New experimental observations on the anhydrous solidus for peridotite KLB‐1

By C. Herzberg, P. Raterron, Jianzhong Zhang. 2000

172 citations recorded by the source corpus.

Subfields: Electronic, Optical and Magnetic Materials, Geophysics

View Paper: https://www.semanticscholar.org/paper/e8d48b53b637bd0d153a88e919061709352ed440

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In Electronic, Optical and Magnetic Materials

In Geophysics

Citations in the corpus

Near-solidus Melting of the Shallow Upper Mantle: Partial Melting Experiments on Depleted Peridotite (2003, background): “total alkali contents of peridotites and their solidus temperatures (Herzberg et al., 2000; Hirschmann, 2000) suggests that, at a given pressure, depleted peridotites will begin to melt at higher temperatures than fertile peridotites.”
Evolution of Helium and Argon Isotopes in a Convecting Mantle: Physics of the Earth and Planetary In (2004, background): “(3), the temperature in some cells may exceed the solidus, which is here based on a fit to experimental data (Zerr et al., 1998; Herzberg et al., 2000)and is composition-independent, except that no melting can occur once the basaltic component has been completely removed (i.”
Thermal and crustal evolution of Mars (2002, background): “Recent experiments on the phase relations of peridotite have provided better constraints on the liquidus and solidus, as well as extending results to higher pressures [Zhang and Herzberg, 1994; Herzberg et al., 2000; Hirschmann, 2000].”
Thermal evolution of the Martian core: Implications for an early dynamo (2004, methodology): “For the initial mantle temperature, we use 2500 K, the mantle solidus at the CMB (Boehler, 1996; Hirschmann, 2000; Herzberg et al., 2000).”
Peridotite melting and mineral–melt partitioning of major and minor elements at 22–24.5 GPa (2002, result): “Although the liquidus temperature determined in our study is slightly lower than that previously determined for KLB-1 [8,9], our inferred solidus temperature is almost identical to that of previous measurements [8,27].”
Evolution of U-Pb and Sm-Nd systems in numerical models of mantle convection and plate tectonics (2004, methodology): “After time-stepping equation (3), the temperature in some cells may exceed the solidus, which is here based on a fit to experimental data [Zerr et al., 1998; Herzberg et al., 2000 ] and is composition-independent, except that no melting can occur once the basaltic component has been completely remo”
PRIMELT3 MEGA.XLSM software for primary magma calculation: Peridotite primary magma MgO contents from the liquidus to the solidus (2015, background): “Our computed anhydrous solidus and its temperature uncertainty are consistent with this experimental database and previous parameterizations [Herzberg et al., 2000; Hirschmann, 2000].”
Internal and tectonic evolution of Mercury (2003, background): “, [41,42]), the iron content of peridotite does not significantly perturb the solidus [43,44].”