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> imaging
system in a self-calibrating bundle adjustment in order to
achieve high accuracy. Extended collinearity equations are
used as the functional model in self-calibrating bundle
adjustments.
m,(X- X) «m,4(Y- Y) m4(Z-Zj)
Mg, (X= Xo) + Mo (Y= Yo) + Myg(2- 20)
X+AX-X,=~C
My (X=Xo) + Mop (Y= Yo) + Myy(Z- 2)
m (X- Xy) *my4(Y- Y5) my(Z-Z;)
y*Ay-yo*-C
(1)
where, x, y are the image coordinates of the image points; X,
Y, and Z denote the object coordinates of the corresponding
object points, and Xy, y and c represent the basic interior
orientation parameters, i.e., the location of the principal point
and the calibrated principal distance; Ax and Ay stand for the
correction terms applied to the image coordinate
measurements, which are the functions of the selected APs;
m, (i,j21, 3) are the elements of the rotation matrix between
image space and object space based on three independent
orientation angles, and X,, Y,, Z, are the object coordinates
of the projection centre.
Many versions of self-calibrating bundle adjustment
algorithms exist. One of the main differences is the selection
of the APs and the composition of Ax and Ay. Due to the
non-linearity of eq.(1), linearization and iterations are
necessary for its solution.
2.2 Digital Camera and Its Calibration
A digital camera is very much like a non-metric camera in
many aspects, except for the substitution of the film with solid
state sensors. Therefore, the images captured by a digital
camera are also suffering from certain distortions due to
systematic errors during imaging, which leads to inaccurate
results. In order to exploit the potential of the
photogrammetric techniques, camera calibration is necessary
to determine the quality of the images and the imaging
system and thus to be able to efficiently compensate for the
systematic influences, which should lead to improved final
accuracy.
On the other hand, the interior geometric structure of a digital
camera is also instable, which means that its geometric
characteristics may alter to a certain extent over time. This
suggests that the calibration has to be carried out
simultaneously with the data reduction rather than as
separate laboratory calibration with subsequent data
evaluation. Consequently, self-calibration seems to be an
ideal tool to combine the two steps.
2.3 UNBASC2 Self-Calibration Method
A self-calibrating bundle block adjustment program
(UNBASC2) was developed for aerotriangulation and close-
range photogrammetric applications (Moniwa, 1977), which
can be successfully applied to a non-metric camera (Faig et
al,1990). Compared to other methods, UNBASC2 possesses
two advantages:
. Itis a photo-variant procedure with no limitation on
the number of photos, the type of camera used,
e.g. metric camera, non-metric camera or even
61
digital camera.
. No approximate initial values are needed for the
adjustment, although linearization and iteration
have to be dealt with. This is convenient for
applications, where the approximations are difficult
to obtain.
In UNBASC2, the error model comprises of the following
three independent functions which model systematic
distortions of the camera system.
2.3.1 Radial Lens Distortion. Odd power polynomials are
used to describe radial symmetric lens distortion:
= 3 5 7
dra kr? «ker ekor^ s.
(2)
which leads to its components in the photo coordinate
system:
dr =X WE 72 Kr rk su
dr,- (y- yo) (Kir? * or^ «kr? «...) (3)
where dr is the radial distortion and dr,, dr, represent the
components in x and y directions, respectively. r refers to the
radial distance between principal point and image point; k; are
the coefficients of radial distortion functions.
2.3.2 Decentering Lens Distortion. The decentering lens
distortion is defined by Conrady-Brown’s model (Brown,
1966) in UNBASC2:
dA Ap 2 prt)
[p, U? +2 (x-X0) + 2p, (XX) (Y-¥o)]
dp, = (1 «DIDI s.)
[pur *2(y-yol * 2p, (x-X3) Q/-9)] (4)
where p; are decentering distortion parameters.
Usually, k,, k,, k, andp ,p, are sufficient to define the
radial and decentering lens distortion for most commercial
non-metric cameras (Faig, 1973). If not, higher order terms
could be included.
2.3.3 Film Deformation. Originally, an affine transformation
is employed to model the film deformation,
dq,- A(y-X,)
dq, - B(y-y)) ©)
where A and B are parameters defining scale change and
non-perpendicularity of coordinate axes. Due to the fact that
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B1. Vienna 1996