Articles | Volume 17, issue 13
https://doi.org/10.5194/amt-17-3995-2024
https://doi.org/10.5194/amt-17-3995-2024
Research article
 | 
05 Jul 2024
Research article |  | 05 Jul 2024

Wind comparisons between meteor radar and Doppler shifts in airglow emissions using field-widened Michelson interferometers

Samuel K. Kristoffersen, William E. Ward, and Chris E. Meek

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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-2023-2369', Anonymous Referee #1, 16 Nov 2023
  • RC2: 'Comment on egusphere-2023-2369', Anonymous Referee #2, 08 Dec 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by William Ward on behalf of the Authors (11 Mar 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (12 Mar 2024) by Jorge Luis Chau
RR by Anonymous Referee #1 (28 Mar 2024)
RR by Anonymous Referee #2 (16 Apr 2024)
ED: Publish subject to technical corrections (16 Apr 2024) by Jorge Luis Chau
AR by William Ward on behalf of the Authors (23 Apr 2024)  Author's response   Manuscript 
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Short summary
In this paper, the relationship between observations from two instruments, a meteor radar and a field-widened Michelson interferometer (ERWIN) which provide complementary information on this region, is investigated. On average the ratio of ERWIN winds to meteor radar winds is ∼ 0.7. Differences between the wind observations may be caused by variations in the airglow brightness associated with dissipating gravity waves.