a zero, and a long bar represented a 1. The entire
control field covered an area of 2.25 m(H) x 2.75
m(W) x 2.41 m(D). The locations and sizes of the
targets were designed so as to provide a minimum of
12 targets of sufficient size and dispersion to
facilitate the calibration of zoom lenses of the
entire focal range of 12.5 mm to 75 mm. The three-
dimensional coordinates of the center of each target
were determined by triangulation. The average
estimated standard errors of the target coordinates
were computed to be: O, - + 0.3 mm, Oy, = + 0.8 mm,
and 6, - 0.4 mm. The X- and Z- axes lied in a
vertical plane, with the X-axis being horizontal and
the Z-axis being in the vertical direction. The Y-
axis was horizontal and approximately along the
depth of the target field.
4. DISTORTION MODEL
After extensive experimental tests, the following
model was found to provide excellent representation
of the distortion characteristics of a vision System
at a given focal length setting( Wiley and Wong,
1990; Wong et al, 1991):
dx s lxr? « [p (r? « 227) * 2p, Xy]
dx = Lyr? + [2p, xy +p, lr? + 2y°)]
x = (X = 2) (1 + &k)
«i
Il
<
l
v
r?-xX4y?
where x and y are image coordinates; and y, are
image coordinates of the principal point; k is a
scale factor for the x-coordinates; I4, is the first
term of symmetric radial distortion; and p, and p;
are the first two terms of decentering lens
distortions.
5. TARGETING ALGORITHM
An algorithm was developed to automatically identify
and locate the center of each target in an image.
It consisted of the following steps:
1. find the approximate locations and identification
numbers of all the targets in an image using the
method reported in Wong et al (1988);
2. perform sub-pixel edge detection along the
boundary of each target using local thresholds;
and
3. compute the image coordinates of the center of
each target by least-squares fitting with an
elliptical template.
The estimated standard error of the computed
coordinates of the target centers typically ranged
between + 0.005 and + 0.02 pixel. There was no
significant difference in the targeting accuracy of
the two types of cameras used, in spite of the
slightly higher resolution of the Pulnix cameras.
This was largely attributed to the size of the
targets, which typically had a diameter of more than
10 pixels in the calibration images.
6. CALIBRATION IMAGES
Images of the control field were obtained using the
following six different combinations of camera and
zoom lenses:
Combin- Serial Serial
ation Camera No. Lens No.
3 Pulnix TM80 001146 Fujinon 987894
2 Pulnix TM80 001136 Computar 1473508
3 General TCZ-200 7001009 Computar 1472638
4 Pulnix TM80 001146 Fujinon 994104
5 Pulnix TM80 001136 Fujinon 994104
6 General TCZ-200 6027001 Computar 1473508
In each case, the camera-lens combination was
positioned in front of the control field and at a
distance of approximately 5.5 m from the center of
the target field. A total of 16 images were
acquired in sequence for each combination at the
following nominal focal settings: 12.5, 15, 20, 25,
30,:35, 40, 45, 50, 55, 60, 65, 70, 75, 12.5, and 15
mm.
7. FREE CALIBRATION
A free calibration was performed for each focal
setting of each camera-lens combination by a bundle
adjustment. Only the object-space coordinates of
the control targets were constrained in an
adjustment, which yielded the following: six
exterior orientation parameters of the camera (X,
VS, Z°, Q, ¢, and x); and five interior orientation
parameters ( f, k, L., p,, and p,).
Table 1 lists the root-mean-square errors (RMS) of
the residuals for all the adjustments. For focal
length of 35 mm or shorter, the RMS errors were
between + 0.05 and + 0.09 pixel. The small
magnitude of the RMS errors for these adjustment
confirmed the validity of the distortion model as
well as the accuracy capability of the targeting
algorithm. For focal lengths greater than 35 mm,
largely because of the fewer number of control
points available in each calibration image and the
degradation in resection geometry, the RMS errors
were increased to between + .07 and + .17 pixels.
Figure 2 shows the changes in the interior and
exterior orientation parameters with respect to the
focal setting for camera-lens combination 4. Space
limitation does not permit the inclusion of similar
plots for the other five cases. As can be expected,
there were small systematic changes in the exterior
orientation parameters. Changing the focal setting
resulted in a small movement of the exposure center
and, in some cases, small changes in the direction
of' the optical axis. In all six cases, the changes
in the interior orientation parameters were also
highly systematic.
Of particular interest from the free calibration
results are that 1) there were large linear shift of
the principal point, and 2) decentering distortions
were quite large. For camera-lens combinations Nos.
2 and 5, which involved the same camera, linear
shift of the principal point amounted to about 90
pixels, and decentering distortions amounted to
about 5 pixels near the edge of the images acquired
with f- 75 mm. Discussions with A. Burner of NASA
led to the conclusion that both of these phenomena
were most likely caused by tilting of the optical
axis with respect to the focal plane. Burner
reported that tilts of up to 0.5 degree were not
uncommon in this type of cameras (Burner et al,
1990). A linear. shift of the principal point
amounting to 80 pixels over the zoom range of 12.5
mm to 75 mm would be equivalent to a tilt of only 1
degree.
One obvious approach to zoom lens calibration is to
simply model these patterns with a separate
polynomial for each of the parameters. Another
possible approach is to use these calibration
results directly in a table look-up scheme. The
problem with both of these two approaches is that
corrections for changes in exterior orientation
parameters must be applied for different focal
settings.
Further analysis of the results from free
calibration showed that the RMS errors for the
exterior orientation parameters were quite large
comparing to the magnitude of changes when the focal
length was varied between 12.5 and 75 mm. Much of
the problem was due to the small field of view at