Results 151 to 160 of about 2,520 (206)

Crustal to mantle melt storage during the evolution of Hawaiian volcanoes. [PDF]

open access: yesSci Adv
Gazel E   +5 more
europepmc   +1 more source

3D geothermal model of southern Italy based on the Curie isotherm depth. [PDF]

open access: yesSci Rep
Milano M   +4 more
europepmc   +1 more source

Slab melting boosts the mantle wedge contribution to Li-rich magmas. [PDF]

open access: yesSci Rep
Schettino E   +9 more
europepmc   +1 more source

Mantle xenolith perspectives.

open access: yes, 1987
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]

open access: yesEarth and Planetary Science Letters, 2015
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]

open access: yesGeochemistry, Geophysics, Geosystems, 2006
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
Some of the next articles are maybe not open access.

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Murchison xenoliths

Geochimica et Cosmochimica Acta, 1988
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

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