Study on Dynamic Characteristics of Mars Entry Module in Transonic and Supersonic Speeds

Qi Li, Rui Zhao, Sijun Zhang, W. Rao, Haogong Wei
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引用次数: 2

Abstract

The aerodynamic configuration of the Tianwen-1 Mars entry module that adopts a blunt-nosed and short body shape has obvious dynamic instability from transonic to supersonic speeds, which may bring risk to parachute deployment. The unsteady detached eddy of the entry module cannot be accurately simulated by the Reynolds-Averaged Navier-Stokes (RANS) model, while the computational cost for direct numerical simulation (DNS) and large eddy simulation (LES) is huge. It is difficult to implement these methods in the coupled engineering calculation of unsteady flow and motion. This paper proposes the integrated numerical simulation method of computational fluid dynamics and rigid body dynamics (CFD/RBD) based on detached eddy simulation (DES) and calculates and studies the dynamic characteristics of attitude oscillation of the Mars entry module in free flight from transonic to supersonic speeds with one degree of freedom (1-DOF) at small releasing angle of attack. In addition, the unstable range of Mach number and angle of attack are determined, and the effect of different afterbody shapes on dynamic stability is analyzed.
火星登月舱跨声速和超声速动态特性研究
“天文一号”火星登陆舱采用钝鼻短身型的气动配置,在跨声速到超声速之间存在明显的动力不稳定性,可能给降落伞展开带来风险。reynolds - average Navier-Stokes (RANS)模型无法准确模拟进入舱的非定常分离涡,而直接数值模拟(DNS)和大涡模拟(LES)的计算成本巨大。这些方法在非定常流动耦合工程计算中难以实现。提出了基于分离涡模拟(DES)的计算流体动力学与刚体动力学(CFD/RBD)综合数值模拟方法,计算研究了火星登月舱在小释放攻角下跨声速到超音速自由飞行时姿态振荡的动力学特性。此外,确定了马赫数和攻角的不稳定范围,并分析了不同后体形状对动稳定性的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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