Electronic Theses and Dissertations (PhDs)

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Browsing Electronic Theses and Dissertations (PhDs) by SDG "SDG-15: Life on land"

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    3D seismic constraints on the strato-structural evolution of the deep-water Orange Basin, South Africa
    (University of the Witwatersrand, Johannesburg, 2023) Maduna, Nombuso Gladys; Jinna, Zubair; Manzi, Musa
    This research utilizes seismic attributes and advanced machine learning methodologies to analyse high-resolution 3D reflection seismic data from the deep-water Orange Basin, located offshore western South Africa. The primary goal is to gain valuable insights into the basin's tectonic setting, depositional environment, and hydrocarbon potential. Significant features are delineated within the basin including (1) a gravitational collapse system in the Mesozoic Late Cretaceous, (2) mass flow features in the Cenozoic, (3) natural gas and fluid escape structures, (4) a large slope-perpendicular submarine canyon cutting Oligocene strata, and (5) multiple slope-parallel, sinusoidal channel features in the Miocene. The Late Cretaceous succession exhibits a gravitational collapse system with a translational and compressional domain detaching on seaward-dipping Turonian shales. Gravitational collapse during margin uplift formed fold-and-thrust belts along the slope characterizing the compressional domain. As they are commonly linked to hydrocarbons, the compressional domain of these systems has been extensively studied, while the translational domain has been poorly constrained due to its structural complexity. In this research, the translational domain is shown to contain a mixture of extensional tectonics (normal faults) up-dip and compressional tectonics (thrusts) down-dip, with extensive oblique-slip faults cutting thrusts perpendicularly during the translation of sediment. Variance and chaos, conventional seismic attributes, were used to manually pick and interpret the >500 regional-scale faults arising from the gravitational collapse system. Fault-net, a convolutional neural network (CNN), was compared with these edge-enhancing seismic attributes for extracting faults from the seismic volume. The CNN offers several notable advantages over conventional seismic attributes, such as automation, accelerated analysis, and improved time-efficiency on large datasets. Analysing the distribution, type, and geometry of faults within the basin gave valuable insights into the potential hydrocarbon system at work. Numerous natural gas and fluid escape features are identified in the seismic volume including an elongated mud volcano, pockmarked surfaces, and polygonal faults. The stability of the evolving margin is influenced by the underlying structure of a Late Cretaceous gravitational collapse system, also referred to as a deep-water fold and thrust belt (DWFTB) system. The fault framework within provides primary migration pathways for hydrocarbons. Major seafloor slumping occurs directly above a syncline of the Late Cretaceous DWFTB system. This slumping surrounds a structurally controlled, 4.2 km long elongated mud volcano situated between the translational and compressional domains of the underlying DWFTB system. The late Campanian has the largest accumulation of hydrocarbons evidenced by (1) an anticline with a positive high amplitude anomaly situated at the intersection of the two domains, and (2) >950 pockmarks preserved on the palaeo-surface compared to the 85 pockmarks observed on the seafloor. In addition to tectonics, the onset of stratified oceanographic circulation patterns and climate played a large role in changing depositional trends since the mid-Cenozoic. The Oligocene is characterized by a ~2.3 km wide, >13 km long, slope-perpendicular canyon formed at ~30 Ma during a major sea-level fall by a turbidity current. The Miocene is characterized by a ~14 km wide zone of slope-parallel, sinusoidal channels between water depths of 1 200–1 500 m. The formation and preservation of these features during the Miocene are attributed to the erosive interaction between two distinct water currents: (1) the Antarctic Intermediate Water flowing northwards, and (2) the deep North Atlantic Deep Water bottom currents flowing southwards; and the effects of the Benguela Upwelling System and a dry climate prevailing in southwest Africa all intensifying around 11 Ma. While pre-Miocene hydrocarbons originate from Turonian and Aptian source rocks, the origin of hydrocarbons on the seafloor is likely biogenic, arising from organic-rich sediment in the Miocene
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    Constraints on the genesis of orbicular granites and sulphide mineralization in the Koperberg Suite, South Africa and the Diana’s Pool area, Zimbabwe
    (University of the Witwatersrand, Johannesburg, 2024) Dumisa, Senamile Siyaya
    This work tackles a long-standing problem in petrology, the formation of orbicular granitoids. These bodies occur as entire facies or as areas enriched in orbicules within distinct facies of plutons. Some European examples are highly prized for their decorative qualities. However, their origin is a matter of much debate going back to times when the origins of granitoids themselves were not obvious and are confused by topics such as ‘granitization’ and over-exaggeration of metasomatic effects. Here, poorly studied outcrops of orbicular rocks from the Matopos granite batholith in the Diana’s Pool area, Zimbabwe and the Koperberg Suite, South Africa are tackeld. Enzman (1953) and Garvie (1969; 1971) studied the Koperberg Suite and the Diana’s Pool orbicules, respectively and employed field observations and petrography to examine and characterize the genesis of these rocks. However, there is little evidence presented to confirm their theories on how these rocks formed as previous work lacks detailed geochemical, mineral chemistry and isotope data to support Enzman and Gravie’s conclusions on the genesis of these rocks. Furthermore, there is no connection between the metallogenesis of the sulphide mineralization and the origin of orbicular rocks, which is a unique characteristic of particular orbicule sites in the Koperberg Suite. This study focuses on four different orbicular bodies (Orbicule Koppie, Henderson South, Henderson North and Hoogkraal Lease) from the Koperberg Suite, hosted in lithologies ranging from diorite to pyroxenite compositions. The orbicules from different orbicular share similar characteristics. Coarse- grained felsic cores, fine-grained and alternating ferromagnesian and feldspathic shells, and coarse- grained to pegmatitic matrices characterize them. The orbicules are generally spherical to ellipsoidal in shape, however, some appear to be abraded and deformed (e.g., Orbicule Koppie). The compositions and grain sizes of cores and the matrix are comparable in all localities. Both the matrix and the cores are medium- to coarse-grained and dominated by plagioclase (the matrix probably in slightly lesser proportions), microcline (in variable proportions, and seemingly absent in some cores), quartz, biotite, magnetite and orthopyroxene (in the case of Hoogkraal Lese, Henderson North and Henderson South). Contrary to the cores and matrix, shells are fine-grained and exhibit polygonal textures. In addition to this, the shells are dominated by biotite and orthopyroxene. Plagioclase in the Henderson North and Henderson South orbicules is more calcic than plagioclase in Hoogkraal Lease and Orbicule Koppie orbicules. Biotite in the Henderson North and the Orbicule Koppie orbicules is more magnesian than those at Henderson South and Hoogkraal Lease orbicules. Plagioclase in the Henderson North orbicules are characterized by elevated and radiogenic initial 87Sr/86Sr ratios than the other orbicule localities. There is also a variation in 87Sr/86Sr ratios within the individual orbicular structures (cores, shells and matrices) in individual localities. The orbicules at Henderson South, Orbicule Koppie and the Jubilee Pit host a bornite-dominated sulphide assemblage where disseminated chalcopyrite and bornite grains are characterized by granular textures and chalcopyrite is replaced by magnetite and bornite. Bismuth, Ni and Se in these sulphides appear to partition into bornite while Ag, In, Cd, Sn, Mn, Ge and Co partition into chalcopyrite. Diana’s Pool orbicular samples exhibit closely packed orbicules in a granitic matrix characterized by different types of orbicules containing coarse-grained felsic cores, fine-grained and alternating ferromagnesian and feldspathic shells, and a coarse-grained to pegmatitic matrix. The orbicules are generally spherical to ellipsoidal in shape, however, some appear to be abraded and deformed. The compositions and grain sizes of cores and the matrix are comparable. Both the matrix and the cores are medium- to coarse-grained and dominated by plagioclase (the matrix probably in slightly lesser proportions), microcline (in variable proportions, and seemingly absent in some cores), quartz, biotite and accessory hornblende and magnetite. Contrary to the cores and matrix, shells are fine-grained and exhibit polygonal textures. In addition to this, the shells are dominated by biotite and magnetite; however, they do not contain hornblende. Plagioclase in cores, shells and matrices shows an almost complete overlap of An contents. Biotite composition in the shells is significantly less magnesian than in core and matrix, whose compositions overlap. Initial 87Sr/86Sr ratios from plagioclase in shells are slightly more radiogenic than in the matrix and cores. Formation of both the Koperberg Suite and Diana’s Pool orbicules has been attributed to metasomatic processes. However, modelling of the Koperberg Suite orbicules using the Magma Chamber Simulator and a variety of textural and geochemical constraints rules out a metasomatic origin. The quartz + biotite-dominated diorite (Orbicule Koppie) and the pyroxene-diorites (Hoogkraal Lease, Henderson South, Henderson North), together with more felsic anorthosite and the more mafic pyroxenites, are all produced by progressive AFC + recharge processes, where the magma was most likely anatectic melts of the country rocks that were at granulite grade. In both Diana’s Pool and the Koperberg Suite, cores are autoliths, which are plagioclase-rich, cumulate, or rim fragments reworked by new magma inputs or injections. Heterogeneous nucleation leading to the formation of orbicular shells around the cores is attributed to adiabatic decompression of magma pulses ascending in dykes leading to superheating and resorption of early solids, and volatile exsolution, inducing undercooling, supersaturation, and shell crystallization. An alternative process that triggered superheating is magma mixing (e.g., Henderson South and Henderson North). The coarse-grained matrix crystallized later, after the orbicules formed, creating the groundmass, and locking the orbicules in place. The deformation of shells and cores (e.g., Orbicule Koppie and Diana’s Pool) suggests that the orbicules continued to evolve in the presence of a melt (matrix material) until they were emplaced at their present setting. The in situ sulphide assemblages in the Koperberg Suite have been reassessed in view of recent research on sulphide behavior. The bornite-chalcopyrite assemblage is atypical of the intermediate solid solution (iss) assemblage (chalcopyrite and pyrrhotite) observed in most Cu-Ni magmatic sulphide deposits. The high concentrations of trace elements that are incompatible with monosulphide solid solution and the depletion of Ni and Co in the sulphides are consistent with the derivation of sulphides from a Cu-rich sulphide melt that separated from a Ni-rich sulphide melt prior to magma emplacement and orbicule formation. The oxidation and Cu-enrichment of a sulphide melt that formed the mineralization in the orbicules and Koperberg Suite more generally began prior to the emplacement of the silicate Koperberg Suite magmas that formed the orbicules, suggesting no link between orbicule genesis and sulphide metallogenesis.
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    Utilizing legacy seismics and non-seismic geophysical methods for deep mineral targeting and near-surface characterization: implications for mine development planning
    (University of the Witwatersrand, Johannesburg, 2023) Mutshafa, Ndamulelo; Manzi, Musa
    This thesis demonstrates through several case studies how the reprocessing of legacy reflection seismic data using advanced algorithms can be of value to mineral exploration and mine development, especially in hard-rock environments. The thesis also showcases how the integration of seismic and non-seismic geophysical datasets can assist in delineating near- surface geological structures (e.g., boulders and fractures) for mine planning and designs. Papers I and II demonstrate how the reprocessed legacy reflection seismic data have been used to delineate and image the world-class gold deposits such as the Black Reef (BLR) and Ventersdorp Contact Reef (VCR) of the Witwatersrand goldfields in South Africa. The two legacy reflection seismic profiles (Paper I) were acquired in 1988 for deep mineral exploration and mine planning over an area that is dominated by dolomitic outcrops that cause scattering of seismic energy at the near-surface, preventing energy propagation into the subsurface. Various migration approaches, namely, pre-stack time, pre-stack depth, and post-stack time migration were applied to test their capabilities in improving structural imaging. Reprocessing results from the pre-stack depth migration using the Kirchhoff algorithm provided the most improved subsurface images, especially the deeper targets due to its ability to honour complex lateral variations in the velocity field. In addition, Kirchhoff's pre-stack and post-stack time migration techniques improved the continuity of the near-surface reflections below the dolomitic rocks. Paper II presents the results from the recovered and processed 25.3 km long legacy seismic survey that was acquired in 1983 by the Gold Division of Anglo-American as part of the Witwatersrand goldfields exploration program. The reprocessing of the data improved the imaging of the gold-bearing horizon termed Ventersdorp Contact Reef (VCR), which is situated at depths between ~2400 and ~4100 m below the ground surface near the South Deep mine in Fochville, South Africa. The pre-stack time and phase-shift migration approaches were tested during processing, and both revealed a dipping reflection associated with the gold-bearing horizon and major steeply dipping faults that crosscut and displace the deposit. The interpretation of the results was constrained using borehole logs and surface geology. This is encouraging and motivates the use of legacy seismic data in the exploration of deep-seated targets. Papers III, IV and V present the results from the use of multi-geophysical methods (resistivity, magnetics, seismic, ground penetrating radar and multichannel analysis of surface waves) at Tharisa platinum mine to provide a comprehensive understanding of the subsurface geology by accurately delineating and locating boulders, mapping fractures and groundwater aquifers to improve Platinum Group Elements (PGEs) mining efficiency and reduce risks. The results from these integrated geophysical methods were successful in complementing each other in terms of providing a clear picture of the near-surface geological structures to help the mine plan better for future operations.