Articles | Volume 23, issue 7
Research article
05 Apr 2023
Research article |  | 05 Apr 2023

Numerical modelling of relative contribution of planetary waves to the atmospheric circulation

Andrey V. Koval, Olga N. Toptunova, Maxim A. Motsakov, Ksenia A. Didenko, Tatiana S. Ermakova, Nikolai M. Gavrilov, and Eugene V. Rozanov


Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on acp-2022-816', Anonymous Referee #1, 27 Jan 2023
    • AC1: 'Reply on RC1', Andrey Koval, 27 Jan 2023
  • CC1: 'Comment on acp-2022-816', Elena N. Savenkova, 30 Jan 2023
  • RC2: 'Comment on acp-2022-816', Anonymous Referee #2, 28 Feb 2023
    • AC2: 'Reply on RC2', Andrey Koval, 28 Feb 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Andrey Koval on behalf of the Authors (13 Mar 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (13 Mar 2023) by John Plane
AR by Andrey Koval on behalf of the Authors (13 Mar 2023)  Manuscript 
Short summary
Periodic changes in all hydrodynamic parameters are constantly observed in the atmosphere. The amplitude of these fluctuations increases with height due to a decrease in the atmospheric density. In the upper layers of the atmosphere, waves are the dominant form of motion. We use a model of the general circulation of the atmosphere to study the contribution to the formation of the dynamic and temperature regimes of the middle and upper atmosphere made by different global-scale atmospheric waves.
Final-revised paper