Sensitivity and the Lorenz Attractor¶
Copyright (C) 2026 Andreas Kloeckner
MIT License
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In [4]:
import numpy as np
import matplotlib.pyplot as plt
import matplotlib.gridspec as gridspec
from scipy.integrate import solve_ivp
def log_norm_2(A):
"""
Logarithmic norm (matrix measure) μ₂(A) = λ_max((A + Aᵀ)/2).
This is the tightest Lipschitz constant available from the 2-norm:
‖e^{At}‖₂ ≤ exp(μ₂(A)·t).
"""
S = 0.5 * (A + A.T)
return np.max(np.linalg.eigvalsh(S))
In [3]:
SIGMA = 10.0
RHO = 28.0
BETA = 8.0 / 3.0
def lorenz(t, y):
x, y_, z = y
return np.array([
SIGMA * (y_ - x),
x * (RHO - z) - y_,
x * y_ - BETA * z,
])
def lorenz_jac(y):
"""Jacobian of the Lorenz vector field at y."""
x, y_, z = y
return np.array([
[-SIGMA, SIGMA, 0.0 ],
[RHO - z, -1.0, -x ],
[y_, x, -BETA ],
])
In [36]:
T_END = 20
# T_END = 80
EPSILON = 1e-6
# EPSILON = 1e-2
Y0 = np.array([1.0, 0.0, 0.0])
Y0_PERT = Y0 + EPSILON * np.array([1.0, 0.0, 0.0])
t_eval = np.linspace(0, T_END, 8000)
print("Integrating reference trajectory …")
sol_ref = solve_ivp(lorenz, [0, T_END], Y0, t_eval=t_eval,
method='RK45', rtol=1e-10, atol=1e-12)
print("Integrating perturbed trajectory …")
sol_pert = solve_ivp(lorenz, [0, T_END], Y0_PERT, t_eval=t_eval,
method='RK45', rtol=1e-10, atol=1e-12)
t = sol_ref.t
Y = sol_ref.y # shape (3, N)
Yp = sol_pert.y
Integrating reference trajectory … Integrating perturbed trajectory …
In [37]:
fig = plt.figure(figsize=(14,10))
ax3d = plt.gcf().add_subplot(projection='3d')
ax3d.plot(*Y, lw=0.5, alpha=0.7, label="reference")
ax3d.plot(*Yp, lw=0.5, alpha=0.7, label=f"perturbed (ε={EPSILON:.0e})")
ax3d.scatter(*Y[:, 0], s=20, zorder=5)
ax3d.scatter(*Yp[:, 0], s=20, zorder=5)
ax3d.set_xlabel("x", )
ax3d.set_ylabel("y", )
ax3d.set_zlabel("z", )
ax3d.legend(fontsize=7, loc="best")
Out[37]:
<matplotlib.legend.Legend at 0x7f662908b0e0>
In [38]:
separation = np.linalg.norm(Y - Yp, axis=0)
plt.plot(t, separation)
Out[38]:
[<matplotlib.lines.Line2D at 0x7f6628db6660>]
In [39]:
# (a) Tight bound: integrate μ₂(J(y(t))) along the reference orbit.
# ‖δy(t)‖ ≤ ε · exp(∫₀ᵗ μ₂(J(y(s))) ds)
print("Computing logarithmic norms along orbit …")
log_norms = np.array([log_norm_2(lorenz_jac(Y[:, i])) for i in range(len(t))])
# Cumulative integral via trapezoidal rule
log_norm_integral = np.zeros_like(t)
log_norm_integral[1:] = np.cumsum(
0.5 * (log_norms[:-1] + log_norms[1:]) * np.diff(t)
)
bound_tight = EPSILON * np.exp(log_norm_integral)
# (b) Crude bound: use the supremum of μ₂ over the observed orbit.
L_crude = np.max(log_norms)
bound_crude = EPSILON * np.exp(L_crude * t)
print(f" max log-norm along orbit: {L_crude:.4f}")
print(f" (compare: largest Lyapunov exponent ≈ 0.906)")
Computing logarithmic norms along orbit … max log-norm along orbit: 14.0256 (compare: largest Lyapunov exponent ≈ 0.906)
In [41]:
plt.semilogy(t, separation, lw=1.5, label="actual ‖δy(t)‖")
plt.semilogy(t, bound_tight, lw=1.2, ls="--",
label=r"tight P-L: $\varepsilon\exp\!\left(\int_0^t \mu_2(J)\,ds\right)$")
plt.semilogy(t, bound_crude, lw=1.0, ls=":",
label=rf"crude P-L: $\varepsilon\exp(L_\max t)$, $L={L_crude:.2f}$")
plt.xlabel("t")
plt.ylabel("‖y(t) − ŷ(t)‖")
plt.legend(loc="best")
Out[41]:
<matplotlib.legend.Legend at 0x7f6628b37cb0>
In [ ]: