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  2. John William Strutt, 3rd Baron Rayleigh - Wikipedia

    en.wikipedia.org/wiki/John_William_Strutt,_3rd...

    John William Strutt, 3rd Baron Rayleigh (/ ˈ r eɪ l i /; 12 November 1842 – 30 June 1919), was an English physicist and mathematician.He spent all of his academic career at the University of Cambridge.

  3. Rayleigh scattering - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_scattering

    Rayleigh-type λ −4 scattering can also be exhibited by porous materials. An example is the strong optical scattering by nanoporous materials. [ 23 ] The strong contrast in refractive index between pores and solid parts of sintered alumina results in very strong scattering, with light completely changing direction each five micrometers on ...

  4. Rayleigh - Wikipedia

    en.wikipedia.org/wiki/Rayleigh

    Rayleigh waves; Rayleigh (unit), a unit of photon flux named after the 4th Baron Rayleigh; Rayl, rayl or Rayleigh, two units of specific acoustic impedance and characteristic acoustic impedance, named after the 3rd Baron Rayleigh; Rayleigh criterion in angular resolution; Rayleigh distribution; Rayleigh fading; Rayleigh law on low-field ...

  5. It Takes The Entire Rainbow Of Colors To Make The Sky Blue ...

    www.aol.com/takes-entire-rainbow-colors-sky...

    It might seem like a simple question. But the science behind a blue sky isn't that easy. For starters, it involves something called the Rayleigh effect, or Rayleigh scattering. But that same ...

  6. Scattering - Wikipedia

    en.wikipedia.org/wiki/Scattering

    Rayleigh scattering is a process in which electromagnetic radiation (including light) is scattered by a small spherical volume of variant refractive indexes, such as a particle, bubble, droplet, or even a density fluctuation. This effect was first modeled successfully by Lord Rayleigh, from whom it gets its name.

  7. Ultraviolet catastrophe - Wikipedia

    en.wikipedia.org/wiki/Ultraviolet_catastrophe

    The ultraviolet catastrophe, also called the Rayleigh–Jeans catastrophe, was the prediction of late 19th century and early 20th century classical physics that an ideal black body at thermal equilibrium would emit an unbounded quantity of energy as wavelength decreased into the ultraviolet range.

  8. Rayleigh distribution - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_distribution

    In probability theory and statistics, the Rayleigh distribution is a continuous probability distribution for nonnegative-valued random variables. Up to rescaling, it coincides with the chi distribution with two degrees of freedom .

  9. Rayleigh number - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_number

    K is the mean permeability (of the initial portion of the mush) L is the characteristic length scale; α is the thermal diffusivity; ν is the kinematic viscosity; R is the solidification or isotherm speed. [8] A-segregates are predicted to form when the Rayleigh number exceeds a certain critical value.