Waves & Sound

The Doppler Effect, Measured

By Lucian — builder & engineer, LK Forge

Everyone has heard it: an ambulance races past and its siren sags from a high whine to a low drone in a single instant. That drop is a number, and a musical one. We took the moving-source physics from the Doppler simulator and worked out exactly how far the pitch falls — and what happens when the source is fast enough to catch its own sound.

 ·  6 min read  ·  exact from f = f0·v/(v∓vₛ)

3 semitones
pitch drop of a siren passing at 108 km/h (a minor third)
482 → 405
Hz: a 440 Hz horn, approaching vs receding at 30 m/s
→ ∞ at Mach 1
the approaching pitch as the source nears the sound barrier
30°
shock-cone half-angle at twice the speed of sound

The split widens with speed

Approaching, the waves bunch and the pitch rises; receding, they stretch and it falls. The two branches start together at the rest pitch and pull apart as the source speeds up — but not symmetrically. The receding branch flattens toward half the frequency, while the approaching branch curves upward and heads for the ceiling as the source nears the speed of sound.

0 400 800 1200 1600 rest pitch 440 Hz approaching → ∞ at Mach 1 receding 50100150200250 source speed (m/s) → Hz

Observed frequency vs source speed. The approaching pitch curves toward infinity at the 343 m/s sound barrier; the receding pitch sags toward 220 Hz. The gap between them is what you hear as the drop.

The drop, in Hz and in music

Frequencies are easier to feel as musical intervals. At walking-past-fast speeds the drop is a couple of semitones; at highway speed it is a clear minor third; a racing car crossing at 60 m/s drops a tritone; and by 200 m/s the pitch falls two full octaves from approach to retreat.

Source speedApproachingRecedingDropIn semitones
10 m/s (36 km/h) 453.2 Hz 427.5 Hz 26 Hz 1.01 st
30 m/s (108 km/h) 482.2 Hz 404.6 Hz 78 Hz 3.04 st
60 m/s (216 km/h) 533.3 Hz 374.5 Hz 159 Hz 6.12 st
100 m/s (360 km/h) 621.1 Hz 340.7 Hz 280 Hz 10.4 st
200 m/s (720 km/h) 1055.4 Hz 277.9 Hz 778 Hz 23.1 st

440 Hz source, stationary listener, speed of sound 343 m/s. Semitones = 12·log₂(approach ÷ recede). 12 semitones is one octave; a whole octave of drop needs a source doing about 114 m/s.

Past the sound barrier: the shock cone

Right at Mach 1 the approaching pitch is infinite because the source keeps pace with its own wavefronts — they stack into a single wall of pressure, the sonic boom. Go faster and the source leaves its sound behind, and all those fronts fall on a cone dragging behind it. The cone’s half-angle is arcsin(1/Mach): a right angle at Mach 1, closing to a sharp point as the speed climbs.

30° 60° 90° 90° 56.4° 41.8° 30° 19.5° 14.5° 11.522.533.54 Mach number → cone ½-angle

Shock-cone half-angle μ = arcsin(1/Mach). The faster the source, the tighter the cone dragging its boom behind it.

Reproduce it yourself

Two fractions give the whole thing. The pitch drop as a source passes is just the ratio of the two, turned into semitones.

const v = 343, f0 = 440, vs = 30;   // m/s, Hz, source speed

const approach = f0 * v / (v - vs);   // 482.2 Hz  (-> infinity as vs -> v)
const recede   = f0 * v / (v + vs);   // 404.6 Hz
const drop_st  = 12 * Math.log2(approach / recede);  // 3.04 semitones

// beyond Mach 1: shock-cone half-angle
const coneDeg = M => Math.asin(1 / M) * 180 / Math.PI;   // coneDeg(2) = 30

The frequency and cone formulas are lifted straight from the Doppler solver; the speed sweep is the small script behind this post.

Watch the waves bunch

Open the simulator, drag the source speed up, and watch the wavefronts crowd ahead and stretch behind — then push past Mach 1 and see the shock cone snap into place.

Open the Doppler lab →
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Related reading

Common questions

Why does a siren drop in pitch as it passes you?

As the source approaches, each wavefront is emitted a little closer than the last, so the waves bunch up: shorter wavelength, higher frequency. Once it passes, the waves stretch out behind it: longer wavelength, lower frequency. The observed frequency is f0·v/(v−vs) coming toward you and f0·v/(v+vs) going away. For a 440 Hz horn at 30 m/s (108 km/h) that is 482 Hz then 405 Hz — a 77 Hz, ~3-semitone drop (about a minor third) that happens in the instant it goes by.

How fast would something have to move to shift its pitch by an octave?

An octave means the approaching-to-receding frequency ratio (v+vs)/(v−vs) equals 2, which needs vs = v/3 ≈ 114 m/s (about 410 km/h). Our benchmark shows the drop growing from about 1 semitone at 10 m/s to 3 at 30 m/s, 6 at 60, over 10 (nearly an octave) at 100 m/s, and roughly two octaves at 200 m/s. The effect accelerates because the approaching frequency f0·v/(v−vs) blows up as the source speed nears the speed of sound.

What happens at the speed of sound — and beyond?

As the source speed approaches v = 343 m/s, the denominator v−vs goes to zero and the approaching frequency runs to infinity: every wavefront the source ever emitted arrives at once, piling into a single shock — the sonic boom. Above Mach 1 the source outruns its own sound and the shock trails as a cone whose half-angle is μ = arcsin(1/Mach): 90° right at Mach 1, 30° at Mach 2, and 14.5° at Mach 4 — the faster it goes, the tighter the cone.