Articles | Volume 25, issue 21
https://doi.org/10.5194/acp-25-15453-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
Saharan dust transport event characterization in the Mediterranean atmosphere using 21 years of in-situ observations
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- Final revised paper (published on 12 Nov 2025)
- Supplement to the final revised paper
- Preprint (discussion started on 27 Mar 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-2025-1278', Anonymous Referee #1, 29 Apr 2025
- AC1: 'Reply on RC1', Franziska Vogel, 24 Jul 2025
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RC2: 'Comment on egusphere-2025-1278', Anonymous Referee #2, 03 Jun 2025
- AC2: 'Reply on RC2', Franziska Vogel, 24 Jul 2025
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Franziska Vogel on behalf of the Authors (24 Jul 2025)
Author's response
Author's tracked changes
Manuscript
ED: Referee Nomination & Report Request started (25 Jul 2025) by Marco Gaetani
ED: Publish subject to minor revisions (review by editor) (18 Sep 2025) by Marco Gaetani
AR by Franziska Vogel on behalf of the Authors (08 Oct 2025)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (09 Oct 2025) by Marco Gaetani
AR by Franziska Vogel on behalf of the Authors (09 Oct 2025)
General comment
The manuscript by Vogel et al. (2025) present the analysis of 21 years of optical particle counter (OPC) in-situ observations at the remote Monte Cimone site as an extension of the work by Duchi et al. (2016). The authors analyse the OPC data to provide an estimate of the trend for the annual fractions of dust transport days (DTDs) and PMcoarse, describe the PMcoarse variability compared to background values (enhancement factor) and investigate the correlation between dust events and PMcoarse concentrations.
From a general point of view, although the paper is well written, the analysis could benefit from further refinement and inclusion of additional data sources (i.e. satellite data or reanalysis) and a more accurate and clear presentation of the results (e.g. discussion of measurement uncertainties), which I see as the added value of this work compared to Duchi et al. (2016). I would recommend considering publication once the comments have been adequately addressed.
Specific comments
Minor Comments
- I would rather suggest adding a section in the introduction on aerosol optical depth as a proxy for dust outbreaks, as it represents a more informative parameter compared to surface PM measurements.
- Please consider adding a few sentences describing the structure of the paper at the end of the introduction.
L.37 Please add a reference
L.38 if dust particles remain in the upper layers there will be no increase in the surface PM concentration.
L.76-77 the GRIMM 1.108 starts at 0.3 µm and not at 0.25 µm with the 780 nm operating wavelength
L.81 Please include the number of bins that you consider for the “coarse” mode.
L.92-103 I suggest introducing a list of items instead of the text to identify the different steps of the algorithm.
L.102 how many months are available in 21 years of data?
L.105 Why are back trajectories missing? Due to missing meteorological data?
L.108-110 “consecutive days”, how many consecutive days do you consider? I see it in Figure 1 but it should be written also here.
L.117 Please add more details, which is the average particle density you obtain?
L.138 “user-defined alpha value”, which is?
L.168 replace “merging” by “grouping” and “years” by “DTD yearly values”.
L.168-170 here it could be very interesting to compare with the aerosol optical depth. Your results are consistent with the seasonal cycle in the aerosol optical depth climatology observed for the Po Valley in (Di Antonio et al, 2023) using satellite data.
https://acp.copernicus.org/articles/23/12455/2023/
L.199-200 which is the uncertainty linked to this value?
L.226 Background concentrations are also expected to show diurnal variability in summer compared to winter.
L.218-239 What is the key message then here? What do we learn with the seasonal cycle? It is not very clear to me.
L.242-243 this should go in the methods
L.279 the median is always below the WMO threshold.
L.286-87 I would avoid to make such a suggestion based on the analysis of a single point data source.
L.297-301 I do not fully agree with this statement. On the one hand, dust transport over the Mediterranean basin is generally favoured during the summer months due to the development of a deeper planetary boundary layer (PBL) over the Sahara, on the other hand, it is also strongly influenced by synoptic-scale weather patterns that facilitate such transport. I would rather say that DTE appears to be more closely associated with the persistence of high-pressure systems over the region, rather than directly linked to PBL development over the Sahara. Given the considerable distance from the source areas, the observations primarily reflect atmospheric transport processes rather than continuous Saharan emissions. It may be helpful to investigate reanalysis data to assess whether the occurrence of longer DTEs is associated with more specific stable atmospheric conditions (looking at geopotential height for example).
L.314 aerosol or dust optical depth?
L.314 what do you mean with “reanalysis data from satellites”?
Technical comments
Methods and results can be presented in a clearer way:
- Could you kindly list the different key processes that the dataset has undergone (i.e. Sec. 2.2, 2.3, 2.4) rather than describing them in a block of text?"
- You can summarize major results (such as the average conditions for background/non-background) in tables.
L.40 replace “mineral aerosol” by “dust particles”
L.40 PM “surface” values
Figures: Adding markers to the line can improve the clarity of the plot.
L.263 add space