2018 Vol. 45, No. 6
Article Contents

YUAN Fang, XIE Yuanyun, CHI Yunping. 2018. Material characteristics of dust fallouts during the dust-storm weather in Harbin: Constraint on the provenance[J]. Geology in China, 45(6): 1177-1187. doi: 10.12029/gc20180608
Citation: YUAN Fang, XIE Yuanyun, CHI Yunping. 2018. Material characteristics of dust fallouts during the dust-storm weather in Harbin: Constraint on the provenance[J]. Geology in China, 45(6): 1177-1187. doi: 10.12029/gc20180608

Material characteristics of dust fallouts during the dust-storm weather in Harbin: Constraint on the provenance

    Fund Project: Supported by the National Natural Science Foundation of China (No. 41471070)
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  • Author Bio: YUAN Fang, female, born in 1992, master candidate, mainly engages in the study of Asian aeolian dust systems; E-mail: 535038276@qq.com
  • Corresponding author: XIE Yuanyun, male, born in 1971, doctor, professor, mainly engages in teaching and study of Quaternary geology; E-mail: xyy0451@163.com 
  • The dry- and wet-deposited dust depositions of the dust-storm event in Harbin on May 11, 2011 as well as the surface sediments from the potential sources were collected for investigation of grain-size, REE and Sr-Nd isotopic compositions. Some conclusions have been reached:The dry-deposited dusts are marked by bimodal grain-size distributions with fine mode at 3.6 μm and coarse mode at 28 μm whereas the wet-deposited dusts are indicative of unimodal grain-size modes with a fine mode at 6 μm. The grain-size modes for Harbin dust-storm dusts are compatible with CLP loess and Pliocene eolian red clay as well as the eolian dust entrained for a long distance in other regions of the world. These dust- storm depositions have a derivation from distinct sources. There are identical REE patterns and Sr-Nd isotopic compositions for dry- and wet-deposited dusts, suggestive of the derivation from Horqin Sandy Land and, to a certain extent, Onqin Daga Sandy Land. The corresponding Sr- Nd isotopic compositions for dry- and wet-deposited dusts give clues to suggest that fine grains in the CLP loess deposits are expected to be of derivation identical to coarse grains.

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