Authors / CoAuthors
Carson, C. | McLaren, S. | Roberts, J. | Boger, S.D. | Blankenship, D.
Abstract
Numerical models are the primary predictive tools for understanding the dynamic behavior of the Antarctic ice sheet. But a key boundary parameter - the magnitude of sub-glacial heat flow - is controlled by geological factors and remains poorly constrained. We show that variations in the abundance and distribution of heat producing elements (U, Th and K) within the Antarctic continental crust give rise to regional sub-glacial heat flows as much as 2-3 times greater than previously assumed in ice modeling studies. We also recognize that, prior to the breakup of Gondwana, much of the East Antarctic continental crust was contiguous with southern Australia where extensive high-heat producing Proterozoic-aged rocks, and correspondingly elevated regional heat flows, are well documented. Such crustal rocks almost certainly extend beneath the modern east Antarctic ice sheet. This means that high sub-glacial heat flows are likely to be a regional phenomenon. Such fundamental geological controls on sub-glacial heat flow must be considered in accurately modelling ice dynamics, permitting more refined predictions of ice mass balance and sea level change.
Product Type
nonGeographicDataset
eCat Id
75002
Contact for the resource
Custodian
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Custodian
Cnr Jerrabomberra Ave and Hindmarsh Dr GPO Box 378
Canberra
ACT
2601
Australia
Keywords
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- External PublicationScientific Journal Paper
- ( Theme )
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- geothermal
- ( Theme )
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- Antarctic data
- ( Theme )
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- antarctica
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- AQ
- Australian and New Zealand Standard Research Classification (ANZSRC)
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- Earth Sciences
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- Published_External
Publication Date
2012-11-15T00:00:00
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unknown
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geoscientificInformation
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[-70, -60, 75, 150]
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Paper describes geothermal heat flow from two areas within the Australian Antarctic Territory, 1) Prydz Bay coastline and 2) George V Land. 75 80 -70 -65