2019
DOI: 10.1016/j.marpetgeo.2018.12.033
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Genesis and depositional model of subaqueous sediment gravity-flow deposits in a lacustrine rift basin as exemplified by the Eocene Shahejie Formation in the Jiyang Depression, Eastern China

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Cited by 47 publications
(54 citation statements)
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“…Debris flows are one kind of sub-aqueous sediment gravity flows, which are caused by excessive sediment density (Yang et al, 2019). They are defined as a laminar plastic flow in which sediment is supported by the matrix strength, grain-to-grain interactions, excess pore fluid pressure, or buoyancy (Talling et al, 2012;Yang et al, 2019).…”
Section: Introductionmentioning
confidence: 99%
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“…Debris flows are one kind of sub-aqueous sediment gravity flows, which are caused by excessive sediment density (Yang et al, 2019). They are defined as a laminar plastic flow in which sediment is supported by the matrix strength, grain-to-grain interactions, excess pore fluid pressure, or buoyancy (Talling et al, 2012;Yang et al, 2019).…”
Section: Introductionmentioning
confidence: 99%
“…Debris flows are one kind of sub-aqueous sediment gravity flows, which are caused by excessive sediment density (Yang et al, 2019). They are defined as a laminar plastic flow in which sediment is supported by the matrix strength, grain-to-grain interactions, excess pore fluid pressure, or buoyancy (Talling et al, 2012;Yang et al, 2019). Although more detailed classifications exist, debris flows can be typically subdivided into two types: sandy (or non-cohesive) debris flows, and muddy (or cohesive) debris flows (Shanmugam, 1996;Talling et al, 2012;Shanmugam, 2000;Yang et al, 2019).…”
Section: Introductionmentioning
confidence: 99%
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“…In contrast to many well-documented sub-marine fan fringe deposits, there is much less information about the sub-lacustrine ones. Lacustrine sediment gravity flow deposits are probably different from marine ones, because marine environments are characterized by larger-scale depositional systems, deeper water, and a longer runout distance (Yang et al 2019). Most sub-lacustrine fan deposits were interpreted mostly as debrites or/and turbidites, including the well-known Eocene Dongying depression and the Upper Triassic turbidites in the Ordos Basin (Zou et al 2012;Liu et al 2017;Yang et al 2017Yang et al , 2019.…”
Section: Introductionmentioning
confidence: 99%
“…A debris flow is a gravity-driven mass flow with plastic rheology and laminar state, it is predominantly supported by the matrix strength, grain-to-grain interactions, excess pore fluid pressure, or buoyancy, and accumulated by en masse settling (Coussot & Meunier, 1996;Locat & Lee, 2005;Naylor, 1980;Qian & Das, 2019;Shanmugam, 2016;Talling, Masson, Sumner, & Malgesini, 2012;Yang, Cao, et al, 2019). Deposits formed by debris flows are termed debrites, which can also be sandy and muddy in composition (Coussot & Meunier, 1996;Locat & Lee, 2005) (Shanmugam, 2016;Talling et al, 2012).…”
Section: Introductionmentioning
confidence: 99%