在细长体尾迹中超音速展开的圆盘带隙降落伞模型的发展

Clara O’Farrell, Suman Muppidi, Joseph M. Brock, John W. Van Norman, I. Clark
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引用次数: 9

摘要

先进超音速降落伞膨胀研究和实验(ASPIRE)项目将研究圆盘间隙带(DGB)降落伞在细长机身后的超音速展开、膨胀和空气动力学。这些降落伞将是2012年火星科学实验室使用的dgb的全尺寸版本,并计划用于NASA的火星2020项目,并将通过从NASA的沃洛普斯飞行设施发射的探空火箭交付到火星飞行的目标部署条件。降落伞将在一个细长的有效载荷后进行测试,其直径大约是用于火星任务的入口太空舱的六分之一。降落伞的展开、充气和气动性能模型对于设计实验的关键方面是必要的,包括:确定降落伞和有效载荷的预期载荷和适用裕度;引导传感器的选择与放置;评估车辆轨迹的目标,范围安全和回收操作。此外,为了解释探空火箭实验的结果,并确定它们与火星上钝体后的预期性能之间的关系,需要了解降落伞在细长和钝体后的行为差异。然而,由于历史测试数据和建模先例的缺乏,对超声速DGB在细长身体后的性能进行建模是具有挑战性的。本文介绍了为ASPIRE探空火箭试验研制的超声速细长体尾流中DGBs的气动性能模型。这些模型的开发是基于在超声速细长体尾迹中部署的四种DGB的可用飞行试验,以及在钝体尾迹中部署的DGB的过去飞行和风洞实验数据,以及在过去任务中在火星上重建的DGB性能,以及计算流体动力学模拟。为了研究降落伞在两种尾迹下所遇到的流场差异,对超音速流动中钝体和细长体尾迹进行了模拟。这些模拟使该项目能够调查探空火箭试验与火星任务期间DGB飞行之间的根本区别,并评估用于评估火星飞行性能的探空火箭试验结构的局限性。
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Development of models for disk-gap-band parachutes deployed supersonically in the wake of a slender body
The Advanced Supersonic Parachute Inflation Research and Experiments (ASPIRE) project will investigate the supersonic deployment, inflation, and aerodynamics of Disk-Gap-Band (DGB) parachutes in the wake of a slender body. The parachutes will be full-scale versions of the DGBs used by the Mars Science Laboratory in 2012 and planned for NASA's Mars 2020 project and will be delivered to targeted deployment conditions representative of flight at Mars by sounding rockets launched out of NASA's Wallops Flight Facility. The parachutes will be tested in the wake of a slender payload whose diameter is approximately a sixth that of entry capsules used for Mars missions. Models of the deployment, inflation, and aerodynamic performance of the parachutes are necessary to design key aspects of the experiment, including: determining the expected loads and applicable margins on the parachute and payload; guiding sensor selection and placement; evaluating the vehicle trajectory for targeting, range safety, and recovery operations. In addition, knowledge of the differences in the behavior of the parachutes in the wake of slender and blunt bodies is required in order to interpret the results of the sounding rocket experiment and determine how they relate to expected performance behind blunt bodies at Mars. However, modeling the performance of a supersonic DGB in the wake of a slender body is challenging due to the scarcity of historical test data and modeling precedents. This paper describes the models of the aerodynamic performance of DGBs in supersonic slender-body wakes being developed for the ASPIRE sounding rocket test campaign. Development of these models is based on the four available flight tests of DGBs deployed in supersonic slender-body wakes as well as on data from past flight and wind-tunnel experiments of DGBs deployed in the wake of blunt bodies, on the reconstructed at-Mars DGB performance during past missions, and on computational fluid dynamics simulations. Simulations of the wakes of blunt and slender bodies in supersonic flow have been conducted in order to investigate the differences in the flowfields encountered by parachutes deployed in both wake types. The simulations have allowed the project to investigate the fundamental differences between the sounding rocket tests and the flight of a DGB during a Mars mission and to assess the limitations of the sounding rocket test architecture for evaluating flight performance at Mars.
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