Journal
MONTHLY WEATHER REVIEW
Volume 140, Issue 3, Pages 1023-1043Publisher
AMER METEOROLOGICAL SOC
DOI: 10.1175/MWR-D-11-00026.1
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This work presents an analysis of the vertical wind shear during the early stages of the remarkable 8 May 2009 central U. S. derecho-producing convective system. Comments on applying Rotunno-Klemp-Weisman (RKW) theory to mesoscale convective systems (MCSs) of this type also are provided. During the formative stages of the MCS, the near-surface-based shear vectors ahead of the leading convective line varied with time, location, and depth, but the line-normal component of the shear in any layer below 3 km ahead of where the strong bow echo developed was relatively small (6-9 m s(-1)). Concurrently, the midlevel (3-6 km) line-normal shear component had magnitudes mostly >10 m s(-1) throughout. In a previous companion paper, it was hypothesized that an unusually strong and expansive low-level jet led to dramatic changes in instability, shear, and forced ascent over mesoscale areas. These mesoscale effects may have overwhelmed the interactions between the cold pool and low-level shear that modulate system structure in less complex environments. If cold pool-shear interactions were critical to producing such a strong system, then the extension of the line-normal shear above 3 km also appeared to be critical. It is suggested that RKW theory be applied with much caution, and that examining the shear above 3 km is important, if one wishes to explain the formation and maintenance of intense long-lived convective systems, particularly complex nocturnal systems like the one that occurred on 8 May 2009.
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