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    Analysis of Hurricane Maria’s Impact on the Arecibo Telescope

    Source: Journal of Performance of Constructed Facilities:;2025:;Volume ( 039 ):;issue: 004::page 04025021-1
    Author:
    Zhi Zhang
    ,
    Xin Chu
    ,
    Reyhaneh Abbasi
    ,
    Pierre Ghisbain
    ,
    Liling Cao
    ,
    John Abruzzo
    DOI: 10.1061/JPCFEV.CFENG-4821
    Publisher: American Society of Civil Engineers
    Abstract: The Arecibo Telescope in Puerto Rico collapsed on December 1, 2020. After the incident, Thornton Tomasetti Inc. (TT) was engaged by the Florida Space Institute to conduct a forensic investigation of the root cause of the collapse. An essential focus of the investigation was the impact of wind loads and particularly of Hurricane Maria in 2017, the strongest hurricane that the telescope had experienced in its service life. Computational fluid dynamic (CFD) analysis can be used to simulate the response of unusual structures’ to wind loads; however, it can be computationally expensive for complex structures or winds with long durations. Conducting this type of analysis may be feasible by involving high-performance computing systems. However, given the scope of the investigation, as well as the limited time and budget, performing such a sophisticated CFD analysis of the telescope subjected to the full hurricane time history was infeasible. TT adopted a cost-effective method to simulate the wind loads on the telescope during Hurricane Maria and apply those forces to a structural analysis model. The technique uses a combination of CFD analysis, previous wind tunnel test results, and wind speed records. A CFD model of the telescope was used to generate wind forces at a constant wind speed and was validated by previous wind tunnel tests on a physical model of the telescope. The validation shows that the CFD analysis can adequately depict the wind tunnel test results and that the wind forces can be scaled based on wind speeds. The wind forces from CFD analysis were then scaled to time-varying forces based on the on-site measured wind speeds during Hurricane Maria. The time-varying forces were subsequently applied to a finite element (FE) model of the telescope to evaluate its dynamic response during Hurricane Maria. This paper provides an in-depth description of each analysis step, validation of the wind force scaling method, and the telescope’s response to Hurricane Maria. The results show that the forces in the cables supporting the telescope increased 14% during Hurricane Maria.
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      Analysis of Hurricane Maria’s Impact on the Arecibo Telescope

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    contributor authorZhi Zhang
    contributor authorXin Chu
    contributor authorReyhaneh Abbasi
    contributor authorPierre Ghisbain
    contributor authorLiling Cao
    contributor authorJohn Abruzzo
    date accessioned2025-08-17T23:02:25Z
    date available2025-08-17T23:02:25Z
    date copyright8/1/2025 12:00:00 AM
    date issued2025
    identifier otherJPCFEV.CFENG-4821.pdf
    identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4307817
    description abstractThe Arecibo Telescope in Puerto Rico collapsed on December 1, 2020. After the incident, Thornton Tomasetti Inc. (TT) was engaged by the Florida Space Institute to conduct a forensic investigation of the root cause of the collapse. An essential focus of the investigation was the impact of wind loads and particularly of Hurricane Maria in 2017, the strongest hurricane that the telescope had experienced in its service life. Computational fluid dynamic (CFD) analysis can be used to simulate the response of unusual structures’ to wind loads; however, it can be computationally expensive for complex structures or winds with long durations. Conducting this type of analysis may be feasible by involving high-performance computing systems. However, given the scope of the investigation, as well as the limited time and budget, performing such a sophisticated CFD analysis of the telescope subjected to the full hurricane time history was infeasible. TT adopted a cost-effective method to simulate the wind loads on the telescope during Hurricane Maria and apply those forces to a structural analysis model. The technique uses a combination of CFD analysis, previous wind tunnel test results, and wind speed records. A CFD model of the telescope was used to generate wind forces at a constant wind speed and was validated by previous wind tunnel tests on a physical model of the telescope. The validation shows that the CFD analysis can adequately depict the wind tunnel test results and that the wind forces can be scaled based on wind speeds. The wind forces from CFD analysis were then scaled to time-varying forces based on the on-site measured wind speeds during Hurricane Maria. The time-varying forces were subsequently applied to a finite element (FE) model of the telescope to evaluate its dynamic response during Hurricane Maria. This paper provides an in-depth description of each analysis step, validation of the wind force scaling method, and the telescope’s response to Hurricane Maria. The results show that the forces in the cables supporting the telescope increased 14% during Hurricane Maria.
    publisherAmerican Society of Civil Engineers
    titleAnalysis of Hurricane Maria’s Impact on the Arecibo Telescope
    typeJournal Article
    journal volume39
    journal issue4
    journal titleJournal of Performance of Constructed Facilities
    identifier doi10.1061/JPCFEV.CFENG-4821
    journal fristpage04025021-1
    journal lastpage04025021-19
    page19
    treeJournal of Performance of Constructed Facilities:;2025:;Volume ( 039 ):;issue: 004
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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