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Wang, Youjun, Jia, Jia, Liu, Hao, Lu, Hao, Lu, Caichen, Xia, Dunsheng (2018) Iron mineralogy characteristics of the desert sediments of the Tarim Basin and its provenance implications. Canadian Journal of Earth Sciences, 55 (12) 1384-1388 doi:10.1139/cjes-2018-0105

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Reference TypeJournal (article/letter/editorial)
TitleIron mineralogy characteristics of the desert sediments of the Tarim Basin and its provenance implications
JournalCanadian Journal of Earth Sciences
AuthorsWang, YoujunAuthor
Jia, JiaAuthor
Liu, HaoAuthor
Lu, HaoAuthor
Lu, CaichenAuthor
Xia, DunshengAuthor
Year2018 (December)Volume55
Issue12
PublisherCanadian Science Publishing
DOIdoi:10.1139/cjes-2018-0105Search in ResearchGate
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Mindat Ref. ID485429Long-form Identifiermindat:1:5:485429:0
GUID0
Full ReferenceWang, Youjun, Jia, Jia, Liu, Hao, Lu, Hao, Lu, Caichen, Xia, Dunsheng (2018) Iron mineralogy characteristics of the desert sediments of the Tarim Basin and its provenance implications. Canadian Journal of Earth Sciences, 55 (12) 1384-1388 doi:10.1139/cjes-2018-0105
Plain TextWang, Youjun, Jia, Jia, Liu, Hao, Lu, Hao, Lu, Caichen, Xia, Dunsheng (2018) Iron mineralogy characteristics of the desert sediments of the Tarim Basin and its provenance implications. Canadian Journal of Earth Sciences, 55 (12) 1384-1388 doi:10.1139/cjes-2018-0105
In(2018, December) Canadian Journal of Earth Sciences Vol. 55 (12) Canadian Science Publishing
Abstract/Notes The vast desert area of the Tarim Basin contains a large amount of loose sediment, and consequently, it is one of the most important sources of aeolian dust in the mid-latitudes of the Northern Hemisphere. However, only limited research has been undertaken on the provenance of the desert sediments. In this study, we investigated the iron mineralogy including magnetic (Mt), hematite (Hm), and goethite (Gt) characteristics of desert sediments from the Tarim Basin and used them to determine their provenance. The results show that the sediments are characterized by a high content of Gt that comprises up to 0.16, 0.45, and 0.99 wt.% of the 31–63, 8–31, and 2–8 ΞΌm fractions, respectively. In contrast to Hm and Mt, Gt is significantly enriched in the fine particle size fraction. Consequently, we propose that the desert sediments originate in a cold and humid environment, which favors the formation of Gt and limits the formation of Mt and Hm. The surrounding high mountains appear to be the only location within this vast region with the climatic conditions favoring Gt formation.


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