Syn-kinematic strata influence the structural evolution of emergent fold-thrust belts

Robert W.H. Butler (Corresponding Author)

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Abstract

Whether thrusts are ramp-dominated and form imbricate fans, or run out onto the synorogenic surface, forming “thrust-allochthons”, is governed by the activity of secondary “upper” detachments along the syn-orogenic surface, activations of which are inhibited by syn-kinematic sedimentation at the thrust front. In the northern Apennines, where thrust systems are ramp-dominated and form an emergent imbricate fan, syn-kinematic sedimentation was abundant and accumulated ahead and above each thrust. In the southern Apennines, the far-travelled Lagronegro allochthon achieved its high displacements (>65 km) while the foredeep basin received little sediment. The imbricate fan at the front of the main Himalayan arc developed within a foredeep that experienced high rates of syn-kinematic sedimentation. In contrast, further west, the Salt Range Thrust emerged into a distal, weakly developed foredeep with significantly reduced rates of sediment accumulation. Displacements were strongly localized onto this thrust (c 25 km displacement) which activated an upper detachment along the synorogenic surface. It is an arrested thrust-allochthon. Lateral variations into the adjacent, ramp-dominated but still salt-detached, Jhelum fold-belt is marked by increases in synkinematic sedimentation. As sedimentation styles can vary in space and time, individual thrusts and thrust systems can evolve from being allochthon-prone to imbricate-dominated.
Original languageEnglish
Pages (from-to)1-22
Number of pages22
JournalGeological Society Special Publications
Volume490
Early online date15 Aug 2019
DOIs
Publication statusPublished - 1 Oct 2019

Keywords

  • imbricate stacks
  • NW Himalayas
  • Salt Range
  • Apennines
  • thrust-allochthons

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