Fig. 15
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Stability maps in the plane (σ0, a) close to the 3/1 MMR in the presence of the four giant planets with I = 0° (top) and I = 30° (bottom). Each panel is parametrised by a different initial eccentricity, e = 0.3 (left), e = 0.5 (middle), and e = 0.7 (right). The colour scale corresponds to the relative frequency diffusion index in logarithmic scale (Eq. (22)).
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