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Repository of data supporting the results in Daher et al. (JGR, submitted)
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** CONTENT of this part of the repository:

   README_Figure4           This file
   OceanTide_Energies_DissipationRates_ksinchi.mat:
			    Structure containing all of the data in Figure 4 of the paper
                            sidereal rotation periods in hours
                               (4 extra values were used with the 55Ma geometry)
                            KE and APE of M2 and O1 simulations, with all four basin
                               geometries (PD, 55Ma, 116Ma, 252ma), in units of 10^17 Joules
                            Dissipation of M2 and O1 simulations, with all four basin
                               geometries, in units of TW 
                            ksinchi of M2 and O1 simulations, with all four basin geometries

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** 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 4)
   Michael Schindelegger, schindelegger@igg.uni-bonn.de