EGU23-9561, updated on 25 Apr 2023
https://doi.org/10.5194/egusphere-egu23-9561
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

CHAPS: A New, Compact Hyperspectral Imager for Air Pollution Remote Sensing

William Swartz1, Nickolay Krotkov2, Lok Lamsal3,2, Frank Morgan1, Benjamin Stewart1, Walter Zimbeck1, Gerard Otter4, Floris van Kempen4, Pieternel Levelt5, and Pepijn Veefkind6
William Swartz et al.
  • 1Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA (bill.swartz@jhuapl.edu)
  • 2NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
  • 3University of Maryland, Baltimore County, Baltimore, Maryland, USA
  • 4The Netherlands Organization for Applied Scientific Research, Delft, The Netherlands
  • 5National Center for Atmospheric Research, Boulder, Colorado, USA
  • 6Royal Netherlands Meteorological Institute, De Bilt, The Netherlands

Current and planned low Earth orbit and geostationary satellite instruments have long provided global surveys, revealing air pollution characteristics and trends. Targeted pollution observations with even finer spatial and temporal resolution would better characterize, quantify, and monitor emissions from urban areas, power plants, and other anthropogenic activities, with both scientific and societal benefits. The Compact Hyperspectral Air Pollution Sensor (CHAPS) is an imaging spectrometer in a CubeSat form factor, made possible by the use of freeform optics and additive manufacturing. CHAPS has the potential to complement global surveyors and provide targeted observations valuable for understanding air quality at urban scales. The instrument is designed to make measurements of atmospheric composition at 300–500 nm (@ 0.6-nm spectral resolution) at unprecedented spatial resolution from low Earth orbit (1 x 1 km2). The NASA Earth Science Technology Office has funded the development of a CHAPS–Demonstrator (CHAPS-D), which will result in an airborne demonstration of a CHAPS prototype instrument. The CHAPS-D project is a joint collaboration of JHU/APL (USA) and TNO (The Netherlands). CHAPS-D freeform optics derive heritage from the Sentinel-5 Precursor (TROPOMI) mission. Freeform optics has potentially huge advantages over traditional optical designs, including fewer optical surfaces and lower mass and volume, while maintaining optical performance, and CHAPS-D will fit within the design constraints of a 6U CubeSat. The CHAPS-D mechanical structure and some optical elements will be fabricated using additive manufacturing, using a next-generation aluminum alloy. This approach simplifies the construction of the instrument and allows for integral stray light baffling features not possible using traditional fabrication approaches. The compact size and relatively lower cost of CHAPS makes a constellation feasible for the first time, with unprecedented spatiotemporal sampling of global point pollution sources. The project will culminate in an airborne demonstration of CHAPS-D, with 30-m spatial resolution. We will retrieve NO2, SO2, HCHO, ozone, and other trace species relevant to air quality from solar backscatter measurements. We present the science context, measurement requirements, and preliminary design of CHAPS-D, as well as results from breadboard testing.

How to cite: Swartz, W., Krotkov, N., Lamsal, L., Morgan, F., Stewart, B., Zimbeck, W., Otter, G., Kempen, F. V., Levelt, P., and Veefkind, P.: CHAPS: A New, Compact Hyperspectral Imager for Air Pollution Remote Sensing, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-9561, https://doi.org/10.5194/egusphere-egu23-9561, 2023.