Y. Onuma, Koji Fujita, N. Takeuchi, M. Niwano, T. Aoki
{"title":"Modelling the development and decay of cryoconite holes in northwestern Greenland","authors":"Y. Onuma, Koji Fujita, N. Takeuchi, M. Niwano, T. Aoki","doi":"10.5194/tc-17-3309-2023","DOIUrl":null,"url":null,"abstract":"Abstract. Cryoconite holes (CHs) are water-filled cylindrical holes with cryoconite (dark-coloured sediment) deposited at their bottoms, forming on ablating\nice surfaces of glaciers and ice sheets worldwide. Because the collapse of CHs may disperse cryoconite on the ice surface, thereby decreasing the\nice surface albedo, accurate simulation of the temporal changes in CH depth is essential for understanding ice surface melt. We established a novel\nmodel that simulates the temporal changes in CH depth using heat budgets calculated independently at the ice surface and CH bottom based on\nhole-shaped geometry. We evaluated the model with in situ observations of the CH depths on the Qaanaaq ice cap in northwestern Greenland during the\n2012, 2014, and 2017 melt seasons. The model reproduced the observed depth changes and timing of CH collapse well. Although earlier models have\nshown that CH depth tends to be deeper when downward shortwave radiation is intense, our sensitivity tests suggest that deeper CH tends to form when\nthe diffuse component of downward shortwave radiation is dominant, whereas CHs tend to be shallower when the direct component is dominant. In\naddition, the total heat flux to the CH bottom is dominated by shortwave radiation transmitted through ice rather than that directly from the\nCH mouths when the CH is deeper than 0.01 m. Because the shortwave radiation transmitted through ice can reach the CH bottom regardless of\nCH diameter, CH depth is unlikely to be correlated with CH diameter. The relationship is consistent with previous observational\nstudies. Furthermore, the simulations highlighted that the difference in albedo between ice surface and CH bottom was a key factor for reproducing\nthe timing of CH collapse. It implies that lower ice surface albedo could induce CH collapse and thus cause further lowering of the albedo. Heat\ncomponent analysis suggests that CH depth is governed by the balance between the intensity of the diffuse component of downward shortwave radiation\nand the turbulent heat transfer. Therefore, these meteorological conditions may be important factors contributing to the recent surface darkening of\nthe Greenland ice sheet and other glaciers via the redistribution of CHs.\n","PeriodicalId":56315,"journal":{"name":"Cryosphere","volume":" ","pages":""},"PeriodicalIF":4.4000,"publicationDate":"2023-08-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Cryosphere","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.5194/tc-17-3309-2023","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOGRAPHY, PHYSICAL","Score":null,"Total":0}
引用次数: 1
Abstract
Abstract. Cryoconite holes (CHs) are water-filled cylindrical holes with cryoconite (dark-coloured sediment) deposited at their bottoms, forming on ablating
ice surfaces of glaciers and ice sheets worldwide. Because the collapse of CHs may disperse cryoconite on the ice surface, thereby decreasing the
ice surface albedo, accurate simulation of the temporal changes in CH depth is essential for understanding ice surface melt. We established a novel
model that simulates the temporal changes in CH depth using heat budgets calculated independently at the ice surface and CH bottom based on
hole-shaped geometry. We evaluated the model with in situ observations of the CH depths on the Qaanaaq ice cap in northwestern Greenland during the
2012, 2014, and 2017 melt seasons. The model reproduced the observed depth changes and timing of CH collapse well. Although earlier models have
shown that CH depth tends to be deeper when downward shortwave radiation is intense, our sensitivity tests suggest that deeper CH tends to form when
the diffuse component of downward shortwave radiation is dominant, whereas CHs tend to be shallower when the direct component is dominant. In
addition, the total heat flux to the CH bottom is dominated by shortwave radiation transmitted through ice rather than that directly from the
CH mouths when the CH is deeper than 0.01 m. Because the shortwave radiation transmitted through ice can reach the CH bottom regardless of
CH diameter, CH depth is unlikely to be correlated with CH diameter. The relationship is consistent with previous observational
studies. Furthermore, the simulations highlighted that the difference in albedo between ice surface and CH bottom was a key factor for reproducing
the timing of CH collapse. It implies that lower ice surface albedo could induce CH collapse and thus cause further lowering of the albedo. Heat
component analysis suggests that CH depth is governed by the balance between the intensity of the diffuse component of downward shortwave radiation
and the turbulent heat transfer. Therefore, these meteorological conditions may be important factors contributing to the recent surface darkening of
the Greenland ice sheet and other glaciers via the redistribution of CHs.
期刊介绍:
The Cryosphere (TC) is a not-for-profit international scientific journal dedicated to the publication and discussion of research articles, short communications, and review papers on all aspects of frozen water and ground on Earth and on other planetary bodies.
The main subject areas are the following:
ice sheets and glaciers;
planetary ice bodies;
permafrost and seasonally frozen ground;
seasonal snow cover;
sea ice;
river and lake ice;
remote sensing, numerical modelling, in situ and laboratory studies of the above and including studies of the interaction of the cryosphere with the rest of the climate system.