Kakiuchi, Tsutomu
3 CAMERA CALIBRATION USING VIDEO THEODOLITE
For camera calibration, control points should be generated and its image
coordinates also should be acquired. Camera calibration procedures are as
follows: When the telescope is pointing to Py point under the condition
that the distance is D from the center of the video theodolite to R,
horizontal angle H, and vertical angle V;, the image point to Po is taken as
po on the right and left image respectively. Next, when the video
theodolite is rotated H; angle, the image point to Po is taken as p; on the
right and left image, and the object position to image point p; becomes Pj.
Similarly, when the video theodolite is rotated V; angle, the image point
to Py is taken as p», the object to p? becomes P». Repeating this operation, : sine
control points are taken on the stereo image and are produced in the space Figure 5. Camera calibration
respectively based on Figure 5.
Ground coordinates for these control points are calculated following equation.
X; = DcosV, sin(H, H,)
1
Y;- Dos V;sinV, sinV;cosV, cos(H; H, X (1)
Z; = Disinv, sinV, + cosV; cos V, cos(H, H,)
Camera calibration for the right and left image was performed using 9 control points, which were produced in the above
procedure.
4 PRE EXPERIMENT
4.1 Experiment Method
In order to estimate the accuracy of 3D measurement of the stereo vision system and the relationship between the
rotation parameters ( " ) and the reading angles (zenith, horizontal) of the video theodolite, the following pre-
experiments were performed using the test field (Figure 6).
Figure 7 shows the three test models (Z=0mm, 20mm, 50mm) were used in this paper. The black white rectangular
target is a control point corresponds the above Py, and other 38 black circle points are check points for checking 3D
accuracy
® 00 00
4cm - Control Point (Po)
€ es.
dem d «€ e Z = 0mm, 20mm, 50mm
4cm
i ® 00 00
cm
f ® 00 00
cm
® 00 0600
"HFeejeejee
4cm 7cm 4cm 7cm 4cm
Figure 6. Test site Figure 7. Test model
The following image A1 (Figure 8) was taken from 2.4980m as the original
orientation image. The left-hand number superimposed in the upper left corner
shows the horizontal angle Ho=0 00). The number just to the right is the
zenith (Vo=0 00, V=90 -Zenith angle) and the distance (D=2.4980m).
Figure 9 shows the right and left image for camera calibration which was
interpolated by above concept.
Camera calibration for the right and left image was performed by the same
procedure noted above using one control point on the test model.
For the unknown parameters, exterior orientation parameters( "o, 0, 0
(rotation parameters), Xo, Yo, Zo (camera positions) and interior orientation
parameters (f, xo, yo (principal points), a;, a? (scale factor), p ;(lens distortion)}.
Figure 8. Orientation image
416 International Archives of Photogrammetry and Remote Sensing. Vol. XXXIII, Part B5. Amsterdam 2000.