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A Level H2 Physics Waves Sound Light Quiz

Free A Level H2 Physics Waves Sound Light quiz, HY3 Exam version, with questions, answers, and A Level-style practice for Singapore students.

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A Level H2 Physics From Real Exams Generated by Tencent HY3 Free Updated 2026-08-17

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Answers

A-Level Physics H2 Quiz - Waves Sound Light (Answer Key)

Total Marks: 40
Topic: Waves, Sound & Light


Section A

1. [1 mark]
Wavelength is the distance between two consecutive points in phase (e.g. two adjacent crests or troughs) of a progressive wave.
Teaching note: Progressive waves transfer energy; wavelength λ\lambda is measured in metres.

2. [2 marks]
Use v=fλλ=v/fv = f\lambda \Rightarrow \lambda = v/f.
λ=340/440=0.773 m\lambda = 340 / 440 = 0.773\ \text{m} (3 s.f.).
Marks: 1 for formula, 1 for answer with unit.

3. [2 marks]
Transverse waves have oscillations perpendicular to direction of travel, so a plane of vibration exists and can be filtered by a polariser. Longitudinal waves oscillate parallel to travel, so no unique plane to select.
Marks: 1 for transverse explanation, 1 for longitudinal.

4. [1 mark]
With 3 antinodes on a string fixed at both ends, there are 4 nodes (including the two ends).

5. [2 marks]
Path difference from the two sources = nλn\lambda (where n=0,1,2,n = 0,1,2,\dots) and the waves arrive in phase.
Marks: 1 path diff, 1 in phase.

6. [3 marks]
d=1/(5.0×105)=2.0×106 md = 1/(5.0\times10^5) = 2.0\times10^{-6}\ \text{m}.
nλ=dsinθsinθ=λ/d=600×109/2.0×106=0.300n\lambda = d\sin\theta \Rightarrow \sin\theta = \lambda/d = 600\times10^{-9} / 2.0\times10^{-6} = 0.300.
θ=sin1(0.300)=17.5\theta = \sin^{-1}(0.300) = 17.5^\circ.
Marks: 1 grating spacing, 1 substitution, 1 angle.

7. [2 marks]
I=P/(4πr2)=2.0/(4π×4.02)=2.0/201.1=9.95×103 W m2I = P/(4\pi r^2) = 2.0 / (4\pi \times 4.0^2) = 2.0 / 201.1 = 9.95\times10^{-3}\ \text{W m}^{-2}.
Marks: 1 formula, 1 answer.

8. [1 mark]
I=I0cos2θI = I_0 \cos^2\theta where I0I_0 is intensity after polariser, θ\theta angle between polariser and analyser.

9. [2 marks]
Compare y=Asin(ωt)y = A\sin(\omega t): A=0.02 mA = 0.02\ \text{m}, ω=4π rad s1\omega = 4\pi\ \text{rad s}^{-1}.
Marks: 1 each.

10. [2 marks]
Diffraction: spreading of waves past an obstacle/aperture. Interference: superposition of two/more coherent waves to form maxima/minima.
Marks: 1 each.


Section B

11. [3 marks]
λ=dΔx/D=(0.50×103×1.44×103)/1.20=6.0×107 m=600 nm\lambda = d\Delta x / D = (0.50\times10^{-3} \times 1.44\times10^{-3}) / 1.20 = 6.0\times10^{-7}\ \text{m} = 600\ \text{nm}.
Marks: 1 convert units, 1 formula, 1 answer.

12. [2 marks]
(a) Wavelength = 20 cm (two loops over 40 cm → λ/2=20\lambda/2 = 20 cm, so λ=40\lambda = 40 cm? Wait: 2 complete loops = 2 half-wavelengths? Actually 2 loops = 1 full wavelength if loop = half-wave; 2 loops = λ\lambda = 40 cm). From labels: nodes at 0,20,40 → distance between nodes = 20 cm = λ/2\lambda/2, so λ=40\lambda = 40 cm. [1]
(b) Adjacent nodes = 20 cm. [1]

13. [3 marks]
d=1/(2.0×105)=5.0×106 md = 1/(2.0\times10^5) = 5.0\times10^{-6}\ \text{m}.
Using n=1n=1: λ=dsin18=5.0×106×0.309=1.545×106 m\lambda = d\sin18^\circ = 5.0\times10^{-6}\times0.309 = 1.545\times10^{-6}\ \text{m}.
Check n=2n=2: 2λ=dsin37.5=5.0×106×0.609=3.045×1062\lambda = d\sin37.5^\circ = 5.0\times10^{-6}\times0.609 = 3.045\times10^{-6}λ=1.52×106 m\lambda = 1.52\times10^{-6}\ \text{m}. Avg 1.53×106 m\approx 1.53\times10^{-6}\ \text{m}.
Marks: 1 spacing, 1 calc, 1 consistency.

14. [3 marks]
(a) T=4 msf=1/T=250 HzT = 4\ \text{ms} \Rightarrow f = 1/T = 250\ \text{Hz}. [1]
(b) v=fλ=250×0.80=200 m s1v = f\lambda = 250 \times 0.80 = 200\ \text{m s}^{-1}. [2]

15. [2 marks]
Intensity decreases with distance according to inverse square law: I1/r2I \propto 1/r^2.
Marks: 1 law, 1 statement.


Section C

16. [5 marks]
(a) Fundamental: λ=2L=1.60 m\lambda = 2L = 1.60\ \text{m}, f=v/λ=160/1.60=100 Hzf = v/\lambda = 160/1.60 = 100\ \text{Hz}. [2]
(b) Second harmonic = 2×100=200 Hz2\times100 = 200\ \text{Hz}. [1]
(c) Incident and reflected waves of same frequency/amplitude superpose, forming nodes (zero displacement) and antinodes. [2]

17. [5 marks]
Apparatus: laser, double slit (dd), screen, metre rule.
Procedure: shine laser through slits onto screen, measure fringe separation Δx\Delta x over several fringes, measure DD.
Use λ=dΔx/D\lambda = d\Delta x/D. Repeat for accuracy.
Mark descriptors: apparatus (1), procedure (2), formula use (1), reducing error (1).

18. [5 marks]
(a) After polariser: I0/2I_0/2. [1]
(b) I=(I0/2)cos230=0.5I0×0.75=0.375I0I = (I_0/2)\cos^2 30^\circ = 0.5 I_0 \times 0.75 = 0.375 I_0. [2]
(c) Glare is horizontally polarised; polarising sunglasses block that plane, reducing reflected light. [2]

19. [4 marks]
Each slit acts as source; waves superpose. Principal maxima when dsinθ=nλd\sin\theta = n\lambda. Larger nn → larger sinθ\sin\theta → larger θ\theta.
Marks: superposition (1), condition (1), angle relation (2).

20. [5 marks]
(a) Closed at one end: λ=4L=4×(340/512)=2.66 m\lambda = 4L = 4\times(340/512) = 2.66\ \text{m}. [2]
(b) L=λ/4=0.664 mL = \lambda/4 = 0.664\ \text{m}. [1]
(c) Node at closed end, antinode at open; only quarter-wave odd multiples fit. [2]