Oceanic controls on the mass balance of Wilkins Ice Shelf, Antarctica
Oceanic controls on the mass balance of Wilkins Ice Shelf, Antarctica
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DOI:
10.1029/2011jc007301
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发表时间:
2012
影响因子:
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通讯作者:
L. Padman;D. Costa;M. Dinniman;H. Fricker;M. Goebel;Luis A. Hückstädt;A. Humbert;I. Joughin;J. Lenaerts;S. Ligtenberg;T. Scambos;M. Broeke
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文献类型:
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作者:
L. Padman;D. Costa;M. Dinniman;H. Fricker;M. Goebel;Luis A. Hückstädt;A. Humbert;I. Joughin;J. Lenaerts;S. Ligtenberg;T. Scambos;M. Broeke
� 0.8 m a � 1 , driven by a mean basal melt rate of 〈wb〉 = 1.3 � 0.4 m a � 1 . Interannual variability was large, associated with changes in both surface mass accumulation and 〈wb〉. Basal melt rate declined significantly around 2000 from 1.8 � 0.4 m a � 1 for 1992–2000 to � 0.75 � 0.55 m a � 1 for 2001–2008; the latter value corresponding to approximately steady-state ice-shelf mass. Observations of ocean temperature T obtained during 2007–2009 by instrumented seals reveal a cold, deep halo of Winter Water (WW; T ≈ � 1.6°C) surrounding WIS. The base of the WW in the halo is � 170 m, approximately the mean ice draft for WIS. We hypothesize that the transition in 〈wb〉 in 2000 was caused by a small perturbation (� 10–20 m) in the relative depths of the ice base and the bottom of the WW layer in the halo. We conclude that basal melting of thin ice shelves like WIS is very sensitive to upper-ocean and coastal processes that act on shorter time and space scales than those affecting basal melting of thicker West Antarctic ice shelves such as George VI and Pine Island Glacier.