SPACE TRIANGULATION USING AFFINE TRANSFORMATION
ATSUSHI OKAMOTO
KYOTO UNIVERSITY KYOTO JAPAN
COMMISSION III
ABSTRACT
If the DLT method is applied for space triangula-
tion with satellite photographs, high correlations
arise among the orientation unknowns due to very
small height differences in the terrain for the fly-
ing height of the platform. This difficulty can
however be overcome by using ground point co-
ordinates calculated by means of affine transfor-
mation as the initial values for the iterative solu-
tion. This approach is tested with simulated ex-
amples and is revealed to have a fairly good accu-
racy.
INTRODUCTION
The DLT method(Abdel-Aziz and Karara(1971))
is a general orientation approach of photographs.
This method is usually applied for the analysis of
non-metric photographs. Employing the DLT ap-
proach for the analysis of satellite photographs,
the attained accuracy may not be so high due to
very high correlations among the orientation pa-
rameters, because height differences in the pho-
tographed terrain are very small in comparison
with the flying height of the platform. In order to
overcome this problem, this paper proposes an
orientation method of adopting ground point co-
ordinates as the initial values for the iterative so-
lution, which were calculated by means of an ori-
entation theory of photographs based on affine
transformation(Okamoto, et al(1989,1991,1992)).
Also, the proposed method is applied for space tri-
angulation with simulated satellite photographs
taken consecutively in a convergent manner. The
camera is assumed to be a non-metric one. Fur-
ther, the analysis of satellite CCD camera im-
ageries with a very narrow field angle is per-
formed using the orientation theory based on
affine transformation.
OUTLINE OF THE PROPOSED ORIENTATION
METHOD
The basic theory for analyzing affine imageries
346
has first been constructed by Okamoto(1989) and
in detail explained in the paper by Okamoto, et
al(1991,1992). However, this theory cannot be
applied for the analysis of conventional pho-
tographs without transforming the central-per-
spective imageries into affine ones. Thus, this
transformation will first be discussed.
Let the ground surface be flat and a central-per-
spective photograph be taken with the rotation
angles o and 9. The reference coordinate sys-
tem (X,Y,Z) is selected as a right-handed, rectan-
gular Cartesian system with its origin at the pro-
jection center of the photograph and with its X-Y
plane parallel to the scaled ground surface, as is
demonstrated in Figure-1. Further, the photo-
graph is considered to intersect the scaled ground
surface in such a way that its principal point H lies
on the surface. The three-dimensional coordinates
(Xp, Yp.Zp) of an image point p(x,y) of the central-
perspective photograph are expressed with respect
to the reference coordinate system in the form
Xp cose Osing |[1 O0 0 X
35.451..0..1.—0 0 coso -sino || Y | (1)
Zp sing 1 cose [LO sinw coswlL-C
y
Da (Xa, ya)
Figure-1 : transformation of a central-perspective
photograph into an affine one
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