Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/94230
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dc.contributorDepartment of Mechanical Engineeringen_US
dc.creatorCao, Wen_US
dc.creatorXu, Len_US
dc.creatorSu, Zen_US
dc.creatorPang, Ben_US
dc.creatorChi, Ren_US
dc.creatorWang, Len_US
dc.creatorWang, Xen_US
dc.date.accessioned2022-08-11T01:09:27Z-
dc.date.available2022-08-11T01:09:27Z-
dc.identifier.issn0020-7403en_US
dc.identifier.urihttp://hdl.handle.net/10397/94230-
dc.language.isoenen_US
dc.publisherPergamon Pressen_US
dc.rights© 2021 Elsevier Ltd. All rights reserved.en_US
dc.rights© 2021. This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/.en_US
dc.rightsThe following publication Cao, W., et al. (2021). "Modeling of pitting damage-induced ultrasonic nonlinearity in AL-Whipple shields of spacecraft: Theory, simulation, and experimental validation." International Journal of Mechanical Sciences 207: 106659 is available at https://dx.doi.org/10.1016/j.ijmecsci.2021.106659.en_US
dc.subjectFinite element modelingen_US
dc.subjectHypervelocity impacten_US
dc.subjectPitting damageen_US
dc.subjectQuantitative characterizationen_US
dc.subjectUltrasonic nonlinearityen_US
dc.titleModeling of pitting damage-induced ultrasonic nonlinearity in AL-Whipple shields of spacecraft : theory, simulation, and experimental validationen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume207en_US
dc.identifier.doi10.1016/j.ijmecsci.2021.106659en_US
dcterms.abstractPitting damage in the Whipple shield of spacecraft, engendered by a hypervelocity impact (HVI, exceeding 3.0 km/s), is a specific damage modality in large-scale spacecraft (e.g., Space Station). Typically, it features multitudinous craters and cracks disorderedly scattered over a wide region, accompanied with a diversity of microstructural damages (e.g., dislocation plasticity, micro-voids and cracks). This damage modality induces highly complex, mutually-interfering wave scattering in the received ultrasonic waves, making signal interpretation a daunting task, let alone the quantitative characterization of a pitted region. With this motivation, a dedicated modeling technique is proposed to scrutinize the modulation mechanism of various modalities of pitting damage on the probing ultrasonic waves, based on retrofitted nonlinear constitutive equations by comprehensively considering all nonlinearities originated from different damage sources (e.g., inherent material imperfections, as well as the above HVI-induced intensified plasticity and micro-cracks, etc.). On this basis, a quantitative correlation between the nonlinear features (i.e., second harmonics) of ultrasonic waves and the pitting damage severity is established. The modeling technique is experimentally corroborated, and the results demonstrate good consistency in between, revealing that: (1) the proposed modeling approach is feasible to faithfully simulate and precisely evaluate pitting damage-incurred nonlinearities manifested in ultrasonic waves; (2) the ultrasonic nonlinearity intensifies with the increase of pitting damage severity; and (3) the detection sensibility and cumulative effect of second harmonics are related to the “internal resonance” conditions, representing by the excitation frequency. This study yields a structural health monitoring strategy for accurately characterizing pitting-type damage at an embryo stage and surveilling material deterioration progress continuously.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationInternational journal of mechanical sciences, 1 Oct. 2021, v. 207, 106659en_US
dcterms.isPartOfInternational journal of mechanical sciencesen_US
dcterms.issued2021-10-01-
dc.identifier.scopus2-s2.0-85111004536-
dc.identifier.eissn1879-2162en_US
dc.identifier.artn106659en_US
dc.description.validate202208 bchyen_US
dc.description.oaAccepted Manuscripten_US
dc.identifier.FolderNumberME-0018-
dc.description.fundingSourceOthersen_US
dc.description.fundingTextthe 4th Advance Research Program of Manned Space Flighten_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS54444402-
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