马笼头 发表于 2025-3-28 17:32:07
http://reply.papertrans.cn/24/2323/232255/232255_41.png他去就结束 发表于 2025-3-28 20:14:36
http://reply.papertrans.cn/24/2323/232255/232255_42.pngConstrain 发表于 2025-3-29 01:56:32
Book 2004 embraces dynamic rupture and wave propagation, computational environment and algorithms, data assimilation and understanding, and applications of models to earthquakes. This part also contains articles on the computational approaches and challenges of constructing earthquake models..调色板 发表于 2025-3-29 05:19:30
http://reply.papertrans.cn/24/2323/232255/232255_44.png迫击炮 发表于 2025-3-29 08:00:46
http://reply.papertrans.cn/24/2323/232255/232255_45.png装入胶囊 发表于 2025-3-29 14:54:49
https://doi.org/10.1007/978-3-662-68569-3tained for each model are similar, showing that the solution of the dynamic problem is non-unique. In other words, it is not always possible to separate strength drop and the slip-weakening distance using rupture modeling, in agreement with the conclusions by GUATTERI and SPUDICH (2000).疲惫的老马 发表于 2025-3-29 17:35:16
https://doi.org/10.1007/978-3-663-02052-3ssimilation of non-primary data could yield biased simulation results. We present a primary data set for the San Andreas and Imperial faults for comparison with non-primary data in existing databases, and propose standard formats and structure for paleoseismic data assimilation into numerical simulation models.EPT 发表于 2025-3-29 20:30:21
Guided Waves from Sources Outside Faults: An Indication for Shallow Fault Zone Structure?ll outside a FZ continuous with depth. The results support, in conjunction with recent observational evidence, a model for natural faults with shallow trapping structures rather than ones that span the entire seismogenic zone. This may have implications for fault mechanics as well as for aspects of shaking hazard near faults.characteristic 发表于 2025-3-30 02:03:00
http://reply.papertrans.cn/24/2323/232255/232255_49.png反话 发表于 2025-3-30 07:10:58
Assimilation of Paleoseismic Data for Earthquake Simulationssimilation of non-primary data could yield biased simulation results. We present a primary data set for the San Andreas and Imperial faults for comparison with non-primary data in existing databases, and propose standard formats and structure for paleoseismic data assimilation into numerical simulation models.