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Doppler Effect
The Doppler Effect: An Overview
The Doppler Effect is the change in Apparent Frequency of a wave when the source and observer are in Relative Motion.
$$f_{obs} \neq f_{source}$$
The observed frequency deviates from the source frequency due to motion.
$f_{obs}$=Frequency heard by observer(Hz)
$f_{source}$=Frequency emitted by source(Hz)
Frequency-Pitch Link: In sound, this is perceived as a change in Pitch.
Wave Fronts: Motion causes Wave Fronts to bunch up or spread out in the medium.
Key Distinction: The source frequency $f$ never changes — only the observed frequency $f'$ shifts due to motion.
Medium Dependence: The Doppler effect for sound depends on motion relative to the medium (air), not just relative motion between source and observer.
Case 1: The Observer is Moving
When an observer moves towards a Stationary Source, they encounter wave crests more frequently, increasing the Modified Frequency.
$$f_A = f \left( \frac{v \pm u_o}{v} \right)$$
The relative speed of the waves changes as the observer moves through the medium.
$v$=Speed of sound in medium(m/s)
$u_o$=Velocity of the observer(m/s)
$f$=Source frequency(Hz)
$u_o$ towards source
→Use $+$ (Higher frequency)
$u_o$ away from source
→Use $-$ (Lower frequency)
Wavelength Stability: Unlike a moving source, the physical wavelength in the medium remains constant.
Relative Velocity: The observer perceives a higher wave speed ($v + u_o$) when moving toward the source.
Proportionality: The fractional frequency shift is $\Delta f / f = u_o / v$ — directly proportional to observer speed.
Limiting Case: When $u_o = 0$, $f' = f$ — no shift. When $u_o = v$ (observer at speed of sound towards source), $f' = 2f$ — frequency doubles.
Case 2: The Source is Moving
A moving source physically alters the wavelength in the medium, causing Wavelength Compression ahead and expansion behind.
$$f_C = f \left( \frac{v}{v \mp u_s} \right)$$
The distance between wave crests changes because the source 'chases' its own emitted waves.
$u_s$=[Source Velocity](m/s)
$v$=Speed of sound(m/s)
$u_s$ towards observer
→Use $-$ in denominator (Increases frequency)
$u_s$ away from observer
→Use $+$ in denominator (Decreases frequency)
Doppler Shift: The change in wavelength is calculated as $\Delta \lambda = u_s / f$.
Wave Speed: The speed of waves ($v$) relative to the medium is unaffected by the source's speed.
Asymmetry: Source approaching gives $f' = f \cdot v/(v - u_s)$ and receding gives $f' = f \cdot v/(v + u_s)$. The approaching shift is always larger than the receding shift for the same speed.
Limiting Case: As $u_s \to v$, the denominator $(v - u_s) \to 0$ and $f' \to \infty$ — the source catches up to its own waves, creating a Shock Wave (sonic boom).
Case 3: Both Source and Observer Moving
When both the source and observer are in motion, both effects combine into a single general formula for the Modified Frequency.
$$f' = f \left( \frac{v \pm u_o}{v \mp u_s} \right)$$
The numerator handles observer motion (changes how fast the observer encounters waves) and the denominator handles source motion (changes the physical wavelength).
$v$=Speed of sound in medium(m/s)
$u_o$=Observer velocity(m/s)
$u_s$=Source velocity(m/s)
Both approaching each other
→$f' = f(v + u_o)/(v - u_s)$ — maximum frequency increase
Both receding from each other
→$f' = f(v - u_o)/(v + u_s)$ — maximum frequency decrease
Same speed, same direction
→$f' = f$ — no shift (relative velocity is zero)
Sign Convention: Use $+u_o$ when observer moves towards source, $-u_o$ when away. Use $-u_s$ when source moves towards observer, $+u_s$ when away.
Memory Aid: Think 'towards = higher frequency'. In the formula: numerator increase or denominator decrease both raise $f'$.
Echo Problems: When sound reflects off a surface (wall, cliff), treat it as two Doppler shifts — the reflecting surface acts as both receiver and re-emitter.
Applications in Technology and Astronomy
The Doppler Effect is a fundamental tool for measuring velocity in Radar, Sonar, and medical imaging.
$$\Delta \lambda = \lambda_{obs} - \lambda_{source}$$
The Doppler shift in wavelength indicates the direction and speed of relative motion.
$\Delta \lambda$=Change in wavelength(m (or nm for light))
$\lambda_{obs}$=Wavelength measured by observer
$\lambda_{source}$=Wavelength emitted at rest
$\Delta \lambda > 0$
→Red Shift — source moving away (wavelength increases)
$\Delta \lambda < 0$
→Blue Shift — source approaching (wavelength decreases)
Red Shift: Distant galaxies moving away exhibit a shift toward longer (red) wavelengths — key evidence for the expanding universe.
Blue Shift: Stars or galaxies approaching Earth have spectra shifted toward shorter (blue) wavelengths.
Radar Speed Trap: Microwaves reflected off a moving car are Doppler-shifted; the shift is doubled because the signal bounces back.
Sonar: Underwater echo-ranging uses sound waves. Doppler detection measures target speed via frequency shift of echoes — used for submarine detection and depth measurement.
Echolocation: Bats and dolphins use Doppler shifts of reflected ultrasound to determine the speed of moving prey.
Blood Flow: Medical ultrasound (5–10 MHz) directed at arteries detects backscattered signal shifts to measure blood flow velocity.