ULTRAFAST UPWELLING BURSTING THROUGH THE UPPER MANTLE

dc.contributor.authorLarsen T.B.
dc.contributor.authorYuen D.A.
dc.date.accessioned2020-12-14T10:49:46Z
dc.date.available2020-12-14T10:49:46Z
dc.date.issued1997
dc.description.abstractA high-resolution calculation of strongly time-dependent thermal convection in the upper mantle with non-Newtonian, temperature-dependent rheology shows that, for an effective Rayleigh number of around 106, extremely fast upwellings, at times exceeding 10 m/yr, can be generated a few hundred kilometers below the lithosphere. There is a clear separation of timescales between this fast jet and the more slowly convecting mantle. Within this fast vertical shear layer is embedded a thermal boundary layer with a width of the order of 50 km. The development of the fast non-Newtonian upwelling is characterized by the growth of the plume head to a large enough size, before the plume takes off rapidly at a depth of around 350 km. Upon impinging the base of the lithosphere, this fast plume thins the lithosphere and the flow then becomes a horizontally moving hot sheet, extending out for around 1000 km. This scenario is found to repeat itself at the same location about 10 Myr after the first plume impingement.
dc.identifierhttps://elibrary.ru/item.asp?id=267704
dc.identifier.citationEarth and Planetary Science Letters, 1997, , 3, 393-399
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/20766
dc.subjectUPPER MANTLE
dc.subjectUPWELLING
dc.subjectPLUMES
dc.subjectMODELS
dc.subjectCONVECTION
dc.titleULTRAFAST UPWELLING BURSTING THROUGH THE UPPER MANTLE
dc.typeСтатья

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