Brierley & Fedorov (2010) demonstrated that mid-latitude SST vari

Brierley & Fedorov (2010) demonstrated that mid-latitude SST variability is affected by precipitation and global radiative forcing (e.g. water vapour and total cloud cover). Moreover, Skliris et al. (2012) claimed that Mediterranean SST spatiotemporal variability is significantly affected by increasing warming from Atlantic inflow. In general, wind forcing has

significantly affected the Mediterranean SST, especially in the northern Adriatic Sea (Bora winds; Ferrarese et al. 2009), Aegean Sea (Etesian winds; Metaxas & Bartzokas 1994), LPC sub-basin (Mistral winds; Jiang et al. 2003) and Alboran Sea (the Levanter and Vendaval winds; Anonymous 1988). LPC sub-basin refers to the Liguro-Provencal and Catalan sub-basins. The Mediterranean SST has also been linked to sea level pressure (Jung et al.

2006). Determining the correlations between the above-mentioned Epigenetic Reader Domain inhibitor parameters and SST is an aim of the present work. Using a high-resolution ocean model forced by the A2 climate scenario, Somot et al. (2006) projected that the Mediterranean SST would increase by 3.1 °C over the 1961–2099 period. Using climate scenarios B1, A1B, and A2, Parry et al. (2007) projected that the global SST would rise by 1.5, 2.2, and 2.6 °C, respectively, during the 21st century. In late 2008, a new climate Selleck Ganetespib experiment was conducted involving coordinated climate models and 20 groups of climate modellers. The Coupled Model Intercomparison Project, phase five (CMIP5), included four new climate scenarios, i.e. RCP26, RCP45, RCP60 and RCP85, for the 21st century; RCP stands for ‘representative Etomidate concentration pathways’ and the following number indicates

ten times the radiative forcing at the end of the 21st century. The RCP26 scenario incorporates peak radiative forcing of ~ 3 W m− 2 (~ 490 ppm CO2) before 2100, followed by declines to 2.6 W m− 2 by 2100 (Van Vuuren et al. 2007). The radiative forcing in 2100 is approximately 3 W m− 2 (~ 490 ppm CO2) in the RCP45 scenario (Clarke et al. 2007), approximately 6 W m− 2 (~ 850 ppm CO2) in the RCP60 scenario (Fujino et al. 2006) and approximately 8.5 W m− 2 (~ 1370 ppm CO2) in the RCP85 scenario (Riahi et al. 2007). The present study examines the response of the Mediterranean SST to global climate change in these four scenarios. According to Taylor et al. (2012), the CMIP5 scenarios are intended to improve on the success of the earlier CMIP phases. The CMIP scenarios address most of the World Climate Research Programme’s (WCRP) component properties and suggestions. Spatiotemporal SST variability over the Mediterranean Sea was further studied for the period ending 2008 (e.g. Skliris et al. 2012); the present study expands on this work, analysing spatiotemporal SST variability up to 2012. Similarly, the effects of atmospheric parameters on Mediterranean SST variability were further studied for the period ending 2008.

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