Journal of Seismology

, Volume 20, Issue 4, pp 1059–1073 | Cite as

Diversity of the 2014 Iquique’s foreshocks and aftershocks: clues about the complex rupture process of a Mw 8.1 earthquake

  • Sergio León-Ríos
  • Sergio Ruiz
  • Andrei Maksymowicz
  • Felipe Leyton
  • Amaya Fuenzalida
  • Raúl Madariaga


We study the foreshocks and aftershocks of the 1 April 2014 Iquique earthquake of Mw 8.1. Most of these events were recorded by a large digital seismic network that included the Northern Chile permanent network and up to 26 temporary broadband digital stations. We relocated and computed moment tensors for 151 events of magnitude Mw ≥ 4.5. Most of the foreshocks and aftershocks of the Iquique earthquake are distributed to the southwest of the rupture zone. These events are located in a band of about 50 km from the trench, an area where few earthquakes occur elsewhere in Chile. Another important group of aftershocks is located above the plate interface, similar to those observed during the foreshock sequence. The depths of these events were constrained by regional moment tensor (RMT) solutions obtained using the records of the dense broad band network. The majority of the foreshocks and aftershocks were associated to the interplate contact, with dip and strike angles in good agreement with the characteristics of horst and graben structures (>2000 m offset) typical of the oceanic Nazca Plate at the trench and in the outer rise region. We propose that the spatial distribution of foreshocks and aftershocks, and its seismological characteristics were strongly controlled by the rheological and tectonics conditions of the extreme erosive margin of Northern Chile.


Earthquake Chile Nazca Plate Moment tensor Erosive margin 

1 Introduction

On 1 April 2014, a Mw 8.1 earthquake occurred offshore of the city of Iquique, located in the Tarapaca Region in Northern Chile. This region had been identified as a seismic gap because the last mega-earthquake took place on 9 May 1877 with a magnitude greater than Mw 8.5 (Kelleher 1972; Comte and Pardo 1991) (see Fig. 1a). Several events larger than seven occurred in this area since 1911 (Malgrange and Madariaga 1983; Comte and Pardo 1991; Pacheco and Sykes 1992; Ruegg et al. 1996; Engdahl and Villaseñor 2002; Peyrat et al. 2010). Inversions of geodetic data (interferometry and GPS) by Béjar-Pizarro et al. (2013) and Métois et al. (2013) found high values of interseismic coupling on the coastal region of Northern Chile anticipating the occurrence of a major earthquake in this zone. The 2014 Iquique earthquake filled the central region of the Northern Chile seismic gap (see Fig. 1).
Fig. 1

Iquique Earthquake of 1 April 2014 in its context. On the left (a), the stars show the main foreshock of 16 March 2014, the main event of 1 April 2014, and its main aftershock of 3 April 2014. We also included the 2007 Mw 7.7 Tocopilla earthquake and the 2005 Mw 7.8 Tarapaca earthquake. Triangles show the broad band instruments available for the localization and RMT determination. Black squares are the IPOC network; green and red triangles are the temporary stations available before and after the main event, respectively. Inset in the figure is the slip model for the 2014 Iquique earthquake and its main aftershock obtained by Ruiz et al. (2014) in order to show the rupture zone of the events. On the right (b) is the seismicity that preceded the main event of 1 April and its main aftershock of 3 April 2014. The events are color coded according to the date of occurrence

The possible occurrence of a future mega-earthquake in Northern Chile led in 2006 to the deployment of a seismological network by the Integrated Plate boundary Observatory in Chile (IPOC) and the National Seismological Center (CSN) of the Universidad de Chile. After the beginning of the immediate precursors on 16 March 2004, these networks were supplemented by 26 temporary broadband stations, constituting a denser network that recorded the final seismic process leading to the 2014 Iquique earthquake and its aftershocks (Fig. 1a). The seismic sequence that ended in the Mw 8.1 event started several years earlier. Seismicity near Iquique started to increase when an event of Mw 6.3 occurred on 4 February 2008 south of Iquique. Since then, seismicity steadily increased until it reached a peak 2 weeks before the main shock (Ruiz et al. 2014; Schurr et al. 2014; Lay et al. 2014; Hayes et al. 2014) (see Fig. 1b). On 16 March 2014, the largest foreshock, an Mw 6.7 earthquake occurred within the overriding South American plate. The focal mechanism of this event was a reverse fault, with a strike direction at large angle with respect to the trench. After 16 March, the precursory seismicity migrated 50 km to the north where several Mw ∼6.0 reverse events occurred along the contact between the Nazca and South American plates. Finally, on 1 April, an estimated rupture zone of 100 km × 50 km was broken by the main event of magnitude Mw 8.1 (Ruiz et al. 2014; Hayes et al. 2014; Schurr et al. 2014). The largest aftershock occurred on April 3, with magnitude Mw 7.6 in the deeper zone of the seismogenic contact, 100 km south of the hypocenter of the mainshock.

The seismicity on the plate interface from 2008 until the 1 April earthquake took place in a region that is usually considered with low background activity by many researchers (see, e.g., Scholz 1998). Lay et al. (2012) identified this area as type B, a region that produces low short period energy. Hubbard et al. (2015) discussed these classifications. It is thus important to study why a persistent zone of active seismicity developed at shallow depths in the Tarapaca Region of Northern Chile. Seismicity close to the trench of the subduction interface is rare in Chile, even if we take into consideration that until 2006, the seismic network was not good enough to detect smaller events in that area. A similar sequence of events occurred in July 1997 offshore of the Coquimbo Region of central Chile. Those events were followed 3 months later by the Mw 7.6 Punitaqui earthquake of 15 October 2007 (see Gardi et al. 2006). The 1997 event was an intermediate depth along slab compressional event, and the Coquimbo region was broken on 16 September 2016 by Illapel Mw 8.3 earthquake. It is important to understand why a long-term sequence of events occurred westward Iquique, close to the trench.

Another possible explanation for the origin of shallow seismicity is that the Iquique sequence took place in an erosive subduction margin (Ranero et al. 2006; Contreras Reyes et al. 2012). Northern Chile is characterized by a small frontal accretionary prism. In this context, the horst and graben structure (>2000 m offset) present in the first 50 km to the east of the trench of the oceanic Nazca Plate may control the diversity of events observed during foreshocks (Ruiz et al. 2014; Hayes et al. 2014; Schurr et al. 2014) and aftershocks. This behavior of the seismicity, with several types of events, has been observed in other large subduction earthquakes such as Maule 2010 (Agurto et al. 2012) and Tohoku 2011 (Zhan et al. 2012), but in these cases, the tectonic setting is quite different from that of the Northern Chile margin. For the Maule 2010 earthquake in Central South Chile, the events occurred under an accretionary margin that generates a large frontal prism that probably controls the updip limit of the interplate seismicity (Moscoso et al. 2011; Cubas et al. 2013; Maksymowicz et al. 2015). On the other hand, the Northeast Japanese area, where the Tohoku earthquake occurred has been recognized as an erosive margin (von Huene and Culotta 1989) with several heterogeneities in the subducting plate that could have been involved in the diversity of aftershocks observed in the deeper area of the rupture zone (Asano et al. 2011; Zhan et al. 2012).

In order to quantify this problem, we use the permanent and temporary network to relocate and estimate the focal mechanism of more than 150 events with magnitude larger than Mw 4.5. The high quality of the seismic and geodetic data obtained for this earthquake provided detailed information about the complex rupture process of this large subduction earthquake. These events include foreshocks and aftershocks that took place from 1 March to 31 July 2014. Then, we compare the distribution of foreshocks and aftershocks and discuss the tectonic context in which they occurred. Finally, we relate the seismicity to the rheological conditions of the Nazca and South American convergent margin.

2 The Iquique earthquake and its precursors

Northern Chile has been considered as a soon to break gap since the studies by Kelleher (1972); McCann et al. (1979), and Nishenko (1985). The last mega-earthquake occurred in this area on 9 May 1877 (see Fig. 1a). This event generated a large tsunami that flooded all the ports from Arica to Antofagasta and further south. More detailed studies of this event were provided by Montessus de Ballore (1912), Kausel (1986), and Comte and Pardo (1991). The region around Iquique has had a somewhat rare but non negligible seismicity in the twentieth century, including earthquakes in 1911 (M 7.1), 1933 (Mw 7.6), 1940 (mb 7.10) 1967 (Mw 7.4), 1995 (Mw 8.0), and 2007 (Mw 7.8). All these events are listed by Pacheco and Sykes (1992) and Urrutia and Lanza (1993), and appear in the centennial catalog of Engdahl and Villaseñor (2002) (see Fig. 1b). A few more magnitude 7 events before 1970 are listed by Comte and Pardo (1991). Activity at intermediate depth in Northern Chile was continuous with more than 30 events listed by Engdahl and Villaseñor (2002) (see Fig. 1b). In 2005, a large earthquake of Mw 7.7 took place under the town of Pica, located 115 km to the East of Iquique, in the forearc of the Andes mountain range in the Tarapaca Region (see Fig. 1b). This event usually referred to as the Tarapaca intermediate depth earthquake was well recorded by local GPS and far field seismic data (Peyrat et al. 2006).

In 2006, the IPOC network was installed in Northern Chile to survey the seismicity of the gap. On 14 November 2007, an earthquake of Mw 7.8 occurred near Tocopilla (Peyrat et al. 2010). A few months later, an event of magnitude 6.4 occurred near Iquique on 12 March 2008. Activity in this area increased steadily after that event, with events larger than M 6 in 2009, 2010, and 2014 (see Fig. 1b). After 2013 recurrent seismicity, sometimes swarms of small events occurred offshore Iquique, midway between the continent and the trench. More details about those early “precursors” can be found in the papers by Hayes et al. (2014), Kato and Nakagawa (2014), Ruiz et al. (2014), Schurr et al. (2014), Yagi et al. (2014), Meng et al. (2015). Although details of the activity vary among these different studies, it is clear that a vast area about 50 km wide located to the east of the trench was very active between 2008 and 1 April 2014 when the main Mw 8.1 Iquique event occurred.

3 Data and methods

The IPOC network in Northern Chile was created by a consortium of the Universities of Chile, the GFZ of Germany, and IPGP in France and was installed progressively starting from 2006. The network consists of 20 sites with broadband seismometers, accelerometers, and double frequency GPS receivers. After the large precursor of 16 March 2014, the IPOC network was extended by a temporary seismic network deployed by National Seismological Center (CSN). Installation started a few days before the mainshock and finished 2 weeks after the April 1, 2014, Iquique earthquake. Figure 1a shows the location of the broadband instruments used in this work and the time at which they were installed before or after the mainshock. All the stations shown in Fig. 1a recorded continuously in time with a sampling rate of 100 Hz.

We use these data to locate and compute the centroid and depth of the moment tensor for the foreshocks and aftershocks. We initially created a catalog with events of magnitude greater than Ml 4.5 extracted from the CSN catalog, which for this zone and period is complete starting from magnitude Ml ∼4.0 (see Fig. 1 on Electronic Supplementary Material). The events were relocated using the arrival time of P and S waves hand-picked from all available traces with a visually good signal-to-noise ratio. The events were relocated using the Nonlinloc software (Lomax et al. 2000). We used the seismic velocity model proposed by Husen et al. (1999), who determined it for a region located about 200 km south of the present study area.

In Fig. 2, we compare the relocated events with the locations listed in the CSN catalogue for foreshocks and aftershocks. Figures 2 and 3 on Electronic Supplementary Material show the error bars for the relocated events. Our locations were improved with respect to those by CSN thanks to the much denser network of instruments which includes the temporary stations. As shown by Fuenzalida et al. (2013), locations determined using hand-picked arrivals are more accurate than those that use automatic picking because of the difficulty of automatic reading of head waves. However, the depths determined by phase picking have a high degree of uncertainty which can be improved by calculating the Regional Moment Tensor.
Fig. 2

Foreshocks and aftershocks of the 2014 Iquique earthquake. Foreshocks (diamonds) and aftershocks (circles) located using the NonLinLoc software (red symbols) compared with locations in the CSN catalogue (blue symbols). a Map view. The stars correspond to the epicenters of the main events of the Iquique sequence. b, c Vertical profiles along lines A-B and C-D corresponding to the in-depth projection of the events. The segmented black line represents the seismogenic contact proposed by Hayes et al (2012)

Once the earthquakes were relocated, we computed the regional moment tensor using the programs in Computer Programs in Seismology package (CPS) (Herrmann 2013). For this purpose, the epicenter location was fixed and we searched for the centroid depth and the best fitting double-couple source mechanism. This was done by a grid search: For each possible depth, we tested all possible double-couples and kept those that minimized the variance between observed and simulated traces. The final depth was the one that best fits the data. All available data were filtered between 0.02 and 0.06 Hz, which, after several tests, proved to be the best frequency range to model events with magnitude between Mw 4.5 and 6.5. For the computation of synthetic seismograms, we used the same velocity model as for the localization (Husen et al. 1999) (see Figs. 3 and 4).
Fig. 3

Determination of moment tensor for a large aftershock of the 1 April 2014 earthquake. On the top, comparison between focal mechanisms solutions for the April 4, 2014 at 01:37:50 Mw 6.0 event, with hypocenter −20.61°–70.74° and 28-km depth, obtained by a this work, b USGS, and c GFZ. d Fit curve for the solution of this work. e Synthetic (blue) and observed (red) waveforms for the stations used in this event

Fig. 4

Comparison between focal mechanism solutions for the aftershock of April 15, 2014 at 16:21:16. An event of Mw 5.0 with hypocenter −20.20°, −70.87°, and 8-km depth. Mechanisms obtained by a this work, b USGS, and c GFZ. d Fit curve for the solution of this work. e Synthetic (blue) and observed (red) waveforms for the stations used in this event

In order to validate our obtained moment tensors, we compared them with the solutions proposed by GFZ and USGS (see Figs. 4, 5, 6, 7, 8, 9, 10, 11, 12, and 13 on Electronic Supplementary Material). For the majority of the events, the MT depths present a better agreement with the slab model proposed by Hayes et al. (2012). The agreement is even better for the aftershocks, when the temporary network was in full operation. For the focal mechanisms, we obtained a fit better than 0.7 and good correlation between observed and synthetic waveforms. Figures 3 and 4 show some examples of the fits between the synthetic and real data and the comparison of our proposed focal mechanism with GFZ and USGS solutions.

4 Results

In our database, we identified two kinds of events: interplate thrust events and crustal events located on the overriding South American plate. For the classification, we considered the centroid depth with respect to the plate interface defined by the model of Hayes et al. (2012) and the focal mechanism of each event. The proposed interplate thrust events have reverse focal mechanisms, with one focal plane close to the dip of subduction zone. It is possible, however, that the actual focal plane of some events was the steeper one if the event was located within the Nazca or South American plate.

The crustal events were identified mainly from their locations, above the seismogenic contact. In general, these events show reverse mechanism, with a rotated strike with respect to the trench. Finally, a significant number of events have locations or focal mechanisms that do not permit us to clearly fit them in this classification. These events were left as unclassified and corresponds to normal or rotated interplate events. Figure 5 presents an example of observed data for the three kinds of events identified in this work.
Fig. 5

Three events in the foreshock and aftershock series of the 1 April 2014 Iquique earthquake. a Map view of three selected events. bd Observed data for the PSGCX station for an intraslab (red), an interplate (blue), and an unclassified (gray) event, respectively

Figure 6 shows the location and focal mechanism of the March foreshock sequence. This period is similar to that observed by Ruiz et al. (2014), who determined focal mechanisms for the foreshocks that occurred after 16 March 2014. Those events were computed using the permanent network plus a few temporary stations installed during this period (see Fig. 1a). For this time span, we observe crustal (upper-plate) events and interplate events and some unclassified—rotated interplate, rare strike angle—earthquakes. The seismicity shows a time migration to the north for about 40 km from 20° S to 20.4° S, toward the location of the epicenter of the Mw 8.1 main event (Ruiz et al. 2014). The strike angle of these events is mainly oriented northwest to southeast for the interplate events, with a more diverse orientation for the other events, as shown in the inset of Fig. 6a. An interesting feature observed in the foreshock distribution is that the dip angle of the interplate seismicity is larger than the dip of the subducted slab. This high angle of rupture is clearly observed in the shallower events (see Fig. 6b).
Fig. 6

Foreshocks with magnitude greater than Mw 4.5 of the 2014 Iquique earthquake. We interpret the blue focal mechanism as interplate events, red focal mechanism as crustal events inside the upper plate, and the gray focal mechanism as events we could not classify. a Map view of foreshocks. The stars correspond to the epicenters of the main events of the Iquique sequence, and the gray segmented line shows the selection width in the AB profile presented in Fig. 1b. The inset correspond to the strike angle, and the color is related with each type of event. b Profile showing the distribution as a function of depth of the foreshocks, the segmented line correspond to seismogenic zone proposed by Hayes et al. (2012). The focal mechanism of the Mw 6.7 event is that proposed by Ruiz et al. (2014)

Figure 7 shows the location and focal mechanism of the aftershocks from April 1 to July 31, 2014. The aftershock sequence does not present a clear migration as was observed during the foreshocks (Ruiz et al. 2014). We observe fewer crustal events with magnitude greater than Mw 4.5 in comparison with the precursory events. We identified only five crustal events, four of them located outside of the foreshock area. The aftershocks show a clear concentration of events with magnitude greater than Mw 4.5 close to the trench. Most of these events are located in the first 50 km from the trench to the coast, in good agreement with the proposed depth of the slab geometry, as shown in Fig. 7b. Similar to the observed tendency in the foreshocks, the strike angle of the interplate events is mainly oriented northwest to southeast, while the other events present a more diverse orientation (see inset in Fig. 7a). Moreover, as with the foreshocks, the dip of the interplate aftershocks is steeper than the seismogenic contact; with angles between 10° and 50°, this feature becomes even more evident for the events located ∼50 km landward from the trench (see Fig. 7a, b).
Fig. 7

Aftershocks of the 2014 Iquique earthquake with magnitude greater than Mw 4.5. Similar to Fig. 6, we interpret the blue focal mechanisms as interplate events, red focal mechanism as crustal events, and the gray focal mechanism as events we could not classify. a Map view of the aftershocks. The stars correspond to the epicenters of the main events of the Iquique sequence, and the gray segmented lines show the selection width for the AB and BC profiles projected in Fig. 2b, c. The inset corresponds to the strike angle, and the color is related with each type of event. b, c Profiles showing the distribution as a function of depth of the aftershocks, the segmented line, correspond to the seismogenic zone proposed by Hayes et al. (2012)

5 Discussion and conclusions

The event distribution shown in Fig. 7 presents a clear pattern with respect to the boundaries of the slip distribution of the two largest earthquakes of the Iquique sequence and the low coupling zones identified by Métois et al. (2013) (see Fig. 8 in this document and Fig. 14 on Electronic Supplementary Material). Figure 8 presents the distribution of interplate thrust events and the slip distribution of the Mw 8.1 and Mw 7.6 Iquique earthquakes proposed by Ruiz et al. (2014). In general, the events are distributed to the southwest the rupture zone surrounding the trench-ward boundary of the maximum coseismic slip. A similar situation has been observed in other interplate subduction earthquakes, such as Maule 2010 (Mw 8.8) and Tohoku 2011 (Mw 9.0) (Asano et al. 2011; Agurto et al. 2012), where the larger aftershocks surround the maximum slip of the rupture zone, confirming previous observations of Das and Henry (2003).
Fig. 8

Map view showing the slip distribution of the Mw 8.1 Iquique earthquake and its largest aftershock of magnitude Mw 7.6 (Ruiz et al. 2014) and the interplate aftershocks from Fig. 9. The stars are the epicenters of the main earthquakes of the Iquique sequence. The aftershocks clearly surround the rupture zone of the mainshock

The most obvious difference with Maule and Tohoku is that the Iquique foreshocks and aftershocks were concentrated on the shallow interplate interface, westward of the maximum slip area, reaching closer to the trench. We propose that the distribution of foreshocks and aftershocks is not only related to the slip distribution of the mainshock, but it is also related to the rheological conditions and the tectonics of the subduction margin. As we noted earlier, the majority of foreshocks and aftershocks of the 2014 Iquique earthquake (Figs. 6 and 7) are concentrated westward of the main rupture zone, closer to the trench. In the case of Maule 2010 Mw 8.8, the number of aftershocks with large magnitude decreased toward the trench in the two segments where the largest slip was located; this can be related to a decrease of effective basal friction below a wide accretionary prism (Moscoso et al. 2011; Cubas et al. 2013; Maksymowicz et al. 2015). In contrast, in the Iquique sequence which is located in an erosive segment of the Chilean margin (Ranero et al. 2006; Contreras Reyes et al. 2012), the largest Mw 4.5 aftershocks are observed in the shallower area of the contact zone. This may be explained by the lack of a large accretionary prism.

If the subducted Nazca Plate, below the accretionary prism, has similar features to those observed seaward from the trench—an irregular bathymetry with horst and graben structures that have more than 2000 m offset—it is likely that these structures control the location and focal mechanism of events of magnitude larger than Mw 4.5. Projecting the profile obtained by von Huene and Ranero (2003) to the west of the Mejillones Peninsula, we observe an irregular contact for about 50 km from the trench to the east (see Fig. 9). After this shallow zone, the number of large magnitude aftershocks decreases, which could be caused by a smoother contact generated by tectonic erosion in the shallow portion of the subducted plate. The strike angles of interplate events are in good agreement with the NW orientation of the horst and graben structures of the subducted Nazca Plate. A similar hypothesis was proposed by Zhan et al. (2012) for the 2011 Tohoku earthquake.
Fig. 9

Schematic profile of the Northern Chile subduction zone (∼20° S). The diamonds and circles correspond to the computed centroid of the foreshocks and aftershocks with magnitude greater than Mw 4.5, respectively. a, b corresponds to profiles AB and CD shown in Fig. 7a. The segmented red line corresponds to our interpretation of the irregularities in the Nazca Plate proposed by von Huene and Ranero (2003). The segmented black line shows our proposition for the seismogenic contact in Northern Chile in comparison with that proposed by Hayes et al. (2012) shown by the gray segmented line. Solid black line, in profiles AB and CD, represents the estimated in-depth rupture of the mainshock and largest aftershock, respectively. Vertical exaggeration 2:1

Assuming that the main features of the erosive Northern Chile margin remain similar, we can interpret our results with reference to two marine seismic profiles located in Antofagasta (∼22.5° S) and Tocopilla (∼22° S) (Ranero et al. 2006; Contreras Reyes et al. 2012). This allows us to relate the characteristics of the Iquique sequence with the main features observed in the seismic profiles (see Fig. 9): lack of sediments in the trench, a small frontal accretionary prism, and an eroded continental wedge of about 50 km width associated to relatively low P wave velocity that presents pervasive fracturing with high-angle landward-vergent faults. Both foreshocks and aftershocks located here present a strong correlation with the tectonic units of the continental plate. The interplate seismicity stops near the trench where the small frontal accretionary wedge probably inhibits fast seismic ruptures. The shallow interplate seismicity is concentrated below the eroded continental wedge, extending close to 50 km landward from the trench. In this part of the subduction zone, tectonic erosion at the base of the continental wedge seems to be the first-order deformation process. Furthermore, the transition between the shallow interplate events and the less numerous events located in the deeper contact—as well as the updip limit of the rupture of the mainshock—roughly coincides with the landward limit of the eroded wedge, which can be explained by the strong decrease of basal and internal friction due to the fracturing and fluids content in the eroded wedge. Likewise, the crustal events in the upper plate (like the foreshock of March 16) are also located near the landward limit of the eroded wedge. Their high angle reverse fault mechanism suggests that the limit of the eroded wedge can work as a reverse fault and/or that the landward vergent normal faults present in the erosive wedge can be reactivated as reverse faults as the main rupture approaches.

Finally, we observe that the seismogenic contact for South America proposed by Hayes et al. (2012) was used as a reference for this work. There are some problems in the shallower contact zone, similar to those observed in Southern Chile (Maksymowicz et al. 2015). In order to better take into account the distribution of the shallower interplate events, we modified the seismogenic contact in Fig. 9 and propose that in the shallower zone, the dip angle is close to 10°, compared with the value between 15° and 20° of the slab 1.0 model of Hayes et al. (2012). This is similar to what was observed by Contreras Reyes et al. (2012) in the seismic profile at 22° S. On the other hand, the angle of the deeper interplate contact events shows a subduction angle in good agreement with the values from Hayes et al. (2012) and Contreras Reyes et al. (2012). The abrupt change in the subduction dip angle suggests very strong slab bending forces in this zone.

In summary, we computed the location and moment tensor of 151 foreshocks and aftershocks of the Iquique 2014 earthquake. The analyzed events are concentrated in a band of about 50 km to the east from the trench. The obtained solutions for the moment tensor showed a very good adjustment for most of the waveforms giving us better constrained depths which are critical for a correct interpretation of the tectonic structures observed in the scope area. Moreover, the fault plane solutions for the aftershocks present a better fit than that obtained for the foreshocks, showing the importance of having a dense local network to compute the regional moment tensor.

We propose that the distribution of the observed seismicity may be controlled by the irregularities in the contact between the subduting Nazca Plate and South American plate. This behavior, with a large diversity of events, is apparently a common characteristic for erosive margins due to the lack of sediments. In contrast, the accretionary margins add fluids and sediments to the subducting plate filling the heterogeneities and creating a “smoother” interplate contact that could generate less diversity of earthquakes. Furthermore, an important number of crustal events in the South American plate are a sign of the complexities related with the subduction process in Northern Chile and how the extreme erosive margin in that area affect the overriding plate creating fractured zones with the capacity of potentially generating a large tsunamigenic earthquake. Finally, we propose the presence of a slab bending that could be responsible of the abrupt change in the dip angle of the seismogenic contact.



We thank the support of the Chilean National Science Foundation project FONDECYT No. 11130230 and Programa Riesgo Sísmico (AIN, Universidad de Chile). A.M was supported by project FONDECYT 3150160. We thank Centro Sismológico Nacional ( and IPOC consortium for making raw data available to us.

Supplementary material

10950_2016_9568_MOESM1_ESM.doc (6.5 mb)
ESM 1(DOC 6611 kb)


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Copyright information

© Springer Science+Business Media Dordrecht 2016

Authors and Affiliations

  • Sergio León-Ríos
    • 1
  • Sergio Ruiz
    • 1
  • Andrei Maksymowicz
    • 1
  • Felipe Leyton
    • 2
  • Amaya Fuenzalida
    • 3
  • Raúl Madariaga
    • 4
  1. 1.Departamento de Geofísica, Facultad de Ciencias Físicas y MatemáticasUniversidad de ChileSantiagoChile
  2. 2.Centro Sismológico Nacional, Facultad de Ciencias Físicas y MatemáticasUniversidad de ChileSantiagoChile
  3. 3.School of Environmental SciencesUniversity of LiverpoolLiverpoolUK
  4. 4.Laboratoire de GeologieUMR8538 CNRS Ecole Normale SuperieureParisFrance

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