Spatial and temporal variation of Syrian Arc structures in the onshore and offshore Eastern Mediterranean region

Abstract Syrian Arc structures form a belt of folds and faults oriented northeast to southwest and north-northeast to south-southwest extending from the Western Desert of Egypt (and farther westward to Tunisia) via northern Sinai to Levant eastward. Detailed studies of surface and subsurface areas in onshore Egypt as well as the offshore Eastern Mediterranean show evidence for continued deformation since the Santonian with local mild start during the Turonian. Santonian deformation was the strongest, whereas the later continued deformation was less. Previous studies of Syrian Arc structures proposed discrete phases of deformation, but the present study shows evidence that deformation was continuous since the Santonian. The lack of a continuous rock record, erosion of the crestal areas of some folds, nondeposition of younger sediments, and the scattered nature of younger rocks at the exposed Syrian Arc folds led some investigators to propose a short period(s) of Syrian Arc deformation. The relatively well-preserved subsurface stratigraphic record of Syrian Arc structures in some onshore and offshore areas led to the conclusion that the Syrian Arc folding continued to present time. However, the intensity of deformation and the associated structural relief have varied through time and space with its climax during Santonian time. We consider the Late Cretaceous–Cenozoic Syrian Arc structures to be the manifestation of the closure history of the Neo-Tethys Ocean and its successor, the Mediterranean Sea.