2020
DOI: 10.1306/03172017081
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Gravity-flow deposits caused by different initiation processes in a deep-lake system

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Cited by 22 publications
(52 citation statements)
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“…The successive lithofacies changes from facies Cas to facies Sps, facies Mps or facies Ms gradually support the erosional origin. Meanwhile, the erosion processes are also indicated by the obvious erosion contact in the sole of facies Cas and the mixed mud clast with different shapes and colours (Figure 3i) (Yang et al, 2020). Therefore, type B beds are interpreted as the products of sustained high‐density turbidity currents with strong erosion capacity in the relatively proximal part of the flow.…”
Section: Resultsmentioning
confidence: 99%
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“…The successive lithofacies changes from facies Cas to facies Sps, facies Mps or facies Ms gradually support the erosional origin. Meanwhile, the erosion processes are also indicated by the obvious erosion contact in the sole of facies Cas and the mixed mud clast with different shapes and colours (Figure 3i) (Yang et al, 2020). Therefore, type B beds are interpreted as the products of sustained high‐density turbidity currents with strong erosion capacity in the relatively proximal part of the flow.…”
Section: Resultsmentioning
confidence: 99%
“…Gravity flow mainly experiences the transformation from sustained high-density turbidity current to quasisteady low-density turbidity current from the proximal to the distal and lateral edges of the depositional system (Girard et al, 2012;Mulder & Chapron, 2011;Yang et al, 2019Yang et al, , 2020Zavala, 2020) (Figure 14). The strong erosion of sustained high-density turbidity current can form clast-rich argillaceous debris flow deposits (Talling et al, 2012;Talling, Malgesini, & Felletti, 2013;Zavala et al, 2011).…”
Section: The Controlling Of Sediment Supplymentioning
confidence: 99%
“…These clinothems are easy to collapse, controlled by both internal factors (such as rapid progradation) and external factors (earthquake or storm wave reworking) (Clare et al, 2016;Liu et al, 2020). Therefore, many lenticular sediment gravity flow deposits will be caused by sediment failures (Liu et al, 2020;Yang et al, 2019Yang et al, , 2020. These sediment gravity flow deposits are dominated by sandy debrites accompanied by slides and slumps (Liu et al, 2017(Liu et al, , 2020Sztanó et al, 2013;Yang et al, 2019Yang et al, , 2020 (Figure 11c).…”
Section: Depositional Model Of Highstand Sublacustrine Fansmentioning
confidence: 99%
“…Sub‐aqueous sediment gravity flows transport large volumes of sediment, commonly characterised by high proportions of sand, into generally mud‐prone deep‐marine settings (e.g. Bouma, 2000; Heller & Dickinson, 1985; Mutti & Normark, 1987, 1991; Richard et al, 1998; Talling, 2013), and have been shown to have the potential to deposit excellent reservoir‐quality sandstones in deep‐lacustrine settings (Dodd et al, 2019; Yang et al, 2019, 2020). The scale geometry and internal character of deepwater fans can also be used to infer structural information, with different fan systems developing in response to a particular set of characteristics, such as recent fault activity or changes in regional hinterland drainage patterns (Bowman, 1985; Richard et al, 1998).…”
Section: Introductionmentioning
confidence: 99%