International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part BS. Istanbul 2004
number of parameters in photogrammetric adjustment
and strengthens it.
Bh
NX
Figure 3: First and second steps of GPSSIT supported
terrestrial photogrammetry
3. MATHEMATICAL MODEL
Bundle adjustment is the most appropriate adjustment
method used in digital photogrammetery since it depends
on analytical principals and is a numerical technique.
Colinearity condition, which depends on a line aligning
the points on object, perspective center of camera and on
the image of the object, is the algorithm that forms the
mathematical model of GPSSIT supported terrestrial
photogrammetry. Respecting this condition, all the lines
passing through a central point and touch to two parallel
planes at the each ends of the line are divided in two parts
by the camera perspective center and the rate of these two
parts on the same line one to another will be the same and
constant for the other lines as well. Point of
photogrammetric view, the central point described here is
the camera perspective center and the plane close to the
point is called as image plane and it is a real plane. The
important description here, which does not match the
theory above, is that the other plane is not a plane in
practice. It is often an actual 3D space. For a metrical
evaluation, image and object mediums both must be
referred to one apiece metric system. These two reference
systems are called image and object reference systems in
photogrammetry. In GPS supported terrestrial
photogrammetry, image coordinate system is the same as
image coordinate system in the current digital
photogrammetry, in spite of that the object coordinate
system is designated with respect to GPS coordinate
system that uses WGS84 datum. The coordinates
obtained in GPS coordinate system can be transformed
into a desired local coordinate system if it is required.
This requirement comes out only if there is an offset
between the point determined by GPS antenna and the
point that the camera perspective center is referred. In the
other case, the mathematical model to be formed
photogrammetrically can be described directly in GPS
coordinate system without the need for such a
transformation. In this case and even considering that the
coordinate systems are not parallel one another, the
equation, which expresses the relationship between image
coordinate system and GPS coordinate system that the
object is described in, can be given as below;
m d —
X aps. X) 7*9 X aps. j
Y zm AR, y d Yo == Yops- ( 1 )
trs! E f Zps- j
where,
[Xars-i Yaps-i Zasil : Is GPS coordinates of r'th object
point, :
[Xarsj Yars-j Zaps] : is GPS coordinates of perspective
center of j'th image,
xj and y; : 1s image coordinates of i'th object
point in j’th image,
X, and y, : is image coordinates of image
center,
i : is scale factor of i'th point in the
j th image,
R; : is rotation matrix of j'th image
with respect to GPS coordinate system and
f : 1s focal length of the camera used.
After moving the term of [Xaps-i Y Gps. Zi in
equation 1 to the left side of the equation and then
multiplying the both sides of the arranged equation by
]
—R , the new form of the equation can be written as
pe ir
below when it is divided the first and second rows of the
equation by the third one.
A 4 d 5 7
zt n ri Xess -Xops;) * Tix; CYobs; 7 Yrs ) +r, +i (Zaps = Zins) > (2)
Xi = 3 ; T = = t 0
à Duos; = Xorsid * aaa Yorsi ^ Yursi) t Nai (Zaps z Zorsi?
+ -f Ly; (Kips = Xorsi) * og Yon EY, sj) t Po (Zarss ~Zorsi) € ( 3 )
n hu (Xopsi -Xcrsj )* Fo (Yop 4 Yos; ) + hes -Zops;) T?
, ; 2 T
Cis Piper; are elements rotation matrix of R;
between image coordinate system and WGS84 coordinate
systems. Here it is worth to mention that the coordinates
of camera perspective center (XGps-j, Yaps-j Zaps-) in the
above equation are not any longer unknown and they
enter to the equation above as constant values. Since they
are determined by GPS antenna when GPSSIT supported
terrestrial photogrammetry is used in the field. In this
case, 7 unknown parameters in normal case reduce to 4, if
the used camera is a camera whose image coordinates of
its image center and its focal length (x,, y,, f) are known.
If the used camera is not a metric camera and image
coordinates of its image center and its focal length (Xo, Yo
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