A New Equation of State for H2O Ice Ih

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A Gibbs function for seawater thermodynamics for -6 to 80 °C and salinity up to 120gkg-1 (2008, methodology): “(6.28) at SA ¼ 0 and normal pressure is tfpure(0) ¼ 0.002519 1C (Feistel and Wagner, 2006).”
Full numerical simulations of catastrophic small body collisions (2008, methodology): “Hence, we developed a new SESAME table for H2O that includes vapor, liquid, and three solid phases (ices Ih, VI, and VII) that is based on experimentally determined phase boundaries, shock Hugoniots, and thermodynamic properties (Wagner and Pruss 2002; Frank et al. 2004; Stewart and Ahrens 2005; Fei”
Sublimation pressure and sublimation enthalpy of H2O ice Ih between 0 and 273.16 K (2007, methodology): “The Gibbs function of ice is taken from Feistel and Wagner (2006).”
Ab Initio Equation of State Data for Hydrogen, Helium, and Water and the Internal Structure of Jupiter (2007, positive): “For the phases ice I and liquid water we apply accurate data tables named ‘‘FW’’ (Feistel & Wagner 2006) and ‘‘WP’’ (Wagner & Prusz 2002), respectively.”
Impact crater formation in icy layered terrains on Mars (2006, methodology): “The EOS for ice Ih is calculated using the equations given in Feistel and Wagner (2006).”