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Dynamics and Coastal Effects of Tsunamis Generated by Asteroids Impacting the Black Sea

机译:小行星撞击黑海产生海啸的动力学和海岸效应

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Two-dimensional (2D) and one-dimensional (1D) shallow-water models are used to evaluate the seashore effects of the tsunami generated by an asteroid impacting the western regions of the Black Sea about 208 km from the coast. The tsunami's speed and the effects on the coastal regions depend on many factors, among which the most important is asteroid size. The tsunami generated by a 250-m asteroid reaches the nearest land location in 24 min and needs about 2 h to arrive at all Black Sea coast. The run-up value is about 7 m high on the Turkish and Crimean coasts. In the western Black Sea regions the wave height is two or three times smaller. The run-up values strongly depend on bathymetry and topography peculiarities. The run-in value in case of the tsunami generated by a 1,000-m asteroid is up to eight times larger than in case of a 250-m impactor, depending on location. The results reported herein are upper limit values. In case of the 250-m asteroid, the real wave amplitude may be up to two times smaller. The uncertainty factor decreases in case of larger asteroids. Ways of diminishing the social consequences are briefly discussed.
机译:二维(2D)和一维(1D)浅水模型用于评估小行星撞击距海岸约208公里的黑海西部地区所产生的海啸对海岸的影响。海啸的速度及其对沿海地区的影响取决于许多因素,其中最重要的是小行星的大小。由250米小行星产生的海啸在24分钟内到达最近的陆地位置,大约需要2小时才能到达黑海的所有海岸。在土耳其和克里米亚半岛海岸,起钻价值约为7 m。在黑海西部地区,波浪高度小两到三倍。上升值在很大程度上取决于测深法和地形特征。根据位置的不同,在1,000米小行星产生海啸的情况下,磨合值比250米撞击器的磨合值大八倍。本文报道的结果为上限值。如果是250米小行星,则实际波幅可能小两倍。对于较大的小行星,不确定性因素会降低。简要讨论了减少社会后果的方法。

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