Articles | Volume 44, issue 1
https://doi.org/10.5194/angeo-44-331-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Studies of noctilucent clouds from the stratosphere during the 2024 TRANSAT balloon flight
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- Final revised paper (published on 18 May 2026)
- Preprint (discussion started on 11 Dec 2025)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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RC1: 'Comment on egusphere-2025-5757', Anonymous Referee #1, 14 Jan 2026
- AC1: 'Reply on RC1', Peter Dalin, 22 Jan 2026
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RC2: 'Comment on egusphere-2025-5757', Anonymous Referee #2, 09 Feb 2026
- AC2: 'Reply on RC2', Peter Dalin, 24 Mar 2026
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) (26 Mar 2026) by Petr Pisoft
AR by Peter Dalin on behalf of the Authors (31 Mar 2026)
Author's response
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ED: Publish subject to minor revisions (review by editor) (13 Apr 2026) by Petr Pisoft
AR by Peter Dalin on behalf of the Authors (17 Apr 2026)
Author's response
Author's tracked changes
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ED: Publish as is (19 Apr 2026) by Petr Pisoft
AR by Peter Dalin on behalf of the Authors (20 Apr 2026)
Review of " Studies of noctilucent clouds from the stratosphere during the 2024 TRANSAT balloon flight " by Peter Dalin et al.
General Comment:
The prime objective of this manuscript is to investigate the dynamics and variability of noctilucent clouds (NLC) through unprecedented stratospheric balloon-based imaging, supported by ground-based lidar and satellite observations. Key results from the comprehensive observations and multi-instrument analysis indicate that NLC were detected nearly continuously over 3.8 days, with their disappearance linked to a localized warm region in the mesopause caused by the intrusion of mid-latitude air. Furthermore, observed double-layer NLC structures moving in opposite directions were consistent with wind shear and inertial-gravity wave activity. Overall, most of the analysis in this manuscript is well executed and the conclusions are well-reasoned. However, the present manuscript has some shortcomings, and that is why the manuscript can be considered for publication after minor revisions from my point of view. I would like to give my comments below that need to be addressed.
Specific Comments: