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Phase equilibrium modelling of partial melting in the upper mantle: A comparison between different modelling methodologies and experimental results by Tahnee Otto; Gary Stevens; Matthew Jason Mayne; Jean-François Moyen is a Earth and Planetary Sciences article available to read on EtoBox.

What is Phase equilibrium modelling of partial melting in the upper mantle: A comparison between different modelling methodologies and experimental results about?

Recent advances in thermodynamic modelling now allow phase equilibrium studies of partial melting in mafic and ultramafic sources under upper mantle conditions. This potentially offers several advantages over experimental investigations, including the fact that capsule-sample interactions are avoided, there is no uncertainty over the volatile content of the charge, the process is much faster, and open system behaviour can be investigated with relative ease. Two different thermodynamic datasets are in common use for phase equilibrium investigations of mantle rocks, compiled alongside a range of constantly evolving phase solution models. This study compares the results of published experimental studies on partial melting in the upper mantle with phase equilibrium modelling results from the popular pMELTS software (Ghiorso et al., 2002), which uses an embedded dataset from Berman (1988), and with results from the Rcrust software (Mayne et al., 2016), which uses the dataset of Holland & Powell (2011). The aim of this comparative study is to investigate the suitability of each combination of software specific calculation routines, thermodynamic datasets and phase solution models to prov

Who reads Phase equilibrium modelling of partial melting in the upper mantle: A comparison between different modelling methodologies and experimental results?

It is typically read by researchers, students, and practitioners in Earth and Planetary Sciences.

Author
Tahnee Otto; Gary Stevens; Matthew Jason Mayne; Jean-François Moyen
Publisher
Elsevier BV
Published
2023
Language
EN
Field
Earth and Planetary Sciences (Physical Sciences)

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