A245-01
OCO-3 SAM mode: Spatiotemporal Variability of XCO2 over the Los Angeles Megacity
Wednesday, 16 December 2020: 19:00
Virtual
Matthäus Kiel1, Annmarie Eldering1, Dustin Roten2, Ruixue Lei3, Sha Feng4, John C Lin2, Thomas Lauvaux5, Coleen Marie Roehl6 and Tom Oda7, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)University of Utah, Atmospheric Sciences, Salt Lake City, UT, United States, (3)Pennsylvania State University Main Campus, University Park, United States, (4)Pennsylvania State University, Department of Meteorology and Atmospheric Science, University Park, PA, United States, (5)LSCE Laboratoire des Sciences du Climat et de l'Environnement, Gif-Sur-Yvette Cedex, France, (6)California Institute of Technology, Pasadena, CA, United States, (7)Goddard Earth Sciences Research and Technology, Universities Space Research Association, Columbia, United States
Abstract:
The OCO-3 instrument was launched on May 4, 2019 from Kennedy Space Center to the International Space Station. Since August 2019, the instrument has taken measurements of reflected sunlight in three near-infrared bands from which column averaged dry-air mole fractions of carbon dioxide (XCO
2) are derived. The instrument was specifically designed to measure anthropogenic emissions and its snapshot area map (SAM) and target (TG) observational modes allow to scan large contiguous areas (up to 80×80 km
2) on a single overpass over emission hotspots like cities, power plants, or volcanoes. These measurements result in fine-scale spatial maps of XCO
2 unlike what can be done with any other current space-based instrument.
Here, we present and analyze XCO2 distributions over the Los Angeles (LA) megacity derived from multiple OCO-3 TG and SAM mode observations using the vEarly data product. We find that urban XCO2 values are elevated by 2-6 ppm relative to a clean background. The dense, high resolution OCO-3 observations reveal fine-scale, intra-urban variations of XCO2 over the LA megacity that have not been observed from space before.
We further analyze the intra-urban characteristics and compare the XCO2 enhancements observed by OCO-3 with simulated values from two models that can resolve XCO2 variations across the city: an Eulerian (WRF-Chem) and a Lagrangian approach (X-STILT). We show that the observed variations are mainly driven by the complex and highly variable meteorological condition in the LA Basin. Median XCO2 differences between model and observation are typically below 1.3 ppm over the entirety of the LA megacity with slightly larger differences for some sub regions. Further, we find that OCO-3’s multi-swath measurements capture about three times as much of the city emissions compared to single-swath overpasses. In the future, these observations will help to better constrain urban emissions at finer spatiotemporal scales.
