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NUMERICAL KINEMATIC RUPTURE SIMULATION

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dc.contributor.author Anand, Tejaswi
dc.date.accessioned 2025-05-11T15:17:39Z
dc.date.available 2025-05-11T15:17:39Z
dc.date.issued 2018-05
dc.identifier.uri http://localhost:8081/jspui/handle/123456789/16207
dc.description.abstract The numerical simulation of strong ground motion (SGM) based on the physics of rupture propagation is of prime importance in earthquake engineering for the prediction of site-specific ground motion, cost effective earthquake resistant designs and assessment of vulnerability and risk. The development of an efficient numerical method for SGM prediction is must for the future earthquake engineering since the available empirical relations and simulation methods like stochastic metod and empirical Green's method do not provide the characteristics of the individual seismic phases, particularly in the basins and shallow earthquake cases. Further, the SGM recorders do not prove the characteristics of very low frequency ground motion, particularly in the case of very large earthquakes. Furthermore, there is lack of SGM records in the epicentral zone of great earthquakes. Earthquake source dynamics provides key elements for the prediction of ground motion, and to understand the physics of earthquake initiation, propagation, and healing. A physical understanding of the spontaneous rupture process is important for advancing our understanding of earthquake physics. en_US
dc.description.sponsorship INDIAN INSTITUTE OF TECHNOLOGY, ROORKEE en_US
dc.language.iso en en_US
dc.publisher IIT ROORKEE en_US
dc.subject Modified Yoffe Function en_US
dc.subject Palmer And Rice Function en_US
dc.subject Kinematic Rupture Model en_US
dc.subject Dynamic Rupture Model en_US
dc.title NUMERICAL KINEMATIC RUPTURE SIMULATION en_US
dc.type Other en_US


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