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OPEN SOURCE SOFTWARE OPENFOAM AS A NEW AERODYNAMICAL SIMULATION TOOL FOR ROCKET-BORNE MEASUREMENTS

机译:开源软件OPENFOAM作为一种新型的火箭弹测量气动仿真工具

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The only way to do in-situ measurements, which are very important experimental studies for atmospheric science, in the mesoshere/lower thermosphere (MLT) is to use sounding rockets. The drawback of using rockets is the shock wave appearing because of the very high speed of the rocket motion (typically about 1000 m/s). This shock wave disturbs the density, the temperature and the velocity fields in the vicinity of the rocket, compared to undisturbed values of the atmosphere. This effect, however, can be quantified and the measured data has to be corrected not just to make it more precise but simply usable. The commonly accepted and widely used tool for this calculations is the Direct Simulation Monte Carlo (DSMC) technique developed by G.A. Bird which is available as stand-alone program limited to use a single processor. Apart from complications with simulations of flows around bodies related to different flow regimes in the altitude range of MLT, that rise due to exponential density change by several orders of magnitude, a particular hardware configuration introduces significant difficulty for aerodynamical calculations due to choice of the grid sizes mainly depending on the demands on adequate DSMCs and good resolution of geometries with scale differences of factor of 10~3. This makes either the calculation time unreasonably long or even prevents the calculation algorithm from converging. In this paper we apply the free open source software OpenFOAM (licensed under GNU GPL) for a three-dimensional CFD-Simulation of a flow around a sounding rocket instrumentation. An advantage of this software package, among other things, is that it can run on high performance clusters, which are easily scalable. We present the first results and discuss the potential of the new tool in applications for sounding rockets.
机译:在中上/下热圈(MLT)中进行原位测量(这对大气科学而言是非常重要的实验研究)的唯一方法是使用探空火箭。使用火箭的缺点是由于火箭运动的速度非常高(通常约为1000 m / s),因此会出现冲击波。与大气的未扰动值相比,该冲击波扰乱了火箭附近的密度,温度和速度场。但是,可以量化这种影响,不仅要使其更加精确,而且必须简单地使用它,就必须对测量数据进行校正。由G.A.开发的直接模拟蒙特卡洛(DSMC)技术是用于此计算的公认的且广泛使用的工具。 Bird可以作为独立程序使用,仅限于使用单个处理器。除了与MLT高度范围内不同流态相关的物体周围流场模拟的复杂性(由于指数密度变化几个数量级而增加)外,由于选择了网格,特殊的硬件配置也给空气动力学计算带来了极大的困难。尺寸主要取决于对适当DSMC的要求以及良好的几何分辨率,比例差异为10〜3。这使得计算时间过长,甚至阻止了计算算法的收敛。在本文中,我们将免费的开放源代码软件OpenFOAM(在GNU GPL下获得许可)用于探测火箭仪器周围流的三维CFD模拟。除其他事项外,该软件包的一个优点是它可以在易于扩展的高性能群集上运行。我们介绍了第一个结果,并讨论了该新工具在探空火箭应用中的潜力。

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