Articles | Volume 42, issue 1
https://doi.org/10.5194/angeo-42-285-2024
© Author(s) 2024. This work is distributed under the Creative Commons Attribution 4.0 License.
On the relationship between the mesospheric sodium layer and the meteoric input function
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- Final revised paper (published on 26 Jun 2024)
- Preprint (discussion started on 17 Jul 2023)
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 angeo-2023-20', Anonymous Referee #1, 05 Aug 2023
- AC1: 'Reply on RC1', Yanlin Li, 16 Sep 2023
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RC2: 'Comment on angeo-2023-20', Anonymous Referee #2, 11 Aug 2023
- AC2: 'Reply on RC2', Yanlin Li, 16 Sep 2023
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
ED: Reconsider after major revisions (further review by editor and referees) (02 Oct 2023) by Hiroatsu Sato
AR by Yanlin Li on behalf of the Authors (04 Oct 2023)
Author's response
Author's tracked changes
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ED: Referee Nomination & Report Request started (09 Oct 2023) by Hiroatsu Sato
RR by Anonymous Referee #1 (09 Oct 2023)
RR by Anonymous Referee #2 (11 Nov 2023)
ED: Reconsider after major revisions (further review by editor and referees) (13 Nov 2023) by Hiroatsu Sato
AR by Yanlin Li on behalf of the Authors (19 Dec 2023)
Author's response
Author's tracked changes
Manuscript
ED: Referee Nomination & Report Request started (15 Jan 2024) by Hiroatsu Sato
RR by Anonymous Referee #1 (20 Jan 2024)
RR by Anonymous Referee #2 (12 Feb 2024)
ED: Publish subject to revisions (further review by editor and referees) (26 Feb 2024) by Hiroatsu Sato
AR by Yanlin Li on behalf of the Authors (06 Mar 2024)
Author's response
Author's tracked changes
Manuscript
ED: Publish subject to revisions (further review by editor and referees) (20 Mar 2024) by Hiroatsu Sato
ED: Referee Nomination & Report Request started (21 Mar 2024) by Hiroatsu Sato
RR by Anonymous Referee #2 (16 Apr 2024)
ED: Publish subject to minor revisions (review by editor) (26 Apr 2024) by Hiroatsu Sato
AR by Yanlin Li on behalf of the Authors (07 May 2024)
Author's response
Author's tracked changes
Manuscript
ED: Publish subject to technical corrections (13 May 2024) by Hiroatsu Sato
AR by Yanlin Li on behalf of the Authors (14 May 2024)
Manuscript
Comments on the paper on the relationship between the mesospheric sodium layer and the meteoric input function.
The paper is a study of a new sodium chemistry model using the continuity equation without making any steady-state assumption. The model includes all sodium-bearing species and runs at a high temporal resolution of millisecond. The study shows the meteor input functions (MIF) from the meteor radiant and derived from the new sodium model. The study could contribute to simulations of sodium concentration in the MLT region.
Some comments that need to be addressed:
1) The authors compared the meteor input functions (MIF) obtained between two types of meteor input function in Figure 6. They should provide more comparison of sodium species between the model and the Colorado State University (CSU) and the Andes Lidar Observatory (ALO), which can present the performance of the model.
2) The authors mentioned the variation by atmospheric dynamics in the discussion. The diurnal sodium profile is the mean of observations of thousands of days, thus the variation by atmospheric dynamics should be much less prominent. As I didn’t see comparison of sodium species between model and lidar observations, the influence of meridional transport of metallic sodium ions and atoms on the seasonal variability of sodium number density in the model cannot be considered less prominent.
3) How long could the model run steadily since the model is not a self-consistent dynamical transport model? What is the global distribution of the sodium species?
4) How did the authors conclude that the uptake of sodium species onto meteoric smoke particles removes approximately three times more than the dimerization of NaHCO3?