Physics-accurate Doppler shift + volume attenuation. Upload a short loop, set geometry, listen.
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55 mph
30 ft
300%
0 Β’
1.0Γ
Pitch factor
β
Distance
β
Gain
β
Progress
β
f = fβ Β· c / (c β v_radial) | gain β 1/distance | drive-by window: Β±5 s from closest approach
What is Dopplerize?
Dopplerize is a free, browser-based physics simulator that applies the
Doppler effect
to any audio file. Hear how a car's music changes pitch as it speeds past youβjust like in real life.
Perfect for musicians, physics students, sound designers, and curious listeners.
No download, no signup, 100% client-side.
π Related searches: Doppler effect simulator, pitch shift audio online, physics sound demo,
car audio Doppler, real-time frequency modulation, Web Audio API demo, educational audio tool
π Why Does Pitch Bend When Things Move? (The Doppler Deep Dive)
The Doppler effect isn't magic β it's geometry + wave physics. When a sound source moves toward you, each wave crest gets emitted from a slightly closer position. The waves compress β higher frequency β higher pitch. When it recedes, waves stretch β lower pitch.
The formula (no panic):
f_observed = f_source Γ c / (c β v_radial)
c = speed of sound (343 m/s) β’ v_radial = how fast the source moves toward/away from you
ποΈ Your Controls, Decoded
π Vehicle speed (mph)
Faster car = bigger pitch swing. At 300 mph, the shift is dramatic (~Β±20%). At 10 mph, it's subtle.
Try: 65 mph + 5 ft distance for that classic "NASCAR flyby" sound.
π Road distance (ft)
This is your orthogonal distance β how far you stand from the road's edge.
Close (5 ft) = sudden "WHEEE-oooom" pitch drop. Far (200 ft) = gentle, sweeping glide.
Physics reason: radial velocity changes fastest when you're near the path.
π Volume
Real sound obeys the inverse-distance law: double the distance = quarter the intensity.
We normalize this so "100%" = loudest at closest approach. Crank to 300β500% for headphone-friendly "car stereo" levels.
ποΈ Manual pitch bend (cents)
Override physics! 100 cents = 1 semitone. Bend +1200 = shift up an octave.
Pro use: Compensate for recording pitch, or create alien vehicle sounds.
β±οΈ Simulation speed
Time dilation for your ears. 0.5Γ = slow-mo analysis. 3Γ = quick demo.
Doesn't change physics β just how fast the car "drives" through the 10-second window.
βοΈ Freeze at closest point
Lock the pitch shift at the moment of closest approach.
Why? Sustain that "peak Doppler" tone for analysis, or create a static shifted loop.
β Reverse direction
Flip the car's travel direction. Physics is symmetric, but perception isn't β
approaching high pitch β receding low pitch feels different than the reverse.
π Doppler in the Wild
π Ambulances: That iconic "nee-naw" is Doppler + siren modulation. The pitch drop at closest approach is ~15β25% for typical speeds.
ποΈ F1 cars: At 200 mph, the shift is ~Β±30%. Combined with engine harmonics, it creates that visceral "scream-then-growl" effect.
π Astronomy: Redshift/blueshift of starlight uses the exact same math β but with light speed (c = 300,000 km/s). Hubble measured universe expansion this way.
π¦ Bats & dolphins: They emit calls and listen for Doppler-shifted echoes to calculate prey velocity. Nature's radar.
π§ͺ Try This Experiment:
Set Speed=65 mph, Distance=10 ft, Volume=300%
Click Play, then slowly drag Distance from 10 β 200 ft
Listen: the pitch transition changes from "sudden drop" to "smooth glide"
Why? Radial velocity derivative dv_radial/dt is largest at small distances
π‘ Fun fact: Christian Doppler predicted this effect in 1842 using light from binary stars. It took 3 years for someone to test it with trumpeters on a moving train. Science: sometimes you need brass + rails.
Wave compression (approaching) vs. stretching (receding)
Audio Attribution & License:
"Alien Nation" by 1st Contact
is licensed under CC BY-SA 4.0.
This app applies real-time Doppler processing (derivative work).
To comply with ShareAlike, Dopplerize and all modifications are released under
CC BY-SA 4.0.