PE&RS July 2016 Public - page 526

as
transferring the patches from the base image to the target
image
(as shown in Figure 1).
Change Analysis
Since the major reason for proposing the
PWCR
method in
this study, is to be able to use the multi-view-angle images for
change detection, it has to be proven that after the coregistra-
tion, changed patches can be detected by comparing the spec-
tral properties of the corresponding patches in the bi-temporal
images. Therefore, we examined the so-produced coregistered
patches in change detection. We tested two change detection
criteria: Image Differencing and
MAD
Transform. Image dif-
ferencing is a simple method and
MAD
transform is a more
advanced method for change detection. In this section, more de-
tails are provided regarding the used change detection criteria.
Image Differencing
The subtraction between coregistered multispectral images
provides a simple way to detect changes. With this crite-
rion, small intensity differences indicate no change, while
large positive or negative values indicate changes. Decision
thresholds specify the significance of change which are usu-
ally expressed in terms of standard deviation from the mean
difference value (Canty, 2014).
In this study, we use the mean value of the correspond-
ing patches in the Image Differencing algorithm to detect the
changed patches.
MAD Transform
MAD
Transform, which can be considered as an extended
version of
PCA
(principle component analysis), is used as
another change identifier in this study. In
PCA
change detec-
tion, the primary component contains consistent information
between the bi-temporal datasets, whereas the secondary
component captures the difference (Chen and Hutchinson,
2007). However, as Nielsen
et al.
, (1998) state,
PCA
is depen-
dent on scale, number of channels, and forces the same gain
setting of intensity measurements (in the sensors), while
MAD
is designed to compensate for the shortages of
PCA
. A
MAD
Transform is linear scale invariant; which means it is insensi-
tive to linear radiometric and atmospheric effects (Nielsen
et
al.
, 1998). Because of the linear model of the
MAD
Transform,
it can be inferred that this method is also capable of compen-
sating for the slight individual bandwidth dissimilarities (if
they are linear) in different sensors.
MAD
Transform is based on measuring the difference of a
linear transformation of two multispectral vectors from bi-
temporal images, X and Y, in such a way that the variance of
the intensities is maximized (Canty, 2014):
D a X b Y
T
T
= −
(7)
in which,
a
and
b
are coefficients calculated based on Canoni-
cal Correlation Analysis. As a result, the multispectral bands
are transformed into a new space (
D
) in which the changes are
highlighted.
Study Area
The proposed framework is implemented on four bi-temporal
satellite image datasets, from the city of Hobart, Tasmania,
Australia, and Fredericton, New Brunswick, Canada, each
covering at least a one square kilometer area. The coverage
areas contain typical urban structures with combinations of
small to large and low to moderately high elevated buildings.
Photographs of the study areas are presented in Figure 6.
Table 1 reports the specifications of the satellite images
used in this study. The bi-temporal combinations of the im-
ages and DSMs for change detection are presented in Table 2.
The datasets are selected from images with different view-
ing angles (both azimuth and off-nadir angles are different),
Figure 6. Photographs of the study areas: (a) a combination of houses and elevated condos, Fredericton, Canada (dataset ID: DT4); (b) a
combination of houses and industrial buildings in Hobart, Australia (dataset IDs: DT1 and DT2); and (c) a typical developed urban envi-
ronment in Hobart, Australia (dataset ID: DT3)
T
able
1. M
etadata
of
S
atellite
I
mages
U
sed
in
this
S
tudy
Data
IK62
IK74
IK75
Geo000
Geo001
WV2
WV2
Satellite name
Ikonos
Ikonos
Ikonos
GeoEye1
GeoEye1
Wordview2
Wordview2
City name
Hobart
Hobart
Hobart
Hobart
Hobart
Fredericton Fredericton
Country
Australia
Australia
Australia
Australia
Australia
Canada
Canada
Date
2003-02-22
2003-02-22
2003-02-22
2009-02-05
2009-02-05
2011-07-20
2013-08-18
Sat. Az (deg)
293.74
329.42
235.74
193.69
53.48
169.9
226.6
Sat. Elev. (deg)
75.17
69.14
69.20
70.06
63.87
72.9
59.1
Solar Az. (deg)
47.1
47.21
46.9
59.58
59.58
154.8
167.9
Solar Zenith (deg)
41.2
41.23
41.1
40.62
40.62
23
33.4
Approx. GSD (m)
0.9
0.9
0.9
0.5
0.5
0.5
0.58
T
able
2. B
i
-
temporal
C
ombinations
of
S
atellite
I
mages
U
sed
in
this
S
tudy
Dataset
ID
Target
Image
Base
Image
Source
of DSM
DSM
Accuracy
DT1
IK62
Geo000
Geo000-Geo001
stereo imagery
0.5m
DT2
IK75
Geo000
Geo000-Geo001
stereo imagery
0.5m
DT3
IK74
Geo001
Geo000-Geo001
stereo imagery
0.5m
DT4
WV2-2013 WV2-2011 LiDAR data
0.5m
526
July 2016
PHOTOGRAMMETRIC ENGINEERING & REMOTE SENSING
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