2010
DOI: 10.1016/j.epsl.2010.10.002
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Geochemical and geophysical estimates of lithospheric thickness variation beneath Galápagos

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Cited by 93 publications
(143 citation statements)
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“…These predictions arise out of the dynamics of mantle flow and melting: the southern edges of the hotspot melting zone are more influenced by EC, where this material is the primary material melting, and the central, north, and northeast side of the hotspot see a relatively greater contribution from DC, where DC and EC are melting at more similar rates (Figures 13.3J-K). An analogous process for creating more depleted compositions between the hotspot center and the ridge axis has been proposed in recent geochemical studies [Hoernle et al, 2000;Gibson and Geist, 2010]. The predicted arc of high 206 Pb/ 204 Pb around the perimeter of the hotspot melting zone crudely resembles the horseshoe shape of the observed isotope pattern around the Galápagos Archipelago (Figure 13.1B).…”
Section: Model 2: High Viscosity In the Shallowest Upper Mantle Withsupporting
confidence: 65%
“…These predictions arise out of the dynamics of mantle flow and melting: the southern edges of the hotspot melting zone are more influenced by EC, where this material is the primary material melting, and the central, north, and northeast side of the hotspot see a relatively greater contribution from DC, where DC and EC are melting at more similar rates (Figures 13.3J-K). An analogous process for creating more depleted compositions between the hotspot center and the ridge axis has been proposed in recent geochemical studies [Hoernle et al, 2000;Gibson and Geist, 2010]. The predicted arc of high 206 Pb/ 204 Pb around the perimeter of the hotspot melting zone crudely resembles the horseshoe shape of the observed isotope pattern around the Galápagos Archipelago (Figure 13.1B).…”
Section: Model 2: High Viscosity In the Shallowest Upper Mantle Withsupporting
confidence: 65%
“…We start with a mantle mineral mode consistent with a fertile lherzolite (ol: 0.55; opx: 0.25; cpx: 0.15; gt: 0.05). The primitive mantle starting composition and chondrite normalization for Lu and Hf are from Sun and McDonough [1989], and partitioning coefficient mineral are from Gibson and Geist [2010] and McKenzie and O'Nions [1991] (Table SI12).…”
Section: Results Of the Major Elements Forward Modelingmentioning
confidence: 99%
“…Partition coefficients were taken from the compilation of ref. 39 and the garnet-spinel transition depth was set from 86-100 km in the model runs, based on the experimental results of ref. 40.…”
Section: Methodsmentioning
confidence: 99%