Paleomagnetism of the Upper Cretaceous red-beds from the eastern edge of the Lhasa Terrane: New constraints on the onset of the India-Eurasia collision and latitudinal crustal shortening in southern Eurasia
Paleomagnetism of the Upper Cretaceous red-beds from the eastern edge of the Lhasa Terrane: New constraints on the onset of the India-Eurasia collision and latitudinal crustal shortening in southern Eurasia
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拉萨地体东缘上白垩统红层的古地磁:印度-欧亚大陆碰撞发生和欧亚大陆南部地壳纬度缩短的新制约
DOI:
10.1016/j.gr.2017.04.018
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发表时间:
2017-08
影响因子:
6.1
通讯作者:
Zongwen Pu
中科院分区:
文献类型:
--
作者:
Yabo Tong;Zhenyu Yang;Junling Pei;Heng Wang;Yinchao Xu;Zongwen Pu
The Late Cretaceous location of the Lhasa Terrane is important for constraining the onset of India-Eurasia collision. However, the Late Cretaceous paleolatitude of the Lhasa Terrane is controversial. A primary magnetic component was isolated between 580 °C and 695 °C from Upper Cretaceous Jingzhushan Formation red-beds in the Dingqing area, in the northeastern edge of the Lhasa Terrane, Tibetan Plateau. The tilt-corrected site-mean direction isDs/Is= 0.9°/24.3°,k= 46.8,α95= 5.6°, corresponding to a pole ofPlat./Plon.= 71.4°/273.1°, withA95= 5.2°. The anisotropy-based inclination shallowing test of Hodych and Buchan (1994) demonstrates that inclination bias is not present in the Jingzhushan Formation. The Cretaceous and Paleogene poles of the Lhasa Terrane were filtered strictly based on the inclination shallowing test of red-beds and potential remagnetization of volcanic rocks. The summarized poles show that the Lhasa Terrane was situated at a paleolatitude of 13.2° ± 8.6°N in the Early Cretaceous, 10.8° ± 6.7°N in the Late Cretaceous and 15.2° ± 5.0°N in the Paleogene (reference point: 29.0°N, 87.5°E). The Late Cretaceous paleolatitude of the Lhasa Terrane (10.8° ± 6.7°N) represented the southern margin of Eurasia prior to the collision of India-Eurasia. Comparisons with the Late Cretaceous to Paleogene poles of the Tethyan Himalaya, and the 60 Ma reference pole of East Asia indicate that the initial collision of India-Eurasia occurred at the paleolatitude of 10.8° ± 6.7°N, since 60.5 ± 1.5 Ma (reference point: 29.0°N, 87.5°E), and subsequently ~ 1300 ± 910 km post-collision latitudinal crustal convergence occurred across the Tibet. The vast majority of post-collision crustal convergence was accommodated by the Cenozoic folding and thrust faulting across south Eurasia.
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影响因子:
2.8
作者:
Deenen, Martijn H. L.;Langereis, Cor G.;Biggin, Andrew J.
通讯作者:
Biggin, Andrew J.
DOI:
10.1002/2014jb011362
发表时间:
2014-10
期刊:
Journal of Geophysical Research: Solid Earth
影响因子:
--
作者:
Yiming Ma;Tianshui Yang;Zhenyu Yang;Shihong Zhang;Huaichun Wu;Haiyan Li;Huai-kun Li;Weiwei Chen-
通讯作者:
Yiming Ma;Tianshui Yang;Zhenyu Yang;Shihong Zhang;Huaichun Wu;Haiyan Li;Huai-kun Li;Weiwei Chen-
影响因子:
3
作者:
Yabo Tong;Zhenyu Yang;Liang Gao;Heng Wang;Xudong Zhang;Chunzhi An;Yingchao Xu;Z. Han
通讯作者:
Yabo Tong;Zhenyu Yang;Liang Gao;Heng Wang;Xudong Zhang;Chunzhi An;Yingchao Xu;Z. Han
影响因子:
2.9
作者:
R. Voo
通讯作者:
R. Voo
DOI:
--
发表时间:
2010
期刊:
--
影响因子:
--
作者:
Samuel Epstein;Ralph Buchsbaum;Heinz Lowenstam
通讯作者:
Samuel Epstein;Ralph Buchsbaum;Heinz Lowenstam