Stretching and Distortion of Material Line Elements in Two-Dimensional Turbulence

1992 ◽  
Vol 61 (10) ◽  
pp. 3547-3558 ◽  
Author(s):  
Takashi Ishihara ◽  
Yukio Kaneda
1985 ◽  
Vol 22 (4) ◽  
pp. 506-513 ◽  
Author(s):  
W. M. Schwerdtner

Simple two-dimensional techniques are used to make an estimate of the total shortening across a narrow greenstone belt in northwestern Ontario. The techniques are based on the basic principle of restoring the predeformational geometry of a horizontal traverse across the belt. Depending on the technique used this traverse is a string of line elements or a chain of finite elements. The strain ratios available for the restoration are minimal values and need to be increased significantly to obtain realistic results. Depending on the strain values selected for the restoration, amounts of horizontal shortening range from 17 to 49%. The actual amount remains unknown, but is thought to be < 50%.In view of the apparent variation in longitudinal strain along the greenstone belt, a three-dimensional treatment seems to be necessary. This would require that strain measurements be taken systematically throughout, rather than along a single traverse across, a greenstone belt segment.


Author(s):  
J.C.R. Hunt

Some of the basic principles of vortex dynamics arc reviewed in this paper and applied to calculating and understanding various kinds of turbulent flows. After setting out the basic equations and boundary conditions, the different principles are illustrated for special eases where different simplifications are justified. The displacement of two-dimensional vorticity is applied to two-dimensional shear flows over slender shapes (such as humps or hills on surfaces where the ‘triple-deck’ method is explained in terms of vorticity). The general changes of vorticity and velocity are related to the movement of fluid-line elements. A new geometrical proof for the changes in velocity is given. These concepts are applied to distorted turbulent flows (isotropic and anisotropic) and shear flows. Recent results on the forces on and motions of finite fluid volumes in rotational, non-uniform flows are reviewed and it is shown that the inertial or added mass effects are generally of greater importance than the distortion of the vorticity field. This gives some new insight into Prandtl’s mixing length theory. A simple class of interaction between vortices is reviewed to illustrate how the interactions differ depending on the relative strengths of the vortices. Finally, some new ideas are reviewed on vorticity shed from surfaces and how this interacts with vorticity advected onto a body from upstream.


Author(s):  
S. L. Han ◽  
O. A. Bauchau

In flexible multibody systems, many components are approximated as shells. Classical shell theories, such as Kirchhoff or Reissner-Mindlin shell theory, form the basis of the analytical development for shell dynamics. While such approach is capable of capturing the kinetic energy of the system accurately, it cannot represent the strain energy adequately. For instance, it is well known from three-dimensional elasticity theory that the normal material line will warp under load for laminated composite shells, leading to three-dimensional deformations that generate complex stress states. To overcome this problem, a novel three-dimensional shell theory is proposed in this paper. Kinematically, the problem is decomposed into an arbitrarily large rigid-normal-material-line motion and a warping field. The sectional strains associated with the rigid-normal-material-line motion and the warping field are assumed to remain small. As a consequence of this kinematic decomposition, the governing equations of the problem fall into two distinct categories: the global equations describing geometrically exact shells and the local equations describing local deformations. The governing equations for geometrically exact shells are nonlinear, two-dimensional equations, whereas the local equations are linear, one dimensional, provide the detailed distribution of three-dimensional stress and strain fields. Based on a set of approximated solutions, the local equations is reduced to the corresponding global equations. In the reduction process, a 9 × 9 sectional stiffness matrix can be found, which takes into account the warping effects due to material heterogeneity. In the recovery process, three-dimensional stress and strain fields at any point in the shell can be recovered from the two-dimensional shell solution. The proposed method proposed is valid for anisotropic shells with arbitrarily complex through-the-thickness lay-up configuration.


1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


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