1-D-ice flow modelling at EPICA Dome C and Dome Fuji, East Antarctica

被引:110
作者
Parrenin, F. [1 ]
Dreyfus, G.
Durand, G.
Fujita, S.
Gagliardini, O.
Gillet, F.
Jouzel, J.
Kawamura, K.
Lhomme, N.
Masson-Delmotte, V.
Ritz, C.
Schwander, J.
Shoji, H.
Uemura, R.
Watanabe, O.
Yoshida, N.
机构
[1] CNRS, Lab Glaciol & Geophys Environm, Grenoble, France
[2] Univ Grenoble 1, Grenoble, France
[3] Lab Sci Climat & Environm, Gif Sur Yvette, France
[4] Niels Bohr Inst Astron Phys & Geophys, Copenhagen, Denmark
[5] Natl Inst Polar Res, ROIS, Tokyo 173, Japan
[6] Tohoku Univ, Ctr Atmospher, Sendai, Miyagi 980, Japan
[7] Tohoku Univ, Ocean Studies Grad Sch Sci, Sendai, Miyagi 980, Japan
[8] Univ Bern, Inst Phys, Bern, Switzerland
[9] Kitami Inst Technol, New Energy Resources Res Ctr, Kitami, Hokkaido 090, Japan
[10] Frontier Collaborat Res Ctr, Yokohama, Kanagawa, Japan
关键词
D O I
10.5194/cp-3-243-2007
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
One-dimensional ( 1-D) ice flow models are used to construct the age scales at the Dome C and Dome Fuji drilling sites ( East Antarctica). The poorly constrained glaciological parameters at each site are recovered by fitting independent age markers identified within each core. We reconstruct past accumulation rates, that are larger than those modelled using the classical vapour saturation pressure relationship during glacial periods by up to a factor 1.5. During the Early Holocene, changes in reconstructed accumulation are not linearly related to changes in ice isotopic composition. A simple model of past elevation changes is developed and shows an amplitude variation of 110-120m at both sites. We suggest that there is basal melting at Dome C ( 0.56 +/- 0.19 mm/yr). The reconstructed velocity profile is highly non-linear at both sites, which suggests complex ice flow effects. This induces a non-linear thinning function in both drilling sites, which is also characterized by bumps corresponding to variations in ice thickness with time.
引用
收藏
页码:243 / 259
页数:17
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