74
Chapter 2. Geometrical optics
This gives
k M
−1 δy I =
2
A ) ]
B [ 4 y A (x
2
A + y
+ C [ 2 y O (x O x A + y O y A ) ]
D [ 2 y A (x O + y
2
2
O ) ]

+

E [ y O (x O + y
2
O ) ]
2
2
+

F [ y O (x A + y
2
) + 2 y A (x O x A + y O y A ) ]
+

A
e [ x O (x O + y
2
2
O ) ]
2
+

c [ −x A (x
2
O
2
− y O ) + 2 x O y O y A ]
A ) + 2 y A (x O y A − y O x A ) ].
+

2 + y
A
+ f [ x O (x
(2.217)
We notice that
δx Oj = M
−1 δx Ij
(2.218)
is the aberration, demagnified to the object plane z O . We call δx Oj
the aberration referred to the object plane. This is of interest for
a transmission electron microscope, for example, where the object
coordinates form the natural reference for the expression of image
quality. Similarly, one has the option of substituting x O = M
−1 x I
and y
1
O = M
− y I on the right sides of (2.216, 2.217), thus referring the aberrations to the image plane z I . This is of interest for
a probe forming system, like a scanning electron microscope or
focused ion beam system, where one typically forms a demagnified image of a source. In this case, the image coordinates form
the natural reference. Either object or image coordinates correctly
express the aberrations.
A significant simplification is possible by choosing the rotation
of coordinate axes so that y O = 0; i.e., the off-axis object position
is located along the x-axis. There is no loss of generality, owing to
the axial symmetry, as the coordinates for any single object point
can always be chosen in this way.
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