Abstract

Abstract. The Tropospheric Monitoring Instrument (TROPOMI) on the ESA Copernicus Sentinel-5 satellite (S5-P) measures carbon monoxide (CO) total column concentrations as one of its primary targets. In this study, we analyze TROPOMI observations over Mexico City in the period 14 November 2017 to 25 August 2019 by means of collocated CO simulations using the regional Weather Research and Forecasting coupled with Chemistry (WRF-Chem) model. We draw conclusions on the emissions from different urban districts in the region. Our WRF-Chem simulation distinguishes CO emissions from the districts Tula, Pachuca, Tulancingo, Toluca, Cuernavaca, Cuautla, Tlaxcala, Puebla, Mexico City, and Mexico City Arena by 10 separate tracers. For the data interpretation, we apply a source inversion approach determining per district the mean emissions and the temporal variability, the latter regularized to reduce the propagation of the instrument noise and forward-model errors in the inversion. In this way, the TROPOMI observations are used to evaluate the Inventario Nacional de Emisiones de Contaminantes Criterio (INEM) inventory that was adapted to the period 2017–2019 using in situ ground-based observations. For the Tula and Pachuca urban areas in the north of Mexico City, we obtain 0.10±0.004 and 0.09±0.005 Tg yr−1 CO emissions, which exceeds significantly the INEM emissions of <0.008 Tg yr−1 for both areas. On the other hand for Mexico City, TROPOMI estimates emissions of 0.14±0.006 Tg yr−1 CO, which is about half of the INEM emissions of 0.25 Tg yr−1, and for the adjacent district Mexico City Arena the emissions are 0.28±0.01 Tg yr−1 according to TROPOMI observations versus 0.14 Tg yr−1 as stated by the INEM inventory. Interestingly, the total emissions of both districts are similar (0.42±0.016 Tg yr−1 TROPOMI versus 0.39 Tg yr−1 adapted INEM emissions). Moreover, for both areas we found that the TROPOMI emission estimates follow a clear weekly cycle with a minimum during the weekend. This agrees well with ground-based in situ measurements from the Secretaría del Medio Ambiente (SEDEMA) and Fourier transform spectrometer column measurements in Mexico City that are operated by the Network for the Detection of Atmospheric Composition Change Infrared Working Group (NDACC-IRWG). Overall, our study demonstrates an approach to deploying the large number of TROPOMI CO data to draw conclusions on urban emissions on sub-city scales for metropolises like Mexico City. Moreover, for the exploitation of TROPOMI CO observations our analysis indicates the clear need for further improvements of regional models like WRF-Chem, in particular with respect to the prediction of the local wind fields.

Highlights

  • Carbon monoxide (CO) is an atmospheric trace gas emitted by incomplete combustion to the atmosphere

  • We found that the emissions of the central part of Mexico City (CdMx) are assumed to be too high in the adapted Inventario Nacional de Emisiones de Contaminantes Criterio (INEM) inventory (0.25 Tg yr−1), where Tropospheric Monitoring Instrument (TROPOMI) measurements indicate lower values for CdMx (0.14±0.006 Tg yr−1)

  • We found that urban pollution can be monitored by the TROPOMI CO data

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Summary

Introduction

Carbon monoxide (CO) is an atmospheric trace gas emitted by incomplete combustion to the atmosphere (e.g., biomass burning, industrial activity, and traffic). Its background concentration is relatively low with an atmospheric residence time varying from days to month (Holloway et al, 2000) depending on the atmospheric concentration of the hydroxyl radical (Spivakovsky et al, 2000). These characteristics established CO as a tracer for air pollution and transport pro-. The TROPOMI CO dataset was validated with groundbased measurements of the Total Carbon Column Observing Network (TCCON) (Borsdorff et al, 2018a) and intercompared with simulated CO fields of the European Centre for Medium-Range Weather Forecasts (ECMWF) Integrated Forecasting System (Borsdorff et al, 2018b). On 11 July 2018, it was concluded that the TROPOMI CO data quality is fully compliant with the mission requirements of 15 % precision and 10 % accuracy and so it was released for public usage (https://scihub.copernicus.eu, last access: 16 December 2020)

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