CONTINENTAL GROWTH DURING A 1.9-GA SUPERPLUME EVENT

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dc.contributor.author Condie K.C.
dc.date.accessioned 2021-04-19T02:32:54Z
dc.date.available 2021-04-19T02:32:54Z
dc.date.issued 2002
dc.identifier https://www.elibrary.ru/item.asp?id=1094453
dc.identifier.citation Journal of Geodynamics, 2002, 34, 2, 249-264
dc.identifier.issn 0264-3707
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/28054
dc.description.abstract The growth of juvenile continental crust during a possible superplume event at 1.9-Ga occurred chiefly in the form of new arc systems (esp. continental-margin arcs), which were accreted to cratons during supercontinent formation at 1880-1840 Ma. Although oceanic plateaus may have been widespread during the superplume event, they are not a major component of juvenile crust. A possible reason is that they did not attain sufficient thickness to resist subduction during the superplume event. To explain the significant increase in continental growth at 1.9 Ga, recycling rate of continental crust back into the mantle must have decreased relative to the extraction rate of crust from the mantle. A major contributing factor to a decrease in crustal recycling may have been a decrease in sediment subduction rate. Because of a probable high sea level at 1.9 Ga, more sediment was stored on cratons and was not available for subduction.
dc.title CONTINENTAL GROWTH DURING A 1.9-GA SUPERPLUME EVENT
dc.type Статья


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