PLATE GENERATION IN A SIMPLE MODEL OF LITHOSPHERE-MANTLE FLOW WITH DYNAMIC SELF-LUBRICATION

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dc.contributor.author Bercovici D.
dc.date.accessioned 2020-11-21T07:53:52Z
dc.date.available 2020-11-21T07:53:52Z
dc.date.issued 1996
dc.identifier https://elibrary.ru/item.asp?id=488733
dc.identifier.citation Earth and Planetary Science Letters, 1996, , 1, 41-51
dc.identifier.issn 0012-821X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/19212
dc.description.abstract One of the more enigmatic features of the Earth's style of mantle convection is plate tectonics itself, in particular the existence of strike-slip, or toroidal, motion. Toroidal motion is uncharacteristic of basic thermal convection, but necessarily forms through the interaction of convective flow and nonlinear rheological mechanisms. Recent studies have implied that the empirically determined power-law rheologies of mantle silicates are not sufficient to generate the requisite toroidal motion. A simple source-sink model of mantle or lithospheric flow shows that dynamic self-lubrication, which arises through the coupling of viscous heating and temperature-dependent viscosity, is highly successful at generating strike-slip motion. In particular, as the viscosity of the fluid system becomes more temperature dependent, the toroidal flow field makes an abrupt transition from a state of weak, unplate-like motion to a state with intense and extremely focused structure. In essence, the fluid dynamical model develops strike-slip faults.
dc.subject PLATE TECTONICS
dc.subject PLATES
dc.subject MANTLE
dc.subject CONVECTION
dc.subject VISCOSITY
dc.subject STRIKE-SLIP FAULTS
dc.title PLATE GENERATION IN A SIMPLE MODEL OF LITHOSPHERE-MANTLE FLOW WITH DYNAMIC SELF-LUBRICATION
dc.type Статья


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