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Webster 1913 Edition


Refraction

Re-frac′tion

(r?-fr?k′sh?n)
,
Noun.
[F.
réfraction
.]
1.
The act of refracting, or the state of being refracted.
2.
The change in the direction of ray of light, heat, or the like, when it enters obliquely a medium of a different density from that through which it has previously moved.
Refraction
out of the rarer medium into the denser, is made towards the perpendicular.
Sir I. Newton.
3.
(Astron.)
(a)
The change in the direction of a ray of light, and, consequently, in the apparent position of a heavenly body from which it emanates, arising from its passage through the earth’s atmosphere; – hence distinguished as atmospheric refraction, or astronomical refraction.
(b)
The correction which is to be deducted from the apparent altitude of a heavenly body on account of atmospheric refraction, in order to obtain the true altitude.
Angle of refraction
(Opt.)
,
the angle which a refracted ray makes with the perpendicular to the surface separating the two media traversed by the ray.
Conical refraction
(Opt.)
,
the refraction of a ray of light into an infinite number of rays, forming a hollow cone. This occurs when a ray of light is passed through crystals of some substances, under certain circumstances. Conical refraction is of two kinds; external conical refraction, in which the ray issues from the crystal in the form of a cone, the vertex of which is at the point of emergence; and internal conical refraction, in which the ray is changed into the form of a cone on entering the crystal, from which it issues in the form of a hollow cylinder. This singular phenomenon was first discovered by Sir W. R. Hamilton by mathematical reasoning alone, unaided by experiment.
Differential refraction
(Astron.)
,
the change of the apparent place of one object relative to a second object near it, due to refraction; also, the correction required to be made to the observed relative places of the two bodies.
Double refraction
(Opt.)
,
the refraction of light in two directions, which produces two distinct images. The power of double refraction is possessed by all crystals except those of the isometric system. A uniaxial crystal is said to be optically positive (like quartz), or optically negative (like calcite), or to have positive, or negative, double refraction, according as the optic axis is the axis of least or greatest elasticity for light; a biaxial crystal is similarly designated when the same relation holds for the acute bisectrix.
Index of refraction
.
See under
Index
.
Refraction circle
(Opt.)
,
an instrument provided with a graduated circle for the measurement of refraction.
Refraction of latitude
,
longitude
,
declination
,
right ascension
,
etc., the change in the apparent latitude, longitude, etc., of a heavenly body, due to the effect of atmospheric refraction.
Terrestrial refraction
,
the change in the apparent altitude of a distant point on or near the earth's surface, as the top of a mountain, arising from the passage of light from it to the eye through atmospheric strata of varying density.

Webster 1828 Edition


Refraction

REFRAC'TION

,
Noun.
The deviation of a moving body, chiefly rays of light, from a direct course. This is occasioned by the different densities of the mediums through which light passes.
Refraction out of a rarer medium into a denser, is made towards the perpendicular.
Refraction may be caused by a body's falling obliquely out of one medium into another.
Refraction double, the separation of a ray of light into two separate parts, by passing through certain transparent mediums, as the Iceland crystal. All crystals, except those whose primitive form is either a cube or a regular octahedron, exhibit double refraction.

Definition 2021


refraction

refraction

See also: réfraction

English

A soda straw in a glass of liquid shows the refraction of light in the liquid.

Noun

refraction (plural refractions)

  1. (physics) The turning or bending of any wave, such as a light or sound wave, when it passes from one medium into another of different optical density.
  2. (metallurgy) The degree to which a metal or compound can withstand heat

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