Results 131 to 140 of about 10,806 (258)
The global distribution of CO<sub>2</sub>-rich magmas is determined by lithospheric thickness. [PDF]
Bowman EE, Gibson SA, Sui S, Lebedev S.
europepmc +1 more source
Abstract This study integrates new zircon U–Pb ages, zircon εHf(t)–δ18O isotopic data, and whole‐rock geochemistry to refine the temporal and spatial framework of magmatism in the southern Northern Andes (SNA) from ∼65 to 6 Ma. The San Lucas, Catamayo, Portachuela, and Gonzanamá batholiths and magmatic suites, along with Late Miocene plutons, display ...
J. Iglesias +14 more
wiley +1 more source
Continental evolution influenced by relamination of deeply subducted continental crust. [PDF]
Gómez-Frutos D +3 more
europepmc +1 more source
Constraining the Permeability and Outer‐Rise Hydration at the Central America Margin
Abstract Subduction zones are important drivers of Earth's geochemical evolution; the presence of water within the subduction system has substantial implications for geohazards, including the style of seismicity and the volume of magma generated at arc volcanoes.
D. Douglas +3 more
wiley +1 more source
Progressive sub-arc mantle oxidation modulated by sediment melt. [PDF]
Gao M, Wang Y, Xu YG.
europepmc +1 more source
Abstract Accurate characterization of the compressional to shear (P‐to‐S) wave‐speed ratio (vp/vs ${v}_{p}/{v}_{s}$) within the Antarctic Ice Sheet (AIS) is crucial for understanding its internal structure, mechanical stability, and vulnerability to a changing climate.
Ammu Sanjayan +2 more
wiley +1 more source
Unveiling the metallogenic continuum of an Archean craton. [PDF]
Demmer M, Ezad I, Fiorentini M.
europepmc +1 more source
Massive Rocky Planets May Suppress Deep Melting
Abstract Melting properties of silicates are critical to understanding the thermal evolution of rocky planetary interiors. In the deep mantles of massive rocky planets, post‐post‐spinel Mg2SiO4 ${\text{Mg}}_{2}{\text{SiO}}_{4}$ is potentially one of the most abundant mineral phases, yet its melting behavior remains unconstrained. Here, we determine the
Donghao Zheng, Yihang Peng, Jie Deng
wiley +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
Abstract The Cenozoic topographic growth of the Iranian Plateau, situated at the Arabia‐Eurasia collision front, provides insights into continental collision dynamics. However, the relative contributions of tectonic shortening versus deep mantle processes to crustal thickening remain debated because systematic quantitative constraints on paleo‐crustal ...
Jun Hu +4 more
wiley +1 more source

