whereas for objects near unit magnification (q = 2f),
7 e». (29)
This indicates that the percentage variation in distortion between near field and far
field limits of the photographic field diminishes with increasing magnification, being
only about 1/8 as much at unit magnification as at zero magnification.
CONDITION FOR INVARIANCE OF DISTORTION BETWEEN NEAR AND FAR
FIELD LIMITS
From (27) it is clear that there are two conditions which will lead to
invariant distortion throughout the photographic field, namely, when either
q-1 = O or 2-p = 0. The first condition corresponds to the trivial situation of infinite
magnification (and hence zero depth of field). On the other hand, the second
condition which requires that p = 2 (or equivalently that K; = 4K, 2e ) appears to
be physically attainable by design. Evidence for this is provided in Table 1 in which
we have listed the values of p corresponding to 22 Hypergon lenses as computed from
measured data presented by Magill (1955). By design, the Hypergon is a perfectly
symmetric lens. Accordingly, p should ideally have a value of zero. As is shown
in Table 1 only two of the samples achieve this ideal value, while the remainder
have values ranging from a low of -6.7 to a high of 45.2. This demonstrates that
p can be highly sensitive to manufacturing variations.
TABLE 1. Values of p for 22 Hypergon lenses as
computed from data given by Magill (1955).
r^
o
=
wn
Lens p p
46
.22
17
il
86
13
67
.14
. 64
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Qo 4. 0 U 5» dg o
Qo =
o q
>>> >>> >>> >>
t
+
PP STREET
7
EXAMPLES OF LENS-TO-LENS VARIATIONS IN CLOSE RANGE DISTORTION
e The effect that the value of p has on the behavior of distortion is illustrated
in Figures 3 and 4 in which results for four of the Hypergons listed in Table 1 are
employed. Of the selected lenses two correspond to the smallest and largest values