Articles | Volume 19, issue 4
https://doi.org/10.5194/amt-19-1487-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Validation and comparison of cloud properties retrieved from passive satellites over the Southern Ocean
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- Final revised paper (published on 27 Feb 2026)
- Preprint (discussion started on 19 Feb 2025)
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Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2025-209', Anonymous Referee #1, 30 Mar 2025
- AC1: 'Reply on RC1', Arathy A Kurup, 28 Jul 2025
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RC2: 'Comment on egusphere-2025-209', Anonymous Referee #2, 31 Mar 2025
- AC2: 'Reply on RC2', Arathy A Kurup, 28 Jul 2025
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CC1: 'Comment on egusphere-2025-209', Andrew Heidinger, 03 Apr 2025
- AC3: 'Reply on CC1', Arathy A Kurup, 28 Jul 2025
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AR by Arathy A Kurup on behalf of the Authors (07 Aug 2025)
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ED: Referee Nomination & Report Request started (22 Aug 2025) by Linlu Mei
RR by Anonymous Referee #1 (21 Nov 2025)
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ED: Publish subject to minor revisions (review by editor) (30 Nov 2025) by Linlu Mei
AR by Arathy A Kurup on behalf of the Authors (20 Dec 2025)
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ED: Publish as is (04 Jan 2026) by Linlu Mei
AR by Arathy A Kurup on behalf of the Authors (18 Jan 2026)
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The Southern Ocean is an important area of cloud research and this is a worthwhile inter-comparison. The background in the Introduction is also quite thorough and does a good job of framing this study in a larger context. There are some inconsistencies with the description of the datasets, particularly PATMOS-x, and the collocation process used in Figure 7. In order to have confidence in the results of this inter-comparison these need to be addressed, and at least some of the analysis will need to be redone. Specific comments below.
Line 133: The POES satellites were operated by NOAA so I believe this would typically be NOAA Polar Operational Environmental Satellites (POES).
Line 135: It says here NOAA-19 is used for the L2 comparisons, but in Table 1 it says the cloud optical properties being compared (COD and CER) are derived from the 1.6-micron channel. Channel 3ab on the AVHRR can either measure the 1.6 or 3.75, but not at once. NOAA-19 is switched to 3b, meaning it measures the 3.75, so it shouldn’t be possible to have 1.6-micron properties for CMSAF and PATMOS-x.
Line 146: Here and elsewhere PATMOS should be PATMOS-x
Line 154: For version 6.0 ACHA uses 11 and 13.3 channels, not 11 and 12.
Line 231: I’m a little confused using the term ‘granules’ here. THE AVHRR GAC data is reported in ascending and descending orbits. Is that the meaning of granule here, or is it the global L2b data?
Line 410: retreive -> retrieve
Line 453: CMSAF and PATMOS-x both use AVHRR GAC data so they shouldn’t have different spatial resolutions for L2 products. The sampling may be different, but that’s not the same thing.
Line 603: ‘The AVHRR PATMOS sensors exhibited the lowest correlation and the highest bias in both the overall CTH and the multilayer and single-layer cases.’ The numbers reported in Figure 8 don’t seem to support this conclusion. The PATMOS-x RMSE and MBE is lower than MYD and CMSAF for the multi-layer cases and lower than CMSAF for all cases.
Figure 2.: It seems strange to me that the collocation coverage for CMSAF and PATMOS-x are different since they are derived using the same AVHRR measurements.
I suspect the odd PATMOS-x behavior in Figure 7 can be explained by a collocation problem due to an issue with how the PATMOS-x L2b global file is created. The L2b files are created by sampling orbits for a single day to a 0.1-degree global grid. Final orbits from the previous day are included because the orbit can cross from one day to another. So, if you are looking at the end of the day, and that orbit is missing, you can get a situation where the orbit used is from the previous day (this issue was addressed for recent file deliveries but still exists for most of the record). Below is a list of the orbits used in the NOAA-19 L2b ascending file from January 10th, 2015 (this is from the ‘source’ global attribute in the file). The pertinent files have been italicized. The start and end times in the last two files show a time gap, suggesting an orbit wasn’t processed. This time gap coincides with the start and end times from the first file, which is from January 9th. This gap coincides with the reported collocation time of 22:50 UTC in Figure 7, suggesting the PATMOS-x orbit being analyzed was from a day previous than Cloudsat, MODIS, and CMSAF.
clavrx_NSS.GHRR.NP.D15009.S2214.E0001.B3051617.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15009.S2356.E0146.B3051718.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S0140.E0335.B3051819.SV.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S0329.E0524.B3051920.WI.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S0518.E0711.B3052021.WI.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S0705.E0853.B3052122.WI.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S0847.E1029.B3052223.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S1204.E1351.B3052425.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S1345.E1531.B3052526.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S1525.E1657.B3052627.WI.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S1652.E1836.B3052728.WI.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S1830.E2025.B3052729.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S2019.E2208.B3052930.GC.hirs_avhrr_fusion.level2.nc
clavrx_NSS.GHRR.NP.D15010.S2344.E0134.B3053132.GC.hirs_avhrr_fusion.level2.nc
It's worth reiterating this is an issue with how the PATMOS-x L2b files are created and would be difficult for the authors to identify without looking at imagery to ensure the products are observing the same scenes. Regardless it brings into question the results of Figure 7, and potentially all of the L2 comparison results, depending on how frequently this issue occurs. This should be looked at more carefully.