The two-lobed Lorenz attractor traced as thousands of fine overlapping orbits, projected onto the x–z plane.

Lorenz attractor

Lorenz, 1963. σ = 10, ρ = 28, β = 8/3.

The set every trajectory of the Lorenz equations settles onto: a bounded, non-periodic attractor on which nearby orbits separate exponentially.

Field
Dynamical systems
Nature
Exact computation of a published object; not a Lixiviant result.
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