Electromagnetic Spectrum and Polarisation
All electromagnetic waves are transverse and travel at m s⁻¹ in free space. Wavelengths run from kilometres (radio) to less than m (gamma); visible light is – nm. Only transverse waves can be polarised. A polariser halves unpolarised light; after that, Malus's law gives .
Learning objectives
- Recall the order and approximate wavelengths of the regions of the EM spectrum.
- Use with m s⁻¹.
- Explain polarisation and why it shows waves are transverse.
- Use Malus's law .
Look at a phone screen through polarising sunglasses and slowly tilt your head. The screen goes dark at one angle. Why?
Core idea
Light reflected off a lake is mostly vibrating horizontally. Polarising sunglasses only let vertical vibrations through, so the glare vanishes. Polarisation is also the proof that light is a transverse wave.
Polarised: oscillation in one plane. Only transverse waves polarise. Malus's law: .
1. Polarising filters
- Only the component along the analyser's axis passes.
- Intensity ∝ amplitude².
- Combine.
Unpolarised 40 W m.
- Goal
- Final intensity.
- Strategy
- Half, then Malus.
- First filter halves.
- Second.
Polarised light through an analyser.
- Goal
- .
- Strategy
- Solve .
- Square root.
- Inverse cos.
Why can't sound be polarised?
Summary
- Transverse only.
- .
- Plane polarised
- Oscillating in one plane.
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