Earthquake source parameters for the January, 2010, Haiti mainshock and aftershock sequence Meredith Nettles1,2 and Vala Hjörleifsdóttir1,3 1 2 Lamont-Doherty Earth Observatory of Columbia University Department of Earth and Environmental Sciences, Columbia University 3 Now at Universidad Nacional Autónoma de México submitted to GJI May 27, 2010 Accepted —- ; Received —- ; in original form 2010 May 27 Abbreviated title: Haiti earthquake source parameters Corresponding author: Meredith Nettles tel: +1 845 365 8613 fax: +1 845 365 8150 email: [email protected] 1 Summary 2 Previous analyses of geologic and geodetic data suggest that the obliquely compressive relative mo- 3 tion across the Caribbean–North America plate boundary in Hispaniola is accommodated through 4 strain partitioning between near-vertical transcurrent faults on land and low-angle thrust faults 5 offshore. In the Dominican Republic, earthquake focal-mechanism geometries generally support 6 this interpretation. Little information has been available about patterns of seismic strain release 7 in Haiti, however, due to the small numbers of moderate-to-large earthquakes occurring in west- 8 ern Hispaniola during the modern instrumental era. Here, we analyze the damaging MW =7.0 9 earthquake that occurred near Port au Prince on January 12, 2010, and aftershocks occurring in 10 the four months following this event, to obtain centroid–moment-tensor (CMT) solutions for 50 11 earthquakes with magnitudes as small as MW =4.0. While the January 2010 mainshock exhibited 12 primarily strike-slip motion on a steeply dipping nodal plane (strike=250◦ , dip=71◦ , rake=22◦ ), we 13 find that nearly all of the aftershocks show reverse-faulting motion, typically on high-angle (30◦ – 14 45◦ ) nodal planes. Two small aftershocks (MW 4.2 and 4.6), located very close to the mainshock 15 epicenter, show strike-slip faulting with geometries similar to the mainshock. One aftershock lo- 16 cated off the south coast of Haiti shows low-angle thrust faulting. We also analyze earthquakes 17 occurring in this region from 1977–2009 and find evidence for both strike-slip and reverse fault- 18 ing. The pattern of seismic strain release in southern Haiti thus indicates that partitioning of plate 19 motion between transcurrent and reverse structures extends far west within Hispaniola. While we 20 see limited evidence for low-angle underthrusting offshore, most reverse motion appears to oc- 21 cur on high-angle fault structures adjacent to the Enriquillo fault. Our results highlight the need 22 to incorporate seismogenic slip on compressional structures into hazard assessments for southern 23 Haiti. 24 Keywords: Earthquake source observations; Seismicity and tectonics; Caribbean tectonics 1 25 1 Introduction 26 A large and destructive earthquake of MW 7.0 occurred on January 12, 2010, near the densely 27 populated capital city of Haiti, Port au Prince. The earthquake occurred in a region of known, but 28 poorly characterized, historical seismicity (e.g., Scherer, 1912), on the Enriquillo–Plaintain Garden 29 fault system. This system accommodates primarily transform motion between the Caribbean and 30 North American plates (e.g., Mann et al., 1995). The overall relative plate motion is transpressional 31 (e.g., Sykes et al., 1982; Deng & Sykes, 1995; Dixon et al., 1998; DeMets et al., 2000; Manaker et 32 al., 2008), and many compressional geological features have been mapped in the region (Mann et 33 al., 1995). However, the only mapped throughgoing fault structure near the source of the January 34 12 earthquake, the Enriquillo fault, exhibits primarily transcurrent motion, and is believed to dip 35 nearly vertically (Mann et al., 1995, 2002). 36 No earthquakes larger than M∼5 have occurred in southern Haiti during the last 34 years, 37 approximately the era of modern instrumental recording and the timespan (1976–2009) covered 38 by the Global Centroid–Moment Tensor (GCMT) catalog (Ekström et al., 2005; Dziewonski et 39 al., 1981). One earthquake in northern Haiti, on March 2, 1994, of MW 5.4, exhibits left-lateral 40 strike-slip motion on a nodal plane striking east-southeast, consistent with the mapped geometry 41 of the Septentrional fault associated with the northern part of the plate-boundary zone (Prentice et 42 al., 1993; Mann et al., 1998). The most recent large earthquake on the island of Hispaniola, prior 43 to the January 12, 2010, event, occurred on September 22, 2003, in the Dominican Republic, with 44 moment magnitude MW 6.4. The focal mechanism for that event, as for all other earthquakes of 45 MW 6.0 or larger occurring in the Dominican Republic and included in the GCMT catalog, shows 46 thrust faulting. 47 Paleoseismic investigations and historical reports make it clear that large earthquakes have 48 occurred in Haiti previously (e.g., Scherer, 1912; Prentice et al., 1993). Recent studies using ge- 49 ological and geodetic data have also highlighted the potential for earthquakes of M∼7–7.5 on the 50 Enriquillo and Septentrional faults (Calais et al., 2002; Manaker et al., 2008). Little is known, 51 however, about the character of smaller, recent earthquakes in the Enriquillo fault region, or about 2 52 background seismicity rates, because of the absence of a local seismic network in Haiti. Follow- 53 ing the great 2004 Sumatra–Andaman earthquake and the large tsunami it generated, the United 54 States Geological Survey (USGS) invested in a significant improvement to broadband seismolog- 55 ical observing capabilities in the Caribbean, installing nine broadband seismometers in the region 56 (network code CU), each with near-realtime telemetry capabilities. The combined network cover- 57 age provided by the CU and global-network stations, along with improvements to moment-tensor 58 determination techniques (Arvidsson & Ekström, 1998; Ekström et al., 1998) now make analysis 59 of smaller earthquakes possible. 60 Knowledge of seismic strain-release patterns prior to and following the January 2010 main- 61 shock is important for understanding how strain is accommodated throughout the region, and for 62 understanding possible effects of static stress changes related to the mainshock and larger after- 63 shocks. The minimum magnitude threshold for global CMT analysis is normally set at M∼5, 64 which would lead to GCMT analyses of fewer than a dozen events for the current Haiti se- 65 quence. Here, we present centroid–moment-tensor solutions for 50 earthquakes of the 2010 Haiti 66 mainshock–aftershock sequence, including events with magnitudes as small as MW =4.0. We also 67 present analyses of four earthquakes of magnitude 4.3–4.9 occurring prior to the mainshock, during 68 the years 1990–2008. 69 2 70 We apply the centroid–moment-tensor approach (Dziewonski et al., 1981; Dziewonski & Wood- 71 house, 1983; Ekström et al., 2005) to obtain moment tensors, centroid locations and centroid times 72 for the January 12, 2010, Haiti mainshock and aftershock sequence. We attempt to analyze all 73 earthquakes in the map region shown in Figure 1 reported by the USGS National Earthquake In- 74 formation Center (NEIC) as of May 20, 2010, with preliminary magnitudes of 4.0 and larger for 75 the four months following the mainshock (2010/01/12–2010/05/12). In addition, we attempt to 76 analyze all events reported in the USGS monthly listing with magnitude 4.0 or larger during the Data and methods 3 77 period 1977–2009. 78 For larger events (approximately MW ≥5.0), we follow the standard procedures used for global 79 CMT analysis (Ekström et al., 2005). These analyses incorporate long-period body waves in the 80 period range 50–150 s; mantle waves in the period range 125–350 s; and intermediate-period sur- 81 face waves in the period range 50–150 s. The determination of source parameters for smaller 82 events relies primarily on the intermediate-period surface waves; the surface-wave analysis is im- 83 plemented as described by Arvidsson & Ekström (1998) and Ekström et al. (1998). For some 84 events, we adjust the filter towards shorter periods, which typically provide better signal-to-noise 85 ratios for shallow earthquakes. Most such events are analyzed in the 40–100 s band. For the small- 86 est events, typically those of MW ≤ 4.5, the closest stations (∆ ≤ 15◦ ) are analyzed in the period 87 range 35–75 s. The filter is selected on a station-by-station basis in this case. We use data recorded 88 at the stations of the GSN, Geoscope, Geofon, the Lamont-Doherty Cooperative Seismographic 89 Network (LCSN), and the USGS Caribbean network (CU) for our analyses, as well as stations of 90 the Abbreviated Seismic Research Observatory (ASRO) network for early events. 91 3 92 We are able to obtain CMT solutions for 50 earthquakes of the January 12, 2010, sequence, and 93 four events occurring prior to 2010. Focal mechanisms for these events are shown in Figure 1 94 and source parameters are presented in Supplementary Table 1. The source parameters can also 95 be downloaded in electronic format from our website (www.globalcmt.org). In the figures 96 and table, we identify 14 of the events as having less-well constrained focal mechanisms. These 97 are events with fewer usable data records, either due to small event size or the presence of large 98 amplitude waveforms from earlier events. As can be seen in Figure 1, the results for these events 99 are consistent with those for the best-constrained events. Analysis and Results 4 100 3.1 The January 12, 2010, mainshock 101 The source parameters obtained for the mainshock are similar to those for the quick CMT dis- 102 tributed within hours of the event. The refined solution has scalar moment M0 = 4.4 × 1026 dyne- 103 cm (MW =7.0). The presumed fault plane strikes 250◦ and dips 71◦ north-northwest. The slip 104 angle of 22◦ indicates primarily left-lateral motion, with a moderate thrust component. The best- 105 fitting moment tensor includes a non-double-couple component that is relatively large, with the 106 intermediate eigenvalue ∼20% the size of the absolutely largest eigenvalue. The size of the non- 107 double-couple component is not well constrained, but is also consistent with a thrust contribution 108 to the mainshock. The geometry of the focal mechanism obtained when the solution is required 109 to represent a perfect double couple is very similar to the double-couple part of the unconstrained 110 solution, with strike 252◦ , dip 66◦ , and rake 28◦ . 111 The mainshock focal mechanism, which corresponds to the best point-source representation 112 of the earthquake geometry, is consistent with oblique slip on a single fault plane or, if the non- 113 double-couple component represents a source feature, nearly simultaneous slip on two separate 114 fault planes experiencing left-lateral and reverse slip. To assess seismological constraints on the 115 geometry of the mainshock fault or faults, we perform two analyses. 116 First, we invert the waveforms used to determine the mainshock moment tensor for a CMT 117 solution composed of two subsources to determine the geometry of the reverse mechanism that, 118 paired with a near-vertical strike-slip fault, best explains the observed waveforms. One subsource is 119 constrained to have a nodal plane oriented 250◦ with pure left-lateral slip and a dip of either 71◦ or 120 90◦ , while the geometry of the second subsource is constrained to be a double couple, but otherwise 121 left free. The retrieved geometry of the second subsource depends somewhat on the subsource time 122 separation, but we find that a reverse-faulting subsource with a strike of ∼ 250–270◦ , dip of ∼65◦ , 123 and scalar moment 30–40% that of the total moment, combined with a subsource of near-vertical 124 dip and left-lateral slip, explains the data well. 125 Second, we conduct an analysis of how well we are able to resolve the dip of the mainshock 126 fault plane under the assumption that the fault slipped obliquely on a single planar fault. We 5 127 perform a series of inversions in a grid search over the source geometry. The strike is fixed to either 128 252◦ (for a north-dipping nodal plane) or 72◦ (for a south-dipping nodal plane), the rake is varied 129 between −45◦ and +45◦ and the dip is varied between 55◦ and 90◦ , in 5◦ increments, in an approach 130 similar to that taken by Henry et al. (2000) for the Antarctic plate earthquake. The residual misfit 131 between observed and synthetic waveforms is shown in Figure 2a. We find two minima in the 132 misfit function, with the deeper minimum corresponding to the best-fit double-couple solution 133 described earlier, with a north-dipping fault plane. The shallower minimum corresponds to a south- 134 dipping fault plane, with strike 72◦ , dip 65◦ and rake 25◦ . The residual variance is dominated by 135 the contribution from the long-period mantle waves, and the difference in misfit for the north- 136 and south-dipping solutions is relatively small. However, the body waves for the south-dipping 137 fault plane are fit poorly, especially at several stations in nodal directions. An example of the 138 difference in waveform fits to the body waves for the north- and south-dipping fault planes is 139 shown in Figure 2b. We conclude that the fault plane must indeed dip to the north, under the 140 assumption that all of the slip occurred on a single planar fault. 141 3.2 142 The most surprising result of our CMT analysis is that nearly all of the aftershocks for which 143 we are able to obtain solutions show reverse faulting (Fig. 1). Indeed, we find only two after- 144 shocks, an MW 4.2 event on January 16 and an MW 4.6 event on February 23, both located very 145 close to the mainshock hypocenter, that show dominantly strike-slip motion (Fig. 1). Most of 146 the reverse-faulting events exhibit steeply dipping (30◦ –45◦ ) nodal planes, though a few have one 147 nodal plane of shallower dip. One event, which occurred off the south coast of Haiti (January 15, 148 2010; MW 4.6), shows underthrusting on a plane dipping 13◦ to the north. All of the events are 149 found to be shallow (≤22 km), with most solutions returning depths of 12 km, the minimum depth 150 allowed for standard CMT inversions in the absence of additional depth constraints. The aftershock sequence 151 Aftershocks occurring immediately after the mainshock can be difficult to analyze because 152 of interference from the large mainshock surface waves at all stations. We have paid particular 6 153 attention to these early aftershocks to assess whether they might exhibit transcurrent, rather than 154 reverse, motion. In several cases, we have performed joint inversions for earthquakes occurring 155 close in time to confirm that interference between wave packets does not bias our results. We find 156 that even those events occurring within the first hours after the mainshock are dominated by reverse 157 motion, including a MW 6.0 event seven minutes after the mainshock. 158 The directions of maximum compression for the reverse-faulting events are oriented NE–SW in 159 all but three cases, with P-axis azimuths ranging from 0–50◦ , and most falling in the range 5–35◦ . 160 We find some suggestion for two preferred P-axis orientations, one near 10◦ and one near 30◦ , but 161 the clustering is not strong. We believe the variability in retrieved CMT parameters reflects true 162 variability in the geometry of the earthquake sources: the relative orientations of the individual 163 sources are well constrained by our analysis, which uses a nearly identical subset of stations for 164 earthquakes of similar magnitude. The variation in source geometry is also clear in many of the 165 waveforms, as shown in Figure 3. 166 3.3 167 We are able to obtain CMT solutions for four earthquakes, of MW = 4.3–4.9, occurring prior to 168 the January 2010 mainshock. The focal mechanisms we retrieve for the pre-mainshock events are 169 consistent with those observed for the aftershock sequence: three of the four moment tensors show 170 reverse faulting, with the fourth showing strike-slip faulting on an approximately E–W trending 171 nodal plane. The reverse-faulting events are located to the west of the January 2010 mainshock, 172 and the geometry of the events occurring in the aftershock zone is similar to that observed for the 173 2010 sequence. The strike-slip event is located to the east of the 2010 mainshock, in a region of 174 relatively weak aftershock activity. One event (December 31, 1990) for which we are unable to 175 obtain a robust CMT solution nonetheless appears to have both a location and source geometry 176 similar to the underthrusting event of January 15, 2010, off the south coast. As for the aftershocks, 177 the P-axis orientations of these earlier events lie in the range 0–50◦ . Earthquakes prior to 2010 7 178 4 Discussion and Conclusions 179 The dominance of reverse faulting in the aftershock sequence for this large strike-slip earthquake 180 is unusual, and we are not aware of previous examples of aftershock sequences which are both so 181 different from the mainshock geometry and so internally consistent. While the 1989 Loma Prieta 182 earthquake generated an aftershock sequence in which many events differed in geometry from 183 the mainshock, the aftershocks also exhibited great internal variability, with examples of left- and 184 right-lateral strike-slip, normal, and reverse faulting (Beroza & Zoback, 1993). 185 The locations of the Haiti aftershocks are distributed over a wide area, mostly to the west of 186 the mainshock hypocenter. The centroid locations we determine are systematically shifted to the 187 north with respect to the hypocenter locations reported by the NEIC, probably as a result of station 188 coverage dominated by North American stations and because of the very slow raypaths through 189 the Gulf of Mexico and northern Caribbean. However, the centroid locations remain as widely 190 distributed as the reported hypocenter locations, and the combination of geographical distribution 191 of the earthquake locations and the variation in focal geometry suggest that the aftershocks occur 192 on multiple, distributed fault structures, rather than on a single reverse fault. 193 Nearly all of the aftershocks occur on planes striking WNW–ESE. If the reverse component of 194 the mainshock occurred on a separate reverse fault, rather than as oblique slip on the Enriquillo 195 fault, our analysis suggests that this reverse fault strikes ENE–WSW to E–W, like the Enriquillo 196 fault itself, and that it must be large enough to accommodate an earthquake of approximately 197 MW 6.8. However, further knowledge of the accommodation of reverse motion during the main- 198 shock will require detailed analysis of higher-frequency body waves and satellite remote-sensing 199 data. 200 The reverse motion we observe in the Haiti aftershocks is consistent with the presence of mul- 201 tiple thrust structures mapped in the region (Mann et al., 1995) and with a measured component 202 of compression across the island of Hispaniola (Manaker et al., 2008). However, previous studies 203 of strain partitioning in the northern Caribbean have concluded that the overall east-northeastward 204 motion is divided between the Enriquillo and Septentrional strike-slip faults on land and low-angle 8 205 underthrusting structures off the north and southeast coasts of Hispaniola (Mann et al., 2002; Man- 206 aker et al., 2008). Our results, from the aftershock sequence and earlier earthquakes, indicate that 207 strain partitioning in southwest Hispaniola occurs through left-lateral slip on the Enriquillo fault 208 and reverse slip on adjacent high-angle faults. We infer that many anticlinal structures observed on 209 land (Mann et al., 1995) are fault cored. 210 The prevalence of reverse faulting for the earthquakes analyzed, apart from the January 12, 211 2010, mainshock, emphasizes the need to incorporate seismogenic slip on compressional structures 212 into hazard assessments for southern Haiti. While the reverse events appear to occur on multiple 213 fault structures, rather than a single, large thrust fault, probably limiting the maximum size of such 214 events, even earthquakes of MW 4–5 are large enough to cause damage at local distances. Further, 215 we see some evidence for thrust faulting off the south coast of Haiti with geometry similar to that 216 of larger underthrusting events that have occurred to the east in the Dominican Republic. The 217 seismic deformation occurring on reverse faults should also be taken into account in stress-transfer 218 models like those used to assess probable loading on the Enriquillo fault and its branches (e.g., Lin 219 et al., 2010). 220 Acknowledgments 221 We thank R. S. Stein, F. Waldhauser, T. Diehl, N. Seeber, and G. Ekström for suggestions and 222 discussions. The GSN data were collected and distributed by IRIS and the USGS. We thank the 223 operators of the GSN, LCSN, Geoscope, and Geofon for collecting and archiving the seismic data 224 used here. This work was supported by NSF awards EAR-0824694 and EAR-0710842. 9 225 References 226 Ali, S. T., Freed, A.M., Calais, E., Manaker, D. M. & McCann, W. R., 2008. Coulomb stress 227 evolution in the Northeastern Caribbean over the past 250 years due to coseismic, postseismic 228 and interseismic deformation, Geophys. J. Int., 174, 904–918. 229 230 231 232 Arvidsson, R. & Ekström, G. 1998. Global CMT analysis of moderate earthquakes, MW ≥ 4.5, using intermediate-period surface waves, Bull. Seism. Soc. Am., 88, 1003–1013. Beroza, G. C. & Zoback, M. D., 1993. Mechanism diversity of the Loma Prieta aftershocks and the mechanics of mainshock–aftershock interaction, Science, 259, 210–213. 233 Calais, E., Mazabraud, Y., de Lapinay, B. M., Mann, P., Mattioli, G. & Jansma, P., 2002. Strain par- 234 titioning and fault slip rates in the north-eastern Caribbean from GPS measurements, Geophys. 235 Res. Lett., 29, doi:10.1029/2002GL015397. 236 DeMets, C., Jansma, P., Mattioli, G., Dixon, T., Farina, F., Bilham, R., Calais, E. & Mann, P., 2000. 237 GPS geodetic constraints on Caribbean–North America plate motion, Geophys. Res. Lett., 27, 238 437–440. 239 Deng, J., & Sykes, L. R., 1995. Determination of Euler pole for contemporary relative motion of 240 Caribbean and North American plates using slip vectors of interplate earthquakes, Tectonics, 241 14, 39–53. 242 Dixon, T.H., Farina, F., DeMets, C., Jansma, P., Mann, P. & Calais, E., 1998. Relative motion 243 between the Caribbean and North American plates and related plate boundary deformation 244 based on a decade of GPS observations, J. Geophys. Res., 103, 15,157–15,182. 245 Dziewonski, A. M., Chou, T.-A. & Woodhouse, J. H., 1981. Determination of earthquake source 246 parameters from waveform data for studies of global and regional seismicity, J. Geophys. Res., 247 86, 2825–2852. 248 Dziewonski, A. M. & Woodhouse, J. H., 1983. An experiment in systematic study of global seis- 249 micity: Centroid-moment tensor solutions for 201 moderate and large earthquakes of 1981, J. 250 Geophys. Res., 88, 3247–3271. 251 Ekström, G., Dziewonski, A. M., Maternovskaya, N. N. & Nettles, M., 2005. Global seismicity of 10 252 2003: centroid-moment-tensor solutions for 1087 earthquakes, Phys. Earth Planet. Inter., 148, 253 327–351. 254 Ekström, G., Morelli, A., Boschi, E. & Dziewonski, A. M., 1998. Moment tensor analysis of the 255 central Italy earthquake sequence of September–October 1997, Geophys. Res. Lett., 25, 1971– 256 1974. 257 258 Henry, C., Das, S. & Woodhouse, J. H., 2000. The great March 25, 1998, Antarctic Plate earthquake: Moment tensor and rupture history, J. Geophys. Res., 105, 16,097–16,118. 259 Lin, J., Stein, R. S., Sevilgen, V. & Toda, S., 2010. USGS–WHOI–DPRI Coulomb stress-transfer 260 model for the January 12, 2010, MW =7.0 Haiti earthquake, U. S. Geological Survey Open-File 261 Report 2010-1019, 7 pp. 262 Manaker, D. M., Calais, E., Freed, A. M., Ali, S. T., Przybylski, P., Mattioli, G., Jansma, P., 263 Prépetit, C. & de Chabalier, J. B., 2008. 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Motion of Caribbean Plate during last 7 million 276 years and implications for earlier Cenozoic movements, J. Geophys. Res., 87, 10,656–10,676. 11 277 Figure captions 278 Figure 1. Top: Focal mechanisms for 50 earthquakes of the January 12, 2010, Haiti mainshock– 279 aftershock sequence. Bottom: Focal mechanisms for four earthquakes occurring in 1990–2008, 280 prior to the 2010 mainshock. All events are plotted at the NEIC epicentral locations. The mecha- 281 nisms shown in gray are less well constrained than those shown in red. 282 Figure 2. (a) Residual misfit for pure double-couple solutions, with strike 252◦ (left side of image) 283 and 72◦ (right side of image) and varying rake and dip; note non-linear color bar. There are two 284 minima, one for the north-dipping fault plane (left) and one for the south-dipping fault plane (right). 285 The residual misfit for the north-dipping plane is slightly smaller than that for the south-dipping 286 plane. (b) An example of waveform fits to the body waves for the solutions corresponding to the 287 two minima in (a). Shown is the vertical component of displacement (blue: data; red: model), 288 band-pass filtered between 50 and 150 seconds, from station KDAK (Alaska), at a distance of 69◦ 289 and azimuth of 326◦ . Shaded regions lie outside the body-wave window and are excluded from the 290 inversion. 291 Figure 3. Observed (blue) and synthetic (red) surface-wave seismograms (vertical component of 292 displacement) for events 201001130132A (black arrows) and 201001130136A (green arrows) at 293 several stations located at epicentral distance ∆ and azimuth α. All records are band-pass filtered 294 between 50 and 150 seconds. The relative amplitudes of the arrivals for the two events vary with 295 azimuth, indicating different focal geometries for the two events, which have similar depths and 296 source locations. The filter used in the analysis is acausal, leading to the apparent arrival of surface- 297 wave energy prior to the event onset (0 seconds). 12 Figures Figure 1: Top: Focal mechanisms for 50 earthquakes of the January 12, 2010, Haiti mainshock–aftershock sequence. Bottom: Focal mechanisms for four earthquakes occurring in 1990–2008, prior to the 2010 mainshock. All events are plotted at the NEIC epicentral locations. The mechanisms shown in gray are less well constrained than those shown in red. 13 (a) (b) 0.900 North-dipping fault plane 0.800 0.700 0.600 0.500 0.450 0.400 South-dipping fault plane 0.350 0.320 0.310 0.305 0.300 0.295 Figure 2: (a) Residual misfit for pure double-couple solutions, with strike 252◦ (left side of image) and 72◦ (right side of image) and varying rake and dip; note non-linear color bar. There are two minima, one for the north-dipping fault plane (left) and one for the south-dipping fault plane (right). The residual misfit for the north-dipping plane is slightly smaller than that for the south-dipping plane. (b) An example of waveform fits to the body waves for the solutions corresponding to the two minima in (a). Shown is the vertical component of displacement (blue: data; red: model), band-pass filtered between 50 and 150 seconds, from station KDAK (Alaska), at a distance of 69◦ and azimuth of 326◦ . Shaded regions lie outside the body-wave window and are excluded from the inversion. 14 ∆ = 1.7, α = 69 ∆ = 2.6, α = 307 ∆ = 14, α = 237 ∆ = 30, α = 188 Figure 3: Observed (blue) and synthetic (red) surface-wave seismograms (vertical component of displacement) for events 201001130132A (black arrows) and 201001130136A (green arrows) at several stations located at epicentral distance ∆ and azimuth α. All records are band-pass filtered between 50 and 150 seconds. The relative amplitudes of the arrivals for the two events vary with azimuth, indicating different focal geometries for the two events, which have similar depths and source locations. The filter used in the analysis is acausal, leading to the apparent arrival of surface-wave energy prior to the event onset (0 seconds). 15 ∗ 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 11 12 13 14 15 ∗ 16 17 ∗ 18 19 ∗ 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 ∗ 38 39 40 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 2010 51 52 53 54 2 3 3 4 1 1 1 1 1 1 1 1 2 2 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 4 4 5 8 1 1 1 1 1 1 23 1 28 15 22 23 24 25 25 26 26 27 4 22 15 15 15 16 17 17 20 20 21 21 13 13 13 13 13 14 14 14 14 15 13 13 13 13 13 13 13 13 13 13 28 28 12 5 12 12 13 13 13 13 D 6 10 7 13 12 2 21 12 18 11 14 0 5 9 13 20 21 16 17 18 11 15 16 16 12 12 14 21 22 5 8 10 12 8 1 2 5 5 5 5 6 6 7 12 19 21 0 9 21 22 0 1 1 1 h 26 37 16 4 54 29 51 30 40 16 3 57 0 36 41 4 4 0 51 19 3 12 45 54 41 53 43 26 21 3 15 32 39 56 57 11 3 18 24 49 24 58 23 28 29 22 58 49 53 0 59 32 36 55 m 24.7±0.5 36.0±0.7 19.0±0.4 59.4±0.4 16.7±0.6 18.8±0.8 58.4±0.9 22.7±0.8 30.5±0.2 60.0±0.8 16.2±0.9 27.1±0.3 2.5±0.7 7.5±0.6 42.7±0.5 13.1±0.6 50.3±0.6 0.5±0.5 11.0±0.7 20.4±0.6 47.6±0.1 13.1±0.8 22.6±0.3 10.8±0.2 45.4±0.6 52.3±0.6 46.7±0.2 17.4±0.3 17.0±0.3 8.4±0.6 43.8±0.4 27.4±0.6 4.1±0.3 6.6±0.3 37.0±0.3 31.3±1.1 0.1±0.1 5.7±0.2 3.2±0.5 25.1±1.0 19.2±0.6 27.4±0.7 3.4±0.3 26.5±0.6 8.2±0.3 47.0±0.7 3.3±0.6 22.0±0.5 17.1±0.1 46.1±0.6 10.3±0.9 47.7±0.3 36.5±0.3 17.3±0.9 Time sec indicates less-well constrained event (see text). ∗ ∗ 41 42 43 ∗ 44 45 46 47 48 ∗ 49 ∗ 50 ∗ ∗ ∗ ∗ ∗ 1990 1990 2005 2008 2010 2010 2010 2010 2010 2010 Date Y M 1 2 3 4 5 6 7 8 9 10 No. 3.8 0.2 1.7 0.6 2.9 -0.8 3.2 2.1 1.9 0.2 0.2 0.1 1.3 4.4 -0.9 1.1 3.1 4.6 2.1 0.0 4.3 2.2 0.9 1.2 1.2 4.9 1.9 1.0 3.6 1.8 1.5 -1.4 0.8 1.6 2.4 0.6 2.6 3.2 0.9 2.2 3.2 1.3 -0.5 1.8 3.4 1.3 3.3 5.6 6.9 4.6 5.2 3.5 5.1 1.3 δt0 18.62±.02 18.72±.05 18.61±.03 18.78±.03 18.81±.05 18.73±.07 18.60±.13 18.77±.05 18.64±.02 18.63±.05 18.22±.08 18.65±.02 18.68±.04 18.65±.04 18.44±.05 18.37±.07 18.05±.04 18.69±.03 18.68±.07 18.64±.04 18.67±.00 18.51 18.72±.03 18.63±.02 18.60±.06 18.67±.07 18.71±.01 18.64±.02 18.67±.02 18.67±.04 18.46±.04 18.45±.05 18.66±.02 18.47±.03 18.64±.02 18.59±.08 18.64±.01 18.51±.02 18.57±.05 18.72±.05 18.69±.05 18.62±.04 18.56±.03 18.72±.05 18.58±.03 18.63±.03 18.48±.03 18.83±.04 18.61±.00 18.58±.06 18.66±.06 18.63±.02 18.60±.02 18.59±.07 0.17 0.31 0.15 0.23 0.33 0.23 0.09 0.26 0.15 0.13 -0.17 0.27 0.18 0.16 0.34 0.17 0.04 -0.12 -0.07 0.24 0.10 0.17 0.25 0.25 0.26 0.27 0.15 0.32 0.18 0.12 0.01 0.30 0.07 0.24 0.18 0.26 0.19 0.12 0.30 0.31 0.18 0.17 0.31 0.12 0.21 0.01 0.27 0.16 0.19 0.31 0.21 0.20 0.26 Centroid Parameters Latitude λ δλ0 -72.55±.03 -72.96±.07 -72.94±.04 -72.95±.04 -72.97±.08 -71.96±.08 -72.74±.15 -73.13±.08 -72.94±.03 -72.98±.10 -72.01±.12 -73.03±.03 -72.48±.06 -72.57±.03 -72.79±.05 -72.73±.05 -72.34±.05 -72.44±.02 -72.77±.09 -72.84±.08 -72.81±.01 -72.79 -72.82±.03 -72.86±.03 -73.44±.07 -72.92±.08 -72.95±.02 -72.52±.03 -72.52±.04 -72.97±.05 -72.86±.05 -72.88±.06 -72.88±.04 -72.81±.04 -73.02±.03 -73.23±.10 -72.92±.01 -72.83±.02 -72.89±.06 -72.96±.09 -73.07±.05 -72.93±.07 -72.95±.04 -73.05±.08 -72.79±.04 -72.62±.07 -72.45±.04 -73.63±.03 -72.62±.01 -72.88±.06 -72.97±.08 -72.98±.03 -72.98±.03 -73.08±.08 0.04 -0.11 -0.06 -0.15 -0.52 0.01 -0.10 -0.16 0.01 0.20 0.13 -0.11 0.29 -0.01 0.03 -0.12 0.03 0.10 -0.04 0.10 -0.23 0.01 0.00 -0.60 -0.11 -0.02 -0.02 0.05 -0.10 -0.11 -0.16 -0.16 0.03 -0.14 -0.20 -0.02 0.06 -0.08 0.01 -0.18 -0.03 -0.11 -0.24 0.11 0.24 -0.14 -0.07 -0.07 -0.09 -0.16 -0.12 -0.15 -0.23 Longitude φ δφ0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 20.4± 2.7 12.0 12.0 12.0 12.0 18.0± 2.3 12.0 12.0 12.0 16.8± 2.3 12.0 12.0 12.0 12.0 21.3± 3.4 12.7± 3.7 12.0 12.0 14.0± 1.4 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 14.1± 1.2 12.0 12.0 17.5± 2.1 12.0 12.0 12.0 12.0 12.0 12.0 19.2 12.0 12.0 12.0 13.5± 1.3 13.2± 1.4 14.1± 3.7 -4.6 6.8 8.0 4.0 11.3 2.7 7.5 4.1 3.5 3.2 4.1 Depth h δh0 1.1 1.0 1.0 1.1 1.0 1.0 1.0 1.0 0.6 1.0 1.0 1.2 1.0 1.1 0.7 0.7 0.7 0.5 0.4 0.5 2.1 0.6 0.7 0.7 0.6 1.0 0.9 0.7 0.6 0.6 0.5 0.5 0.7 0.6 1.4 1.3 1.9 1.1 0.8 1.1 0.6 0.5 0.6 1.0 1.1 1.1 1.0 1.0 8.1 3.1 1.5 1.6 1.5 1.2 Half Drtn 23 22 23 22 22 22 22 22 23 22 22 23 22 22 22 23 23 22 22 23 25 22 23 23 23 22 23 23 23 22 23 22 23 23 24 23 24 24 23 23 23 23 23 22 23 23 22 22 26 25 24 24 24 23 Scale Factor 10ex 1.0 3.8 0.9 6.4 3.3 1.3 2.7 4.0 2.3 4.4 5.4 1.9 2.6 7.4 6.7 1.0 1.1 6.6 5.3 0.9 0.7 2.5 2.8 2.3 0.8 3.2 5.8 3.0 2.0 6.7 1.0 8.2 2.4 1.1 1.8 3.3 5.4 0.9 2.1 0.8 1.5 1.2 1.9 3.5 3.3 0.9 3.8 8.3 4.4 1.2 0.9 3.4 2.8 6.3 M0 0.24±0.08 3.43±0.33 0.93±0.04 6.35±0.31 2.07±0.28 1.19±0.19 2.78±0.32 3.55±0.34 2.36±0.06 4.14±0.42 4.98±1.46 1.95±0.06 2.16±0.24 2.69±0.47 6.11±0.43 0.72±0.15 0.51±0.04 -0.63±0.45 5.67±0.38 0.85±0.16 0.76±0.00 1.57±0.23 2.82±0.08 2.24±0.06 0.51±0.15 2.93±0.89 5.87±0.09 2.75±0.07 1.93±0.16 4.60±0.35 0.73±0.06 6.25±0.47 2.27±0.08 0.87±0.05 1.84±0.05 2.38±0.48 5.53±0.05 0.77±0.07 1.97±0.13 0.76±0.09 1.31±0.23 1.09±0.10 1.81±0.07 2.95±0.29 3.40±0.17 1.01±0.12 0.74±0.41 5.89±0.82 1.74±0.02 1.22±0.08 0.81±0.10 3.34±0.28 2.80±0.26 5.84±1.62 Mrr -0.14±0.07 -2.95±0.29 -0.76±0.04 -5.23±0.31 -3.24±0.25 -0.98±0.19 -1.99±0.32 -3.50±0.31 -2.07±0.06 -3.85±0.38 -2.56±0.91 -1.78±0.06 -2.24±0.21 -3.70±0.38 -3.97±0.50 -0.18±0.10 -0.45±0.04 -4.78±0.40 -4.36±0.36 -0.75±0.12 -0.63±0.00 -1.32±0.24 -2.12±0.08 -2.12±0.06 -0.79±0.16 -1.42±0.55 -5.62±0.08 -2.56±0.07 -1.55±0.11 -3.89±0.32 -0.57±0.06 -3.83±0.56 -2.01±0.08 -0.52±0.05 -1.58±0.05 -2.69±0.38 -4.83±0.05 -0.38±0.04 -1.21±0.14 -0.78±0.08 -0.86±0.17 -1.06±0.08 -1.50±0.07 -2.83±0.29 -3.01±0.12 -0.83±0.07 -2.89±0.31 -1.83±0.62 -3.87±0.02 -0.91±0.08 -0.70±0.09 -3.03±0.19 -2.74±0.17 -4.66±1.15 Mθθ -0.11±0.06 -0.48±0.30 -0.17±0.04 -1.12±0.28 1.17±0.29 -0.22±0.16 -0.78±0.30 -0.06±0.30 -0.28±0.05 -0.29±0.35 -2.42±0.98 -0.17±0.06 0.09±0.19 1.01±0.40 -2.14±0.35 -0.54±0.09 -0.06±0.03 5.42±0.34 -1.31±0.36 -0.11±0.07 -0.13±0.00 -0.25±0.21 -0.70±0.08 -0.12±0.06 0.27±0.09 -1.51±0.46 -0.26±0.08 -0.19±0.07 -0.38±0.09 -0.72±0.28 -0.16±0.06 -2.41±0.41 -0.26±0.08 -0.35±0.04 -0.26±0.05 0.31±0.45 -0.69±0.05 -0.39±0.04 -0.76±0.12 0.02±0.08 -0.45±0.12 -0.03±0.08 -0.31±0.07 -0.12±0.25 -0.39±0.19 -0.18±0.13 2.14±0.36 -4.06±0.51 2.13±0.02 -0.31±0.09 -0.11±0.08 -0.31±0.14 -0.06±0.12 -1.17±0.79 -0.53±0.17 -0.92±1.06 -0.10±0.13 -1.68±1.07 -1.14±1.12 0.29±0.46 -0.74±2.46 -1.62±1.09 0.38±0.23 1.54±1.36 2.33±0.99 0.45±0.20 -0.43±0.60 -6.21±0.97 2.75±1.62 0.64±0.22 0.95±0.13 3.67±0.93 0.83±2.45 0.18±0.20 -0.02±0.01 1.85±0.41 -0.74±0.41 0.22±0.23 0.14±0.15 -0.83±1.26 0.62±0.33 1.35±0.32 -0.38±0.22 4.18±1.06 0.62±0.22 5.37±1.73 -0.14±0.32 0.63±0.17 0.13±0.13 -1.71±0.84 -0.14±0.12 -1.00±0.77 -1.24±0.53 -0.14±0.38 0.55±1.65 -0.87±0.83 -0.15±0.27 -0.41±1.42 -0.46±1.06 -0.14±0.19 1.33±0.39 0.92±1.01 2.22±1.38 0.14±0.16 -0.16±0.12 -1.55±0.93 0.57±1.65 -0.04±0.17 -0.04±0.01 -0.20±0.43 -0.31±0.38 -0.47±0.22 -0.43±0.12 -0.36±0.97 0.06±0.38 -0.48±0.32 0.29±0.25 -2.79±0.82 -0.27±0.19 -1.46±1.59 -0.70±0.29 0.03±0.15 -0.42±0.17 -1.53±1.13 -0.11±0.17 0.25±0.06 -0.51±0.42 0.10±0.20 -0.07±0.20 -0.27±0.32 -0.81±0.24 -0.60±0.50 -0.85±0.77 0.72±0.78 -1.06±0.10 0.19±0.27 -0.26±0.19 0.21±0.29 -0.31±0.26 -3.02±1.40 0.43±0.88 -4.57±0.99 -0.53±0.10 -0.03±0.41 -0.36±0.27 -0.97±0.33 -0.13±0.25 -0.86±1.69 -0.11±0.16 -1.05±1.46 0.18±0.17 -0.10±0.07 0.58±0.66 -0.02±0.24 -0.74±0.29 -0.47±0.26 0.19±0.30 -1.45±1.31 -0.24±0.41 Mrφ -0.14±0.63 Elements of Moment Tensor Mφφ Mrθ 0.85±0.04 0.87±0.25 0.14±0.03 1.89±0.22 0.01±0.25 0.50±0.12 0.67±0.33 0.08±0.29 0.46±0.05 -0.83±0.39 2.18±0.63 0.18±0.05 -0.52±0.16 2.59±0.29 2.48±0.37 0.35±0.06 0.07±0.04 1.83±0.32 1.07±0.37 0.32±0.06 0.21±0.00 0.67±0.21 0.93±0.07 0.39±0.05 0.08±0.08 1.80±0.26 0.21±0.08 0.18±0.07 -0.84±0.06 1.29±0.25 0.46±0.04 2.68±0.37 0.73±0.06 0.49±0.03 0.23±0.04 1.04±0.41 1.22±0.04 0.61±0.02 0.85±0.10 -0.04±0.06 0.60±0.07 0.02±0.07 0.59±0.06 1.21±0.23 0.47±0.09 0.19±0.05 2.64±0.28 4.48±0.39 2.74±0.01 0.50±0.05 0.23±0.05 0.81±0.08 0.21±0.07 1.91±0.45 Mθφ Supplementary Table 1. Centroid–moment-tensor solutions for 54 earthquakes occurring in southern Haiti, 1990–5/2010. Headings are as in standard Global CMT reports (Ekström et al., 2005).
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