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multiple time scale dynamics with two fast variables and one slow ...

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The return map of the Shilnikov model is constructed from <strong>two</strong> comp<strong>one</strong>nts:<br />

the flow map past an equilibrium point, approximated by the flow map of a lin-<br />

ear vector field, composed <strong>with</strong> a regular map that gives a “global return” of<br />

the unstable manifold of the equilibrium to its stable manifold [54]. Place <strong>two</strong><br />

cross-sectionsΣ1 <strong>and</strong>Σ2 moderately close to the equilibrium point <strong>and</strong> model<br />

the flow map fromΣ1 toΣ2 via the linearization of the vector field at the equilib-<br />

rium.<br />

x2<br />

y<br />

x1<br />

R<br />

C0<br />

Figure 5.6: Sketch of the geometric model for the homoclinic bifurcations.<br />

Only parts of the sectionsΣi for i=1, 2 are shown.<br />

The degree <strong>one</strong> coefficient of the characteristic polynomial at the equilibrium<br />

has order O(ǫ), so the imaginary eigenvalues at the Hopf bifurcation point have<br />

magnitude O(ǫ 1/2 ). The real part of these eigenvalues <strong>scale</strong>s linearly <strong>with</strong> the<br />

distance from the Hopf curve. Furthermore we note that the real eigenvalue of<br />

the equilibrium point remains bounded away from 0 asǫ→ 0.<br />

Letψ(x1, x2, y)=(u, v, w) be a coordinate change near q so thatψ(q)=0 <strong>and</strong><br />

the vector field is in Jordan normal form up to higher order terms. We denote<br />

the sections obtained from the coordinate change into Jordan form coordinates<br />

135<br />

ψ<br />

u<br />

v<br />

0<br />

Σ1<br />

w<br />

F12<br />

Σ2<br />

F21

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