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Calculations of asteroid impacts into deep and shallow water

机译:小行星撞击深水和浅水的计算

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摘要

Contrary to received opinion, ocean impacts of small (<500 m) asteroids do not produce tsunamis that lead to world-wide devastation. In fact the most dangerous features of ocean impacts, just as for land impacts, are the atmospheric effects. We present illustrative hydrodynamic calculations of impacts into both deep and shallow seas, and draw conclusions from a parameter study in which the size of the impactor and the depth of the sea are varied independently. For vertical impacts at 20 km/s, craters in the seafloor are produced when the water depth is less than about 5-7 times the asteroid diameter. Both the depth and the diameter of the transient crater scale with the asteroid diameter, so the volume of water excavated scales with the asteroid volume. About a third of the crater volume is vaporised, because the kinetic energy per unit mass of the asteroid is much larger than the latent heat of vaporization of water. The vaporised water carries away a considerable fraction of the impact energy in an explosively expanding blast wave which is responsible for devastating local effects and may affect worldwide climate. Of the remaining energy, a substantial portion is used in the crown splash and the rebound jet that forms as the transient crater collapses. The collapse and rebound cycle leads to a propagating wave with a wavelength considerably shorter than classical tsunamis, being only about twice the diameter of the transient crater. Propagation of this wave is hindered somewhat because its amplitude is so large that it breaks in deep water and is strongly affected by the blast wave's perturbation of the atmosphere. Even if propagation were perfect, however, the volume of water delivered per metre of shoreline is less than was delivered by the Boxing Day 2004 tsunami for any impactor smaller than 500 m diameter in an ocean of 5 km depth or less. Near-field effects are dangerous for impactors of diameter 200 m or greater; hurricaneforce winds can extend tens of kilometers from the impact point, and fallout from the initial splash can be extremely violent. There is some indication that near-field effects are more severe if the impact occurs in shallow water.
机译:与已收到的意见相反,小型(小于500 m)小行星的海洋影响不会产生导致全球性破坏的海啸。实际上,海洋影响和陆地影响一样,最危险的特征是大气影响。我们介绍了对深海和浅海的影响的示例性水动力计算,并从参数研究得出结论,在该研究中,冲击器的大小和海深是独立变化的。对于20 km / s的垂直撞击,当水深小于小行星直径的5-7倍时,会在海底产生火山口。瞬变陨石坑的深度和直径均与小行星直径成正比,因此,挖出的水量与小行星体积成正比。因为小行星每单位质量的动能比水的汽化潜热大得多,所以约有三分之一的火山口被汽化了。汽化水在爆炸性爆炸波中带走了相当一部分冲击能量,爆炸波造成了毁灭性的局部后果,并可能影响全球气候。在剩余的能量中,相当大的一部分用于冠顶飞溅和回弹射流,后者在瞬变陨石坑坍塌时形成。坍塌和回弹周期导致传播的波的波长比传统海啸短得多,仅为瞬变陨石坑直径的两倍。该波的传播受到某种程度的阻碍,因为它的振幅太大,以至于它在深水中破裂并且受到爆炸波对大气扰动的强烈影响。即使传播是完美的,但是对于直径小于或等于5 m的海洋中直径小于500 m的任何撞击器,每米海岸线的输水量仍少于节礼日2004年海啸时的输水量。对于直径200 m或更大的撞击器,近场效应是危险的;飓风可以从撞击点延伸数十公里,并且初始飞溅的辐射可能非常剧烈。有迹象表明,如果影响发生在浅水中,近场影响会更严重。

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