Journal of African Earth Sciences 102 (2015) 70–85 Contents lists available at ScienceDirect Journal of African Earth Sciences journal homepage: www.elsevier.com/locate/jafrearsci Fracturing of doleritic intrusions and associated contact zones: Implications for fluid flow in volcanic basins Kim Senger a,b,c,⇑, Simon J. Buckley a, Luc Chevallier d, Åke Fagereng e,1, Olivier Galland f, Tobias H. Kurz a, Kei Ogata b,2, Sverre Planke g,h, Jan Tveranger a a Centre for Integrated Petroleum Research, Uni Research, Allégaten 41, 5007 Bergen, Norway Department of Arctic Geology, University Centre in Svalbard, P.O. Box 156, 9171 Longyearbyen, Norway Department of Earth Science, University of Bergen, Allégaten 41, 5007 Bergen, Norway d Council for Geosciences, 3 Oos Street, 7535 Bellville, South Africa e Department of Geological Sciences, University of Cape Town, 13 University Avenue, 7701 Rondebosch, South Africa f Physics of Geological Processes (PGP), Department of Geosciences, University of Oslo, Postboks 1047, Blindern, 0316 Oslo, Norway g Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Postboks 1028, Blindern, 0315 Oslo, Norway h Volcanic Basin Petroleum Research AS, Oslo Innovation Center, Gaustadalléen 21, 0349 Oslo, Norway b c a r t i c l e i n f o Article history: Received 31 January 2014 Received in revised form 29 October 2014 Accepted 31 October 2014 Available online 21 November 2014 Keywords: Karoo Igneous intrusions Fluid flow Fracturing Permeability Dolerite a b s t r a c t Igneous intrusions act as both carriers and barriers to subsurface fluid flow and are therefore expected to significantly influence the distribution and migration of groundwater and hydrocarbons in volcanic basins. Given the low matrix permeability of igneous rocks, the effective permeability in- and around intrusions is intimately linked to the characteristics of their associated fracture networks. Natural fracturing is caused by numerous processes including magma cooling, thermal contraction, magma emplacement and mechanical disturbance of the host rock. Fracturing may be locally enhanced along intrusion–host rock interfaces, at dyke–sill junctions, or at the base of curving sills, thereby potentially enhancing permeability associated with these features. In order to improve our understanding of fractures associated with intrusive bodies emplaced in sedimentary host rocks, we have investigated a series of outcrops from the Karoo Basin of the Eastern Cape province of South Africa, where the siliciclastic Burgersdorp Formation has been intruded by various intrusions (thin dykes, mid-sized sheet intrusions and thick sills) belonging to the Karoo dolerite. We present a quantified analysis of fracturing in- and around these igneous intrusions based on five outcrops at three individual study sites, utilizing a combination of field data, high-resolution lidar virtual outcrop models and image processing. Our results show a significant difference between the three sites in terms of fracture orientation. The observed differences can be attributed to contrasting intrusion geometries, outcrop geometry (for lidar data) and tectonic setting. Two main fracture sets were identified in the dolerite at two of the sites, oriented parallel and perpendicular to the contact respectively. Fracture spacing was consistent between the three sites, and exhibits a higher degree of variation in the dolerites compared to the host rock. At one of the study sites, fracture frequency in the surrounding host rock increases slightly toward the intrusion at approximately 3 m from the contact. We conclude by presenting a conceptual fluid flow model, showing permeability enhancement and a high potential for fluid flow-channeling along the intrusion–host rock interfaces. Ó 2014 Elsevier Ltd. All rights reserved. 1. Introduction ⇑ Corresponding author at: Electromagnetic Geoservices ASA, Dronning Mauds gt. 15, 0250 Oslo, Norway. Tel.: +47 95291592. E-mail addresses: ksenger@emgs.com, senger.kim@gmail.com (K. Senger). 1 Present address: School of Earth & Ocean Sciences, Cardiff University, Park Place, CF10 3AT Cardiff, United Kingdom. 2 Present address: Dipartimento di Fisica e Scienze della Terra ‘Macedonio Melloni’, Università degli Studi di Parma, Campus Universitario – Parco Area delle Scienze 157/ A, I-43124 Parma, Italy. http://dx.doi.org/10.1016/j.jafrearsci.2014.10.019 1464-343X/Ó 2014 Elsevier Ltd. All rights reserved. The matrix of crystalline igneous rocks is typically tight, with sub-milliDarcy permeability (e.g., Sruoga et al., 2004) and primary porosity commonly less than 0.5–1% (e.g., Petford, 2003; van Wyk, 1963). Fractured igneous aquifers may nonetheless be considered as potential groundwater reservoirs (e.g., Gustafson and Krásný, 1994; Woodford and Chevallier, 2002) due to the presence of fracture networks, a characteristic feature of virtually all igneous 71 Ecca Grp Stormberg Grp B East London Port Elizabeth Main Karoo Basin boundary 100km B E L. Elliot Burgersdorp Katberg Nonesi’s neck L Permian Hillcrest Golden Valley 10km E L D Ecca Bonkola C C U. Elliot Molteno M D Karoo dolerites L Triassic Cape Fold Belt Cape Town Drakensberg Prince Albert Dwyka Beaufort Grp E Fm V V V V V V VV V V V VV V Gp V Dwyka Grp Stormberg Drakensberg Grp Beaufort VV V V V A Jurassic Prd K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 E Bonkola GV_W_1 GV_E_2 GV_E_3 GV_W_2 GV_E_4 GV_E_6 Nonesi’s neck GV_E_1 GV_W_3 GV_E_8 GV_E_7 Hillcrest 3km 3km Fig. 1. Location and geological setting of the study area. (A) Location of study area (black rectangle) superimposed on a simplified geological map of southern Africa, after Smith (1990) and Svensen et al. (2012). (B) Satellite image of the study area, illustrating the sills (dark red polygons) and dykes (bright red lines). Note the evident exposure of the saucer-shaped intrusions and the study area locations (yellow pins). (C) Close-up of the Golden Valley saucer-shaped sill, and the locations of the photo-mosaics (photographed rim segments and photograph location) presented in this study. (D) Close-up of the Queenstown area, with the three lidar scan sites marked. Refer to Table 1 for details. (E) Simplified stratigraphic column of the Karoo Supergroup, after Tankard et al. (2009). The star at 183 Ma indicates the timing of the Karoo dolerite emplacement (Svensen et al., 2012). All satellite images from Google Earth. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.) rocks. This dual nature of the permeability of igneous intrusions causes them to influence reservoir fluid flow in an apparently non-predictable manner, sometimes forming fully sealing, impermeable barriers (e.g., Gurba and Weber, 2001; Thomaz Filho et al., 2008), at other times high-permeability pathways (e.g., Mège and Rango, 2010; Sankaran et al., 2005), and sometimes both (e.g., Rateau et al., 2013; Stearns, 1942). The economic and societal consequences of improved understanding of fractured igneous aquifers is significant, with underexplored fractured igneous reservoirs, such as in the Argentinian 72 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 Table 1 List of studied localities. The locations are given in the WGS84 datum. Study site Latitude Longitude Bonkola N 31°470 18.7700 S 26°570 14.7000 E 0 00 0 00 Scan size (width * height) Igneous features Intrusion contact (dip dir/dip angle) Outcrop orientation Host rock 36 * 5 m 2 m thick dyke 110/75 057/237 Burgersdorp Fm. Burgersdorp Fm. Burgersdorp Fm. Burgersdorp Fm. Burgersdorp Fm. Burgersdorp Fm. Bonkola S 31°47 18.77 S 26°57 14.70 E 47 * 12 m 2 m thick dyke 119/63 057/237 Nonesi’s neck Hillcrest N 31°500 28.7000 S 26°590 24.5400 E 69 * 14 m 324/74 024 (curving) 31°530 25.2300 S 26°480 9.9600 E 110 * 13 m 256/36 293/113 0 5 m thick inclined intrusion >80 m wide inclined sheet >100 m wide inclined sheet 18 * 10 km saucershaped sill Poor exposure 293/113 N/A Variable 0 00 00 Hillcrest S 31°53 25.23 S 26°48 9.96 E 150 * 10 m Golden Valley 31°550 28.7000 S 26°170 5.8000 E No scan Neuquén Basin, hosting commercial quantities of hydrocarbons (e.g., Bermúdez and Delpino, 2008; Gudmundsson and Løtveit, 2012; Rodriguez Monreal et al., 2009; Schutter, 2003; Witte et al., 2012). Applied aspects of permeability associated with intrusions can be best illustrated by the regional-scale exploration for groundwater in the semi-arid Karoo Basin, which has focussed on identifying and mapping fracture zones yielding high flow (Chevallier et al., 2001; van Wyk, 1963). Extensive drilling and A Nonesi’s Neck injection tests (12 wells) across an inclined dolerite sheet at Qoqodala in the Eastern Cape province confirmed this fact, highlighting how the igneous body itself forms a barrier to fluid flow, whereas the intensely fractured lower dolerite–host rock interface channels groundwater flow along the contact (Chevallier et al., 2004). The influence of fractures on groundwater yields is undisputed, but many studies rely on fracture information from boreholes and regional lineament analyses from remote sensing. The Lidar Photograph on si tru . 5 m n i a c intrusion Que ens tow n R39 NND_ 6 B Hillcrest N 01 C Lidar Photograph Photograph blast marks interpreted fractures Lidar measuring tape scanline ‘virtual’ scanline Fig. 2. Outcrop photographs and screenshots of the virtual outcrops illustrating the level of detail and applicability for fracture measurements. (A) Nonesi’s neck. Car (circled) and intrusion (ca. 5 m thick) for scale. (B) Side-view of the Hillcrest N locality, illustrating the structural details of the virtual outcrop model. Field notebook (circled) and measuring tape for scale. (C) Detail of a blast mark at Hillcrest N. Measuring tape for scale. 73 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 Table 2 Summary of scanlines (Lidar, fieldwork and photo-mosaics) and structural stations, with corresponding fracture characteristics. Refer to Table 3 for additional details on virtual profiles. ID Data set Lithology Length (m) Number of fractures Fractures/meter (avg) Scanlines BD_01 BD_01L HC_01 HC_01L NND_01 NND_01P NND_02 Fieldwork Lidar Fieldwork Lidar Fieldwork Photo-mosaic Fieldwork Mixed Mixed Mixed Mixed Mixed Mixed Mixed 10 10.4 20 20 24 23.4 10 67 49 124 61 158 79 37 6.7 4.7 6.2 3.1 6.6 3.4 3.7 Structural stations Bonkola S Bonkola S Bonkola N Bonkola N Hillcrest S Hillcrest S Hillcrest N Hillcrest N Nonesi’s Neck Nonesi’s Neck Lidar Lidar Lidar Lidar Lidar Lidar Lidar Lidar Lidar Lidar Host rock Dolerite Host rock Dolerite Host rock Dolerite Host rock Dolerite Host rock Dolerite N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A 176 60 158 50 308 532 55 473 134 101 N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A number of detailed field-based studies of fractures in igneous rocks is relatively limited (e.g., Delaney et al., 1986; McCaffrey et al., 2003). Our study focusses on the fracture patterns in- and around doleritic intrusions within the Karoo Basin and presents new outcropscale fracture data from three sites in the Eastern Cape Province of South Africa. We acquired new data, combining both state-of-theart digital techniques, in particular lidar scanning (Buckley et al., 2008), and traditional field methods. Our objectives are two-fold. Firstly, we illustrate, assess and verify various methods of collecting fracture spacing and orientation data from igneous intrusions at different scales. Secondly, we apply this data set to investigate the fracture patterns at intrusion–host rock contacts, presenting a conceptual model for fracture-channeled permeability at intrusion–host rock contact zones. 2. Fracturing in igneous rocks The complexity of fracturing within and around igneous intrusions is partly related to the distinct formation mechanisms developing three main types of fractures: (1) emplacement-induced fractures in the host-rock, (2) post-emplacement fractures within the intrusion (i.e., cooling joints), and (3) non-intrusion related fractures (i.e., tectonic fractures) in both the intrusion and country rock. The first set of fractures occurs in the country rock (referred to as ‘syn-emplacement fractures’, SEF for short, in this contribution, and as ‘inflation fractures’ by Kattenhorn and Schaefer (2008)), and is induced by the emplacement of the intrusion. Because the magma is overpressured when it is emplaced (e.g., Lister and Kerr, 1991; Rubin, 1995), it triggers substantial damage in the country rock at both local (e.g., Abdelmalak et al., 2012; Delaney and Pollard, 1981; Delaney et al., 1986; Galland and Scheibert, 2013; Meriaux et al., 1999; Schofield et al., 2012a) and regional scale (e.g., Jackson and Pollard, 1990; Rubin and Pollard, 1988). Abdelmalak et al. (2012) show how the deformation pattern reflects the mechanism of emplacement of the magma intrusions. Quantitative detailed mapping of fracture patterns around intrusions, however, have rarely been carried out, and a proper understanding of the fracture pattern induced by magma intrusions in the country rock is lacking. The second set of fractures (referred to as ‘post-emplacement fractures’, ‘PEF’ for short, and as ‘cooling fractures’ by Kattenhorn and Schaefer (2008)) forms within the intrusion and is induced by post-emplacement processes, such as thermal contraction during cooling (e.g., Hetényi et al., 2012). The third set of fractures (referred to as ‘tectonic fractures’, TF for short) forms due to tectonic forces unrelated to the intrusion emplacement. Tectonic fractures may be present both in the intrusion (if tectonism post-dated the magma emplacement) and in the host rock (both pre- and post-emplacement). These three sets of fractures (i.e., ‘SEF’, ‘PEF’, and ‘TF’) are juxtaposed, and the way they interact and are connected is unknown. 3. Geological setting All studied localities exhibit dolerites of the Karoo large igneous province (e.g., Svensen et al., 2012 and references therein) emplaced into the Permo-Triassic siliciclastic Beaufort Group, which is part of the regional Karoo Supergroup (Fig. 1). Tectonically, the Karoo Basin is traditionally interpreted as a retro-arc foreland basin bounded by the Cape Fold Belt to the south (e.g., Johnson et al., 1996). The depositional history of the Karoo Supergroup is well covered in the published literature (e.g., Smith, 1990; Tankard et al., 2009) and only briefly summarized here. Deposition commenced during the Permo-Carboniferous with glacio-marine sedimentation (Dwyka Group), followed by shallow marine (Lower Ecca Group), deltaic (Upper Ecca Group) and fluvial/lacustrine (Beaufort Group) deposition (Smith, 1990). The Burgersdorp Formation, comprising the uppermost unit of the Beaufort Group and forming the host rock at the studied localities, consists of grayish-red and greenish-gray mudstone with subordinate fine-grained sandstone units (Hiller and Stavrakis, 1984). The top of the Burgersdorp Formation marks the base of the Stormberg Group, comprising, from the base upwards, perennial braid-plain deposits (Molteno Formation) overlain by continental red beds (Elliot Formation) and aeolian and playa deposits (Clarens Formation; Smith, 1990). The rapid emplacement of magma at ca. 183 Ma led to the formation of an extensive (ca. 367 000 km3 of magma) sill complex (Svensen et al., 2012). At that time, the associated lava complex, the Drakensberg Group, likely exceeded the 140 000 km2 remnant exposed today (Bristow and Saggerson, 1983; Smith, 1990). This volcanism effectively terminated deposition of the Karoo Supergroup and the resistant dolerites and basalts have protected the underlying sedimentary succession from denudation since the Early Jurassic. It thus offers a rare glimpse into a relatively undisturbed ancient intrusion–host rock complex 74 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 Table 3 Summary of virtual profiles with associated fracture parameters. Profile ID Locality Vertical/horizontal Lithology Length (m) High-resolution profiles B-S-1 Bonkola South B-S-2 Bonkola South B-S-3 Bonkola South B-S-4 Bonkola South B-S-5 Bonkola South B-S-6 Bonkola South B-N-1 Bonkola North B-N-2 Bonkola North B-N-3 Bonkola North B-N-4 Bonkola North B-N-A Bonkola North B-N-B Bonkola North B-N-C Bonkola North HC-N-01 Hillcrest North HC-N-02 Hillcrest North HC-N-03 Hillcrest North HC-N-04 Hillcrest North HC-N-05 Hillcrest North HC-N-06 Hillcrest North HC-N-A Hillcrest North HC-N-B Hillcrest North HC-N-C Hillcrest North HC-N-D Hillcrest North HC-N-E Hillcrest North HC-N-F Hillcrest North HC-N-G Hillcrest North HC-N-H Hillcrest North HC-N-I Hillcrest North H-S-A Hillcrest South H-S-B Hillcrest South H-S-C Hillcrest South Horizontal Horizontal Horizontal Horizontal Diagonal Diagonal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Vertical Vertical Vertical Vertical Vertical Vertical Vertical Vertical Vertical Horizontal Horizontal Horizontal Mixed Mixed Mixed Mixed Mixed Mixed Mixed Mixed Mixed Mixed Host rock Host rock Host rock Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Host rock Host rock Host rock 22.1 22.1 22.1 22.1 12.5 13.5 12.1 12.1 12.1 11.8 14.7 14.7 14.6 20.8 20.5 20.4 20.4 20.3 20.4 11.7 11.4 11.5 11.7 11.8 11.8 11.8 11.5 11.6 19.5 29.5 29.7 51 49 53 45 31 39 44 50 63 50 20 24 25 25 24 25 19 18 12 4 4 11 11 9 6 8 9 9 34 74 62 2.3 2.2 2.4 2.0 2.5 2.9 3.6 4.1 5.2 4.2 1.4 1.6 1.7 1.2 1.2 1.2 0.9 0.9 0.6 0.3 0.4 1.0 0.9 0.8 0.5 0.7 0.8 0.8 1.7 2.5 2.1 Regional-scale profiles GV_E_2 Golden Valley GV_E_3 Golden Valley GV_E_4 Golden Valley GV_E_6 Golden Valley GV_E_7 Golden Valley GV_E_8 Golden Valley GV_W_1a Golden Valley GV_W_1b Golden Valley GV_W_2 Golden Valley GV_W_3 Golden Valley Mary Eastern Cape Graaf Reinet Eastern Cape R364 Eastern Cape R364_2 Eastern Cape Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Horizontal Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite Dolerite 700 140 170 250 340 190 310 80 260 360 140 190 70 70 205 30 47 62 53 36 93 19 80 135 39 69 27 42 0.3 0.2 0.3 0.2 0.2 0.2 0.3 0.2 0.3 0.4 0.3 0.4 0.4 0.6 1845 908 0.5 1.8 Total (all): Total (high-resolution only): 3782.8 512.8 Number of fractures Fractures/meter (avg) and its associated fracturing patterns. The Karoo igneous rocks were studied with respect to regional geochemistry across southern Africa (Bristow and Saggerson, 1983), and have been linked to synchronous igneous complexes in Antarctica (Ferrar) and South America (Paraná; Cox, 1992). The regional geometry of the dolerites and associated fracturing was particularly well studied by the South African Water Resource Commission in conjunction with groundwater exploration and management (e.g., Chevallier et al., 2001; Chevallier and Woodford, 1999; Woodford and Chevallier, 2002). geometries include a thick (>100 m thick) inclined dolerite sheet (Hillcrest), a thin (ca. 2 m thick) dyke (Bonkola), and a moderately-sized (ca. 5 m thick) inclined intrusion (Nonesi’s Neck). The road-cut exposures at both Hillcrest and Bonkola facilitated lidar acquisition at both sides of the road. Blast marks, and related fractures associated with road construction can be clearly identified both on lidar and field data and were not included in the analyses. The well-studied Golden Valley sill (e.g., Polteau et al., 2008; Schofield et al., 2010) was chosen as a site for the large-scale fracturing study. 4. Methods and study sites 4.2. Lidar scanning 4.1. Study sites Terrestrial laser scanning (also known as lidar) is a well-established 3D measurement technique that can be used for collecting large amounts of digital, topographic data for building spatially complete and precise models of geological outcrops. It is particularly used for studying outcrop analogues of reservoirs targeted by the hydrocarbon industry (e.g., Enge et al., 2007). In this paper, The sites for this study were selected based on two criteria: They should display a range of intrusion geometries within a similar geologic setting, and all should thus be located within the Burgersdorp Formation (Table 1 and Fig. 1). The observed igneous 75 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 LiDAR Fieldwork Fracture frequency diagrams 14 BD_01 Numberoffractures Bonkola N BD_01L Continuous 12 Discontinuous 10 Lidar profile 8 6 4 2 0 1 3 2 4 5 6 7 8 9 10 Distancealongscanline (m) Continuous 12 Numberoffractures Hillcrest S HC_01L HC_01 Discontinuous 10 Lidar profile 8 6 4 2 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 Distancealongscanline (m) Nonesi’s Neck intrusion 20 Bed-confined 18 Continuous 16 Discontinuous 14 ImageJ 12 10 8 6 4 Numberoffractures 22 Through-going 2 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Distancealongscanline (m) Fig. 3. Comparison of field data and digital data sources (lidar and photo-mosaics) from selected localities. Stereoplots are shown with an equal-area lower hemisphere projection, with fractures displayed as contoured poles to planes. The fracture frequency diagrams show the field data (vertical bars, subdivided by fracture type) compared to the digitally interpreted scanlines (red line). See Table 2 for details on the various data sets. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.) the method has been applied as described by Buckley et al. (2008), with a Riegl LMS-Z420i terrestrial lidar scanning system employed for data acquisition. Data gaps within the lidar point cloud were kept to a minimum by positioning the instrument at multiple locations. The lidar instrument was equipped with a Nikon D200 (10.2 MP) camera, which allows automatic registration of calibrated digital photographs within the lidar coordinate system. The main processing steps involve the registration of several high-density lidar point clouds in a common coordinate system, point cloud reduction and point cloud triangulation to create a meshed 3D surface. The meshed surface is then textured with the photographs, resulting in photorealistic 3D outcrop models used to conduct fracture measurements. While the 3D information of the lidar data allows structural measurements, the lithology (e.g., contact between dolerite and host rock) can be easily recognized from the photographs, which would be difficult from the lidar point cloud alone. Fracture characterization was conducted manually using the in-house software LIME. At such close range (maximum 30 m from scanner to outcrop), the virtual outcrop model provided nearly as high resolution as traditional photography (less than one centimeter), as illustrated by the blast mark and measuring tape in Fig. 2C. 4.3. Photo-based interpretation Due to limited accessibility and scanning range restrictions imposed by the size of the outcrop and the unavailability of a helicopter-mounted lidar scanner (e.g., Rittersbacher et al., 2013), the outer rims of the Golden Valley saucer-shaped intrusion were photographed at a distance of 0.5–3 km with a Nikon D90 digital camera (12.9 MP) with a telephoto lens (focal length of 200 mm). The resultant images were stitched together as a conventional flattened photo-mosaic, fractures were interpreted manually and subsequently processed using the ImageJ image processing software 76 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 fractures in host rock A Nonesi’s Neck Bonkola S Hillcrest S Bonkola N All Hillcrest N 1 2 n=176 n=134 n=308 n=158 n=55 n=831 Bonkola S Bonkola N Hillcrest S n=60 n=50 n=532 All Hillcrest N fractures in dolerite B Nonesi’s Neck n=101 n=473 n=1216 0-10 10-20 20-30 30-40 40-50 50-60 60-70 70-80 80-90 n=59 n=50 n=53 n=49 n=51 n=67 n=55 n=100 n=61 n=40 n=36 n=39 n=60 90-100m Hillcrest S C n=60 n=31 Hillcrest N n=57 n=59 n=78 Fig. 4. Structural data derived from the virtual outcrop models. See Table 2 for details on the data sets. (A) Fracture orientations mapped in sedimentary rocks at the three study sites. The rose diagram shows the strike of all the fractures in the host rock. The master jointing sets from the Western Karoo published by Woodford and Chevallier (2002) are shown for comparison: (1) Master joints with a predominant NNW-trend, (2) E–W jointing set particularly prominent in the Graaff-Reinet area. (B) Fractures in dolerite compared to the main dyke orientation and the outcrop orientation. The rose diagram shows the strike of all the fractures in dolerite. (C) Orientation of fractures in the Hillcrest igneous bodies, grouped in 10 m intervals away from the contact zone. Both the northern and southern outcrops are shown for comparison. All stereoplots are illustrated using an equal-area, lower hemisphere projection, with a Schmidt grid. The main dyke orientation (solid blue line) and the outcrop orientation (green stippled line) are shown where applicable. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.) (Abràmoff et al., 2004) to provide ‘virtual scanlines’. The resolution and accuracy of this method is much lower than for terrestrial lidar scanning, but it is nonetheless very useful for determining whether the overall fracturing frequency changes around a single largescale intrusion. Furthermore, in order to ensure a robust comparison during subsequent analysis, the same method was also successfully applied for determining fracture spacing on manually interpreted high-resolution images generated from the virtual outcrop models. 4.4. Field work Traditional field methods were employed at the scan localities in order to ground-truth the digital data. The line-intersection method (i.e., scanlines; Singhal and Gupta, 2010) was used to characterize the fractures (e.g., fracture orientation, fracture infill) along 1D transects at Hillcrest, Bonkola and Nonesi’s neck. Fractures in dolerites were classified as either continuous (main fractures extending across most of the outcrop) or discontinuous (shorter fractures often abutting against other fractures). Fracture orientation (strike and dip) was measured using both a standard geological compass and a digital GeoClino clinometer, both of which were controlled for unwanted magnetic interference from the dolerites. A magnetic declination correction of 24.1° west was applied prior to data analysis (NOAA, 2013). 5. Results Results from scanlines and structural stations are compiled in Table 2, while virtual profiles from all localities are listed in Table 3. 5.1. Field versus digital data An initial comparison of the lidar-derived virtual outcrop models (VOMs) and digital photographs highlight the differences in resolution (Fig. 2). The most significant advantage of VOM compared to traditional 2D photo-mosaics is the three-dimensional rendering of the outcrop which in many cases allows direct measurement of fracture orientations on the model. The uncertainty attached to using VOM is related to scan-resolution, scanning angle and 77 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 A B 13 12 number of fractures per 10m 11 GV_W_1 GV_E_2 GV_E_3 GV_W_2 GV_E_4 GV_E_6 GV_W_3 GV_E_7 GV_E_8 10 9 8 7 6 5 4 3 2 1 100 80 60 10 40 D R364-2 R364 Graaf Reinet Mary GV_E_8 GV_E_7 GV_E_6 GV_E_4 GV_E_3 GV_E_2 GV_W_1b 12 ln(Y) = -2.3574 * ln(X) + 6.3036 8 20 frequency fracture spacing (m) C GV_W_3 5 km GV_W_2 GV_W_1a 0 6 4 2 10 8 6 4 0 GV_W_3 GV_W_2 GV_W_1b GV_W_1a GV_E_8 GV_E_7 GV_E_4 GV_E_2 2 1 0.8 1 2 4 6 8 10 20 40 fracture spacing (m) Fig. 5. Regional study of the outer rims of the Golden Valley sill, illustrating fracture frequency in different segments of the saucer-shaped intrusion. (A) Location of the studied segments on the eastern and western limbs of the sill. (B) Whisker plots (minimum, lower quartile, mean, upper quartile, maximum) illustrating the variable fracture frequency in 10 m intervals at the Golden Valley ‘virtual scanlines’ as well as control locations. (C) Whisker plots illustrating the individual fracture spacing at selected ‘virtual scanlines’ at Golden Valley. (D) Log–log plot of all the fracture spacing measurements at the sites shown in (C), grouped into 0.25 m wide bins. The data suggests a power-law distribution in the 3–30 m interval. influences introduced during processing, such as point cloud decimation or smoothing (Buckley et al., 2008). Both VOM and photo-mosaic data were checked using traditional field techniques at all localities (scanlines, Fig. 3). The orientations show some discrepancy, particularly at Bonkola N, where orientations are hampered by the overall dip of the VOM toward the road. Depending on whether fracture planes are measured along a line (i.e., virtual scanline) or across the whole outcrop, the well-exposed road-facing fracture surfaces may thus be overrepresented. Orientation of field data, on the other hand, may be somewhat hampered by the highly magnetic dolerite, which may influence measurements made using a magnetic compass, even though the absence of this effect was checked in the field. Fracture frequency data collected using ‘real’ and ‘virtual’ scanlines show good agreement. More fractures, particularly the shorter discontinuous fractures, were identified using conventional field techniques compared to both VOMs (Bonkola N, Hillcrest S) and photo-mosaics (Nonesi’s Neck). Qualitatively, the overall pattern of higher fracture frequency within the intrusions is evident in all data sets. However, the VOMs, photo-mosaics and field data each sample a specific range of fracture sizes due to their differing resolutions, and quantitative comparison of the results from the different methods should be treated with caution. 5.2. Fracture orientation Analysis of fracture orientation was primarily carried out using the virtual outcrop models, with control data provided by a limited number of traditional scanlines (Table 2). Orientations are presented as poles to planes in Fig. 4, illustrating the dominant orientation of fractures in the sedimentary host rock (Fig. 4A), fractures in the dolerite (Fig. 4B) and fractures in the dolerite at specific intervals from the intrusion contact (Fig. 4C). An interesting observation is that the fractures are typically aligned parallel to the outcrop orientation. This is counter-intuitive for traditional scanlines, which tend to be biased toward fractures oriented perpendicular to the outcrop orientation, since these are more likely to intersect the outcrop-parallel scanlines. However, on virtual outcrop models fractures aligned sub-parallel with the outcrop are rendered more clearly on the 3D image, and consequently more easily identified during interpretation. Bias correction (e.g., Lato et al., 2010) can be applied, but small fractures C HC-N-I HC-N-H HC-N-F HC-N-E HC-N-D HC-N-C HC-N-A A HC-N-G K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 HC-N-B 78 intrusion contact 10 fractures HC-N-06 HC-N-05 HC-N-04 HC-N-03 HC-N-02 HC-N-01 intrusion contact D E G F H I _0 6 _N C C H H _N _0 5 _0 4 _N _0 3 C _N C H H _N C C _N 10 5 _0 2 _0 1 D H HC-N-06 4 3 2 1 C B H B A 0 2 4 6 8 10 12 14 16 18 2 1 fracture spacing (m) 3 HC_N_I HC_N_H 0 HC_N_G 20 15 10 5 0 4 HC_N_F HC-N-01 4 3 2 1 0 5 vertical profiles HC_N_E 20 15 10 5 0 HC_N_D HC-N-02 4 3 2 1 1 HC_N_C 20 15 10 5 2 HC_N_B HC-N-03 4 3 2 1 3 HC_N_A 20 15 10 5 4 cumulative number of fractures fractures per metre HC-N-04 4 3 2 1 horizontal profiles 20 15 10 5 fracture spacing (m) 5 HC-N-05 4 3 2 1 20 Distance (m) Fig. 6. Fracturing pattern within 20 m of the contact zone at Hillcrest N. (A) High-resolution screen capture of the virtual outcrop model, with interpreted fractures (black lines) and profile locations (yellow stippled lines). (B) Histograms and cumulative frequency plots of the six horizontal profiles HC-N-01 to HC-N-06 away from the contact. (C) Cumulating frequency plots of the eight vertical profiles HC-N-A to HC-N-I at varying distance from the contact. (D) Whisker plots (minimum, lower quartile, mean, upper quartile, maximum) illustrating the fracture spacing in the horizontal and vertical profiles. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.) aligned perpendicular to the outcrop will often remain undersampled, due to the line-of-sight effect and smoothing during lidar processing. Fractures observed in the sedimentary rocks display a wide range of orientations (Fig. 7A), but mainly align along an E–W and a NW–SE axis. As stated above, there is a clear bias due to individual outcrop orientation, which in turn influences statistics of the complete dataset. This can be illustrated by the Hillcrest S (n = 308) locality which dominates the orientation plot as it contains 37% of all fractures analyzed in the sedimentary host rock. The Hillcrest S and Hillcrest N localities also illustrate the effect of analyzing outcrops on opposite sides of road-cuts. As expected, fractures predominantly dip to the north (toward the road) at Hillcrest S, and to the south (also toward the road) at Hillcrest N. Fracture orientation data from host rocks and intrusions exhibit significant differences, as shown in Fig. 4. While fractures in the host rock are likely related to regionally extensive joint patterns, fractures in the dolerite are aligned mainly along a NW–SE trend and a sub-ordinate E–W trend. This is remarkably similar to the regional dyke orientation, but the orientations at the Hillcrest site (supplying the majority of measurements) also align to the outcrop orientation. This may mask the natural fracturing pattern. At Hillcrest, the fracture orientation was sampled along 10 m wide segments to investigate potential orientation changes toward 79 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 A B-N-C Intrusion B-N-B B-N-A B-N-C 4 3 2 1 4 3 2 1 B-N-B 4 3 2 1 B-N-A 0 20 15 10 5 20 15 10 5 Intrusion 20 15 10 5 1 2 3 4 5 6 7 8 9 10 11 12 13 cumulative number of fractures fractures per metre 1m Distance(m) B H-S-C H-S-B Intrusion H-S-A 4 3 2 1 4 3 2 1 H-S-C 60 40 20 H-S-B 60 40 20 H-S-A 60 40 20 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 cumulative number of fractures 4 3 2 1 Intrusion contact fractures per metre 1m Distance(m) Fig. 7. Fracture frequency in sedimentary layers away from intrusion contacts. Fractures in dolerite are not represented in this figure. (A) Fracture frequency in three sandstone layers within 15 m of the thin dyke at Bonkola N. The fracture frequency is displayed both as a histogram (binned fractures/meter, scale on left) and cumulative number of fractures toward the contact (scale on right). (B) Fracture frequency in three sandstone layers within 30 m of the inclined dolerite sheet at Hillcrest S. the intrusion contact at 0 m (Fig. 4C). The stereoplots on both sides of the road (Hillcrest S and Hillcrest N) both indicate a broader spread in fracture orientations 0–10 m from the contact zone. This may suggest enhanced structural complexity at the contact zone. However, similarly variable fracture orientations are also evident at some distance from the contact zone (particularly in the 30–40 m and 50–70 m intervals) that may be related to intrusion-internal structural complexities. In the segment closest to the contact at Hillcrest N, there appears to be a minor overlap between the fracture orientation and the orientation of the main dyke (blue diamond illustrated in Fig. 4C). This overlap is not clearly evident in the inner part of the intrusion. However, the large scale and uncertain overall geometry of the inclined sheet exposed at Hillcrest may generate complex external geometries with irregular contacts as well as correspondingly complex internal fracturing patterns. 5.3. Fracture spacing The fracture spacing, directly linked to overall permeability in crystalline rocks with low or no matrix porosity, was investigated both at the regional and local scale. On the regional scale, high-resolution photo-mosaics were acquired at both limbs of the Golden Valley saucer-shaped intrusion (Fig. 5A). The analyzed data, plotted as whisker-plots together with some ‘control sills’ in the vicinity (Fig. 5B), show a similar fracture density spanning from 1 to 4 80 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 B-N-4 B-N-3 B-N-2 B-N-1 1m fractures per metre 40 20 B-N-3 6 4 2 40 20 B-N-2 6 4 2 40 20 B-N-1 6 4 2 0 host rock 40 intrusion 20 cumulative number of fractures B-N-4 6 4 2 0 0 1 2 3 4 5 6 7 8 9 10 11 12 Distance (m) Fig. 8. Fracturing patterns at Bonkola N. The analyzed fracture frequency profiles (histograms and cumulative frequency) are shown at the same scale below. fractures per 10 m (mean) in all the photo-mosaics. The fracture spacing (Fig. 5C) was approximately 3 m (mean), though it can be longer locally (e.g., profile GV_E_7, ca. 5 m). Maximum fracture spacing was generally below 15 m, though in some profiles poor exposure has resulted in significant maxima. A log–log plot of fracture spacing versus frequency (Fig. 5D) illustrates a typical powerlaw distribution above approximately 3 m, considered to represent the lower separation limit on this regional scale. On the local scale, the dolerite-internal fracturing was extensively analyzed within 20 m of the contact at the Hillcrest N locality. Six horizontal virtual profiles and nine vertical profiles are illustrated in Fig. 6. The horizontal profiles (Fig. 6B) clearly illustrate a fracture swarm aligned roughly perpendicular to the contact, and intersecting the lowermost profile (HC-N-01) at 9 m. The 2 m thick fracture swarm generates the highest fracture frequency (up to 4 fractures per meter; f/m) in all profiles, and was also well imaged on two vertical profiles (HC-N-C and HC-N-D). Apart from this fracture swarm, no obvious fracture frequency increase is apparent toward the contact on either horizontal or vertical profiles at this site. Fracturing was also investigated in the sedimentary host rocks around the intrusion, using the thin dyke at Bonkola N and thick inclined sheet at Hillcrest S as case studies (Fig. 7). At Bonkola N (Fig. 8), three horizontal virtual profiles along three distinct sandstone beds all illustrated enhanced fracturing within 2–4 m of the intrusion contact. This was most obvious from the cumulative fracture plots, but even the binned fracture frequency was typically (except for profile B-N-C, see Fig. 7A) highest in this interval (up to 4 f/m). Away from the intrusion, background fracturing was typically 0–2 f/m in all three layers. At Hillcrest S, the background fracturing, measured up to 25 m away from the contact, was somewhat higher (1–4 f/m; Fig. 7B). This is likely related to the strengthening of the host rock due to contact metamorphism associated with the emplacement of this relatively large-scale intrusion (Haave, 2005). Closer to the contact, fracture frequency appeared similar to background fracturing. On the two uppermost profiles (H-S-B and H-S-C), which follow sandstone bodies presumably wedged up by the intrusion, the cumulative frequency curve was nonetheless somewhat steeper within the first 3 m away from the intrusion. Fracture frequency in virtual profiles across both sedimentary rocks and the intrusion were investigated using the Bonkola dyke as a case study (Figs. 8 and 9). At Bonkola N, four virtual profiles across an interpreted high-resolution screen capture of the virtual outcrop model revealed a complex fracture network, particularly in the host rock. In the intrusion itself, fractures were typically aligned both perpendicular and parallel to the contact. Fracturing appeared to be minimal within the intrusion (profile B-N-3), though this may be an artifact due to poor fracture exposure in the dyke, which is partly covered by vegetation. The pervasive fracturing of the host rock, particularly in the shale between profiles B-N-1 and B-N-2, may be related to surficial weathering given that the fractures do not display any distinct orientation. On the other side of the road, at Bonkola S, enhanced fracturing is evident within the intrusion, as are clearer, continuous, fractures within the host rock (Fig. 9). The dipping intrusion emphasizes the two main fracture sets within the dyke, namely parallel and perpendicular to the intrusion contact. Both of these sets contrast with the predominantly vertical fracture exposures in the country rock. A limited number of fractures in the host rock are also aligned 81 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 parallel to the intrusion contact (highlighted by arrows in Fig. 9), but all occur within 1 m of the intrusion. Comparing the fracture spacing in dolerites and host rocks illustrates the broad range of fracture spacing in dolerites, particularly when measured along vertical profiles (Fig. 10). The range of fracture spacing was well-constrained for both host rock and mixed lithology profiles, with the upper to lower quartile falling between 0.1 and 1 m on all profiles. In dolerites, however, the fracture spacing spanned from 0.01 m (min) to 4 m (max), and the mean spacing varied between 0.3 and 1.5 m. Scanlines, due to their higher resolution, displayed a consistent mean fracture spacing of approximately 0.1–0.2 m, corresponding well with the mixed lithology profiles at Bonkola N. 2m B -S -6 5 S- B- B-S-4 B-S-3 B-S-2 B-S-1 B-S-4 3 1 B-S-3 fractures per metre 3 40 30 20 10 2 1 B-S-2 3 40 30 20 10 2 1 B-S-1 3 40 30 20 10 0 2 1 0 0 2 3 4 5 6 7 8 9 Distance(m) B-S-5 6 f/m 1 13 14 B-S-6 15 16 17 18 19 20 21 cumulative number of fractures 40 30 20 10 2 22 20 fractures 4 2 0 0 1 2 3 host rock 4 5 6 7 intrusion 8 9 1 2 3 4 5 6 7 8 9 10 11 12 Distance(m) Fig. 9. Fracturing patterns at Bonkola S. The analyzed fracture frequency profiles (histograms and cumulative frequency) are shown at the same scale below. 82 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 10 fracture spacing (m) Dolerite Host rock Mixed lithology Scanlines 1 0.1 0.01 NND-02 HC-01 NND-01 B-N-4 BD-01 B-N-3 B-N-2 B-N-1 B-S-6 B-S-5 B-S-4 B-S-3 B-S-2 B-S-1 H_S_C H_S_B H_S_A B_N_C B_N_B B_N_A HC_N_I HC_N_H horizontal profiles HC_N_G HC_N_F HC_N_E HC_N_D HC_N_C HC_N_B HC_N_A vertical profiles HC_N_06 HC_N_05 HC_N_04 HC_N_03 HC_N_02 HC_N_01 horizontal profiles Fig. 10. Summary of fracture spacing from a variety of high-resolution profiles and scanlines, subdivided by the dominant lithology. The whisker-plots illustrate the minimum, lower quartile, mean, upper quartile and maximum fracture spacing at each profile. Note the logarithmic scale. Refer to Table 3 for details. 6. Discussion 6.1. Heterogeneity of fracture networks and tectonic setting The most striking result of this study relates to the pervasive heterogeneity of the study sites. Even within the same outcrop face, profiles do not reflect a consistent pattern of fracturing both in the host rock and the intrusion. Furthermore, the primary fracture orientations are significantly different at the three sites, being heavily biased by the outcrop orientation. This complex fracturing pattern may be related to tectonic pre- and post-intrusion heterogeneities within the host rock (‘TF’), juxtaposed with syn-emplacement fractures in the host rock (‘SEF’) and post-emplacement fractures in the intrusion (‘PEF’). A good example is illustrated in the profiles at Bonkola S, where the intrusion-related fracturing was masked by the pervasive fracturing in the host rock, particularly on the north side of the intrusion. In order to simplify the complex fracturing patterns, we discuss the three main fracture sets introduced previously: (1) syn-emplacement fractures in host rock, (2) post-emplacement fractures in the intrusions and (3) tectonic fractures in both intrusion and host rock. 6.2. Syn-emplacement fracturing in host rock The emplacement of intrusions has mechanical consequences for the surrounding host rock, as exemplified, for example, by the jacked-up country rock at Nonesi’s Neck. Theoretically, the increased deformation associated with magma emplacement should lead to enhanced fracturing of the host rock in the vicinity of the intrusions. We have shown limited increase (doubling of the background fracture frequency within one meter of the intrusion, but only in one profile) in host rock fracturing toward the intrusion contacts, most developed at the Bonkola N site. The lack of a clear increase in fracture frequency toward the intrusion is thought to be masked by the underlying host rock heterogeneity, and, to some extent, also the resolution limit of the virtual outcrop models, which clearly underestimate the frequency of short discontinuous fractures. On the regional scale within the Karoo Basin, dyke-related fracturing was extensively studied due to its direct influence on groundwater potential. Woodford and Chevallier (2002) suggested that fractures related to the emplacement of dykes are present within 5–15 m from the dyke, forming a structurally complex zone of enhanced fracturing. 6.3. Post-emplacement fracturing patterns in intrusions Our study illustrates that the fractures within the same intrusion are typically oriented perpendicular and parallel to the contact, best exemplified at Bonkola N (Fig. 9). These fractures are thus interpreted as related to thermal contraction during cooling, with the cooling front propagating from the relatively cool host rock interface. This is in accordance with our observations, as well as numerical modeling by Kattenhorn and Schaefer (2008) who predicted four types of fractures: column-bounding, column-normal, entablature (all of which are cooling fractures, ‘PEF’), and inflation fractures (‘SEF’). This observation is also in good agreement with the analyses of Bermúdez and Delpino (2008). Fractures related to magma cooling will clearly also be controlled by the intrusion geometry and the magma emplacement chronology and direction. Schofield et al. (2012b), using both outcrops and 3D seismic data, describe the development of magma lobes within a single sill complex. Proximal to the magma source, these lobes coalesce into a single sheet. In distal settings, however, the same sill will form numerous magma lobes. Needless to say, the fracturing pattern is expected to be different in a large-sized sheet compared to smaller, more localized and structurally complex magma lobes. It is also expected that the fracturing pattern will be different in a large-sized sheet compared to smaller, more localized and 83 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 Positive topographic relief Negative topographic relief Groundwater well Terrain surface HOST ROCK Shale Fracture Set 1: syn-emplacement (SEF); parallel to contact within zone 3 Increasing due to weathering and reduced lithostatic pressure DOLERITE DYKE ct ur es Sandstone or tio n of o pe n Fracture Set 3: background tectonic deformation (TF); not aligned to intrusion Pr op 4 fra Fracture Set 2: post-emplacement (PEF); a: perpendicular to contact b: parallel to contact) Sandstone 3 not to scale 2 Shale Most complex fracture pattern in the central part of zone 1 and entire zone 2 HOST ROCK Decreasing due to increased lithostatic pressure 1 2 43 Conglomerate Sandstone Zone 4: due to low-grade contact metamorphism) Zone 3: contact aureole of host sediments “Hornfels zone”, calcite veining, alteration of petrophysical properties due to contact metamorphism Zone 2: chilled margin of dolerite dyke (increased fracturing => permeability pathway?) Zone 1: Fig. 11. Conceptual model of fracturing along a hypothetical inclined intrusion, representative of both sills and dykes. The fractures are subdivided into three main sets: (1) syn-emplacement fractures within the country rock formed during magma emplacement, (2) post-emplacement fractures within the intrusion formed primarily by cooling mechanisms, and (3) tectonic fractures formed by processes unrelated to the intrusions. At depth (i.e., below the weathering depth), many fractures are closed and the intrusion primarily acts as a barrier. At shallower levels, where pre-existing fractures may be opened due to weathering, the intrusion may act as a carrier, particularly along the structurally complex intrusion–host rock interface (zones 2 and 3). structurally complex magma lobes, as observed by for example Witte et al. (2012). Nevertheless, it is not trivial to interpret the differences of fracture patterns observed on the studied outcrops in terms of intrusion thickness only. Indeed, both the size and the shapes of each studied intrusion are different, such that it is challenging to discriminate between the effects of the intrusion shape from those of the intrusion thickness on the observed fracture patterns, in particular based on three outcrops only. More systematic measurements are thus necessary. 6.4. Tectonic fracturing Tectonic fractures (including compaction and exhumation fractures) are present at all studied localities, as evidenced by the background fracturing pattern in the host rock away from the intrusion contacts. They may both pre- and post-date the intrusive activity. Tectonic fractures may also be present in the intrusions themselves, provided that the tectonic event post-dates the intrusive event. Slicken-sided surfaces along fractures within intrusions 84 K. Senger et al. / Journal of African Earth Sciences 102 (2015) 70–85 are a clear indicator of post-intrusive tectonism (e.g., Ogata et al., 2014). 6.5. Conceptual model of fracturing at intrusion–host rock contact zones On the basis of our field observations and the current state-ofknowledge, we propose a conceptual model of fracturing in- and around a hypothetical intrusion, with focus on the contact zones (Fig. 11). This structural model should be considered together with studies on aureole processes in different host rock lithologies (e.g., Haave, 2005), which will influence the size of the hornfels zone (zone 3). The model assumes a symmetric fracturing pattern at the base and top of the intrusion, and is thus applicable for both sills and dykes, but not for lava flows. The schematic zonation ranges from the inner part of the intrusion (zone 1), through the highly fractured chilled margin (zone 2) and the baked margin of the host rock (zone 3) to the structurally unaffected country rock (zone 4). Clearly, the nature of the magmatism (e.g., intrusion geometry, melt temperature, emplacement duration and direction) and the host rock properties (e.g., matrix permeability and porosity, pre-existing fracture network, temperature, fluid presence) will superimpose heterogeneities onto this conceptual framework. In our model, we simplify the fracturing pattern into the three main sets: (1) synemplacement fractures in the host rock, (2) post-emplacement fractures in the intrusion, and (3) tectonic fractures in both host rock and intrusion. Many individual fractures in fracture sets 1 and 2 are thought to be aligned parallel to the intrusion contact. Fractures perpendicular to the contact within zone 1 reflect the development of columnar joints. The permeability through the fracture network will, in addition to the obvious fracture network distribution identified in our model, be a function of the fracture connectivity and the fracture aperture. Cooling fractures perpendicular to the contact are often viewed as primary permeability pathways (e.g., Rateau et al., 2013), and the multi-sided pervasive jointing exposes much of the intrusion to percolating fluids. However, as pointed out by Petford (2003), the geometry of columnar joints lacks the fracture connectivity required for high levels of permeability. In essence, the columnar joints may locally provide permeability pathways across the intrusion, provided that they are open, but permeability is thought to be higher parallel to the intrusion contacts. This hypothesis was confirmed by hydraulic testing of the Palisades sill in New Jersey (Matter et al., 2006) and an inclined doleritic sheet at Qoqodala in the Eastern Cape province (Chevallier et al., 2004), both of which revealed increased permeability along the fracture system located at the host rock–intrusion interface. The fracture aperture is a critical parameter directly related to the flow rate (Singhal and Gupta, 2010). As illustrated in our conceptual model, fracture aperture, and thereby fracture permeability, is likely to decrease with depth due to various factors, including decreasing weathering, an increasing lithostatic pressure and increasing thermal expansion of rocks (Singhal and Gupta, 2010). This phenomenon of decreasing permeability with depth across individual dykes is well-known and clearly illustrated by the influence of dykes on the water table at different depths, corresponding to the weathering depth (Perrin et al., 2011). Nonetheless, the determination of fracture aperture at outcrops is hampered by uncertainty, and proxies such as packer tests are used to estimate the fracture aperture in various crystalline rocks to less than 400 lm (Cook, 2003 and references therein). Goldberg and Burgdorff (2005) used an acoustic televiewer at the Palisades Sill to illustrate very open (cm-scale) fractures, though it is unclear whether these relate to individual fractures or fracture corridors. This indicates that additional work focussed on fracture apertures is required to constrain the applicability of the conceptual model with depth. To summarize, the fracturing in the contact zone is particularly important since it drives the majority of the successful groundwater boreholes (van Wyk, 1963; Woodford and Chevallier, 2002), and the proposed model (Fig. 11) may provide a framework on which to conduct additional research. 7. Conclusions On the basis of our field observations of fracturing patterns in and around igneous intrusions within the Eastern Cape we infer the following: – The studied Karoo dolerite intrudes the Burgersdorp Formation host rock at three study sites. The dolerite exhibits different forms, namely a thin dyke (Bonkola), a medium-sized inclined intrusion (Nonesi’s Neck) and a thick inclined sheet (Hillcrest). – Fractures are classified into three groups based on the likely mode of formation, namely (1) syn-emplacement fractures in host rocks, (2) post-emplacement fractures in dolerite and (3) tectonic fractures in both host rock and dolerite. – The primary fracture orientations are significantly different at the three sites, being heavily biased by the outcrop orientation. – Fracture spacing is consistent between the three sites, and is shown to be more variable and irregular within the dolerite compared to the host rock. – At one of the sites (Bonkola N), fracturing in the surrounding host rock increases qualitatively toward the intrusion within approximately 3 m of the contact. – Based on our field observations and the current state-of-the-art, we propose a conceptual model for fluid flow along intrusion– host rock interfaces. The four-zoned model spans from the unaffected country rock to the central part of igneous intrusions, and predicts that fluid flow will most likely be focussed along the intrusion–host rock contact zones. Acknowledgements This work was partly financed by the Research Council of Norway, through the CLIMIT program (‘Geological input to carbon storage’ project) and through its Centres of Excellence funding scheme (project number 223272). Fieldwork was funded by a World Universities Network researcher mobility grant and a Meltzerfondet stipend, both to K.S. Lilith Kuckero assisted during the field work. The Council for Geosciences kindly provided digital geological maps of the study area. OpenStereo (Grohmann and Campanha, 2010) was used for plotting stereoplots, Google provided an academic license of Google Earth Pro and Riegl GmbH provided ongoing software support. We thank the participants of the LASI V workshop, held in Port Elizabeth 29–30 October 2012, for fruitful discussions. 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