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Fig. 1 Location map showing also the observed maximum width and the sediment texture classification (percentages in relation to the total) of the (71) beaches with increased touristic potential at the northern, eastern and southern coast of E. Crete  under great pressure. In 2011, there were more than 2.8 million direct foreign tourist arrivals at the island airports with 2.16 million tourists landing at the eastern Cretan Heraklion airport (SETE 2012); these tourists form only a part of the annual, highly seasonal tourist influx that has to be accommodated and use the eastern Cretan beaches as environments of leisure.  Cretan geology is dominated by pre-alpine and alpine formations that constitute a complex nappe and Neogene sediments that fill the basins forming between the moun- tains (Fytrolakis 1980). The island forms the central (and largest) island of the Cretan Arc, an island chain bounded by deep basins both to the north (Cretan Sea) and the south (Ionian and Levantine Basins); the Cretan Arc straits control the water exchanges between the Aegean Sea and the Eastern Mediterranean (Tsimplis et al. 1999; Velaoras et al.2014). The climate is of ‘Mediterranean type’, ie., cool and wet in the November—March period, and hot and dry in the May—September period. The annual wind field is dominated by a prevalence of northerly winds, which show a double maximum: the first during winter (December— February) and the second (known as the ‘Etesians’) during summer (July and August); recent studies project increases in the mean wind speeds of the area in the following decades (Weisse et al. 2014). Astronomical tides are small (few tens of cm on springs) and offshore wind waves are associated with average and extreme storm wave heights of less than 1.5 m and more than 6 m, respectively. With regard to storm surges, these are generally moderate in the  Eastern Mediterranean, having heights that rarely exceed 0.4 m (Tsimplis and Shaw 2010).

Figure 1 Location map showing also the observed maximum width and the sediment texture classification (percentages in relation to the total) of the (71) beaches with increased touristic potential at the northern, eastern and southern coast of E. Crete under great pressure. In 2011, there were more than 2.8 million direct foreign tourist arrivals at the island airports with 2.16 million tourists landing at the eastern Cretan Heraklion airport (SETE 2012); these tourists form only a part of the annual, highly seasonal tourist influx that has to be accommodated and use the eastern Cretan beaches as environments of leisure. Cretan geology is dominated by pre-alpine and alpine formations that constitute a complex nappe and Neogene sediments that fill the basins forming between the moun- tains (Fytrolakis 1980). The island forms the central (and largest) island of the Cretan Arc, an island chain bounded by deep basins both to the north (Cretan Sea) and the south (Ionian and Levantine Basins); the Cretan Arc straits control the water exchanges between the Aegean Sea and the Eastern Mediterranean (Tsimplis et al. 1999; Velaoras et al.2014). The climate is of ‘Mediterranean type’, ie., cool and wet in the November—March period, and hot and dry in the May—September period. The annual wind field is dominated by a prevalence of northerly winds, which show a double maximum: the first during winter (December— February) and the second (known as the ‘Etesians’) during summer (July and August); recent studies project increases in the mean wind speeds of the area in the following decades (Weisse et al. 2014). Astronomical tides are small (few tens of cm on springs) and offshore wind waves are associated with average and extreme storm wave heights of less than 1.5 m and more than 6 m, respectively. With regard to storm surges, these are generally moderate in the Eastern Mediterranean, having heights that rarely exceed 0.4 m (Tsimplis and Shaw 2010).