EGU25-4839, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-4839
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Wednesday, 30 Apr, 09:20–09:30 (CEST)
 
Room M1
Monitoring urban CO2 emissions from space: current status and future potential
Abhishek Chatterjee1, Doyeon Ahn2, Dustin Roten1, Matthaus Kiel1, Robert Nelson1, Thomas Kurosu1, Dien Wu3, John Lin4, and Kevin Gurney5
Abhishek Chatterjee et al.
  • 1NASA JPL, Caltech, Earth Science, Pasadena, United States of America (abhishek.chatterjee@jpl.nasa.gov)
  • 2Morgan State University, NASA Goddard Space Flight Center, Greenbelt, United States of America
  • 3Colorado State University, Fort Collins, United States of America
  • 4University of Utah, Salt Lake City, United States of America
  • 5Northern Arizona University, Flagstaff, United States of America

Cities with their large, dense populations are concentrated sources of CO2 emissions to the atmosphere. Although more than 60% of global fossil fuel CO2 emissions are from cities, yet we lack high-quality city-level emissions inventories and/or independent verification datasets across the majority of global cities. Several cities have also adopted ambitious goals of reaching net-zero emissions by 2030 or 2050. In fact, most recently at COP28, several cities, including those in non-Annex I countries, signed up to be part of the Coalition for High Ambition Multilevel Partnerships for Climate Action (CHAMP ; UNFCCC COP28), thereby obligating themselves to report emissions on a timely basis. So, how can we assist city-scale and local policy and decision-making entities to utilize information from space-based observations to monitor and track GHG emissions? In this presentation, I will show the application of OCO-2 and OCO-3 data across a suite of global cities worldwide. I will show that well-defined and robust mathematical frameworks can exploit the information content in dense, fine-scale, space-based CO2 data to deliver not only whole-city or total emission estimates but also attribute them to individual sectors, such as large point sources, on-road emissions, etc. I will also show some examples from recent studies that illustrate the value of exploiting co-located emissions of other species (such as CO, NO2, CH4) to obtain novel insights into sectoral emission characteristics. Examples from OCO-3, TROPOMI and EMIT data will be shown to demonstrate the value of assimilating information from disparate tracers for reliable source attributions. Even though there are methodological challenges in setting up a multi-species framework, the problem is not insurmountable. Development and refinement of such multi-species frameworks need to start now in order to unlock the true potential of space-based datasets. This is also crucial to optimally utilizing the information from future space-based CO2 emission monitoring sensors, such as Carbon Mapper, ESA’s CO2M, JAXA’s GOSAT-GW and other planned missions. The presentation will conclude with a discussion of implications of space-based datasets for tracking city- and country-level progress towards meeting proposed CO2 emission reduction goals and its value and benefit for advancing bottom-up emission inventories.

How to cite: Chatterjee, A., Ahn, D., Roten, D., Kiel, M., Nelson, R., Kurosu, T., Wu, D., Lin, J., and Gurney, K.: Monitoring urban CO2 emissions from space: current status and future potential, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4839, https://doi.org/10.5194/egusphere-egu25-4839, 2025.