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The D Sr fluid / melt data in the haplogranite water system of the present study are larger than those by Borchert et al. (2009, 2010a) at similar pressures.
Two D Pb fluid / melt data points by Bureau et al. (2007) at 0.7 and 0.9 GPa (Figure 4A) were obtained using dilute saline fluids (0.26 M NaCl/kg water), which is discussed later.
D Rb fluid / melt data reported by Borchert et al. (2009, 2010a) are plotted at a lower Dfluid/melt for each pressure than those of the present study, except for a datum at D = 0.22 and 0.7 GPa (Figure 4B).
Because our experimental conditions are relevant to that of the mantle wedge, our D F mineral / melt and D C l mineral / melt data were used to model Cl/F ratio in arc magmas produced by fluid induced melting.
CD melt data from 205 30000 nm were deconvoluted into component spectra using the singular value decomposition procedure in Matlab (The Mathworks), and their statistical significance was calculated based on singular values.
MODIS melt data are not plotted if the gap-filled cloudiness is >11% of the ice sheet area.
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For this, we used last ice melting data to obtain an equivalent wt.% NaCl.
In addition, first ice melting data indicate that the salts dissolved in the inclusions comprise a significant proportion of divalent cations.
Last, we provide a practical section on the use of commercially available software (KaleidaGraph) to fit melting data, along with a consideration of error propagation.
A molten core for the entire evolution is possible if the core contains at least ~5 wt.% of sulfur (Williams and Nimmo 2004), although the more recent Fe FeS melting data of Stewart et al. (2007) suggest a sulfur threshold of at least 10 wt.% or even higher, depending on the efficiency of core cooling (see Fig. 12).
Direct comparisons of observed melting data for TTR/CLU mixtures were also examined.
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