Numerical gas-dynamic computational methods in problems of rarefied jet flow about obstacles

T.G. Smila, L. Pecherytsia
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Abstract

The development of competitive space hardware calls for continuing improvements in the accuracy of simulation of gas-dynamic processes in the space vehicle vicinity. This may contribute to extending the active life of spacecraft, thus improving the economic efficiency of space activities. In particular, quite a topical problem is the simulation of the interaction of rarefied jets from the propulsion system of a spacecraft with its individual components. To solve this problem in the case of a rather high surrounding vacuum, use is made of the molecular-kinetic concept of the gas structure based on the Boltzmann equation. The aim of this paper is to overview existing methods of simulation of gas-dynamic processes near spacecraft in a rarefied gas flow with account for propulsion system jets and to choose the most promising approaches to the solution of this problem. Among the methods considered, several main lines are set off: approximate, analytical, and numerical methods. Approximate methods use physical models of jet flow, approximation of numerical results, or a combination of both approaches. Analytical methods are based on essentially simplified assumptions and are intended for a very narrow class of problems. Numerical methods are the most universal tool of theoretical study. At the same time, each numerical method has a range of application of its own. At present, the most used and promising methods are statistical simulation methods: the direct simulation Monte Carlo method (DSMCM) and the test particle method (TPM). The former splits the continuous process of molecule motion and collisions in a rarefied gas into two successive independent stages (free-molecular transfer and relaxation) at each small time step. The simulation is done by time steps and in fact reproduces a nonstationary process. The latter, the TPM, consist in a statistical successive simulation of the wandering of test particles (molecules) on the background of field ones about the cells of the computational grid. Test particles, which move within the cells of the computational area, periodically collide with the obstacle in the flow and field particles, and in doing so they gradually change both their velocity and the field characteristics. For both statistical approaches, the simulation accuracy, as can be expected, is inversely proportional to the square root of the number of tests: the number of time steps and modeling particles for the DSMCM and the number of successively simulated test particle trajectories for the TPM. This may greatly affect the possibility of attaining a desired accuracy.
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障碍稀薄射流问题的数值气动力计算方法
竞争性空间硬件的发展要求不断提高空间飞行器附近气体动力学过程模拟的精度。这可能有助于延长航天器的有效寿命,从而提高空间活动的经济效率。特别是,一个相当热门的问题是模拟来自航天器推进系统的稀薄射流与其各个部件之间的相互作用。为了在周围真空相当高的情况下解决这个问题,使用了基于玻尔兹曼方程的气体结构的分子动力学概念。本文的目的是概述在稀薄气流中考虑推进系统射流的航天器附近气体动力学过程的现有模拟方法,并选择最有前途的方法来解决这一问题。在所考虑的方法中,提出了几条主线:近似方法、解析方法和数值方法。近似方法使用射流的物理模型,近似数值结果,或两种方法的结合。分析方法基本上是以简化的假设为基础的,用于解决一类非常狭窄的问题。数值方法是理论研究中最通用的工具。同时,每种数值方法都有自己的应用范围。目前应用最多、最有前途的方法是统计模拟方法:直接模拟蒙特卡罗法(DSMCM)和测试粒子法(TPM)。前者将稀薄气体中分子运动和碰撞的连续过程在每个小时间步长上分成两个连续的独立阶段(自由分子转移和弛豫)。模拟是通过时间步长完成的,实际上再现了一个非平稳过程。后者,即TPM,包括对测试粒子(分子)在计算网格细胞周围的场粒子背景上的漂移进行统计连续模拟。在计算区域的单元内移动的测试粒子周期性地与流和场粒子中的障碍物碰撞,并在此过程中逐渐改变其速度和场特性。对于这两种统计方法,可以预期的是,模拟精度与测试次数的平方根成反比:DSMCM的时间步长和建模粒子的数量以及TPM的连续模拟测试粒子轨迹的数量。这可能会极大地影响获得所需精度的可能性。
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