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RESEARCH ON THE BASIS OF ACCRETIONARY PRISM FORMATION IN VIEW OF DEFORMATION AND DIAGENESIS OF PELAGIC SEDIMENTS

RESEARCH ON THE BASIS OF ACCRETIONARY PRISM FORMATION IN VIEW OF DEFORMATION AND DIAGENESIS OF PELAGIC SEDIMENTS
远洋沉积物变形与成岩作用下的增生棱柱形成基础研究
批准号:
10304037
负责人:
OGAWA Yujiro
金额:
$18.75万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (A).
财政年份:
1998
资助国家:
日本
项目状态:
已结题
起止时间:
1998 至 2000

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中文摘要
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英文摘要
These three year project on deep-sea sediments (pelagic sediments) has done the research on the process of sedimentation and accretion to the accretionary prism. We mainly focused the project on the mechanism and the role of the pelagic sediments when they are accreted. The main target is the textural change during accretion, particularly how the sediments work during the diagenesis and deformation ; for the original pelagic sediments on the open ocean suffer compaction due to vertical loading, while they get horizontal stress with higher temperature and pressure within the accretionary prisms. The sediments have their own depositional environments and age control, so that the biostratigraphic data by means of microfossils, and provenance determination are also important. In addition the chemical and mineralogical change of the minerals and bulk rocks are also related to the physical change. Many methods were used, but the SEM is above all the most important way to know the texture of … More the sediments. We obtained many results as follows ;The representative pelagic sediment minerals are clays, and they are locally different ; smectite is largely deposited in front of volcanic arcs ; siliceous microfossils are dominant within the pelagic sediments, and they are useful for determination of the ages ; smectite-bearing horizon is most important for the accretionary prism formation ; this zone becomes the decollement (the mechanical boundary) of the prism ; siliceous deposits in the open ocean have only very slow change of texture and chemical/mineralogncal diagenesis, while they vastly change into chert during incorporation into the accretionary prism ; this means the pelagic sediments have the most important role for the formation of the accretionary prism ; pelagic sediments are responsible for the large structures which are characterized by duplex structures ; reconstruction of the accretionary prism need radiolarian biostratigraphy and chromian spinel sandstone petrography. Less
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Ogawa, Y.: "Tectono-stratigraphy of the Glen App area, Southern Uplands, Scotland : anatomy of an Ordovician accretionary complex."Journal of Geological Society (London). vol.155. 651-662 (1998)
小川,Y.:“苏格兰南部高地格伦阿普地区的构造地层学:奥陶纪增生杂岩的解剖学。”地质学会杂志(伦敦)。
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Yamamoto, Y., Otha, Y., and Ogawa, Y.: "Implication for the two-stage layer-parallel faults in the context of the lzu forearc collision zone : examples from the Miura accretionary prism, Central Japan."Tectonophysics. vol.325. 133-144 (2000)
Yamamoto, Y.、Otha, Y. 和 Okawa, Y.:“lzu 弧前碰撞带背景下两阶段层平行断层的含义:日本中部 Miura 增生棱镜的例子。”构造物理学。
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21
    Systematic and precise investigation of beam dynamics in a high-intensity, electron linac for the injector of the B-meson experiment
    Study on the relation between sedimentation and igenous activity in the forearc area.
    • 批准号:
      62420014
    • 项目类别:
      Grant-in-Aid for General Scientific Research (A)
    • 资助金额:
      $12.03万
    • 财政年份:
      1987
    • 负责人:
      OGAWA Yujiro
    • 依托单位:
    海外基金