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Edexcel International GCSE Physics (4PH1) · Section 3 — Waves
Mini-Lesson

Waves

This mini-lesson walks you through the whole of 4PH1 Section 3 — Waves: wave types and their properties, the wave equations, reflection & refraction, refractive index, total internal reflection and the critical angle, the electromagnetic spectrum, and sound.

a particle just bobs up and down energy travels →
A wave transfers energy and information through a medium — but the medium itself is not carried along.

Work through each screen, answer the questions as you go (some are wordy, some are calculations) and collect ⭐ stars. Press Start when you're ready.

3.2 · 3.4 — Wave types

Transverse and longitudinal

A wave carries energy and information from place to place without transferring matter. There are two families:

Transverse — oscillations ⟂ to travel amplitude wavelength λ direction of travel Longitudinal — oscillations ∥ to travel compression rarefaction compression direction of travel
Transverse: water ripples, light, all EM waves. Longitudinal: sound — a pattern of compressions (squashed) and rarefactions (stretched).

Misconception: a wave does not carry the medium along. Each particle just oscillates about its rest position — only the energy moves through.

Quick check

Which kind of wave?

?In a sound wave travelling through air, the air particles vibrate back and forth along the same line that the wave is travelling. What type of wave is this?
3.1 · 3.3 — Describing a wave

Amplitude, wavelength, frequency, period

  • Amplitude — the maximum displacement from the undisturbed (rest) position. Measured in metres (m).
  • Wavelength (λ) — distance from one point on a wave to the same point on the next (peak→peak). In metres (m).
  • Frequency (f) — number of complete waves passing a point each second. In hertz (Hz).
  • Period (T) — time for one complete wave to pass a point. In seconds (s).
  • Wavefront — a line joining points all at the same stage of their cycle (e.g. all the crests).

4PH1 units to recognise: degree (°), hertz (Hz), metre (m), metre/second (m/s) and second (s).

3.5 · 3.6 — The wave equations

Speed, frequency and wavelength

For any wave — sound or electromagnetic — the speed links to frequency and wavelength:

v = f × λwave speed (m/s) = frequency (Hz) × wavelength (m)

Frequency and period are simply reciprocals of each other:

f = 1 ÷ Tfrequency (Hz) = 1 ÷ time period (s)
Worked example

A water wave has frequency 2.5 Hz and wavelength 0.40 m.

v = f × λ = 2.5 × 0.40 = 1.0 m/s

Rearranging: f = v ÷ λ and λ = v ÷ f. Keep units in metres, hertz and metres/second.

Calculate

Your turn — wave speed

1A wave on a string has a frequency of 12 Hz and a wavelength of 0.25 m. Calculate its speed.
m/s
Hint: v = f × λ = 12 × 0.25.
Calculate

Your turn — find the wavelength

2A sound wave travels at 340 m/s with a frequency of 170 Hz. Calculate its wavelength.
m
Hint: rearrange to λ = v ÷ f = 340 ÷ 170.
Calculate

Your turn — frequency from period

3A pendulum-driven wave has a time period of 0.05 s. Calculate its frequency.
Hz
Hint: f = 1 ÷ T = 1 ÷ 0.05.
Core Practical — measuring wave speed

Measuring the speed of a wave

The 4PH1 practical work uses suitable equipment to find the speed, frequency and wavelength of a wave in a ripple tank and on a stretched string.

λ vibrating dipper sets the frequency
Straight wavefronts in a ripple tank. Measure several wavelengths to reduce error, read frequency from the vibrator, then use v = f × λ.

Tip: you can also use v = distance ÷ time — time a wavefront (or pulse on a string) across a measured distance, then divide.

3.9 — Reflection & refraction

All waves can be reflected and refracted

Reflection — a wave bounces off a boundary; the angle of incidence equals the angle of reflection.

Refraction — a wave changes speed when it crosses into a new medium, so its direction bends. Its wavelength changes but its frequency stays the same.

air (less dense) glass (more dense) normal i r
Entering a denser medium the ray slows down and bends towards the normal (so r < i). Leaving into a less dense medium it speeds up and bends away.

Misconception: refraction is fundamentally a change of speed. The bending of direction is just the visible consequence — and the frequency never changes.

Quick check

Into the glass

?A ray of light passes from air into a glass block. Which statement is correct?
3.18 — Refractive index

How much a material bends light

The refractive index n measures how strongly a material slows and bends light. From the angles at the surface:

n = sin i ÷ sin rrefractive index = sin(angle of incidence) ÷ sin(angle of refraction)

Because light bends towards the normal entering a denser medium, r < i, so n is always greater than 1 for glass, water or perspex.

Worked example

Light hits glass at i = 50° and refracts to r = 30°.

n = sin 50° ÷ sin 30° = 0.766 ÷ 0.500 = 1.53

Core Practical (3.19): shine a ray into a glass block, trace it in and out, measure i and r and calculate n = sin i ÷ sin r.

Calculate

Your turn — refractive index

4Light enters a transparent block at an angle of incidence of 45° and refracts to an angle of 28°. Calculate the refractive index. (sin 45° = 0.707, sin 28° = 0.469)
Hint: n = sin i ÷ sin r = 0.707 ÷ 0.469.
3.20 · 3.21 · 3.22 — Total internal reflection

The critical angle & optical fibres

When light travels from a denser medium towards a less dense one, raising the angle of incidence eventually reaches the critical angle c. Beyond it, none of the light escapes — it is all reflected back inside. This is total internal reflection (TIR).

sin c = 1 ÷ ncritical angle relates to refractive index of the medium
optical fibre (light pipe) i > c → all reflected
Each time the light hits the wall above the critical angle it totally reflects, so it stays trapped — guiding signals along the fibre with almost no loss.

Uses (3.20): total internal reflection guides light along optical fibres (fast internet, endoscopes) and turns light through right angles inside prisms (periscopes, binoculars).

Calculate

Your turn — critical angle

5A type of glass has a refractive index of 1.5. Calculate sin c for its critical angle.
(sin c)
Hint: sin c = 1 ÷ n = 1 ÷ 1.5.
3.10 · 3.11 — The EM spectrum

The electromagnetic spectrum

Light is one slice of a continuous family of transverse waves. They all travel at the same speed in a vacuum (3 × 10⁸ m/s). In order of decreasing wavelength (and increasing frequency):

Radio Micro-wave Infrared Visiblelight UV X-ray Gammaray longer wavelength higher frequency
Radio · Microwave · Infrared · Visible · Ultraviolet · X-ray · Gamma. Gamma rays have the shortest wavelength and highest frequency.

Misconception: in a vacuum, all EM waves travel at the same speed — gamma rays are not "faster" than radio. What differs is their wavelength and frequency.

Order it

Build the spectrum

Tap the regions in order of increasing frequency (longest wavelength first).

3.12 · 3.13 — Uses & dangers

What each region does — and risks

  • Radio — broadcasting & communications.
  • Microwave — cooking & satellite transmissions. Risk: internal heating of body tissue.
  • Infrared — heaters & night-vision. Risk: skin burns.
  • Visible light — optical fibres & photography.
  • Ultraviolet — fluorescent lamps. Risk: damage to surface cells & blindness.
  • X-rays — medical imaging & checking internal structures.
  • Gamma rays — sterilising food & medical equipment. Risk: cancer, mutation.

Protection: limit exposure time, increase distance, and use shielding (e.g. lead aprons for X-rays, sunscreen and sunglasses against UV).

Match up

Region → use

Tap a region on the left, then its main use on the right.

Region
Use
3.23 · 3.24P · 3.25P — Sound

Sound is a longitudinal wave

Sound is a longitudinal wave: vibrating particles pass on compressions and rarefactions. It needs a medium — it cannot travel through a vacuum. Like all waves, it can be reflected (echoes) and refracted.

The frequency range for human hearing is 20 Hz to 20 000 Hz (20 kHz). Below 20 Hz is infrasound; above 20 kHz is ultrasound.

Core Practical (3.25P): measure the speed of sound in air — e.g. time an echo over a known distance, or use two microphones a measured distance apart, then v = distance ÷ time.

Quick check

The range of human hearing

?A healthy young person can typically hear sounds across which frequency range?
3.26P · 3.28P · 3.29P — Sound on a screen

Pitch, loudness & the oscilloscope

A microphone turns a sound wave into an electrical signal, which an oscilloscope (CRO) displays as a trace of voltage against time:

  • Pitch ↔ frequency — a higher frequency (waves closer together on screen) sounds higher in pitch.
  • Loudness ↔ amplitude — a bigger amplitude (taller trace) sounds louder.
low pitch · loud (big amplitude) high pitch · quiet (small amplitude)
Left: low frequency, large amplitude. Right: higher frequency, smaller amplitude. Core Practical 3.27P uses this to find a sound's frequency.
Quick check

Reading the trace

?On an oscilloscope, one sound's trace has taller peaks than another's but the peaks are the same distance apart. Compared with the second sound, the first is:
Recap

The equations to know

Wave speed: v = f × λ  (also v = distance ÷ time)

Frequency & period: f = 1 ÷ T

Refractive index: n = sin i ÷ sin r

Critical angle: sin c = 1 ÷ n

Human hearing: 20 Hz – 20 000 Hz

EM order (↑frequency): Radio→Micro→IR→Visible→UV→X-ray→Gamma

You've covered all of 4PH1 Section 3 — Waves: wave types & properties, the wave equations, reflection & refraction, refractive index, total internal reflection & the critical angle, the electromagnetic spectrum, and sound. Press Finish to see your score.

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