scholarly journals Free Vibration of a Spinning Polar Orthotropic Shallow Spherical Shell.

Author(s):  
Yukinori KOBAYASHI ◽  
Gen YAMADA
1993 ◽  
Vol 115 (1) ◽  
pp. 70-74 ◽  
Author(s):  
D. N. Paliwal ◽  
V. Bhalla

Large amplitude free vibrations of a clamped shallow spherical shell on a Pasternak foundation are studied using a new approach by Banerjee, Datta, and Sinharay. Numerical results are obtained for movable as well as immovable clamped edges. The effects of geometric, material, and foundation parameters on relation between nondimensional frequency and amplitude have been investigated and plotted.


2014 ◽  
Vol 578-579 ◽  
pp. 890-894
Author(s):  
Xian Qin Hou

Shallow spherical shell is one of the structure shapes and is adopted extensively in engineering. Based on the exact solution of free vibration of the shallow-spherical shell, the frequency equations of the shallow spherical shell with clamped edge are derived and calculated numerically. Then the first third-order frequency curve and modal curve and solved. Comparing these with the results of the exact-solution method, the range of of the shallow-spherical shell when calculated by use of practical-solution method can be derived.


1971 ◽  
Vol 38 (3) ◽  
pp. 601-607 ◽  
Author(s):  
R. J. Beckemeyer ◽  
W. Eversman

The results of a numerical analysis of the free-vibration characteristics of a thin shallow spherical shell spinning about its polar axis are presented. The shell is fully clamped by a central hub. The static equilibrium equations are formulated allowing for finite rotations. The free-vibration equations are derived by considering small perturbations about the spinning equilibrium configuration. Both flexural rigidity and membrane restoring forces due to spin are considered. Known techniques for the solution of stationary shell problems are extended to the more difficult case of the spinning shell. Plots of transverse frequency as a function of shell geometry are presented for the first two modes for shells with one and two nodal diameters for various values of inertia loading. Continuous transition from shell to flat disk results with increasing shell radius of curvature is shown.


2011 ◽  
Vol 94-96 ◽  
pp. 350-357
Author(s):  
Yong Li ◽  
Jia Chu Xu

This paper deals with non-linear free vibration of double-deck reticulated shallow spherical shell by applying the non-linear theory of double-deck reticulated shallow spherical shell established by the author. Model function is supposed to be theory solution of small deflection. The proper equation of double-deck reticulated shallow spherical about time functions with two types of boundary conditions is derived by using Galerkin’s method. At the same time, the analytical expression of ratio of non-linear vibration and linear vibration is deduced and the non-linear effect about amplitude is discussed. Numerical examples are given as well.


1999 ◽  
Author(s):  
Hwan-Sik Yoon ◽  
Gregory Washington

Abstract In this study, a smart aperture antenna of spherical shape is modeled and experimentally verified. The antenna is modeled as a shallow spherical shell with a small hole at the apex for mounting. Starting from five governing equations of the shallow spherical shell, two governing equations are derived in terms of a stress function and the axial deflection using Reissner’s approach. As actuators, four PZT strip actuators are attached along the meridians separated by 90 degrees respectively. The forces developed by the actuators are considered as distributed pressure loads on the shell surface instead of being applied as boundary conditions like previous studies. This new way of applying the actuation force necessitates solving for the particular solutions in addition to the homogeneous solutions for the governing equations. The amount of deflections is evaluated from the calculated stress function and the axial deflection. In addition to the analytical model, a finite element model is developed to verify the analytical model on the various surface positions of the reflector. Finally, an actual working model of the reflector is built and tested in a zero gravity environment, and the results of the theoretical model are verified by comparing them to the experimental data.


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