understand and use the terms displacement, amplitude, phase difference, period, frequency, wavelength and speed

Progressive (Traveling) Waves – Cambridge AS & A Level Physics 9702

This note covers all the wave‑related requirements of Section 7 of the Cambridge syllabus (9702). It links the seven fundamental wave quantities to energy transport, wave speed in different media, and the experimental techniques you will encounter in the exams.

1. Fundamental Wave Quantities

TermSymbolDefinition / Typical FormulaSI Unit
Displacementy (or s)Instantaneous distance of a particle from its equilibrium positionmetre (m)
AmplitudeAMaximum magnitude of the displacement (|y| ≤ A)metre (m)
PhaseϕArgument of the sinusoidal function; ϕ = kx − ωt + ϕ₀radian (rad) or degree (°)
Phase DifferenceΔϕAngular separation between two points: Δϕ = kΔx − ωΔtrad (or °)
PeriodTTime for one complete oscillation at a fixed pointsecond (s)
FrequencyfNumber of cycles per second; f = 1/Thertz (Hz = s⁻¹)
WavelengthλDistance between successive points that are in phase (e.g. crest‑to‑crest)metre (m)
Wave‑numberkSpatial angular frequency; k = 2π/λrad m⁻¹
Angular FrequencyωTemporal angular frequency; ω = 2πf = 2π/Trad s⁻¹
Wave SpeedvRate at which a given phase propagates; v = fλ = ω/k = λ/Tmetre per second (m s⁻¹)
IntensityIPower transmitted per unit area; I = ½ ρ v ω² A² ∝ A²watt per square metre (W m⁻²)

2. Types of Progressive Waves

Wave TypeParticle MotionCommon ExampleTypical Diagram
TransverseParticle motion ⟂ to direction of propagationString wave, water‑surface rippleFigure 1 – a string with arrows up/down while the wave travels right
LongitudinalParticle motion ‖ to direction of propagationSound in air, compression wave in a springFigure 2 – alternating compressions and rarefactions along the axis

Both wave types can be described by the same sinusoidal function; only the physical meaning of the displacement variable changes (vertical displacement for transverse, longitudinal displacement for longitudinal).

3. Phase and Phase Difference

  • The quantity inside the sine (or cosine) function is the phase ϕ.
  • Two points are in phase when Δϕ = 0, 2π, 4π … and opposite in phase when Δϕ = π, 3π …

General relation:

\$\Delta\phi = k\,\Delta x - \omega\,\Delta t\$

Example: Points separated by one wavelength (Δx = λ) at the same instant (Δt = 0) have Δϕ = kλ = 2π → they are in phase.

4. Period, Frequency and the Cathode‑Ray Oscilloscope (CRO)

  • Period (T) – measured at a fixed position; the time between successive peaks on a CRO trace.
  • Frequency (f) – reciprocal of the period, f = 1/T.
  • On a CRO the horizontal axis is time (Δt) and the vertical axis shows voltage, which is proportional to the wave’s displacement (or pressure for sound). By counting divisions you obtain T and, consequently, f.

5. Wavelength, Wave‑Number & Angular Frequency

From the definition of wavelength (a 2π phase change):

\$k = \frac{2\pi}{\lambda}\qquad\text{[rad m⁻¹]}\$

From the definition of period (a 2π phase change in time):

\$\omega = \frac{2\pi}{T}=2\pi f\qquad\text{[rad s⁻¹]}\$

6. Wave Speed – General and Media‑Specific Forms

General relationship linking spatial and temporal characteristics:

\$v = f\lambda = \frac{\lambda}{T} = \frac{\omega}{k}\qquad\text{[m s⁻¹]}\$

Media‑specific formulas (required for AO2):

  • Transverse wave on a taut string – \(v = \sqrt{T/\mu}\) where T is the tension (N) and μ is the linear mass density (kg m⁻¹).
  • Longitudinal wave in a solid – \(v = \sqrt{E/\rho}\) where E is Young’s modulus (Pa) and ρ is the density (kg m⁻³).
  • Sound in a gas – \(v = \sqrt{\gamma R T/M}\) (γ = ratio of specific heats, R = universal gas constant, T = absolute temperature, M = molar mass).
  • Electromagnetic wave in vacuum – \(v = c = 3.00\times10^{8}\,\text{m s}^{-1}\).

7. Doppler Effect (Sound)

When source and/or observer move relative to the medium, the observed frequency \(f'\) changes:

\$f' = f\;\frac{v \pm v{o}}{v \mp v{s}}\$

where

  • \(v\) = speed of sound in the medium
  • \(v_{s}\) = speed of the source (positive if moving towards the observer)
  • \(v_{o}\) = speed of the observer (positive if moving towards the source)

Worked example (ambulance): A siren of \(f = 700\) Hz is heard at \(f' = 770\) Hz by a stationary observer as the ambulance approaches at 30 m s⁻¹. Using \(v = 340\) m s⁻¹, confirm the speed.

8. Electromagnetic Spectrum

RegionTypical Wavelength (λ)Typical Frequency (f)Common Uses
Radio10⁻¹ – 10³ m10⁶ – 10⁹ HzBroadcast, radar, communication
Microwave10⁻³ – 10⁻¹ m10⁹ – 10¹¹ HzCooking, satellite links
Infra‑red7 × 10⁻⁷ – 10⁻³ m10¹¹ – 10¹⁴ HzThermal imaging, remote sensing
Visible4 × 10⁻⁷ – 7 × 10⁻⁷ m4.3 × 10¹⁴ – 7.5 × 10¹⁴ HzHuman eye, colour photography
Ultraviolet10⁻⁸ – 4 × 10⁻⁷ m10¹⁵ – 10¹⁶ HzSterilisation, fluorescence
X‑ray10⁻¹¹ – 10⁻⁸ m10¹⁶ – 10¹⁹ HzMedical imaging, crystallography
Gamma‑ray<10⁻¹¹ m>10¹⁹ HzRadioactive decay, cancer treatment

All electromagnetic waves travel at the same speed \(c\) in vacuum; the differences lie in wavelength and frequency, which determine their interaction with matter.

9. Polarisation (Transverse Waves)

  • Only transverse waves can be polarised because the oscillation direction is defined.
  • Linear polarisation: the electric‑field vector vibrates in a single plane.
  • Malus’s law (intensity after a second polariser):

\$I = I_{0}\cos^{2}\theta\$

Practical example: placing two Polaroid sheets in the path of a laser beam. Rotating the second sheet changes the transmitted intensity according to the angle θ between their transmission axes.

10. Energy Transport & Intensity

  • For a sinusoidal wave the instantaneous kinetic and potential energy densities are proportional to the square of the amplitude.
  • Time‑averaged intensity (power per unit area) is

\$I = \frac{1}{2}\,\rho\,v\,\omega^{2}A^{2}\qquad\text{[W m⁻²]}\$

Consequences:

  • Doubling the amplitude increases intensity by a factor of four.
  • Intensity falls off as \(1/r^{2}\) for a point source (spherical wavefronts).

11. Experimental Techniques (Paper 3 & 5)

ApparatusWave TypeQuantities MeasuredTypical Method
Ripple tankTransverse water surfaceλ (crest spacing), v (by timing a marker), A (probe displacement)Strobe light or video analysis; measure distance travelled in a known time.
String‑pulse set‑upTransverse on a stretched stringv (distance/time), T (period of a standing‑wave pattern)Photogate or high‑speed camera; count pulses.
Closed air column (organ pipe)Longitudinal soundf (tuning fork), λ (resonant length), v (via v = fλ)Microphone + CRO; adjust column length until resonance.
Cathode‑ray oscilloscope (CRO)Electrical analogue of any periodic wavef, T, A (voltage amplitude)Read time/div and volts/div settings; use cursors for accuracy.
Polaroid set‑upPolarised light (EM wave)I as a function of angle θRotate second Polaroid, record intensity with a light‑meter.
Doppler‑shift apparatusSoundObserved frequency f′ for known source speedSpeaker on a cart, microphone + CRO; compare f′ with f.

Design skill (AO2): You should be able to sketch a simple set‑up, explain which two of \(f, \lambda, v\) you will measure directly, and show how to calculate the third using the appropriate formula.

12. Worked Example (String Wave)

  1. Problem: A string under tension \(T = 120\) N has linear mass density \(\mu = 2.5\times10^{-3}\) kg m⁻¹. It is driven at \(f = 80\) Hz. Determine (a) the wave speed, (b) the wavelength, and (c) the intensity if the measured amplitude is \(A = 1.2\) mm and the surrounding medium is air‑like with \(\rho = 1.2\) kg m⁻³.
  2. Solution

    • (a) Wave speed on a string

      \$v = \sqrt{\frac{T}{\mu}} = \sqrt{\frac{120}{2.5\times10^{-3}}}\approx 2.19\times10^{2}\ \text{m s}^{-1}\$

    • (b) Wavelength

      \$\lambda = \frac{v}{f} = \frac{2.19\times10^{2}}{80}\approx 2.74\ \text{m}\$

    • (c) Intensity

      \(\omega = 2\pi f = 2\pi(80)=5.03\times10^{2}\ \text{rad s}^{-1}\)

      Convert amplitude: \(A = 1.2\ \text{mm}=1.2\times10^{-3}\ \text{m}\).

      \$\$I = \frac12\,\rho\,v\,\omega^{2}A^{2}

      =\frac12(1.2)(2.19\times10^{2})(5.03\times10^{2})^{2}(1.2\times10^{-3})^{2}

      \approx 1.1\ \text{W m}^{-2}\$\$

13. Summary Checklist – What You Must Be Able to Do (AO1 & AO2)

  • Write the sinusoidal displacement function \(y(x,t)=A\sin(kx-\omega t+\phi_{0})\) and identify each symbol.
  • Distinguish transverse from longitudinal progressive waves; sketch labelled diagrams.
  • Calculate phase differences using \(\Delta\phi = k\Delta x - \omega\Delta t\) and state the conditions for “in‑phase” and “opposite‑phase”.
  • Convert between period and frequency; read both from a CRO trace.
  • Determine wavelength from a standing‑wave pattern or ripple‑tank measurement; use \(k = 2\pi/\lambda\).
  • Apply the general speed relation \(v = f\lambda = \omega/k\) and, where required, the medium‑specific formulas for strings, solids, gases and EM waves.
  • Explain the Doppler shift for sound and use the formula \(f' = f\frac{v\pm v{o}}{v\mp v{s}}\) in a short calculation.
  • Identify the region of the electromagnetic spectrum that corresponds to a given wavelength or frequency and recall that all EM waves travel at \(c\) in vacuum.
  • State what polarisation means for transverse waves, write Malus’s law, and describe a simple laboratory demonstration.
  • Calculate the intensity of a sinusoidal wave and explain why \(I\propto A^{2}\) and why intensity falls off as \(1/r^{2}\) for a point source.
  • Design a basic experiment (ripple tank, string‑pulse, or sound tube) to measure any two of \(f, \lambda, v\) and then compute the third.
  • Interpret data tables and graphs (e.g., \(x\)–\(t\) plots) to extract wave quantities and discuss experimental uncertainties.

Suggested diagram (not shown): an \(x\)–\(t\) graph of a right‑travelling sinusoidal wave, with labelled amplitude A, wavelength λ, period T, speed v, and two points illustrating a phase difference Δϕ.