2018
DOI: 10.1111/bre.12328
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Tectonic and oceanographic process interactions archived in Late Cretaceous to Present deep‐marine stratigraphy on the Exmouth Plateau, offshore NW Australia

Abstract: Deep‐marine deposits provide a valuable archive of process interactions between sediment gravity flows, pelagic sedimentation and thermohaline bottom‐currents. Stratigraphic successions can also record plate‐scale tectonic processes (e.g. continental breakup and shortening) that impact long‐term ocean circulation patterns, including changes in climate and biodiversity. One such setting is the Exmouth Plateau, offshore NW Australia, which has been a relatively stable, fine‐grained carbonate‐dominated continenta… Show more

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Cited by 27 publications
(21 citation statements)
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“…Massive and/or repetitive mass‐wasting processes as documented in stage 1 can be caused by tectonic activities, resulting in MTD‐dominated sedimentation in the deep‐water environments (Figure 13b). This tectonic‐driven sedimentation pattern has been reported in many areas of the world (Frey Martínez et al., 2005; Gamboa, Alves, Cartwright, & Terrinha, 2010; Hampton, Lee, & Locat, 1996; Moscardelli et al., 2006; Nugraha et al., 2019; Pickering & Corregidor, 2005). In particular, in the fold‐and‐thrust belts, a variation of the source area, distribution, and geometry of MTDs could reflect the evolution of thrust faults and related folds (Festa, Ogata, Pini, Dilek, & Codegone, 2015; Ortiz‐Karpf et al., 2018).…”
Section: Discussionsupporting
confidence: 66%
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“…Massive and/or repetitive mass‐wasting processes as documented in stage 1 can be caused by tectonic activities, resulting in MTD‐dominated sedimentation in the deep‐water environments (Figure 13b). This tectonic‐driven sedimentation pattern has been reported in many areas of the world (Frey Martínez et al., 2005; Gamboa, Alves, Cartwright, & Terrinha, 2010; Hampton, Lee, & Locat, 1996; Moscardelli et al., 2006; Nugraha et al., 2019; Pickering & Corregidor, 2005). In particular, in the fold‐and‐thrust belts, a variation of the source area, distribution, and geometry of MTDs could reflect the evolution of thrust faults and related folds (Festa, Ogata, Pini, Dilek, & Codegone, 2015; Ortiz‐Karpf et al., 2018).…”
Section: Discussionsupporting
confidence: 66%
“…The poor continuity and chaotic reflectors of this seismic facies indicate that rapid and non‐uniform deposition predominantly occurred. Many studies suggest that these seismic expressions derived from the MTD formed by slope deformational processes, including slide, slump and debris flow with plastic behaviour (Table 1; Brackenridge, Nicholson, Sapiie, Stow, & Tappin, 2020; Kim et al., 2020; Lee et al., 2001; Moernaut & De Batist, 2011; Nugraha, Jackson, Johnson, Hodgson, & Reeve, 2019; Pérez et al., 2016; Posamentier & Martinsen, 2011; Tournadour et al., 2015). SF2 is characterised by parallel and continuous well‐stratified reflections with high amplitude (Table 1).…”
Section: Data Sets and Methodologymentioning
confidence: 99%
“…We adopt the seismic-stratigraphic framework of Nugraha et al (2018), which is based on their analysis of the Exmouth Plateau, c. 50 km SW of the study area (Figure 2a). Our study interval falls within SU3 of Nugraha et al (2018), within which we map four horizons based on the seismic continuity, amplitude, and frequency/spacing, as well as the seismic facies characteristics of the packages they bound. The lithology and geotechnical properties (i.e.…”
Section: Dataset and Methodologymentioning
confidence: 99%
“…We divide the studied stratigraphic interval into three seismic units (SU-1-3). SU-1 is c. 500 m thick near the axis of the Kangaroo syncline, thinning westward and eastward to c. 200 m. SU-1 contains packages of chaotic, medium-to high-amplitude seismic reflections interpreted as stacked MTCs (Figure 3b-c) (Hengesh et al, 2012;Nugraha et al, 2018). SU-2 is thinner than SU-1, but also varies in thickness, being slightly thicker near the centre of the Kangaroo Syncline (c. 60 m) and thinning gradually westward and eastward to c. 30 m (Figure 3b).…”
Section: Su-1 and Su-2mentioning
confidence: 99%
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