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Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies

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dc.contributor.author Shatalov, MY
dc.contributor.author Joubert, SV
dc.contributor.author Coetzee, CE
dc.date.accessioned 2011-12-05T13:28:47Z
dc.date.available 2011-12-05T13:28:47Z
dc.date.issued 2011-01
dc.identifier.citation Shatalov, MY, Joubert, SV and Coetzee, CE. 2010. Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies. Journal of Sound and Vibration, Vol 330(1), pp 127-135 en_US
dc.identifier.issn 0022-460X
dc.identifier.uri http://www.sciencedirect.com/science/article/pii/S0022460X10005262
dc.identifier.uri http://hdl.handle.net/10204/5362
dc.description Copyright: 2011 Elsevier. This is an ABSTRACT ONLY en_US
dc.description.abstract Standing waves can exist as stable vibrating patterns in perfect structures such as spherical bodies, and inertial rotation of the body causes precession (Bryan’seffect). However, an imperfection such as light mass anisotropy destroys the standing waves. In this paper, an imperfection is introduced in the form of light mass anisotropy for a vibrating, slowly rotating spherical body. Assuming this light mass imperfection throughout this paper, the effects of slow rotation and light isotropic viscous damping are considered in a system of variables consisting of the amplitudes of principal and quadrature vibrating patterns, the angle of the rotation of the vibrating pattern(called the precession angle) and the phase shift of the vibrating pattern. We demonstrate how a combination of both qualitative and quantitative analysis (using, interalia, the method of averaging) predicts that the inertial angular rate does not influence changes with time in the amplitudes of the principal and quadrature vibrations or the phase shift. The light mass imperfection causes changes with time which appear to be of a damped oscillatory nature for both the quadrature component as well as the principal component. The precession angular rate appears todepend on the inertial angular rate as well as the quadrature component of the vibration but is not influenced by the damping factor. It is not directly proportional to the inertial angular rate as is the case for a perfect isotropically damped structure. If the quadrature component is not suppressed, then a‘‘capture effect’’appears to occur, namely that the precession angle will not grow at a constant rate but is‘‘captured’’and show speriodic behaviour. It is evident that the damping factor does not influence changes with time in the phase shift and that the mass imperfection substantially influences these hanges. The phase shift appears to be negative, strictly decreasing and unbounded. en_US
dc.language.iso en en_US
dc.publisher Elsevier en_US
dc.relation.ispartofseries Workflow request;5005
dc.subject Standing waves en_US
dc.subject Light mass anisotropy en_US
dc.subject Light mass imperfection en_US
dc.subject Spherical bodies en_US
dc.subject Sound en_US
dc.subject Vibration en_US
dc.title Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies en_US
dc.type Article en_US
dc.identifier.apacitation Shatalov, M., Joubert, S., & Coetzee, C. (2011). Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies. http://hdl.handle.net/10204/5362 en_ZA
dc.identifier.chicagocitation Shatalov, MY, SV Joubert, and CE Coetzee "Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies." (2011) http://hdl.handle.net/10204/5362 en_ZA
dc.identifier.vancouvercitation Shatalov M, Joubert S, Coetzee C. Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies. 2011; http://hdl.handle.net/10204/5362. en_ZA
dc.identifier.ris TY - Article AU - Shatalov, MY AU - Joubert, SV AU - Coetzee, CE AB - Standing waves can exist as stable vibrating patterns in perfect structures such as spherical bodies, and inertial rotation of the body causes precession (Bryan’seffect). However, an imperfection such as light mass anisotropy destroys the standing waves. In this paper, an imperfection is introduced in the form of light mass anisotropy for a vibrating, slowly rotating spherical body. Assuming this light mass imperfection throughout this paper, the effects of slow rotation and light isotropic viscous damping are considered in a system of variables consisting of the amplitudes of principal and quadrature vibrating patterns, the angle of the rotation of the vibrating pattern(called the precession angle) and the phase shift of the vibrating pattern. We demonstrate how a combination of both qualitative and quantitative analysis (using, interalia, the method of averaging) predicts that the inertial angular rate does not influence changes with time in the amplitudes of the principal and quadrature vibrations or the phase shift. The light mass imperfection causes changes with time which appear to be of a damped oscillatory nature for both the quadrature component as well as the principal component. The precession angular rate appears todepend on the inertial angular rate as well as the quadrature component of the vibration but is not influenced by the damping factor. It is not directly proportional to the inertial angular rate as is the case for a perfect isotropically damped structure. If the quadrature component is not suppressed, then a‘‘capture effect’’appears to occur, namely that the precession angle will not grow at a constant rate but is‘‘captured’’and show speriodic behaviour. It is evident that the damping factor does not influence changes with time in the phase shift and that the mass imperfection substantially influences these hanges. The phase shift appears to be negative, strictly decreasing and unbounded. DA - 2011-01 DB - ResearchSpace DP - CSIR KW - Standing waves KW - Light mass anisotropy KW - Light mass imperfection KW - Spherical bodies KW - Sound KW - Vibration LK - https://researchspace.csir.co.za PY - 2011 SM - 0022-460X T1 - Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies TI - Influence of mass imperfections on the evolution of standing waves in slowly rotating spherical bodies UR - http://hdl.handle.net/10204/5362 ER - en_ZA


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