Articles | Volume 17, issue 11
https://doi.org/10.5194/amt-17-3597-2024
https://doi.org/10.5194/amt-17-3597-2024
Research article
 | 
13 Jun 2024
Research article |  | 13 Jun 2024

Stability requirements of satellites to detect long-term stratospheric ozone trends based upon Monte Carlo simulations

Mark Weber

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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 egusphere-2023-3070', Anonymous Referee #1, 31 Jan 2024
  • RC2: 'Comment on egusphere-2023-3070', Anonymous Referee #2, 19 Feb 2024

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Mark Weber on behalf of the Authors (15 Apr 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (03 May 2024) by Gerrit Kuhlmann
AR by Mark Weber on behalf of the Authors (06 May 2024)
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Short summary
We investigate how stable the performance of a satellite instrument has to be to be useful for assessing long-term trends in stratospheric ozone. The stability of an instrument is specified in percent per decade and is also called instrument drift. Instrument drifts add to uncertainties of long-term trends. From simulated time series of ozone based on the Monte Carlo approach, we determine stability requirements that are needed to achieve the desired long-term trend uncertainty.