Year 12

AQA A level Physics Waves Notes

Waves

— Physics · AS Level (CIE 7408) —
★ Exam Tip: Waves is one of the highest-yield AS topics — graphs (x–d and x–t), phase difference, intensity, Doppler effect and polarisation each show up as their own MCQs and as structured questions almost every series. Know every formula box below cold.

1. Types of Waves

By energy transfer:

  • Progressive waves — transfer energy from one place to another.
  • Stationary waves — do not transfer energy.

By direction of vibration:

  • Transverse waves — vibration/motion of particles is perpendicular to the direction of travel of the wave / direction of propagation of energy. Can travel in a vacuum. e.g. EM spectrum, water waves.
  • Longitudinal waves — vibration/motion of particles is parallel to the direction of travel of the wave / direction of propagation of energy. Require a medium to travel. e.g. sound waves.
directionof travel λ
transverse — vibration ⊥ travel
direction of travel → compressionrarefaction
longitudinal — vibration ∥ travel (dots bunch = compression, spread = rarefaction)
Note: in a longitudinal wave, at a compression the local pressure is greater than surrounding pressure; at a rarefaction it is lower than surrounding pressure.

2. Displacement–Distance Graphs

(snapshot of the whole wave at one instant in time)

Definitions: Displacement — distance moved by a particle from its mean position.
Distance — distance moved along the wave.
Amplitude — maximum displacement of a particle from its mean position (scalar).
Wavelength (λ) — distance between 2 consecutive points in phase.
Trick: to tell which way a particle moves on an x–d graph, draw the next wave slightly ahead (dashed) — the particle moves toward where that next curve sits.

Phase difference

Tells how much of a wave is completed: 0° ⇒ 0% of a wave, 360° ⇒ 100% of a wave. 1 "transition" (¼ wave) ⇒ ¼×360° = 90°.

Phase difference = Δxλ × 360°
A B C D E F G H x/md/m λ
points A,C,E,G on the axis; B,F crests; D,H troughs — one full wave A→E = λ
worked examplephase difference from a d–x graph

Using points on the wave above (λ = 4 m):

A & C: 180° A & E: 360° (or 0°) D & F: 180° C & H: 450° (or 90°) D & G: 270°

For points X (d = 1.65 m) & Y (d = 3.75 m) on a wave of λ = 4 m:

phase diff = Δxλ × 360° = 3.75 − 1.654 × 360° = 189°
CIE MCQwater wave — max upward speed

Vertical cross-section of a water wave moving left→right. At which labelled point is the water moving upwards with maximum speed?

Max speed happens where displacement = 0 (mean position) — not at the crest/trough (there v=0). Since the wave moves right, the point just behind the crest (on its rising side) is about to become the crest, so it is moving up through zero at that instant.

Answer: the zero-crossing point rising toward the next crest (labelled B in the original figure).

CIE MCQwhich x–d graph correctly labelled?

A wave has period T, wavelength λ and amplitude A, shown on a graph of displacement x against distance d. Which graph is correctly labelled?

A ✓ λ labelled correctly as one full wave-cycle along the d-axis, A labelled as the peak height B ✗ labels "T" on the d-axis — T is a time, it never belongs on a distance axis C ✗ labels the full peak-to-trough height as "2A" — amplitude is measured from the mean line, not peak-to-trough D ✗ same peak-to-trough mistake, "2A" instead of A

Answer: A

CIE MCQwave pulse on a rope

A wave pulse moves right along a stretched rope. Which graph correctly shows the variation with time t of the displacement s of a fixed particle P on the rope, as the pulse passes it?

Trace what P does as the pulse (whatever shape it is) arrives, passes under it, then leaves — match the rope's shape at each instant to a value of s at the corresponding t.

Answer: D

CIE MCQripple tank — phase difference X & Y

X and Y are two points on the surface of water in a ripple tank. A source of constant frequency generates waves that travel past X then Y, causing them to oscillate.

Read off how many whole + partial wavelengths separate X and Y along the direction of travel, then convert using phase diff = (Δx/λ)×360°.

Answer: 270°

3. Displacement–Time Graphs

(one particle, tracked over time — not a snapshot of the whole wave)

Definitions: Time period (T) — time taken for one complete wave to form (seconds).
Frequency (f) — number of complete waves formed in 1 second.
f = nt = 1T
Where: n = number of complete waves | t = time for n waves to form | T = time period
Phase difference = ΔtT × 360°

Practice: drawing a wave X° out of phase

d/m
90° out of phase (¼ wave shift)
d/m
180° out of phase (½ wave shift — mirror image)
d/m
270° out of phase (¾ wave shift)

Phase difference between two waves — general method

Works the same way whether comparing distance (x–d graph) or time (x–t graph) — just swap Δx/λ for Δt/T.

Phase diff = Δxλ × 360°
Phase diff = ΔtT × 360°

e.g. two waves of the same λ (same T) offset by 2 boxes out of 4 ⇒ (2/4)×360° = 180° either way.

CIE MCQlongitudinal/transverse from an x–t graph

The graph represents a sound wave: displacement/μm against time/ms, period 20 ms, 3 full cycles shown by 55 ms.

f = 1/T = 1/(20×10⁻³) f = 50 Hz check: f = n/t = 2/(40×10⁻³) = 50 Hz ✓
A ✗ longitudinal, period 25 ms — wrong period read off graph B ✓ longitudinal (sound), frequency 50 Hz C ✗ "transverse" — sound is longitudinal; amplitude 3 μm is also a graph-reading trap D ✗ "transverse" and confuses the period (20 ms) with a wavelength

Answer: B

CIE structuredwhale sound — oscilloscope time-base

A whale produces sound of frequency 5 Hz, displayed on an oscilloscope.

f = 1/T ⇒ T = 1/f T = 1/5 = 0.2 s screen shows 1 wave over 4 divisions ⇒ 0.2/4 = 0.05 s/div 0.05 s = 100 ms/div

Answer: D — 100 ms div⁻¹

CIE MCQCRO amplitude & frequency

Time-base = 5.0 ms/div, Y-gain = 5.0 mV/div. Four complete waves fill the screen.

f = 1/(4×5×10⁻³) f = 50 Hz

Amplitude read as 2 divisions × 5.0 mV = 10 mV.

Answer: A — 10 mV, 50 Hz

4. Velocity of a Wave

Derivation 1 speed = distance/time v = λ × (1/T) v = fλ (since f = 1/T)
Derivation 2 (n cycles) n cycles cover distance nλ in time t v = distance/time = nλ/t v = fλ (since n/t = f)
v = fλ
CIE MCQdeep-water waves — straight-line graph

Speed of deep-water waves: v² = gλ/2π. A student measures λ and f. Which graph gives a straight line through the origin?

v = fλ ⇒ v² = f²λ² f²λ² = gλ/2π f² = (g/2π) × (1/λ) ← y = m·x form

Answer: D — f² against 1/λ

CIE structuredsound wave in a gas — displacement-time & phase

Displacement–time graph of a gas molecule as a continuous sound wave passes; period read as 500 μs. Speed of sound in the gas = 330 m/s.

f = 1/T = 1/(500×10⁻⁶) f = 2000 Hz v = fλ ⇒ 330 = 2000 × λ λ = 0.165 m

A second molecule sits 0.165 m further from the source — exactly one whole λ away, so:

phase diff = (Δx/λ)×360° = (0.165/0.165)×360° = 360° (i.e. 0°) — identical graph, same zero time

Answer: D (same displacement–time graph as the original, no shift)

CIE structureddeducing v = fλ from first principles

A source has frequency f, produces sound of wavelength λ.

  1. Frequency of source = number of complete waves produced in 1 s by the source.
  2. Distance moved by a wavefront during n oscillations, in terms of λ = nλ.
v = distance/time = nλ / (n/f) v = fλ

Given time-base = 2.0 ms/cm and 3 divisions per cycle read off the CRO trace:

T = 3 × 2.0 ms = 6 ms f = 1/(6×10⁻³) = 167.77 f ≈ 170 Hz

A second wave, same frequency & amplitude, phase difference 90° from the first ⇒ shifted by ¼ cycle (drawn as a red curve on the same axes, starting a quarter-cycle ahead of the grey original).

5. Transverse vs Longitudinal (exam wording)

CIE structureddefinitions & phase difference from a graph

Distinguish, by reference to vibrations of particles & direction of energy transfer:

Transverse: vibrations are perpendicular to the direction of energy transfer. Longitudinal: vibrations are parallel to the direction of energy transfer.

Polarised wave — vibration of particles is restricted to one plane only, that plane being perpendicular to the direction of propagation of the wave.

On a y/cm–x/m graph: amplitude read as 2.8 cm; phase difference between points A (x=0.1) and B (x=0.4) on a wave of λ = 0.8 m:

phase diff = 0.4 − 0.10.8 × 360° = 135°

6. Finding Compressions & Rarefactions

Method: at any point on the displacement–distance graph, look at 3 particles — one at that point, one slightly to its left, one slightly to its right — and mark their displacement (velocity) vectors according to your sign convention.

→ → → or ← ← ← (all same way) = normal pressure
→ · ← (converging) = compression (pressure > atmospheric)
← · → (diverging) = rarefaction (pressure < atmospheric)
x/m CRC P/P₀ CRC
compressions (C, pressure peak) & rarefactions (R, pressure trough) sit at the zero-crossings of the displacement graph
Note: at atmospheric pressure line, P = 1.013×10⁵ Pa (standard atmospheric pressure).

7. Intensity of a Wave

Definition: intensity is the power incident per unit area. Scalar. Units W m⁻².

I = P/A ⇒ P = dW/dt = ΔW/Δt I = ΔW/(A×Δt) most of the time the area is the surface of a sphere, A = 4πr²
bulbr I = P/4πr²
intensity spreads over a sphere of radius r

Learn these 3 relationships:

① I ∝ amplitude²  ⇒  I₁a₁² = I₂a₂²
② I ∝ 1/distance²  ⇒  I₁r₁² = I₂r₂²
③ I ∝ frequency² (not as important)
worked exampleamplitude needed to double intensity
I ∝ a² ⇒ I/A² = 2I/a₂² a₂ = √2 × A
worked exampledistance needed to double intensity
I ∝ 1/r² ⇒ I·r² = 2I·r₂² r₂ = r/√2
CIE MCQamplitude vs distance from a constant-power source

I = P/4πr² for a source of constant power P. How does amplitude a of the vibrating air molecules vary with r?

I ∝ a² and I ∝ 1/r² ⇒ a² ∝ 1/r² a ∝ 1/r

Answer: A — a ∝ 1/r

CIE MCQsound wave loses intensity, keeps constant frequency

Which statement is correct?

A ✓ the maximum displacement (amplitude) changes from one particle to the next as it decays outward B ✗ phase difference between adjacent particles is not zero — they still oscillate slightly out of step C ✗ wavelength is the distance between points with phase diff of 0°/360°, not 180° D ✗ particles 360° apart have the same phase, but amplitude still shrinks with distance from the source

Answer: A

CIE MCQintensity halved — which x–t graph?

A sound wave's displacement–time graph is given; intensity is then halved. Which graph correctly shows the new wave?

I/a² = (½I)/a₂² a₂² = a²/2 ⇒ a₂ = 0.71 × a (same frequency, smaller amplitude)

Answer: D — same frequency, reduced amplitude (A, B, C all wrongly change the frequency or scale the amplitude incorrectly)

CIE structuredwater wave — ratio of intensities

Fig 5.1: x/mm–t graph, T = 0.60 s. Fig 5.2: x/mm–d graph at one instant, λ = 4.0 cm, amplitude decreasing with distance (2 mm at source → 1.1 mm at 6.0 cm).

v = fλ = (1/0.6)×(4×10⁻²) v = 0.067 m/s

Losing power? Yes — the wave is losing power as it moves away from the source, because the amplitude decreases with distance.

I₁/I₂ = a₁²/a₂² = 2² / (1.1)² = 400/121 = 3.3057 ratio ≈ 3.3
CIE structuredtwo waves P & Q — phase diff, intensity ratio, superposition

Fig 4.1: x/mm–t graphs of two waves P (amplitude 3.0 mm) and Q (amplitude 2.0 mm) at the same point, T = 0.60 s. Speed of both waves = 20 cm/s.

v = fλ ⇒ 20 = (1/0.6)×λ λ = 12 cm
phase diff = (Δt/T)×360° = (0.35−0.15)/0.60 ×360° = 120°
I_Q/I_P = a_Q²/a_P² = 2²/3² = 4/9 ≈ 0.44

At t = 0.45 s the two waves superpose (add algebraically); reading each wave's displacement off Fig 4.1 at that instant and summing gives the resultant displacement.

8. The Doppler Effect

Definition: the change in observed frequency due to relative motion between an observer and a source.

General formf₀ = vv ± v_s f_s
Where: f₀ = observed frequency | f_s = source frequency | v = speed of the wave in the medium | v_s = speed of the source (constant)
Approaching: f₀ = vv − v_s f_s
Separating: f₀ = vv + v_s f_s
v_s = 0: | | | | | |f const v_s → (approach): ||||| | |f ↑ (steady, higher) v_s → (recede): | | | | |f ↓ (steady, lower)
ambulance siren: wavefronts bunch ahead of an approaching source, spread out behind a receding one

Redshift (worked example)

Redshift: wavelength of light stretched to a longer wavelength due to the separation velocity between galaxies.

worked examplegalaxy recession speed from redshift

Galaxy A emits blue light λ_s = 450 nm; stationary Galaxy B detects it at λ₀ = 780 nm (red). c = 3×10⁸ m/s.

v = f_s λ_s ⇒ 3×10⁸ = f_s (450×10⁻⁹) f_s = 6.67×10¹⁴ Hz v = f₀λ₀ ⇒ 3×10⁸ = f₀(780×10⁻⁹) f₀ = 3.85×10¹⁴ Hz f₀ < f_s ⇒ galaxies are separating f₀ = v/(v−v_s) × f_s 3.85×10¹⁴ = [3×10⁸/(3×10⁸−v_s)] × 6.67×10¹⁴ v_s = 2.2×10⁸ m/s
CIE MCQvehicle with microwave transmitter — variation in f₀

Vehicle emits const-frequency microwaves, moves toward a stationary observer at const speed (f₀>F_s), then accelerates and holds a higher steady speed (f₀ even higher), then decelerates to a stop (f₀→F_s).

Answer: C — observed frequency rises, remains steady, then falls back to F_s (as v_s→0, f₀→f_s)

CIE MCQsource passes a stationary observer

A source of constant f_s moves at constant speed directly toward, then passes, then moves directly away from an observer.

Answer: B — a step up to a steady high f₀ while approaching, then a step down to a steady low f₀ (below f_s) once receding

CIE MCQjet aircraft — frequency heard

Jet travels at 0.8v (v = speed of sound) toward a stationary observer; emitted frequency 100 Hz.

f₀ = v/(v−v_s) × f_s = v/(v−0.8v) × 100 = v/(0.2v) × 100 = 500 Hz

Answer: D — 500 Hz

CIE MCQsiren — correct expression

Siren f_s = 1000 Hz moves at 20 m/s toward a stationary observer; speed of sound = 330 m/s.

Answer: B — (1000×330)/(330−20)

CIE structuredcar horn — find the car's speed

Car moves at constant speed toward a stationary observer; horn f_s = 510 Hz, observer hears f₀ = 550 Hz; speed of sound = 340 m/s.

f₀ = v/(v−v_s) × f_s 550 = 340/(340−v_s) × 510 340 − v_s = (340×510)/550 v_s = 340 − (340×510/550) = 24.7 v_s ≈ 25 m/s
CIE structuredchild on a rotating platform — max & min frequency

Child moves in a circle at 7.5 m/s, blowing a whistle (f_s = 950 Hz) starting at point P (moving toward a distant observer) and stopping at point Q (moving away). Speed of sound = 330 m/s.

f₀(max) = v/(v−v_s) × f_s = 330/(330−7.5) × 950 = 972.1 ≈ 970 Hz

Variation heard: frequency decreases from 970 Hz (at P) through 950 Hz (at the point level with the observer, X) down to 930 Hz (at Q) — i.e. it falls smoothly from the max value, through f_s itself, to the min value f₀(min) = 330/(330+7.5)×950 = 930 Hz.

CIE structuredchecking SI base units of I = Kvρf²A²

I is intensity (power per unit area), K a unitless constant, v = speed of sound, ρ = density of air, f = frequency, A = amplitude. Show both sides have the same SI base units.

LHS: I = P/A_area = W/(m²) = (kg m² s⁻³)/m² = kg s⁻³ RHS: K·(m s⁻¹)·(kg m⁻³)·(s⁻¹)²·(m²) = kg·s⁻³ · (m·m⁻³·m²) = kg s⁻³ ✓ shown
CIE structureddescribing the Doppler effect & redshift (recap wording)

Describe the Doppler effect: the change in observed frequency due to relative motion between source and observer.

A distant star moves away from a stationary observer — effect on the light observed? Light will be redshifted — the wavelength stretches to a longer value / the observed frequency is less than the source frequency.

9. The Electromagnetic Spectrum

★ Learn everything on this page: examiners love mixing wavelength ranges, frequency, and uses into one MCQ.
  • Group of transverse waves.
  • All travel at 3×10⁸ m/s in a vacuum.
Region Wavelength range /m Typical use
Radio waves 10³ < λ ≤ 10⁰ FM radio / RC cars
Microwaves 10⁰ < λ ≤ 10⁻³ Microwave ovens / network signals
Infrared 10⁻³ < λ ≤ 10⁻⁶ Infrared cameras / TV remotes
Visible light ≈ 10⁻⁶ We use this to see!
Ultraviolet 10⁻⁶ < λ ≤ 10⁻⁸ Disinfection
X-rays 10⁻⁸ < λ ≤ 10⁻¹⁰ X-ray scans
Gamma rays 10⁻¹⁰ < λ ≤ 10⁻¹² Cancer treatment / detecting leaks / PET scans
Mnemonic (longest → shortest λ): "Raging martians invaded Venus using X-ray guns" — Radio, Microwave, Infrared, Visible, Ultraviolet, X-ray, Gamma.
Visible light colours (typical λ): Red 780 nm | Green 550 nm | Blue 400 nm
CIE MCQCRO display of an EM wave

1 wavelength spans 1.0 cm on screen; time-base = 0.20 μs/cm.

T = 5 div × 0.20 μs = 0.4×10⁻⁶ s f = 1/T = 2.5 MHz

Answer: A — 2.5 MHz, radio wave region

CIE MCQnaming waves at 100 pm and 100 μm
100×10⁻¹² = 1×10⁻¹⁰ m → X-ray range 100×10⁻⁶ = 1×10⁻⁴ m → infrared range

Answer: C — X-rays, infrared

CIE MCQorders of magnitude table

Which row shows the correct order-of-magnitude wavelengths for microwaves, infrared, ultraviolet, X-rays?

Answer: C — 10⁻², 10⁻⁶, 10⁻⁸, 10⁻¹⁰ m respectively

CIE structuredseven regions A–G, wavelength decreasing →

Property of EM waves not shared with other transverse waves: travel in a vacuum at 3×10⁸ m/s.

Naming regions B, E, F (with typical wavelength):

B = Microwaves, λ ≈ 1×10⁻² m E = Ultraviolet, λ ≈ 1×10⁻⁷ m F = X-rays, λ ≈ 1×10⁻⁹ m

Frequency for a wavelength of 500 nm:

v = fλ ⇒ 3×10⁸ = f × (500×10⁻⁹) f = 6×10¹⁴ Hz

10. General Wave Properties

Wavefront: an imaginary line joining all points in phase on different waves.

Reflection laws:

  1. Incident wave, reflected wave and the normal all lie in the same plane.
  2. ∠i = ∠r
incidentreflected ir
∠i = ∠r, measured from the normal (dashed)

11. Refraction

The bending of a wave as it passes from a rarer to a denser medium or vice versa — caused by a velocity change.

Deep → shallow:

  • frequency stays the same
  • λ decreases
  • v↓ = fλ↓ ⇒ wave bends

Shallow → deep:

  • frequency stays the same
  • λ increases
  • v↑ = fλ↑ ⇒ wave bends the other way
deepshallow (block)deep λ longer, v fasterλ shorter, v slower
wave enters a shallow region, slows, wavelength shortens, direction bends toward the normal

12. Diffraction

Spreading of a wave into a region it would not reach if it travelled in straight lines — i.e. spreading into its geometric shadow — as it passes a narrow slit or edge.

★ Exam Tip: diffraction is most significant when slit size ≈ wavelength.
λ≈gap
narrow slit — strong circular diffraction
gap≫λ
wide slit — very little diffraction
grating
many narrow slits — each diffracts, less per slit
Remember: λ, frequency and velocity are all unchanged by diffraction — only the direction of spreading changes. Be careful when drawing!
CIE MCQwavefronts through a gap — what changes at Q?

Plane wavefronts pass through a gap (P before, Q after).

I ∝ 1/r² and I ∝ a² ⇒ a ∝ 1/r ⇒ amplitude falls as the wave spreads out

Answer: C — amplitude changes (velocity, frequency and wavelength are all unchanged by diffraction)

CIE MCQmost-diffracted EM wave for an atomic lattice

Lattice spacing ≈ 10⁻¹⁰ m. Diffraction is most significant when slit size ≈ wavelength.

Answer: D — X-rays (λ range 10⁻⁸–10⁻¹⁰ m, matching the lattice spacing)

CIE MCQdiagrams X (obstacle) & Y (gap) — diffraction or interference?

Answer: A — diagrams X and Y both illustrate diffraction (spreading round an edge / through a gap)

13. Polarisation

The process of confining the oscillations of particles in one direction only (and always perpendicular to the direction of travel).

Note: for EM waves, the electric and magnetic fields are always perpendicular to each other and to the direction of travel — when discussing polarisation we only consider the electric field component.
unpolarised (random directions, all ⊥ travel)
plane-polarised (one direction only)

How to polarise light

Use a polaroid sheet/filter, which acts as a polariser.

  • Oscillations parallel to the axis of the slit → pass through completely.
  • Oscillations perpendicular to the axis of the slit → completely blocked.

A polaroid filter is made of long chains of organic molecules; the axis of the slit is perpendicular to the chains.

Note: only transverse waves show polarisation — longitudinal waves cannot (no cancellation takes place along the direction of travel).

Two types:

  1. Partial polarisation — vibrations not fully restricted to one direction (e.g. reflection off water).
  2. Full / complete plane polarisation — vibrations fully restricted to one direction only.

Malus' Law

θ = angle between the electric field vector and the axis of the (second) slit.

  1. I ∝ a² (recall)
  2. amplitude ∝ electric field strength ⇒ a ∝ E, a² ∝ E²
  3. I ∝ a² and a² ∝ E² ⇒ I ∝ E²
I = KE² ⇒ I₁/E₁² = K = I₂/E₂² I₀/E₀² = I/(E₀cosθ)² I = I₀ cos²θ
I = I₀ cos²θ
Important: Malus' Law only works for light that is already polarised before hitting the analyser. Unpolarised light has its intensity halved passing through the first polaroid filter (regardless of angle).
Iθ 0°90°180° 270°360° line of symmetry
I = I₀cos²θ — max I₀ at 0°/180°/360°, zero at 90°/270°, symmetric about those lines
Uses of polarisation: glare-reduction glasses · 3D movies · improving TV signal reception · stress analysis of materials
CIE structureddemonstrating partial polarisation of reflected light

Light reflected from a water surface is partially plane polarised. Describe briefly how you would demonstrate this.

  1. Make the reflected light incident on a polaroid filter.
  2. Rotate the filter about its axis.
  3. You will see maximums and minimums of intensity (never falling fully to zero — proving it's only partially polarised).
worked examplethree polarising filters — show intensity is not zero

Vertically polarised light (I₀) hits filter 1 (axis vertical), then filter 2 (axis 45° to vertical), then filter 3 (axis horizontal). Show the final intensity is not zero.

Filter 1: θ=0° (light already vertical, matches axis) ⇒ I₁ = I₀cos²(0°) = I₀ Filter 2: θ=45° ⇒ I₂ = I₁cos²(45°) = I₀/2 Filter 3: angle between filter 2 (45°) and filter 3 (horizontal, 90°) is also 45° I₃ = I₂cos²(45°) = I₀/4 ≠ 0 — shown
worked exampleangle for a resultant intensity of I₀/6 (same 3-filter setup)
I₀/6 = (I₀/4)cos²θ √(4/6) = cosθ θ = cos⁻¹(√(4/6)) θ ≈ 35.3°
CIE structuredvertically-polarised beam onto a rotating filter

Filter's transmission axis is initially vertical (transmitted intensity = incident intensity).

(a) Angle to the vertical that gives no transmitted beam: 90° or 270°.

(b) Ratio I/I₀ = 0.75 when the filter is at angle θ:

cos²θ = I/I₀ = 0.75 θ = cos⁻¹(√0.75) = 30°

Ratio (amplitude transmitted)/(amplitude incident):

I ∝ a² ⇒ a/a₀ = √(I/I₀) = √0.75 = 0.87
CIE structuredfilter at 20°, then rotated back to the same intensity
I_T/I₀ = cos²(20°) = 0.8830 a_T/a₀ = √0.8830 = 0.94

Rotating so θ (to the vertical) increases from 20°, the transmitted intensity first falls (max at 0°, min at 90°) then rises again — it returns to its starting value (cos² symmetric about 90°) at θ = 160° (since 90°+(90°−20°) = 160°).

minimum rotation = 160° − 20° = 140°
CIE structuredtwo filters A & B — meaning & rotation angle

Meaning of polarisation: the process of confining oscillations of the electric field vector to one direction only, while still perpendicular to the direction of propagation.

Why light can be plane polarised but sound cannot: light waves are transverse, sound waves are longitudinal.

Filter A (vertical axis) polarises unpolarised light to intensity I₀; filter B (rotatable) starts horizontal. After rotation, intensity emerging from B is ¼I₀ — find the rotation angle from B's starting position.

I₀/4 = I₀cos²θ ⇒ cosθ = √(1/4) θ = cos⁻¹(½) = 60° or 120° (both roots, symmetric about 90°) rotation from horizontal (90° to A) = 120° − 90° = 30°
✓ Quick Recap — Polarisation
  • Only transverse waves polarise; the E-field is what's confined to one plane.
  • I = I₀cos²θ (Malus' Law) — only for already-polarised light.
  • Unpolarised light through the first filter always loses half its intensity, regardless of angle.
  • I vs θ graph is symmetric about 90° and 270° — two angles either side of a symmetry line always give the same intensity.

14. The Cathode-Ray Oscilloscope (C.R.O)

heatere⁻ anodeY-platesX-plates (time) screen (ZnS)
thermionic emission → accelerated by anode → deflected by Y-plates (signal) & X-plates (time) → hits zinc-sulphide screen, which emits light
Y-plate sensitivity — basically the setting for the displacement axis (V/div).
Time-base setting — basically the setting for the time axis (s/div).
worked examplereading a and T off a CRO trace

Time-base = 1 ms/cm; Y-plate sensitivity = 0.2 mV/cm. Trace spans 4 cm per full wave, peak height 2 cm.

1cm : 1ms = 4cm : T ⇒ T = 4 ms 0.2mV : 1cm = a : 2cm ⇒ a = 0.4 mV f = 1/(4×10⁻³) = 250 Hz

What each screen shows

Y-plates off & time-base off → single dot
Y-plates on, time-base off → vertical line
Y-plates off, time-base on → flat horizontal line

✓ Full Chapter Cheat-Sheet — Waves
  • Transverse: vibration ⊥ travel, travels in vacuum. Longitudinal: vibration ∥ travel, needs a medium.
  • Phase diff (distance) = (Δx/λ)×360°  |  Phase diff (time) = (Δt/T)×360°
  • v = fλ
  • I = P/A  |  I ∝ a²  |  I ∝ 1/r²  |  I₁/a₁² = I₂/a₂²  |  I₁r₁² = I₂r₂²
  • Doppler: f₀ = v/(v∓v_s) × f_s  (− for approach, + for separation)
  • EM spectrum (long→short λ): Radio, Microwave, Infrared, Visible, Ultraviolet, X-ray, Gamma — all at 3×10⁸ m/s in vacuum
  • Refraction: bending due to velocity change; f constant, λ & v change together
  • Diffraction: most significant when slit size ≈ λ; λ, f, v all unchanged
  • Malus' Law: I = I₀cos²θ (already-polarised light only); unpolarised light halves through the first filter
  • CRO: Y-sensitivity sets the displacement axis, time-base sets the time axis