DOI: 10.1130/2015.2514(11)
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Seafloor topography and the thermal budget of Earth

Abstract: The subsidence of an aging seafl oor starts to slow down at ∼70 m.y. old with respect to that expected from simple half-space cooling, and this phenomenon has long been known as seafl oor fl attening. The fl attening signal remains even after removal of the infl uence of the emplacement of hotspot islands and oceanic plateaus. The combination of small-scale convection and radiogenic heating has been suggested as a mechanism to explain seafl oor fl attening, and this study explores the possibility of using the … Show more

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Cited by 9 publications
(24 citation statements)
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References 89 publications
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“…In addition to using the plate model, which helps to explain the subsidence of old seafloor, Grose and Afonso [] reduced thermal expansivity to fit the subsidence of young seafloor. We do not adopt the plate model as it hinders our effort to understand seafloor subsidence in a dynamically meaningful manner [ Korenaga , ], and by the same token, we would like to identify physically plausible mechanisms that can explain the discrepancy between the predicted and observed subsidence rates. This will be discussed in the next section.…”
Section: Resultsmentioning
confidence: 99%
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“…In addition to using the plate model, which helps to explain the subsidence of old seafloor, Grose and Afonso [] reduced thermal expansivity to fit the subsidence of young seafloor. We do not adopt the plate model as it hinders our effort to understand seafloor subsidence in a dynamically meaningful manner [ Korenaga , ], and by the same token, we would like to identify physically plausible mechanisms that can explain the discrepancy between the predicted and observed subsidence rates. This will be discussed in the next section.…”
Section: Resultsmentioning
confidence: 99%
“…Seafloor subsidence can also be affected by a slight temperature gradient in the convecting mantle produced by radiogenic heat production [ Korenaga , ]. The amount of heat‐producing elements such as U and Th in the convecting mantle is very small, with the estimate of their total heat production being on the order of 1‐3×10 −12 W kg −1 (equivalent to 4–12 TW for the entire mantle) [ Jochum et al , ; Korenaga , ], which would lead to only <10 K increase over 100 Myr.…”
Section: Resultsmentioning
confidence: 99%
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