EGU25-6723, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-6723
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Complementarity of GEO, LEO, and Lagrange-1 Point Satellite Aerosol Observations 
Omar Torres1, Changwoo Ahn2, Hiren Jethva3, and Diego Loyola4
Omar Torres et al.
  • 1NASA Goddard Space Flight Center, Atmospheric Chemistry and Dynamics Laboratory, Greenbelt, United States of America (omar.o.torres@nasa.gov)
  • 2Science Systems and Applications, Inc, Lanham, Maryland, USA
  • 3Morgan State University, Baltimore, Maryland, USA
  • 4German Aerospace Center, Oberpfaffenhofen, Germany

Currently deployed (GEMS, TEMPO) and soon-to-be launched (S4-UVN) sensors constitute the first GEO satellite constellation for Air Quality observations in the northern hemisphere. The simultaneous availability of similar observations from platforms at LEO and L1 orbital configurations offers a unique  opportunity for the integration of a quasi-global  Air Quality observing system. In this presentation, we will discuss specific aerosol events to show the complementary nature of GEO aerosol observations and those of LEO (S5P-TROPOMI and S5-UVNS), and Langrange1-EPIC measurements. Integrated GEO, LEO and L1 observations will be used to demonstrate inter-instrument synergy for sensor calibration transfer, and the understanding of  the nature of local events in regional and global contexts.   

How to cite: Torres, O., Ahn, C., Jethva, H., and Loyola, D.: Complementarity of GEO, LEO, and Lagrange-1 Point Satellite Aerosol Observations , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6723, https://doi.org/10.5194/egusphere-egu25-6723, 2025.