Crustal structure from the Lutzow-Holm Bay to the inland plateau of East Antarctica, based on onshore gravity surveys and broadband seismic deployments

被引:3
|
作者
Kanao, Masaki [1 ]
Hansen, Samantha E. [2 ]
Kamiyama, Kokichi [1 ]
Wiens, Douglas [3 ]
Higashi, Toshihiro [4 ]
Nyblade, Andrew A. [5 ]
Watanabe, Atsushi [6 ]
机构
[1] Res Org Informat & Syst, Natl Inst Polar Res, Tachikawa, Tokyo 1908518, Japan
[2] Univ Alabama, Dept Geol Sci, Tuscaloosa, AL 35487 USA
[3] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[4] Kyoto Univ, Grad Sch Sci, Dept Geophys, Sakyo Ku, Kyoto 6068502, Japan
[5] Penn State Univ, Dept Geosci, University Pk, PA 16802 USA
[6] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan
基金
美国国家科学基金会;
关键词
Crustal structure; Land gravity survey; Broadband seismic deployments; Lutzow-Holm Bay; Dome-F; Gamburtsev Mountains; TECTONIC IMPLICATIONS; CONTINENTAL-CRUST; MIZUHO PLATEAU; ICE-SHEET; MANTLE; LITHOSPHERE; MOUNTAINS; GONDWANA; VELOCITY; BENEATH;
D O I
10.1016/j.tecto.2012.01.014
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Onshore gravity measurements were conducted over the inland traverse routes from Syowa Station (69.0S, 39.6E; SYO) to Dome-F (77.4 degrees S, 39.6 degrees E) by the Japanese Antarctic Research Expeditions (1992, 1997, and 1998). The crustal density structure between Lutzow-Holm Bay (LHB) and the inland plateau was inferred from Bouguer gravity anomalies along these routes by assuming an initial model of the P-wave structure derived from seismic refraction surveys in the LHB. A decrease in the Bouguer anomalies down to -200 mGal toward the inland plateau indicate that the crust thickens from 38-40 km at LHB to 48-50 km beneath Dome-F. During the International Polar Year in 2007-2008, the GAmburtsev Mountain SEISmic experiment (GAMSEIS) deployed many broadband stations over the large highland on the ice sheet from the crest of the Gambursev Subglacial Mountains (GSM) to the vicinity of Dome-F. S-wave receiver functions and Rayleigh phase velocities determined using the GAMSEIS data indicate that the cratonic crust surrounding the GSM is 40-47 km thick. These thickness estimates agree with those beneath Dome-F from the JARE's gravity surveys and are also consistent with average Pre-Cambrian terrains. Beneath the GSM, the crustal thickness increases to 55-58 km and has been interpreted as providing isostatic compensation for the high mountain elevations. Accordingly, a long-distance crustal model extending over 3000 km from LHB to Dome-F and to the GSM was compiled, providing significant information for future studies of the tectonic evolution of the Antarctic craton. (C) 2012 Elsevier B.V. All rights reserved.
引用
收藏
页码:100 / 110
页数:11
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