2008
DOI: 10.3133/sim3046
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Bedrock Geologic Map of the Greater Lefkosia Area, Cyprus

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Cited by 12 publications
(15 citation statements)
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“…Ophiolite and slower wave speed underlying Anatolian continental crust (Mackenzie et al 2006;Feld et al 2017) may introduce receiver function complexity. Terrestrial sediments of thickness ∼3 km (Harrison et al 2008) surrounding the ophiolite may also generate additional P-to-S conversions (Fig. 1c).…”
Section: A S E S T U Dy 2 -T H E E T H I O P I a N T R A P S : N E mentioning
confidence: 99%
“…Ophiolite and slower wave speed underlying Anatolian continental crust (Mackenzie et al 2006;Feld et al 2017) may introduce receiver function complexity. Terrestrial sediments of thickness ∼3 km (Harrison et al 2008) surrounding the ophiolite may also generate additional P-to-S conversions (Fig. 1c).…”
Section: A S E S T U Dy 2 -T H E E T H I O P I a N T R A P S : N E mentioning
confidence: 99%
“…Recent P wave tomography interpretations largely support these geodynamic interpretations, including a large tear between the Cyprus and Aegean slabs, a minor tear between western Cyprus and the Isparta Angle (approximately along the Paphos transform (PT), Figure 1), and apparently no slab to the east of Cyprus [ Biryol et al , 2011]. Some authors have suggested that Cyprus itself overlies a locked portion of the subduction zone [e.g., Harrison et al , 2008]. Such locking may be linked to the collision of the Erathosthenes Seamount with the Cyprus Arc, as the collision appears to have induced structural changes throughout the E Mediterranean [ Schattner , 2010].…”
Section: Geologic and Tectonic Settingmentioning
confidence: 99%
“…Calon et al () identified that the Larnaca Ridge is uplifted in Middle to late Miocene time as the sediments are thick toward the north (away from the Ridge) but thin rapidly toward the Ridge. Mid‐Miocene thrusting activity is also identified onshore in the Mesaoria Basin (Cleintuar et al, ; Harrison et al, ) as the Ovgos Fault zone is thrusting the deeper Kythrea flysch Formation next to the shallower pelagic marls and chalks of the Pakhna Formation (Cleintuar et al, ).…”
Section: Discussionmentioning
confidence: 97%