EGU26-11301, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-11301
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Characterizing Anthropogenic and Biogenic Sources of CO2 and CH4 in Houston, Texas, USA
Bernhard Rappenglück1,2 and Irfan Karim1,2
Bernhard Rappenglück and Irfan Karim
  • 1University of Houston, Department of Earth and Atmospheric Sciences, Houston, United States of America (brappenglueck@uh.edu)
  • 2Institute of Climate and Atmospheric Science, Houston, United States of America

This study presents a comprehensive 2022 dataset of continuous in-situ measurements of δCO2 and CH4, δ¹³CO2 and δ¹³CH4 in Houston, Texas, USA complemented by targeted canister sampling to characterize key anthropogenic and biogenic emission sources. It also integrates ground-based in-situ measurements with satellite observations to characterize CO₂ and CH₄ emission hotspots in Houston, Texas.

Seasonal background variability reflects distinct biogeochemical processes: CO₂ declines from ~435 ppm in winter to ~410 ppm in summer due to photosynthetic uptake, while CH₄ decreases from ~2.02 to ~1.88 ppm primarily through OH oxidation. Regional contrasts are evident, with lower marine-influenced backgrounds (~410 ppm CO₂, ~1.85 ppm CH₄) compared to continental sectors (>435 ppm CO₂, >2.05 ppm CH₄).

Boundary-layer-height (BLH)-corrected enhancements reveal strong seasonal patterns in anthropogenic emissions. ΔCO₂ peaks in winter-fall (up to ~138 ppm hourly; ~20.6 ppm monthly) and drops to ~8.96 ppm in summer, while ΔCH₄ shows maxima in winter-spring (~5.45 ppm hourly; ~0.10 ppm monthly) and a summer minimum (~0.08 ppm). The 2022 mean ΔCH₄/ ΔCO₂ ratio (8.8 ppb/ppm) is ~14% higher than Philadelphia's in-situ winter value and ~35-40% above EDGAR v8.1 and EPA inventories, but broadly consistent with recent satellite-based estimates across U.S. cities.

Bivariate ΔCH₄/ ΔCO₂ mapping identifies major hotspots at McCarty, Blue Ridge, and Coastal Plains landfills (>40-60 ppb/ppm), which are underestimated or absent in inventories. Sharp enhancements at the Ship Channel and McCarty landfill align with satellite NO₂ and HCHO peaks, confirming these as multi-source hotspots. The BLH-corrected in-situ approach captures rapid emission events and diurnal variability, providing finer-scale source attribution and plume detection within the satellite sub-pixel domain that are missed by single overpasses.

Temporal analysis revealed distinct seasonal variability: δ¹³CO2 was most depleted in winter, reflecting enhanced combustion-related CO2, whereas δ¹³ CO2 showed the most negative values in summer and fall, consistent with intensified microbial methanogenesis under warm, humid conditions. Background δ¹³CO2 ranged from –11.8‰ to –13.2‰ depending on air mass origin, while δ¹³CH4 varied between –47.2‰ and –50.7‰, reflecting marine–continental transitions. Spatially, bivariate plots and isotopic mapping identified strong CH₄ enhancements (>0.5 ppm) and highly depleted δ¹³ CH4  (−50.5‰ to −51‰) over the McCarty landfill, indicating dominant microbial methane generation, further confirmed by canister measurements δ¹³CH4 ≈ −60.3‰. Estimated emissions from the McCarty Landfill, based on our isotopic mass-balance analysis, were ~2,100 kg CH₄ h⁻¹ ±55%, exceeding the EPA GHGRP inventory value (~857 kg CH₄ h⁻¹) and moderately higher than the Carbon Mapper satellite-derived flux but within combined uncertainties (~1,427 kg CH₄ h⁻¹ ±91%). highlighting that bottom-up inventories underestimate methane emissions from large urban landfills such as McCarty. Overall, the isotopic evidence demonstrates that integrating δ¹³C analyses data provides critical insights into source attribution and the relative roles of combustion, industrial, and microbial processes shaping Houston’s CO2 and CH4 emission landscape.

How to cite: Rappenglück, B. and Karim, I.: Characterizing Anthropogenic and Biogenic Sources of CO2 and CH4 in Houston, Texas, USA, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11301, https://doi.org/10.5194/egusphere-egu26-11301, 2026.

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