Stefan-Boltzmann constant oor Spaans
Stefan-Boltzmann constant
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constante de Stefan-Boltzmann
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"CODATA Value: Stefan–Boltzmann constant".
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The Stefan-Boltzmann constant How much heat does a blackbody emit when it’s at a certain temperature?
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Display Boltzmann Constant, Atomic Mass Unit, Molar Gas Constant, Stefan-Boltzmann Constant or Avogadro 's Number
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(1-25) where 5.67 108 W/m2 · K4 or 0.1714 108 Btu/h · ft2 · R4 is the Stefan–Boltzmann constant.
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Furthermore, the Stefan–Boltzmann constant allows for temperature (K) to be converted to units for intensity (W⋅m−2), which is power per unit area.
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It is usual to write U/V=(4 σ/c) T4, where c is the speed of light and σ is called the Stefan-Boltzmann constant.
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It is a universal constant composed of other basic constants (vacuum permeability, Boltzmann’s constant, Stefan-Boltzmann’s constant...).
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The brightness of a star is: L = 4is the Stefan-Boltzmann constant, R the radius of the star and T the temperature.
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where the total energy is per unit area per second emitted by the back body, T is its absolute (thermodynamic) temperature and is the Stefan-Boltzmann constant.
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Where stands for the total thermal radiation, is the body emissivity, stands for the temperature and is the Stefan-Boltzmann constant, being the total thermal radiation equivalent to the area under each curve on the figure below.
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Determine the coefficient of emissivity or absorptivity, the constant of Stefan Boltzmann.
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11 sinne gevind in 12 ms. Hulle kom uit baie bronne en word nie nagegaan nie.