火星探测降落伞模型高速风洞变迎角试验技术

为获得火星探测器物伞系统动力学仿真中需要使用的降落伞轴向力、法向力、俯仰力矩系数，开展了火星探测降落伞模型高速风洞变迎角试验技术研究，研制了火星探测降落伞模型高速风洞变迎角试验装置，进行了火星探测降落伞模型高速风洞变迎角试验，获得了火星探测降落伞模型在马赫数范围0.4～0.8、迎角范围0°～25°时的轴向力、法向力和俯仰力矩系数，并对支撑干扰及洞壁干扰影响进行了扣除修正。试验结果表明：火星探测降落伞模型的轴向力系数随迎角变化较小；常规透气伞的法向力系数随迎角增大而增大，在马赫数为0.4和0.6时，低透气伞的法向力系数在小迎角时随迎角增大而减小；在马赫数范围0.4～0.8时，常规透气伞静稳定，低透气伞的静稳定性较常规透气伞减小，在马赫数为0.4和0.6时，低透气伞在零迎角时静不稳定，出现了非零配平 迎角。     

火星进入气体辐射加热研究进展

针对飞行器进入火星大气时气体辐射加热对防热设计带来不确定性，在简述火星探测和气体辐射研究的发展历程的基础上，对火星进入气体辐射加热研究的进展进行综述。首先，针对火星大气环境描述了气体辐射加热的概念和问题由来。其次，重点综述了近年来火星进入气体辐射加热基础模型的数值和试验研究进展，其中包括：热化学非平衡气体动力学、气体辐射特性和辐射传输的计算模型与方法等数值研究；地面测试设备、试验技术和模拟火星大气环境的气体辐射测量与验证等试验研究。再次，综述了流动辐射耦合和后体气体辐射加热等火星进入器设计方面开展的研究。最后，对未来火星进入气体辐射加热研究进行了展望，提出了研究建议。     

Planetary penetrators: Their origins,history and future

Penetrators, which emplace scientific instrumentation by high-speed impact into a planetary surface, have been advocated as an alternative to soft-landers for some four decades. However, such vehicles have yet to fly successfully. This paper reviews in detail, the origins of penetrators in the military arena, and the various planetary penetrator mission concepts that have been proposed, built and flown. From the very limited data available, penetrator developments alone (without delivery to the planet) have required ∼$30M: extensive analytical instrumentation may easily double this. Because the success of emplacement and operation depends inevitably on uncontrollable aspects of the target environment, unattractive failure probabilities for individual vehicles must be tolerated that are higher than the typical ‘3-sigma’ (99.5%) values typical for spacecraft. The two pathways to programmatic success, neither of which are likely in an austere financial environment, are a lucky flight as a ‘piggyback’ mission or technology demonstration, or with a substantial and unprecedented investment to launch a scientific (e.g. seismic) network mission with a large number of vehicles such that a number of terrain-induced failures can be tolerated.     

火星卫星的冻结轨道研究

冻结轨道是一种稳定的轨道,地球、火星、月球的卫星因引力场的南北不对称,都存在冻结轨道.由于主星体引力场的不同,它们卫星的冻结轨道也有不同的特性.地球卫星的冻结执道的偏心率非常小,对卫星遥感非常有利,国内外已有相当多的近地遥感卫星采用这种轨道.月球卫星的冻结轨道偏心率随轨道倾角的不同有很大的变化,对月球卫星冻结轨道的研究...     

Disturbance observer-based robust guidance for Mars atmospheric entry with input saturation

With low-lifting capability taken into account,a robust guidance law for Mars entry vehicles with low lift-to-drag ratios,such as Mars Science Laboratory(MSL),is presented.Consider the nonlinear term in the drag dynamic equation and bounded disturbances as a lumped disturbance,and design a linear disturbance observer(DOB)to estimate it.With the consideration of the control input saturation,an innovative sliding surface and a virtual system are introduced to design the guidance law.Analyses of disturbance observer performance and Lyapunov-based transient performance are also presented.It is shown that the drag tracking error can be adjustable by explicit choices of design parameters.Simulation results confirm the effectiveness of the proposed guidance law.     

火星进入器壁面脉动压力环境数值模拟

为研究跨超声速阶段来流马赫数、来流攻角及配平翼展开角的变化对进入器壁面脉动压力环境的影响规律，本文采用脱体涡方法对火星进入器模型开展非定常数值模拟，获取壁面不同位置处的脉动压力信息。研究表明：在跨超声速阶段，进入器壁面脉动压力环境随马赫数的增加而趋于减缓。配平翼迎风面分离区受脱体激波影响明显，当来流马赫数较小时，可压缩效应较弱，分离区涡流运动剧烈，诱导的脉动压力环境较强；随着来流马赫数的增加，脱体激波对分离区抑制作用增强，分离区运动受到限制，诱导的脉动压力环境趋于平缓。此外，随着来流攻角增加，配平翼迎风面上再附点的位置向翼根方向转移，从而使翼根处的脉动压力环境趋于恶劣。当配平翼展开180°时，分离区再附点位置基本固定，配平翼迎风面脉动压力环境得到一定程度的减缓。功率谱分析表明，在配平翼迎风面上诱导的脉动压力能量主要集中在中低频区域。     

模型参数扰动下的火星大气进入鲁棒状态估计方法

针对火星大气进入段模型参数扰动及动力学系统的强非线性影响导航系统状态精确估计问题，提出了一种模型参数扰动下的鲁棒插值滤波（DDF）方法。该方法在传统插值滤波方法代价函数的基础上，通过把扰动参数对状态估计精度影响的度量矩阵乘积的迹增广到代价函数，推导了具有解析滤波增益形式的鲁棒插值滤波方法。同时，通过实时计算进入过程中导航系统的非线性，基于系统非线性度给出了鲁棒插值滤波方法阶次自适应选取准则。只在系统强非线性阶段采用高阶鲁棒插值滤波方法，既保证状态估计精度，同时满足导航系统实时性需求。仿真结果表明，提出的鲁棒插值滤波方法比传统的一阶插值滤波方法估计精度更高，能达到二阶鲁棒插值滤波方法的估计精度，比整个进入过程采用二阶鲁棒插值滤波方法具有更高的解算效率。     

Improved uncertainty propagation method of dynamic model for Mars entry spacecraft

In order to research the uncertainty propagation laws of Mars entry dynamic equations for the Mars entry phase,an improved method was presented for analyzing the effect of the initial state uncertainties and uncertainty factor on the system state in the state trajectories.When applying the method to the entry phase of one of the NASA Mars exploration missions,the simulation results agreed well with the Monte Carlo method,especially the flight path angle simulation at least reaching 92%.It is found that the improved method can not only predict the uncertainty propagation laws with high accuracy of at least 92%in flight path angle simulation and large application scope from-0.1degree to 0.1degree,compared with local linearization method,but also save several hours relative to Monte Carlo method.     

火星着陆关键环节多学科交叉设计与验证

针对火星着陆任务在飞行环境、地面验证、系统间关联性等方面面临的技术挑战,根据火星着陆关键环节涉及的气动减速、降落伞减速、动力下降和着陆缓冲四个主要阶段,分别分析了大气进入方式、进入初始条件、气动外形、防热、开伞控制、大底弹射、背罩规避机动与触火关机等关键要素,并介绍了天问一号与其他典型火星着陆任务开展的多学科交叉设计过...     

Spectroscopic evaluation of polyurea crosslinked aerogels,as a substitute for RTV-based chromatic calibration targets for spacecraft

Room temperature vulcanizing (RTV)-based components have been used on Mars Pathfinder, the Mars rovers, Spirit and Opportunity, as well as the Phoenix Lander as a support matrix for pigmented panoramic camera calibration targets. RTV 655 has demonstrated superiority to other polymers due to its unique range of material properties namely mechanical stability between −115 and 204 °C and UV radiation tolerance. As a result, it has been the number one choice for many space-related missions. However, due to the high mass density and the natural tendency for electrostatic charging RTV materials have caused complications by attracting and retaining dust particles (Sabri et al., 2008). In the current project we have investigated the relevant properties of polymer-reinforced (crosslinked) silica aerogels with the objective of substituting RTV-based calibration targets with an aerogel based design. The lightweight, mechanical strength, ability to accept color pigments, and extremely low dust capture makes polyurea crosslinked aerogels a strong candidate as a chromatic standard for extraterrestrial missions. For this purpose, the reflection spectra, gravimetric analysis, and low temperature response of metal oxide pigmented, polyurea crosslinked silica aerogels have been investigated and reported here.