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  2. Photometry (optics) - Wikipedia

    en.wikipedia.org/wiki/Photometry_(optics)

    Luminous intensity (photometric) and radiant intensity (radiometric) In photometric quantities every wavelength is weighted according to how sensitive the human eye is to it, while radiometric quantities use unweighted absolute power. For example, the eye responds much more strongly to green light than to red, so a green source will have ...

  3. Radiometry - Wikipedia

    en.wikipedia.org/wiki/Radiometry

    Comparison of photometric and radiometric quantities. Radiometry is a set of techniques for measuring electromagnetic radiation, including visible light.Radiometric techniques in optics characterize the distribution of the radiation's power in space, as opposed to photometric techniques, which characterize the light's interaction with the human eye.

  4. Category:Units of photometry - Wikipedia

    en.wikipedia.org/wiki/Category:Units_of_photometry

    cd/m 2 (= lm/(sr⋅m 2)) L −2 ⋅J: Luminous flux per unit solid angle per unit projected source area. The candela per square metre is sometimes called the nit. Illuminance: E v: lux (= lumen per square metre) lx (= lm/m 2) L −2 ⋅J: Luminous flux incident on a surface Luminous exitance, luminous emittance M v: lumen per square metre lm/m ...

  5. Template:SI radiometry units - Wikipedia

    en.wikipedia.org/wiki/Template:SI_radiometry_units

    2 = any non-empty string other than "self" The template will display a "(Compare)" link (as above). However, the link will point to the corresponding photometry table in the separate article on " Photometry (optics) ", not to within the article, where the {{SI radiometry units}} template has been included.

  6. Radiance - Wikipedia

    en.wikipedia.org/wiki/Radiance

    Comparison of photometric and radiometric quantities. Radiance is useful because it indicates how much of the power emitted, reflected, transmitted or received by a surface will be received by an optical system looking at that surface from a specified angle of view.

  7. Photometric system - Wikipedia

    en.wikipedia.org/wiki/Photometric_system

    For each photometric system a set of primary standard stars is provided. A commonly adopted standardized photometric system is the Johnson-Morgan or UBV photometric system (1953). At present, there are more than 200 photometric systems. [citation needed] Photometric systems are usually characterized according to the widths of their passbands:

  8. Light intensity - Wikipedia

    en.wikipedia.org/wiki/Light_intensity

    Luminous intensity, a photometric quantity measured in lumens per steradian (lm/sr), or candela (cd) Irradiance, a radiometric quantity, measured in watts per square meter (W/m 2) Intensity (physics), the name for irradiance used in other branches of physics (W/m 2) Radiance, commonly called "intensity" in astronomy and astrophysics (W·sr −1 ...

  9. Spectral flux density - Wikipedia

    en.wikipedia.org/wiki/Spectral_flux_density

    It is a radiometric rather than a photometric measure. In SI units it is measured in W m −3, although it can be more practical to use W m −2 nm −1 (1 W m −2 nm −1 = 1 GW m −3 = 1 W mm −3) or W m −2 μm −1 (1 W m −2 μm −1 = 1 MW m −3), and respectively by W·m −2 ·Hz −1, Jansky or solar flux units.