An autonomous differential equation in three variables. Its linear planar rotation couples to a nonlinear vertical variable through . Depending on parameters, its solutions can approach an equilibrium point, a periodic orbit, or a more complicated attractor. The specialization is used in the 2011 Oxford combined paper.
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.
Articles by others on the same topic
There are currently no matching articles.