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Earth’s Structure, Upper Mantle

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Encyclopedia of Solid Earth Geophysics

Part of the book series: Encyclopedia of Earth Sciences Series ((EESS))

Definition

The upper mantle is defined as that part of the mantle between the crust and the phase transition of γ-olivine to perovskite. The total mass of the upper mantle is 1.06 × 1024 kg, about a quarter of the total mass of the mantle. Its volume, 2.95 × 1011 km3, is a third of the total volume of the mantle.

Until the discovery of a major transition near 660-km depth, the upper mantle was better known as Bullen’s “layer B,” extending to 400-km depth. A sharp gradient or discontinuity in seismic velocity causes a bend in the travel time curves of P-wave arrivals near 20°, such that the slowness drops from more than 12 s/deg to 10 s/deg. This phenomenon was observed as early as 1931 by Jeffreys, who correctly adopted a suggestion by J.D. Bernal that it represents a high-pressure modification of olivine. The modern notion of the upper mantle actually extends into Bullen’s next layer, “layer C,” which has now been abandoned as a physically meaningful subdivision.

The depths to the top...

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Nolet, G. (2011). Earth’s Structure, Upper Mantle. In: Gupta, H.K. (eds) Encyclopedia of Solid Earth Geophysics. Encyclopedia of Earth Sciences Series. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-8702-7_44

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