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  2. Kirchhoff's law of thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Kirchhoff's_law_of_thermal...

    Kirchhoff's law of thermal radiation has a refinement in that not only is thermal emissivity equal to absorptivity, it is equal in detail. Consider a leaf. Consider a leaf. It is a poor absorber of green light (around 470 nm), which is why it looks green.

  3. Emissivity - Wikipedia

    en.wikipedia.org/wiki/Emissivity

    Kirchhoff's law is rigorously applicable with regard to the spectral directional definitions of emissivity and absorptivity. The relationship explains why emissivities cannot exceed 1, since the largest absorptivity—corresponding to complete absorption of all incident light by a truly black object—is also 1. [ 12 ]

  4. Idealized greenhouse model - Wikipedia

    en.wikipedia.org/wiki/Idealized_greenhouse_model

    The surface emits a radiative flux density F according to the Stefan–Boltzmann law: = where σ is the Stefan–Boltzmann constant. A key to understanding the greenhouse effect is Kirchhoff's law of thermal radiation. At any given wavelength the absorptivity of the atmosphere will be equal to the emissivity. Radiation from the surface could be ...

  5. Thermal radiation - Wikipedia

    en.wikipedia.org/wiki/Thermal_radiation

    Beer can being imaged by a FLIR thermal camera to demonstrate temperature differences caused by emissivity. The characteristics of thermal radiation depend on various properties of the surface from which it is emanating, including its temperature and its spectral emissivity, as expressed by Kirchhoff's law. [5]

  6. Skin temperature (atmosphere) - Wikipedia

    en.wikipedia.org/wiki/Skin_temperature_(atmosphere)

    Assuming the skin layer is at some temperature T s, and using Kirchhoff's law (absorptivity = emissivity), the total radiation flux produced by the skin layer is given by: F o u t , T o t a l = 2 ϵ σ T s 4 {\displaystyle F_{out,Total}=2\epsilon \sigma T_{s}^{4}} where the factor of 2 comes from the fact that the skin layer radiates in both ...

  7. Radiative equilibrium - Wikipedia

    en.wikipedia.org/wiki/Radiative_equilibrium

    In this case, Kirchhoff's law of equality of radiative absorptivity and emissivity holds. [ 24 ] Two bodies in radiative exchange equilibrium, each in its own local thermodynamic equilibrium, have the same temperature and their radiative exchange complies with the Stokes-Helmholtz reciprocity principle .

  8. Thermal equilibrium - Wikipedia

    en.wikipedia.org/wiki/Thermal_equilibrium

    In this situation, Kirchhoff's law of equality of radiative emissivity and absorptivity and the Helmholtz reciprocity principle are in play. Change of internal state of an isolated system [ edit ]

  9. Kirchhoff's laws - Wikipedia

    en.wikipedia.org/wiki/Kirchhoff's_laws

    Kirchhoff's laws, named after Gustav Kirchhoff, may refer to: Kirchhoff's circuit laws in electrical engineering; Kirchhoff's law of thermal radiation; Kirchhoff equations in fluid dynamics; Kirchhoff's three laws of spectroscopy; Kirchhoff's law of thermochemistry; Kirchhoff's theorem about the number of spanning trees in a graph