Challenges and benefits of using NOx as a quantitative proxy for fossil fuel CO2 in an urban area based on radiocarbon measurements

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Abstract

Radiocarbon (14CO2) observations are the benchmark for quantifying fossil fuel CO2 (ffCO2) in the atmosphere, but continuous 14CO2 measurements are not yet available. Continuous estimates of ffCO2 can be made by observing continuously measurable proxies that are co-emitted during fossil fuel combustion. This paper investigates the potential and challenges of using in situ NOx observations in urban areas to quantitatively estimate hourly ffCO2 enhancements, in the example of the ICOS pilot station in Heidelberg, Germany. The short atmospheric lifetime of NOx limits the use of the observed signal to a local area. Thus, a local NOx and ffCO2 background was approximated using the Stochastic Time-Inverted Lagrangian Transport (STILT) model and bottom-up emission estimates from the Netherlands Organisation for Applied Scientific Research (TNO). Using 14CO2 data from 185 hourly integrated flask samples between 2020–2021, mean ratios of local excess NOx (1NOx) to local excess ffCO2 (1ffCO2) of 1.40ppbppm−1 for winter and 2.12ppbppm−1 for summer were calculated. These ratios were applied to the 1NOx time series to construct continuous 1ffCO2 estimates. The uncertainty of the 1NOx-based 1ffCO2 record was estimated at 3.94ppm. Comparisons with 14CO2-based and 1CO-based 1ffCO2 estimates showed good agreement, while still demonstrating distinct behaviour for individual events. 1NOx shows considerable potential as 1ffCO2 proxy and as useful addition to 1CO-based estimates, as both proxies have different footprints due to their lifetimes. A key challenge remains in reliably determining the seasonal and diurnal cycle of average 1NOx to 1ffCO2 ratios.

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APA

Juchem, H., Maier, F., Levin, I., Jordan, A., Pöhler, D., Rosendahl, C., … Hammer, S. (2025). Challenges and benefits of using NOx as a quantitative proxy for fossil fuel CO2 in an urban area based on radiocarbon measurements. Atmospheric Chemistry and Physics, 25(24), 18373–18388. https://doi.org/10.5194/acp-25-18373-2025

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