Paleothermal structure of the Nankai inner accretionary wedge estimated from vitrinite reflectance of cuttings
Paleothermal structure of the Nankai inner accretionary wedge estimated from vitrinite reflectance of cuttings
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根据岩屑镜质体反射率估算南开内增生楔的古热结构
DOI:
10.1002/2017gc006928
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发表时间:
2017
期刊:
影响因子:
--
通讯作者:
Ashi Juichiro
中科院分区:
文献类型:
--
作者:
Fukuchi Rina;Yamaguchi Asuka;Yamamoto Yuzuru;Ashi Juichiro
The paleothermal structure and tectonic evolution of an accretionary prism is basic information for understanding subduction zone seismogenesis. To evaluate the entire paleotemperature profile of the Integrated Ocean Drilling Program (IODP) Site C0002 located in the off‐Kumano region of the Nankai Trough and penetrate the inner accretionary wedge down to 3058.5 m below the seafloor (mbsf), we performed a vitrinite reflectance analysis for cuttings and core samples during IODP expeditions 338 and 348: Nankai Trough seismogenic zone experiment. Although vitrinite reflectance values (Ro) tend to increase with depth, two reversals of these values suggested the existence of thrust fault zones with sufficient displacements to offset the paleothermal structure. The estimated maximum paleotemperatures are 42–70°C at 1200–1300 mbsf, 44–100°C at 1600–2400 mbsf, and 56–115°C at 2600–3000 mbsf, respectively. These temperatures roughly coincide with estimated modern temperatures; however, at a smaller scale, the reconstructed partial paleogeothermal gradient (∼60–150°C/km) recorded at the hanging‐ and footwall of the presumed thrust fault zone is higher than the modern geothermal gradient (∼30–40°C/km). This high paleogeothermal gradient was possibly obtained prior to subduction, reflecting the large heat flow of the young Philippine Sea Plate.
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DOI:
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1992
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