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RayleighBenard

Systems / ODEs / Climate & geophysics

A three-mode Saltzman truncation of thermal convection heated from below — the convection family from which the Lorenz attractor descends.

continuous · ODE3 dimensionschaotic

Interactive: drag to rotate

Definition

\[ \begin{aligned} \dot{y_{0}} &= - a y_{0} + a y_{1} \\ \dot{y_{1}} &= r y_{1} - y_{0} y_{2} \\ \dot{y_{2}} &= - b y_{2} + y_{0} y_{1} \end{aligned} \]

Parameters

Symbol Default Role
a 30 Prandtl-like diffusion ratio
b 5 geometric aspect-ratio damping
r 18 reduced Rayleigh number (convective driving)

Properties

Lyapunov spectrum
$+1.933,\; +0.001941,\; -18.94$
computed at build
Kaplan–Yorke dimension
$D_{KY} = 2.102$
Divergence ∇·f
$\nabla\!\cdot f = - a - b + r$
constant
Equilibria
3 equilibria
0 stable · 3 unstable

Define it in TSDynamics

import tsdynamics as ts

sys = ts.systems.RayleighBenard()
traj = sys.integrate(final_time=100.0, dt=0.01)

exps = sys.lyapunov_spectrum()
ts.kaplan_yorke_dimension(exps)

Reference

Yanagita & Kaneko (1995), Physica D 82, 288-313

BibTeX
@misc{rayleighbenard,
  title = {RayleighBenard system},
  note = {Yanagita & Kaneko (1995), Physica D 82, 288-313}
}