2.2 Subproject 94 Sub-Project 2.2 Agulhas-Karoo Geoscience Transect: A land-sea deep crustal seismic, MT and petrological transect across the Agulhas Plateau, the Agulhas Fracture Zone, the Agulhas Bank, the Cape Fold Belt and into the Karoo Province Participants * Coordinators Institutions Names Email addresses Alfred Wegener Institute (AWI) K. Gohl* G.Uenzelmann-Neben kgohl@awi-bremerhaven.de guenzelmann@awi-bremerhaven.de GeoForschungs-Zentrum Potsdam (GFZ) O. Ritter* U. Weckmann M. Weber A. Schulze T. Ryberg oritter@gfz-potsdam.de uweck@gfz-potsdam.de mhw@gfz-potsdam.de robert@gfz-potsdam.de trond@gfz-potsdam.de University of Cape Town (UCT) H.E. Frimmel* G. Viola A.P. le Roex Z. Ben-Avraham M.J. de Wit hef@geology.uct.ac.za viola@geology.uct.ac.za aleroex@geology.uct.ac.za zba@geology.uct.ac.za maarten@cigces.uct.ac.za Council for Geoscience E. Stettler C. de Beer edgars@geoscience.org.za coenie@geobell.org.za Univ. Witwatersrand S. Webb sue@geophysics.geol.wits.ac.za Univ. Port Elizabeth R. Shone P. Booth glarws@upe.ac.za glapwb@upe.ac.za Univ. Natal M. Watkeys watkeys@nu.ac.za Univ. Stellenbosch R. Scheepers rsc@sun.ac.za Petroleum Agency of SA I. McLachlan mclachlai@petroleumagencysa.com Fugro Airborne Surveys L. Ameglio lameglio@fugroairborne.co.za Green’s Geophysics R. Green - Requested Funding Total for the 5-year duration project beginning in 2004: Euros 2381300 AWI GFZ RSA Totals 2004 0 101000 62600 163600 2005 461600 618000 131400 1211000 2006 74600 418000 99600 592200 2007 72600 168000 45800 286400 2008 72600 40500 15000 128100 2.2 Subproject 95 Summary Southern Africa and its southern continental margin offer an unrivalled region, where continental accretion processes over a period of more than 3.5 billion years can be studied. Along a geoscientific transect, stretching from the offshore Agulhas Plateau across the Agulhas Fracture and the Outeniqua Basin, continuing across the Cape Fold Belt, the Namaqua-Natal Belt and into the Karoo Province and the southern Kaapvaal Craton, geophysical and geological/ geochemical data and samples will be collected in order to build a model of the evolution and crustal accretion as well as the continental break-up of this region. With such a single transect, multifold significant objectives can be addressed such as the Mesoproterozoic accretion processes along the southern margin of the Kaapvaal Craton, the extent of Pan-African inliers in the Cape Fold Belt, the extent and formation of the Cape Fold Belt, the sources for the Beattie Magnetic Anomaly and the Southern Cape Conductivity Belt, the continental/ oceanic origin of the Agulhas Plateau, the formation of the Agulhas Fracture Zone and its consequences for basin formation and uplift processes relevant for the hydrocarbon producing provinces of the Outeniqua Basin. A combined land-sea deep crustal seismic reflection and refraction survey as well as a magnetotelluric survey along the transect will provide detailed structures and constraints for physical parameters from the upper crust to the upper mantle which will be integrated with geological, petrological and geochemical analysis on rock composition, age and alteration history to form an overarching geodynamic model for the evolution of the region and its tectonic units. 2.2 Subproject 96 Scientific Background Continents are known to be made up of a collage of displaced terranes of various origins that accumulate or accrete when continental margins are active. Today, oceanic plateaux, which can be extinct island arcs, extinct spreading ridges, seamounts, or disrupted fragments of continental crust, are passive features that are embedded within the oceanic lithosphere. When large enough, they resist subduction, do not return to the mantle but accrete to existing continents. A prime example of such an oceanic plateau is the Agulhas Plateau situated offshore southern Africa. It can be expected that this plateau will collide with the present African continent when the southern African margin becomes active again. Southern Africa offers an unrivalled region, where continental accretion processes over a period of more than 3.5 billion years can be studied: A composite Archean (>2.5 Ga) craton (Kaapvaal Craton) is flanked by progressively younger crust (Fig. 2.2.1), recording four main stages of continental lithosphere formation: 2.06 - 1.80 Ga (Eburnian) Kheis Belt, 1.2 - 1.0 (Grenvillian) Namaqua Natal Belt, 0.58 - 0.48 (Pan-African) Saldania Belt, and the 0.25 (Gondwanide) Cape Fold Belt. Large areas of the Namaqua-Natal Belt are covered by Mesozoic Karoo sediments, and most of the Saldania Belt is overlain by rocks of the younger Cape Fold Belt. Only a few exposures in form of basins such as the Kangoo and the Kaaimans Inlier can provide reliable data on tectonism which are vital for the understanding of accretion and collision in southern South Africa. The eastern margin of the craton has been reworked by Mesozoic Gondwana tectonic processes. This left a sharp break, manifest at the surface by the Lebombo monocline (a priority target of Subproject 2.3, see below). The best region to study the successive accretions of continental lithosphere onto the Kaapvaal Craton since its stabilisation around 2.0 Ga is its southern margin. The proposed geophysical (seismic and magnetotelluric) transect cuts across all of the above <2.0 Ga tectonic belts and thus also at least three major continental suture zones of vastly different age. The same area also hosts two of Earth’s largest known geophysical anomalies, the Beattie Magnetic Anomaly (BMA) and the Southern Cape Conductive Belt (SCCB). Both anomalies extend for almost 1000 km in eastwest direction across the whole of southern South Africa (Fig. 2.2.2). The surface expressions of these anomalies seem to coincide with the mapped boundaries of the Cape Fold Belt and the Namaqua Natal Belt. The nature of both geophysical anomalies remains enigmatic; they have been interpreted as a slice of paleo-oceanic lithosphere or alternatively as thrust zones, but neither their relative age nor their extent to depth and internal structure are known. A better understanding of their geometry and origin is essential for any meaningful reconstruction of the subsequent break-up processes. By extending the transect offshore to the Agulhas Plateau (Fig. 2.2.3), not only can the question of continent formation, but also that of the demise of continents be addressed. Late Mesozoic basins, both onshore and offshore, formed subsequent to Gondwana break-up. Today they are important exploration targets for the petroleum industry. The nature and origin of the Agulhas Plateau are poorly known and this project promises to provide major new insights into this oceanic plateau. Finally, the southern tip of South Africa, though surrounded by passive continental margins, displays a considerable relief. This gives rise not only to spectacular landscapes, but also to the recognition that southernmost Africa is affected by active neotectonic activity. Both causes and hazards as well as the utilization potential of this neotectonic activity are not fully understood. The proposed project, in conjunction with the other Working Groups, offers an opportunity to address these issues. 2.2 Subproject 97 Figure 2.2.1. Distribution of tectonic units around the Archaean Kaapvaal Craton in southern Africa. Large parts of the Namaqua Natal Belt and the southern segment of the Kaapvaal Craton are covered with Karoo sediments. Fig. 2.2.2. The Beattie Magnetic Anomaly (red and magenta colours and white dots) and the Southern Cape Conductive Belt (SCCB, black and white dashed lines) are continental scale geophysical anomalies. They stretch from east to west for more than 1000 km across the whole of southern South Africa (after Harvey et al., 2001). 2.2 Subproject 98 Fig. 2.2.3. (Top) Proposed offshore seismic transects across the Agulhas Plateau and the southern margin of the African plate. (Bottom) Proposed geophysical transects across the SCCB and the BMA. (Yellow: onshore/offshore seismic experiment, blue: near vertical reflection seismic, red: magnetotelluric profiles) 2.2 Subproject 99 Key references Allen, R.B., Tucholke, B.E. (1981). Petrography and implications of continental rocks from the Agulhas Plateau, southwest Indian Ocean. Geology, 9, 463-468. Bauer, K., Schulze, A., Ryberg, T., Sobolev, S. V. and Weber, M. (2003): Classification of lithology from seismic tomography. A case study from the Messum igneous complex, Namibia. Journ. Geophys. Res., 108(B3), 2152, doi: 10.1029/2001JB001073 . Ben-Avraham, Z., Hartnady, C.J.H., Malan, J.A. (1993) Early tectonic extension between the Agulhas Bank and the Falkland Plateau due to the rotation of the Lafonia microplate. Earth Planet. Sci. Lett. 117, 43-58. Ben-Avraham, Z., Hartnady, C.J.H., le Roex, A.P. (1995) Neotectonic activity on continental fragments in the southwest Indian Ocean: Agulhas Plateau and Mozambique Ridge. J. Geophys. Res., 100, 6199-6211. Ben-Avraham, Z. (1995) Neotectonic activity offshore southeast Africa and its implications, S. Afr. J. Geol., 98, 202-207. Ben-Avraham, Z., Hartnady, C.J.H., Kitchin, K.A. (1997) Tectonics of the Agulhas-Falkland transform. Tectonophys.,282, 83-98. Frimmel, H.E., Hartnady, C.J.H., Koller, F. (1996) Geochemistry and tectonic setting of magmatic units in the Pan-African Gariep Belt, Namibia. Chem. Geol., 130, 101-121. Frimmel, H.E., Frank, W. (1998) Neoproterozoic tectono-thermal evolution of the Gariep Belt and its basement, Namibia/South Africa. Precambr. Res., 90, 1-28. Frimmel, H.E., Fölling, P.G., Diamond, R. (2001) Metamorphism of the Permo-Triassic Cape Fold Belt and its basement, South Africa. Mineral. Petrol., 73, 325-346. Frimmel, H.E., Fölling, P.G., Eriksson, P. (2002) Neoproterozoic tectonic and climatic evolution recorded in the Gariep Belt, Namibia and South Africa. Basin Research, 14, 55-67. Frimmel, H.E. (in press a) Neoproterozoic sedimentation rates and timing of glaciations - a southern African perspective. - In: Condie, K C, Veenstra, F (eds.) Tempos and Events in Precambrian Time, Elsevier (Amsterdam). Frimmel, H.E. (in press b) Formation of a late Mesoproterozoic supercontinent: The South Africa East Antarctica connection. In: Condie, K.C., Veenstra, F. (eds.) Tempos and Events in Precambrian Time, Elsevier (Amsterdam). Gohl, K. & Uenzelmann-Neben, G. (2001). The crustal role of the Agulhas Plateau, southwest Indian Ocean: evidence from seismic profiling. Geophys. J. Int., 144, 632-646. Hartnady, C.J.H., Ben-Avraham, Z., Rogers, J. (1992) Deep-ocean basins and submarine rises off the continental margin of southeastern Africa: new geological research developments. South African J. Sci., 88, 534-539. Harvey, J.D., de Wit, M.J., Stankiewicz, J., and Doucouré, M. (2001). Structural variations of the crust in the southwestern Cape derived from seismic receiver functions. S A Journal Geology, 104, 231-242. Lyakhovsky, V., Ben-Avraham, Z., Reznikov, M. (1994) Stress distribution over the Mozambique Ridge. Tectonophys., 240, 21-27. McMillan, I.K., Brink, G.J., Broad, D.S. & Maier, J.J. (1997). Late Mesozoic sedimentary basins off the south coast of South Afrika. In: Selley, R.C. (Ed.), Sedimentary Basins of the World: The African Basins. Elsevier, Amsterdam, 319-376. Niemi, T.M., Ben-Avraham, Z., Hartnady, C.J.H. (2000) Post-Eocene seismic stratigraphy of the deep ocean basin adjacent to the southeast African continental margin: a record of geostrophic bottomcurrent systems. Marine Geology, 162, 237-258. Raith, J.G., Cornell, D.H., Frimmel, H.E., de Beer, C.H. (2003) New insights into the geology of the Namaqua Tectonic Province, South Africa, from ion microprobe dating of detrital and metamorphic zircon. J. Geol., in press. Ritter, O., Weckmann, U., Vietor, T. and Haak, V. (2003) A magnetotelluric study of the Damara Belt in Namibia 1. Regional scale conductivity anomalies, Phys. Earth Planet. Inter., 138:71-90, 2003, doi:10.1016/S0031-9201(03)00078-5 Ritter, O., Ryberg, T., Weckmann, U., Hoffmann-Rothe, A., Abueladas, A., and Garfunkel, Z., (2003) Geophysical images of the Dead Sea Transform in Jordan reveal an impermeable barrier for fluid flow, Geophys. Res. Lett., 30(14):1741-1744, 2003, doi:10.1029/2003GL017541 2.2 Subproject 100 Tucholke, B.E., Houtz, R.E., Barrett, D.M. (1981). Continental crust beneath the Agulhas Plateau, southwest Indian Ocean. Journal of Geophysical Research, 86, 3791-38061. Uenzelmann-Neben, G., Gohl, K., Ehrhardt, A. & Seargent, M.J. (1999). Agulhas Plateau, SW Indian Ocean: New evidence for excessive volcanism. Geophys. Res. Lett., 26, 1941-1944. Uenzelmann-Neben, G. (2001). Seismic characteristics of sediment drifts: An example from the Agulhas Plateau, southwest Indian Ocean. Marine Geophysical Researches, 22, 323-343 . Uenzelmann-Neben, G. (2003). Contourites on the Agulhas Plateau, SW Indian Ocean: Indications for the evolutions of currents since Paleogene times. In: Stow, D., Pudsey, C., Howe, J., Faugeres, J.C., Viana, A.R. (eds), Deep-water contourite systems: Modern drifts and ancient series. Geological Society of London, Memoir, 22, 271-288. Weckmann, U., Ritter, O. and Haak, V. (2003) A magnetotelluric study of the Damara Belt in Namibia 1. MT phases over 90° reveal the internal structure of the Waterberg Fault/Omaruru Lineament, Phys. Earth Planet. Inter., 138:91-112, 2003, doi:10.1016-S0031-9201(03)00079-7 Key questions arising are: Does the Mesoproterozoic crust continue from the Namaqua Belt in the west to the Natal Belt in the east? If yes, what is the geometry of this belt along the southern flank of the Kaapvaal Craton? How much and what type of Neoprotererozoic crust exists to the south of the Kaapvaal Craton? Are some (and if yes, which) of the Pan-African inliers in the Cape Fold Belt synorogenic intramontane molasse basins? What is the Pan-African kinematic history of these inliers and how does it relate to that of the Gariep Belt and the Ross Orogen? What is the subsurface geometry of major tectonic and stratigraphic boundaries within the Cape Fold Belt; how do the features mapped on the surface continue to depth? To what extent can the Cape Fold Belt be followed off-shore to the south? Do the Beattie magnetic anomaly and the Southern Cape Conductivity Belt (SCCB) have the same source? Can we resolve structural details within the SCCB and its depth extent? Is the SCCB caused by partially serpentinized rocks or is it connected with tectonic processes of the orogenic front (Cape Fold Belt)? Is the Agulhas Plateau oceanic or continental? What is the age and the source of the volcanics of the Agulhas Plateau and how can the magmatic volume added to the Agulhas Plateau and its surroundings be quantified? Under what geodynamic process did the sheared margin of South Africa evolve? What is the origin of the Agulhas Fracture Zone? Has any magmatism been associated with break-up along the Agulhas Fracture Zone, and has the Fracture Zone been reactivated through present times? How did the Outeniqua Basin form and what is the nature of the underlying basement and deep crust? Objectives Ten main objectives to be addressed within a number of sub-projects are briefly explained below in a sequence that reflects the progressively younger ages of geological phenomena of interest: 2.2 Subproject 101 Nature of the basement to the Karoo Supergroup rocks and the extent to which it fits into a postulated contiguous Namaqua-Natal Belt: The new geophysical data are expected to provide new insights into the geometry of the main Mesoproterozoic crustal structures and thus yield crucial information for the modelling of Mesoproterozoic accretion processes along the southern margin of the Kaapvaal Craton. A combination of petrological, structural and geochemical studies, combined with the geophysical data, are aimed at assigning the various tectono-stratigraphic units of the Saldania Belt (Fig. 2.2.4) to the different stages of Pan-African basin development and to place them into a regional, intercontinental framework of Gondwana assembly. Particularly their relationship to other Pan-African units along the western margin of southern Africa (Gariep, Damara, Kaoko Belt and equivalents in South America) and the Ross Orogen in Antarctica will be tested. The expected geophysical data will be supplemented by systematic ground gravimetric measurements on the George Pluton and surrounding rocks in order to delineate the shape of the pluton at depth, calculated by gravity data inversion, and also its spatial relationships with the surrounding rocks. The accretion process that gave rise to the Cape Fold Belt remains enigmatic, as no highgrade metamorphic core complexes or syn-orogenic igneous activity are known. The new geophysical data, combined with extensive structural and stratigraphic studies, will serve as basis on which to establish the geometry of major tectonic features by tracing tectonic and stratigraphic boundaries from surface outcrops into depth through the crust. The up to 200 km wide SCCB was mapped in the late 1960s by means of magnetometerarray studies with stations separated by tens to hundreds of kilometers. A common source for the BMA and the SCCB has been proposed by several authors but remains uncertain because direct observations are missing. Preliminary seismic work across the BMA indicates zones of high reflectivity in the upper crust, while receiver functions studies identify sharp crustal discontinuities at depths of 8 and 18 km which are interpreted as a 10km thick block of altered Mesoproterozoic mafic-ultramafic rocks. However, this is by no means the only possible interpretation and we note that in some cases, low-resolution geophysical data sets are more a hindrance than a help for geodynamic understanding. For example the interpretation of the SCCB, as a serpentinized slice of paleo-oceanic crust is doubtful in view of recent magnetotelluric investigations with a much higher resolution from the Damara Mobile Belt in Namibia (Ritter et al., 2003). This new data set resolves the internal structure of a comparable high conductivity belt and shows clearly that conductive zones correlate with deep reaching fossil shear zones. Thermo-mechanical forward modelling of the terrane accretion/ continental collision will investigate the geodynamic significance of the BMA and SCCB geophysical anomalies. One process we wish to model is the progressive magnetisation of crustal rocks as they pass the Curie isotherm during syntectonic and posttectonic exhumation. Additionally, the distribution of strain within the models will shed light on the distribution of the shear zones and their final geometry in the eroded orogen. The results will be applicable to collisional settings in general. The extensional history of the Cape Fold Belt related to the break-up of Gondwana during the Mesozoic will form part of the study, where normal faults and related structures can be identified along the planned transect through the Cape Fold Belt. 2.2 Subproject 102 The nature of the Agulhas Plateau (oceanic versus continental) and the amount of magmatic material added to it at various times is a premier target of the offshore studies. Recent deep seismic surveying of the southern central Agulhas Plateau indicates very high P-wave velocities (>7 km/s) in the lower two-thirds of the 25 km thick crustal column, suggesting an oceanic crustal affinity. However, this is in conflict with the interpreted continental origin of quartzo-feldspathic samples dredged from the plateau. It is uncertain if the observed velocity-depth distribution is symptomatic for the entire plateau or if continental crustal fragments are embedded in the plateau. An important aim is to understand the role of young volcanism near the northern Agulhas Plateau. Origin of the Agulhas Fracture Zone and its relationship to the separation of the Falkland Plateau. Furthermore, the question of any magmatism having been associated with breakup and the tectonic as well as magmatic consequences of possible repeated re-activation of the fracture zone along the continental margin will be addressed. On the Outeniqua Basin of the Agulhas Bank, the nature and position of the crust-mantle boundary will be examined, as well as the development of the oil-producing sedimentary basin and its deep-seated fractures during break-up. C dt e an err e ran ter rg nd rbe e ge an Ty terr 33 S l an Bo la art Sw o A P E Mid-Palaeozoic to Cenozoic cover Gamtoos Group Cape Granite Suite Klipheuwel Group Kaaimans Group Kansa Subgroup Kango Goegamma Subgroup Group Boland Subgroup Malmesbury Tygerberg Subgroup Group Swartland Subgroup Kango inlier Worcester FOL D Gamtoos inlier Oudtshoorn BELT Cape Town 34oS Port Elizabeth Kaaimans inlier Atlantic Ocean o 18 E N Indian Ocean o 20 E 22oE o 24 E Fig. 2.2.4. Distribution of Pan-African units within the Cape Fold Belt. Methodologic approach and techniques Seismic onshore/offshore experiments Two offshore multichannel reflection and refraction/wide-angle seismic profiles will be conducted (see Fig. 2.2.3). While both profiles cross the sheared margin of the Agulhas Fracture Zone, one profile is primarily aimed for imaging the deep structure of the Agulhas Plateau, and the other profile targets the Outeniqua Basin and the transition to the Cape Fold Belt. The latter profile will be supplemented by a simultaneous onshore wide-angle seismic line (WRR) which extends for approximately 300 km into the Cape Fold Belt. From the 2.2 Subproject 103 combined experiment we intend to resolve structural details of the Agulhas Fault Zone and the velocity structure of the ocean continent transition. This marine part of the project will be conducted in cooperation with Working Group 3, Sub-Project “Neogene evolution of the southern African margin related to tectonism, ocean currents and changes in sea-level”. A proposal (AISTEK-I) for shiptime on RV Sonne was submitted to PTJ-BMBF (Germany). The positive review resulted in a recommendation that this project be included in the next RV Sonne cruise schedule. Combined near vertical reflection (NVR) seismic and magnetotelluric (MT) experiments. Two combined high resolution seismic and MT experiments (MT1, MT2 and NVR1 and NVR2) are planned to resolve the crustal constitution of the Cape Fold and Namaqua-Natal mobile belts. The first profile coincides with the onshore part of the onshore/offshore line from the coast across the Cape Fold Belt. This profile will be continued northwards in a second field experiment. Focus of this experiment will be the deep structures of the NamaquaNatal Mobile belt and particularly the Beattie Magnetic Anomaly. The combined length of these onshore profiles is approximately 300 km. They cross major accretionary complexes and the above mentioned continental scale geophysical anomalies (see Fig. 2.2.2). Along this profile we plan to extend the already successfully tested method of so-called petrotomography (Bauer et al., 2003) to greater depths. This gives a unique opportunity to map the subsurface distribution of petrological units to depths as much as approx. 10 km. The electrical image of the Namaqua-Natal Belt to Kaapvaal Craton transition Most of the Namaqua-Natal Mobile Belt and particularly its northern boundary into the Kaapvaal Craton are obscured by the Karoo sedimentary cover (see Fig. 2.2.1). Magnetotelluric measurements can potentially identify large scale paleo-shear zones and may be able to resolve the craton boundary at depth. Acquiring seismic and magnetotelluric data along coincident profiles is an excellent opportunity to utilize the combined imaging power of the two methods. The coverage of the craton boundary will require a continuation the magnetotelluric profiles mentioned above in a northeastern direction for approximately 200 km. Geochemical/geochronological studies Provenance and geochronological studies of surface samples from the Pan-African inliers within the Cape Fold Belt for establishing their stratigraphic position within the regional framework of Pan-African belts. Collecting (dredging) samples from outcropped basement of several sites of the Agulhas Plateau will provide data on the composition and age of the volcanics as well as potential continental rocks. The geochemical analysis will be integrated with the geophysical data for build a consistent evolutionary model. Structural Geology Structural geological studies to delineate the lateral distribution of stratigraphic and tectonic units within the Cape Fold Belt. 2.2 Subproject 104 Drilling of the Agulhas Plateau and the Beattie Magnetic Anomaly In addition to dredging rock samples off the sea-floor, drilling into the basement at several sites of the Agulhas Plateau would provide invaluable information about the origin and evolutionary process of the plateau’s crust. Participation in the IODP proposal ISOLAT with a site on the plateau or even a separate drill proposal is aimed for within this project. Continental deep drilling of the Beattie magnetic anomaly, accompanied with intensive geophysical, petrological and geochemical analyses may be the only way to really understand (in situ) the true nature of this major anomaly. Thermo-mechanical numerical modelling of continental collision Forward models of collisional settings simulate the progressive magnetisation of crustal rocks while they pass the Curie isotherm during syn-tectonic and post-tectonic exhumation. Modelling strain distribution will shed light on the distribution and geometry of shear zones in the eroded orogen. Logistic/equipment requirements Access to a suitable research vessel for conducting new seismic reflection and refraction lines and petrological sampling (RV Sonne approval for seismic work is pending); Access to existing seismic lines of Agulhas Bank (Petroleum Agency of SA); Access to existing seismic lines across the Cape Fold Belt and southern Natal Belt (Council for Geoscience); Access to gravity and magnetic data acquisition equipment; Drilling facilities (on- and offshore); Access to analytical facilities for petrological, geochemical and geochronological studies (EMPA, SHRIMP or equivalent single mineral grain dating facility, XRF, ICP-MS). Expected outcomes/deliverables Better understanding of the nature and significance of lithospheric structures in continental break-up processes. Documentation of the crustal architecture of southern Africa and its continental margins; Improved understanding of the relation of geophysical anomalies to geodynamics of accretion/collision Significant improvement in the understanding and quantification of asthenospherelithosphere mass transfer; Reconstruction of Mesozoic paleo-geography; 2.2 Subproject 105 Estimated Funding Requirements Manpower: (all salaries are based on the German public service scale (BAT)) 1 post-doc for marine deep crustal seismic data geodynamic modelling Administrative: AWI Salary group: BAT IIa (€ 4800/month) Duration: 01/2005 – 12/2005 01/2006 – 12/2006 01/2007 – 12/2007 01/2008 – 12/2008 processing, modelling and interpretation; € € € € 57,600 57,600 57,600 57,600 subtotal: € 230,400 1 post-doc for wide-angle reflection/refraction seismic (WRR) data processing, modelling and interpretation; lithospheric evolution of southern African continent Administrative: GFZ Salary group: BAT IIa-O (€ 4250/month) Duration: 01/2005 – 12/2005 € 51,000 01/2006 – 12/2006 € 51,000 01/2007 – 12/2007 € 51,000 subtotal: € 204,000 1 PhD student for near vertical reflection seismic (NVR) data processing, modelling and interpretation; lithospheric evolution of southern African continent Administrative: GFZ Salary group: BAT IIa-O/2 (€ 2125/month) Duration: 01/2005 – 12/2005 € 25,500 01/2006 – 12/2006 € 25,500 01/2007 – 12/2007 € 25,500 subtotal: € 76,500 1 post-doc for magnetotelluric surveys MT1, MT2 and MT3; experiment coordination; data acquisition, processing, modelling Administrative: GFZ Salary group: BAT IIa-O (€ 4250/month) Duration: 07/2004 – 12/2004 € 25,500 01/2005 – 12/2005 € 51,000 01/2006 – 12/2006 € 51,000 01/2007 – 12/2007 € 51,000 01/2008 – 06/2008 € 25,500 subtotal: € 204,000 1 PhD student for magnetotelluric survey MT1 and MT2; integrated modelling of MT and seismic NVR data Administrative: GFZ Salary group: BAT IIa-O/2 (€ 2125/month) 2.2 Subproject Duration: 106 01/2004 – 12/2004 01/2005 – 12/2005 01/2006 – 12/2006 € 25,500 € 25,500 € 25,500 subtotal: € 76,500 subtotal: € 86,400 1 PhD student for sediment provenance/stratigraphic studies Administrative: RSA Salary group: BAT IIa/2 (€ 2400/month) Duration: 01/2004 – 12/2004 € 28,800 01/2005 – 12/2005 € 28,800 01/2006 – 12/2006 € 28,800 1 PhD student for petrology/geochemistry of Agulhas Plateau samples Administrative: RSA Salary group: BAT IIa/2 (€ 2400/month) Duration: 01/2005 – 12/2005 € 28,800 01/2006 – 12/2006 € 28,800 01/2007 – 12/2007 € 28,800 subtotal: € 86,400 3 MSc students for structural geological work in the Cape Fold Belt Administrative: RSA Salary group: 3 x € 1200/month Duration: 01/2004 – 12/2004 € 14,400 01/2005 – 12/2005 € 14,400 subtotal: € 28,800 1 MSc student for ground gravimetric study of George Pluton Administrative: RSA Salary group: € 1200/month Duration: 01/2004 – 12/2004 € 14,400 01/2005 – 12/2005 € 14,400 subtotal: total staff: € 28,800 ========= €1,021,800 Field work (excluding ship costs): Magnetotelluric surveys MT1, MT2 and MT3 (3 x 100 km profile) Administrative: GFZ Duration: 02/2004 – 04/2004 € 50,000 02/2005 – 04/2005 € 50,000 02/2006 – 04/2006 € 50,000 subtotal: € 150,000 subtotal: € 380,000 Marine seismic survey (instrument operating/rental costs, freight, consumables) Administrative: AWI Duration: 02/2005 – 03/2005 € 380,000 2.2 Subproject 107 WRR seismic survey (300 km profile) Administrative: GFZ Duration: 02/2005 – 03/2005 € 200,000 subtotal: € 200,000 subtotal: € 400,000 subtotal: € 50,000 subtotal: € 10,000 NVR1 and NVR2 seismic surveys (2 x 100 km profile) Administrative: GFZ Duration: 03/2005 – 04/2005 € 200,000 03/2006 – 04/2006 € 200,000 Petrological, geochemical and geo-chronological studies Administrative: RSA Duration: 01/2005 – 12/2005 € 25,000 01/2006 – 12/2006 € 25,000 Structural geology studies Administrative: Duration: RSA 07/2004 – 12/2004 01/2005 – 06/2005 € € 5,000 5,000 total field work: ========= € 1,190,000 Travel expenses: a) Congresses and workshops: Participation of project scientists at scientific congresses Basis: 1 international (2000 €), 1 national (1000 €) per year for 5 scientists Administrative: GFZ Time frame: 2005-2008 € subtotal: € 60,000 60,000 Participation of project scientists at scientific congresses Basis: 1 international (2000 €), 1 national (1000 €) per year for 5 scientists Administrative: AWI Time frame: 2005-2008 € subtotal: € 60,000 60,000 Participation of project scientists at scientific congresses Basis: 1 international (2000 €), 1 national (1000 €) per year for 5 scientists Administrative: RSA Time frame: 2005-2008 € subtotal: € 60,000 60,000 Annual project workshops, alternately in Germany and South Africa Basis: 10 participating scientists, 1 week duration Time frame: 2004-2008 subtotal: € 100,000 € 100,000 2.2 Subproject 108 b) Training courses for South African students: Seismic training of one South African student at AWI (4 months) Administrative: AWI Time frame: 2005 subtotal: Seismic/MT training of one South African student at GFZ (4 months) Administrative: GFZ Time frame: 2006 Subtotal total travel: € € 7,000 7,000 € € 7,000 7,000 ========= € 366,000 2.2 Subproject Project plan and timetable 109