2.2 The Accuracy of the Operator in Orienting
the Imaainary Camera(or theodolite ) and the
Metric Camera in the Field.
The accuracy of measuring the spac
co-ordinates(8X$,8Ys and 8Ds)of the metric
camera , imaginary camera and/or theodolite
stations should be nearly the same, and that is
because we used the same stations and the same
co-ordinate system , while the accuracy from
setting the orientation parameters(w, 9 , k ) in
the field for the metric camera depends mainly
on the type of camera .
In artificial cameras or theodolites , we can
achieve accuracy in setting the orientation
parameters Sw , 50 and Sk between 0".0 in the
imaginary cameras to 1".0 or less in the
theodolite which cannot be achieved by using
metric cameras .
2. The Pointing Errors of th rator
There is no need for a comparator to measure
the fictitious image co-ordinates , and
consequently there are no pointing errors for
the artificial photographs . In the metric
photographs the pointing accuracy of a
photogrammetric operator is a function of many
parameters such as the model scale , the
operator experience and the model's
photographic contrast . The pointing accuracy
can be estimated from the repeated
measurements of different points S
-2.4 _ Aspects of Results
As a result , we can exnect that the accuracy
obtained theoretically by using (APPT) method
is better than that obtained by using (MPPT)
method .
3. EXPERIMENTAL COMPARISON
Three different cameras (Zeiss (Jena) UMK ,
Wild P32 and Galileo Santoni metric cameras )
were used in the comparison between the MPPT
and APPT methods . A non - metric camera was
also used (Nikon FM 35 mm ) , as well as a Wild
T2 one second theodolite .
1 Field Work
Four photographs were taken with each of the
three metric cameras and the non - metric
camera . For each camera two of the
photographs were taken from the left camera
station (S1) and two from the right camera
station (S2).The base distance (B,) was
28.508m and the elevation difference between
the two stations (By) was 0.232 m .
The spatial positions of (9) control points
(which were not lying in one plane ) were
surveyed on the same co-ordinate system of the
camera stations, using a Wild T2 theodolite .
3.2 Laboratory Work
The image co-ordinates of the non - metric
photography and the nine control points on each
metric photograph were measured on a Hilger
and Watts stereocomparator The ground
co-ordinates of (24) control points were
computed(using a bundle solution).
By applying the perspective transformation and
using the points (4,5,6 and 7 ) , the image
co-ordinates on the non - metric photograph
were transformed to metric image co-ordinates
The artificial image co-ordinates of the control
points 4,5,6 and 7 were calculated from the
space co-ordinates .
By applying the perspective transformation the
image co-ordinates on the non - metric
photograph were transformed to image
co-ordinates on the artificial photograph .
The mean standard deviation values (&Xm , SYm ,
&Dm and SRm ) of the space co-ordinates of a
total of 18 targets (control points ) computed
from the APPT , MPPT ( Zeiss (Jena) UMK , Wild
P32 and Galileo Santoni ) and the Direct linear
Transformation (DLT) method , are listed in
Table 1 . The standard deviation values ( SX , SY
, §D) were calculated by using the emprical
accuracy indicator (Gruen,1978).
4. ANALYSIS OF RESULTS, CONCLUDING
REMARKS AND RECOMMENDATIONS
(1)In the APPT method there is no need for
development and processing of the artificial
image . Also there is no need for a comparator
to measure the imaginary camera image
co-ordinates which are obtained from the
observed control points .
(2)In the APPT method there is no limitations on
the depth of field and the format size .