74 
Table 17. Exterior orientation. Terrestrial Metric Camera, TMK. Values in 
millimeter and radians. 
y o 
CO 
cp 
X 
s 
s 
s 
s 
s 
s 
xo 
Y0 
ZO 
CO 
cp 
X 
First series: 
Station 1 
+ 3759.423 
+ 1.675 
—2519.291 
+ 0.032 
+ 0.977 
—0.038 
1.211 
0.691 
1.050 
<0.0005 
<0.0005 
<0.0005 
” 2 
+ 3680.258 
+ 92.492 
—2421.642 
+ 0.009 
+ 0.943 
+ 1.547 
1.114 
0.743 
1.060 
<0.0005 
<0.0005 
<0.0005 
” 3 
+ 3706.730 
—4.235 
—2654.332 
—0.061 
+ 0.912 
+ 3.212 
1.354 
0.734 
1.342 
<0.0005 
<0.0005 
<0.0005 
” 4 
+ 3677.770 
+ 19.465 
—2444.782 
—0.004 
+ 0.874 
+ 4.664 
1.157 
0.660 
1.153 
<0.0005 
<0.0005 
<0.0005 
Second series: 
Station 1 
+ 3721.276 
+ 2.155 
—2539.032 
+ 0.025 
+ 0.804 
—0.030 
1.116 
0.822 
1.015 
<0.0005 
<0.0005 
<0.0005 
” 2 
—3137.720 
+ 34.976 
—2697.152 
—0.044 
—0.708 
—0.062 
0.999 
0.848 
0.905 
<0.0005 
<0.0005 
<0.0005 
” 3 
+ 92.559 
+ 2051.690 
—2917.325 
—0.537 
+ 0.026 
—0.008 
0.958 
1.101 
1.186 
<0.0005 
<0.0005 
<0.0005 
” 4 
—50.680 
—1522.905 
—2432.777 
+ 0.456 
+ 0.034 
—0.042 
0.663 
0.853 
0.904 
<0.0005 
<0.0005 
<0.0005 
X 0 , Y 0 , Z 0 , oj, cp, x provide, in total, thirty unknown quantities. The observations 
were given equal weights. The calculation was programmed for the CD 3200* 
In the first series the camera station was the same for the four exposures but 
the camera was given four different ^-values. In the second series there were 
four different camera stations symmetrically located with the camera directed 
towards the center of the test field. The convergence of the solution was obtai 
ned after five iterations in both cases. The standard errors of unit weight was 
7.8 /¿m and 9.2 ¡urn respectively. The computed interior orientation is given in 
Table 16 and in Fig. 24. The resulting exterior orientations are given in Table 
Table 17. The number of degrees of freedom is 42 in both cases. The radial dis 
tortion curves, that were obtained from the computations, are transformed so 
that they are located near the r-axis. This changes the camera constants to Ci = 
59.990 and c 2 — 59.880 mm. See Fig. 24. 
The observations have also been adjusted with the interior orientation defi 
ned by the parameters x 0 , y 0 and c, i.e. the radial distortion has not been deter 
mined. The same standard errors of unit weight as above were obtained. This 
is due to the fact that almost all points have approximative^ the same radius. 
The results are shown in Table 18. 
26110. 
not