Telegraph Equation Slider
IFST · Parabolic ↔ Hyperbolic

Kelvin’s cable, Heaviside’s cable

τ ∂²u∂t² + ∂u∂t = D ∂²u∂x²
τ = 1.00
t = 3.00
TypeHYPERBOLIC
b² − 4ac = 4Dτ4.00
Front speed v = √(D/τ)1.000
Regime at this tt/τ = 4.0
Snapshot u(x, t)line of length 40, ends grounded (u = 0)
telegraph solution τ = 0 reference fronts x₀ ± (w + vt)
Space–time mapcolour ∝ √|u|, so weak tails show
characteristics dx/dt = ±v current t

τ = 0: parabolic

The discriminant is zero and the only characteristics are the lines t = const. The initial pulse is zero for |x − x₀| > w, yet at t = 0⁺ the blue curve is already non-zero at every x. Only u(x,0) can be prescribed.

τ > 0: hyperbolic

Any τ, however small, gives two real characteristics dx/dt = ±√(D/τ). Outside the cone |x − x₀| < w + vt, u is exactly zero. Now u_t(x,0) is also needed; here it is zero, so the pulse splits into two halves that leave a wake behind them.

t ≫ τ: diffusion returns

The ∂u/∂t term damps the waves as e−t/2τ. At late times the yellow curve approaches the blue one. This is how strongly scattered wave energy, such as coda, ends up obeying a diffusion law.

Model: D = 1, line 0 ≤ x ≤ 40 with u = 0 at both ends, initial pulse u = cos²(π(x − x₀)/2w) for |x − x₀| < w (x₀ = 20, w = 1) and zero elsewhere, u_t(x,0) = 0. Exact solution by expansion in 400 sine modes; each mode is a damped oscillator τ a″ + a′ + D k² a = 0 (overdamped for long wavelengths, underdamped for short ones). Keys: Space play/pause, ←→ on a slider to step.