1The changing pitch
A moving ambulance sends out each crest from where it is at that moment. Ahead of it the crests are bunched: a shorter wavelength, more crests per second, a higher pitch. Behind it they are spread out: a lower pitch. The siren itself never changes.
The Doppler effect is the change in the frequency you receive when the source, the listener, or both move. It happens with all waves: sound, water waves and light.
2A moving source
The source sends a crest every period . In that time a crest moves (the speed of sound in the air), but the source moves after it. So the gap ahead is only . The listener still receives the crests at speed , so :
3A moving observer
With the source still, the crests keep their normal spacing . A listener moving toward the source at meets them at :
- 500 Hz, walking toward it at 17 m/s: Hz. For 550 Hz you need m/s.
- Moving source and moving listener are not the same: at 34 m/s toward a 500 Hz sound, a moving listener hears 550 Hz but a moving source gives Hz. A moving source changes the wavelength in the air itself; a moving listener only meets the same waves faster.
4The general formula
- Listener moving toward the source: on top; away: .
- Source moving toward the listener: below; away: .
- Check: coming together must raise the pitch, moving apart must lower it.
5Echoes and radar
A bat flying at toward a wall: first the wall is a still listener receiving ; then the wall is a still source and the bat a listener moving toward it: .
- A bat at 10 m/s sending 40 kHz hears kHz.
- Radar and ultrasound use : 10 GHz radar and a 2 kHz shift give m/s.
- Uses: police radar, weather radar (rain and wind), ultrasound scans of blood flow and baby heartbeats, bat echolocation.
6Doppler effect for light
Light needs no medium, so only the relative speed v of source and observer matters (v positive when approaching), and the sound formula does not apply.
- A 600 nm line seen at 660 nm: , m/s, moving away.
- A 656 nm line seen at 655.3 nm: blueshift, approaching at about km/s.
- Distant galaxies are all redshifted, the farther the more (Hubble's law, v = H₀d): the universe is expanding.
- Astronomers also use it for star speeds, planets that make their stars wobble, and rotating galaxies.
7Angles and shock waves
Only motion along the line of sight changes the pitch. A passing ambulance sounds highest far away while coming, exactly its true note at the closest point (), then lower and lower: the pitch slides down smoothly.
A source faster than sound () outruns its crests and the formula breaks down. The crests pile up on a cone, a shock wave, heard as a sonic boom. In the time the source moves a crest spreads :
Summary
Key ideas
- The received frequency changes when the source or the listener moves; the source's own frequency does not.
- A moving source squeezes the waves ahead of it and stretches them behind.
- A moving listener meets unchanged waves faster or slower.
- General formula: f′ = f(v ± v_o)/(v ∓ v_s), with signs chosen so that approaching raises the pitch.
- The same speed gives different shifts for a moving source and a moving listener.
- No relative motion (both moving the same way at the same speed) means no shift.
- Echoes from moving reflectors are shifted twice: Δf/f ≈ 2v/v_sound, or 2v/c for radar.
- For light only the relative speed matters: Δf/f = v/c; receding gives a redshift, approaching a blueshift.
- At an angle, only the velocity component along the line of sight counts.
- Faster than sound, crests form a shock cone with sin θ = 1/M.
Every equation
- Source approaching
- Source receding
- Wavelength ahead
- Listener approaching
- Listener receding
- General
- Moving reflector
- Small reflector speed
- Radar
- Light, slow
- Light, any speed
- Redshift
- Hubble's law
- At an angle
- Mach number
- Shock cone