Doppler shift
(W3.3.1) W3.3 · The Doppler Effect →The observed frequency f′ when source and observer move relative to the medium at speed v_s and v_o respectively.
| observed frequency | Hz | |
| source frequency | Hz | |
| wave speed in the medium | m/s | |
| observer, source speed | m/s |
Source and observer speeds much less than the wave speed in the medium (for sound) — otherwise relativistic corrections apply.
Assumes source and observer speeds much less than the wave speed in the medium — near or above the wave speed (e.g. supersonic sources) requires relativistic or shock-wave treatment instead.
A moving observer encounters wavefronts at a different rate than a stationary one; a moving source compresses wavefronts ahead of it and stretches them behind — combining both effects gives the general shift.
As the source speed v_s approaches the wave speed v, the denominator approaches zero:
This divergence marks the onset of a shock wave — the source is about to outrun its own wavefronts entirely.
Sign convention: use + in the numerator when the observer moves TOWARD the source, and − in the denominator when the source moves TOWARD the observer (opposite signs for motion away). Getting a sign wrong shifts the frequency the wrong way.