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Paleomagnetic analysis of the Marwar Supergroup, Rajasthan, India and proposed interbasinal correlations

机译:印度拉贾斯坦邦的Marwar超群的古地磁分析和拟建的基底间相关性

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摘要

The Marwar Supergroup refers to a 1000-2000 m thick marine and coastal sequence that covers a vast area of Rajasthan in NW-India. The Marwar Basin uncomformably overlies the ~750-770 Ma rocks of the Malani Igneous Suite and is therefore considered Late Neoproterozoic to Early Cambrian in age. Upper Vindhyan basinal sediments (Bhander and Rewa Croups), exposed in the east and separated by the Arav-alli-Delhi Fold Belt, have long been assumed to coeval with the Marwar Supergroup. Recent studies based on detrital zircon populations of the Marwar and Upper Vindhyan sequences show some similarity in the older populations, but the Vindhyan sequence shows no zircons younger than 1000 Ma whereas samples taken from the Marwar Basin show distinctly younger zircons. This observation led to speculation that the Upper Vindhyan and Marwar sequences did not develop coevally. While there are alternative explanations for why the two basins may differ in their detrital zircon populations, paleomagnetic studies may provide independent evidence for differences/similarities between the assumed coeval basins. We have collected samples in the Marwar Basin and present the paleomagnetic results. Previous paleomagnetic studies of Marwar basinal sediments were misinterpreted as being indistinguishable from the Upper Vindhyan sequence. The vast majority of our samples show directional characteristics similar to the previously published studies. We interpret these results to be a recent overprint. A small subset of hematite-bearing rocks from the Jodhpur Formation (basal Marwar) exhibit directional data (Dec = 89° Inc =-1° α95 = 9°) that are distinct from the Upper Vindhyan pole and may offer additional support for temporally distinct episodes of sedimentation in these proximal regions. A VGP based upon our directional data is repotted at 1°S 344°E (dp = 5°, dm = 9°). We conclude that the Marwar Supergroup developed near the close of the Ediacaran Period and is part of a larger group of sedimentary basins that include the Huqf Supergroup (Oman), the Salt-Range (Pakistan), the Krol-Tal belt (Himalayas) and perhaps the Molo Supergroup (Madagascar).
机译:马尔瓦尔超级群(Marwar Supergroup)指的是1000-2000 m厚的海洋和沿海序列,覆盖了印度西北部拉贾斯坦邦的广阔地区。马尔瓦尔盆地不均匀地覆盖了玛拉尼火成岩组的〜750-770 Ma岩石,因此在年龄上被认为是新元古代晚期至早寒武纪。长期以来,人们一直认为上部的Vindhyan盆地沉积物(Bhander和Rewa Croups)在东部暴露并被Arav-alli-Delhi褶皱带分隔开来。基于Marwar和Upper Vindhyan序列的碎屑锆石种群的最新研究表明,在较老的种群中有些相似,但是Vindhyan序列显示没有小于1000 Ma的锆石,而从Marwar盆地采集的样本显示明显较年轻的锆石。这一发现导致人们推测,上Vindhyan和Marwar层序并没有明显发展。虽然对于这两个盆地的碎屑锆石种群为何不同可能有其他解释,但古磁研究可能为假定的古代盆地之间的差异/相似性提供独立的证据。我们已经在马尔瓦尔盆地收集了样本,并提出了古磁结果。先前对马尔瓦尔盆地沉积物的古地磁研究被误解为与上Vindhyan序列无法区分。我们的绝大多数样本都显示出与以前发表的研究相似的方向特征。我们认为这些结果是最近的叠印。来自焦特布尔组(基底马尔瓦尔)的一小块赤铁矿岩表现出的方​​向数据(Dec = 89°Inc = -1°α95= 9°)不同于上Vindhyan极,可能为时间上的不同提供额外的支持这些近端区域的沉积现象。基于我们的方向数据的VGP会在1°S 344°E(dp = 5°,dm = 9°)时重新注入。我们得出的结论是,Marwar超级集团在Ediacaran时期结束时发展起来,并且是更大的沉积盆地群的一部分,包括Huqf超级集团(阿曼),Salt-Range(巴基斯坦),Krol-Tal带(喜马拉雅山)和也许是Molo Supergroup(马达加斯加)。

著录项

  • 来源
    《Journal of Asian earth sciences》 |2014年第9期|339-351|共13页
  • 作者单位

    Department of Geological Sciences, University of Florida, 355 Williamson Hall, Gainesville, Fl 32611, USA,Jackson School of Geosciences, University of Texas-Austin, Austin, TX, USA;

    Department of Geological Sciences, University of Florida, 355 Williamson Hall, Gainesville, Fl 32611, USA;

    Department of Geology, University of Rajasthan, Jaipur 302004, Rajasthan, India;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Gondwana; Paleomagnetism; Purana; India; Marwar; Vindhyan;

    机译:冈瓦纳古罗马主义;神话;印度;马尔瓦尔温迪扬;

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