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DEM generation from Worldview-2 stereo imagery and vertical accuracy assessment for its application in active tectonics

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The DEM-generation technology from high-resolution satellite imagery enables us to generate a wide range of high-resolution topographic data rapidly, improving the efficiency of data acquisition greatly. This method is more efficient than airborne Light Detection And Ranging (LiDAR) in terrain reconstruction, since satellite imagery covers a larger area without difficulties in field deployment. Previous researches evaluated the accuracy of DEMs generated from stereo imagery of different satellite sensors, however there is not enough quantitative analysis concerning the capability of satellite-based DEM in active tectonic studies. Therefore, in this paper, we presented a study to investigate the accuracy to measure heights of fault scarps using the DEM obtained from Worldview-2 stereo imagery and chose the Kumysh fault in the southern margin of Kumysh Basin (Eastern Tian Shan, China) as our test site. Point cloud data were obtained from stereo satellite imagery, both with and without GCPs respectively. Prior to the generation of the DEM, we compared the overall elevation differences of the point clouds and the fault scarp swaths. The overall elevation difference ranges from −1.2 to 0.4 m, with the mean value of −0.57 m, while the elevation difference of fault scarp swaths range from −1.1 to 0 m, with the mean value of −0.4 m. Afterwards, we generated a 0.5 m resolution DEM of 5-km swath along the Kumysh fault, measured the heights of fault scarps on different levels of alluvial fans, and compared the topographic profiles obtained from DEM and post-processed differential GPS (ppGPS) survey. Our results show that: (1) the elevation difference between the topographic profiles ranges from −2.82–4.47 m, the shape of the fault scarp can be accurately reconstructed by satellite-based DEM with the deviation of 0.29 m after elevation correction; (2) the accuracy of the height measurement of fault scarps can reach 0.25 m. These findings indicate that the DEM generated from Worldview-2 stereo imagery is capable of measuring relative deformed topographic features, which could be of great interest to professionals exploring the use and accuracy of satellite stereo imagery for active tectonic applications.
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DEM generation from Worldview-2 stereo imagery and vertical accuracy
assessment for its application in active tectonics
Siyu Wang
a,b
,ZhikunRen
a,b,
,ChuanyongWu
c,d
, Qiyun Lei
e
,WenyuGong
a
,QiOu
f
, Huiping Zhang
a
,
Guangxue Ren
b
, Chuanyou Li
b
a
State Key Laboratory of Earthquake Dynamics, Institute of Geology, China Earthquake Administration, Beijing 100029, China
b
Key Laboratory of Active Tectonics and Volcano, Institute of Geology, China Earthquake Administration, Beijing 100029, China
c
Guangdong Provincial Key Laboratory of Geodynamics and Geohazards, School of Earth Sciences and Engineering, Sun Yat-sen University, Guangzhou, China
d
Earthquake Administration of Xinjiang Uygur Autonomous Region, Urumchi 830001, China
e
Earthquake Administration of Ningxia Hui Autonomous Region, Yinchuan 750001, China
f
COMET, Department of Earth Sciences, University of Oxford, Oxford OX1 3QR, UK
abstractarticle info
Article history:
Received 16 August 2018
Received in revised form 12 March 2019
Accepted 15 March 2019
Available online 19 March 2019
The DEM-generation technology from high-resolution satellite imagery enables us to generate a wide range of high-
resolution topographic data rapidly, improving the efciency of data acquisition greatly. This method is more ef-
cient than airborne Light Detection And Ranging (LiDAR) in terrain reconstruction, since satellite imagery covers a
larger area without difculties in eld deployment. Previous researches evaluated the accuracy of DEMs generated
from stereo imagery of different satellite sensors, however there is not enough quantitative analysis concerning the
capability of satellite-based DEM in active tectonic studies. Therefore, in this paper, we presented a study to inves-
tigate the accuracy to measure heights of fault scarps using the DEM obtained from Worldview-2 stereo imagery
and chose the Kumysh fault in the southern margin of Kumysh Basin (Eastern Tian Shan, China) as our test site.
Point cloud data were obtained from stereo satellite imagery, both with and without GCPs respectively. Prior to
the generation of the DEM, we compared the overall elevation differences of the point clouds and the fault scarp
swaths. The overall elevation difference ranges from 1.2 to 0.4 m, with the mean value of 0.57 m, while the el-
evation difference of fault scarp swaths range from 1.1 to 0 m, with the mean value of 0.4 m. Afterwards, we
generated a 0.5 m resolution DEM of 5-km swath along the Kumysh fault, measured the heights of fault scarps
on different levels of alluvial fans, and compared the topographic proles obtained from DEM and post-
processed differential GPS (ppGPS) survey. Our results show that: (1) the elevation difference between the topo-
graphic proles ranges from 2.824.47 m, the shape of the fault scarp can be accurately reconstructed by
satellite-based DEM with the deviation of 0.29 m after elevation correction; (2) the accuracy of the height measure-
ment of fault scarps can reach 0.25 m. These ndings indicate that the DEM generated from Worldview-2 stereo
imagery is capable of measuring relative deformed topographic features, which could be of great interest to profes-
sionals exploring the use and accuracy of satellite stereo imagery for active tectonic applications.
© 2019 The Authors. Published by Elsevier B.V. This is an open access article under the C CB Y-NC-ND license (http://
creativecommons.org/licenses/by-nc-nd/4.0/).
Keywords:
Stereo imagery
DEM
Fault scarp
Active tectonics
Accuracy analysis
1. Introduction
Digital Elevation Model (DEM) enables us to quantify the stages of
surface processes using discrete mathematical model to characterize
surface topography (Burbank and Anderson, 2011). High spatial resolu-
tion terrain data could be used to monitor earth surface deformation, es-
pecially for some inaccessible areas by comparing multi-temporal DEM,
including active tectonics (Binet, 2005;Mitchell and Chadwick, 1999;
Ren et al., 2014;Zhou et al., 2015), landslide (Mora et al., 2003;
Stumpf et al., 2014), polar resea rch (Shean et al., 2016) and glacier mon-
itoring (Fieber et al., 2018). In the study of active tectonics, substantial
researchhas been conducted using high-resolution DEM, which can dis-
play detailed displacement offault and provides a new method to study
the pattern of surface rupture and fault geometry (Barišin et al., 2015;Bi
et al., 2018;Hashimoto et al., 2010;Turker and Cetinkaya, 2005).
Several techniques are suitable for high quality DEM generation,
such as real-time dynamic data from GPS, Interferometric Synthetic Ap-
erture Radar (InSAR) images, Light Detection And Ranging (LiDAR)
technology, Unmanned Aerial Vehicles (UAV) survey, high resolution
satellite stereo imagery and so on. Traditional eld topographic survey
is time-consuming, labor-intensive and inefcient; InSAR has shown a
Geomorphology 336 (2019) 107118
Corresponding author at: State Key Laboratory of Earthquake Dynamics, Institute of
Geology, China Earthquake Administration,Beijing 100029, China.
E-mail addresses: rzk@ies.ac.cn,lzkren@gmail.com (Z. Ren).
https://doi.org/10.1016/j.geomorph.2019.03.016
0169-555X 2019 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
Contents lists available at ScienceDirect
Geomorphology
journal homepage: www.elsevier.com/locate/geomorph
great potential for capturing surface deformation caused by various geo-
physical phenomenon with high resolution and precision (Hashimoto
et al., 2010;Massonnet et al., 1992;Wright, 2004;Zebker et al., 1994).
But the quality is limited by the geometry and temporal baseline, atmo-
spheric artifacts and existence of ground deformation; LiDAR is an effec-
tive way to study the distribution characteristics of seismic deformation
and the mode of strong earthquake rupture (Kondo et al., 2008;Ren
et al., 2015;Ren et al., 2018;Zielke et al., 2010) since it can scan the
fault zone in a wide range and gets topographic data of decimeter
level. However, high cost limits its wide application; In recent years,
UAV technology combined with Structure from Motion (SfM) has
greatly improved the efciency of the acquisition of topographic data
(Angster et al., 2016;d'Oleire-Oltmanns et al., 2012;James and
Robson, 2012;Westoby et al., 2012). Nevertheless, it is limited by the
weather condition and can only obtain photos over small areas. With
the development of digital photogrammetry and image matching tech-
nology, high-resolution satellite imagery has become another source
high-resolution DEMs (Aguilar et al., 2013;Shean et al., 2016;Zhou
et al., 2015). In the study of active tectonics, a small number of stereo
imagery is sufcient to cover the entire study area, which greatly re-
duces the cost and is especially helpful for the regions with harsh cli-
mate and accessible difculties, providing a robust method for
measuring the surface deformation.
High-resolution surface topography and the height of fault scarps
are valuable for studying coseismic deformation and fault geometry. It
enables us to measure three-dimensional surface displacements in the
earthquake and to calculate accurate slip rate. High accuracy height of
scarp can reduce the uncertainty of slip-rate calculation. With the ad-
vent of the very high-resolution (VHR) optical satellites, such as
IKONOS, Pleiades, GeoEye-1, Worldview-2 and so forth, a large number
of researches have documentedthe accuracy of DEM extracted from ste-
reo imagery and its effectiveness in terms of different applications
(Deilami and Hashim, 2011;Fabris and Pesci, 2005;Poli et al., 2015;
Reinartz et al., 2006;Saldaña et al., 2012;San and Suzen, 2005;Shaker
et al., 2010;Zhou et al., 2015). Saldaña et al. (2012) analyzed the plani-
metric and vertical accuracy of DSM generated from GeoEye-1 stereo
pairs and the results were better than 0.5 m. Shaker et al. (2010) tested
Indian Remote Sensing (IRS) - 1D stereo images and IKONOS stereo im-
ages. The accuracy of the extracted features was found to be within a
pixel-level by empirical mathematical models. The vertical accuracy of
DEM extracted from Pleiades Tri-stereo-pair can reach 0.3 m, compared
with LiDAR data (Zhou et al., 2015). However, there are still few studies
on the quantitative analysis of the accuracy of DEM generated from
Worldview-2 stereo imagery in studying active tectonics. In this study,
we chose the Kumysh fault as the research subject with less vegetation,
used Worldview-2 panchromatic band stereo imagery to generate DEM
and Geo post-processed differential GPS (ppGPS) to survey ground
control points (GCPs). Then we analyzed the accuracy of generated
point clouds under the condition of without GCPs and with GCPs. In
order to evaluate the accuracy of DEM in terms of describing the feature
of fault scarps and its validation in measuring the height of scarps, four
topographic proles across fault scarps in the eld were surveyed and
Fig. 1. Active tectonic map of the study area and stereo imagery coverage region. (a) Tectonic setting of the Eastern Tian Shan. The Cenozoic tectonism due to Eurasia-India collision is
responsible for the north-south shortening of theTian Shan. The black dashed rectangle is the location of (b). (b) Themajor faults of the Eastern Tian Shan.Black rectangle shows the cov-
erage of Worldview-2 stereo imagery (c). (c) Distribution of GCPs and topographic proles surveyed across the fault scarps. YMTF: YaMaTe fault; BGDSF: Bogda southern fault; HSKF:
HuoYanShan fault; BAF: Bolokenu-Aqikekuduke fault; BETF: Baoertu faut; KMSF: Kumysh fault; YQNF: North-edge fault of Yanqi basin; YQSF: South-edge fault of Yanqi basin.
108 S. Wang et al. / Geomorphology 336 (2019) 107118
compared to proles measured from DEM. This work will provide infor-
mation about geometric distribution and deformation characteristics of
Kumysh fault. The aim of this study is to quantitatively evaluate
whether this method is suitable for a wide range application of active
tectonic research.
2. Study site and datasets
2.1. Study site
In the past few decades, many studies focused on the deformation
characteristics and slip rates of northern Tian Shan and southwestern
Tian Shan (Burchel et al., 1999;Dumitru et al., 2001;Huang et al.,
2015;Thompson et al., 2002;Wang, 2004;Xiao et al., 2013;Yin et al.,
1998). There is still little attention on the internal tectonic deformation
of Tian Shan. The study site Kumysh Basin is located in the eastern seg-
ment of Tian Shan (Fig. 1). The late Quaternary movement characteris-
tics of faults around the Kumysh Basin are rarely reported. It is a typical
basin-mountain landform with multiple levels of alluvial fans develop-
ing at the edgeof the basin. There are different heights of fault scarps de-
veloping on the alluvial fans formed by the thrust fault. Because of the
strong collision between the Indian and Eurasian plate, the Tibetan Pla-
teau had been greatly uplifted and it blocks warm wet air from the
Indian Ocean. Since the Quaternary, theKumysh Basin had been charac-
terized by a typical continental arid climate with annual precipitation
less than ~ 150 mm/yr and sparse vegetation coverage. Thus, it is an
ideal site to test the applicability of VHR stereo imagery in active
tectonics.
2.2. Dataset
Worldview-2 is a high-resolution commercial satellite launched by
DigitalGlobe in the United States on October 8, 2009. It runs in a sun-
synchronous orbit at the altitude of 770 km and the average revisit pe-
riod is 1.1 days. The Worldview-2 sensor provides panchromatic imag-
ery with the resolution of 0.46 m (0.52 m resolution imagery when
deviating from sub-satellite point of 20°) and multispectral band
image with the resolution of 1.8 5 m (2.07 m resolution imagery
when deviating from sub-satellite point of 20°) (Jawak and Luis,
2011). The data used in this paper are Worldview-2 panchromatic ste-
reo imagery with sub-meter resolution. It covers the south edge of
Kumysh Basin, and were acquired on November 25, 2013. The overlap
of images is 90% without clouds. There was no recorded strong earth-
quake that may cause surface deformation in the study area and sur-
rounding area since the images were acquired. More detailed
information is shown in Table 1.
Field surveying and mapping of GCPs and cross-scarp topographic
proles were completed on November 15, 2017. GPS observations
were recorded using the Trimble Geo handheld Global Navigation
Satellite Systems with an external Trimble Zephyr 2 antennas (Fig. 2).
This measurement system uses the FastStatic GNSS surveying mode,
whose horizontal precision is 3 mm + 1 ppm RMSand vertical precision
is 3.5 mm + 0.5 ppm RMS. The maximum distance between the rover
and master is more than 12 km (http://www.trimble.com/, accessed
on 19 December 2018). In the mountainous area, this measurement sys-
tem does not need real-time communication of two stations and would
not be affected by the terrain, which is portable and much lighter than
the real time kinematic (RTK) differential system. The coordinate sys-
tem employed was UTM Zone 45 N, each point was recorded every 1 s
until its vertical precision was stable within 2 cm. Post-processing cor-
rections were applied in the software GPS Pathnder. Error reports
showed the error was controlled within 15cm,whichcanmeetthere-
quirements of this research to measure topographic prolesacrossfault
scarps and accuracy analysis.
3. Methodology
The basic theory of using satellite stereo imagery to acquire DEM is
to match the feature points according to the image overlaps and gener-
ate the 3D coordinates from these points, then further reconstruct a spa-
tial stereo model and obtain ne 3D information of the ground (Fig. 3).
Worldview-2 provides a rational polynomial coefcient (RPC) le con-
taining a rational function model representing the relationship between
object and image coordinates (Dolloff and Theiss, 2012). The ratio poly-
nomial is dened as below:
L¼LSNumlU;V;WðÞ
DenlU;V;W
ðÞ
þL0;S¼SSNumSU;V;WðÞ
DenSU;V;W
ðÞ
þS0;ð1Þ
NumlðU;V;WÞ
DenlðU;V;WÞ;
NumsðU;V;WÞ
DensðU;V;WÞis the normalized image coordinates, (U,V,W)
is the normalized ground coordinates, (L
s
,S
s
) is the normalized propor-
tional parameter, (L
0
,S
0
) is the normalized translation parameter. Num
l
Fig. 2. Geo 7x and Zephyr 2 antennas for ppGPS surveying. (a) The master station. (b) The rover station.
Table 1
The metadata information of the stereo images.
File name Rows Columns Acquisition
time
Solor elevation
Angle
Solar
azimuth
Satellite elevation
Angle
Satellite
azimuth
Cloud
coverage
Forward Image 13NOV25051910 16,280 35,820 2013-11-25
05:19:01 26.7° 170.8° 71.0° 52.2° 0%
Backward
Image 13NOV25052028 16,284 35,860 2013-11-25
05:20:21 26.7° 171.1° 61.0° 169.9° 0%
109S. Wang et al. / Geomorphology 336 (2019) 107118
(U,V,W), Den
l
(U,V,W), Num
s
(U,V,W), Den
s
(U,V,W) can be expressed as
the following polynomial respectively:
m¼a1þa2Vþa3Uþa4Wþa5VW þa6VW þa7UW þa8V2þa9U2
þa10W2þa11 UVW þa12 V3þa13VU2þa14VW 2þa15 V2U
þa16U3þa17 UW2þa18V2Wþa19 U2Wþa20 W3
ð2Þ
The total coefcients of 4 polynomial functions are stored in one le
containing 80 rational polynomial coefcients (RPC), through which we
can calculate the ground coordinates.
Erdas 2015 Leica Photogrammetry Suite (LPS) platform was used to
carry out relative orientation, absolute orientation, automatically
matching tie points and aerotriangulation. Its core module contains
all the functions required for orthophoto mapping, supports a
Fig. 4. Extracted DEM fromstereo imagery. (a)The DEM generated without addingGCPs. (b) The zoom-inpicture of DEM withoutGCPs (c) The DEM generated withadding GCPs. (d) The
zoom-in picture of DEM with GCPs, same location as (b). The red stars represent the location of zoom-in picture. (For interpretation of the references to color in this gure legend, the
reader is referred to the web version of this article.)
Fig. 3. Principle diagram of DEM generation from stereo imagery.
110 S. Wang et al. / Geomorphology 336 (2019) 107118
wide range of satellite sensor models, and provides an application
platform for geometric correction, orthophoto correction, information
extraction and engineering mapping. We used the eATE module to
extract digital terrestrial model as its more advanced algorithm
for high precision terrain model generation and terrain analysis
than ATE. It can output the extracted elevation information in high-
density point cloud format, which can be then ltered, and interpolated
to DEM (Zhou et al., 2015). The major steps are illustrated as
followed.
3.1. Create a block le
The initial task is to determine the geometric model, with the devel-
opment of satellites, some new commercial high-resolution satellites
starts to provide Rational Polynomial Coefcient (RPC) model only,
which contains the relationship between object coordinates and
image coordinates without sensor parameters (Büyüksalih et al., 2012;
Dolloff and Theiss, 2012). This study selected the Worldview RPC
model and UTM projection.
3.2. Automatic relative orientation
After importing forward and backward images, we need to create
pyramid model and carry out interior orientation based on the RPC
model to establish the conversion relationship between object and
image coordinates.
3.3. Absolute orientation
There are 12 GCPs evenly distributed on the image. They were sur-
veyed by Geo 7x ppGPS in the eld, with centimeter level measurement
accuracy. LPS predicts the position of GCPs automatically when we im-
port them. If the matching position is inaccurate, manual ne-tuning
can be performed to improve accuracy.
3.4. Automatically match tie points
We took the corresponding image points to calculate the relation-
ship of two images according to the position of the GCPs, and to com-
plete relative orientation in LPS. Setting larger search window size can
get higher accuracy. We then carried out absolute orientation by calcu-
lating external orientation elements.
3.5. Aerial triangulation
The number of iteration is set to 10. The generated accuracy reports
show that the accuracy is 0.166 pixels with GCPs, and 0.921 pixels with-
out GCPs.
Fig. 5. (a) Elevation difference of the point cloudswith and without GCPs.X-Xand Y-Yare two swath proles across the faultscarps. (b) Thedistribution of elevation difference. (c)Gauss
distribution of elevation difference.
Table 2
Accuracy analysis for the DEM without ground control points.
Points number Δx(m) Δy(m) Δz(m)
1 0.01 0.02 0.17
20.56 0.80 0.12
30.79 0.11 0.42
4 0.10 0.39 0.01
50.70 0.44 1.32
6 0.13 0.27 2.39
70.62 0.03 0.42
80.12 0.44 0.45
9 0.18 1.04 4.88
10 0.47 0.68 1.70
11 0.13 0.10 0.95
12 0.03 0.03 0.89
RMSE 0.44 0.51 1.82
111S. Wang et al. / Geomorphology 336 (2019) 107118
Fig. 6. Compared point clouds across fault scarp. Swath proleX-Xacross the fault data (a) and corresponding distribution of elevation difference (b). Projected elevation difference for
prole X-Xin latitude direction (c) and Gauss distribution of elevation difference (d). Swath prole Y-Yacross the fault in the compared point cloud data (e) and corresponding
distribution of elevation difference (f). Projected elevation difference for prole Y-Yin latitude direction (g) and Gauss distribution of elevation difference (h). The locations of X-X
and Y-Yare showed in the Fig. 5a.
112 S. Wang et al. / Geomorphology 336 (2019) 107118
3.6. Generate DEM
Using eATE module to generate point cloud le and convert it into
text format, we then ltered it in 0.5 m cell, and used continuous tension
curvature spline interpolate method (Smith and Wessel, 1990) with
tension coefcient of 0.75 to generate DEM.
The generated DEMs are shown in Fig. 4. Apart from the mountain
area that is in the low quality due to the shadow effects from the optical
satellite imagery, the topography of the rest area is well described. Com-
paring the DEMs generated with GCPs and without GCPs, the terrain
relief of the later one is more distinct and elevation value is about 1 m
larger than the DEM with no GCPs added. As can be seen from the
zoom-in pictures (Fig. 4b, d), the DEM is much smoother and has less
null value after adding GCPs.
4. Accuracy analysis
The application of digital photogrammetry, computer vision and
image matching technology achieves large area three-dimensional
measurement, but there are many factors affecting its accuracy
Fig. 7. Fourtopographicproles surveyedby ppGPS in the eld (see Fig. 1c for locationon the DEM). (a) The locationsof Prole 1, Prole 2. (b) Fieldphoto of fault scarp of Prole1. (c) Field
photo of faultscarp of Prole 2. (d) The location of Prole 3. (e)Field photo of faultscarp of Prole 3. (f)The location of Prole 4.(g) Field photo of faultscarp of Prole 4. Thered arrows in
(a), (d), and (f) represent the fault trace.
113S. Wang et al. / Geomorphology 336 (2019) 107118
including rational function model, distribution and measurement of
GCPs, image matching methods and so on. The accuracy of DEM de-
termines the results of quantitative active tectonics studies. In the
common accuracy assessments of active tectonics, although some
of them had performed accuracy assessment of topographic data
generated from different methods (James and Robson, 2012;
Johnson et al., 2014;Salisbury et al., 2015;Zhou et al., 2015), there
are rare researches regarding the accuracy analysis of measuring
the height of fault scarp. Previous studies have shown that the
plane accuracy of DEM generated from Worldview-2 stereo imagery
is much higher than vertical accuracy (Toutin et al., 2012), so the
goal here is (1) to assess the elevation difference between the DEM
with GCPs and without GCPs; (2) to evaluate vertical accuracy for
measuring the height of fault scarp by comparing topographic pro-
les derived from ppGPS and DEM.
4.1. Elevation comparison of generated DEM with and without GCPs
Generating high quality DEM without GCPs has been applied in
many studies (Poli et al., 2015;Toutin et al., 2012;Zhou et al., 2015).
Poli et al. (2015) applied well-dened texture points in theoriented ste-
reo pair as GCPs and used these points for image orientation, the RMSEs
they got was around 0.3 m in plane and elevation; Toutin et al. (2012)
processed Worldview-1 and -2 stereo images without GCPs, elevation
Fig. 9. Comparison of topographic proles 14 across the fault scarp, derived from theDEM and that surveyed by ppGPS in the eld. (a), (e), (i), (m) Digital elevation model of four fault
scarps. (b) (f) (g) (n) arethe histogram graphs of elevation differences distribution. (c), (g), (k),(o) Searching for the elevation correction valueΔH. Black solidlines in (d), (h), (l),(p) are
the proles surveyed by ppGPS; Grey solid lines are proles extracted from the DEM; Grey dashed lines are proles after elevation correction.
Fig. 8. The two fault outcrops detected in the eld. Red arrows indicate the faults; black arrows indicate the fault strike. (a) Deformation evidence shows the displaced gravel layer and
unconformity between strata. (b) The wedge-shaped layers deposited in front of the scarp.
114 S. Wang et al. / Geomorphology 336 (2019) 107118
errors with 68% condence level compared to the accurate GCPs was
1020 cm; Zhou et al. (2015) extracted DEM from Pleiades stereo imag-
ery without GCPs and compared it with LiDAR data, the results show
that the vertical accuracy of DEM can reach about 0.3 m. A small number
of GCPs can improve the position accuracy of rational function model
(Aguilar et al., 2013). In this study, 12 GCPs selected from the intersec-
tion of road and river on the images were uniformly distributed and ac-
curately surveyed in the eld. We generated DEM from stereo imagery
without GCPs based on rational function model and used 12 GCPs mea-
sured in the eld (Fig. 1) as check points to evaluate the plane and ver-
tical accuracy. The root mean square error (RMSE) in Table 2 clearly
shows that the plane accuracy is better than the vertical accuracy.
Thus, it is necessary to compare the elevation difference of DEMs with
GCPs and without GCPs.
In order to discuss the elevation difference between the DEM de-
rived with and without GCPs, the point cloud data were compared in
Cloud Compare software. Using point cloud data with GCPs as a refer-
ence, we calculated the distance between them (Fig. 5a). Distribution
of elevation difference histogram graph (Fig. 5b) shows 95.7% points'
value is less than 0.8 m. The value of points without GCPs is smaller
than that with GCPs and the overall elevation difference is 1.2
0.4 m, the average difference is 0.57 m. The differences of the point
cloud in the mountain area are higher and reach 1.0 m, which might
be due to the large elevation variation, shadow effects of the stereo im-
agery etc. The average elevation differences in alluvialand village have a
lower range of 0.5 m. This part is also the main study area that the fault
scarps developed.
The goal of this research is to obtain the most accurate height of fault
scarp. Therefore, we extracted two swath proles across the fault in the
elevation difference point cloud data (Fig. 6a, e) and projected the coor-
dinates in the latitude direction (Fig. 6c, g). Compared with the overall
elevation difference of 1.20.4 m, the difference near the fault scarp
is 1.10.01 m. The average elevation difference is 0.4 m, with only
a few abnormal points. The result of vertical difference distribution
shows that the position accuracy of rational function model of
Worldview-2 satellite is high. We could also get high quality DEM
under harsh natural condition without surveying GCPs in the eld.
4.2. Comparison of topographic proles
Measuring height of fault scarp requires tting the hanging wall and
footwall according to the topographic prole. Hence, accuracy of the
surveyed topographic prole is the basis for obtaining accurate height
of a fault scarp. There are a number of alluvial fans displaced by Kumysh
fault, which are obvious on the Google Earth images (Fig. 7). Two fault
outcrops were detected in the eld (Fig. 8). We chose four sites to get
topographic proles derived from DEM and surveyed by ppGPS across
the fault scarps (Fig. 1,Fig. 7). The results are projected in the latitude
direction (Fig. 9). The overall outline and trend of proles measured
by two different methods are in good agreement, but there is a certain
elevation deviation. This might due to the coordinates of the reference
station calculated by the satellite are different from GCPs survey or
lose of ne feature due to the resolution limit of satellite imagery. So,
we rst made the elevation correction for each prole of the generated
DEM, and then calculated the RMSE of two-method proles to evaluate
the elevation difference between the DEM and ppGPS. In the eld
measurement of topographic proles using ppGPS, the point was
surveyed about every 0.25 m, while the point interval was about
0.5 m surveyed from DEM because of the spatial resolution. So, we
used the points on the ppGPS proles as reference, searched the
nearest points on the DEM proles as corresponding points (Fig. 10),
and calculated elevation difference di between the two points.
Assuming that the translation of elevation correction is ΔH,which
makes the minimum quadratic sum of elevation difference after transla-
tion [(d1ΔH
2
)+(d2ΔH
2
)+ +(dn ΔH
2
)]. After the trans-
lation, the ppGPS data is used as the reference value, and the root mean
square error (RMSE)of the whole prole iscalculated to evaluate the ac-
curacy of DEM data to portray the prole of fault scarp.
It can be seen from the prole comparison and difference histogram
in Fig. 8 that there is deviation between two groups of proles. The off-
set ranges from 2.824.47 m and the average RMSE of the two groups
is 0.29 after elevation correction. Hence, the average difference is 0.29 m
for the topographic proles across fault scarps, measured from the ex-
tracted DEM and ppGPS in the eld respectively. (See Table 3.)
4.3. Comparison of the height of fault scarps
In the study of active tectonics, measuring the offset along the fault is
essential. When measuring the height of fault scarp, it is necessary to be
perpendicular to thefault scarps and select the geomorphic surface with
less gully and erosion.The results are projected in the vertical direction
of scarps and tted to the hanging wall, footwall (h1, h2). We then used
Table 3
DEM accuracy analysis for proles 14.
Proles Prole1 Prole2 Prole3 Prole4
|di_min|(m) 1.85 2.52 0.87 1.06
|di_max|(m) 3.43 4.48 2.38 2.82
Translation ValueΔH(m) 2.76 3.24 1.42 1.37
RMSE(m) 0.27 0.33 0.29 0.26
Fig. 10. Schematic diagram of calculating elevation difference of surveyed proles between DEM and ppGPS.
115S. Wang et al. / Geomorphology 336 (2019) 107118
the average height of hanging wall and footwall to calculate the height
of fault scarps and also computed the standard deviation between the
elevation and average values as the measurement error (Hetzel et al.,
2004). Furthermore, we compared four groups of scarps' heights to an-
alyze the accuracy for measuring the height of scarp, by comparing the
heights measured from the extracted DEM and ppGPS eld survey
(Fig. 11).
The RMSE between the heights of fault scarps measured by DEM and
ppGPS is 0.25 m, and the deviation range is 0.3 to 0.17 m. It is much
smaller than the elevation difference of 2.82 to 4.47 m for the topo-
graphic proles. The measurement accuracy is signicantly increased,
which indicates that the relative error is small even though the overall
deviation is large. So, the DEM generated from stereo imagery has
high relative accuracy and can identify fault scarps higher than
0.25 m. However, in the quantitative study of active tectonics, it is not
enough to only use height difference of hanging wall and footwall as
true heightof fault scarp. The erosion of hanging wall and accumulation
of footwall caused by geomorphological evolution cannot be ignored.
We should use trench near the fault to identify the true height of fault
scarp formed by paleoearthquakes according to the stratigraphic
information.
5. Discussion
We suggest that the vertical uncertainty is mainly due to the follow-
ing three factors:
(1) Error introduced by the complex topography and geomorphol-
ogy. In the mountainous areas with steep slopes, large relief am-
plitude, vegetation (Chaplot et al., 2006;Fisher and Tate, 2006),
due to the inuence of solar elevation angle, azimuth, and sensor
angle, all rises shadows that lead to low contrast and poor
matching accuracy. The accuracy of DEM is the highest in the
plain area without vegetation in our study, followed by the resi-
dential areas and the worst in the mountain areas (Fabris and
Pesci, 2005;Fisher and Tate, 2006).
(2) Error caused by rational function model. The rational function
model uses terrain independentmethod relating ground coor-
dinates to corresponding image coordinates by a ground-to-
image polynomial generated from the physical sensor model,
the effect of RPC errors is the same as physical sensor (Aguilar
et al., 2013;Dolloff and Theiss, 2012), affected by satellite orbit
parameters, sensor parameters and ight attitude. The error of
generated DEM in the absence of GCPs mostly comes from ratio-
nal function model error. Topographic proles measured by DEM
and DGPS have deviation along the whole line, but the
distribution is not uniform. This may be largely affected by ratio-
nal function model.
(3) Data errors introduced by GPS surveying and mapping. The dis-
tribution and number of GCPs have a great impact on the
accuracy of DEM generation (Aguilar et al., 2013;Poli et al.,
2015). Since there are few intersection points of road and drain-
age with obvious features, errors will be caused when the sur-
veyed GCPs are projected onto the image and adjusted manually.
(4) Cloud noise and vegetation of stereo imagery are also non-
negligible factors that affect the quality of DEM. The existence
of cloud and mist makes it difcult to obtain clear feature infor-
mation and image matching. This problem can be mostly over-
come by three methods: 1) Using multitemporal images to
mosaic the cloud-free areas and to generate a new one (Lin
et al., 2013;Tseng et al., 2008); 2) Using the multi-spectral data
to detect and remove clouds (Wang et al., 2005); 3) Treating
cloud as noise to remove (Feng et al., 2004). In addition, point
cloud data obtained from stereo imagery contain information of
both ground points and vegetation. Several ltering algorithms
have been developed for this drawback (Deng and Shi, 2013;
Hu et al., 2014;Sithole and Vosselman, 2004), which have dispa-
rate performance in different landscape and environment. We
should choose appropriate cloud denoising and vegetation elim-
ination method according to our study area.
In addition to the above factors, spatial resolution of satellite images,
band characteristics and the method of interpolation could also affect
DEM-generation accuracy to some extent.
6. Conclusion
This paper mainly introduces the basic principle and processing ow
of DEM generation using Worldview-2 stereo imagery by extracting
0.5 m resolution DEM of the southern margin of Kumysh Basin in the
eastern Tian Shan. Three main ndings can be summarized as follows:
(1) Using GCPsas check points to evaluate accuracy of the DEM with-
out GCPs, the vertical accuracy is ~1.82 m. The elevation differ-
ence between the DEM with and without GCPs is 1.20.4 m
while the elevation difference is 1.10.01 m for the point
cloud swath proles across the fault scarps;
(2) Under the condition of 12 GCPs, the morphological difference be-
tween the two methods is ~0.29 m, as obtained by comparing the
topographic proles across fault scarps derived from the gener-
ated DEM and ppGPS eld survey;
(3) In the research of active tectonic, by analyzing the height of the
fault scarps using DEM and ppGPS, we got the accuracy of scarp
height measured by DEM is 0.25 m.
The results show that Worldview-2 stereo imagery is feasible to es-
tablish accurate DEM with very few GCPs. In the absence of GCPs, the
Fig. 11. Comparison of the height of fault scarps measured from the DEM and ppGPS survey in the eld.
116 S. Wang et al. / Geomorphology 336 (2019) 107118
vertical accuracy of DEM is higher than 1.82 m. The topographic proles
can be accurately depicted under a small number of GCPs and the mea-
surement accuracy can reach 0.29 m. With this method, we can obtain
the ne geometric structure of faults quickly and accurately. It also pro-
vides us with reference to choose trench-excavation site and
chronological-sample collection site. Generating DEM from stereo im-
agery costs less than airborne LiDAR and has a wide ight range of cov-
erage compared with UAV, which has a broad application prospect in
the study of active tectonic.
There are still some deciencies in this paper: 1) The study area is lo-
cated in the piedmont alluvial fans. There is a certain error in GCPs sur-
vey because of the lack of landmark features; 2) Mountain shadow of
the stereo imagery we purchased is severe, which would affect the
DEM accuracy. This error may be carried over to our follow-up analysis.
Fortunately, the faults we concerning with are located on the alluvial
fans uncovered by shadows rather than on the mountain, but it is nec-
essary to use mountain part to carry out analysis of tectonic-
geomorphology, which will affect the results; 3) Due to the limitation
of Worldview-2 stereo imagery resolution, this method will be ineffec-
tive for small fault scarps less than 0.25 m.
Acknowledgements
This research was funded by National Nonprot Fundamental
Research Grant of China (IGCEA1607IGCEA1803), and National Natu-
ral Science Foundation of China (41472201, 41761144071). We thank
Ming Ai dueto all the heights of fault scarps aremeasured with the help
of him. We appreciate Jiahong Luo for his help in writing Matlab code.
The authors would also like to thank the editor and reviewers for their
useful comments.
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This paper presents detailed elevation and volume analysis of 16 individual glaciers, grouped at four locations, spread across the Antarctic Peninsula (AP). The study makes use of newly available WorldView-2 satellite stereo imagery to exploit the previously untapped value of archival stereo aerial photography. High resolution photogrammetric digital elevation models (DEMs) are derived to determine three-dimensional glacier change over an unprecedented time span of six decades with an unparalleled mean areal coverage of 82 % per glacier. The use of an in-house robust surface matching algorithm ensured rigorous alignment of the DEMs to overcome inherent problems associated with processing archival photography, most notably the identification and correction of scale error in some datasets. The analysis provides insight into one of the most challenging and data scarce areas on the planet by expanding the spatial extent north of the AP to include previously unstudied glaciers located in the South Shetland Islands. 81 % of glaciers studied showed considerable loss of volume over the period of record. The mean annual mass loss for all glaciers yielded 0.24 ±0.08 m.w.e. per year, with a maximum mass loss of up to 62 m.w.e. and frontal retreat exceeding 2.2 km for Stadium Glacier, located furthest north on Elephant Island. Observed volumetric loss was broadly, though not always, correlated with frontal retreat. The combined mass balance of all 16 glaciers yielded -1.862 ± 0.006 Gt, which corresponds to -0.005 26 mm sea level equivalent (SLE) over the 57 year observation period. The full text of the article can be access at the following link: http://eprints.glos.ac.uk/5172/
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Reconstruction of the along-fault slip distribution provides an insight into the long-term rupture patterns of a fault, thereby enabling more accurate assessment of its future behavior. The increasing wealth of high-resolution topographic data, such as LiDAR and photogrammetric DEMs, allows us to better constrain the slip distribution, thus greatly improving our understanding of fault behavior. The South Heli Shan Fault is a major active fault on the northeastern margin of the Tibetan Plateau. In this study, we built a 2-m resolution DEM of the South Heli Shan Fault based on high-resolution GeoEye-1 stereo satellite imagery, and then measured 302 vertical displacements along the fault, which increased the measurement density of previous field surveys by a factor of nearly 5. The cumulative displacements show an asymmetric distribution along the fault, comprising three major segments. An increasing trend from west to east indicates that the fault has likely propagated westwards over its lifetime. The topographic relief of Heli Shan shows an asymmetry similar to the measured cumulative slip distribution, suggesting that the uplift of Heli Shan may result mainly from the long-term activity of the South Heli Shan Fault. Furthermore, the cumulative displacements divide into discrete clusters along the fault, indicating that the fault has ruptured in several large earthquakes. By constraining the slip-length distribution of each rupture, we found that the events do not support a characteristic recurrence model for the fault.
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We adapted the automated, open source NASA Ames Stereo Pipeline (ASP) to generate digital elevation models (DEMs) and orthoimages from very-high-resolution (VHR) commercial imagery of the Earth. These modifications include support for rigorous and rational polynomial coefficient (RPC) sensor models, sensor geometry correction, bundle adjustment, point cloud co-registration, and significant improvements to the ASP code base. We outline a processing workflow for ∼0.5 m ground sample distance (GSD) DigitalGlobe WorldView-1 and WorldView-2 along-track stereo image data, with an overview of ASP capabilities, an evaluation of ASP correlator options, benchmark test results, and two case studies of DEM accuracy. Output DEM products are posted at ∼2 m with direct geolocation accuracy of <5.0 m CE90/LE90. An automated iterative closest-point (ICP) co-registration tool reduces absolute vertical and horizontal error to <0.5 m where appropriate ground-control data are available, with observed standard deviation of ∼0.1–0.5 m for overlapping, co-registered DEMs (n = 14, 17). While ASP can be used to process individual stereo pairs on a local workstation, the methods presented here were developed for large-scale batch processing in a high-performance computing environment. We are leveraging these resources to produce dense time series and regional mosaics for the Earth’s polar regions.
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High-resolution surface topography is valuable for studying coseismic fault zone deformation and fault geometry. It enables us to measure three-dimensional surface displacements in earthquakes, as shown in recent studies that used light detection and ranging (lidar) to determine coseismic motion. However, the applicability of lidar is limited by its relatively high cost and low availability. In this study, we use the 2010 El Mayor-Cucapah earthquake to demonstrate the capability of Pleiades stereo imagery to measure coseismic vertical ground displacement. We acquired post-earthquake Pleiades tristereo imagery from backward, near-nadir, and forward orientations for a 45 km × 7 km portion of the epicentral area. One meter resolution digital elevation models (DEMs) were produced with the four different combinations of incidence angles and compared to the post-earthquake lidar DEM. Elevations from tristereo have slightly (∼15%) smaller uncertainties than bistereo as the tristereo DEM incorporates more observations. Elevation differences between the Pleiades and post-earthquake lidar DEMs show that the vertical accuracy of the Pleiades DEMs is ∼0.3 m. By differencing the Pleiades DEM and the pre-earthquake, 5 m resolution lidar DEM, we mapped meter and submeter offsets along the faults obtaining results comparable to a previous study that differenced the two lidar DEMs. This is the first case study of assessing very high resolution (VHR) satellite stereo imagery to determine submeter vertical ground displacement in an earthquake. By extension, we expect it to be possible to measure submeter vertical offsets occurring in earthquakes using pre-earthquake and post-earthquake VHR stereo imagery. Key Points: First case study of assessing VHR stereo imagery to determine height changes in an earthquake Elevations from tristereo have slightly (∼15%) smaller uncertainties than bistereo Coseismic height changes mapped using the Pleiades DEM are comparable to differential lidar
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How strain is distributed and partitioned on individual faults and folds on the margins of intermontane basins remains poorly understood. The Haermodun (Ha) anticline, located along the northern margin of the Yanqi Basin on the southeastern flank of the Tian Shan, preserves flights of passively deformed alluvial terraces. These terraces cross the active anticline and can be used to constrain local crustal shortening and uplift rates. Geologic and geomorphic mapping, in conjunction with high-resolution dGPS topographic surveys, reveal that the terrace surfaces are perpendicular to the fold's strike, and display increased rotation with age, implying that the anticline has grown by progressive limb rotation. We combine 10Be terrestrial cosmogenic nuclide (TCN) depth profile dating and optically stimulated luminescence (OSL) dating to develop a new chronology for the terraces along the Huangshui He since 550 ka. Our in situ 10Be dating of fluvial gravels capping strath terraces suggests a relationship between the formation and abandonment of the terraces and glacial climate cycles since the middle-late Pleistocene. These data indicate that the formation of the four terraces occurred at ~550, ~430, ~350, and~60 ka. We suggest that episodes of aggradation were facilitated by high sediment supply during glacial periods, followed by subsequent incision that led to abandonment of these terraces during deglaciation. Combining uplift and shortening distance with ages, we found the vertical uplift gradually decreased from 0.43 to 0.11 mm/a, whereas the shortening rate was constant at ~0.3 mm/a since the anticline began to grow. The shortening rates of the Ha anticline from geomorphology agree with current GPS measurements, and highlight the importance of determining slip rates for individual faults in order to resolve patterns of strain distribution across intermontane belts. ©, 2015, Editorial Office of Seismology and Geology. All right reserved.
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The terranes composing the basement of the Tian Shan were originally sutured together during two collisions in Late Devonian-Early Carboniferous and Late Carboniferous- Early Permian time. Since then, the range has repeatedly been uplifted and structurally reactivated, apparently as a result of the collision of island arcs and continental blocks with the southern margin of Asia far to the south of the range. Evidence for these deformational episodes is recorded in the sedimentary histories of the Junggar and Tarim foreland basins to the north and south of the range and by the cooling and exhumation histories of rocks in the interior of the range. Reconnaissance apatite fission-track cooling ages from the Chinese part of the range cluster in three general time periods, latest Paleozoic, late Mesozoic, and late Cenozoic. Latest Paleozoic cooling is recorded at Aksu (east of Kalpin) on the southern flank of the range, at two areas in the central Tian Shan block along the Dushanzi-Kuqa Highway, and by detrital apatites at Kuqa that retain fission-track ages of their sediment source areas. Available 40Ar/39Ar cooling ages from the range also cluster within this time interval, with very few younger ages. These cooling ages may record exhumation and deformation caused by the second basement suturing collision between the Tarim-central Tian Shan composite block and the north Tian Shan. Apatite data from three areas record late Mesozoic cooling, at Kuqa on the southern flank of the range and at two areas in the central Tian Shan block. Sedimentary sections in the Junggar and Tarim foreland basins contain major unconformities, thick intervals of alluvial conglomerate, and increased subsidence rates between about 140 and 100 Ma. These data may reflect deformation and uplift induced by collision of the Lhasa block with the southern margin of Asia in latest Jurassic-Early Cretaceous time. Large Jurassic intermontane basins are preserved within the interior of the Tian Shan and in conjunction with the fission-track data suggest that the late Mesozoic Tian Shan was subdivided into a complex of generally east-west-trending, structurally controlled subranges and basins. Apatite data from five areas record major late Cenozoic cooling, at sites in the basin-vergent thrust belts on the northern and southern margins of the range, and along the north Tian Shan fault system in the interior of the range. The thrust belts and fault system have been sites of active shortening and exhumation since at least ca. 25 Ma, apparently induced by the collision of the Indian subcontinent with the southern margin of Asia. On the basis of regional relations, the north Tian Shan fault system is likely an important active right-lateral transpressional structure that has reactivated the north Tian Shan-central Tian Shan suture zone. In general, most of the Chinese Tian Shan appears to have been exhumed only limited amounts through Mesozoic and Cenozoic time. Within our sampling areas, only limited areas along the north Tian Shan fault zone and in parts of the rangemargin thrust belts were exhumed more than &3 km during the Cenozoic India-Asia collision. Modern intermontane basins are present within the Tian Shan and help divide it into a number of subranges, much like the late Mesozoic Tian Shan. This modern physiography likely reflects in part reactivation of pre-Cenozoic structural trends.