| 语境共现(KWIC) |
| , and deepening of the magma ocean as Earth grew. Mantle noble gas isotopic compositions and the mantle ab |
| w. Mantle noble gas isotopic compositions and the mantle abundance of elements that partition into the cor |
| le differentiation appears to have been erased by mantle convection within ?1.5 billion years of Earth for |
| atures similar to those of the present Earth, and mantle melting, and perhaps plate subduction, was produ |
| Earth differentiation may still exist in the deep mantle and continue to influence patterns of large-scale |
| and continue to influence patterns of large-scale mantle convection, sequestration of some trace elements, |
| e for plant-dinosaur coevolutionary interactions. Mantle minerals at shallow depths contain iron in the hi |
| as early as the 1960s, and minerals in the lower mantle were suggested to contain iron in the low-spin st |
| d experiments and calculations prove that iron in mantle minerals transforms from high-spin to low-spin at |
| ls transforms from high-spin to low-spin at lower-mantle pressures. This transition has important conseque |
| dynamics and thermochemical state of the lower mantle, through combined effects on density, elasticity, |
| the physics and chemistry in Earth's lower(most) mantle. Virtually all biotic, dark abiotic, and photoche |
| subduction channel dewatering into the overlying mantle wedge or as the metasomatic replacement by such |
| ost lower crust is less dense than the underlying mantle, but mafic lowermost crust could be unstable and |
| me eclogites and may continue to descend into the mantle, whereas more silica-rich rocks are transformed i |