that were
used in the preceding pages. Then we shall derive two different linear
transformations, one corresponding to a translation,
the other to a refraction
operation. They will be characterized by a translation
matrix and a refraction matrix respectively.
With these two matrices we shall be able to treat any
optical system according to the first order theory.

The meaning of the variables y and
can be seen
from Fig. 1. For a
given plane PP the variable y represents the height
above the x axis that the
ray strikes the plane PP. The variable
represents
the angle the ray makes
with the x axis and since the slope
(dy/dx) = tan(
)
=
for
small angles, we may
take
as representing the slope of the ray as it passes
the plane PP. The
distance y above the plane is positive, below the plane
negative. The sign
of the angle
is determined from the sign of the slope
and is positive in Fig. 1.
2. The Translation Matrix

,
at PP and
',
'
we may write another linear equation as

| (15) |

A series of translations may be represented according to the rules of
matrix multiplication already discussed. For example,
suppose that the ray
strikes a further plane WW at a distance T from QQ at
angle
'' and height y ''.
In matrix form we could write




The distances T and D are always taken as positive quantities as the transformation is defined in terms of the ray direction. With the convention chosen here for expressing the unprimed coordinates as functions of the primed coordinates as in equation 15, the order of the matrices is in the direction of the ongoing ray, i.e. from left to right.
3. The Refraction Matrix At each surface separating two transparent media within an optical system, the direction of the ray may be changed according to Snell's law, which we take in the approximate form for small angles. We may express this refraction at the surface in terms of two linear equations which gives rise to the refraction matrix.

In Fig. 4, VV represents the spherical refracting
surface separating
transparent media of indices n and
may be considered to refer to
the plane through O
perpendicular to the optic axis.
At the surface the angle
changes from
to
'
| (16) |
at this
surface using
Snell's law. From Fig. 4,


| (17) |
![]() | (18) |
| (19) |
![]() | (20) |
