C.5 Doppler effect
- Syllabus
- First assessment 2025
- Topic
- —
- Level
- HL
• Nature of the Doppler effect for sound waves and electromagnetic waves.
• Represent Doppler effect with wavefront diagrams for moving source or observer.
• For light at low relative speed: Δf/f = Δλ/λ ≈ v/c.
• Spectral line shifts reveal motion of stars and galaxies.
• HL: Doppler formulas for sound/mechanical waves.
• Distinguish moving-source and moving-observer cases.