TY - JOUR A1 - Nishihara, Yu A1 - Ohuchi, Tomohiro A1 - Kawazoe, Takaaki A1 - Spengler, Dirk A1 - Tasaka, Miki A1 - Kikegawa, Takumi A1 - Suzuki, Akio A1 - Ohtani, Eiji T1 - Rheology of fine-grained forsterite aggregate at deep upper mantle conditions JF - Journal of geophysical research : Solid earth KW - high-pressure KW - olivine KW - rheology KW - upper mantle Y1 - 2014 U6 - https://doi.org/10.1002/2013JB010473 SN - 2169-9313 SN - 2169-9356 VL - 119 IS - 1 SP - 253 EP - 273 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Vinnik, Lev A1 - Silveira, Graca A1 - Kiselev, Sergei A1 - Farra, Veronique A1 - Weber, Michael H. A1 - Stutzmann, Eleonore T1 - Cape verde hotspot from the upper crust to the top of the lower mantle JF - Earth & planetary science letters N2 - We investigate the crust, upper mantle and mantle transition zone of the Cape Verde hotspot by using seismic P and S receiver functions from several tens of local seismograph stations. We find a strong discontinuity at a depth of similar to 10 km underlain by a similar to 15-km thick layer with a high (similar to 1.9) Vp/Vs velocity ratio. We interpret this discontinuity and the underlying layer as the fossil Moho, inherited from the pre-hotspot era, and the plume-related magmatic underplate. Our uppermost-mantle models are very different from those previously obtained for this region: our S velocity is much lower and there are no indications of low densities. Contrary to previously published arguments for the standard transition zone thickness our data indicate that this thickness under the Cape Verde islands is up to similar to 30 km less than in the ambient mantle. This reduction is a combined effect of a depression of the 410-km discontinuity and an uplift of the 660-km discontinuity. The uplift is in contrast to laboratory data and some seismic data on a negligible dependence of depth of the 660-km discontinuity on temperature in hotspots. A large negative pressure-temperature slope which is suggested by our data implies that the 660-km discontinuity may resist passage of the plume. Our data reveal beneath the islands a reduction of S velocity of a few percent between 470-km and 510-km depths. The low velocity layer in the upper transition zone under the Cape Verde archipelago is very similar to that previously found under the Azores and a few other hotspots. In the literature there are reports on a regional 520-km discontinuity, the impedance of which is too large to be explained by the known phase transitions. Our observations suggest that the 520-km discontinuity may present the base of the low-velocity layer in the transition zone. KW - hotspot KW - plume KW - crust KW - upper mantle KW - mantle transition zone KW - receiver function Y1 - 2012 U6 - https://doi.org/10.1016/j.epsl.2011.12.017 SN - 0012-821X VL - 319 IS - 4 SP - 259 EP - 268 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Zobir, Soraya Hadj A1 - Oberhänsli, Roland T1 - The sidi Mohamed peridotites (Edough Massif, NE Algeria) - evidence for an upper mantle origin JF - Journal of earth system science N2 - The Hercynian Edough massif is the easternmost crystalline massif of the Algerian coast. It consists of two tectonically superposed units composed of micaschists, gneisses, and peridotite. This study concentrates on the small and isolated Sidi Mohamed peridotite outcrop area (0.03 km(2)). The Sidi Mohamed peridotite is composed mainly of harzburgites (Mg-rich olivine and orthopyroxene as major minerals). The Ni (2051-2920 ppm), Cr (2368-5514 ppm) and MgO (similar to 28-35 wt.%) whole-rock composition and the relative depletion in Nb make these harzburgites comparable to depleted peridotites related to a subduction zone. We suggest that the Sidi Mohamed ultramafic body was derived directly from the upper mantle and tectonically incorporated into the gneiss units of the Edough metamorphic core complex in a subduction environment. KW - Peridotites KW - upper mantle KW - Edough KW - Algeria Y1 - 2013 U6 - https://doi.org/10.1007/s12040-013-0358-z SN - 0253-4126 SN - 0973-774X VL - 122 IS - 6 SP - 1455 EP - 1465 PB - Indian Academy of Science CY - Bangalore ER -