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  2. Longitudinal wave - Wikipedia

    en.wikipedia.org/wiki/Longitudinal_wave

    c is the speed of the wave; and; ω is the angular frequency of the wave. The quantity x/c is the time that the wave takes to travel the distance x. The ordinary frequency (f) of the wave is given by =. The wavelength can be calculated as the relation between a wave's speed and ordinary frequency.

  3. Wavelength - Wikipedia

    en.wikipedia.org/wiki/Wavelength

    In physics and mathematics, wavelength or spatial period of a wave or periodic function is the distance over which the wave's shape repeats. [1][2] In other words, it is the distance between consecutive corresponding points of the same phase on the wave, such as two adjacent crests, troughs, or zero crossings.

  4. Radio wave - Wikipedia

    en.wikipedia.org/wiki/Radio_wave

    Air is tenuous enough that in the Earth's atmosphere radio waves travel at very nearly the speed of light. The wavelength is the distance from one peak (crest) of the wave's electric field to the next, and is inversely proportional to the frequency of the wave. The relation of frequency and wavelength in a radio wave traveling in vacuum or air is

  5. Wavenumber - Wikipedia

    en.wikipedia.org/wiki/Wavenumber

    In the physical sciences, the wavenumber (or wave number), also known as repetency, [1] is the spatial frequency of a wave, measured in cycles per unit distance (ordinary wavenumber) or radians per unit distance (angular wavenumber). [2][3][4] It is analogous to temporal frequency, which is defined as the number of wave cycles per unit time ...

  6. Schwarzschild's equation for radiative transfer - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild's_equation...

    In the study of heat transfer, Schwarzschild's equation[1][2][3] is used to calculate radiative transfer (energy transfer via electromagnetic radiation) through a medium in local thermodynamic equilibrium that both absorbs and emits radiation. The incremental change in spectral intensity, [4] (dIλ, [W/sr/m 2 /μm]) at a given wavelength as ...

  7. Refractive index - Wikipedia

    en.wikipedia.org/wiki/Refractive_index

    The refractive index, , can be seen as the factor by which the speed and the wavelength of the radiation are reduced with respect to their vacuum values: the speed of light in a medium is v = c/n, and similarly the wavelength in that medium is λ = λ 0 /n, where λ 0 is the wavelength of that light in vacuum.

  8. Balmer series - Wikipedia

    en.wikipedia.org/wiki/Balmer_series

    where λ is the wavelength of the absorbed/emitted light and R H is the Rydberg constant for hydrogen. The Rydberg constant is seen to be equal to ⁠ 4 / B ⁠ in Balmer's formula, and this value, for an infinitely heavy nucleus, is ⁠ 4 / 3.645 0682 × 10 −7 m ⁠ = 10 973 731.57 m −1. [3]

  9. Hubble's law - Wikipedia

    en.wikipedia.org/wiki/Hubble's_law

    e. Hubble's law, also known as the Hubble–Lemaître law, [1] is the observation in physical cosmology that galaxies are moving away from Earth at speeds proportional to their distance. In other words, the farther they are, the faster they are moving away from Earth.

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