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ted in the foreground. Behind, the HR lens is visible,
arranged between two additional lenses for multispectral
data acquisition.
Fig. 1: Optical system of MOMS-02
For the illustration of the functional model, the object
coordinate system XYZ and the image coordinate systems
of the HR lens xy, yy, Zu and the forward looking lens x; Yr,
z, are represented in Figure 2. All coordinate systems are
right handed Cartesian, at which the image coordinate sy-
stems are defined as follows:
>» origin: centre of the first active pixel of the sensor line,
» direction of z-axis: parallel to the optical axis, pointing
downward,
> direction of y-axis: straight line through all pixel
centres,
» direction of x-axis: orthogonally completed, close to
direction of flight.
For each inclined lens an additional 6 parameter trans-
formation was introduced to rigorously model the displace-
ments Ax,Ay,Az of the projection centres (PC) and the
rotations Ag,Aw,Ax of the image coordinate system with
respect to the image coordinate system of the HR lens.
Thus, the MOMS-02 camera geometry is described by 21
parameters: 2 x 9 parameters (A @gp, A pp, App, AXpp, AYig,
AZgg, Xorps Yors Cp) for the forward and the backward (EB)
looking lens each, and 3 parameters (Xu, Yon, cy) for the
nadir looking lens. In principle, these parameters can simul-
taneously be estimated by the bundle adjustment. In
practice they will be treated as constant values, determined
by camera calibration previously. The extended collinearity
equations (2) are derived from the general approach (1)
and are applied for the inclined lenses. In case of the nadir
looking lens (Ax,=Ay,=Az,=0, M=I) the classical
collinearity equations are obtained from (2).
X, Y : image coordinates of the object point
Xo, Yo : image coordinates of the principal point
k : scale factor
M, D, R : rotation matrices (M" D" — R7?)
X, Y,Z : ground coordinates of the object point
459
X, Y» Z, : ground coordinates of the projection centre of
the nadir looking HR lens (position)
Po, 9,» K : rotation angles of exterior orientation of the
nadir looking HR lens (attitude)
Fig. 2: Coordinate systems
X-Xo X - (X,* AX)
y-yxy| = k MT(A@,Aw,Ax) D'(gy ok) | Y - (Y,*AY)
18 Z - (Z,+AZ)
AX, Ax
with |AY,| - D(os, ek) |Ay (1)
AZ, Az
ax REX) RAT Y) +R, (2-25) - (M, Ax+M, Ay+M, A7]
Tw Ry(X-X) *R4(-Y) *R4(Z-Z) - [MjAx*MjAy*MjAz]
(2)
jon RyC-X) «RJ(O-Y) *R(Z-Z) - [Mj Ax*M, Ay «MyAz]
Ry(X-X) *RÁQ-Y) *RAG-Z) - [Mj,Ax*«MAAy *MaAz]
This general approach allows for processing randomly orien-
tated image coordinate systems of lenses with different inte-
rior orientations (X, y, c). Self-calibration using additional
parameters for the correction of systematic image errors can
be applied as usual.
To demonstrate the influence of different focal lengths c,
and cz, the standard deviations oy, oy, 0, of a symmetrical
3-ray forward intersection (standard deviations of image
coordinates o, flying height h, baselength b, @,=w,=x,=0)
are listed (3). It is conspicuous, that the height accuracy
does not depend on cy, whereas all 3 rays contribute to the
planimetric accuracy. The MOMS-02 geometry (c:c;4 —
3:1) improves the accuracy in planimetry by a factor of