023

Empirical upscaling of OzFlux eddy covariance for high-resolution monitoring of terrestrial carbon uptake in Australia

Chad A. Burton, Luigi J. Renzullo, Sami W. Rifai, and Albert I. J. M. Van Dijk

Abstract. We develop high resolution (1 km) estimates of Gross Primary Productivity (GPP), Ecosystem Respiration (ER) and Net Ecosystem Exchange (NEE) over the Australian continent for the period January 2003 to June 2022 by empirical upscaling of flux tower measurements. We compare our estimates with nine other products that cover the three broad categories that define current methods for estimating the terrestrial carbon cycle and assess if consiliences between datasets can point to the correct dynamics of Australia’s carbon cycle. Our results indicate that regional empirical upscaling greatly improves upon the existing global empirical upscaling efforts, outperforms process-based models, and agrees much better with the dynamics of CO2 flux over Australia as estimated by two regional atmospheric inversions. Our nearly 20-year estimates of terrestrial carbon fluxes revealed Australia is a strong net carbon sink of -0.44 (IQR=0.42) PgC/year on-average, with an inter-annual variability of 0.18 PgC/year and an average seasonal amplitude of 0.85 PgC/yr. Annual mean carbon uptake estimated from other methods ranged considerably, while carbon flux anomalies showed much better agreement between methods. NEE anomalies were predominately driven by cumulative rainfall deficits and surpluses, resulting in larger anomalous responses from GPP over ER. In contrast, we show that the long-term average seasonal cycle is dictated more by the variability in ER than GPP, resulting in peak carbon uptake typically occurring during the cooler, drier Austral autumn, and winter months. This new estimate of Australia’s terrestrial carbon cycle provides a benchmark for assessment against Land Surface Model simulations, and a means for monitoring of Australia’s terrestrial carbon cycle at an unprecedented high-resolution. We call this new estimate of Australia’s terrestrial carbon cycle, “AusEFlux” (Australian Empirical Fluxes).

Chad A. Burton et al.

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-1057', Anonymous Referee #1, 22 Jun 2023
    • AC1: 'Reply on RC1', Chad Burton, 13 Jul 2023
  • CC1: 'Comment on egusphere-2023-1057', Elise Pendall, 17 Jul 2023
    • AC3: 'Reply on CC1', Chad Burton, 04 Aug 2023
  • RC2: 'Comment on egusphere-2023-1057', Anonymous Referee #2, 20 Jul 2023
    • AC2: 'Reply on RC2', Chad Burton, 04 Aug 2023

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-1057', Anonymous Referee #1, 22 Jun 2023
    • AC1: 'Reply on RC1', Chad Burton, 13 Jul 2023
  • CC1: 'Comment on egusphere-2023-1057', Elise Pendall, 17 Jul 2023
    • AC3: 'Reply on CC1', Chad Burton, 04 Aug 2023
  • RC2: 'Comment on egusphere-2023-1057', Anonymous Referee #2, 20 Jul 2023
    • AC2: 'Reply on RC2', Chad Burton, 04 Aug 2023

Chad A. Burton et al.

Data sets

AusEFlux: Empirical upscaling of OzFlux eddy covariance flux tower data over Australia Chad Burton, Luigi Renzullo, Sami Rifai, and Albert Van Dijk https://doi.org/10.5281/zenodo.7947265

Model code and software

NEE Modelling Chad Burton https://github.com/cbur24/NEE_modelling

Chad A. Burton et al.

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Short summary
Australia’s land-based ecosystems play a critical role in controlling the variability of the global land carbon sink. However, uncertainties in the methods used for quantifying carbon fluxes limit our understanding. We develop high resolution estimates of Australia's land carbon fluxes using machine learning methods and find that Australia is, on average, a stronger carbon sink than previously thought, and that the seasonal dynamics of the fluxes differ from those described by other methods.