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Near and far-field hazards of asteroid impacts in oceans

机译:小行星撞击海洋的近场和远场危害

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摘要

Hazards resulting from asteroid ocean impacts were modelled using hydrocode simulations to examine the near-field effects including the initial formation and subsequent long range propagation of tsunami waves that can transport potentially damaging energy far from the impact site.Three-dimensional simulations of oblique impacts into deep water, with trajectory angles ranging from 27 degrees to 60 degrees above the horizontal, were performed with the Los Alamos Rage hydrocode. The simulations include atmospheric effects such as ablation and airbursts. These oblique impact simulations are performed in order to help determine whether there are additional dangers due to the obliquity of impact not covered by previous studies. The energy transferred to both the air blast wave and the water are calculated as well as the amount of sea water lofted into the upper atmosphere. Water crater sizes and subsequent surface elevation profiles, surface pressures, and depth-averaged mass fluxes within the water are prepared for use in far-field propagation studies. Like previous three-dimensional simulations, these simulations show that except at exceedingly shallow entry angles below those simulated here the resulting waves are roughly circular and that the initial waves and central jet oscillation are highly turbulent and dissipate a lot of the energy.Two-dimensional axisymmetric simulations of long range propagation of impact tsunami were performed using the Lawrence Livermore ALE3D hydrocode on the NASA Pleiades supercomputer. These simulations showed that impacts under 1 gigaton TNT equivalent into the deep ocean basins will create deep-water waves that undergo dispersion, whereas impacts onto continental shelves will create shallow-water waves that do not suffer dispersion. The simulations also showed that on the order of 1% of the kinetic energy of the impact is converted into the tsunami wave. This is an order of magnitude less than previous semi-empirical estimates of similar to 15% based on explosion test data and laboratory scale impacts.
机译:小行星海洋撞击造成的危害已使用水力法模拟来建模,以检查近场影响,包括海啸波的初始形成和随后的远距离传播,这些海啸波可能将潜在的破坏性能量转移到撞击点以外的地方。 Los Alamos Rage液压代码执行了深水运动,其弹道角在水平上方的27度到60度之间。模拟包括大气效应,例如烧蚀和爆炸。进行这些倾斜冲击模拟是为了帮助确定是否由于先前研究未涵盖的冲击倾斜而造成其他危险。计算传递到鼓风波和水中的能量,以及流入高层大气的海水量。准备好水坑的尺寸和随后的表面高度剖面,表面压力以及水中的深度平均质量通量,以用于远场传播研究。像以前的三维模拟一样,这些模拟表明,除了在此处模拟的入射角以下非常浅的入射角之外,所得波大致呈圆形,并且初始波和中心射流振荡高度湍流并耗散了大量能量。在美国宇航局Pleiades超级计算机上使用Lawrence Livermore ALE3D液压代码进行了冲击海啸远程传播的轴对称模拟。这些模拟表明,在1吨TNT当量以下的冲击进入深海盆地将产生深水波,而该波将经历弥散,而对大陆架的冲击将产生不遭受波幅的浅水波。模拟还显示,冲击的动能的大约1%被转换为海啸波。根据爆炸测试数据和实验室规模的影响,这比以前的半经验估计值低了一个数量级,后者约为15%。

著录项

  • 来源
    《Acta astronautica》 |2019年第3期|262-277|共16页
  • 作者单位

    NASA, Ames Res Ctr, Sci & Technol Corp, Moffett Field, CA 94035 USA;

    Los Alamos Natl Lab, Los Alamos, NM USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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