Panels A, B, and C show

,

and

versus

; note the logarithmic scale for

. The initial conditions are

,

,

,

and

. The parameters are as in Table 1 with

and

. The blue line in panel D shows the Fourier power spectrum density of

over a time interval of 3,500 years. The yellow line represents the moving average of the spectrum density. Panels E and F show the global spectral decomposition in Difference-of-Gaussians (DoG) wavelets of stochastic orbits versus

and

, respectively. Each spectrum is an average over 100 wavelet transforms of individual stochastic realizations of the orbit over 3,300 years (this time interval gives 95% confidence to the peaks of each wavelet transform; the fluctuations are due to the stochasticity of the realizations of the model). The color map represents the power scale measured in

. The dotted lines mark the positions of the stochastic realization presented on the left within the corresponding panels.