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activity over the Indian Ocean are evident. The resulting pressure gradient over the GMR is relatively strong (10–20 hPa from the western to eastern Mediterranean or even greater), and its variability defines the onset of trade wind systems like the etesians over the Aegean Sea. Figure 1 is produced with the use of mean monthly sea level pressure fields for August of 2001 from the European Centre for Medium-Range Weather Forecasts (ECMWF) analysis fields. The general pattern of the flow over the GMR
activity over the Indian Ocean are evident. The resulting pressure gradient over the GMR is relatively strong (10–20 hPa from the western to eastern Mediterranean or even greater), and its variability defines the onset of trade wind systems like the etesians over the Aegean Sea. Figure 1 is produced with the use of mean monthly sea level pressure fields for August of 2001 from the European Centre for Medium-Range Weather Forecasts (ECMWF) analysis fields. The general pattern of the flow over the GMR
