4/11/2024 0 Comments Intensity of light equation powerSunlight is also subject to Raman scattering, which changes the rotational state of the molecules and gives rise to polarization effects. Rayleigh scattering of sunlight in Earth's atmosphere causes diffuse sky radiation, which is the reason for the blue color of the daytime and twilight sky, as well as the yellowish to reddish hue of the low Sun. The particles may be individual atoms or molecules it can occur when light travels through transparent solids and liquids, but is most prominently seen in gases. The particle, therefore, becomes a small radiating dipole whose radiation we see as scattered light. The oscillating electric field of a light wave acts on the charges within a particle, causing them to move at the same frequency. Rayleigh scattering results from the electric polarizability of the particles. For light frequencies well below the resonance frequency of the scattering medium (normal dispersion regime), the amount of scattering is inversely proportional to the fourth power of the wavelength, e.g., a blue color is scattered much more than a red color as light propagates through air. Rayleigh scattering ( / ˈ r eɪ l i/ RAY-lee), named after the 19th-century British physicist Lord Rayleigh (John William Strutt), is the predominantly elastic scattering of light, or other electromagnetic radiation, by particles with a size much smaller than the wavelength of the radiation. Rayleigh scattering causes the blue color of the daytime sky and the reddening of the Sun at sunset. For the wireless communication effect, see Rayleigh fading. For the stochastic distribution, see Rayleigh distribution. For the magnetic phenomenon, see Rayleigh law. This article is about the optical phenomenon.
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