Articles | Volume 22, issue 6
Atmos. Chem. Phys., 22, 4187–4200, 2022
https://doi.org/10.5194/acp-22-4187-2022
Atmos. Chem. Phys., 22, 4187–4200, 2022
https://doi.org/10.5194/acp-22-4187-2022
Research article
31 Mar 2022
Research article | 31 Mar 2022

Evolution of the intensity and duration of the Southern Hemisphere stratospheric polar vortex edge for the period 1979–2020

Audrey Lecouffe et al.

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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 acp-2021-676', Anonymous Referee #1, 08 Oct 2021
    • AC1: 'Reply on RC1', Audrey Lecouffe, 26 Jan 2022
  • RC2: 'major revisions required', Anonymous Referee #2, 20 Oct 2021
    • AC2: 'Reply on RC2', Audrey Lecouffe, 26 Jan 2022

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Audrey Lecouffe on behalf of the Authors (26 Jan 2022)  Author's response    Author's tracked changes    Manuscript
ED: Referee Nomination & Report Request started (12 Feb 2022) by Peter Haynes
RR by Anonymous Referee #1 (15 Feb 2022)
ED: Publish subject to technical corrections (21 Feb 2022) by Peter Haynes
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Short summary
This study uses a model developped at LATMOS (France) to analyze the behavior of the Antarctic polar vortex from 1979 to 2020 at 675 K, 550 K, and 475 K isentropic levels. We found that the vortex edge intensity is stronger during the September–October–November period, while its edge position is less extended during this period. The polar vortex is stronger and lasts longer during solar minimum years. Breakup dates of the polar vortex are linked to the ozone hole and maximum wind speed.
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