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C.5 Doppler Effect

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2024/07/05 08:43
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C.5.1 The Doppler Effect

The Doppler effect
When a source of sound, such as the whistle of a train or the siren of an ambulance, moves away from an observer :
It appears to decrease in frequency, i.e. it sounds lower in pitch
Although, the source of the sound remains at a constant frequency
When the observer and the source of wave are both stationary :
The waves appear to remain at the same frequency for both the observer and the source
C.5.1-1 Diagram of doppler effect (stationary)
When the source starts to move towards the observer, the wavelength of the waves is shortened
The sound, therefore, appears at a higher frequency to the observer
C.5.1-2 Diagram of doppler effect (moving source)
Redshift/Blueshift of EM Radiation
In space the Doppler effect of light can be observed when spectra of distant stars and galaxies are observed, this is known as :
Redshift if the object is moving away from the Earth
Blueshift if the object is moving towards the Earth
C.5.1-3 Diagram of redshift
Redshift : The fractional increase in wavelength due to the source and observer receding from each other
Doppler redshift can be defined with equation :
Δλλ=Δff=vc(Δλ=shift in wavelength,λ=wavelength of source)(Δf=shift in frequency,f=frequency of source)(v=speed of recession,c=speed of light)\frac{\Delta\lambda}{\lambda} = \frac{\Delta f}{f} = \frac{v}{c}\\ (\Delta\lambda = \textit{shift in wavelength}, \quad \lambda = \textit{wavelength of source})\\ (\Delta f = \textit{shift in frequency}, \quad f = \textit{frequency of source})\\ (v = \textit{speed of recession}, \quad c = \textit{speed of light})

C.5.2 The Doppler Equation

Doppler Equation
When a source of sound waves moves relative to a stationary observer, the observed frequency can be calculated using the equation below :
f=f(vv±u)(f=observed frequency,f=source frequency)(v=velocity of wave,u=velocity of source)f' = f \left( \frac{v}{v \pm u} \right)\\ (f' = \textit{observed frequency}, \quad f = \textit{source frequency})\\ (v = \textit{velocity of wave}, \quad u = \textit{velocity of source})
The ± depends on whether the source is moving towards or away from the observer
If the source is moving towards the observer, the denominator is v - u
If the source is moving away from the observer, the denominator is v + u
the observer is moving relative to the source, the observed frequency can be calculated using the equation below :
f=f(v±uv)(f=observed frequency,f=source frequency)(v=velocity of wave,u=velocity of observer)f' = f \left( \frac{v \pm u}{v} \right)\\ (f' = \textit{observed frequency}, \quad f = \textit{source frequency})\\ (v = \textit{velocity of wave}, \quad u = \textit{velocity of observer})
The ± depends on whether the observer is moving towards or away from the source
If the observer is moving towards the source, the numerator is v + u
If the observer is moving away from the source, the numerator is v − u