Crustal to mantle melt storage during the evolution of Hawaiian volcanoes. [PDF]
Gazel E +5 more
europepmc +1 more source
Missing molybdenum and the composition of the continental crust inferred from molybdenum isotopes. [PDF]
Tian Y +5 more
europepmc +1 more source
3D geothermal model of southern Italy based on the Curie isotherm depth. [PDF]
Milano M +4 more
europepmc +1 more source
Slab melting boosts the mantle wedge contribution to Li-rich magmas. [PDF]
Schettino E +9 more
europepmc +1 more source
Geochemical data of Al-rich diopside pyroxenites from the Premosello mantle peridotite massif, Ivrea-Verbano Zone, Southern Alps. [PDF]
Ogunyele AC +4 more
europepmc +1 more source
Olivine and Fe-isotopes in kimberlites indicate an iron-rich substrate for CLIPPIR and other sub-lithospheric diamonds. [PDF]
Howarth GH +4 more
europepmc +1 more source
There are records of approx 3500 basaltic xenolith localities and a similar number of kimberlitic occurrences, although actual figures are much greater. The xenoliths group into: spinel-bearing peridotites from alkali basalts from oceanic, circum-oceanic, and young continental (rift) regions; spinel-garnet peridotites from peralkaline basaltic rocks in
Nixon, P. H., Davies, G. R.
core +3 more sources
Frozen melt–rock reaction in a peridotite xenolith from sub-arc mantle recorded by diffusion of trace elements and water in olivine [PDF]
Inferring the ambient state of the lithospheric mantle from xenoliths may be misleading if the magmatic activity responsible for the exhumation has modified the xenolith.
Joerg Hermann, H Şt C O'Neill
exaly +2 more sources
Magmatic processes in developing oceanic crust revealed in a cumulate xenolith collected at the East Pacific Rise, 9°50′N [PDF]
Author Posting. © American Geophysical Union, 2006. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution.
Michael Perfit
exaly +2 more sources
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C3 xenoliths in a C2 host (Murchison) are unique among known meteoritic xenolith-host occurrences. They offer an opportunity to determine possible effects on the xenoliths by the hydrated host. Eleven xenoliths were found ranging from 2 to 13 mm. Four of these Murchison Xenoliths (MX1, MX2, MX3 and MX4) have been studied in detail.
Olsen, Edward J. +5 more
openaire +2 more sources

