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Surface thermodynamic characteristics of hook echoes and rear -flank downdrafts, with implications for tornado genesis and maintenance.

机译:钩状回波和后翼向下气流的表面热力学特征,对龙卷风的发生和维持有影响。

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摘要

Since its first documentation in 1953, the "hook echo" has been perhaps the best-recognized radar feature of supercell storms. Hook echoes have been associated with a region of subsiding air to the rear of both tornadic and non-tornadic supercells. Today this feature usually is referred to as the "rear-flank downdraft" (RFD). For over twenty years, the RFD has been hypothesized to play an important role in the final concentration of vorticity at the surface that gives rise to tornadoes.;Despite the long-surmised importance of the hook echo and RFD in tornadogenesis, only a scarce few direct observations have been obtained at the surface within hook echoes and RFDs. In this dissertation, in situ surface observations within hook echoes and RFDs are analyzed. These "mobile mesonet" data have unprecedented horizontal spatial resolution, and were obtained from the Verifications of the Origins of Rotation in Tornadoes Experiment (VORTEX) and additional field experiments conducted since the conclusion of VORTEX. The surface thermodynamic characteristics of hook echoes and RFDs associated with tornadic and non-tornadic supercells are investigated to address whether certain types of hook echoes and RFDs are favorable (or unfavorable) for tornadogenesis.;Evidence is presented that evaporative cooling and entrainment of midlevel potentially cold air play a smaller or negligible role in the forcing of RFDs associated with tornadic supercells compared to non-tornadic supercells. Tornadogenesis is more likely and tornado intensity and longevity increase as the surface buoyancy, potential buoyancy, and equivalent potential temperature in the RFD increase, and as the convective inhibition associated with RFD parcels at the surface decreases. Furthermore, baroclinity at the surface within the hook echo is not a necessary condition for tornadogenesis. It also will be shown that environments characterized by high boundary layer relative humidity (and low cloud base) are more conducive to RFDs associated with relatively high buoyancy than environments characterized by low boundary layer relative humidity (and high cloud base).
机译:自1953年首次发布文档以来,“钩回波”可能一直是超级单体风暴最公认的雷达功能。钩回波已经与隆隆和非隆隆超级电池后部的空气沉降区域相关联。如今,此功能通常称为“后翼下降气流”(RFD)。 20多年来,人们一直认为RFD在最终引起龙卷风的表面涡度集中中起着重要作用;尽管长期以来人们一直怀疑钩回波和RFD在龙卷风成因中的重要性,但很少在钩状回波和RFD内的表面已获得直接观测。本文分析了钩状回波和RFD中的地表观测。这些“移动介子”数据具有空前的水平空间分辨率,并且是从“龙卷风旋转起源验证”(VORTEX)验证以及自VORTEX结束以来进行的其他野外实验中获得的。研究了与旋风和非旋风超级电池相关的钩回波和RFD的表面热力学特征,以研究某些类型的钩回波和RFD是否有利于(或不利于)龙卷风成因;证据表明蒸发冷却和夹带中层潜在与非隆突超级电池相比,冷空气在与隆突超级电池相关的RFD的强迫中起着较小或可忽略的作用。随着RFD中表面浮力,潜在浮力和等效潜在温度的升高,以及与RFD包裹在表面的对流抑制作用的降低,龙卷风发生的可能性更高,龙卷风强度和寿命也会增加。此外,钩形回波内表面的斜压不是成岩作用的必要条件。还将显示,与以低边界层相对湿度(和高云层)为特征的环境相比,以高边界层相对湿度(和低云层)为特征的环境更有利于与相对较高浮力相关的RFD。

著录项

  • 作者

    Markowski, Paul Michael.;

  • 作者单位

    The University of Oklahoma.;

  • 授予单位 The University of Oklahoma.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 2000
  • 页码 217 p.
  • 总页数 217
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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