Abstract

Abstract. This work deals with the hypothesis that synoptically-driven heavy rains in the Mediterranean region are connected with the occurrence of synoptic-dynamic anomalies. We investigate this hypothesis by conducting a diagnostic study of a cyclogenesis event from 18–21 July 2001. Cyclogenesis started over the western Mediterranean Sea and was triggered by the approach of a pre-existing upper trough over a lower frontal zone. The event was first accompanied by heavy convective rains in northern Italy and later by heavy, widespread and steady rains of non-convective character in Central Europe. Using re-analyses from the database ERA-40, we evaluate the synoptic-dynamic anomalies by the cumulative distribution function relatively to July–August area-related climatology over the reference period from 1958 to 2002. For the duration of cyclogenesis, we detect significant anomalies associated with the processes that support the completion of vertical coupling between the lower frontal zone and the upper vorticity maximum. The periods of heavy rains in both the Mediterranean region and Central Europe were characterised by the occurrence of anomalies that created synoptic-scale conditions favourable for triggering and sustaining heavy rains. Although these anomalies were somewhat weaker in the period of heavy rains in Central Europe than in the Mediterranean region, the analysis of their spatio-temporal correspondence over the reference rainfall events in the Czech Republic shows that they are typical of heavy rains there. Due to the relatively high variability of the causal synoptic-scale conditions, this study would benefit post-processing procedures aimed at improving warning about this hazardous weather phenomenon to further investigate which anomalies generally occur during synoptically-driven heavy rains in the Mediterranean region and the strengths of these anomalies.

Highlights

  • Most of the heaviest rains in the western Mediterranean region are attributed to mesoscale convective systems (Fernandez et al, 1995)

  • We examined the relationship between the occurrence of synoptic-dynamic anomalies and heavy rains in the Mediterranean region by conducting a diagnostic study of a cyclogenesis event from 18–21 July 2001 that arose over the western Mediterranean Sea

  • Cyclogenesis took place according to the classic Petterssen scheme of a type B-development (Petterssen, 1971), where a pre-existing upper trough, connected to the upper low over Western Europe, spread over an area lacking cold thermal advection near the frontal zone

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Summary

Introduction

Most of the heaviest rains in the western Mediterranean region are attributed to mesoscale convective systems (Fernandez et al, 1995) Such organised convection is dynamically driven by synoptic-scale processes, in the eastward and poleward sectors of surface cyclones, where quasigeostrophic upward motions and sustained and intense low-level inflows of moist, potentially unstable air dominate (Martın et al, 2006; Jansaet al., 2001; Ramis et al, 1994). Muller: Cyclogenesis in the Mediterranean basin the close relationship between this synoptic-scale circulation pattern and heavy rainfall events in the Czech Republic (CR) to demonstrate that this pattern is regularly connected with the appearance of anomalous values of certain dynamic and thermodynamic variables in specific synoptic-scale areas They referred to these areas as the synoptic-dynamic anomalies, and they showed that the combined strength of some of them is distinctly correlated with the intensity of heavy rains. We aimed at (i) describing the principles of the method used to detect and evaluate synoptic-dynamic anomalies, and (ii) discussing the most significant anomalies, which occurred immediately before and during heavy rains

Data and diagnostic methodology
Detection of synoptic-dynamic anomalies
Spatio-temporal correspondence of synopticdynamic anomalies
Event 18–21 July 2001
Event overview
Diagnosis using synoptic-dynamic anomalies
Mediterranean region
Central Europe
Conclusions
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