Articles | Volume 26, issue 2
https://doi.org/10.5194/acp-26-1623-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Detection and climatology of Saharan dust frequency and mass at the Jungfraujoch (3580 m a.s.l., Switzerland)
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- Final revised paper (published on 30 Jan 2026)
- Supplement to the final revised paper
- Preprint (discussion started on 03 Sep 2025)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2025-4162', Anonymous Referee #1, 16 Oct 2025
- AC1: 'Reply on RC1', Martine Collaud Coen, 08 Dec 2025
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RC2: 'Comment on egusphere-2025-4162', Anonymous Referee #2, 27 Oct 2025
- AC2: 'Reply on RC2', Martine Collaud Coen, 08 Dec 2025
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AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Martine Collaud Coen on behalf of the Authors (08 Dec 2025)
Author's response
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ED: Publish as is (06 Jan 2026) by Stelios Kazadzis
AR by Martine Collaud Coen on behalf of the Authors (12 Jan 2026)
Manuscript
The interesting article presents a 23-year time series for recording Saharan dust at the Jungfraujoch GAW and ACTRIS station and compares different methods and instrumentation in terms of their characteristics for identifying Saharan dust. Possible conclusions on the climatology of Saharan dust events are presented from a cautious perspective.
The comparisons of methods and instruments are very valuable and underscore the importance of in situ dust detection and characterization.
Overall Comments:
* It is not always clear in the text whether this refers to the complete data set or to data with applied noise thresholds (eg. L 225 ff, L 585 f)
* The article focuses very much on Jungfraujoch data and the role of Mt. Helmos is not clear for the reader
* With regard to the noise threshold values, an evaluation should be carried out to rule out the possibility that this could introduce a certain influence or bias. Since the upper wavelength range (red or IR) will be the decisive criterion for the threshold value in both the nephelometer and the aethalometer (lowest scattering and absorption), a change in the AE also influences whether or not the noise threshold value is exceeded and hence, this might introduce a slight artifact.
Detailed suggestions:
L 109: as far as I know, AE31 measures at different wavelengths: 370, 450, 520, 590, 660, 880 und 950 nm
Diagram 1: The differences in detail are very difficult to identify. For example, AE could be restricted to the range from -2 to 5.
L 266f : The line implies that the hours of Saharan dust at Sonnblick are overestimated. There is no evidence to support this assumption.
L 282 ff: which thresholds were used for Ecotech Nephelometer
L 416: space after comma between February and May
L 445 ff: As mentioned in the article, the Flexpart method also has its issues, and it could also be events that were detected using coarse-mode particle concentration but do not contain Saharan dust at all.
L 571: 24 years or 23 years? I understand the difference between 24 calender years and 23 years time series but you Ok, not important