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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

    There is a fundamental relationship (Gustav Kirchhoff's 1859 law of thermal radiation) that equates the emissivity of a surface with its absorption of incident radiation (the "absorptivity" of a surface). Kirchhoff's law is rigorously applicable with regard to the spectral directional definitions of emissivity and absorptivity.

  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. Low emissivity - Wikipedia

    en.wikipedia.org/wiki/Low_emissivity

    A black body would have an emissivity of 1 and a perfect reflector would have a value of 0. Kirchhoff's law of thermal radiation states that absorption equals emissivity opaque (ε opaque) for every specific wavelength/frequency (materials often have quite different emissivities at different wavelengths). Therefore, if the asphalt has an ...

  8. Diathermal wall - Wikipedia

    en.wikipedia.org/wiki/Diathermal_wall

    For investigation of Kirchhoff's law of thermal radiation the notions of absorptivity and emissivity are necessary, and they rest on the idea of one-way radiation. These things are important for the study of the Einstein coefficients , which relies partly on the notion of thermodynamic equilibrium .

  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