Bulletin of the Seismological Society of America, Vol. 104, No. 3, pp. 1100–1110, June 2014, doi: 10.1785/0120130222 Ⓔ Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone by P. Martin, P. Arroucau, and G. Vlahovic Abstract This study investigates crustal anisotropy in the New Madrid Seismic Zone (NMSZ) by analyzing shear-wave splitting measurements from local earthquake data. In addition to the waveforms provided by the Center for Earthquake Research and Information (CERI) for over 3000 events, seismograms recorded by the portable array for numerical data acquisition (PANDA) network were obtained for over 800 events. Data reduction led to a final data set of 168 and 43 events from the CERI and PANDA data, respectively. One-hundred and eighty-six pairs of measurements were produced from the CERI data set by means of the automated shear-wave splitting measurement program mfast and 49 from the PANDA data set. Two dominant directions, respectively striking northeast–southwest and west-northwest–east-southeast, are identified and interpreted to be due to stress-aligned microcracks. The northeast–southwest polarization direction is consistent with the maximum horizontal stress orientation of the region and has previously been observed in the NMSZ, whereas the west-northwest–east-southeast polarization direction has not. Path-normalized time delays range from 1 to 33 ms=km for the CERI network data and 2 to 31 ms=km for the PANDA data. These results produce a range of estimated differential shear-wave anisotropy between 1% and 8%. These values are higher than those previously determined in the region. The majority of large path-normalized time delays (> 20 ms=km) are located along the Reelfoot fault segment. These high values are believed to be indicative of high crack densities and high pore fluid pressures, which agrees with previous results from local earthquake tomography and microseismic swarm analysis. Online Material: Tables of stations, events, and associated shear-wave splitting measurements. Introduction The New Madrid Seismic Zone (NMSZ) is an active intraplate seismic zone centrally located in the United States, spanning portions of western Tennessee, northeastern Arkansas, and southeastern Missouri (Fig. 1a). With over 5000 recorded earthquakes since 1974 (Center for Earthquake Research and Information [CERI], New Madrid catalog), the NMSZ has the highest level of seismicity in the United States east of the Rocky Mountains (Hamilton and Johnston, 1990). Although small magnitude (M < 4) seismic events are currently dominant in the region, the NMSZ is also the location in which three of the largest known earthquakes that took place in the contiguous United States (magnitude > 7), occurred during the winter of 1811–1812 (Johnston, 1996). There are four major segments of seismicity in the NMSZ (Fig. 1a). The two segments that trend northeast to north-northeast appear as almost vertical, dextral strike-slip faults (Vlahovic et al., 2000). The longest of these two segments outlines the Axial fault (AF), whereas the shorter segment in the north outlines portions of the Western Rift Margin (WM). These two segments are connected via the 60 km central segment trending northwest, where the seismic activity is located along planes dipping between 30° and 50° SW (Himes et al., 1998; Vlahovic et al., 2000). This central segment is associated with the Reelfoot fault (RF), in which the largest concentration of the seismic activity occurs in the region (Himes et al., 1998). The fourth segment of seismicity trends west-northwest and is loosely spatially associated with the Grand River Tectonic Zone (GRTZ). Although there exists some seismicity near the eastern Rift Margin faults (EM), there is not an appreciable amount for it to be considered a dominant source. The large-magnitude earthquakes that occurred in 1811– 1812 caused extensive damage in the region, and if similar magnitude events were to occur today, the local population and infrastructure would be at risk. The possibility of such a catastrophic scenario has made the NMSZ the focus of many 1100 Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone 1101 Figure 1. (a) Map of faults and seismicity in the New Madrid Seismic Zone (NMSZ). Earthquake epicenters (white circles) in the NMSZ from 1974 to present (provided by Center for Earthquake Research and Information [CERI] New Madrid catalog), with the large events of 1811–1812 shown as solid black circles (location from National Earthquake Information Center [NEIC] catalog of significant historical events). Regional faults shown from Csontos and Van Arsdale (2008), including the Reelfoot fault (RF), Axial fault (AF), western Rift Margin fault (WM), and the Grand River tectonic zone (GRTZ). Other faults include Osceola fault zone (OFZ), Bolivar-Mansfield tectonic zone (BMTZ), central Missouri tectonic zone (CMTZ), and the eastern Rift Margin faults (EM). Rift margin faults (EM and WM) outline the Reelfoot rift. (b) Simplified movements (thin arrows) along faults in NMSZ derived from Johnston (1996). Large arrows indicate direction of maximum horizontal compressional stress within the NMSZ (Zoback and Zoback, 1991; Hurd and Zoback, 2012). studies investigating possible mechanisms for seismicity in the region. Some proposed mechanisms favor activation of faults in the NMSZ by regional stresses, specifically the North American stress field (Zoback and Zoback, 1991; Frankel et al., 2012; Hurd and Zoback, 2012) (see Fig. 1b); faults that are favorably oriented with respect to the northeast–southwest regional stress field (Zoback and Zoback, 1980; Heidbach et al., 2008) are activated by the buildup of stress over time, without the need for local anomalous behavior. Recent interpretations of Global Positioning System (GPS) measurements in the region (Frankel et al., 2012) are in agreement with this scenario, in which the motion between GPS stations that crossed the Reelfoot fault was found to be on the order of 0:37 mm=year. Motions of this magnitude agree with an ∼4 mm=year interseismic slip at 12–20 km depth, which if constant through time could produce the necessary slip for M 7.3 earthquake along the shallow Reelfoot fault with an occurrence rate of 500 years. This would produce the necessary occurrence intervals of larger earthquakes in the NMSZ of 500 (300) years, as proposed by Tuttle et al. (2002). Other interpretations of GPS measurements in the NMSZ only give surface velocities along faults a magnitude of 0:2 mm=year (Calais and Stein, 2009). If steady-state stress accumulation was the only driving force of horizontal movement along faults in the NMSZ, velocities of 0:2 mm=year would require a minimum of 10,000 years to repeat a magnitude 7 earthquake and a minimum of 100,000 years to repeat a magnitude 8 (Calais and Stein, 2009). These slip rates would therefore not satisfy the recurrence intervals of 500 (300) years that were proposed by Tuttle et al. (2002). In this scenario, mech- anisms for activation of faults in the NMSZ must include local stress concentrations or anomalous behavior of the lithosphere. Such mechanisms have been proposed, including flexure uplift leading to the unclamping of faults due to sediment removal (Calais et al., 2010) or creep at depth promoted by the abundance of quartz, fluid overpressure conditions, and the associated shear strain loading (Powell et al., 2010). This study seeks to further investigate any indications of local anomalous behavior in stress and fluid pressure within the NMSZ, by studying the phenomenon known as shear-wave splitting through the analysis of local earthquake data. Anisotropy and Shear-Wave Splitting Anisotropy is the term that characterizes directional dependence within a given medium; this includes seismic anisotropy, which is manifested by the dependence of velocity on propagation direction. Although there are various sources of seismic anisotropy, the common cause in the upper crust results from the opening and extension of fluidfilled cracks known as extensive-dilatancy anisotropy (EDA) cracks (Crampin and Atkinson, 1985). When microcracks are the cause of anisotropy, the fast component of the split shear wave is polarized parallel to the preferential orientation of the cracks, which in turn lay parallel to the direction of maximum stress. This results in a measured fast polarization direction (ϕ) that is therefore directly related to the direction of maximum stress. The measurement of time delay of slow shear wave (δt) in the case of microcracks is directly related to the density, ε, and geometric properties of EDA cracks 1102 P. Martin, P. Arroucau, and G. Vlahovic through the relationship ε Na3 =ν, with N representing the number of cracks and a as the crack radius, within a volume, ν (Crampin, 1994). The information gathered through shear-wave splitting measurements can then be used to estimate the percentage of differential shear-wave velocity anisotropy (SWVA), defined by Crampin (1989) as min V max S1 − V S2 ; max V S1 x100 1 in which V S1 and V S2 are the velocities of the fast and slow components of the split shear wave, respectively. For most intact rocks, regardless of rock type, SWVA ranges between 1.5% and 4.5%, which is equivalent to crack densities on the order of 0.015–0.045 (roughly 0:001 × SWVA) (Crampin, 1994). By measuring shear-wave splitting in the upper crust of the NMSZ, properties of stress on both the local and regional scale can be resolved. The dominant fast polarization measurements provide information about the orientation of the microcracks in the crust, which gives insight into the direction of maximum compressional stress in the area. Possible deviations from expected alignment of fast polarization directions and regional stress can be interpreted as due to local stress perturbation or more complex anisotropic fabric. Previous study of shear-wave splitting in the NMSZ by Rowlands et al. (1993) showed that the dominant stress direction was parallel to the regional maximum compressional stress. The authors also concluded that there was no evidence for anomalous distribution of microcracks within the NMSZ and therefore no anomalous local stress environment. Although the results from Rowlands et al. (1993) support mechanisms that favor regional stress as an activation source for seismicity in the NMSZ, the data that the authors analyzed only spanned 3 years (October 1989–June 1991), a time period that may have been too short to capture all the complexity of the stress field in the NMSZ. This study attempts to provide a more complete analysis of shear-wave splitting in the NMSZ, by combining both the data set used in Rowlands et al. (1993) and a data set spanning the time period of 2003–2011, with events being reported by the CERI, Saint Louis University Earthquake Center, and contributions from Southeastern U.S. Seismic Networks (SEUSSN) bulletins (see Data and Resources). Methods Shear-wave splitting measurements in this study were made using the automated program mfast developed by Savage et al. (2010). The program will not be discussed in detail here, but readers are directed to the works of Silver and Chan (1991), Teanby et al. (2004), and Savage et al. (2010). The mfast program relies on the grid-search algorithm from Silver and Chan (1991) to make the initial measurements of (ϕ, δt). The grid search is used to find an inverse operator (which is a function of ϕ and δt) that removes the effects of splitting from the given seismic signal, which can be based on the linearity of the corrected signals particle motion (Silver and Chan, 1991). In order to quantify the linearity, this automated method calculates the covariance matrix between the orthogonal components of the corrected signal. The presence of anisotropy in a signal is represented by the eigenvalues of this matrix. When no anisotropy is present, there should be only one eigenvalue that is non-zero. In the real world, however, where there is always noise, there will be a second non-zero eigenvalue. Therefore, the lower the value of this second eigenvalue, the more the effects of shearwave splitting have been removed from the signal. Thus, the grid search is used to search all possible values of ϕ and δt in a given measurement window, looking for the solution that gives the lowest second eigenvalue. This is done for many measurement windows, and the ϕ and δt measurements that gave the lowest second eigenvalue are stored as the solution for each individual window. The solutions from the grid search are then used in conjunction with the cluster analysis developed in Teanby et al. (2004) to determine the final values and apply grading criteria. Any events that are not rejected by the grading criteria are checked for null measurements. The event is considered null if the difference between incoming and fast polarization falls below 20° or above 70°. It is then assumed that either there is no anisotropy present or that initial shear wave is polarized along the fast polarization direction. Similarly, anomalously high time delay measurements can imply cycle skipping or noisy data (Evans et al., 2006). Therefore any time delay measurements, that is 0.8 times a given maximum δt measurement are also considered null, in which the max δt measurement in this study is 1.0 s as suggested by Savage et al. (2010). An example of a completed measurement can be seen in Figure 2. Two separate data sets were used in this study. The larger data set of 3603 earthquakes spans the time period of 2003–2011, with events being reported by the CERI, Saint Louis University Earthquake Center, and contributions from SEUSSN bulletins. The second data set of 899 earthquakes was collected by the portable array for numerical data acquisition (PANDA) network from October 1989 to June 1991 (Chiu et al., 1992), which was previously analyzed in the study by Rowlands et al. (1993). For an event to provide an accurate shear-wave splitting measurement it must fall within the shear-wave window of at least one seismic station, in which the shear-wave window is defined by all incidence angles less than a critical angle for a given event. This requirement results from distortion that occurs when a shear wave arrives at the free-surface interface, such as the conversion of S to P waves resultant from reflection or the creation of a P wave that is inhomogeneous (Booth and Crampin, 1985). Therefore, the ability to clearly read a shear wave on a seismogram recorded at the surface is directly related to the incident angle of the wave (Booth and Crampin, 1985). Uncertainty in velocity models as well as earthquake locations have led to the use of the apparent incident angle (ia ) as described by equation (2) (Rowlands et al., 1993). Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone 1103 Figure 2. Example of output from mfast program obtained in this study. Visual and numeric output of the mfast program: (a) seismic event shown on all three components of the station DLAR, the event window shown in gray. (b) Horizontal components of seismogram before (top two traces) and after correction (bottom two traces). The first two dotted lines represent the times in which measurement windows can start, and the last two dotted lines represent the times in which measurement windows can end. The window used for this measurement is shown in gray. (c) Plot of measurement results from 80 measurement windows, with the best measurement denoted by the X (note that it is located within a stable region). (d) Plot of clusters from the cluster analysis, the X denotes the best cluster. (e) Waveforms before and after correction for δt in both time domain and particle motion plot. Note the similar waveforms in the time domain and the linearity of the corrected particle motion plot. (f) Contour plot of the grid search for all measurements, through the final measurement window. The minimum value is denoted by the X. (g) Information about the station, event, and measurement window selection. (h) Results including the final measurements for ϕ, which is given here in degrees from north, and δt. The color version of this figure is available only in the electronic edition. 1104 P. Martin, P. Arroucau, and G. Vlahovic Figure 3. Locations of all 185 seismic events (gray dots) used in this study from CERI data set. Only seismic stations that had at least one event fall within their shear-wave window were used in this study shown here by black triangles. ia tan−1 e ; d Figure 4. Locations of all 49 seismic events (gray dots) used in this study from the portable array for numerical data acquisition (PANDA) data set. Only seismic stations that had at least one event fall within their shear-wave window were used in this study shown here by black triangles. 2 in which e is the distance to the epicenter, and d is the earthquake depth. In this study, events from either data set must have their apparent incident angle ia ≤ 35° at least at one station as suggested by Rowlands et al. (1993). Events for use from the CERI data set were subject to further restrictions, such that the event must have a standard horizontal error ≤ 2:5 km and a standard error on depth ≤ 5:0 km; and each event must have a magnitude of 2 or greater. Events for use from the PANDA data set required the same location accuracy; however, most events had a very low magnitude (M < 0:1), so no magnitude threshold was applied. Because of the large difference in magnitudes and to preserve the integrity of both data sets, they were analyzed separately. There were 1160 events from the CERI data set and 504 events from the PANDA data set that met the quality criteria discussed above. There were 681 events from the CERI data and 329 from the PANDA data set, eliminated either due to a low signal-to-noise ratio (SNR) or an inability to distinguish the S-phase pick accurately. Thus, 479 pairs of (ϕ, δt) measurements were made from the remaining CERI events, 288 of which were defined as nulls in the mfast program. Similarly, 175 measurements were made with the remaining PANDA events, in which 111 of these measurements were defined as nulls. Data reductions continued with an additional loss of 30 events from the CERI and 15 from PANDA due to the quality requirement that only measurements with quality B (mfast criteria: SNR > 3, standard deviation of ϕ < 25) or greater be used. The final CERI data set contained a total of 186 pairs of measurements, in which the events used ranged in magnitude from 2.0 to 4.6 and depths from 3.8 to 23.7 km. The final PANDA data set contained a total of 49 pairs of measurements, with magnitudes of 0.0 and depths ranging from 3.2 to 15.3 km. The locations of these events are plotted in Figures 3 and 4, along with the stations that had at least one event fall within their shear-wave window. Ⓔ Tables S1 and S2, which include station, event, and measurement information for both the CERI and PANDA data sets, are available in the electronic supplement to this article. Results The results from the shear-wave splitting analysis of the CERI data set indicate two dominant fast polarization directions: northeast–southwest as well as west-northwest–eastsoutheast. These polarization directions can be seen plotted in Figure 5a–h. The northeast–southwest fast polarization direction has been identified before in the shear-wave splitting study of Rowlands et al. (1993). They attributed this polarization to vertical EDA cracks aligned in the direction of the proposed regional maximum horizontal stress (Zoback and Zoback, 1991; Hurd and Zoback, 2012). The northeast–southwest polarization direction is seen strongly at stations MARM, WALK, and WYBT (Fig. 5a–h). The west-northwest–east-southeast polarization direction is seen strongly at stations CATM, NMDM, and LEPT (Fig. 5a–h). The west-northwest–east-southeast fast polarization direction is found throughout the NMSZ (Fig. 5h) and has not been identified by any previous shear-wave splitting studies in the region. Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone 1105 Figure 5. (a) Rectangles outline stations and earthquakes from CERI data set, grouped into zones 1, 2, and 3. (b) Enlargement of zone 1. Equal area plots show fast polarization directions for a given event (shown as lines), plotted by azimuth and distance in respect to the station’s location (triangle in center), segmented ring indicates shear-wave window of 35° and outer ring at 40°. Dashed lines connect equal area projection plots with station locations. (c) Enlargement of zone 1. Radial histograms (rose diagrams) indicate fast polarization directions measured at each station. The width of each bin is equivalent to 10°, north indicated at top. Each segmented ring within the rose diagram represents a frequency increment of two events. The dashed line indicates station location. (d) Enlargement of zone 2. Equal area plots indicate fast polarization directions. (e) Enlargement of zone 2. Radial histograms (rose diagrams) indicate fast polarization directions measured at each station. (f) Enlargement of zone 3. Equal area plots indicate fast polarization directions. (g) Enlargement of zone 3. Radial histograms (rose diagrams) indicate fast polarization directions measured at each station. (h) Radial histogram (rose diagram) of all measured fast polarization directions from the CERI data set. The width of each bin is equivalent to 10°, north indicated at top. Each segmented ring within the rose diagram represents a frequency increment of five events. The most frequent (northeast–southwest) fast polarization direction as well as the secondary west-northwest–east-southeast direction are clearly visible. Gray arrows indicate direction of maximum horizontal compressional stress within the NMSZ (Zoback and Zoback, 1991; Hurd and Zoback, 2012). 1106 P. Martin, P. Arroucau, and G. Vlahovic Figure 6. (a) Enlargement of zone 1 (see Fig. 5a). Time delays for a given event are shown as scaled circles inside the equal area projection, plotted by azimuth and distance in respect to the station location (triangle in center), segmented ring indicates shear-wave window of 35° and outer ring at 40°. The dashed line indicates station location. (b) Enlargement of zone 2. Time delays for a given event are shown as scaled circles inside the equal area projection, plotted by azimuth and distance in respect to the station’s location (triangle in center), segmented ring indicates shear-wave window of 35° and outer ring at 40°. The dashed line indicates station location. (c) Enlargement of zone 3. Time delays for a given event are shown as scaled circles inside the equal area projection, plotted by azimuth and distance in respect to the station’s location. Our results indicate a wide range of path-normalized time delays. The path-normalized time delays are calculated by dividing each time delay by the length of its associated travel path δt=l, which results in values ranging from 1 to 33 ms=km. As noted by Rowlands et al. (1993), actual pathnormalized time delays could be even larger if the thick top layers of sediments in the Mississippi embayment were considered isotropic, which would reduce the effective path length in the anisotropic medium, thus increasing the pathnormalized time delays. Stations GRAT, LEPT, and RDGT surround a cluster of the largest time delays in the section of southern Reelfoot. Detailed results for these stations can be seen in Figure 6a–c. It is important to note that path-normalized time delays larger than 20 ms=km in this study have an associated event depth range between 5 and 10 km (Fig. 7). The short-effective path length due to shallow event depths in the southern Reel- foot region coupled with the large time delays measured there suggest a high density of EDA cracks and a higher percent of SWVA, possibly due to the presence of high pore fluid pressure. There is also a possibility that this behavior results from the confinement of EDA anisotropy to above 10 km depth. This is consistent with the results from the Bisrat et al. (2012) study of swarm activity in the southern Reelfoot region between 1995 and 2008. Their study identified the Ridgley swarm area as the most active swarm region in the NMSZ and attributed it to changes in pore fluid pressure within highly fractured basement rock. The locations of large time delays in this study are also consistent with prominent low-velocity anomalies from Powell et al. (2010). In their study, Powell et al. (2010) describe the velocity anomalies that occur in the northern portion of the Reelfoot fault as caused by variations in rock composition. However, they attribute the velocity anomalies located in the central as well as the southern Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone Figure 7. Path-normalized time delays plotted against event depth for the CERI and PANDA data sets. Reelfoot fault section to fluid-saturated, highly fractured crust. In the central Reelfoot fault segment where low V P values are found, the low V S velocity anomalies are even more pronounced. This suggests that the resultant high V P =V S ratio is consistent with high pore pressure and fluid-filled, smallaspect ratio cracks. In the southern Reelfoot fault segment, the low V P velocity anomalies are of smaller magnitude than the low V S velocity anomalies. Therefore, Powell et al. (2010) concluded that the resultant low V P =V S value was due to the existence of high aspect ratio, fluid-filled cracks. Results from the PANDA data set are similar to those from the CERI data, including northeast–southwest dominant fast polarization direction and a second, less dominant west-northwest–east-southeast polarization direction (see Fig. 8a,b). Path-normalized time delays range from 2 to 31 ms=km, with a cluster of large delays concentrated in the southern Reelfoot fault segment, analogous to the results from the CERI data analysis (Fig. 9). The larger path-normalized time delays from the PANDA data are not located as far south as those from the CERI analysis but are still within the area where the presence of high pore fluid pressure is indicated by other studies (Powell et al., 2010; Bisrat et al., 2012). Discussion The majority of fast polarization directions found in this study were northeast–southwest oriented, which is consistent with the dominant fast polarization direction identified by Rowlands et al. (1993) in their shear-wave splitting study and is coincident to North American stress field (see Zoback and Zoback, 1980; Heidbach et al., 2008). Both of these results are attributed to EDA cracks polarized in the direction of maximum horizontal compressional stress within the NMSZ (Zoback and Zoback, 1991; Hurd and Zoback, 2012). The second dominant fast polarization direction found in this 1107 study is west-northwest–east-southeast, which was not identified by Rowlands et al. (1993). The widespread distribution of this secondary fast polarization direction throughout the NMSZ suggests that it is not due to a local change in maximum horizontal stress. Fast polarization directions offset up to 90° from the direction of the crack strike are possible in cases of shallow-dipping or intersecting fracture systems (Rial et al., 2005). Thus, geometry of upper crustal anisotropy in NMSZ may be more complex than vertical EDA cracks. Similarly, the distribution of the secondary westnorthwest–east-southeast fast polarization gives no evidence of an association with any local igneous intrusions or plutons in the region (Hildenbrand, 1985; Hildenbrand and Hendricks, 1995), which suggests that there is no local buildup of stresses that occurs around their boundaries. For example, the polarization directions measured closest to the large Bloomifield pluton (located north-northeast of the Reelfoot fault; Hildenbrand and Hendricks, 1995) exhibit similar directions to polarizations measured along the AF where more felsic intrusions are believed to exist (Johnston and Schweig, 1996). The existence of a secondary dominant fast polarization direction, significantly offset from the direction of regional maximum horizontal compressive stress, has been observed before in other fault zones. For example, Zhang et al. (2007) observed fast polarization directions recorded at stations near the San Andreas fault that were parallel or subparallel to the strike of the fault (northwest–southeast) and significantly offset from north-northeast–southsouthwest fast polarizations that were suggested to be due to the direction of regional maximum horizontal compressive stress. The polarization directions oriented along the strike of the fault were concluded to be due to the shear fabric in the fault region. Another possible mechanism for two dominant fast polarization directions can be a change of anisotropy with depth (Winterstein and Meadows, 1991). Results of our study show no indication of a relationship between depth and fast polarization directions (Fig. 10). Path-normalized time delays found in this study were assumed to be caused by EDA cracks and ranged from 1 to 33 ms=km. The measured time delays in this study are assumed to be the result of EDA cracks within the shallow crust. This assumption allows the path-normalized time delays combined with the average shear-wave velocity along the travel path, to be related to crack densities in the region. This relationship can be shown with a (unit-less) apparent crack density, calculated by δt ; ε υS l 3 in which ε is the apparent crack density, υS is the shear velocity in the uncracked medium, and δt=l is the path-normalized time delay (O’Connell and Budiansky, 1974; Hudson, 1981). The value for υS in this study was estimated using a weighted average of the S velocities for all layers in the velocity model of Chiu et al. (1992) along the straight ray 1108 P. Martin, P. Arroucau, and G. Vlahovic Figure 8. (a) Enlargement of PANDA station locations. Equal area plots indicate fast polarization directions for a given event (shown as lines), plotted by azimuth and distance in respect to the station’s location (triangle in center). Segmented ring indicates shear-wave window of 35° and outer ring at 40°. The dashed line indicates station location. (b) Enlargement of PANDA station locations. Radial histograms (rose diagrams) indicate fast polarization directions measured at each station. The width of each bin is equivalent to 10°, north indicated at top. Each segmented ring within the rose diagram represents a frequency increment of two events. The dashed line indicates station location. Figure 10. Fast polarization directions plotted against depth for CERI data set. Figure 9. Enlargement of PANDA station locations. Time delays for a given event are shown as scaled circles inside the equal area projection, plotted by azimuth and distance in respect to the station’s location (triangle in center), segmented ring indicates shear-wave window of 35° and outer ring at 40°. The dashed line indicates station location. path for each event. The resulting average velocities are considered a conservative estimate, however, as the low S velocity (0:6 km=s) in the upper layer of sediments was included in the calculation. A hundredth of the percentage of SWVA (see equation 1) is considered to be the approximate value of the crack density (Crampin, 1994), allowing the estimate of SWVA through; SWVA εx100. This in turn gives estimated differential shear-wave anisotropy between 1% and 8%. These values are higher than those from the previous shearwave splitting study by Rowlands et al. (1993), in which path-normalized time delays ranged from 1.4 to 14:6 ms=km, with anisotropy on the order of 4%. Large time delays found in this study were concentrated in the southern Reelfoot segment. The large time delays could be explained by the existence of elevated pore fluid pressure and are consistent with the results of Bisrat et al. (2012), in which swarm activity in this area was attributed to changes in pore fluid pressure within highly fractured basement rock. Similarly, Shear-Wave Splitting Study of Crustal Anisotropy in the New Madrid Seismic Zone Powell et al. (2010) attribute the P- and S-velocity anomalies that they identified in the same location of the southern Reelfoot fault section to a fluid-saturated volume, with a saturating medium of meteoric water or gas. Hurd and Zoback (2012) concluded that the existence of elevated pore fluid pressure, or local changes in stress, was not needed to explain the faulting within the NMSZ. Instead their study showed that faults in the NMSZ are favorably oriented for slip in the east-northeast–west-southwest compressive stress field. If this is the case, then the existence of high pore fluid pressure in the Reelfoot region as indicated by this study, Bisrat et al. (2012), and Powell et al. (2010), would only help facilitate slip in the region. Conclusion In this work, we performed and analyzed shear-wave splitting measurements from a total of 235 seismic events that occurred within the NMSZ, recorded by the PANDA network (Chiu et al., 1992) from the years 1989–1991 and by the CERI from the years 2003 to 2011. The anisotropy detected by the split waves is assumed to be due to EDA cracks in the shallow crust. The results have shown two dominant fast polarization directions throughout the NMSZ. The most frequent northeast–southwest fast polarization direction is consistent with EDA cracks oriented in the direction of maximum horizontal compressional stress within the NMSZ. The source of the secondary west-northwest–east-southeast fast polarization direction may be, among others, shallow-dipping EDA cracks, two intersecting fracture systems, or pervasive shear fabric within the NMSZ. The path-normalized time delay measurements exhibit a wide range, from 1 to 33 ms=km, with a cluster of large time delays occurring in the lower portion of the southern Reelfoot section. The large time delays are believed to be due to elevated pore fluid pressure within volumes of highly fractured basement rock. These findings agree with previous results from local earthquake tomography (Powell et al., 2010) and microseismic swarm analysis (Bisrat et al., 2012) and present a possible mechanism for the facilitation of slip in the region. There are many things that could be done in future work to improve our understanding of the NMSZ through shear-wave splitting from local earthquakes. This includes increasing the density of stations in the region, as well as possible tomographic inversions using time delays. Such an inversion could aid in understanding the precise location where the splitting occurred, which is a limitation of the study presented here. Data and Resources A portion of the seismic data in this study was reported by Center for Earthquake Research and Information (CERI), Saint Louis University Earthquake Center, and contributions from Southeastern U.S. Seismic Networks (SEUSSN) bulletins, at http://www.ceri.memphis.edu/seismic/catalogs/cat _nm.html (last accessed January 2012). A portion of the seis- 1109 mic data used in this study was collected by the portable array for numerical data acquisition (PANDA) network from October 1989–June 1991 (Chiu et al., 1992). Acknowledgments We would like to acknowledge the Center for Earthquake Research and Information as well as Mitch Withers for making data available and Christine Powell for sharing her insight into the New Madrid Seismic Zone. We also acknowledge Jer-Ming Chiu for making the portable array for numerical data acquisition data available. We would like to thank Associate Editor Anton Dainty and the two anonymous reviewers whose suggestions made this a better paper. This study was in part supported by the National Science Foundation under Grant Number HRD-0833184 and National Aeronautics and Space Administration under Award NNX09AV07A. Any opinions, findings, and conclusions or recommendations expressed in this presentation are those of the authors and do not necessarily reflect the views of the funding agencies. References Bisrat, S., H. R. DeShon, and C. Rowe (2012). Microseismic swarm activity in the New Madrid Seismic Zone, Bull. Seismol. Soc. Am. 102, 1167–1178. Booth, D. C., and S. 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