7. Waves
- Syllabus
- 9702–2028–2029
- Section
- 7
- Level
- AS

Wave motion is the progression of a disturbance from one position to another. It transfers energy, while particles of a mechanical medium oscillate about equilibrium rather than travelling with the wave overall.
| Illustration | What progresses | What oscillates locally |
|---|---|---|
| Rope | a pulse or repeated shape along the rope | each section moves across the rope's length direction |
| Spring | a compression/rarefaction pattern along the spring | coils move backwards and forwards along the spring |
| Ripple tank | a ripple pattern across the surface | small surface regions move mainly up and down |
Particle motion and propagation direction are different ideas. The medium does not flow from source to receiver at wave speed, and electromagnetic waves can propagate without a material medium.
| Quantity | Meaning | Unit / relation |
|---|---|---|
| Displacement | signed distance of an oscillating point from equilibrium at an instant | m |
| Amplitude | maximum magnitude of displacement | m |
| Phase difference | difference in position within a cycle | rad or degrees; one cycle = 2π rad = 360° |
| Period T | time for one complete cycle | s |
| Frequency f | cycles per second | Hz; f = 1/T |
| Wavelength λ | shortest distance between points in phase; distance advanced in one period | m |
| Wave speed v | speed at which a fixed phase/disturbance progresses | m s⁻¹ |
A 5.0 Hz source has period 0.20 s. Two points separated by λ/2 are 180° (π rad) out of phase; points separated by one wavelength are in phase.
Amplitude is not wavelength, frequency is not wave speed, and wave speed is not the instantaneous speed of a particle oscillating about equilibrium.
| CRO direction | Setting | Count | Result |
|---|---|---|---|
| Horizontal | time-base in s/div | divisions for one cycle | T = divisions × time/div; f = 1/T |
| Vertical | y-gain in V/div | divisions from centre line to peak | amplitude = divisions × V/div |
One cycle spans 4.0 divisions at 2.0 ms div⁻¹: T = 8.0 ms and f = 125 Hz. A peak 3.0 divisions above the centre at 0.50 V div⁻¹ has amplitude 1.5 V.
Peak-to-peak height is twice the amplitude, so halve it before applying y-gain. Do not use vertical divisions to find period or horizontal divisions to find amplitude.
In one period T, a fixed phase of a progressive wave advances one wavelength λ. Speed = distance/time, so v = λ/T. Frequency is f = 1/T. Therefore v = λ(1/T) = fλ.
v=fλ
v is propagation speed in m s⁻¹, f is source frequency in Hz and λ is wavelength in m. The derivation tracks the travelling pattern, not the local speed of an oscillating particle.
The equation is not dimensional guesswork: its physical step is that one wavelength passes in one period.
For a progressive wave, v=fλ: the wave speed equals frequency multiplied by wavelength.
If the medium fixes v, a change in source frequency changes wavelength inversely. Use metres and hertz so the result is m s⁻¹.
If a wave travels at 12 m s⁻¹ with frequency 4.0 Hz, its wavelength is 3.0 m.
The wave speed is not the same as the speed of individual particles oscillating in the medium.
A progressive wave transfers energy away from its source as the disturbance reaches new positions. The transferred energy can produce an effect at a receiver.
In a mechanical wave, neighbouring parts of the medium interact: local oscillations pass energy onward while particles have no overall journey with the wave. A water ripple can make a floating cork oscillate and deliver energy to the edge.
A material medium is not required for every progressive wave. Electromagnetic waves transfer energy through vacuum as well as through materials.
Energy transfer does not imply net transport of matter, and wave propagation speed is not the same as a medium particle's instantaneous speed.
I=P/SandI∝a2
I is intensity in W m⁻², P is wave power crossing an area S in m², and a is wave amplitude. Distinct symbols prevent transmission area from being confused with amplitude.
A 6.0 W wave spread uniformly over 3.0 m² has intensity 2.0 W m⁻². Under otherwise unchanged conditions, doubling amplitude makes intensity four times larger; halving amplitude makes it one quarter.
The amplitude-squared rule compares the same wave type under comparable medium conditions. Intensity is not amplitude itself, and area in P/S is not the oscillation amplitude.
| Feature | Transverse wave | Longitudinal wave |
|---|---|---|
| Local oscillation or displacement | perpendicular to energy propagation | parallel to energy propagation |
| Mechanical pattern | crests and troughs can represent opposite displacements | compressions and rarefactions arise from crowding and spreading |
| Example | wave on a stretched string; electromagnetic wave | sound wave in air; compression wave in a spring |
| Polarisation | possible | not possible |
Both types can be progressive waves that transfer energy, obey v = fλ, reflect, refract, diffract, interfere and form stationary waves. These shared behaviours do not determine whether a wave is transverse or longitudinal.
To classify a wave, identify the direction in which energy propagates and compare it with the direction of local oscillation. For example, a guitar string oscillates transversely while the sound it produces in air is longitudinal.
Transverse does not always mean vertical: the defining angle is 90° to propagation. Longitudinal does not mean slow, and its particles still oscillate about equilibrium rather than travelling with the wave.
| Representation | What it shows | What can be read |
|---|---|---|
| displacement–distance | all sampled particles at one instant | amplitude and wavelength; phase at different positions |
| displacement–time | one sampled particle at one position | amplitude and period; frequency from f = 1/T |
| particle-position diagram | actual particle locations at one instant | transverse displacement pattern, or longitudinal crowding (compression) and spreading (rarefaction) |
A sinusoidal displacement–distance graph can represent a longitudinal wave. Its vertical coordinate is signed particle displacement parallel to propagation; it is not a literal up-down shape. If positive displacement is defined along the propagation direction, displacement decreasing with distance (negative gradient) marks a compression, while increasing displacement (positive gradient) marks a rarefaction.
For a wave travelling to the right, the instantaneous particle velocity has the opposite sign to the local slope of a displacement–distance graph: positive slope means negative particle velocity, and negative slope means positive particle velocity. At maximum or minimum displacement, instantaneous particle velocity is zero.
Interpret in this order: read both axis labels and units; decide whether the graph is a time record or a spatial snapshot; identify the stated positive displacement and propagation directions; then use spacing, gradient and phase. Equivalent-phase spacing gives λ only on a distance axis and T only on a time axis.
Do not identify wave type from a graph's sinusoidal appearance. For a longitudinal displacement graph, maximum displacement is not the centre of a compression: compression and rarefaction depend on how displacement changes with distance.
For a sound source moving relative to the medium and a stationary observer, the Doppler effect is the difference between observed frequency and the source's emitted frequency caused by the source motion.
| Source motion | Wavefront spacing / wavelength reaching observer | Observed frequency |
|---|---|---|
| towards observer | smaller | higher than source frequency |
| away from observer | larger | lower than source frequency |
The moving source emits successive wavefronts from different positions. In the same medium, sound speed remains v, so the changed wavelength gives a changed arrival frequency through v = fλ. The source itself can continue emitting at one steady frequency.
Greater speed towards the observer gives a greater upward shift; greater speed away gives a greater downward shift. A siren therefore sounds higher before passing and lower after passing a stationary listener.
This syllabus model covers a moving source and stationary observer. Understanding the separate case of a stationary source with a moving observer is not required here, and source motion does not change sound speed in the medium.
fo=fsv/(v±vs)
f_o is observed frequency, f_s is source frequency, v is sound speed in the medium and v_s is source speed relative to the medium. The observer is stationary.
| Source motion | Denominator | Required check |
|---|---|---|
| towards observer | v − v_s | f_o > f_s |
| away from observer | v + v_s | f_o < f_s |
A horn emits 440 Hz while moving towards a stationary observer at 30.0 m s⁻¹; sound speed is 340 m s⁻¹. f_o = 440 × 340/(340 − 30.0) = 483 Hz (3 s.f.). The answer is above 440 Hz, as approach requires.
First predict higher or lower frequency. Then select the sign, substitute speeds in the same units, solve, and compare f_o with f_s. The same equation can be rearranged to find v_s; retain the physical sign and direction.
The minus sign does not mean a negative speed: it makes the denominator smaller for approach. The model requires v_s < v and does not use an observer speed term.
Electromagnetic waves consist of mutually perpendicular electric and magnetic fields, both transverse to the direction of travel, and move at c≈3.00×10⁸ m s⁻¹ in vacuum.
They do not require a material medium; in matter their speed can be lower and depends on the medium.
Radio, visible light and X-rays are different frequencies of the same transverse electromagnetic family.
“Electromagnetic” does not mean longitudinal, and c applies to free space, not every material.
| Region (long λ → short λ) | Approximate free-space wavelength |
|---|---|
| radio | longer than 10⁻¹ m |
| microwave | 10⁻³ m to 10⁻¹ m |
| infrared | 7 × 10⁻⁷ m to 10⁻³ m |
| visible | 4 × 10⁻⁷ m to 7 × 10⁻⁷ m |
| ultraviolet | 10⁻⁸ m to 4 × 10⁻⁷ m |
| X-ray | 10⁻¹¹ m to 10⁻⁸ m |
| gamma | shorter than 10⁻¹¹ m |
From radio to gamma, wavelength decreases while frequency increases because c = fλ in free space. The spectrum is continuous, so quoted boundaries are approximate conventions and may overlap slightly between sources.
Convert first, then classify. Useful anchors are 1 mm = 10⁻³ m, 1 μm = 10⁻⁶ m and 1 nm = 10⁻⁹ m. Thus 2.1 cm = 2.1 × 10⁻² m is microwave, 12 μm = 1.2 × 10⁻⁵ m is infrared, and 138 pm = 1.38 × 10⁻¹⁰ m is X-ray.
If frequency is given, calculate λ = c/f before using the table. For f = 3.0 × 10¹⁶ Hz, λ = 1.0 × 10⁻⁸ m, at the approximate ultraviolet/X-ray boundary; use the convention and options supplied by the question.
Order alone does not satisfy a wavelength-range question. Do not reverse the trend: gamma has the shortest wavelengths and radio the longest. Approximate region labels do not imply gaps in the spectrum.
The visible band is approximately 400–700 nm in free space, from shorter-wavelength violet to longer-wavelength red.
Treat the limits as approximate and use wavelength/frequency trends when identifying colour or neighbouring ultraviolet and infrared.
A 500 nm wave lies in the visible range, while 350 nm is ultraviolet and 900 nm is infrared.
Visible colour is not determined by intensity alone; wavelength sets the nominal colour while intensity affects brightness.
Polarisation is the restriction of a transverse wave's oscillations to one direction perpendicular to propagation. A plane-polarised electromagnetic wave has its electric field oscillating in one fixed transverse direction.
| Wave state | Transverse oscillations |
|---|---|
| unpolarised | distributed among many directions perpendicular to propagation |
| plane polarised | restricted to one direction perpendicular to propagation |
A polarising filter has a transmission axis and transmits the component of the incident electric-field oscillation along that axis. A longitudinal wave oscillates parallel to propagation, so it has no set of transverse directions from which one can be selected; it cannot be polarised.
Rotating a filter in plane-polarised light changes the transmitted intensity and can reduce it to zero when the transmission axis is perpendicular to the incident polarisation direction. Observing polarisation is therefore evidence that a wave is transverse.
The transmission axis lies in the filter plane and specifies the transmitted oscillation direction; it is not the direction in which the wave propagates. Reduced intensity alone is not the definition of polarisation.
I=I0cos2θ
I₀ is the intensity of the plane-polarised wave entering the current filter, I is its transmitted intensity, and θ is the smallest angle between the incoming polarisation direction and that filter's transmission axis.
For each filter in order: find θ from the incoming polarisation direction to the filter axis; calculate I = I₀ cos²θ; use this transmitted I as the next filter's I₀; and set the new polarisation direction equal to the axis of the filter just passed.
Vertically plane-polarised light of intensity 8.0 W m⁻² meets a first axis at 50° and a second axis at 20° to vertical. First, I₁ = 8.0 cos²50° = 3.31 W m⁻². The axes differ by 30°, so I₂ = 3.31 cos²30° = 2.48 W m⁻² ≈ 2.5 W m⁻².
| Relative angle θ | Ideal transmitted intensity |
|---|---|
| 0° | I = I₀ |
| 60° | I = 0.25I₀ |
| 90° | I = 0 |
Use cos²θ, not cos θ. For a series, θ is between the incoming polarisation and the next axis—not automatically an axis angle measured from vertical. This syllabus does not require calculating the intensity reduction when unpolarised light first enters a polarising filter; Malus's-law calculations start from a stated plane-polarised intensity.