## Abstract A thinโtube vortex method is developed to investigate the intrinsic instability within a counterโrotating vortex pair system and the effects from the core size and the wavenumbers (or wavelengths). The numerical accuracy and the advantages of the scheme are theoretically estimated. A ne
Improved Thin-Tube Models for Slender Vortex Simulations
โ Scribed by Omar M. Knio; Rupert Klein
- Publisher
- Elsevier Science
- Year
- 2000
- Tongue
- English
- Weight
- 96 KB
- Volume
- 163
- Category
- Article
- ISSN
- 0021-9991
No coin nor oath required. For personal study only.
โฆ Synopsis
This paper explores three numerical schemes for efficient simulation of slender vortex filaments. The schemes defeat the spatial and temporal stiffness of the equations of motion by requiring only adequate resolution of the filament centerline and allowing large integration time steps. In order to correctly capture the self-induced filament velocity, the first scheme uses an explicit velocity correction method, the second scheme relies on a logarithmic extrapolation of two velocity predictions, and the third scheme employs a local refinement algorithm. The performances of the three schemes are contrasted in light of unsteady computations of a perturbed vortex ring with small core to radius ratio.
๐ SIMILAR VOLUMES
## Abstract In order to improve predicting precision and increase the computation speed of simulation for a finโandโtube condenser, a novel method integrating the fundamental mathematical model with an artificial neural network (ANN) is presented. A threeโzone model is used as the basic mathematica
A method is described for calculating thin รlm /(qz) curves from the corresponding bulk /(qz) curves. A multiple scattering Monte Carlo program was used to simulate more than 300 thin รlm /(qz) curves with di โ erent รlmsubstrate combinations. The simulations were made at normal electron incidence in
This paper presents a method for the dynamic analysis of initially tensioned orthotropic thin-walled cylindrical tubes conveying steady #uid #ow, based on Sanders' non-linear theory of thin shells and the classical potential #ow theory. The method is relatively straightforward, using a hydrodynamic