Results 191 to 200 of about 8,743 (239)

Crustal constraints on the surface expression of mantle upwelling in a back-arc passive margin setting. [PDF]

Sci Rep
Hwang JY, Chang SJ, Sohn YJ, Kim KH.
europepmc   +1 more source

Earth's core-mantle differentiation shaped by water. [PDF]

Sci Adv
Luo H, Zheng D, Deng J.
europepmc   +1 more source

Decadal change of seismic structure in the Earth's lowermost mantle. [PDF]

Nat Commun
Zhang X, Wen L.
europepmc   +1 more source

Electrical and thermal conductivity of Earth's iron-enriched basal magma ocean. [PDF]

Proc Natl Acad Sci U S A
Dragulet F, Stixrude L.
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Mantle Dynamics – A Case Study

2009
Solid state convection in the rocky mantles is a key to understanding the thermochemical evolution and tectonics of terrestrial planets and moons. It is driven by internal heat and can be described by a system of coupled partial differential equations.
Gottschaldt, Klaus, Walzer, U., Stegman, D.R., Baumgardner, J.R., Muhlhaus, Hans B.   +4 more
openaire   +6 more sources

The dynamic mantle

1993
So far, the mantle has been described largely as if it were static; we have been answering questions such as: What is it made of? What changes across the seismic discontinuities? but not: What processes are operating?
G. C. Brown, A. E. Mussett
openaire   +1 more source

Structure and Dynamics of Earth's Lower Mantle

Science, 2008
Processes within the lowest several hundred kilometers of Earth's rocky mantle play a critical role in the evolution of the planet. Understanding Earth's lower mantle requires putting recent seismic and mineral physics discoveries into a self-consistent, geodynamically feasible context.
Edward J, Garnero, Allen K, McNamara
openaire   +2 more sources

Dynamical Processes in the Deeper Mantle

Tectonophysics, 1972
Abstract Runcorn, S.K., 1972. Dynamical processes in the deeper mantle. In: A.R. Ritsema (Editor), The Upper Mantle. Tectonophysics , 13 (1–4): 623–637. That thermal convection occurs in the truly fluid parts of planets is evident and is essential to the understanding of dynamical phenomena in atmospheres and molten cores.
openaire   +2 more sources