Wavelength
Wikipedia, the free encyclopedia - Cite This SourceIn physics, wavelength is the distance between repeating units of a propagating wave of a given frequency. It is commonly designated by the Greek letter lambda (λ). Examples of wave-like phenomena are light, water waves, and sound waves.
In a wave, a property varies with the position. For example, this property can be the air pressure for a sound wave, or the magnitude of the electric or the magnetic field for light. The wavelengths of frequencies audible to the human ear (20 Hz–20 kHz) are between approximately 17 m and 17 mm, respectively. Visible light ranges from deep red, roughly 700 nm to violet, roughly 400 nm (430–750 THz). For other examples, see electromagnetic spectrum.
Relationship with frequency
Wavelength λ is inverse proportional with the frequency, the number of periods per time unit passing a given point, as inIt should be noted that for many wave phenomena, wavelength is not the distance that particles travel during a period. For instance, in acoustics and water waves, the particle displacements during a period are only a small fraction of the wavelength, apart from extreme conditions like breaking waves and shock waves.
In non-vacuum media
The speed of light in most media is lower than in vacuum, which means that the same frequency will correspond to a shorter wavelength in the medium than in vacuum. The wavelength in the medium isDe Broglie wavelength of particles
Louis de Broglie postulated that all particles with momentum have a wavelengthSee also
- Amplitude
- Angular frequency
- Frequency
- Fraunhofer lines, spectral lines traditionally used as standard optical wavelength references
- Periodic function
- Wavevector
External links
- Conversion: Wavelength to Frequency and vice versa - Sound waves and radio waves
- Teaching resource for 14-16yrs on sound including wavelength
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Last updated on Tuesday March 11, 2008 at 02:18:14 PDT (GMT -0700)
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