- A full list of authors appears at the end of the abstract
We present a status overview of the TEMPO mission including its operation, validation and status of baseline data products and upcoming algorithm improvements, implementation of Near-Real-Time (NRT) and other data products.
TEMPO is NASA’s first Earth Venture Instrument (EVI) selected in 2012, and the North America component of the geostationary air quality constellation along with GEMS (launched in Feb. 2020) over Asia and Sentinel-4 (to launch in 2025) over Europe. It is the first spaceborne instrument providing revolutionary hourly daytime air pollution over North America from Mexico City to the Canadian oil sands, and from the Atlantic to the Pacific, at neighborhood scale (~10 km2 at boresight). It uses UV/visible spectroscopy (293-493 nm, 538-741 nm) to measure key elements of tropospheric air pollution chemistry including O3, NO2, HCHO and aerosols, and capture the inherent high variability in the diurnal cycle of emissions and chemistry. TEMPO was successfully launched on board IS-40E into the geostationary orbit at 91°W in April 2023. It conducted its first light Earth observations in early August 2023, kicking off a new era of air quality monitoring from space over North America. It started its nominal operation in October 2023 for a 20-month of baseline Phase E. The baseline mission has been recently extended to September 2026, with further extension via NASA senior reviews. At night, TEMPO can observe city lights, gas flaring, maritime lights from fishing and offshore oil platforms, clouds and snow in the moonlight, lightning, aurorae, and nightglow without interfering with its primary daytime air quality/chemistry mission. Baseline V3 data products were released to the public in May 2024 from NASA’s Atmospheric Science Data Center (ASDC). These data products were upgraded from beta to provisional level in December 2024 after the validation team approval. TEMPO near-real-time (NRT) and other science quality data products were funded by NASA Satellite Needs Working Group (SNWG) to assist in air quality forecasting and modeling efforts and develop better pollution control strategies.
Kevin Daugherty, David Flittner, Juseon Bak, Christopher Brown, Laurel Carpenter, James Carr, Christopher Chan Miller, Ron Cohen, David Edwards, Zachary Fasnacht, Crystal Fenn, Jack Fishman, Lawrence Flynn, Stacey Frith, Jeff Geddes, Dave Haffner, Barron Henderson, Jay Herman, Daniel Jacob, Joanna Joiner, Laura Judd, Emma Knowland, Shobha Kondragunta, Nickolay Krotkov, Can Li, Sergey Marchenko, Nischal Mistra, Aaron Naeger, Robert Neece, Mike Newchurch, Ewan O’Sullivan, Brad Pierce, Wenhan Qin, Prajjwal Rawat, Eric Roback, David Rosenbaum, Colin Seftor, Robert Spurr, Justin Strickland, Jim Szykman, Omar Torres, Luke Valin, Alexander Vasilkov, Jun Wang, Eun-su Yang, Jerry Ziemke, and the TEMPO team
How to cite: Liu, X., Chance, K., Chong, H., Davis, J., Fitzmaurice, J., Gonzalez Abad, G., Houck, J., Hou, W., Nowlan, C., Park, J., Suleiman, R., and Wang, H. and the TEMPO team: A New Era of Air Quality Monitoring from Space over North America with TEMPO: Early Years in Orbit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14388, https://doi.org/10.5194/egusphere-egu25-14388, 2025.