ons. Due to
cameras are
trology. As
racy of the
of a simple
tion of very
requires an
ation model
asks. This
of distortion
and Rollei
00 pixels in
uch as the
ies of 0.01
| have been
using self-
. In theory,
y networks
imately 1 :
,000 image
sed by the
and precise
e not yet
because the
al accuracy
ld suggest.
'e routinely
'grammetric
tes that the
indicator of
latively few
independent
coordinates,
theodolite
. Although
d with such
is of object
stability and consistency of target location measurement,
many independent tests have indicated a significantly
degraded external accuracy when compared to internal
precision.
Clearly, systematic or stochastic errors remain in the
model for the optical and electronic components of still
video cameras or the target location algorithms for image
measurement. Because there are many possible sources
of error, the best approach to the problem is one of
elimination. One area of valid research is the common
use of a simple lens model which assumes radial lens
distortions are constant with respect to the distance
between the lens and the target. This paper will
concentrate on initial research toward the evaluation of
an extended lens model. The intent of the research is the
isolation of the effects of variation of distortion with
focus distance and distance within the object space.
2. VARIATION OF DISTORTION
2.1 Variation with Focus Distance
An image is considered to be in focus at a specific
distance, known as the focus setting or focus distance for
the camera lens. The plane of best focus in the object
field is a plane parallel to the image plane.
It is well known that lens distortion varies with lens
focus. A change in the focus distance for a typical
camera with a simple lens system is achieved by a
change in the principal distance, which changes the
image magnification produced by the camera lens. The
change in the principal distance results in a change in
lens distortion which is proportional to the principal
distance and the focus distance.
Magill (1955) developed a formula for the computation
of lens distortion at any specified focus distance, or
magnification, based on two other determinations of lens
distortion profiles. The computation uses a scale factor
derived from the focal length and focus distances :
o = Os drs + ( 1 - og) ÔTs, (1)
where
org — required lens distortion at focus distance s
Org = predetermined lens distortion at focus
distance s,
Ors, = predetermined lens distortion at focus
distance s,
The scale factor og is derived from :
= $9385814251 sam (2)
S $9 - Sj ST
535
where
s, S,, s,= distances from the camera to specified
focus planes in the object space
focal length of the camera (the principal
distance at infinity focus)
f
The focal length of the camera may not be known, other
than the nominal value given by the manufacturer. The
principal distance at a specified focus distance can be
computed using the thin lens formula :
1 1.4
t omcRL (3)
S e
where
Cz principal distance
This formula can be re-arranged to conveniently give the
focal length as a function of the principal distance and
focus distance :
f. XS (4)
c+s
A focal length value averaged from the two
predetermined calibrations can be computed to provide
the maximum accuracy. Once the focal length is known,
the principal distance corresponding to the required focus
distance used in Magill’s formula can be computed using
equation (3). Other parameters required for a full
specification of the camera calibration, such as the
principal point location, may be determined by
averaging, or perhaps linear or non-linear prediction
from a series of calibrations at different focus distances
(Wiley and Wong, 1995).
The optimum accuracy of the new distortion parameters
will be gained if the two pre-determined lens distortion
profiles are as far apart in distance as possible. One set
of profiles should be obtained at a focus distance of
infinity, and a second set of profiles obtained at as short
a focus distance as possible.
In practical terms, the predetermined profiles will
generally be derived from a targeted test range
calibration, a straight (or plumb) line calibration, or a
combined test range and straight line calibration of the
camera lens (Shortis et al 1995a). The proximity of the
near focus distance calibration will be limited by field of
view and depth of field considerations. The far focus
distance calibration can generally be conducted at
infinity focus, but again field of view may be a
consideration. At the near focus distance the target or
line density may be very low, whilst at the far focus
distance the target array or straight lines may cover only
a small portion of the image format, reducing the
effectiveness of the calibrations.
Shortis et al (1995a) showed that the combination of
target array and straight line calibrations realises
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B5. Vienna 1996