************************************************************************** Repository of data supporting the results in Daher et al. (JGR, submitted) ************************************************************************** ** CONTENT of this part of the repository: README_Figure2_supporting_information This file WardvsWilliamsEqn_EarthMoonevolutionusingoceantidemodel.mat: Structure containing all of the data in Figure 2 of the supporing information section of the paper which contrasts solutions that employ the Ward (1975) equation for lunar equatorial tilt I vs. the Williams et al. (2001) equation for lunar equatorial tilt I The structure contains the following variables: timestep_Williams/Ward: units Ga Earthrotationperiod_Williams/Ward: units hours obliquity_Williams/Ward: units degrees semimajoraxis_Williams/Ward: units Earth radii eccentricity_Williams/Ward: dimensionless inclination_Williams/Ward: units degrees lunarequatorialtilt_Williams/Ward: units degrees ---------------------------------------------------------------------------- ** REFERENCE: Daher H., Arbic B.K, Williams J.G., Ansong J.K., Boggs D.H., et al. (2021), Long-term Earth-Moon evolution with high-level orbit and ocean tide models, Journal of Geophysical Research Planets, submitted. ** CONTACT: Brian K. Arbic, arbic@umich.edu (Figure 2, supporting information) Michael Schindelegger, schindelegger@igg.uni-bonn.de