Articles | Volume 22, issue 2
Atmos. Chem. Phys., 22, 903–916, 2022
https://doi.org/10.5194/acp-22-903-2022
Atmos. Chem. Phys., 22, 903–916, 2022
https://doi.org/10.5194/acp-22-903-2022

Research article 19 Jan 2022

Research article | 19 Jan 2022

A single-peak-structured solar cycle signal in stratospheric ozone based on Microwave Limb Sounder observations and model simulations

Sandip S. Dhomse 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-2021-663', Anonymous Referee #1, 13 Sep 2021
    • AC1: 'Reply on RC1', Sandip Dhomse, 23 Nov 2021
  • RC2: 'Comment on acp-2021-663', Anonymous Referee #2, 05 Oct 2021
    • AC2: 'Reply on RC2', Sandip Dhomse, 23 Nov 2021

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Sandip Dhomse on behalf of the Authors (23 Nov 2021)  Author's response    Author's tracked changes    Manuscript
ED: Referee Nomination & Report Request started (26 Nov 2021) by Jens-Uwe Grooß
RR by Anonymous Referee #2 (08 Dec 2021)
ED: Publish as is (08 Dec 2021) by Jens-Uwe Grooß
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Short summary
Solar flux variations associated with 11-year sunspot cycle is believed to exert important external climate forcing. As largest variations occur at shorter wavelengths such as ultra-violet part of the solar spectrum, associated changes in stratospheric ozone are thought to provide direct evidence for solar climate interaction. Until now, most of the studies reported double-peak structured solar cycle signal (SCS), but relatively new satellite data suggest only single-peak-structured SCS.
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