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Wave Properties

Wave Properties

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Board Coverage AQA Paper 2 | Edexcel CP2 | OCR (A) Paper 2 | CIE P2

Waves on a String

Explore the simulation above to develop intuition for this topic.

1. Progressive Waves

A progressive wave is a disturbance that transfers energy through a medium (or vacuum) without transferring matter. Each particle in the medium oscillates about its equilibrium position.

Key Definitions

  • Displacement yy: the distance of a point on the wave from its equilibrium position (m)
  • Amplitude AA: the maximum displacement from equilibrium (m)
  • Wavelength λ\lambda: the distance between two consecutive points in phase — e.g., crest-to-crest (m)
  • Period TT: the time for one complete oscillation (s)
  • Frequency ff: the number of complete oscillations per unit time (Hz)
  • Phase ϕ\phi: a measure of the position in the cycle of oscillation (rad)

f=1Tf = \frac{1}{T}

The Wave Equation

v=fλ\boxed{v = f\lambda}

Derivation. Consider a wave travelling at speed vv. In one period TT, the wave advances by exactly one wavelength λ\lambda (the source completes one full oscillation, producing one complete wave cycle):

v=LBdistancetravelledRB◆◆LBtimetakenRB=LBλRB◆◆LBTRB=λ1T=fλv = \frac◆LB◆\mathrm{distance travelled}◆RB◆◆LB◆\mathrm{time taken}◆RB◆ = \frac◆LB◆\lambda◆RB◆◆LB◆T◆RB◆ = \lambda \cdot \frac{1}{T} = f\lambda

\square

Intuition. If you shake a rope at 2 Hz with a wavelength of 1.5 m, the crests travel at 3 m/s. Faster shaking or longer waves both make the wave move faster.

Real-World Application: Seismic Waves

When an earthquake occurs, seismic waves carry energy through the Earth. P-waves (primary waves) are longitudinal compressional waves that travel fastest (5 to 8 km/s through the crust) and can pass through solids and liquids. S-waves (secondary waves) are transverse waves that travel slower (3 to 4.5 km/s) and cannot pass through liquids — this is how geophysicists determined that the Earth's outer core is liquid.

Seismographs at different stations detect P-waves and S-waves arriving at different times. By measuring the time difference Δt\Delta t and knowing the approximate speeds vPv_P and vSv_S, the distance to the epicentre can be estimated:

dLBvPvSRB◆◆LBvPvSRBΔtd \approx \frac◆LB◆v_P \cdot v_S◆RB◆◆LB◆v_P - v_S◆RB◆ \cdot \Delta t

Three or more stations are needed to triangulate the epicentre location.

Mathematical Description of a Progressive Wave

A sinusoidal progressive wave travelling in the +x+x direction is described by:

y(x,t)=Asin(kxωt+ϕ0)y(x,t) = A\sin(kx - \omega t + \phi_0)

where:

  • k=LB2πRB◆◆LBλRBk = \frac◆LB◆2\pi◆RB◆◆LB◆\lambda◆RB◆ is the wave number (rad m1^{-1})
  • ω=2πf=LB2πRB◆◆LBTRB\omega = 2\pi f = \frac◆LB◆2\pi◆RB◆◆LB◆T◆RB◆ is the angular frequency (rad s1^{-1})
  • ϕ0\phi_0 is the initial phase

Proof that v=fλv = f\lambda from the wave function. A point of constant phase satisfies kxωt=constkx - \omega t = \mathrm{const}. Differentiating: kdxdtω=0k\frac{dx}{dt} - \omega = 0, so:

v=dxdt=LBωRB◆◆LBkRB=LB2πfRB◆◆LB2π/λRB=fλv = \frac{dx}{dt} = \frac◆LB◆\omega◆RB◆◆LB◆k◆RB◆ = \frac◆LB◆2\pi f◆RB◆◆LB◆2\pi/\lambda◆RB◆ = f\lambda

\square

2. Transverse and Longitudinal Waves

Transverse Waves

The oscillations are perpendicular to the direction of energy propagation.

  • Electromagnetic waves (light, radio, X-rays)
  • Waves on a string
  • Water waves (approximately, for small amplitudes)

Longitudinal Waves

The oscillations are parallel to the direction of energy propagation.

  • Sound waves
  • Pressure waves in springs

Longitudinal waves have compressions (regions of high pressure, where particles bunch together) and rarefactions (regions of low pressure, where particles spread apart).

Real-World Application: Musical Instruments

Sound production in musical instruments relies on creating standing waves (covered in the next topic), but the initial wave type depends on the instrument:

  • Stringed instruments (guitar, violin): A plucked or bowed string vibrates transversely, creating a transverse wave on the string. The vibrating string then pushes air molecules back and forth, producing a longitudinal sound wave. This is a key exam point: the wave on the string is transverse, but the sound wave in air is longitudinal.
  • Wind instruments (flute, clarinet, trumpet): A column of air vibrates longitudinally. The player's lips or a reed create compressions and rarefactions that travel along the air column.
  • Percussion (drums): The drum membrane vibrates transversely, and the resulting pressure changes in the surrounding air produce longitudinal sound waves.

The speed of sound in air at 20°C is approximately 343 m/s. For a concert A (440 Hz), the wavelength in air is λ=343/440=0.78\lambda = 343/440 = 0.78 m. Higher notes have shorter wavelengths; lower notes have longer wavelengths.

warning

Common Pitfall Electromagnetic waves are transverse but do not require a medium — they propagate through vacuum via oscillating electric and magnetic fields. Sound waves are longitudinal and require a medium.

tip

Exam Technique When asked to sketch a longitudinal wave, draw a series of vertical lines representing air molecules. Show compressions (closely spaced) and rarefactions (widely spaced). Label both.

Alternatively, plot displacement vs position — the graph looks sinusoidal, but positive displacement means particles moved to the right (in the direction of propagation), not upward.

3. Polarisation

Definition. Polarisation is the restriction of the oscillation direction of a transverse wave to a single plane.

Proof of Malus's Law

Consider unpolarised light of intensity I0I_0 incident on a polarising filter (analyser) whose transmission axis makes an angle θ\theta with the polarisation direction of the incoming light.

The electric field of the incoming polarised wave can be resolved into components parallel and perpendicular to the analyser's transmission axis:

E=E0cosθ,E=E0sinθE_{\parallel} = E_0 \cos\theta, \qquad E_{\perp} = E_0 \sin\theta

Only the parallel component is transmitted. The transmitted intensity is:

I=12ε0cE2=12ε0cE02cos2θ=I0cos2θI = \frac{1}{2}\varepsilon_0 c E_{\parallel}^2 = \frac{1}{2}\varepsilon_0 c E_0^2 \cos^2\theta = I_0 \cos^2\theta

I=I0cos2θ\boxed{I = I_0 \cos^2\theta}

where I0=12ε0cE02I_0 = \frac{1}{2}\varepsilon_0 c E_0^2 is the intensity of the polarised light incident on the analyser.

Intuition. When θ=0\theta = 0, all light passes through. When θ=90\theta = 90^\circ, no light passes. At θ=45\theta = 45^\circ, the intensity is halved. This is a direct consequence of the vector nature of the electric field.

Polarisation by Reflection (Brewster's Angle)

When light reflects from a dielectric surface, the reflected ray is partially polarised. At Brewster's angle θB\theta_B, the reflected light is fully polarised perpendicular to the plane of incidence:

tanθB=n2/n1\tan\theta_B = n_2/n_1

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Board Note AQA and OCR (A) require Malus's law. CIE focuses on polarisation by filters. Edexcel covers qualitative polarisation.

Polarisation in Real Life

Polarising filters have many practical applications:

  • Polaroid sunglasses reduce glare by blocking horizontally polarised light reflected from horizontal surfaces (water, roads). Reflected light is predominantly horizontally polarised, so vertically oriented filters absorb most of the glare.
  • LCD screens use two crossed polarisers with liquid crystals between them. The crystals rotate the polarisation of light passing through, allowing controlled transmission of each pixel.
  • Stress analysis in engineering: transparent plastic models under stress become birefringent, rotating the polarisation of transmitted light. Viewed between crossed polarisers, stress concentrations appear as coloured fringes (photoelasticity).

Polarisation and Microwaves

Microwave ovens use polarised EM waves (wavelength ~12 cm). The metal mesh on the oven door acts as a polarising grid — the holes are much smaller than the wavelength, so the microwaves are reflected while visible light (with a much shorter wavelength) passes through, allowing you to see inside.

4. The Electromagnetic Spectrum

All EM waves travel at c=3.00×108c = 3.00 \times 10^8 m s1^{-1} in vacuum and are transverse. They are distinguished by wavelength (equivalently, frequency).

RegionWavelength RangeTypical Use
Radio waves>1\gt{} 1 mBroadcasting, communication
Microwaves1 mm – 1 mCooking, satellite signals
Infrared700 nm – 1 mmThermal imaging, remote controls
Visible light400 – 700 nmHuman vision
Ultraviolet10 – 400 nmSterilisation, fluorescence
X-rays0.01 – 10 nmMedical imaging
Gamma rays<0.01\lt{} 0.01 nmCancer treatment, nuclear decay

All EM waves are produced by accelerating charges. In order of increasing frequency: radio (oscillating currents in aerials), microwave (klystrons/magnetrons), infrared/visible/UV (atomic electron transitions), X-rays (electron deceleration), gamma rays (nuclear transitions).

tip

Exam Technique Memorise the order: Radio, Microwave, Infrared, Visible, Ultraviolet, X-ray, Gamma. Mnemonic: "Real Men In Vietnam Use X-ray Guns."

5. Intensity and Amplitude

Definition. The intensity II of a wave is the power per unit area:

I=PAI = \frac{P}{A}

with SI units W m2^{-2}.

Proof that IA2I \propto A^2 for a 2D Wave

Consider a sinusoidal wave on a string. The power transmitted past a point is the rate at which the transverse force does work:

P=Ftransverse×vtransverseP = F_{\mathrm{transverse}} \times v_{\mathrm{transverse}}

For a wave y=Asin(kxωt)y = A\sin(kx - \omega t), the transverse velocity is:

vy=LByRB◆◆LBtRB=Aωcos(kxωt)v_y = \frac◆LB◆\partial y◆RB◆◆LB◆\partial t◆RB◆ = -A\omega\cos(kx - \omega t)

The transverse component of tension is (for small amplitudes):

FyTLByRB◆◆LBxRB=TAkcos(kxωt)F_y \approx -T\frac◆LB◆\partial y◆RB◆◆LB◆\partial x◆RB◆ = -TAk\cos(kx - \omega t)

The instantaneous power is:

P=Fyvy=TAkAωcos2(kxωt)=TA2kωcos2(kxωt)P = F_y \cdot v_y = TAk \cdot A\omega \cos^2(kx - \omega t) = TA^2 k\omega \cos^2(kx - \omega t)

The average power over one cycle (since cos2=1/2\langle\cos^2\rangle = 1/2):

P=12TA2kω\langle P \rangle = \frac{1}{2}TA^2 k\omega

Since v=ω/kv = \omega/k, we have kω=ω2/vk\omega = \omega^2/v. Also, for a string, v=LBT/μRBv = \sqrt◆LB◆T/\mu◆RB◆ where μ\mu is the mass per unit length, so T=μv2T = \mu v^2:

P=12μv2A2LBω2RB◆◆LBvRB=12μvω2A2\langle P \rangle = \frac{1}{2}\mu v^2 A^2 \cdot \frac◆LB◆\omega^2◆RB◆◆LB◆v◆RB◆ = \frac{1}{2}\mu v \omega^2 A^2

The intensity is power per unit... but for a string wave, the "intensity" concept maps to power directly. The key result is:

IA2\boxed{I \propto A^2}

For electromagnetic waves, the intensity is:

I=12ε0cE02I = \frac{1}{2}\varepsilon_0 c E_0^2

which also shows IA2I \propto A^2 (where AA is the electric field amplitude E0E_0).

Intuition. Double the amplitude and you quadruple the energy carried. This is analogous to kinetic energy (Ek=12mv2E_k = \frac{1}{2}mv^2): double the speed and you quadruple the energy. The wave amplitude plays the same role as "speed" for the oscillating particles.

Inverse Square Law for Point Sources

For a wave spreading uniformly from a point source in 3D:

I=LBPRB◆◆LB4πr2RBI = \frac◆LB◆P◆RB◆◆LB◆4\pi r^2◆RB◆

At distance rr, the power is spread over a sphere of area 4πr24\pi r^2. Doubling the distance quarters the intensity.

I1r12=I2r22I_1 r_1^2 = I_2 r_2^2

Intensity and the Decibel Scale

In practice, intensity ratios are often expressed using the decibel scale:

Intensitylevel(dB)=10log10(II0)\mathrm{Intensity level (dB)} = 10 \log_{10}\left(\frac{I}{I_0}\right)

where I0=1.0×1012I_0 = 1.0 \times 10^{-12} W m2^{-2} is the threshold of hearing. This logarithmic scale reflects how human perception of loudness works: a 3 dB increase represents a doubling of intensity, while a 10 dB increase sounds roughly "twice as loud" to human ears.

Example. Normal conversation is approximately 60 dB. A whisper is about 30 dB. The intensity ratio is 10(6030)/10=103=100010^{(60-30)/10} = 10^3 = 1000, meaning conversation is 1000 times more intense than a whisper.

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Board Coverage AQA Paper 2 | Edexcel CP2 | OCR (A) Paper 2 | CIE P2

All boards cover the inverse square law. The decibel scale is explicitly on CIE and sometimes appears in AQA context questions. Edexcel and OCR (A) focus more on IA2I \propto A^2 and I1/r2I \propto 1/r^2 calculations.

Amplitude and the Inverse Square Law

Since IA2I \propto A^2 and I1/r2I \propto 1/r^2, it follows that:

A1rA \propto \frac{1}{r}

The amplitude decreases inversely with distance (not as 1/r21/r^2). This is an important distinction in exam questions that ask about amplitude at different distances.

6. Phase and Phase Difference

Two points on a wave are in phase if they have the same displacement and are moving in the same direction. They are in antiphase (completely out of phase) if their displacements are equal and opposite.

The phase difference between two points separated by distance Δx\Delta x is:

Δϕ=LB2πRB◆◆LBλRBΔx\Delta\phi = \frac◆LB◆2\pi◆RB◆◆LB◆\lambda◆RB◆\Delta x

Special cases:

  • In phase: Δϕ=0,2π,4π,\Delta\phi = 0, 2\pi, 4\pi, \ldots (integer multiples of 2π2\pi)
  • Antiphase: Δϕ=π,3π,5π,\Delta\phi = \pi, 3\pi, 5\pi, \ldots (odd multiples of π\pi)
tip

Exam Technique Phase difference questions often require you to identify two points on a wave graph and calculate Δx\Delta x. Then use Δϕ=360°×Δx/λ\Delta\phi = 360° \times \Delta x / \lambda (using degrees) or Δϕ=2πΔx/λ\Delta\phi = 2\pi \Delta x / \lambda (using radians). Be consistent with units.

Phase Difference from Wave Equations

If two waves are described by:

y1=A1sin(kxωt+ϕ1),y2=A2sin(kxωt+ϕ2)y_1 = A_1\sin(kx - \omega t + \phi_1), \qquad y_2 = A_2\sin(kx - \omega t + \phi_2)

then the phase difference is simply Δϕ=ϕ2ϕ1\Delta\phi = \phi_2 - \phi_1. This constant phase difference is what determines whether two waves interfere constructively (Δϕ=2nπ\Delta\phi = 2n\pi) or destructively (Δϕ=(2n+1)π\Delta\phi = (2n+1)\pi).

Phase Difference from Graphs

When given a displacement--position graph:

  1. Identify the positions of the two points: x1x_1 and x2x_2
  2. Measure the wavelength λ\lambda from the graph (peak to peak)
  3. Calculate Δx=x2x1\Delta x = |x_2 - x_1|
  4. Apply Δϕ=LBΔxRB◆◆LBλRB×360\Delta\phi = \frac◆LB◆\Delta x◆RB◆◆LB◆\lambda◆RB◆ \times 360^\circ (or ×2π\times 2\pi rad)

When given a displacement--time graph at a single point, the phase difference between two instants t1t_1 and t2t_2 is:

Δϕ=LBΔtRB◆◆LBTRB×360°=LBΔtRB◆◆LBTRB×2πrad\Delta\phi = \frac◆LB◆\Delta t◆RB◆◆LB◆T◆RB◆ \times 360° = \frac◆LB◆\Delta t◆RB◆◆LB◆T◆RB◆ \times 2\pi \mathrm{ rad}

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Board Coverage AQA Paper 2 | Edexcel CP2 | OCR (A) Paper 2 | CIE P2

AQA and OCR (A) frequently test phase difference from displacement--position graphs. CIE often combines phase difference with path difference in interference questions. Edexcel emphasises the connection between phase difference and the condition for constructive/destructive interference.

Real-World Application: Doppler Ultrasound

The Doppler effect causes a change in observed frequency when there is relative motion between source and observer. The phase difference between transmitted and received waves is used in Doppler ultrasound to measure blood flow velocity.

When ultrasound of frequency f0f_0 is reflected off blood cells moving with velocity vv away from the transducer, the received frequency is:

f=f0cvcf' = f_0 \cdot \frac{c - v}{c}

where cc is the speed of ultrasound in tissue (~1540 m/s). The frequency shift Δf=f0f\Delta f = f_0 - f' is proportional to blood velocity. By measuring this shift, clinicians can detect narrowed arteries, heart valve problems, and foetal heartbeats.

Problem Set

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Problem 1 A sound wave has frequency 440 Hz and wavelength 0.78 m. Calculate the speed of sound.

Answer. v=fλ=440×0.78=343v = f\lambda = 440 \times 0.78 = 343 m s1^{-1}.

If you get this wrong, revise: The Wave Equation

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Problem 2 A radio station broadcasts at 97.4 MHz. The speed of light is 3.00×1083.00 \times 10^8 m s1^{-1}. Calculate the wavelength.

Answer. λ=cf=LB3.00×108RB◆◆LB97.4×106RB=3.08\lambda = \frac{c}{f} = \frac◆LB◆3.00 \times 10^8◆RB◆◆LB◆97.4 \times 10^6◆RB◆ = 3.08 m.

If you get this wrong, revise: The Wave Equation

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Problem 3 Unpolarised light of intensity I0I_0 passes through two polarising filters. The first filter's axis is vertical. The second filter's axis is at 3030^\circ to the vertical. What is the intensity of the transmitted light?

Answer. After the first filter, the light is vertically polarised with intensity I0/2I_0/2 (unpolarised light has equal components in all directions; only one direction passes).

After the second filter: I=I02cos230°=I02×34=3I08I = \frac{I_0}{2}\cos^2 30° = \frac{I_0}{2} \times \frac{3}{4} = \frac{3I_0}{8}.

If you get this wrong, revise: Proof of Malus's Law

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Problem 4 Two points on a wave are separated by 0.15 m. The wavelength is 0.60 m. Calculate the phase difference in (a) radians and (b) degrees.

Answer. (a) Δϕ=LB2πRB◆◆LB0.60RB×0.15=LBπRB◆◆LB2RB\Delta\phi = \frac◆LB◆2\pi◆RB◆◆LB◆0.60◆RB◆ \times 0.15 = \frac◆LB◆\pi◆RB◆◆LB◆2◆RB◆ rad.

(b) Δϕ=0.150.60×360°=90\Delta\phi = \frac{0.15}{0.60} \times 360° = 90^\circ.

If you get this wrong, revise: Phase and Phase Difference

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Problem 5 A wave on a string has amplitude 5.0 mm and intensity 0.80 W. If the amplitude is increased to 15 mm, what is the new intensity?

Answer. IA2I \propto A^2, so I2/I1=(A2/A1)2=(15/5)2=9I_2/I_1 = (A_2/A_1)^2 = (15/5)^2 = 9. I2=9×0.80=7.2I_2 = 9 \times 0.80 = 7.2 W.

If you get this wrong, revise: Intensity and Amplitude

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Problem 6 A point source emits 50 W of sound power. Calculate the intensity at a distance of 8.0 m from the source.

Answer. I=LBPRB◆◆LB4πr2RB=LB50RB◆◆LB4π(64)RB=50804=0.0622I = \frac◆LB◆P◆RB◆◆LB◆4\pi r^2◆RB◆ = \frac◆LB◆50◆RB◆◆LB◆4\pi(64)◆RB◆ = \frac{50}{804} = 0.0622 W m2^{-2}.

If you get this wrong, revise: Inverse Square Law for Point Sources

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Problem 7 A light source has intensity I0I_0 at 2.0 m. At what distance is the intensity I0/9I_0/9?

Answer. I1r12=I2r22I_1 r_1^2 = I_2 r_2^2. I0×4=I09×r22I_0 \times 4 = \frac{I_0}{9} \times r_2^2. r22=36r_2^2 = 36. r2=6.0r_2 = 6.0 m.

If you get this wrong, revise: Inverse Square Law for Point Sources

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Problem 8 Polarised light of intensity 120 W m2^{-2} is incident on an analyser at 6060^\circ to the polarisation direction. Calculate the transmitted intensity.

Answer. I=120cos260°=120×0.25=30I = 120 \cos^2 60° = 120 \times 0.25 = 30 W m2^{-2}.

If you get this wrong, revise: Proof of Malus's Law

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Problem 9 A wave is described by y=0.03sin(2.5x200t)y = 0.03\sin(2.5x - 200t) m. Find: (a) the amplitude, (b) the wave number, (c) the angular frequency, (d) the wavelength, (e) the frequency, (f) the wave speed.

Answer. (a) A=0.03A = 0.03 m. (b) k=2.5k = 2.5 rad m1^{-1}. (c) ω=200\omega = 200 rad s1^{-1}. (d) λ=2π/k=2π/2.5=2.51\lambda = 2\pi/k = 2\pi/2.5 = 2.51 m. (e) f=ω/(2π)=200/(2π)=31.8f = \omega/(2\pi) = 200/(2\pi) = 31.8 Hz. (f) v=fλ=31.8×2.51=79.9v = f\lambda = 31.8 \times 2.51 = 79.9 m s1^{-1}.

If you get this wrong, revise: Mathematical Description of a Progressive Wave

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Problem 10 Explain why sound waves cannot be polarised but light waves can.

Answer. Polarisation restricts oscillation to a single plane, which is only meaningful for transverse waves (where oscillations are perpendicular to propagation). Sound waves are longitudinal — the oscillations are already along the direction of propagation, so there is no "plane" to restrict. Light waves are transverse, with electric and magnetic fields perpendicular to the direction of travel, so their oscillation direction can be restricted.

If you get this wrong, revise: Transverse and Longitudinal Waves

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Problem 11 A seismic P-wave travels at 6.5 km/s through rock and an S-wave travels at 3.8 km/s through the same rock. A seismograph detects the P-wave 120 s before the S-wave. Estimate the distance from the seismograph to the earthquake epicentre.

Answer. Let dd be the distance. The time for the P-wave is tP=d/vPt_P = d/v_P and for the S-wave is tS=d/vSt_S = d/v_S. The time difference is:

Δt=tStP=d(1vS1vP)=d(vPvSvPvS)\Delta t = t_S - t_P = d\left(\frac{1}{v_S} - \frac{1}{v_P}\right) = d\left(\frac{v_P - v_S}{v_P v_S}\right)

d=LBΔtvPvSRB◆◆LBvPvSRB=LB120×6500×3800RB◆◆LB65003800RB=LB120×2.47×107RB◆◆LB2700RB=LB2.964×109RB◆◆LB2700RB1.10×106m=1100kmd = \frac◆LB◆\Delta t \cdot v_P \cdot v_S◆RB◆◆LB◆v_P - v_S◆RB◆ = \frac◆LB◆120 \times 6500 \times 3800◆RB◆◆LB◆6500 - 3800◆RB◆ = \frac◆LB◆120 \times 2.47 \times 10^7◆RB◆◆LB◆2700◆RB◆ = \frac◆LB◆2.964 \times 10^9◆RB◆◆LB◆2700◆RB◆ \approx 1.10 \times 10^6 \mathrm{ m} = 1100 \mathrm{ km}

If you get this wrong, revise: Real-World Application: Seismic Waves

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Problem 12 Unpolarised light passes through three polarising filters. The first has a vertical axis, the second is at 4545^\circ to the vertical, and the third is horizontal (9090^\circ to the vertical). If the initial intensity is I0I_0, what is the final transmitted intensity? Compare this with the case where the middle filter is removed.

Answer. With all three filters:

  • After filter 1 (vertical): I1=I0/2I_1 = I_0/2, polarised vertically.
  • After filter 2 (4545^\circ): I2=(I0/2)cos245°=(I0/2)(1/2)=I0/4I_2 = (I_0/2)\cos^2 45° = (I_0/2)(1/2) = I_0/4, polarised at 4545^\circ.
  • After filter 3 (horizontal, 4545^\circ from filter 2's axis): I3=(I0/4)cos245°=(I0/4)(1/2)=I0/8I_3 = (I_0/4)\cos^2 45° = (I_0/4)(1/2) = I_0/8.

Without the middle filter (crossed polarisers): I=(I0/2)cos290°=0I = (I_0/2)\cos^2 90° = 0. No light passes.

If you get this wrong, revise: Proof of Malus's Law

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Problem 13 A point source emits sound with power 0.10 W. At a distance of 5.0 m, the amplitude of the sound wave is A1A_1. What is the amplitude at 20 m in terms of A1A_1?

Answer. Since IA2I \propto A^2 and I1/r2I \propto 1/r^2, it follows that A1/rA \propto 1/r. The ratio of amplitudes is:

A2A1=r1r2=5.020=14\frac{A_2}{A_1} = \frac{r_1}{r_2} = \frac{5.0}{20} = \frac{1}{4}

So A2=A1/4A_2 = A_1/4.

If you get this wrong, revise: Amplitude and the Inverse Square Law

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Problem 14 A Doppler ultrasound transducer operates at 5.0 MHz. Blood is flowing away from the transducer at 0.80 m/s. The speed of ultrasound in tissue is 1540 m/s. Calculate the frequency shift of the reflected signal.

Answer. First, the ultrasound hits the moving blood (source at rest, observer moving away):

f1=f0cvc=5.0×106×15400.801540=5.0×106×0.99948=4.9974×106Hzf_1 = f_0 \cdot \frac{c - v}{c} = 5.0 \times 10^6 \times \frac{1540 - 0.80}{1540} = 5.0 \times 10^6 \times 0.99948 = 4.9974 \times 10^6 \mathrm{ Hz}

This reflected signal then travels back to the transducer (source moving away, observer at rest), effectively doubling the shift:

Δf2f0vc=LB2×5.0×106×0.80RB◆◆LB1540RB=LB8.0×106RB◆◆LB1540RB5190Hz5.2kHz\Delta f \approx \frac{2f_0 v}{c} = \frac◆LB◆2 \times 5.0 \times 10^6 \times 0.80◆RB◆◆LB◆1540◆RB◆ = \frac◆LB◆8.0 \times 10^6◆RB◆◆LB◆1540◆RB◆ \approx 5190 \mathrm{ Hz} \approx 5.2 \mathrm{ kHz}

If you get this wrong, revise: Real-World Application: Doppler Ultrasound

Details

Problem 15 Two waves travel in the same direction along a string. Wave 1 is described by y1=0.04sin(3.0x12t)y_1 = 0.04\sin(3.0x - 12t) m and wave 2 by y2=0.04sin(3.0x12t+π/3)y_2 = 0.04\sin(3.0x - 12t + \pi/3) m. State the phase difference between the waves and determine whether their superposition produces a resultant wave with amplitude greater than, less than, or equal to 0.04 m.

Answer. The phase difference is Δϕ=π/3\Delta\phi = \pi/3 rad (60°). Since Δϕ\Delta\phi is neither 00 nor π\pi, the resultant amplitude is intermediate:

Ares=LBA12+A22+2A1A2cosΔϕRB=LB0.042+0.042+2(0.04)(0.04)cos(π/3)RBA_{\mathrm{res}} = \sqrt◆LB◆A_1^2 + A_2^2 + 2A_1 A_2 \cos\Delta\phi◆RB◆ = \sqrt◆LB◆0.04^2 + 0.04^2 + 2(0.04)(0.04)\cos(\pi/3)◆RB◆

=0.04LB2+2×0.5RB=0.0430.069m= 0.04\sqrt◆LB◆2 + 2 \times 0.5◆RB◆ = 0.04\sqrt{3} \approx 0.069 \mathrm{ m}

The resultant amplitude (0.069\approx 0.069 m) is greater than 0.04 m but less than 0.08 m (which would be the fully constructive case at Δϕ=0\Delta\phi = 0).

If you get this wrong, revise: Phase Difference from Wave Equations

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danger

Common Pitfalls

  • Confusing wave speed with particle speed: In a transverse wave, the wave propagates horizontally but the particles oscillate vertically. The wave speed v = f * lambda is the speed of the wave pattern, not the speed of the individual particles. Particles in the medium do NOT travel with the wave.

  • Confusing frequency with period: Frequency f is the number of oscillations per second (Hz). Period T is the time for one complete oscillation (s). They are related by f = 1/T. A common error is to confuse which is the reciprocal of the other or to add them instead of converting.

  • Not distinguishing between transverse and longitudinal waves: In transverse waves, oscillations are PERPENDICULAR to the direction of energy transfer (light, water surface waves, S-waves). In longitudinal waves, oscillations are PARALLEL to the direction of energy transfer (sound, P-waves). Only longitudinal waves have compressions and rarefactions.

  • Misidentifying points on a wave that are in phase: Two points are in phase if the distance between them is a whole number of wavelengths (n * lambda). They are in antiphase if the distance is an odd multiple of half-wavelengths ((n + 0.5) * lambda). The phase difference between adjacent points is 2 * pi * (path difference) / lambda.