Abstract

AbstractDuring 2–3 December 2012, the Black Sea and east coast of Romania were affected by a rapidly deepening Mediterranean cyclone. The cyclone developed a bent-back front along which short-lived (2–4 h) strong winds up to 38 m s−1 were recorded equatorward of the cyclone center. A mesoscale model simulation was used to analyze the evolution of the wind field, to investigate the physical processes that were responsible for the strong winds and their acceleration, and to investigate the relative importance of the stability of the boundary layer to those strong winds. The origin of the air in the wind maximum equatorward of the cyclone center was twofold. The first was associated with a sting jet, a descending airstream from the midlevels of the cloud head and the lower part of the cyclonic branch of the warm conveyor belt. The sting jet started to descend west of the cyclone center, ending at the frontolytic tip of the bent-back front. The second was a low-level airstream associated with the cold conveyor belt that originated northeast of the cyclone center and traveled below 900 hPa along the cold side of the bent-back front, ending behind the cold front. Both airstreams were accelerated by the along-flow pressure gradient force, with the largest accelerations acting on the sting-jet air before entering into the near-surface strong-wind area. The sensible heat fluxes destabilized the boundary layer to near-neutral conditions south of the cyclone center, facilitating downward mixing and allowing the descending air to reach the surface. Mesoscale instabilities appeared to be unimportant in the sting-jet formation.

Highlights

  • Denotes content that is immediately available upon publication as open access.One of the threats of extratropical cyclones is the strong nonconvective surface winds associated with them (e.g., Hewson and Neu 2015)

  • The question that is the focus of this article is: ‘‘What is the cause of these strong winds?’’ Cold conveyor belt? A sting jet? Both? In this article, we investigate the structure, evolution, and physical processes involved in the formation of the wind maximum equatorward of this cyclone

  • The cyclone evolution was simulated using the mesoscale model Weather Research and Forecasting (WRF) and the results showed that the strong winds were associated with two different airstreams: FIG. 14

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Summary

Introduction

One of the threats of extratropical cyclones is the strong nonconvective surface winds associated with them (e.g., Hewson and Neu 2015). Strong winds occur as air is accelerated poleward toward the cyclone center and ascends in the synoptic-scale warm conveyor belt (e.g., Carlson 1980; Harrold 1973; Browning 1990). The descent and acceleration of the sting-jet air have been suggested to be caused by evaporative cooling (Browning 2004; Clark et al 2005), the release of conditional symmetric instability (Parton et al 2009; Gray et al 2011; Martínez-Alvarado et al 2011), and the secondary circulation associated with Petterssen frontogenesis (Schultz and Sienkiewicz 2013; Slater et al 2015, 2017).

Cyclone overview
Model setup
Evolution of the wind field equatorward of the cyclone center
Petterssen frontogenesis
Backward trajectories
Acceleration of the strong wind
Findings
Conclusions
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