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  2. Luminous intensity - Wikipedia

    en.wikipedia.org/wiki/Luminous_intensity

    The frequency of light used in the definition corresponds to a wavelength in a vacuum of 555 nm, which is near the peak of the eye's response to light. If the 1 candela source emitted uniformly in all directions, the total radiant flux would be about 18.40 mW , since there are 4 π steradians in a sphere.

  3. Wavenumber - Wikipedia

    en.wikipedia.org/wiki/Wavenumber

    For example, a wavenumber in inverse centimeters can be converted to a frequency expressed in the unit gigahertz by multiplying by 29.979 2458 cm/ns (the speed of light, in centimeters per nanosecond); [5] conversely, an electromagnetic wave at 29.9792458 GHz has a wavelength of 1 cm in free space.

  4. Spatial frequency - Wikipedia

    en.wikipedia.org/wiki/Spatial_frequency

    The SI unit of spatial frequency is the reciprocal metre (m −1), [1] although cycles per meter (c/m) is also common. In image-processing applications, spatial frequency is often expressed in units of cycles per millimeter (c/mm) or also line pairs per millimeter (LP/mm). In wave propagation, the spatial frequency is also known as wavenumber.

  5. Dispersion relation - Wikipedia

    en.wikipedia.org/wiki/Dispersion_relation

    The top electron has twice the momentum, while the bottom electron has half. Note that as the momentum increases, the phase velocity decreases down to c, whereas the group velocity increases up to c, until the wave packet and its phase maxima move together near the speed of light, whereas the wavelength continues to decrease without bound. Both ...

  6. Wavelength - Wikipedia

    en.wikipedia.org/wiki/Wavelength

    In a dispersive medium, the phase speed itself depends upon the frequency of the wave, making the relationship between wavelength and frequency nonlinear. In the case of electromagnetic radiation—such as light—in free space, the phase speed is the speed of light, about 3 × 10 8 m/s.

  7. Free spectral range - Wikipedia

    en.wikipedia.org/wiki/Free_spectral_range

    where is the vacuum wavelength of light. For a linear cavity, such as the Fabry-Pérot interferometer [ 3 ] discussed below, L = 2 l {\displaystyle L=2l} , where L {\displaystyle L} is the distance travelled by light in one roundtrip around the closed cavity, and l {\displaystyle l} is the length of the cavity.

  8. Electromagnetic spectrum - Wikipedia

    en.wikipedia.org/wiki/Electromagnetic_spectrum

    Longer-wavelength radiation such as visible light is nonionizing; the photons do not have sufficient energy to ionize atoms. Throughout most of the electromagnetic spectrum, spectroscopy can be used to separate waves of different frequencies, so that the intensity of the radiation can be measured as a function of frequency or wavelength ...

  9. Spectral flux density - Wikipedia

    en.wikipedia.org/wiki/Spectral_flux_density

    In a region in which the material is uniform and the radiative field is isotropic and homogeneous, let the spectral radiance (or specific intensity) be denoted by I (x, t ; r 1, ν), a scalar-valued function of its arguments x, t, r 1, and ν, where r 1 denotes a unit vector with the direction and sense of the geometrical vector r from the ...

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