Modelling the development and decay of cryoconite holes in northwestern Greenland

IF 4.4 2区 地球科学 Q1 GEOGRAPHY, PHYSICAL Cryosphere Pub Date : 2023-08-17 DOI:10.5194/tc-17-3309-2023
Y. Onuma, Koji Fujita, N. Takeuchi, M. Niwano, T. Aoki
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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.
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格陵兰岛西北部冰锥洞的发育和衰变模型
摘要冰晶石孔(CH)是一种充满水的圆柱形孔,底部沉积有冰晶石(深色沉积物),形成于世界各地冰川和冰盖的消融表面。由于CH的坍塌可能会将冰锥分散在冰面上,从而降低冰面反照率,因此准确模拟CH深度的时间变化对于理解冰面融化至关重要。我们建立了一个新颖的模型,该模型使用基于孔形几何形状在冰面和CH底部独立计算的热量预算来模拟CH深度的时间变化。我们通过在2012年、2014年和2017年融化季节对格陵兰西北部卡纳克冰盖CH深度的现场观测对该模型进行了评估。该模型再现了观测到的CH坍塌井的深度变化和时间。尽管早期的模型表明,当向下短波辐射强烈时,CH深度往往更深,但我们的灵敏度测试表明,当向下短波辐射的扩散分量占主导时,CH往往形成更深的CH,而当直接分量占主导权时,CH往往较浅。此外,当CH深度大于0.01时,到达CH底部的总热通量主要由通过冰传输的短波辐射控制,而不是直接来自CH口的短波辐射 m。由于通过冰传输的短波辐射可以到达CH底部,而与CH直径无关,因此CH深度不太可能与CH直径相关。这种关系与以前的观测研究一致。此外,模拟强调,冰面和CH底部反照率的差异是再现CH坍塌时间的关键因素。这意味着较低的冰面反照率可能导致CH崩塌,从而导致反照率的进一步降低。热分量分析表明,CH深度由向下短波辐射的扩散分量强度和湍流传热之间的平衡决定。因此,这些气象条件可能是通过甲烷的重新分布导致格陵兰冰盖和其他冰川最近表面变暗的重要因素。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Cryosphere
Cryosphere GEOGRAPHY, PHYSICAL-GEOSCIENCES, MULTIDISCIPLINARY
CiteScore
8.70
自引率
17.30%
发文量
240
审稿时长
4-8 weeks
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.
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