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Remagnetization of carbonate rocks in southern Tibet: Perspectives from rock magnetic and petrographic investigations

The latitudinal motion of the Tibetan Himalayathe northernmost continental unit of the Indian plateis a key component in testing paleogeographic reconstructions of the Indian plate before the India-Asia collision. Paleomagnetic studies of sedimentary rocks (mostly carbonate rocks) from the Tibetan Himalaya are complicated by potentially pervasive yet cryptic remagnetization. Although traditional paleomagnetic field tests reveal some of this remagnetization, secondary remanence acquired prior to folding or tilting easily escapes detection. Here we describe comprehensive rock magnetic and petrographic investigations of Jurassic to Paleocene carbonate and volcaniclastic rocks from Tibetan Himalayan strata (Tingri and Gamba areas). These units have been the focus of several key paleomagnetic studies for Greater Indian paleogeography. Our results reveal that while the dominant magnetic carrier in both carbonate and volcaniclastic rocks is magnetite, their magnetic and petrographic characteristics are distinctly different. Carbonate rocks have wasp-waisted hysteresis loops, suppressed Verwey transitions, extremely fine grain sizes (superparamagnetic), and strong frequency-dependent magnetic susceptibility. Volcaniclastic rocks exhibit pot-bellied hysteresis loops and distinct Verwey transitions. Electron microscopy reveals that magnetite grains in carbonate rocks are pseudomorphs of early diagenetic pyrite, whereas detrital magnetite is abundant and pyrite is rarely oxidized in the volcaniclastic rocks. We suggest that the volcaniclastic rocks retain a primary remanence, but oxidation of early diagenetic iron sulfide to fine-grained magnetite has likely caused widespread chemical remagnetization of the carbonate units. We recommend that thorough rock magnetic and petrographic investigations are prerequisites for paleomagnetic studies throughout southern Tibet and everywhere in general.

Identiferoai:union.ndltd.org:arizona.edu/oai:arizona.openrepository.com:10150/624349
Date04 1900
CreatorsHuang, Wentao, Lippert, Peter C., Zhang, Yang, Jackson, Michael J., Dekkers, Mark J., Li, Juan, Hu, Xiumian, Zhang, Bo, Guo, Zhaojie, van Hinsbergen, Douwe J. J.
ContributorsUniv Arizona, Dept Geosci, Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China, Department of Geology and Geophysics; University of Utah; Salt Lake City Utah USA, Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China, Institute for Rock Magnetism, Department of Earth Sciences; University of Minnesota, Twin Cities; Minneapolis Minnesota USA, Department of Earth Sciences; Utrecht University; Utrecht Netherlands, School of Earth Sciences and Engineering; Nanjing University; Nanjing China, School of Earth Sciences and Engineering; Nanjing University; Nanjing China, Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China, Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education, School of Earth and Space Sciences; Peking University; Beijing China, Department of Earth Sciences; Utrecht University; Utrecht Netherlands
PublisherAMER GEOPHYSICAL UNION
Source SetsUniversity of Arizona
LanguageEnglish
Detected LanguageEnglish
TypeArticle
Rights©2017. American Geophysical Union. All Rights Reserved.
Relationhttp://doi.wiley.com/10.1002/2017JB013987

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