The laws of refraction state that for a refracting surface between two transparent media:
=
n ' sin
',
(Snell's law),
is the angle of incidence and
'
is the angle of refraction, the angle
between the normal to the surface and the
refracted ray, and n and n ' are the
indices of refraction of the media on either
side of the refracting surface.
The index of refraction of a medium is defined
as the ratio of the speed of
light in vacuum to the speed of light in the medium.
In first order theory, which essentially involves
the first term in the
series expansion for the sine of the angle, Snell's
law is used in the
form
n
= n '
'.
A better approximation than the
first order theory involves
higher order terms in the expansion which gives
rise to the third and fifth
order theories. The results of the higher order
theories are usually expressed
in terms of the defects in the image formed by
spherical refracting surfaces,
the so-called monochromatic aberrations.
In what follows we shall concentrate on the subject of refraction, on the basis of first order theory, leaving the subject of reflection to be treated later as a special case.