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拉萨地块保吉地区晚侏罗世——早白垩世地层磁组构特征
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  • 英文篇名:Magnetic fabric study of the Late Jurassic-Early Cretaceous strata in Baoji area of Lhasa block
  • 作者:周亚楠 ; 邵瑞琦 ; 姜南 ; 高扬 ; 于亮 ; 吴汉宁
  • 英文作者:ZHOU Ya'nan;SHAO Ruiqi;JIANG Nan;GAO Yang;YU Liang;WU Hanning;Department of Geology/State Key Laboratory of Continental Dynamics,Northwest University;Institute of Tibetan Plateau Research Chinese Academy Sciences;
  • 关键词:保吉地区 ; 晚侏罗世—早白垩世 ; 吐卡日组 ; 磁组构
  • 英文关键词:Baoji area;;Late Jurassic-Early Cretaceous;;Tukari Formation;;magnetic fabric
  • 中文刊名:地质通报
  • 英文刊名:Geological Bulletin of China
  • 机构:西北大学地质学系/大陆动力国家重点实验室;中国科学院青藏高原研究所;
  • 出版日期:2019-04-15
  • 出版单位:地质通报
  • 年:2019
  • 期:04
  • 基金:国家自然科学基金项目《青藏高原拉萨块体中—晚侏罗世沉积岩与火山岩的古地磁对比研究》(批准号:41702233);《青藏高原晚古生代—早古生代冈瓦纳大陆北界的古地磁研究》(批准号:41674070);《青藏高原羌北地块志留纪至泥盆纪古地理位置的古地磁制》(批准号:41774073);; 陕西省自然科学基础研究计划青年项目《拉萨地块古近纪林子宗群火山岩古地磁学研究》(编号:2017JQ4027)
  • 语种:中文;
  • 页:56-69
  • 页数:14
  • CN:11-4648/P
  • ISSN:1671-2552
  • 分类号:P534.5
摘要
拉萨和羌塘地块拼合形成了青藏高原的核心,但迄今对两者的具体拼合时间仍存在激烈的争论。为进一步寻找约束两者碰撞时限的地质证据,对拉萨地块晚侏罗世—早白垩世地层的磁组构特征进行研究。结果显示:晚侏罗世地层磁组构特征显示其遭遇过较强的构造应力,吐卡日组地层磁化率主轴k_1方位与地层面斜交,但经地层校正后,k_1方位与区域褶皱方向一致,表明应力方位为北北东—南南西向;萨波直不勒组地层k_1方位在地层校正前平行于层面,指示了垂直于主压应力的方向,推断晚侏罗世地层磁组构记录了同一期应力,应力方向均为北北东—南南西向。早白垩世多尼组地层磁组构显示其后期遭受的构造应力场强度弱,且与晚侏罗世应力并非同一期。因此,通过对比晚侏罗世与早白垩世地层的磁组构特征,认为保吉地区晚侏罗世地层磁组构记录了北北东—南南西向较强的构造应力,推断该期应力来源于拉萨-羌塘地块的碰撞拼合事件,而多尼组地层并未受该期应力场的影响,仅记录了区域褶皱隆起时的应力场。
        The Lhasa and Qiangtang blocks are at the heart of the Tibetan Plateau. However, the time for the specific combination of the two blocks is still in heated controversy. To further find geological evidence that can constrain the time limit between the two blocks, the authors studied the characteristics of the magnetic fabric of the Late Jurassic-Early Cretaceous strata in Lhasa block.According to the results obtained, the magnetic structure of Late Jurassic strata encountered strong tectonic stress, and the principal axis k_1 of the magnetic susceptibility of the Tukari Formation was oblique to the ground plane. After the stratigraphic correction, the k_1 azimuth and regional fold direction consensus indicate that the stress azimuth was NNE-SSW; the k_1 orientation of the Sabozhibule Formation was parallel to the plane(NNE-SSW) before the stratigraphic correction, indicating the direction perpendicular to the principal compressive stress and inferring the late tilting. The Late Jurassic formation magnetic structure recorded the same period of stress, and the stress direction was NNE-SSW. The Early Cretaceous Duoni Formation magnetic structure shows that the subsequent tectonic stress field intensity was weak, and was not in the same period as the Late Jurassic stress. Therefore, by comparing the magnetic fabric characteristics of the Late Jurassic and Early Cretaceous strata, the authors concluded that the magnetic fabric of the Late Jurassic in Baoji area recorded a strong tectonic stress in NNE-SSW, and that the stress in this period originated from the LhasaQiangtang block collision event, while the Duoni Formation was not affected by the stress field, only the stress field of the regional fold uplift was recorded.
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