At an equilibrium point of the Rössler system, , , and . Hence
There are two distinct real equilibrium points only if ; they merge if and there are none if . Positivity of alone does not guarantee two. Under the later limits, the nearer one is , while .
The Jacobian matrix of the Rössler system is
At the origin the vertical homogeneous perturbation obeys , so it decays as . Nearby, also relaxes the trajectory toward , close to the – plane. The small fixed-point value of weakly couples planar errors back into ; this is neglected in the requested approximation.
The planar block has trace and determinant , with
For , this is an unstable spiral. Writing and , its linearized trajectories have an envelope proportional to and angular frequency approximately . They rotate counterclockwise: at , . Fast vertical contraction occurs on scale , much shorter than the planar growth scale .
Figure 1.
Counterclockwise outward spiral near the inner Rössler equilibrium
. Details.
Confinement weakens as approaches from below; the approximate vertical relaxation time is , and the quasi-steady value ceases to be small. For , the coefficient of becomes positive, so vertical departures are amplified. The plane is never exactly invariant because there.
Rössler attractor 2026-10-25
A chaotic attractor of a Rössler system for suitable parameter values. Local expansion near an unstable spiral combines with excursions in the third coordinate and global return; the existence of a local expanding direction by itself does not prove a chaotic attractor.