载人小行星探测任务总体方案研究

设计了在近地轨道组装具有分组单元结构的载人深空飞船,包括核热推进单元、燃料储箱与供给单元、主动防辐射单元、人工重力单元、深空居住舱与多任务乘员舱等,给出了各个单元的尺寸与质量参数,并对主要单元的具体组成、功能和技术特点进行了分析。在此基础上,本文以编号4660的Nereus小行星为探测目标,设计了两脉冲转移初始轨道,并进行了轨道优化,得到了发射窗口和最优转移轨道。仿真结果表明,给出的最优两脉冲转移轨道单次施加脉冲在5km/s以内,单程转移时间在160d以内,能够满足未来能量较小的载人小行星探测任务。     

地磁场中卫星不侧置态下磁矩测试方法

对地磁场中卫星不倒置状态下分离卫星Z分量磁矩的测试及数据处理方法进行了研究。利用地球磁场方向特征、卫星剩磁矩与感磁矩在不同测量状态和测量过程中的变化,确定卫星Z分量磁矩含地磁垂直向感磁影响与不含地磁垂直向感磁影响的比例关系,基于积累的不同卫星水平和垂直向的磁测试数据,用近场法计算,获得了卫星Z分量的感磁系数。试验表明:用该法测得的Z分量磁矩测量相对误差不大于30%,工程上有较高的实用价值。     

多约束条件下月亮对IGSO/MEO卫星干扰预报方法

针对IGSO/MEO卫星倾斜轨道(55 °)和偏航主动姿态控制的特殊性,研究了适用倾斜中高轨卫星月球干扰的亮度模型、地球遮挡模型、几何满足模型,提出了多元素约束条件下的月球干扰预报方法,解决了传统预报算法虚警概率较大的问题.实际控制结果表明,该方法实现了对在轨IGSO/MEO卫星地球敏感器月球干扰的准确预报,取得了很好的应用效果.     

Highly Elliptical Orbits for Arctic observations: Assessment of ionizing radiation

The ionizing radiation environment was analyzed for a variety of potential Highly Elliptical Orbits (HEOs) with orbital periods ranging from 6 h to 24 h suitable to continuously monitor the Arctic region. Several models available from the ESA Space Environment Information System (SPENVIS) online tool were employed, including the new-generation AE9/AP9 model for trapped radiation. Results showed that the Total Ionizing Dose (TID) has a well-pronounced local minimum for the 14-h orbit, which is nearly identical to the overall minimum observed for the longest orbital period (24 h). The thickness of slab aluminum shielding required to keep the annual TID below 10, 5 and 3.33 krad (i.e. 150, 75 and 50 krad for 15 years of mission duration) for a 14-h orbit is 2.1, 2.7 and 3.1 mm respectively. The 16-h orbit requires an additional 0.5 mm of aluminum to achieve the same results, while the 24-h orbit requires less shielding in the order of 0.2–0.3 mm. Comparison between the AE8/AP8 and AE9/AP9 models was conducted for all selected orbits. Results demonstrated that differences ranged from −70% to +170% depending on orbit geometry.     

航天器交会对接模拟系统逼近过程自抗扰控制

航天器交会对接地面模拟系统用于研究航天器交会对接过程的动力学、导航与控制等方面的相关问题。模拟器通过气浮轴承悬浮在大理石平台上来模拟太空的无摩擦微重力环境。通常情况下要保证大理石平台足够水平,由于实际平台不可能完全水平,模拟器的重力分量会使模拟器产生下滑现象,这种现象对大型地面模拟器设备尤为严重。针对模拟器的逼近过程设计了轨迹规划。为了减小测量信号噪声的影响,采用跟踪微分器(TD)对整个逼近过程中的测量信号进行滤波。针对逼近过程中模拟器存在下滑力等干扰问题设计控制器,通过扩张状态观测器(ESO)实时估计干扰量,进而对干扰量进行补偿。对模拟器冷喷气推力系统制定了推力器分配策略,采用脉冲宽度调制(PWM)技术实现对推力的近似等效。提出的控制方法应用于航天器交会对接地面模拟系统,实验结果表明所提出的控制方法能有效消除下滑力等干扰的影响。     

多GNSS掩星大气探测卫星星座设计

为减少无线电掩星(RO)大气探测星座的卫星数量并增加探测数据量,将北斗（BD）和GPS、Galileo、GLONASS共同作为探测信源,提出一种多全球导航卫星系统（GNSS）掩星大气探测星座概念和优化设计方法。融合先验大气模型和二维射线追踪算法,建立兼容多GNSS信源的掩星事件前向模拟算法,实现掩星事件快速精确仿真;给出多GNSS掩星大气探测星座参数对探测性能的影响特性,降低了星座模型的复杂度;并利用改进的蚁群算法实现星座参数寻优。设计结果与COSMICII星座相比,卫星数量减少2颗,探测数据量增加了40%,探测均匀性提高了67%。     

一种利用地球敏感器的星光导航方法

针对直接敏感地平的红外地平仪-星光导航系统精度低的问题,提出通过建立扁率误差补偿函数,研究扁率引起的姿态角测量误差;建立地心矢量的姿态角误差模型,通过修正地球扁率误差来补偿姿态角,对卫星施加姿态偏转指令调整地心矢量偏移。同时基于SODERN地球红外辐射模型,考虑红外辐射强度随纬度和季节的变化建立真实红外辐射曲线,通过滤波算法获得精确的地球切线边缘的量测信息,提高红外地平仪测量精度。仿真结果表明,该方法有效提高了基于红外地平仪的星光导航定位方法的可靠性和精度,导航位置误差能达到500m左右,较原有系统提高3倍以上。     

宽频角振动地面模拟试验设备的研制

为了解并减小探月着陆系统之敏感器容易受到宽频角振动影响的任务风险,有必要进行宽频角振动地面模拟试验。文章首先提出了宽频角振动的振动转换结构和测量方法,在此基础上完成了试验设备的研制,之后针对探月着陆系统成像敏感器遭遇的角振动环境进行了地面模拟测试。测试结果表明:该试验设备的宽频角振动模拟频率范围为0~2000 Hz,控制精度达到±15%（2σ）,同时还可模拟包括平移和转动在内的着陆系统刚体运动。该设备已用于敏感器在角振动环境下的地面模拟试验验证。     

Experiments of effects of inlet-air distortion on aerodynamic performance in transonic compressor

The inlet-air distortion which was caused by high angle-of-attack flight was simulated by plugboard.Experiments were conducted on a transonic axial-flow compressor's rotor at 98% rotating speed.The flow-field characteristics and mechanism of performance degradation were analyzed in detail.The compressor inlet was divided into four sectors at circumference under inlet-air distortion.They were undistorted sector,transition sector A where the rotor was rotating into the distortion sector,distorted sector and transition sector B where the rotor was rotating out of the distortion sector.The experimental results show that compared with undistorted sector,there is a subsonic flow in transition sector A,so the pressure ratio is decreased by a large margin in this sector.However, the shock wave is enhanced in distortion sector and transition sector B, and thus the pressure ratio increases in these sectors.Because of the different works at circumference,the phase angle of total pressure changes 90° when the inlet total pressure distortion passes through compressor rotor.In addition,the frequency and amplitude of disturbances in front of the rotor strengthenes under inlet distortion,so the unstable flow would take place in advance.In addition, the position of stall inception is in one of the transition sectors.      

基于Orbiter的航天器升力式再入特性仿真

升力式再入是指航天器进入大气层时产生一定可控升力,对提高落点精度具有重要意义。为了研究升力式再入的动力学特性,采用Orbiter模拟器的应用程序接口,在其飞行动力学模型基础上,对航天器从低轨道升力式再入返回过程进行仿真。通过仿真试验,分析热流、过载、动压等参数的变化规律,初步摸清了升力式再入的动力学特性,并对升力式再入和弹道式再入仿真结果参数进行了比较和分析,结果表明升力式再入能很好解决过载和热流峰值高的问题。