Articles | Volume 41, issue 2
https://doi.org/10.5194/angeo-41-289-2023
https://doi.org/10.5194/angeo-41-289-2023
Regular paper
 | 
24 Jul 2023
Regular paper |  | 24 Jul 2023

Greenhouse gas effects on the solar cycle response of water vapour and noctilucent clouds

Ashique Vellalassery, Gerd Baumgarten, Mykhaylo Grygalashvyly, and Franz-Josef Lübken

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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 angeo-2023-3', Anonymous Referee #1, 30 Mar 2023
    • AC1: 'Reply on RC1', Ashique Vellalassery, 12 Jun 2023
  • RC2: 'Comment on angeo-2023-3', Anonymous Referee #2, 15 May 2023
    • AC2: 'Reply on RC2', Ashique Vellalassery, 12 Jun 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to minor revisions (review by editor) (12 Jun 2023) by Andrew J. Kavanagh
AR by Ashique Vellalassery on behalf of the Authors (12 Jun 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (13 Jun 2023) by Andrew J. Kavanagh
AR by Ashique Vellalassery on behalf of the Authors (16 Jun 2023)  Author's response   Manuscript 
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Short summary
The solar cycle affects the H2O concentration in the upper mesosphere mainly in two ways: directly through photolysis and, at the time and place of NLC formation, indirectly through temperature changes. The H2O–Lyman-α response is modified by NLC formation, resulting in a positive response at the ice formation region (due to the temperature change effect on the ice formation rate) and a negative response at the sublimation zone (due to the photolysis effect).