Observational evidence for exponential tornado intensity distributions over specific kinetic energy -: art. no. L24813

被引:33
作者
Dotzek, N [1 ]
Kurgansky, MV
Grieser, J
Feuerstein, B
Névir, P
机构
[1] DLR, Inst Phys Atmosphare, D-82234 Oberpfaffenhofen, Wessling, Germany
[2] Univ Concepcion, Fac Phys & Math Sci, Dept Geophys, Concepcion, Chile
[3] Russian Acad Sci, AM Obukhov Inst Atmospher Phys, Moscow, Russia
[4] Deutsch Wetterdienst, D-63067 Offenbach, Germany
[5] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
[6] Free Univ Berlin, Inst Meteorol, D-12165 Berlin, Germany
关键词
D O I
10.1029/2005GL024583
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Observational evidence supports the recent analytical prediction that tornado intensities are exponentially distributed over peak wind speed squared (nu(2)), or equivalently, Rayleigh-distributed over v. For large USA data samples, exponential tails are found in the tornado intensity distributions over nu(2) from about F2 intensity on. Similar results follow for smaller worldwide data samples. For the 1990s data from the USA and Oklahoma, deviations from the Rayleigh distribution for weak tornadoes can be explained by the emergence of a separate, likely non-mesocyclonic tornado mode. These bimodal datasets can be modeled by superposition of two Rayleigh distributions. The change in modal dominance occurs at about the F2 threshold (nu approximate to 50 m s(-1)). In France, likely mainly the mesocyclonic tornado mode has been recorded, while in the UK, only a non-mesocyclonic mode seems to be present.
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页码:1 / 5
页数:5
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