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By H. Berckhemer, K. Hsü

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Published via the yankee Geophysical Union as a part of the Geodynamics Series.

The ultimate record on geodynamic examine within the Alpine-Mediterranean zone will be incomplete with out a short historic comic strip at the constitution and actions of ICG-Working team three. it may even be seemed an appreciation to the contributors and sponsors of the operating staff who've taken, over decades, an energetic half within the lifetime of the operating workforce and thereby contributed to the striking growth in our wisdom and figuring out of the geological evolution of this advanced quarter.

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These boundaries define numerous small 'plates' whose displacement history is constrained only by the nature of their boundaries. Whilst this approach incorporates a formidable quantity of evidence it presents methods. diagnosis an difficulties not encountered in other It is critically dependent on correct of plate boundary nature and position, exercise which we have shown to be difficult. The positions of the minor plates are simply 'educated guesses' [Dewey et al. 3138]. The emphasis on plate boundaries rather than on continental margins leaves the continents as illdefined shapes on which it is difficult to locate new data.

85, 1195-1204, 1974. R. , Limits to the expansion of Earth, Moon, Mars and Mercury and to changes in the gravitational constant. Nature. , 271, 316-321, 1978. , region. Plate tectonics Nature. 1970. , Active tectonics of the Mediterregion. Geophys. J. R. astron. , 30, 109-185, 1972. , The East Anatolian Fault: A major structure in eastern Turkey. Earth Planet. Sci. , 29, 189-193, 1976. , Can plate tectonics describe continental deformation? In Biju-Duval, B. & Mon- tadeft, 123, Vol. 7 L. (eds) 'Structural history of the Mediterranean basins', Editions Technip, Paris, 189-196, 1977.

Position of Spain against France and Newfoundland [1965]. depth as thinned areas as still from Bullard, 'sal' thinner (=sial), sial or Everett with 'trous 14. 358]. It is not clear what the guiding principles were for these insights. Though they would be criticized today mainly on the grounds of timing, they are fundamental to any tectonic interpretation. 191-192] believed that many sinuous orogenic belts had been formed by the bending of an originally straight chain. He named such chains 'oroclines', and the wedgeshaped spaces between two subsequently separated stable blocks as 'sphenochasms' [p.

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