Lorenz attractor

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A plot of the trajectory Lorenz system for values ρ=28, σ = 10, β = 8/3

The Lorenz attractor, named for Edward N. Lorenz, is a structure (a so-called strange attractor) that arises in the study of the Lorenz Oscillator, a 3-dimensional dynamical system that exhibits chaotic flow. The Lorenz attractor is noted for its figure eight shape.

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[edit] Overview

In 1963, Edward Lorenz developed a simplified mathematical model for convection rolls arising in the atmosphere. His model is known as the Lorenz Oscillator and the equations are known as the Lorenz Equations. The Lorenz Equations also arise in simplified models for lasers (Haken 1975) and dynamos (Knobloch 1981).

A trajectory of Lorenz's equations, rendered as a metal wire to show direction and 3D structure

From a technical standpoint, the Lorenz oscillator is nonlinear, three-dimensional and deterministic. For a certain set of parameters, the system exhibits chaotic behavior and displays what is today called a strange attractor. The strange attractor in this case is a fractal of Hausdorff dimension between 2 and 3. Grassberger (1983) has estimated the Hausdorff dimension to be 2.06 ± 0.01 and the correlation dimension to be 2.05 ± 0.01.

It's important to note that not all initial states converge to the Lorenz attractor. (See below for more details.)

While the behavior of the Lorenz Oscillator is of mathematical interest, one should be careful in drawing conclusions about the behavior of real-world systems modeled by the Lorenz Equations.

[edit] Equations

Trajectory with scales added

The equations that govern the Lorenz oscillator (known as the Lorenz Equations) are:

\frac{dx}{dt} = \sigma (y - x)
\frac{dy}{dt} = x (\rho - z) - y
\frac{dz}{dt} = xy - \beta z

where \sigma is called the Prandtl number and \rho is called the Rayleigh number. All \sigma, \rho, \beta > 0, but usually \sigma = 10, \beta = 8/3 and \rho is varied. The system exhibits chaotic behavior for \rho = 28 but displays knotted periodic orbits for other values of \rho. For example, with \rho = 99.96 it becomes a T(3,2) torus knot.

A Saddle-node bifurcation occurs at \beta(\rho-1)=0. When σ ≠ 0 and β (ρ-1) ≥ 0, the equations generate three critical points. The critical points at (0,0,0) correspond to no convection, and the critical points at (\pm\sqrt{\beta(\rho-1)}, \pm\sqrt{\beta(\rho-1)}, \rho-1) correspond to steady convection. This pair is stable only if \rho< \sigma\frac{\sigma+\beta+3}{\sigma-\beta-1}, which can hold only for positive \rho if \sigma > \beta+1.

Sensitive dependence on the initial condition
Time t=1 (Enlarge) Time t=2 (Enlarge) Time t=3 (Enlarge)
Lorenz caos1-175.png Lorenz caos2-175.png Lorenz caos3-175.png
These figures — made using ρ=28, σ = 10 and β = 8/3 — show three time segments of the 3-D evolution of 2 trajectories (one in blue, the other in yellow) in the Lorenz attractor starting at two initial points that differ only by 10-5 in the x-coordinate. Initially, the two trajectories seem coincident (only the yellow one can be seen, as it is drawn over the blue one) but, after some time, the divergence is obvious.
Java animation of the Lorenz attractor shows the continuous evolution.

[edit] Rayleigh number

The Lorenz attractor for different values of ρ
Lorenz Ro14 20 41 20-200px.png Lorenz Ro13-200px.png
ρ=14, σ=10, β=8/3 (Enlarge) ρ=13, σ=10, β=8/3 (Enlarge)
Lorenz Ro15-200px.png Lorenz Ro28-200px.png
ρ=15, σ=10, β=8/3 (Enlarge) ρ=28, σ=10, β=8/3 (Enlarge)
For small values of ρ, the system is stable and evolves to one of two fixed point attractors. When ρ is larger than 24.28, the fixed points become repulsors and the trajectory is repelled by them in a very complex way, evolving without ever crossing itself.
Java animation showing evolution for different values of ρ

[edit] Source code

The source code to simulate the Lorenz attractor in GNU Octave follows.

% Lorenz Attractor equations solved by ODE Solve
%% x' = sigma*(y-x)
%% y' = x*(rho - z) - y
%% z' = x*y - beta*z
function dx = lorenzatt(X)
    rho = 28; sigma = 10; beta = 8/3;
    dx = zeros(3,1);
    dx(1) = sigma*(X(2) - X(1));
    dx(2) = X(1)*(rho - X(3)) - X(2);
    dx(3) = X(1)*X(2) - beta*X(3);
    return
end
% Using LSODE to solve the ODE system.
clear all
close all
lsode_options("absolute tolerance",1e-3)
lsode_options("relative tolerance",1e-4)
t = linspace(0,25,1e3); X0 = [0,1,1.05];
[X,T,MSG]=lsode(@lorenzatt,X0,t);
T
MSG
plot3(X(:,1),X(:,2),X(:,3))
view(45,45)
 
% A simple Lorenz Solver in MatLab code
function dxdt=myLorenz(t,x)
% The RHS of the Lorenz attractor
% Save this function in a separate file 'myLorenz.m'
sigma = 10;
r = 28;
b = 8/3;
dxdt=[ sigma*(x(2)-x(1));
r*x(1)-x(2)-x(1)*x(3);
x(1)*x(2)-b*x(3)];
end
%% Main program: Save the program in a separate .m file and run it.
clear all; % clear all variables
t=linspace(0,50,3000)'; % time variables
y0=[-1;3;4]; % Initial conditions
[t,Y] = ode45(@myLorenz,t,y0); %Invoking built-in solver 'ode45'
plot3(Y(:,1),Y(:,2),Y(:,3));  % Plot results
grid on;

[edit] See also

[edit] References

[edit] External links

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