Full text: XVIIIth Congress (Part B5)

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Fig. 1. The adopted camera model. 
  
  
2. THE SYSTEM SETUP 
2.1. Camera Model 
What it is normally meant with camera model is the 
mathematical relationship between the position of a point 
in the three-dimensional space imaged by the camera, 
and the corresponding position of that point on the image 
plane. The scheme of the camera model that we adopted 
for our 3D reconstruction system is shown in Fig. 1, 
where three reference frames are visible: 
e World reference frame, attached to the imaged 
scene; 
e Camera reference frame, attached to the camera 
system. Notice that the Z axis is the optical axis, 
while the X and Y axes are parallel to the image 
plane. 
e Image reference frame, where the x, and y; axes 
respectively define the horizontal and vertical 
directions in the digital image. 
The camera model consists of a set of equations that 
map the 3D world-coordinates (Xy, Yu, Zu) of a generic 
point P into the 2D coordinates (x; y; of its projection 
onto the image plane: 
e Change of reference frame from world-coordinates to 
camera-coordinates: 
X 
cam 
PaT7|Yas|-R: B,*T; 
cam 
Z 
cam 
R and T being the rotation matrix and the translation 
vector, respectively. 
e Perspective projection of a scene point to the image 
plane (the center of projection is the center of the lens 
and the projection plane is the camera CCD sensor): 
X 
P^ end 
Yu z 
cam 
e Lens distortion shift of the point position p,, predicted 
via perspective projection, to the actual position py on 
the image plane. When standard-resolution CCD 
cameras are being used, only radial distortion is 
507 
normally considered. In this case, in fact, the 
tangential distortion can be neglected. Radial 
distortion is usually approximated by a power series: 
K, = (Lkr hor +.) 
This series can be truncated at the fifth order (only 
the first two coefficients are used) as the residual 
error results as being far below 1 pixel [4]. 
e Change of coordinate frame from camera-coordinates 
Pd(XaYa). to  image-coordinates p=(x,y;). This 
operation simply consists of a 2-D translation and 
scale change (see Fig. 1): 
  
X 
x, =C, +++; 
y A de 
Ya 
Gk 
Yr Y d, 
d, and d, being the horizontal and vertical size of an 
image pixel, respectively, and (C,,C,) the image- 
coordinates of the optical center OC. 
As we can see from the above description, a camera 
model is completely specified by a limited set of 
parameters. In particular, the intrinsic parameters (f, ks, 
ks, C,, Cy) incorporate the physical characteristics of the 
camera, while the extrinsic parameters (R and T) define 
the projective geometry, and they all are estimated 
through an appropriate calibration procedure. 
2.2. Multi-View Geometry 
The multi-camera acquisition system is designed in such 
a way to guarantee a satisfactory camera geometry for 
back-projection. More precisely, the cameras are placed 
far enough from each other to guarantee an accurate 3D 
triangulation, and they are approximately pointed to a 
common center in the scene. By doing so, in fact, we 
maximize the 3D volume which is being simultaneously 
imaged by all cameras. 
It is well-known that the minimum number of cameras 
that is required for obtaining a 3D description of the 
scene is two. Increasing the number of cameras, 
however, improves the precision and the reliability of the 
3D reconstruction dramatically [6]. In particular, the 
introduction of a third camera has been proven to provide 
the most significant improvement with respect to the 
binocular setup, with a minimum cost increment. The 
results presented in this paper are thus obtained by using 
a trinocular system. 
Once the cameras are properly placed, camera 
calibration is performed in order to determine the intrinsic 
and extrinsic parameters of the acquisition system. In 
order to do so, a set of calibration target points, whose 
3D world-coordinates are known with good precision, is 
used. It is worth noticing that the camera model 
introduced above is used throughout the whole 3D 
reconstruction chain (matching and  back-projection 
algorithms). This means that there is no need of image 
rectification or any constraint on the camera geometry. 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B5. Vienna 1996 
 
	        
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