International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV,
X. > (A PA)" qd PL (3)
X (K) 2 (A! PA - KI)! A' PL (4)
Xo. (€)=c(A PAY ATPL (5)
where X, 7 least squares (LS) estimation value
X,(K) 7 ridge estimation value
X . (c) = stein estimation value
Stein
I = unit matrix
K =the ridge parameter vector (K, > 0)
C = the stein parameter( ¢ > 0)
If each element in vector K is equal, the ridge estimator is
regarded as the ordinary ridge estimator; else the ridge
estimator is deemed as the generalized ridge estimator. The
second item in equation (2) is constantly zero for the least
square estimator since it is an unbiased estimator. But for the
ridge estimator and the stein estimator the second item is no
longer zero since they are biased estimators.
The combined ridge-stein estimator can be represented below:
Xo (d)=(A"PA+ 1)" (A"PL+dD)X,,
: (6)
- Q(A* I) (^*dl)Q' X,
where — Q - eigenvector matrix
A = eigenvalue matrix
d = the CRS parameter, 0 <d <1
The CRS estimator possesses three favorable characteristics in
comparison with the ridge estimator and the stein estimator.
(1) The CRS estimator is more accurate than the ridge
estimator and the stein estimator.
From the viewpoint of statistics a good estimation value should
have a minor MSE. The MSE value of the CRS estimator is
smaller than the ridge estimator and the stein estimator when
d is optimum, therefore, the CRS estimator is more accurate.
(2) The CRS estimator is superior to the ridge estimator and the
stein estimator in reliability and stability.
To get correct and accurate estimation results, the ill-
conditioned state of the normal equation must be changed. The
CRS estimator alters the ill-conditioned state much more
significantly than the ridge estimator and the stein estimator,
therefore, its reliability and stability are more excellent.
(3) The solution for the CRS estimator is unique and simple.
Since the CRS estimator is a linear function to its estimation
parameter, the optimal value for d is ascertained when
11
MSE(X ,. ) - 0.
d= Poti TTT (7)
: $ d (d) = ó, Y 6: + À, p (d)
e (A «ly ES oA Al)
where Y. (d) is the canonical value for X o5 (0) „which
is imported to facilitate and simplify computation.
Part B4. Istanbul 2004
foy (8)
Y. (d) 2 Q'X (d) S (A1) (^ dI)A" (4Q) L (9)
3. THE CRS ESTIMATOR'S APPLICATION IN
LINEAR PUSHBROOM IMAGERY EXTERIOR
ORIENTATION
3.1 Theoretical Basis
This paragraph is mainly concerned with how to apply the CRS
estimator in linear pushbroom imagery exterior orientation. The
linear pushbroom imagery has multiple perspective centers and
each scan line has an unique set of perspective center and
rotation angles. The collinearity equation between a image pixel
on the ith scan line (x;, 0) and its corresponding object point in
the object spcae (X, Y, Z) is as follows:
AX X) Y) 7 Z)
! " a(X- X )-b(Y-Y)*e(Z-Z,) (10)
Qo ,0(X-X) -(Y-Y)*e(Z-Z.)
7" a(X-X)-bY-Y)*«Z-Z).
The y coordinate along the flight direction is implied in the
position and attitude of the satellite at a given time, which can
be linearly related to the location and attitude of the central
linear array as follows:
9,79, *eky
0-0, &y
K,m/k,* My a1)
Xj-X 4 + X y
y, eV i+ & y
Zelt
so
where f= focal length
A Z ; dis: gas ati
Oy Os Kor X os Yıosl,y = exterior orientation
elements of the central scan line
^ Y . . +
9,0. K Xu 454, ^ exterior orientation elements
of the ith scan line
a;, bj, c; ^ elements of rotation matrix
&, dx, s, X ; *, X — variation rates of exterior
orientation elements.
Each scene has 12 exterior elemets ( Q9, , €, , K,, X unda du
&, dA, i&, XX, Y, &). Among them X, and ,, Y, and
@, are highly correlated. A small change in @, is
indistinguishable from a small change in X , . Similarly, small
changes in Y, and @, can’t be differentiated either. The strong
correlation induces the coefficient matrix of the normal
equation A" PA singular, the normal equation ill-conditioned
and some eigenvalues A, in the eigenvalue matrix A close to
zero as well. Accordingly, the MSE value of least square
728
Intern
estim:
estim:
The ri
the fir
equati
Y (z
i=l
ill-cor
AP
value
A +R
compr
à, 100
with tl
value
and in
A Erin
estima
it hasn
in its ı
specul
Horel-
Galarr
compc
scale
differe
i.e. the
don't «
estima
In the
for A’
and the
toward
the infi
À, / d.
At the
infinite
compre
corres
minor «
conclu
state of
rationa
estimat
MSE v
stein es
The ex
by the (
Step 1:
elemen