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  2. Wien's displacement law - Wikipedia

    en.wikipedia.org/wiki/Wien's_displacement_law

    Formally, the wavelength version of Wien's displacement law states that the spectral radiance of black-body radiation per unit wavelength, peaks at the wavelength given by: = where T is the absolute temperature and b is a constant of proportionality called Wien's displacement constant, equal to 2.897 771 955... × 10 −3 m⋅K, [1] [2] or b ...

  3. Thermal remote sensing - Wikipedia

    en.wikipedia.org/wiki/Thermal_Remote_sensing

    Stefan–Boltzmann law: Surface temperature of any objects radiate energy and shows specific properties. These properties are calculated by Boltzmann law. 2. Wien's displacement law: Wien's displacement law explains the relation between temperature and the wavelength of radiation. It states that the wavelength of radiation emitted from a ...

  4. Category:Eponymous laws of physics - Wikipedia

    en.wikipedia.org/wiki/Category:Eponymous_laws_of...

    Download as PDF; Printable version; ... Radioactive displacement law of Fajans and Soddy ... Von Babo's law; W. Wiedemann–Franz law; Wien's displacement law ...

  5. Wien approximation - Wikipedia

    en.wikipedia.org/wiki/Wien_approximation

    Comparison of Wien’s curve and the Planck curve. Wien's approximation (also sometimes called Wien's law or the Wien distribution law) is a law of physics used to describe the spectrum of thermal radiation (frequently called the blackbody function). This law was first derived by Wilhelm Wien in 1896.

  6. Thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Thermal_radiation

    Wien's displacement law, and the fact that the frequency is inversely proportional to the wavelength, indicates that the peak frequency f max is proportional to the absolute temperature T of the black body. The photosphere of the sun, at a temperature of approximately 6000 K, emits radiation principally in the (human-)visible portion of the ...

  7. Draper point - Wikipedia

    en.wikipedia.org/wiki/Draper_point

    The value of the Draper point can be calculated using Wien's displacement law: the peak frequency (in hertz) emitted by a blackbody relates to temperature as follows: [4] =, where k is the Boltzmann constant, h is the Planck constant,

  8. Wien displacement law - Wikipedia

    en.wikipedia.org/?title=Wien_displacement_law&...

    Download as PDF; Printable version; In other projects Appearance. move to sidebar hide. From Wikipedia, the free encyclopedia. Redirect page. Redirect to: Wien's ...

  9. Wien's law - Wikipedia

    en.wikipedia.org/wiki/Wien's_law

    Wien's law or Wien law may refer to: . Wien approximation, an equation used to describe the short-wavelength (high frequency) spectrum of thermal radiation; Wien's displacement law, an equation that describes the relationship between the temperature of an object and the peak wavelength or frequency of the emitted light