Distinguishing tectonically-and gravity-driven synsedimentary deformation structures along the Apulian platform margin (Gargano Promontory, southern Italy)
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- 作者：Irina Kornevaa ; irina.korneva@unicam.it" class="auth_mail" title="E-mail the corresponding author ; Emanuele Tondia ; Danica Jablonskaa ; Claudio Di Celmaa ; Ian Alsopb ; ian.alsop@abdn.ac.uk" class="auth_mail" title="E-mail the corresponding author ; Fabrizio Agostac ; fabrizio.agosta@unibas.it" class="auth_mail" title="E-mail the corresponding author
- 关键词：Apulian platform ; Maiolica formation ; Synsedimentary faults ; Slumps ; Mass-transport deposits
- 刊名：Marine and Petroleum Geology
- 出版年：2016
- 出版时间：May 2016
- 年：2016
- 卷：73
- 期：Complete
- 页码：479-491
- 全文大小：7833 K
文摘
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Synsedimentary faults along the Apulian margin are gravitational and tectonic.
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Gravity-driven and tectonic faults are orthogonal to each other along NE–SW margin.
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Gravity-driven and tectonic faults are sub-parallel along NW–SE margin.
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Different structural architecture of the margins helps to recognise origin of faults.
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The orientation and distribution of faults influence the migration of geofluids.