the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
A multi-decadal dataset of surface damage on Antarctic ice shelves (1999–2024)
Abstract. Many Antarctic ice shelves have undergone accelerated thinning and retreat in recent decades, weakening their buttressing effect on grounded ice and increasing the risk of further sea-level rise. Surface damage, including crevasses, rifts and heavily fractured areas, is an important indicator of ice shelf structural integrity, but there is limited understanding of its long-term evolution across Antarctic ice shelves. Here we present a new surface damage dataset for nine representative Antarctic ice shelves, derived from Landsat optical imagery covering the period 1999–2024. These ice shelves include Amery, Brunt, Crosson, Dotson, Holmes, Larsen B, Pine Island, Thwaites and Totten, and encompass a range of change behaviours from relatively stable to rapidly changing systems. A deep-learning image segmentation model was trained on a manually annotated dataset from diverse Antarctic ice shelves to automatically map surface damage. To extend the usable record, Landsat 7 scan-line-corrector-off imagery was restored using a diffusion-model-based framework fine-tuned for Antarctic imagery. The final dataset contains 170 surface damage maps at 30 m resolution, each representing a single ice shelf for a specific year. Temporal coverage varies among ice shelves owing to differences in the availability of usable imagery. The model achieved a mean intersection over union of 0.845 on the test set and 0.822 on an independent validation ice shelf not included in model training. The dataset demonstrates good multi-temporal consistency, supporting its use for time-series analysis. Among the nine ice shelves, Pine Island, Thwaites and Larsen B show the most pronounced surface damage changes during the study period. Compared with existing studies, this dataset provides improved temporal continuity over multi-decadal timescales at substantially finer spatial resolution, offering new insights into the long-term evolution of Antarctic ice shelves and contributing to a better understanding of ice shelf instability. The dataset is publicly available at https://doi.org/10.5281/zenodo.20425951 (Tang et al., 2026a).
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Status: final response (author comments only)
- RC1: 'Comment on essd-2026-414', Sepideh Jalayer, 06 Aug 2026
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RC2: 'Comment on essd-2026-414', Ted Scambos, 13 Aug 2026
Review of Tang et al. ESSO --
A multi-decadal dataset of surface damage on Antarctic ice shelves (1999–2024)
The paper presents a potentially useful data set of ice shelf surface damage based on visible-NIR imagery and a machine-learning approach to detecting the surface features indicating damage. The paper is well-written, virtually zero issues with English or grammar, and could be considered publishable as it is, with proper qualification.
But. Ice shelf damage comes in three types: surface damage, (a) rifts and (b) crevasses, and (c) basal fractures. All three weaken shelves, but in differing ways that would be important to modelers seeking to use your data set to explore various ice shelf vulnerabilities. So, while the data set might be valid within the scope of what has been done, and the title, it would be hard to implement for the most logical application(s).
The authors detect surface damage on the basis of sharp linear breaks in pixel brightness – what are the sources of false positives here? Frost patches can produce linear breaks in brightness, were these detected? Please include more of discussion of the false positives, negatives, etc. – what were the causes of these?
In several of the maps of results you _are_ showing surface damage above bottom crevasses, and this stems from surface ruptures initiated by deformation around bottom crevassing (there are many papers to cite here – one is by McGrath for the Larsen C). This is very prevalent on Scar Inlet (your ‘Larsen B’ test area) and the northeastern Larsen C, as well as in the floating parts of Thwaites Western Ice Tongue. This kind of damage is especially common where the ice is thick (in other words, where buoyancy and lateral deformation forces are large).
It would be interesting to consider how to modify the algorithm or segmentation pre-processing to facilitate bottom crevasse detection. This would likely involve a larger cluster of pixels in the segmentation regions and inclusion ice thickness mappings for scaling the detection of the surface undulations that mark bottom crevasses. There are also notable differences in bottom crevasse surface manifestations between warm-water cavities (Bellingshausen-Amundsen Sea coasts) having to do with basal erosion due to melting.
A little more detail on what was manually identified as surface damage would be good to describe. This might only require a few sentences in Section 2.3.1.
In your temporal consistency checks (Section 3.2.5 and 3.3), did you look for seasonal variations in damage extent or detectability? Seasonal variations in snow bridging of crevasses should lead to some reduced evidence of damage in spring, greater evidence in winter (you are close to evaluating this in your Figure 10). ALSO, importantly, was the algorithm affected by solar illumination angle? Low angle autumn images may well reveal more extensive areas exceeding the damage threshold. Further to this --- areas of extremely rough sastrugi might trigger the algorithm to map surface damage. You could look in some key areas of east Antarctica where meter-scale perennial sastrugi form as a test of the algorithm.
Minor comments
In several places, you refer to the remnant Larsen B ice shelf. Consider instead describing this as ‘Scar Inlet Ice Shelf’, as nearly all of the remnant Larsen B is within this ice-shelf-filled bay.
Line 52, cite Scambos et al. (2007) or Haran et al. (NSIDC) for the MOA mosaics. Note, you might also explore the LIMA mosaic (Bindschadler et al.) and RAMP (Jezek et al.) because these are uniformly processed they make a good template for your algorithm. More importantly – run your processing on the REMA mosaic. These different mosaics (esp LIMA and REMA) will establish better baselines for your surface damage processing time-series.
Line 133 – picky, but don’t say ‘austral summer’, say ‘sunlit season’ or similar.
Figure 7 – what is the scale of these image chips? More generally, it would be good to see a close-up view of a test area to see -exactly- what the algorithm is mapping.
Very minor note – I found the lack of spacing or indentation on the paragraphs and the references to be an impediment to quick reading and checking. I suggest adopting some kind of structure to facilitate a quicker scan.
McGrath, D., Steffen, K., Scambos, T., Rajaram, H., Casassa, G. and Lagos, J.L.R., 2012. Basal crevasses and associated surface crevassing on the Larsen C ice shelf, Antarctica, and their role in ice-shelf instability. Annals of glaciology, 53(60), pp.10-18.
Ted Scambos, Senior Research Scientist, ESOC / CIRES
University of Colorado, Boulder
Citation: https://doi.org/10.5194/essd-2026-414-RC2
Data sets
Surface Damage Dataset for Antarctic Ice Shelves 1999–2024 Leyue Tang, Jonathan L. Bamber, Tian Li, and Gang Qiao https://doi.org/10.5281/zenodo.20425951
Model code and software
Surface Damage Segmentation Leyue Tang https://github.com/tly-code/surface-damage-seg
Interactive computing environment
Jupyter notebooks for temporal variation analysis Leyue Tang https://github.com/tly-code/surface-damage-seg
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This manuscript presents a valuable Antarctic ice shelf surface damage dataset. However, several parts of the methodology, model evaluation, validation and dataset description need to be explained more clearly. The following comments need to be addressed before the manuscript can be considered for publication.
In this study, quantifying data uncertainty is particularly important because it can help identify label noise, inherent image noise and uncertainties in the manual annotations.