skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The structure and dynamics of tornado-like vortices

Abstract

The structure and dynamics of axisymmetric tornado-like vortices are explored with a numerical model of axisymmetric incompressible flow based on recently developed numerical methods. The model is first shown to compare favorably with previous results and is then used to study the effects of varying the major parameters controlling the vortex: the strength of the convective forcing, the strength of the rotational forcing, and the magnitude of the model eddy viscosity. Dimensional analysis of the model problem indicates that the results must depend on only two dimensionless parameters. The natural choices for these two parameters are a convective Reynolds number (based on the velocity scale associated with the convective forcing) and a parameter analogous to the swirl ratio in laboratory models. However, by examining sets of simulations with different model parameters it is found that a dimensionless parameter known as the vortex Reynolds number, which is the ratio of the far-field circulation to the eddy viscosity, is more effective than the convention swirl ratio for predicting the structure of the vortex. The parameter space defined by the choices for model parameters is further explored with large sets of numerical simulations. For much of this parameter space it is confirmed thatmore » the vortex structure and time-dependent behavior depend strongly on the vortex Reynolds number and only weakly on the convective Reynolds number. The authors also find that for higher convective Reynolds numbers, the maximum possible wind speed increases, and the rotational forcing necessary to achieve that wind speed decreases. Physical reasoning is used to explain this behavior, and implications for tornado dynamics are discussed.« less

Authors:
 [1];  [2]
  1. Lawrence Berkeley National Lab., CA (United States). Dept. of Mathematics
  2. Harvard Univ., Cambridge, MA (United States). Dept. of Earth and Planetary Sciences
Publication Date:
Sponsoring Org.:
USDOE, Washington, DC (United States); National Science Foundation, Washington, DC (United States)
OSTI Identifier:
684526
DOE Contract Number:  
AC03-76SF00098
Resource Type:
Journal Article
Journal Name:
Journal of the Atmospheric Sciences
Additional Journal Information:
Journal Volume: 56; Journal Issue: 16; Other Information: PBD: 15 Aug 1999
Country of Publication:
United States
Language:
English
Subject:
54 ENVIRONMENTAL SCIENCES; ATMOSPHERIC CIRCULATION; TORNADOES; TURBULENCE; VORTICES; MATHEMATICAL MODELS

Citation Formats

Nolan, D.S., and Farrell, B.F. The structure and dynamics of tornado-like vortices. United States: N. p., 1999. Web. doi:10.1175/1520-0469(1999)056<2908:TSADOT>2.0.CO;2.
Nolan, D.S., & Farrell, B.F. The structure and dynamics of tornado-like vortices. United States. doi:10.1175/1520-0469(1999)056<2908:TSADOT>2.0.CO;2.
Nolan, D.S., and Farrell, B.F. Sun . "The structure and dynamics of tornado-like vortices". United States. doi:10.1175/1520-0469(1999)056<2908:TSADOT>2.0.CO;2.
@article{osti_684526,
title = {The structure and dynamics of tornado-like vortices},
author = {Nolan, D.S. and Farrell, B.F.},
abstractNote = {The structure and dynamics of axisymmetric tornado-like vortices are explored with a numerical model of axisymmetric incompressible flow based on recently developed numerical methods. The model is first shown to compare favorably with previous results and is then used to study the effects of varying the major parameters controlling the vortex: the strength of the convective forcing, the strength of the rotational forcing, and the magnitude of the model eddy viscosity. Dimensional analysis of the model problem indicates that the results must depend on only two dimensionless parameters. The natural choices for these two parameters are a convective Reynolds number (based on the velocity scale associated with the convective forcing) and a parameter analogous to the swirl ratio in laboratory models. However, by examining sets of simulations with different model parameters it is found that a dimensionless parameter known as the vortex Reynolds number, which is the ratio of the far-field circulation to the eddy viscosity, is more effective than the convention swirl ratio for predicting the structure of the vortex. The parameter space defined by the choices for model parameters is further explored with large sets of numerical simulations. For much of this parameter space it is confirmed that the vortex structure and time-dependent behavior depend strongly on the vortex Reynolds number and only weakly on the convective Reynolds number. The authors also find that for higher convective Reynolds numbers, the maximum possible wind speed increases, and the rotational forcing necessary to achieve that wind speed decreases. Physical reasoning is used to explain this behavior, and implications for tornado dynamics are discussed.},
doi = {10.1175/1520-0469(1999)056<2908:TSADOT>2.0.CO;2},
journal = {Journal of the Atmospheric Sciences},
number = 16,
volume = 56,
place = {United States},
year = {1999},
month = {8}
}