Orocline (Figure 1d). This orocline has been suggested based on (1) paleomagnetic data showing block rotations of forearc basin terranes around vertical axes (Geeve et al., 2002; Klootwijk, 2009; Cawood et al., 2011b); (2) the recognition of a contorted serpentinite belt (Korsch and Harrington, 1987); and (3) the curved structure delineated by Early Permian (298-288 Ma) granitoids (Rosenbaum, 2010; Rosenbaum et al., 2012). Nevertheless, structural information supporting the existence of this orocline is more ambiguous. Based on the lateral continuation of early Permian granitoids, an even more complex structural model that involves four bends, has been proposed (Rosenbaum, 2010; Rosenbaum et al., 2012) (Figure 1e). The suggested fourth bend has been named the Nambucca Orocline (Rosenbaum, 2010). The kinematics associated with the development of the New England oroclines is relatively poorly constrained, with only patchy structural, paleomagnetic and geochronological data. In this respect, 'orocline' is used here in a general sense, as referring to orogenic curvatures rather than the strict sense that implies a secondary bending of an originally linear belt (Weil and Sussman, 2004). This paper aims to highlight the structure of the oroclines by outlining the spatiotemporal distribution of different tectonic elements within the southern NEO. This will be followed by a discussion on the large-scale tectonic implications of this spectacularly contorted orogenic structure. Tectonic elements Devonian-Carboniferous subduction complex The greater part of the exposed southern NEO is a Devonian-Carboniferous convergent margin complex (Figure 2) comprising forearc basin rocks of the Tamworth Belt and correlative terranes, and accretionary metasedimentary rocks of the Tablelands Complex. These domains are separated from each other by a tectonic contact, the Peel-Manning Fault System (PFZ and MFZ in Figure 1b), along which a lithological assemblage of serpentinites, blueschists and eclogites, is exposed. This assemblage, hereinafter referred to as the 'serpentinite belt' (Korsch and Harrington, 1987; Aitchison et al., 1994; Och et al., 2003), is most prominent along a long (c. 150 km), A series of tight bends (oroclines) are recognised in the late Paleozoic-early Mesozoic southern New England Orogen between Brisbane and Newcastle, but their exact geometry and tectonic evolution are still debated. This contribution provides an outline of the different tectonic elements within the orogen and the relationships of these elements with the oroclinal structure. Pre-oroclinal tectonic elements were derived from a Devonian-Carboniferous subduction zone, and include forearc basin terranes and accretionary wedge rocks that are separated from each other by a narrow belt of serpentinites and high-pressure rocks. Rocks are predominantly steeply dipping and their map-view pattern delineates three bends: the Z-shaped Texas and Coffs Harbour oroclines in the north and the U-shaped Manning Orocline in the south. During the early Permian (298-2...