Abstract
GEOPHYSICAL RESEARCH LETTERS,
VOL. 32,
L24813,
5 PP., 2005
doi:10.1029/2005GL024583
Observational evidence for exponential tornado intensity distributions over specific kinetic energy
Institut für Physik der Atmosphäre, Deutsche Zentrum für Luft- und Raumfahrt, Wessling, Germany
Department of Geophysics, Faculty of Physical and Mathematical Sciences, Universidad de Concepción, Concepción, Chile
Deutsches Wetterdienst, Offenbach, Germany
Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Institut für Meteorologie, Freie Universität Berlin, Berlin, Germany
Observational evidence supports the recent analytical prediction that tornado intensities are exponentially distributed over peak wind speed squared (v 2), or equivalently, Rayleigh-distributed over v. For large USA data samples, exponential tails are found in the tornado intensity distributions over v 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 (v ≈ 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.
Received 20 September 2005; accepted 17 November 2005; published 28 December 2005.
Citation: (2005), Observational evidence for exponential tornado intensity distributions over specific kinetic energy, Geophys. Res. Lett., 32, L24813, doi:10.1029/2005GL024583.
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