Articles | Volume 17, issue 11
https://doi.org/10.5194/essd-17-6497-2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
Special issue:
In situ surface cloud measurement dataset from four cloud spectrometers during the Pallas Cloud Experiment (PaCE) 2022
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- Final revised paper (published on 26 Nov 2025)
- Preprint (discussion started on 03 Apr 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 essd-2025-163', Anonymous Referee #1, 02 May 2025
- AC1: 'Reply on RC1', Konstantinos Doulgeris, 17 Jun 2025
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RC2: 'Comment on essd-2025-163', Anonymous Referee #2, 18 May 2025
- AC2: 'Reply on RC2', Konstantinos Doulgeris, 17 Jun 2025
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Konstantinos Doulgeris on behalf of the Authors (01 Sep 2025)
Author's response
Author's tracked changes
Manuscript
ED: Publish subject to technical corrections (04 Sep 2025) by Alexander Böhmländer
AR by Konstantinos Doulgeris on behalf of the Authors (05 Sep 2025)
Author's response
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The presented document by Doulgeris et al. (2025) introduces a comprehensive and well-structured dataset of in-situ cloud microphysics measurements collected during the Pallas Cloud Experiment (PaCE) 2022.
The authors provide a clear and detailed overview of the instruments used, including the Cloud Aerosol Spectrometer (CAS), the Forward Scattering Spectrometer Probe (FSSP-100), the Cloud Droplet Analyzer (CDA), and the holographic ICEMET sensor. Particularly noteworthy is the transparent description of instrument characteristics and their respective limitations, such as measurement losses due to icing and alignment issues.
The methodology of data collection and processing, along with accompanying meteorological measurements, is comprehensively described and easy to follow. A central aspect of the document is the detailed quality control, clearly identifying potential sources of error and providing suitable solutions and recommendations for data use, particularly concerning the CAS data due to its fixed orientation.
Issues:
The metadata of the individual instruments could be further expanded (e.g., serial number, calibration values, calibration dates, first installation date, etc.).
To make the dataset more transparent and easier to interpret for future analyses, I suggest introducing a QA flag. This would support the well-documented quality controls and help reduce potential misinterpretations, particularly with regard to CAS and wind direction. One example: 2.November 11:56 – 15:04 Is this gap caused by icing?
The meteorological data from the individual devices differ — for example, the ICE-MET temperature and wind direction are not the same as those in the CDA dataset. Does the CDA dataset include parameters from its internal weather station? This should be clearly stated in the manuscript, as well as in the metadata and the dataset itself.
The ICE-MET dataset contains noticeable LWC outliers that could affect the data when grouped temporally. It is caused by values in the upper bins. Eg. 22. October 3:05 UTC Bin 187
Is there an explanation for that —is it already precipitation?
Nevertheless, the dataset presented constitutes an extremely valuable resource for researchers in the fields of cloud physics, climate research, and meteorology. The careful documentation and provision of data, including uncertainties and boundary conditions, enhance reliability and facilitate their use in future studies.