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  2. Wien's displacement law - Wikipedia

    en.wikipedia.org/wiki/Wien's_displacement_law

    In physics, Wien's displacement law states that the black-body radiation curve for different temperatures will peak at different wavelengths that are inversely proportional to the temperature. The shift of that peak is a direct consequence of the Planck radiation law , which describes the spectral brightness or intensity of black-body radiation ...

  3. 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.

  4. 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 ...

  5. File:Wien's Displacement Law Variations Chart.svg - Wikipedia

    en.wikipedia.org/wiki/File:Wien's_Displacement...

    Formulas for the various peak wavelengths and mean photon energy were taken from the Wikipedia Wien's displacement law page. The median and quartiles were computed by numerically integrating Planck's law ; however, for any who wish to avoid this, information on percentiles is given in the Planck's law article.

  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. Far infrared - Wikipedia

    en.wikipedia.org/wiki/Far_infrared

    Objects within a temperature range of approximately 5 K to 340 K emit radiation in the far infrared range as a result of black-body radiation, in accordance with Wien's displacement law. This characteristic is utilized in the observation of interstellar gases, which are frequently associated with the formation of new stars.

  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