Almost all solids and liquids have refractive indices above 1.3, with aerogel as the clear exception. Gases at atmospheric pressure have refractive indices close to 1 because of their low density. These values are measured at the yellow doublet D-line of sodium, with a wavelength of 589 nanometers, as is conventionally done. ![]() A few examples are given in the adjacent table. PMMA (acrylic, plexiglas, lucite, perspex)įor visible light most transparent media have refractive indices between 1 and 2. Selected refractive indices at λ = 589 nm.įor references, see the extended List of refractive indices. Where the coefficients A and B are determined specifically for this form of the equation. The relative refractive index of an optical medium 2 with respect to another reference medium 1 ( n 21) is given by the ratio of speed of light in medium 1 to that in medium 2. Such lenses are generally more expensive to manufacture than conventional ones. įor lenses (such as eye glasses), a lens made from a high refractive index material will be thinner, and hence lighter, than a conventional lens with a lower refractive index. ![]() In this case, the speed of sound is used instead of that of light, and a reference medium other than vacuum must be chosen. It can also be applied to wave phenomena such as sound. The concept of refractive index applies across the full electromagnetic spectrum, from X-rays to radio waves. Nevertheless, refractive indices for materials are commonly reported using a single value for n, typically measured at 633 nm. For most materials the refractive index changes with wavelength by several percent across the visible spectrum. The imaginary part then handles the attenuation, while the real part accounts for refraction. Light propagation in absorbing materials can be described using a complex-valued refractive index. This effect can be observed in prisms and rainbows, and as chromatic aberration in lenses. ![]() This causes white light to split into constituent colors when refracted. ![]() The refractive index may vary with wavelength. This implies that vacuum has a refractive index of 1, and assumes that the frequency ( f = v/ λ) of the wave is not affected by the refractive index. The refractive index can be seen as the factor by which the speed and the wavelength of the radiation are reduced with respect to their vacuum values: the speed of light in a medium is v = c/ n, and similarly the wavelength in that medium is λ = λ 0/ n, where λ 0 is the wavelength of that light in vacuum. The refractive indices also determine the amount of light that is reflected when reaching the interface, as well as the critical angle for total internal reflection, their intensity ( Fresnel's equations) and Brewster's angle. This is described by Snell's law of refraction, n 1 sin θ 1 = n 2 sin θ 2, where θ 1 and θ 2 are the angle of incidence and angle of refraction, respectively, of a ray crossing the interface between two media with refractive indices n 1 and n 2. The refractive index determines how much the path of light is bent, or refracted, when entering a material. In optics, the refractive index (or refraction index) of an optical medium is a dimensionless number that gives the indication of the light bending ability of that medium. Ratio of the speed of light in vacuum to that in the medium A ray of light being refracted through a glass slab
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