about 2 compared to the ratio of 1:1. The height accuracy
is not affected, as mentioned already.
1 h? 1
0,70,- oy —— 3677 997 3 (3)
2Cp p*CN 2C p
2.2 Reconstruction of the exterior orientation
The functional model of the bundle adjustment is based on
extended collinearity equations. The exterior orientation
parameters are estimated only for so-called orientation
images (OI), which are introduced at certain time intervals.
Between the OI, the parameters of each individual image
line are expressed as functions (e.g. polynomials) of the
parameters of the neighbouring orientation images (Müller,
1991). A variety of different parameter models for the
reconstruction of the exterior orientation were applied in
the past (see survey in Wu, 1986). The goal of each
approach is the minimization of the interpolation error
using as few parameters as possible.
Investigations, based on simulated orbit data, showed that
3rd order polynomial functions approximate the orbit quite
accurately. Therefore the linear interpolation function, used
in the bundle block adjustment program CLIC previously,
was replaced by a Lagrange Polynomial (LP) approach (4).
It,
J
nr (4)
J*
>
P) - Y. P)
i-0
[; 3
-
In (4) the exterior orientation parameters P(t) at time t are
expressed as a linear combination of the related parameters
P(t) assigned to the n+1 neighbouring orientation images i
at time t. The main characteristics of the LPs are: The LP
coefficients are explicitly the (unknown) exterior orientation
parameters of the orientation images; the LP order can
easily be changed by the definition of the parameter n. The
linear interpolation therefore remains applicable by setting
n = 1. The complete extended collinearity equations are
derived by replacing the exterior orientation elements X,,
Yo Lo 9» €» K, in equations (2) by the related expres-
sions (4).
2.3 Introduction of offset and drift parameters
In principle, the reconstruction of the exterior orientation of
three-line-imagery is possible by means of photogrammetric
measurements and ground control information only.
However, precise position and attitude observations
essentially improve the accuracy of point determination,
especially if little or weak ground control information is
available (Ebner et al., 1991).
In case of MOMS-02/D2,
information is available:
» position and attitude data from an onboard Inertial
Navigation System (INS),
» position data from the Tracking Data Relay Satellite
System (TDRSS),
» position data from sophisticated orbit models.
the following additional
All these rather heterogeneous data of position and attitude
have to be combined and transformed into a common
coordinate system.
460
Basically, all measurements are affected by blunders,
random and systematic errors. Blunders must be located
and eliminated a priori by robust estimation methods.
Random errors can be processed by least squares
adjustment. The critical aspect is the influence of systematic
errors. They should be described by the functional model.
In our case the different systematic errors of the position
and attitude data are modeled through additional unknown
parameters. By limitation to constant and linear terms
which, describe the main effects, twelve additional
parameters, namely an offset and a drift parameter for each
exterior orientation parameter, have to be estimated during
the bundle adjustment.
3. SIMULATIONS
In the past a series of simulations was carried out for
MOMS-02/D2 to analyze the effect of certain parameters
on the accuracy of point determination and to give recom-
mendations in the planning phase of the project concerning
the technical design of the camera or additional measure-
ments during the mission (Ebner et al, 1991; Ebner and
Kornus, 1991). Based on these results, new simulations are
performed to show the attainable accuracy using the
extended functional model and realistic input information.
In the following the input information and the results of the
simulations are presented.
3.1 Input information
3.1.1 Camera and mission parameters The geometric
configuration is established by the MOMS-02/D2 camera
and mission specifications. The most conspicuous feature is
the extremely small image angle, which results in a ratio
between flying height and swath width of 8:1. This is an
essential handicap for a precise geometric evaluation.
The parameters used in the simulations are listed in table 1
and match the nominal values of the project to a large
extent.
view direction of the lens forward nadir backward
calibrated focal length [mm] 2372 660.0 2372
pixel size [4m] 10.0 10.0 10.0
ground resolution [m] 13.5 4.5 13.5
convergency angle A« [deg] -21.9 0.0 21.9
orbit height [km] 296
orbit inclination [deg] 28.5
swath width [km] 36
strip length [km] 468
Table 1: Simulation parameters
The camera is mounted on top of the space shuttle, which
will move along a 296 km high orbit with an inclination of
28.5°. Besides the recording of single strips in normal (bay
down) flight attitude of the shuttle, some orbits will be
flown with a shuttle cross inclination of 30°. As shown in
(Ebner et al., 1991) the accuracy of point determination can
be improved by convergent sensor configuration either
obtained by an instrumental sensor line convergency or by
inclining the camera carrier in case of parallel sensor
arrangement.
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