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Geological Society, London, Special Publications; 2006; v. 260; p. 507-520;
DOI: 10.1144/GSL.SP.2006.260.01.21
© 2006 Geological Society of London

A new orogenic model for the External Hellenides

T. Doutsos, I. K. Koukouvelas & P. Xypolias

University of Patras, Department of Geology, Division of Physical Geology, Marine Geology and Geodynamics, 265 00 Patras, Greece iannis{at}upatras.gr

In the context of the External Hellenides, ‘pro’-lithosphere, corresponding to the Apulian microcontinent, converges on ‘retro’-lithosphere, corresponding to the Pelagonian microcontinent. Structural and stratigraphic data in the External Hellenides suggest that the convergence at this margin is fairly well described by the conceptual doubly vergent accretionary wedge model. This new orogenic model for the External Hellenides differs from the classical west-verging assumption and emphasizes that the retro-mass flux is critical for the pro-mass flux. Our model is primarily 2D, and is described in terms of three system components: an accretionary wedge (or pro-wedge), an uplifted plug and a retro-wedge. Three ‘isopic’ zones (Pindos, Gavrovo-Tripolitsa and Ionian) are included in the pro-wedge. The uplifted plug in the north (Epirus area) includes the Pindos ocean ophiolitic rocks and the Pindos zone, the Parnassos zone in central Greece, and the HP belt of the External Hellenides in the Peloponnese. The retro-wedge includes the Mesohellenic Trough in the north and the Argos plain in the south.