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    Parametric Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge Loads

    Source: Journal of Applied Mechanics:;1997:;volume( 064 ):;issue: 001::page 139
    Author:
    Jen-San Chen
    DOI: 10.1115/1.2787264
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: The parametric resonance of a spinning disk under a space-fixed pulsating edge load is investigated analytically. We assume that the radial edge load can be expanded in a Fourier series. With use of the orthogonality properties among the eigenfunctions of a gyroscopic system, the partial differential equation of motion is discretized into a system of generalized Hill’s equations in the first-order form. The method of multiple scale is employed to determine the conditions for single mode as well as combination resonances to occur. For any two modes, with s and υ nodal diameters, respectively, combination resonance occurs only when there exists a specific Fourier component cos kθ in the edge load, where s + υ = ±k. Sum type resonance occurs when both modes are reflected or both modes are nonreflected. On the other hand, difference type resonance occurs when one mode is reflected and the other is nonreflected. In applying this rule, the number of nodal diameters of a forward and a reflected wave is considered as negative. Several typical loadings are discussed, including uniform and concentrated edge loads.
    keyword(s): Stress , Resonance , Rotating Disks , Motion , Waves , Eigenfunctions , Equations , Fourier series AND Partial differential equations ,
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      Parametric Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge Loads

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    http://yetl.yabesh.ir/yetl1/handle/yetl/118254
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    contributor authorJen-San Chen
    date accessioned2017-05-08T23:52:41Z
    date available2017-05-08T23:52:41Z
    date copyrightMarch, 1997
    date issued1997
    identifier issn0021-8936
    identifier otherJAMCAV-26407#139_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/118254
    description abstractThe parametric resonance of a spinning disk under a space-fixed pulsating edge load is investigated analytically. We assume that the radial edge load can be expanded in a Fourier series. With use of the orthogonality properties among the eigenfunctions of a gyroscopic system, the partial differential equation of motion is discretized into a system of generalized Hill’s equations in the first-order form. The method of multiple scale is employed to determine the conditions for single mode as well as combination resonances to occur. For any two modes, with s and υ nodal diameters, respectively, combination resonance occurs only when there exists a specific Fourier component cos kθ in the edge load, where s + υ = ±k. Sum type resonance occurs when both modes are reflected or both modes are nonreflected. On the other hand, difference type resonance occurs when one mode is reflected and the other is nonreflected. In applying this rule, the number of nodal diameters of a forward and a reflected wave is considered as negative. Several typical loadings are discussed, including uniform and concentrated edge loads.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleParametric Resonance of a Spinning Disk Under Space-Fixed Pulsating Edge Loads
    typeJournal Paper
    journal volume64
    journal issue1
    journal titleJournal of Applied Mechanics
    identifier doi10.1115/1.2787264
    journal fristpage139
    journal lastpage143
    identifier eissn1528-9036
    keywordsStress
    keywordsResonance
    keywordsRotating Disks
    keywordsMotion
    keywordsWaves
    keywordsEigenfunctions
    keywordsEquations
    keywordsFourier series AND Partial differential equations
    treeJournal of Applied Mechanics:;1997:;volume( 064 ):;issue: 001
    contenttypeFulltext
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