In a), we present the spectrum of the eccentricity over 65 Myr from the La2010a solution, limited to the interval [0,5′′/yr] (period > 259.2 kyr). In b), the same spectrum is plotted for a solution build with only the 5 main terms of z3 (Table 5). The main peaks are then easily identified and thus also the main peaks of the full eccentricity a).
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