EGU25-14437, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-14437
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 30 Apr, 16:15–18:00 (CEST), Display time Wednesday, 30 Apr, 14:00–18:00
 
Hall X4, X4.74
The First Year of the Hyper-Angular Rainbow Polarimeter (HARP2) on the NASA PACE mission: Performance, Science, and Synergy
Brent McBride1,2, J. Vanderlei Martins1,2, Xiaoguang Xu1,2, Anin Puthukkudy1,2, Roberto Fernandez-Borda1,2, Noah Sienkiewicz1, Rachel Smith1, Meng Gao3,4, Bastiaan van Diedenhoven5, Snorre Stamnes6, Kirk Knobelspiesse3, Andrew Sayer2,3, Chamara Rajapakshe3,4, Bryan Franz3, Frederick Patt3,7, Carissa Arillo1,2, Brian Cairns8, Jeremy Werdell3, and Lorraine Remer1,2
Brent McBride et al.
  • 1Earth and Space Institute, University of Maryland Baltimore County, Baltimore, USA
  • 2Goddard Earth Sciences Technology and Research (GESTAR II), Baltimore, USA
  • 3NASA Goddard Space Flight Center, Greenbelt, USA
  • 4Science Systems and Applications, Incorporated, Greenbelt, USA
  • 5Netherlands Institute for Space Research, Leiden, Netherlands
  • 6NASA Langley Research Center, Hampton, USA
  • 7Science Applications International Corporation, Reston, USA
  • 8NASA Goddard Institute for Space Studies, New York, USA

Over the past year, the Hyper-Angular Rainbow Polarimeter (HARP2) multi-angle imaging polarimeter instrument on the NASA Plankton Aerosol Cloud ocean Ecosystem (PACE) mission observed the entire Earth every two days. HARP2 measures total and polarized radiances over four spectral channels (440/550/670/870 nm), at up to 90 distinct viewing directions, and over a 114° field-of-view (1550 km cross-track swath). This large volume of daily information requires new approaches to on-orbit operations, data processing, calibration, and science. In this work, we celebrate and recap the first year of HARP2 on PACE – from pre-launch to on-orbit calibration (solar/lunar/vicarious), exciting new and synergistic science products for cloud, aerosol, and ocean properties, and co-located intercomparisons with OCI, SPEXone, and AirHARP2 underflights during the recent NASA PACE-PAX field campaign. We close with a look ahead to HARP2 as a pathfinder for upcoming polarimetry missions.

How to cite: McBride, B., Martins, J. V., Xu, X., Puthukkudy, A., Fernandez-Borda, R., Sienkiewicz, N., Smith, R., Gao, M., van Diedenhoven, B., Stamnes, S., Knobelspiesse, K., Sayer, A., Rajapakshe, C., Franz, B., Patt, F., Arillo, C., Cairns, B., Werdell, J., and Remer, L.: The First Year of the Hyper-Angular Rainbow Polarimeter (HARP2) on the NASA PACE mission: Performance, Science, and Synergy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14437, https://doi.org/10.5194/egusphere-egu25-14437, 2025.