“…highly idealized continental geometries (Hay et aI., 1990), atmospheric genernl circulation and oceanic circulation models (Kutzbach et aI., 1990), energy balance climate models (Crow1ey et aI., 1989), models based on analogies with the present-day (parrish, 1982) or general circulation simulations. Among other variables, these models include patterns of surface temperature, precipitation and evaporation balance and sea-level pressure parameters and have provided data on the role of continental configumtion as a climateforcing factor (Barron and Facett, 1995 A simple view of the latitudinal location and the topography of the Iberian Plate shown in the different global palaeogeographical maps for the Late Permian-PTB times (see for example Ziegler, 1988;Ziegler and Stampfli, 2001;Stampfli and Bore!, 2002) clearly allows us to infer a few basic palaeoclimatie characteristics for this western Tethysian area. The Iberian Plate was part of the Central Pangean Mountain Range, made up of the Appalachian-Mauretanide-Variscan orogenic belts that fonned as a result of the diachronous collision between Laurasia and Gondwana (Scotese and Lanford, 1995).…”