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Finite-difference numerical modelling of gravito-acoustic wave propagation in a windy and attenuating atmosphere

机译:引力声波在大风和衰减大气中传播的有限差分数值模拟

摘要

Acoustic and gravity waves propagating in planetary atmospheres have been studied intensively as markers of specific phenomena such as tectonic events or explosions or as contributors to atmosphere dynamics. To get a better understanding of the physics behind these dynamic processes, both acoustic and gravity waves propagation should be modelled in a 3D attenuating and windy atmosphere extending from the ground to the upper thermosphere. Thus, in order to provide an efficient numerical tool at the regional or global scale we introduce a finite difference in the time domain (FDTD) approach that relies on the linearized compressible Navier-Stokes equations with a background flow (wind). One significant benefit of such a method is its versatility because it handles both acoustic and gravity waves in the same simulation, which enables one to observe interactions between them. Simulations can be performed for 2D or 3D realistic cases such as tsunamis in a full MSISE- atmosphere or gravity-wave generation by atmospheric explosions. We validate the computations by comparing them to analytical solutions based on dispersion relations in specific benchmark cases: an atmospheric explosion, and a ground displacement forcing.
机译:在行星大气中传播的声波和引力波已被大量研究,作为特定现象(例如构造事件或爆炸)的标志,或对大气动力学的贡献。为了更好地理解这些动态过程背后的物理原理,应该在从地面延伸到上层热层的3D衰减多风大气中对声波和重力波的传播进行建模。因此,为了在区域或全球范围内提供有效的数值工具,我们引入了时域有限差分(FDTD)方法,该方法依赖于具有背景流(风)的线性可压缩Navier-Stokes方程。这种方法的一个显着优点是它的多功能性,因为它可以在同一模拟中同时处理声波和重力波,这使人们可以观察它们之间的相互作用。可以针对2D或3D现实情况(例如在完整的MSISE大气中发生海啸或通过大气爆炸产生重力波)进行模拟。我们通过将计算结果与基于特定基准情况下的色散关系的解析解进行比较来验证计算结果:大气爆炸和地面位移强迫。

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