Articles | Volume 17, issue 2
https://doi.org/10.5194/amt-17-783-2024
https://doi.org/10.5194/amt-17-783-2024
Research article
 | 
31 Jan 2024
Research article |  | 31 Jan 2024

Assessing atmospheric gravity wave spectra in the presence of observational gaps

Mohamed Mossad, Irina Strelnikova, Robin Wing, and Gerd Baumgarten

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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-2023-1598', Anonymous Referee #1, 28 Sep 2023
    • AC2: 'Reply on RC1', Mohamed Mossad, 07 Nov 2023
  • RC2: 'Comment on egusphere-2023-1598', Anonymous Referee #2, 06 Oct 2023
    • AC1: 'Reply on RC2', Mohamed Mossad, 07 Nov 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Mohamed Mossad on behalf of the Authors (07 Nov 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (09 Nov 2023) by Lars Hoffmann
RR by Anonymous Referee #2 (24 Nov 2023)
ED: Publish subject to minor revisions (review by editor) (25 Nov 2023) by Lars Hoffmann
AR by Mohamed Mossad on behalf of the Authors (04 Dec 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (10 Dec 2023) by Lars Hoffmann
AR by Mohamed Mossad on behalf of the Authors (18 Dec 2023)  Manuscript 
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Short summary
This numerical study addresses observational gaps' impact on atmospheric gravity wave spectra. Three methods, fast Fourier transform (FFT), generalized Lomb–Scargle periodogram (GLS), and Haar structure function (HSF), were tested on synthetic data. HSF is best for spectra with negative slopes. GLS excels for flat and positive slopes and identifying dominant frequencies. Accurately estimating these aspects is crucial for understanding gravity wave dynamics and energy transfer in the atmosphere.