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Near and far-field hazards of asteroid impacts in oceans

机译:海洋中小行星撞击的近乎田间危害

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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:由Sertocode模拟模拟小行星海洋影响的危害,以检查包括初始形成和随后的海啸波的长期效果,这些近似的海啸波的远程传播可能远离冲击部位的潜在损坏能量。斜斜度的三维模拟倾斜的影响用LOS Alamos Rage Sodrocode进行深水,轨迹角度范围从27度到60度,从水平上方延伸到水平。模拟包括大气效应,如消融和空袭。执行这些斜冲模拟,以帮助确定是否存在额外的危险因以前的研究未涵盖的影响。计算转移到空气冲击波和水的能量以及升高到高层大气中的海水量。水火山口尺寸和随后的表面升高型材,表面压力和水中的深度平均质量助量用于广场繁殖研究。类似于先前的三维模拟,这些模拟表明,除了在此模拟的那些下面的浅浅的入口角度,所得到的波是大致圆形的,并且初始波和中央喷射振荡是高湍流的并且耗散很多能量。无台幂使用NASA Pleiades超级计算机上的Lawrence Livermore ALE3D Sodrodode进行冲击海啸的长距离传播的轴对称模拟。这些模拟表明,在深海洋盆地的1个千兆TNT中的影响将产生经过分散的深水波,而在大陆架上的影响将产生不遭受分散的浅水波。该模拟还表明,大约1%的撞击动能的顺序转化为海啸波。这是基于爆炸测试数据和实验室规模的影响的比例为15%的初始半经验估计数。

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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