1 reconstruction of shallow coseismic slip following the...
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Reconstruction of shallow coseismic slip following the 2015 Illapel earthquake 1 2In review at Earth and Planetary Science Letters, May 28, 2016. 3 4Amy Williamsona,*, Andrew Newmana 5 6a School of Earth and Atmospheric Sciences, Georgia Institute of Technology, 311 Ferst 7Drive, Atlanta, GA, 30332, United States 8 9* Corresponding author. E-mail address: [email protected] (A. Williamson) 10
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Abstract 13
On 16 September, 2015, a moment magnitude 8.3 earthquake struck off the coast of 14
Central Chile, generating a large tsunami. Through a trans-coastal geodetic study, including 15
inferred seafloor vertical displacement determined from open-ocean pressure gauges 16
recording tsunami excitation, and sub-areal deformation observed through Interferometric 17
Synthetic Aperture Radar (InSAR) from the Sentinel-1 satellite, we identify that earthquake-18
generated slip dominantly occurred offshore and very near the trench. This tsunamigenic 19
near-trench rupture likely initiated about 80 s after the initial nucleation and is responsible for 20
open ocean tsunami waves up to 10 cm in amplitude. Tide-gauges across Chile and Peru 21
recorded sizable tsunami waves up to 4.7 m in height, with the most distal observation of 22
over 40 cm in the Kuril Islands across the Pacific Ocean. The prevalence of large and 23
shallow thrust along the subduction megathrust raises the question of the likelihood of future 24
such events along central Chile and its implications for future hazardous tsunamigenic 25
earthquakes. 26
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Keywords 28
Chile, earthquake, Illapel, subduction zone, joint inversion 29
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1. Introduction 31
The Atacama trench is globally one of the most seismically active regions with both a 32
contemporary and geologic record of generating great (M > 8) earthquakes with a short 33
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recurrence interval. This propensity for large events is assisted by the region’s rapid plate 34
motion. In the vicinity of central Chile, the Nazca plate subducts beneath the South American 35
plate with a convergence rate of 74 mm/yr (DeMets et al., 2010)(Figure 1). This has led the 36
Atacama, also called the Peru-Chile trench, to be the focus of many studies on tectonic strain 37
accumulation, interseismic coupling, and earthquake excitation (Vigny et al., 2009; Moreno 38
et al., 2010; Moreno et al., 2011). 39
Many of the large earthquakes generated on this fault system also cause large tsunami 40
waves, with intensities that loosely correlate with the size and down-dip location of the 41
mainshock rupture. The largest-ever instrumentally recorded earthquake occurred near 42
Valdivia, Chile in 1960. This moment magnitude (MW) 9.5 event generated a large and 43
devastating transoceanic tsunami. Eyewitness observations near the source region suggest 10 44
to 15 m waves along the coast (NGDC, 2016). On a regional scale, tide gauge recordings 45
near the city of Concepción topped out with zero-to-crest amplitudes of over 2.5 m, and tide 46
gauges in northern Chile and Peru (2,000 to 3,000 km away) recorded waves between 0.5 and 47
1 m in height (NGDC, 2016). 48
More recently, the 2010 MW 8.8 Maule earthquake ruptured a patch of the megathrust 49
just to the north of the 1960 Valdivia earthquake. However, the size of tsunami that was 50
generated was modest in comparison to its mainshock. In the near field, tide gauges recorded 51
waves with amplitudes around 1 m, with the largest wave = 1.3 m occurring in a bay near the 52
city of Coquimbo. Far field recordings in Peru were less than 0.5 m. Nevertheless, the 53
earthquake and tsunami created over 30 billion dollars in damage and resulted in over 500 54
causalities in Chile (USGS report; Fritz et al., 2011). In 2014, the MW 8.1 Iquique earthquake 55
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in northern Chile, while smaller, also produced an observable tsunami (An et al., 2014; 56
Gusman et al., 2015). 57
The latest tsunamigenic addition to the Atacama catalog is the 16 September 2015 58
MW 8.3 Illapel earthquake. This event nucleated offshore from Coquimbo Province 59
(approximately 31.57° S and 71.67° W) at approximately 22:54:32 UTC (NEIC Reference). 60
While this event was modest in size compared to other contemporary tsunamigenic 61
earthquakes near Chile, it produced a locally large tsunami (up to 4.7 m near Coquimbo as 62
measured by a local tide gauge). The tsunami became transoceanic, with tide gauges 63
recordings throughout the Pacific basin, including Oahu, Hawaii (0.23 m), Kuril Islands, 64
Russia (0.44 m), and Aburatsu, Japan (0.22 m). 65
Despite the lower magnitude, the Illapel event produced a transoceanic tsunami that is 66
more in line with a much larger earthquake, like the MW 8.8 Maule event which also 67
produced sub-meter tide gauge signals in Hawaii. The Illapel earthquake is not unique in this 68
disparity. The 1996 Chimbote, Peru earthquake, while only a MW 7.8, produced meter-level 69
waves locally around Peru and Northern Chile, and waves up to 0.3 m near Easter Island, 70
approximately 3800 km away. The disproportionately large tsunami generated by this event 71
is partially a function of its rupture along the shallow part of the megathrust (Heinrich et al., 72
1998). Its source location and its deficiency in radiating high frequency energy led this event 73
to be categorized as a tsunami earthquake by Newman and Okal (1998), a special subclass of 74
tsunamigenic earthquakes characterized by their ability to produce much larger waves than 75
expected given their magnitude (Kanamori, 1972). 76
Tsunami earthquakes are frequently both deficient in radiating seismic energy and 77
excessive in duration, charactering slow rupture propagation (Kanamori, 1972). They also 78
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appear to exclusively rupture the shallow megathrust environment as was inferred from tide-79
gauge inversions of the MW 7.6 1992 Nicaragua earthquake (e.g. Satake 1994), and from 80
very-local coastal geodetic changes due to the MW 7.1 2010 Mentawai earthquake (Newman 81
et al., 2011). 82
To characterize the 2015 Illapel earthquake, we use both on-land Line-Of-Sight 83
(LOS) Interferometric Synthetic Aperture Radar (InSAR) observations and derived seafloor 84
vertical displacements determined from real-time open-ocean tsunami derived fault solutions. 85
The combination of the two datasets, which span the shoreline, allows for maximum 86
resolution of the earthquake slip environment across the subduction megathrust. As we detail 87
below, through a joint inversion of both data types, we find that the maximum coseismic slip 88
occurred along the shallowest portion of the megathrust, as shown in Figure 1. This puts the 89
Illapel event in a category similar to many past tsunami earthquakes, that along with the 1996 90
Chimbote, Peru earthquake, indicates that the Peru-Chile trench is very capable of generating 91
shallow and particularly tsunamigenic earthquakes. 92
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2. Methodology 94
2.1 Data 95
This study incorporates real time fault solutions provided through the Pacific Marine 96
Environmental Lab (PMEL) and Tang et al. (2016), as well as InSAR derived ground-surface 97
displacements from the European Space Agency’s Sentinel-1 satellite to solve for the 98
magnitude and spatial extent of coseismic slip along the Chilean megathrust interface from 99
the Illapal earthquake. We validate our slip geometry by comparing a forward projected 100
tsunami model with observed tsunami waveforms at three regionally located Deep Ocean 101
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Assessment and Reporting of Tsunami (henceforth DART) pressure gauges, and through 102
comparisons of predicted and observed ground deformation along the Chilean coast. 103
We use the LOS displacement field derived from a pair of descending track scenes (24 104
August and 17 September 2015) made by the Sentinel-1 satellite, which was processed by the 105
European Space Agency (Copernicus Service information [2015]). The resultant image 106
(Figure 2) shows up to 150 cm of ground deformation in the LOS direction (looking 75° W 107
of N at approximately 41° off nadir near the maximum deformation, and is the orientation 108
used for this study). Because the data density and interdependence of pixels is extremely 109
high (on the order of 107 pixels per image), it is necessary to down-sample, to make it 110
manageable for computational inversions. To do so, we use a two-dimensional Quadtree 111
decomposition, with the goal of retaining sufficient information to understand the source, 112
while making the total data count sufficiently small that inversion methodologies are 113
tractable. In this study, we require that the data be split whenever a box had a variance in 114
LOS displacement greater than 40% of the total. We assign the location of each of the 115
resulting data points to the ‘center of mass’ of coherent pixels. Because the second pass 116
follows one day after the event, any postseismic signal is likely to remain small. 117
Furthermore, because most observations of early afterslip occur primarily up-dip of the main 118
rupture along subduction zones (e.g. Hsu et al., 2006; Malservisi et al., 2015), we suspect the 119
land-based data to be more representative of coseismic rupture. 120
We incorporate the rapidly determined sea-surface deformation calculated from the 121
full wave tsunami source estimated by Tang et al. (2016) and using unit sources developed 122
by Gica et al. (2008). The Tang et al. (2016) full wave estimation of the tsunami inverts 123
open-ocean signals from nearby DART gauges assuming the linear superposition of 124
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regionally located, pre-computed rectangular slip patches, 50 km wide by 100 km long, with 125
fault geometries coarsely representing the subduction zone in the region. Their published 126
solution uses five patches with slip coefficients ranging from 0.8 to 7.3 m of pure thrust 127
(Figure 3). Both the Tang et al. (2016) and this study incorporate the Method of Splitting 128
Tsunami (MOST) model to compare observed and modeled slip with DART gauges (Titov 129
and Synolakis, 1998; Titov and Goznales, 1997). The MOST model is a finite-difference 130
numerical code based on the long-wave approximation for tsunami waves in deep water. 131
When constrained to the use of only land-based instruments such as GPS and InSAR, 132
the shallow subduction zone region is generally too far offshore to be resolvable using 133
distributed-slip inversions. While seafloor geodetic instruments are feasible, they are often 134
cost prohibitive, causing many communities forgo their use (Newman, 2011). This leads to 135
the possibility of underestimating slip in this highly hazardous, but in these cases poorly 136
resolved, zone. By supplementing this dataset with ocean-based observations, like tide gauge 137
or pressure gauge mareograms, spatial resolvability of the offshore region increases 138
substantially, allowing for better control on the problem (see Model Resolution section, 139
below). 140
2.2 Model Geometry 141
The two-dimensional curvi-planar fault geometry used here has a constant strike of 142
N5°E, with dip that increases with depth, approximating the Slab 1.0 profile (Figure 4) 143
(Hayes et al., 2012), which exhibits almost no along-strike variability across the coseismic 144
region area in this study. The modeled fault plane is discretized into a 450 x 200 km surface, 145
consisting of a regular 18x8 grid, with individual patches about 25 km x 25 km. 146
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Green functions are calculated for both the vertical seafloor and InSAR LOS 147
displacements through an analytic solution to the elastodynamic equations for rectangular 148
dislocations in an elastic half space (Okada, 1985). The code uses here, GTdef Chen et al. 149
(2009), uses a bounded and weighted linear least squares algorithm for slip inversions. We 150
regularize our solution using a two-dimensional Laplacian smoothing factor, which requires 151
an interdependence between adjacent slip patches, which trade-off with misfit (Harris and 152
Segall, 1987). Here, the misfit is determined as the root mean square of the weighted-residual 153
sum of squares (Jónsson et al., 2002), while the roughness term is the degree of two-154
dimensional spatial smoothing. The preferred model is then determined by subjectively 155
choosing the best trade-off between the two parameters. 156
2.3 Model Resolution 157
We approximate the spatial resolvability of our model using a checkerboard test, 158
consisting of 50 km by 50 km blocks with alternating predefined uniform slip magnitudes 159
between 0 and 1 meter. Using these patches as input, we predict deformation at each data 160
point (InSAR, Seafloor, and both) as determined by our Quadtree decomposition. We 161
subsequently invert these synthetic data with our observed data variance, and compare our 162
inverted with our initial models (Figure 5). In areas where the checkerboard is retained, we 163
have high resolvability, which includes the area of most predicted slip (Figure 1). However, 164
we lose resolution towards the edges of our spatial domain, where our Quadtree methodology 165
severely reduces sampling, due to lack of signal change. 166
If only tsunami data are used, resolution is unsurprisingly limited to the offshore 167
environment, while using InSAR data alone allows for resolvability primarily under land, 168
extending modestly offshore (approximately 50 km), but not to the trench. The size of 169
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onshore resolvable slip patches also increases with the depth of the underlying fault, 170
somewhat smoothing subduction megathrust models below land. 171
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3. Results 173
Our preferred model result for the spatial extent of slip along the megathrust (Figure 174
1), has a maximum of 15 m of thrust near to the trench, and averaging just over 2 m across 175
the model domain, corresponding to a seismic moment for the thrust component of 5.3x1021 176
Nm (Mw 8.38) assuming rigidity of 30 GPa. Slip extends from the coastal interior up-dip 177
towards the shallow portion of the fault, near the trench. Because seafloor model inputs are 178
vertical, and the orientation of the satellite track is only about 15° off a longitudinal path, the 179
data have little information along-strike for our model geometry. As such, though along-180
strike motion is inverted, we limit our discussion to the thrust-only component. 181
Over- and under- smoothed results are included in Figure 6 as well as the roughness 182
versus misfit tradeoff curve for modeled smoothness parameters, κ. While some features on 183
the edges of our model change with the changing κ, the overall features in our resolvable 184
zone do not change significantly past the degree imposed by smoothing. 185
We validate our results through a comparison with both the original unwrapped 186
Sentinel-1 interferogram and observed waveforms at DART gauges. For the InSAR data we 187
find that we are able to recreate the general shape and overall magnitude of static offset seen 188
in the observed image (Figure 7), though the model underpredicts surface deformation 189
immediately to the south of the event, and modestly overpredicts deformation to the north 190
along the coast, where model resolution is low. 191
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For the forward tsunami model, we use the ETOPO1 global relief model with a 192
bathymetric data density of 1 arc minute. In order to satisfy the Courant-Friedrichs-Lewy 193
(CFL) condition for the tsunami wave propagation model, a computational time step of six 194
seconds is imposed. Additionally, we impose a reflective coastline as a spatial boundary 195
condition, however we do not quantify inundation levels or wave amplitudes outside of the 196
deep-ocean because of the limited resolution of ETOPO1 data. Observations from DART 197
gauges are processed with a high-pass butterworth filter (wave period> 2 hours) to removed 198
tidal signals. We compare the results from our forward model with the waveforms at the 199
three nearest and regionally located DART gauges (Figure 8; location shown in Figure 1). 200
We also include the rapidly derived results from the Tang et al. (2016) study as a 201
comparison. Our model is in good agreement with the observed waveforms, as it accurately 202
reproduces both the initial positive and negative waves at DART gauge 32402, as well as 203
most of the following wave train. Additionally, our computed wave heights for the initial 204
positive peak are in general agreement with the observed data. Model tsunami time series are 205
shifted forward in time by 140 seconds, similar to the time delay in Heidarzadeh et al. 206
(2015), while results from Tang et al. (2016) are shifted forward 72 seconds. We explore a 207
possible reason for this time shift below. 208
4. Discussion 209
The large thrust along the shallow megathrust environment is responsible for the 210
majority of tsunami excitation. This is likely a leading role in why the Illapel earthquake 211
generated a tsunami that is disproportionally large when compared to events like the larger 212
MW 8.8 2010 Maule earthquake, and the slightly smaller MW 8.1 2014 Iquique earthquake 213
(Figure 1). There are a number of reasons for this. Firstly, and quite obviously, larger slip 214
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causes greater disturbances of the entire environment. When this slip occurs very near the 215
seafloor, there is very little spatial smoothing of deformation from the very thin over-riding 216
plate, as such the displacement field will be larger and more focused than for deeper slips of 217
equivalent magnitude. This larger slip may be aided by both the lack of a substantial 218
overriding elastic layer, and by the absence of a bounded, and slip limited, fault tip at the 219
trench. Lastly, slip-generated vertical motions near the trench occur, almost by requirement, 220
in the deepest parts of the oceans. As such they affect the largest column of ocean, and 221
initiate propagation at higher speeds (tsunami speed, 𝑉" = 𝑔ℎ, where g and h are gravity 222
and ocean depth, respectively). The results become devastating as initial waves slow near the 223
coastlines, and increase in amplitude due to conservation of momentum. 224
Earthquake rupture speeds normally are around 3km/s for most subduction zone 225
earthquakes (e.g. Bilek and Lay, 1999). However, in the case of slow, tsunami earthquakes, 226
rupture can be substantially reduced, down to as little as 1 km/s, greatly extending the 227
duration of rupture, and substantially diminishing the propagated energy, as was the case in 228
the 1996 Chimbote, Peru earthquake (Figure 1) (Kanamori, 1972; Newman and Okal, 1998). 229
The slowed rupture is attributed to slip in the shallowest portion of the interface near the 230
trench (e.g. Bilek and Lay, 1999; Polet and Kanamori, 2000). Based on teleseismic energy 231
back-projections, Yin et al. (2016) identified a substantial and slow delayed rupture 232
component to the 2015 Illapel earthquake, extending between 80 and 130 s from the initial 233
rupture, with the patch occurring up-dip of the initial nucleation, and very near the trench. 234
Using a teleseismic inversion of the spectral contributions from the Illapel earthquake, Lee et 235
al. (2016) similarly found a two-stage rupture process, but with moderately longer durations, 236
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the first lasting 100 s, and the second not terminating until about 250 s after the rupture 237
initiation. 238
Examination of the real-time radiated energy growth, automatically ran at Georgia 239
Tech using RTerg (Convers and Newman, 2011), also shows that this earthquake has some 240
features of a complex and possibly slow rupture that are discernable within the high-241
frequency cumulative time series (Figure 9). While the automated algorithm estimated 242
rupture duration, TR, at 135 s using the cross-over between the rapid initial growth and the 243
later slow-growth of high-frequency energy (between 0.5 and 2 Hz), careful examination 244
shows two near linear trends in the data, one terminating near 83s, and the second at about 245
146s. These windows correspond well with the two periods found by Yin et al (2016). The 246
second stage grows more slowly—such slow rupture is a character also seen in slow tsunami 247
earthquakes using this algorithm (Convers and Newman, 2011; Newman et al., 2011). 248
Finally, the total high-frequency energy is deficient at about 3.0e15 J (corresponding to 249
energy magnitude, Me-hf =7.8), a feature similarly seen as deficient for tsunami earthquakes in 250
Newman and Okal (1998). The corroborating evidence from each the back-projections of 251
Yin et al. (2016), the spectral analysis of Lee et al. (2016) and the earthquake energy 252
determinations following Convers and Newman (2011) strongly support the likelihood of a 253
slow and tsunamigenic rupture in the near-trench region. Finally, the delayed rupture of the 254
tsunamigenic near-trench region, can explain most of the time-shift necessary to best 255
describe the tsunami waveforms recorded at nearby DART stations (Figure 8). 256
This mode of shallow-slip and tsunamigenesis is in contrast to other recent 257
megathrust events along the Peru-Chile trench. After an extended foreshock sequence, the 258
2014 MW 8.1 Iquique earthquake ruptured both further down dip and under a shallower 259
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column of water, with between 4 to 7 m of thrust occurring between 25-35 km depth (Schurr 260
et al., 2014; Gusman et al., 2015). The location of early aftershocks also indicate little 261
activity near the trench (Hayes et al., 2014). The lower amplitude slip and deeper rupture led 262
to less tsunami excitation, as observed at local and regional tide gauges along the South 263
American Pacific coast (Figure 1). 264
Slip inversions for the 2010 MW 8.8 Maule earthquake, including Lorito et al. (2011) 265
and Yue et al. (2014), found peak slips of between 16 to 20 m between 15 and 20 km depth. 266
The models show two broad patches of substantial (>5m slip) extending along-strike for 267
about 450 km, and up-dip from the coastline about 80 km toward the trench, leaving little 268
modeled slip in the last 60 to 90 km closest to the trench. Though the rupture extent of the 269
Maule earthquake was much greater than the most recent Illapel event, the tsunami heights 270
were comparable, and actually smaller in most locales (figure 1). 271
Thus, though the Maule earthquake was more than six times larger than the Illapel 272
event (as measured by seismic moment), it is clear that size alone is not the deciding factor in 273
tsunami generation, but where the slip occurs in relation to the trench. Such near-trench slip 274
is also likely why both the much smaller MW 7.5 1996 Chimbote tsunami earthquake 275
(Newman and Okal, 1998; Bourgeois et al., 1999) and the much larger MW 9.5 1960 Valdivia 276
earthquake were so efficient at generating destructive tsunami waves (Plafker and Savage, 277
1970). 278
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5. Conclusion 279
We conduct trans-coastal joint inversion of regional surface deformation to solve for 280
coseismic slip along the subduction megathrust using tsunami-derived vertical seafloor 281
deformation and Sentinal-1 InSAR data following the 2015 Illapel earthquake. By 282
supplementing the traditional land-based geodetic slip inversion with a tsunami derived 283
dataset, key vertical deformation information about the region between the trench and the 284
coast can be incorporated, substantially increasing the resolution domain for megathrust 285
events. Our preferred result has a large concentration of slip rupturing the shallowest portion 286
of the megathrust near the trench. Our model is in very good agreement with tsunami time 287
series recorded at 3 nearby DART gauges. A necessary time shift is possibly due to delayed 288
and slow rupture of the shallow portion of the fault. The shallow rupture of this event and its 289
large tsunami, along with other recent and notable tsunamigenic earthquakes in the region 290
highlight that the Peru-Chile trench has significant tsunamigenic potential from earthquakes 291
with substantial near-trench rupture. This includes giant earthquakes like Valdivia in 1960, 292
slow rupturing tsunami earthquakes like Chimbote in 1996, and hybrid events like Illapel 293
2015. 294
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6. Acknowledgements 296
This research was supported through State Funds through Georgia Tech to AVN. Figures 297
were generated using Generic Mapping Tools from Wessel et al. [2013]. We appreciate the 298
openly available and processed Sentinal-1 InSAR data and open ocean tsunami waveform 299
datasets that were made accessible by the European Space Agency and the US National 300
Oceanic and Atmospheric Administration, respectively. We are extremely grateful of Y. Wei 301
and V. Titov’s support of ALW’s training in use of the MOST tsunami modeling software. 302
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434 435
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436Figure 1. Regional map of past tsunamigenic earthquakes and their generated tsunamis. The 437epicenter of the 1960 and centroid location for later events (Esktröm et al., 2012) with the 438approximate rupture area are shown by colored stars and transparent polygons beneath 439(Bourgeouis et al., 1999; Lorito et al., 2011; Hayes et al., 2014). For each event, the regional 440tsunami wave height measured by local tide gauges and deep-water pressure sensors (green 441triangles) are shown as columnar bars (1960 is augmented by eyewitness accounts (gray tops, 442and are all divided by 4 to stay on scale) (NGDC, 2016). Observations at Juan Fernandez 443Island (~34°S) are offset for clarity. The Nazca plate motion relative to a stable South 444American plate is also shown (black arrows) (DeMets et al., 2010). (Inset) Surface projection 445of our preferred model from a tsunami-InSAR joint inversion (location shown as black box 446with model in main map). Gray lines indicate depth contours derived from Slab 1.0 (Hayes, 4472012). 448
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449Figure 2. Regional InSAR derived displacements in the direction of satellite line-of-sight 450with Quadtree discretization (white boxes). 33 points, one per box, mark the average value 451within each box, and its location is determined as the ‘center of mass’ of the coherent data. 452The size of each point corresponds to the degree of error, calculated as the overall variance 453within each box. These points, their shown magnitudes and weights define the InSAR data 454used for model inversions. 455
−72˚ −71˚ −70˚
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−25 0 25 50 75 100 125 150Observed LOS Displacement [cm]
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456Figure 3. (a) Rapidly determined fault plane solution using near-field tsunami waveforms 457derived by Tang et al. (2016). The block dimensions and geometry were described in Gica et 458al (2008). (b) Vertical seafloor deformation predicted using the Tang et al. unit sources, 459following Okada (1985). (c) Quadtree decomposition of vertical seafloor deformation, 460yielding 45 boxes total, limited to the region off-shore of central Chile. 461 462
463
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Figure 4. (a) Surface projection of fault discretization. Each patch (outlined in red) is 25 km2 464in area. Gray north-south trending lines indicate the approximate depth of the plate interface 465as derived in Slab 1.0 (Hayes et al., 2012). (b) Trench-normal cross-section showing our 466model geometry (red line), and three profiles representing the 25th, 50th, and 75th percentile of 467the fault length (gray lines). The zero datum, and location of the approximate location of the 468trench (as defined by the southern extent of our model geometry) are shown as vertical and 469horizontal solid black lines, respectively. 470
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471Figure 5. “Checkerboard” resolution test showing: (a) the initial synthetic slip model; (b) 472results of a joint inversion of both tsunami and InSAR datasets, with the area of highest 473resolvability (red dashed box). We also show results for (c) a tsunami-only test, and (d) an 474InSAR-only test, highlighting the spatial sensitivity of the individual data. 475
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476Figure 6. Model results for a number of smoothness-based dampening choices, where higher 477κ values correspond to increased dampening (and decreased roughness). The three shown 478solutions (a) κ = 4,000, (b) κ = 10,000, and (c) κ = 16,000, represent an under-479damped, our preferred, and over-damped models, respectively. (d) The trade-off between 480model roughness, and model misfit is shown for our example cases, as well as other tested 481models. Our preferred solution represents a subjective choice,that attempts to minimize both 482roughness and model misfit. 483
484
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485Figure 7. Comparison of InSAR line-of-sight (LOS) change for data and our preferred 486model. (a) Observed LOS displacement, repeated from Figure 2. (b) LOS projection of the 487optimal model results. (c) Residual LOS displacement, determined by removing the predicted 488(b) from the observed (a) signal. 489
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Figure 8. Comparison between observed waveforms at regional DART gauges (black line), 490results produced in Tang et al. (2016) (blue line) and our preferred model (red line). For each 491location, our model is shifted 140 seconds forward in time and the results produced in Tang 492et al. (2016) are shifted forward 72 seconds in time. 493
494
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e He
ight
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] DART 32401
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Figure 9. The cumulative high-frequency energy radiated from the Illapel earthquake is 495shown (red line) using data from 41 seismic stations available in real-time (red triangles in 496map) and automatically processed following Convers and Newman (2011). The automated 497rupture duration, TR (dashed gray line), two near-linear periods of growth (denoted by thick 498blue lines) and their termination times relative to the earthquake nucleation (dashed black 499lines). The cumulative energy is converted to a high-frequency energy magnitude, which 500appears deficient for this event, similar but more moderate than slow-rupturing tsunami 501earthquakes. 502 503