Articles | Volume 25, issue 6
https://doi.org/10.5194/acp-25-3635-2025
https://doi.org/10.5194/acp-25-3635-2025
Research article
 | 
27 Mar 2025
Research article |  | 27 Mar 2025

Did the 2022 Hunga eruption impact the noctilucent cloud season in 2023/24 and 2024?

Sandra Wallis, Matthew DeLand, and Christian von Savigny

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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-2024-2165', Anonymous Referee #1, 17 Oct 2024
    • AC1: 'Reply on RC1', Sandra Wallis, 14 Jan 2025
  • RC2: 'Comment on egusphere-2024-2165', Anonymous Referee #3, 04 Dec 2024
    • AC2: 'Reply on RC2', Sandra Wallis, 14 Jan 2025

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Sandra Wallis on behalf of the Authors (14 Jan 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish subject to technical corrections (15 Jan 2025) by Matthias Tesche
AR by Sandra Wallis on behalf of the Authors (21 Jan 2025)  Author's response   Manuscript 
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Short summary
The 2022 Hunga Tonga – Hunga Ha'apai eruption emitted about 150 Tg H2O that partly reached the upper polar Southern Hemisphere mesosphere in the beginning of 2024. Noctilucent clouds (NLCs) did not show a clear perturbation in their occurrence frequency, but the slight increase from mid-January to February could potentially have been caused by the additional H2O. It needed 2 years to reach the summer polar mesopause region, analogous to the 1883 Krakatoa eruption that is argued to have caused the first sightings of NLCs.
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