Articles | Volume 17, issue 7
https://doi.org/10.5194/amt-17-2025-2024
https://doi.org/10.5194/amt-17-2025-2024
Research article
 | 
09 Apr 2024
Research article |  | 09 Apr 2024

Characterization of stratospheric particle size distribution uncertainties using SAGE II and SAGE III/ISS extinction spectra

Travis N. Knepp, Mahesh Kovilakam, Larry Thomason, and Stephen J. Miller

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on amt-2023-207', Chris Boone, 01 Nov 2023
  • RC2: 'Comment on amt-2023-207', Anonymous Referee #2, 09 Nov 2023
  • RC3: 'Comment on amt-2023-207', Anonymous Referee #3, 14 Nov 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Travis N. Knepp on behalf of the Authors (26 Jan 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (29 Jan 2024) by Sandip Dhomse
RR by Chris Boone (13 Feb 2024)
ED: Publish subject to technical corrections (13 Feb 2024) by Sandip Dhomse
AR by Travis N. Knepp on behalf of the Authors (16 Feb 2024)  Author's response   Manuscript 
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Short summary
An algorithm is presented to derive a new SAGE III/ISS (Stratospheric Aerosol and Gas Experiment III on the International Space Station) Level-2 product: the size distribution of stratospheric particles. This is a significant improvement over previous techniques in that we now provide uncertainty estimates for all inferred parameters. We also evaluated the stability of this method in retrieving bimodal distribution parameters. We present a special application to the 2022 eruption of Hunga Tonga.