Preprints
https://doi.org/10.5194/egusphere-2024-2409
https://doi.org/10.5194/egusphere-2024-2409
02 Aug 2024
 | 02 Aug 2024

OMPS-LP Aerosol Extinction Coefficients And Their Applicability in GloSSAC

Mahesh Kovilakam, Larry Thomason, Magali Verkerk, Thomas Aubry, and Travis Knepp

Abstract. The Global Space-based Stratospheric Aerosol Climatology (GloSSAC) is essential for understanding and modeling the climatic impacts of stratospheric aerosols. It primarily relies on data from the Stratospheric Aerosol Gas Experiment (SAGE) satellite series, supplemented by the Optical Spectrograph and Infrared Imaging System (OSIRIS) and the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO). GloSSAC currently provides stratospheric aerosol extinction coefficients and aerosol optical depths at 525 and 1020 nm. With CALIPSO decommissioned and OSIRIS nearing the end of its operational life, SAGE III/ISS will soon become the sole data source for GloSSAC, but it will only be available as long as the International Space Station (ISS) is operational, around 2030. Therefore, incorporating other measurements, such as those from the Ozone Mapping and Profiler Suite limb profiler (OMPS-LP), is critical. OMPS-LP has provided continuous aerosol extinction coefficient measurements since 2012 with a retrieval algorithm developed by NASA (OMPS(NASA)). However, OMPS(NASA) has been shown to overestimate aerosol extinction coefficients, particularly after the 2022 Hunga Tonga eruption, compared to the tomographic retrieval of OMPS developed by the University of Saskatchewan (OMPS(SASK)) and SAGE III/ISS. Our analysis shows that OMPS(NASA) indeed exhibits a consistently high bias (>50 %) following large volcanic eruptions and pyrocumulonimbus plumes from intense wildfires, while OMPS(SASK) shows reasonable agreement with SAGE III/ISS between 40° S and 40° N. This overestimation by OMPS(NASA) leads to an overestimation of the aerosol effective radiative forcing (ERF) and the associated model-simulated global surface temperature response by about a factor of two.

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Mahesh Kovilakam, Larry Thomason, Magali Verkerk, Thomas Aubry, and Travis Knepp

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2024-2409', Anonymous Referee #1, 24 Sep 2024
  • RC2: 'Comment on egusphere-2024-2409', Anonymous Referee #2, 24 Sep 2024

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2024-2409', Anonymous Referee #1, 24 Sep 2024
  • RC2: 'Comment on egusphere-2024-2409', Anonymous Referee #2, 24 Sep 2024
Mahesh Kovilakam, Larry Thomason, Magali Verkerk, Thomas Aubry, and Travis Knepp
Mahesh Kovilakam, Larry Thomason, Magali Verkerk, Thomas Aubry, and Travis Knepp

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Short summary
The Global Space-based Stratospheric Aerosol Climatology (GloSSAC) is essential for understanding and modeling the climatic impacts of stratospheric aerosols, comprising data from various space-based measurements. Here, we examine and evaluate the Ozone Mapping and Profiler Suite limb profiler (OMPS) against other datasets, particularly SAGE III/ISS, to discern differences and explore the applicability of OMPS data within the GloSSAC framework.