GSTDTAP  > 气候变化
DOI10.1002/2017GL073596
A new heat flux model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic heat production
Burton-Johnson, A.1; Halpin, J. A.2; Whittaker, J. M.2; Graham, F. S.2; Watson, S. J.2
2017-06-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2017
卷号44期号:11
文章类型Article
语种英语
国家England; Australia
英文摘要

A new method for modeling heat flux shows that the upper crust contributes up to 70% of the Antarctic Peninsula's subglacial heat flux and that heat flux values are more variable at smaller spatial resolutions than geophysical methods can resolve. Results indicate a higher heat flux on the east and south of the Peninsula (mean 81mWm(-2)) where silicic rocks predominate, than on the west and north (mean 67mWm(-2)) where volcanic arc and quartzose sediments are dominant. While the data supports the contribution of heat-producing element-enriched granitic rocks to high heat flux values, sedimentary rocks can be of comparative importance dependent on their provenance and petrography. Models of subglacial heat flux must utilize a heterogeneous upper crust with variable radioactive heat production if they are to accurately predict basal conditions of the ice sheet. Our new methodology and data set facilitate improved numerical model simulations of ice sheet dynamics.


Plain Language Summary As the climate changes, the Antarctic ice sheet represents the single largest potential source of sea level rise. However, one key parameter controlling how the ice sheet flows remains poorly constrained: the effect of heat derived from the Earth's geology on the base of the ice sheet (known as subglacial heat flux). Although this may not seem like a lot of heat, under slow-flowing ice, this heat flux can control how well the ice sheet can flow over the rocks and even lead to melting of the ice at its base. Current models for Antarctica's heat flux use geophysics to determine how thin the crust is and consequently how easily heat from the Earth's mantle can warm the surface. We show here that heat produced by radioactive decay within the Earth's crust can have an even greater and much more variable contribution to the subglacial heat flux than estimated by these previous models. We present a new methodology allowing this crustal heat production to be calculated and combined with the geophysical models, producing a new map of heat flux on the Antarctic Peninsula highlighting the variations in heat flux caused by different rock types.


英文关键词heat flux heat flow Antarctica glaciology heat production glaciological modeling
领域气候变化
收录类别SCI-E
WOS记录号WOS:000404382600023
WOS关键词EAST ANTARCTICA ; ICE-SHEET ; SUBGLACIAL LAKES ; WEST ANTARCTICA ; GEOTHERMAL FLUX ; BREAK-UP ; FLOW ; TEMPERATURE ; GONDWANA ; BASIN
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/28791
专题气候变化
作者单位1.British Antarct Survey, Cambridge, England;
2.Univ Tasmania, Inst Marine & Antarct Studies, Hobart, Tas, Australia
推荐引用方式
GB/T 7714
Burton-Johnson, A.,Halpin, J. A.,Whittaker, J. M.,et al. A new heat flux model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic heat production[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(11).
APA Burton-Johnson, A.,Halpin, J. A.,Whittaker, J. M.,Graham, F. S.,&Watson, S. J..(2017).A new heat flux model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic heat production.GEOPHYSICAL RESEARCH LETTERS,44(11).
MLA Burton-Johnson, A.,et al."A new heat flux model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic heat production".GEOPHYSICAL RESEARCH LETTERS 44.11(2017).
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