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Article: Unraveling the causes of the Seoul Halloween crowd-crush disaster

TitleUnraveling the causes of the Seoul Halloween crowd-crush disaster
Authors
Issue Date12-Jul-2024
PublisherPublic Library of Science
Citation
PLoS ONE, 2024, v. 19, n. 7 How to Cite?
Abstract

As the world steadily recovers from the COVID-19 pandemic, managing large gatherings becomes a critical concern for ensuring crowd safety. The crowd-crush disaster in Seoul in 2022 highlights the need for effective predictive crowd management techniques. In this study, an empirical analysis of this incident is conducted using data from various sources, and model-based simulations are created to replicate hazardous crowd conditions in high-risk areas. In the empirical analysis, mobile device data indicates a significant increase in population above normal levels in the disaster area just hours before the incident occurred. In the simulations, a hydrodynamic model is employed to simulate a bidirectional collision, which quantitatively demonstrates that the average density during the crush reached 7.57 ped/m2 (with a maximum of (9.95)ped/m2). Additionally, the average crowd pressure peaked at 1,063 N/m (with a maximum of 1,961 N/m), and the maximum velocity entropy was 10.99. Based on these findings, it can be concluded that the primary causes of the disaster were the substantial population, bidirectional collision, and escalating panic. The results of controlled simulations under various management strategies are then presented. By implementing effective crowd management techniques, crowd safety can be enhanced through quantitative comparisons of these key indicators.


Persistent Identifierhttp://hdl.handle.net/10722/345608
ISSN
2023 Impact Factor: 2.9
2023 SCImago Journal Rankings: 0.839

 

DC FieldValueLanguage
dc.contributor.authorLiang, Haoyang-
dc.contributor.authorLee, Seunghyeon-
dc.contributor.authorSun, Jian-
dc.contributor.authorWong, SC-
dc.date.accessioned2024-08-27T09:09:58Z-
dc.date.available2024-08-27T09:09:58Z-
dc.date.issued2024-07-12-
dc.identifier.citationPLoS ONE, 2024, v. 19, n. 7-
dc.identifier.issn1932-6203-
dc.identifier.urihttp://hdl.handle.net/10722/345608-
dc.description.abstract<p>As the world steadily recovers from the COVID-19 pandemic, managing large gatherings becomes a critical concern for ensuring crowd safety. The crowd-crush disaster in Seoul in 2022 highlights the need for effective predictive crowd management techniques. In this study, an empirical analysis of this incident is conducted using data from various sources, and model-based simulations are created to replicate hazardous crowd conditions in high-risk areas. In the empirical analysis, mobile device data indicates a significant increase in population above normal levels in the disaster area just hours before the incident occurred. In the simulations, a hydrodynamic model is employed to simulate a bidirectional collision, which quantitatively demonstrates that the average density during the crush reached 7.57 ped/m2 (with a maximum of (9.95)ped/m2). Additionally, the average crowd pressure peaked at 1,063 N/m (with a maximum of 1,961 N/m), and the maximum velocity entropy was 10.99. Based on these findings, it can be concluded that the primary causes of the disaster were the substantial population, bidirectional collision, and escalating panic. The results of controlled simulations under various management strategies are then presented. By implementing effective crowd management techniques, crowd safety can be enhanced through quantitative comparisons of these key indicators.</p>-
dc.languageeng-
dc.publisherPublic Library of Science-
dc.relation.ispartofPLoS ONE-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleUnraveling the causes of the Seoul Halloween crowd-crush disaster-
dc.typeArticle-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1371/journal.pone.0306764-
dc.identifier.pmid38995875-
dc.identifier.scopuseid_2-s2.0-85198587547-
dc.identifier.volume19-
dc.identifier.issue7-
dc.identifier.eissn1932-6203-
dc.identifier.issnl1932-6203-

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