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Wien displacement law constant

Stefan-Boltzmann constant Wien displacement law constant Planck mass Planck temperature Planck length... [Pg.5]

The Wien displacement law states that the wavelength of maximum emission, A , of a blackbody varies inversely with absolute temperature the product A T remains constant. When A is expressed in micrometers, the law becomes... [Pg.727]

Wien displacement law Approximate formula for the wavelength, X, of maximum blackbody emission Xmax - T hc/5k — 2.878 X 10" 3 m K, where T is temperature in kelvins, h is Planck s constant, c is the speed of light, and k is Boltzmann s constant. Valid for T > 100 K. working electrode One at which the reaction of interest occurs. [Pg.705]

By properly choosing the value of the constant ft, Planck found that Eq. (19.11) agreed with the measured distribution within the experimental error To find the maximum, we set duJdX = 0 the Wien displacement law is obtained in the form... [Pg.455]

The Wien displacement law for blackbody radiators states that the product of temperature in kelvin and the wavelength of maximum emission is a constant k k - T - Calculate the wavelength of maximum emission for a Globar infrared source operated at 18(X) K. Use the data In Figure 6-22 for the Nernst glower for the evaluation of the constant. [Pg.160]

Light emitted from a black body solely as a result of high temperature as in electric bulb is known as incandescence or thermal radiation. The quality and quantity of thermal radiation is a function of temperature only. The wavelength of most strongly emitted radiation in the continuous spectrum from black body is given by Wien s Displacement Law-, Amax T —h. (where h is Wien s constant = 2.898 X 10 3 m deg). [Pg.10]

This relation was originally developed by Willy Wien in 1894 using classical thermodynamics, but it can also be obtained by differentiating Eq, 12-4 with respect to A while holding T constant and setting the result equal to zero. A plot of Wien s displacement law, which is the locus of the peaks of the radiation emission curves, is also given in Fig. 12-9. [Pg.684]

Thus the theorem about the displacement of the intensity maximum with temperature follows immediately from Wien s law. The value of the constant, it is true, cannot be determined until the special form of the function F is known. [Pg.188]

Wien s displacement law For a black body, r= constant, where Xm is the wavelength corresponding to the maximum radiation of energy and Tis the thermodynamic temperature of the body. Thus as the temperature rises the maximum of the spectral energy distribution curve is displaced towards the short-wavelength end of the spectrum. The law was stated by Wilhelm Wien (1864-1928). [Pg.874]

Wien s Displacement Law When the temperature of a radiating black body increases, the wavelength corresponding to maximum energy decreases in such a way that the product of the absolute temperature and wavelength is constant. [Pg.812]


See other pages where Wien displacement law constant is mentioned: [Pg.13]    [Pg.13]    [Pg.12]    [Pg.52]    [Pg.9]    [Pg.29]    [Pg.15]    [Pg.9]    [Pg.10]    [Pg.19]    [Pg.28]    [Pg.13]    [Pg.2495]    [Pg.13]    [Pg.13]    [Pg.12]    [Pg.52]    [Pg.9]    [Pg.29]    [Pg.15]    [Pg.9]    [Pg.10]    [Pg.19]    [Pg.28]    [Pg.13]    [Pg.2495]    [Pg.272]    [Pg.5]    [Pg.202]    [Pg.202]    [Pg.191]    [Pg.714]    [Pg.384]    [Pg.156]    [Pg.188]    [Pg.193]    [Pg.160]    [Pg.160]    [Pg.1068]    [Pg.11]    [Pg.412]    [Pg.417]    [Pg.24]    [Pg.402]   
See also in sourсe #XX -- [ Pg.11 ]

See also in sourсe #XX -- [ Pg.11 ]

See also in sourсe #XX -- [ Pg.10 ]




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