1 2 Geochemistry, Geophysics, Geosystems 3 Supporting Information for 4 Varying styles of magmatic strain accommodation in the East African Rift 5 James D. Muirhead1, Simon A. Kattenhorn1,2, Nicolas Le Corvec3 6 7 8 1. Department of Geological Sciences, University of Idaho, Moscow, Idaho 83844, USA 2. ConocoPhillips Company, Houston, Texas 77079, USA 3. Lunar and Planetary Institute, Houston, Texas 77058, USA 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 Contents of the supporting material 25 26 27 28 29 Additional Supporting Information (Files uploaded separately) 30 Introduction 31 32 33 34 35 36 37 38 The supplementary text provides a detailed description of our methods for determining cone lineaments, vent alignments and cone groupings, and a brief review of physical processes driving local modifications of the remote stress field. We provide 4 supporting figures illustrating our methods, 1 showing radial patterns in South Natron and Arusha using a moving average analysis, and 2 figures of 2-D elastic models illustrating tectonomagmatic processes controlling local stress perturbations. The 4 tables provided (additional supporting information) summarize all data used in this study. These tables are available as Excel spreadsheets. Text S1. Stress fields induced by pressurized magma chambers. Text S2. Stress rotations induced by mechanical interactions between rift segments. Text S3. Observational methods: deducing cone lineaments. Text S4. Analytical methods: creation of vent alignments. Text S5. Defining cone field boundaries in the North Tanzanian Divergence and Kenya Rift. Text S6. Cone fields in the North Tanzanian Divergence and Kenya Rift. Figure S1. Two-dimensional elastic models of a pressurized hole in an elastic plate. Figure S2. Moving average analyses of dike trends in the South Natron and Arusha fields. Figure S3. Two-dimensional elastic model of interacting rift segments. Figure S4. Classification of cone morphologies used to determine cone lineaments. Figure S5. Schematic demonstration of the criteria for defining vent alignments. Figure S6. Cone groupings in the North Tanzanian Divergence. Figure S7. Cone groupings in the North Tanzanian Divergence and Kenya Rift. Table S1. Locations and lineament trends produced by volcanic cones in this study. Table S2. Vent alignment locations and orientations. Table S3. Fault locations, lengths and orientations. Table S4. Focal mechanism data for the North Tanzanian Divergence. 1 39 Text S1. Stress fields induced by pressurized magma chambers 40 The stress conditions involved in the generation of radial dike patterns may be 41 modeled in two-dimensions as a pressurized hole in an elastic body subject to a biaxial 42 remote stress field [Muller and Pollard, 1977; Baer and Reches, 1991; Koenig and 43 Pollard, 1998]. Some modeling studies also include additional stress sources, such as 44 an overlying volcanic load [e.g., Pinel and Juapart, 2003; Hurwitz et al., 2009; Le Corvec 45 et al., 2015]. The presence of a pressurized hole, or magma chamber, perturbs the local 46 stress field (Fig. S1). This perturbation results in a radial stress pattern, where the 47 greatest compressive stress (σ1) rotates around the chamber such that the strike of σ 1 48 everywhere converges on the center of the chamber. The magnitude of this local stress 49 perturbation is dependent on magma chamber radius (R), internal magma pressure (P) 50 and the remote differential stress (σ11- σ22) (Fig. S1a). If R and P remain constant, the 51 magnitude of the stress perturbation decreases with increasing differential stress values 52 (Figure S1b-d). 53 This study describes a number of radial dike patterns in the East African Rift 54 (EAR), possibly reflecting these modeled effects. Figure S2 shows a moving average 55 analysis of the radial dike swarms in the North Tanzanian Divergence. Note the change 56 in the mean orientations in the NE, SE, SW and NW sectors around the Oldoinyo Lengai 57 and Meru volcanoes. Around Meru, dikes in the NE and SW sectors exhibit ~NE-SW 58 striking trends, whereas dikes in the NW and SE sectors exhibit ~NW-SE trends, 59 indicative of a radial pattern. This radial trend prevails for cone lineaments both near the 60 volcano (<25 km from the volcano summit), as well as those as far as 40 km from the 61 summit. Radial swarms may also be differentiated using the method of maximum 62 intersections (Ancochea et al. 2008), shown in Figures 6 and 7 of the main text. 63 64 Text S2. Stress rotations induced by mechanical interactions between rift 65 segments 66 Field, analog, and numerical modeling studies show that the lateral growth of en- 67 echelon structural segments, whether joints, faults, dikes or rifts, is accompanied by 68 stress interactions between adjacent segments [Pollard and Aydin, 1984]. In some 69 instances, these stress interactions may cause the lateral ends of segments to rotate, 70 forming two interlocking hooks (Pollard et al., 1982; Olson and Pollard, 1991; Thomas 71 and Pollard, 1993; Tentler, 2003; Koehn et al., 2008). The interaction zone where these 72 rotations occur is located in the area between segment ends (Fig. S3b and c) [Pollard 2 73 and Aydin, 1984]. This behavior is inferred to be scale-invariant, occurring in brittle 74 material over at least 11 orders of magnitude in length scale, from micro-cracks to mid- 75 ocean ridge or continental rift segments [Pollard and Aydin, 1984; Tentler, 2003; Koehn 76 et al., 2010]. The size of these interaction zones thus scales with the size of the 77 interacting structural segments. 78 these interaction zones will be on the order of 10-1 to 100 m2 [Pollard et al., 1982; Pollard 79 and Aydin, 1984]. For continental rift basins 100s of km in length, such as the EAR, 80 these interaction zones, commonly termed transfer zones, may occupy areas of 102 to 81 103 km2 [Ebinger, 1989; Koenh et al., 2010; Corti, 2012]. For macro-scale fractures tens of meters in length, 82 En echelon structural segments in extensional settings may be modeled in two- 83 dimensions as two offset slits (mode I fractures) in an elastic medium subject to remote 84 tensile stresses acting normal to the slit walls [Pollard and Aydin, 1984; Gudmundsson, 85 1995] (Fig. S3a). Early-stage continental rift segments have been modeled previously 86 as underlapping segments [Pollard and Aydin, 1984] (Fig. S3a and b), as would be 87 appropriate for the Natron and Pangani basins shown in Figure S3c. High stress 88 concentrations form at the tips of mode I fractures subjected to an external tensile stress 89 field [Olson and Pollard, 1989]. In the case of two offset fracture or rift segments, stress 90 fields generated at the respective segment tips interact and locally reorient the principal 91 stress directions [Pollard and Aydin, 1984; 92 reorientation causes fracture segments to divert from their original propagation paths, 93 and in some instances form the characteristic interlocking hook shapes between 94 segment ends [Pollard et al., 1982; Tentler, 2003]. For the two underlapping, left- 95 stepping segments modeled in Fig. S3b, the interaction between segments results in a 96 counter-clockwise rotation of the horizontal principal stresses. The dike and fault 97 orientations observed in the interaction zone (transfer zone) between the left-stepping 98 Natron and Pangani rift segments (Fig. S3c) are consistent with this modeled interaction 99 and resulting stress rotation. A similar counter-clockwise stress rotation is inferred for the 100 Rwenzori transfer zone between the left-stepping Lake Albert and Lake Edward rift 101 basins of the EAR, based on fault kinematic and numerical modeling data [Koehn et al., 102 2008, 2010]. This type of stress modification in the interaction zone between segments 103 has been described in a number of studies as a “mechanical interaction” between 104 rift/fracture segments [Pollard et al., 1982; Pollard and Aydin, 1984; Olsen and Pollard, 105 1991; Crider and Pollard, 1998]; hence, we adopt the same terminology in this work. Gudmundsson 1995]. This stress 106 3 107 Text S3. Observational methods: deducing cone lineaments 108 Monogenetic volcanic cones were mapped using aerial photography (0.5 m 109 resolution) and Google Earth satellite imagery (1-2 m resolution), supplemented by 110 published maps [Roberts, 2002; Dawson, 2008; Wauthier, 2011; Smets et al., 2014] (see 111 Table S1). Following Paulsen and Wilson [2010], the idealized shapes (circular to 112 elliptical) of cones and craters were determined and each cone was classified as a cone, 113 cleft cone, linear fissure, or crater (Fig. S4). As the resolution of the imagery (0.5-2.0 m) 114 is an order of magnitude greater than the typical dimensions of the monogenetic cones 115 (30-1000 m radii), the reliability of the cone morphology is not affected by image 116 resolution. The reliability of the shape of each cone was nonetheless ranked (1 = 117 probable; 2 = likely; 3 = unknown) depending on the degree of observable erosion and 118 the likelihood that the cone morphology was affected by wind direction rather than a 119 possible dike-feeder. The cone was considered to produce a lineament if it had a 120 reliability ranking of 1 or 2 and a cone or crater axial ratio (long axis to short axis) >1.2, 121 which is the minimum ratio required to define lineaments from Paulsen and Wilson 122 [2010]. If these criteria were met, the trend of the long axis of the cone was recorded and 123 interpreted to mimic the dike that fed the cone [Tibaldi, 1995; Korme et al., 1997; Bonali 124 et al., 2011]. If both the cone base and cone crater exhibited an axial ratio >1.2, the long 125 axis direction of the crater was used in the analysis. In addition to using cone and crater 126 elongations, the breaching direction (Fig. 4 of main text) was used as a direct indicator of 127 feeder dike orientation [i.e., Tibaldi, 1995], as well as the strike of volcanic fissures (Fig. 128 S4). Throughout this paper these features are described as cone lineaments, and are 129 inferred to reflect the strike of the dike that fed the volcanic cone (Fig. S4). 130 131 Text S4. Analytical methods: creation of vent alignments 132 In addition to identifying cone lineaments, alignment analyses were performed on 133 groups of 3 cones using the linear regression algorithm and MATLAB script of Le Corvec 134 et al. [2013]. For these analyses, each alignment must satisfy a certain “width” and 135 “length” tolerance (Fig. S5). For our analyses, a width tolerance of 50 m was used, which 136 is within the width tolerance for “A grade” alignments of Paulsen and Wilson [2010] (125 137 m). The length tolerance of the alignment depended on the observed distribution of 138 cones within each field, where the mean distance between cones within the alignment 139 had to be less than the expected mean distance between cones from a Poisson 140 distribution (Table 1). 4 141 Following Paulsen and Wilson [2010], the reliability of each alignment was then 142 verified by assessing cone lineaments produced by cones present within each alignment 143 (Fig. S5). In this case, there must be a cone present within the alignment that has a cone 144 lineament trend within 15˚ of the alignment trend for the alignment to be considered for 145 our analysis. As such, each vent alignment satisfied the reliability criteria for vent 146 alignments defined by Paulsen and Wilson [2010]. In our study, if these criteria were 147 met, the trend of the alignment was recorded, and any cones present within the 148 alignment that did not exhibit a cone lineament trend (i.e. have an axial ratio <1.2 and/or 149 a reliability rating of 3) were ascribed a cone lineament trend that matched the 150 alignment. Alignments analyzed in each field are outlined in Supplementary Table S2. 151 Throughout this paper, these features are described as vent alignments and are distinct 152 from cone lineaments, as they represent a structural alignment between 3 points [e.g., 153 Le Corvec et al., 2013] rather than the orientation of a feeder dike below a single cone 154 [e.g., Bonalli et al., 2011]. 155 156 Text S5. Defining cone field boundaries in the North Tanzanian Divergence and 157 Kenya Rift 158 Boundaries delineating cone fields analyzed in the North Tanzanian Divergence 159 and Kenya Rift in this study have not been previously specified, in part due to an 160 incomplete catalog of geochemical data and ages for most cones. Similar problems 161 occur in the EAR as a result of sparse geochemical sampling [e.g., Main Ethiopian Rift: 162 Mazzarini, 2007], as well as in cone fields elsewhere [e,g., Baja California, Mexico: 163 Germa et al., 2013]. Monogenetic fields are, therefore, often grouped using statistical 164 methods, such as agglomerative hierarchical clustering [Mazzarini, 2004; Mazzarini et 165 al., 2013] or kernel density estimations [Connor and Connor, 2009; Germa et al., 2013]. 166 Volcanic cone groupings in the North Tanzanian Divergence in this study did not depend 167 solely on density estimations (Figs. S6 and S7). This is because the distribution of cones 168 appears to be affected by large volcanic edifices (composite volcanoes) and areas of 169 high sediment input, possibly creating artificial clusters. For example, a distinct scarcity 170 of cones was observed in the 1.2 Ma Engaruka (sub-)basin (Fig. S6a); cones erupted 171 into this depression are likely buried by rapidly accumulating sediments in the subsiding 172 basin. Dikes intersecting volcanic edifices are also more likely to erupt on the lower 173 flanks rather than the volcano summit and, in these instances, cones may form clusters 5 174 on the lower flanks of volcanoes [Pinel et al., 2004; Gaffney and Damjanac, 2006; 175 Kervyn et al., 2009] (Fig. S7a). 176 As our analysis addressed the variability in cone lineament and vent alignment 177 data across different structural locations in the North Tanzanian Divergence and Kenya 178 Rift, we chose to approximate boundaries based on general rift structure and the spatial 179 distribution of vents (Figs. S6 and S7). Cones within the defined groups exhibit distinct 180 trends that align locally with fault structures (Fig. 5 of main text), and we therefore 181 consider that dividing up vent groups based on basin structure is appropriate for our 182 analyses. 183 184 Text S6. Cone fields in the North Tanzanian Divergence and Kenya Rift 185 The sections of the North Tanzanian Divergence and Kenya Rift analyzed in our study 186 were divided into 6 cone fields: Naivasha-Nakuru, Natron-Magadi, South Natron, 187 Arusha, Ngorongoro Volcanic Highlands, and Kilimanjaro (Figs. S6 and S7; Fig. 5 of 188 main text). The Natron-Magadi field was delineated based on a distinct lack (n=19) of 189 monogenetic cones over a ~130 km-long section from Gelai volcano in the south to 190 Suswa volcano in the north (Fig. S7a). North of the Natron-Magadi field are volcanic 191 cones of the Naivasha-Nakuru field. The Naivasha-Nakuru basin represents a distinct 192 magmatic-tectonic province (Kenya peralkaline province) of the Kenya Rift [MacDonald 193 and Baginski, 2009], comprising a series of actively deforming composite volcanoes and 194 silicic centers (e.g., Suswa, Longonot, Menegai) [Biggs et al., 2009]. The transition from 195 the Natron-Magadi field north into the Naivasha-Nakuru field is marked by an increase in 196 the number of cones (n=118) north of Suswa volcano, which exhibit significant clustering 197 in the center of the field (Fig. S7b). The South Natron field (cluster 1 in Fig. S6b) has a 198 greater number of cones (n=267) and extends rift-parallel across the southernmost ~40 199 km of the Natron Basin into the northernmost ~10 km of the Ngorongoro-Kilimanjaro 200 Volcanic Belt. 201 orientations (029° and 011° mean strike, respectively), and also align sub-parallel with 202 the orientation of the 2007 Natron dike (027° strike: Calais et al., 2008). It also contains 203 a unique group of cones with a mean ESE-WNW trend that, on closer inspection, forms 204 a sub-radial pattern (section 4.2 of main text). A small group of cones (n=15) ~50 km 205 southwest of the South Natron field exhibit a NE-SW cone lineament trend, and form the 206 Ngorongoro Volcanic Highlands field (cluster 2 in Fig. S6b). East of this field are three 207 clusters of cones (clusters 3, 4 and 5 in Fig. S6b), all of which exhibit a NW-SE trend Here, cone lineaments and faults exhibit primarily spreading-normal 6 208 and are surrounded by NW-SE trending faults. Based on the similar structural trends 209 observed in these clusters, they have been grouped into a single cone field, called the 210 Arusha field. The final cone field delineated in this study is the Kilimanjaro field (clusters 211 6 and 7 in Fig. S6b). This field consists of cones on or around the flanks of Kilimanjaro 212 volcano. These cones exhibit a NW-SE cone lineament trend. Unlike the Arusha field, no 213 faults are identifiable in Google Earth imagery in the Kilimanjaro field. 7 214 Spporting figure captions 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 Figure S1. Two-dimensional elastic models of a pressurized hole (magma chamber) in an elastic plate, modified from Koenig and Pollard [1998]. A: Idealization of the model setup. Pink circle represents the pressurized hole (magma chamber) with radius, R, and internal pressure, P. The hole is subject to remote biaxial loading from a least (σ 22) and greatest (σ11) compressive stress. θ and r indicate the polar coordinate system, the origin of which is located at the center of the hole. B-D: Calculated stress trajectories resulting from a pressurized magma chamber. Black ticks at each grid point represent the local orientation of σ1. In each example, internal magma pressure (100 MPa) and chamber diameter (normalized to 1) are held constant, while the remote stress difference is varied from 2 to 10 to 20 MPa in B, C and D, respectively. Analytical solutions for these models are provided in Koenig and Pollard [1998]. Figure S2. Moving average analyses of dike trends in the South Natron and Arusha fields. The analysis was performed in ArcGIS v. 10.3 and involves non-overlapping neighborhoods (2.5 x 2.5 km in size) and a search radius of 6 km. Neighborhoods colored blue contain cone lineaments with mean strike values in NE and SW quadrants (i.e., 000-090° and 180-270°, respectively). Neighborhoods colored red contain cone lineaments with mean strike values in SE and NW quadrants (i.e., 090-180° and 270360°, respectively). A: Moving average analysis of cone lineaments in the Arusha field for neighborhoods within 40 km of the summit of Meru volcano. B: Same analysis as in A, except that only neighborhoods within 25 km of the summit are presented. C: Analysis of mean strike values of cones in the South Natron field for neighborhoods within 22 km of the summit of Oldoinyo Lengai. Note that in each analysis the mean orientations of cone lineaments varies depending on the position around the volcano. Cones in NE and SW quadrants also show ca. NE-SW striking lineaments. Those in SE and NW quadrants exhibit ca. SE-NW striking lineaments. These geometries are consistent with a radial pattern. Figure S3. Two-dimensional elastic model of interacting rift segments, modified from Pollard and Aydin [1984]. A: Geometry and boundary conditions for two rift segments subject to orthogonal extension. The model considers rift segment length (2b), segment spacing (2k) and segment separation (2s). The remote tectonic stress (tensile) normal to the rift is σr11 and α represents the angle between the rift segment ends with respect to the strike of the rift. B: Contour map of maximum shear stress ((σ1 – σ2)/2) and stress orientations (black ticks represent the orientation of the greatest compressive stress) for left-stepping, underlapping rift segments (α = 45°) subject to far-field tension. Stress magnitudes are normalized to the ambient shear stress. The highest stress occurs near the segment tips and within the interaction zone between the rift segments (dashed box), where the orientations of the principal stresses are locally rotated in a counter-clockwise sense. Analytical solutions applied in this model are provided in Pollard and Aydin [1984]. C: Example of underlapping, left-stepping rift segments in the North Tanzanian Divergence. Dike (grey rose plots) and fault data (black rose plot) are from this study. 8 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 These data show a counter-clockwise rotation of the principal stresses away from the regional stress field, consistent with the model results in B. Figure S4. Example images from Google Earth representing the classification of cone morphologies used to determine cone lineaments from the Virunga Province (A and D), Boset segment (B), and South Natron (C). Double-sided arrows show the orientation of the cone lineaments for each cone based on fissure orientation (A), crater elongation (B & C), and breaching direction (D). Figure S5. Schematic demonstration of the criteria for defining vent alignments, modified from Le Corvec et al. [2013]. The alignment represented by the black line (i) is accepted for analysis because it contains a cone with a lineament trend that has an angular deviation <15˚ from the trend of the alignment. The red alignments are rejected on the basis that they have no cone with a reliable lineament (ii) or, alternatively, have a cone with a lineament that is >15˚ to the trend of the vent alignment (iii). Figure S6. A: Distribution of monogenetic cones in the North Tanzanian Divergence shown on an Aster DEM hillshade map. Note how the cones are largely absent near the summits of stratovolcanoes (transparent purple) and in the Engaruka Basin (transparent brown). B: Kernel density plots of North Tanzanian Divergence cones performed in Arc GIS v.10 using a 15 km search radius. Rose plots are of fault segment and cone lineament trends in the 7 computed clusters. NVH corresponds to Ngorongoro Volcanic Highlands. Figure S7. 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