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The magnitude of the Doppler shift is directly proportional to the relative velocity between the source and the observer.
The Doppler effect refers to the change in frequency or wavelength of a wave in relation to an observer moving relative to the source of the wave. In the context of light waves, this effect is often observed in astrophysics where the light from stars and galaxies can be 'redshifted' or 'blueshifted' depending on their relative motion to us.
The magnitude of this shift is directly influenced by the relative velocities of the source and the observer. If the source and observer are moving closer together, the observed frequency increases and the wavelength decreases, resulting in a blueshift. Conversely, if the source and observer are moving apart, the observed frequency decreases and the wavelength increases, resulting in a redshift. The greater the relative velocity, the greater the shift in frequency or wavelength.
This relationship is quantified by the Doppler effect formula, which for light is given by:
Δλ/λ = v/c
where Δλ is the change in wavelength, λ is the original wavelength, v is the relative velocity of the source and observer, and c is the speed of light. This formula shows that the fractional change in wavelength (and hence the shift in frequency) is directly proportional to the relative velocity.
In the case of sound waves, the Doppler effect is similarly influenced by relative velocities. However, the formula is slightly different due to the dependence on the speed of sound and the direction of motion. Nevertheless, the principle remains the same: the greater the relative velocity, the greater the Doppler shift.
Understanding the influence of relative velocities on the Doppler shift is crucial in many areas of physics. For example, in astrophysics, it allows us to determine the speed at which other galaxies are moving away from us, providing key evidence for the expansion of the universe. In medical imaging, Doppler ultrasound uses this effect to measure the speed of blood flow. Therefore, mastering this concept is not only essential for your IB Physics course, but also for appreciating its wide-ranging applications in the real world.
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