诱发卫星深层充电的高能电子环境模式研究

文章介绍了与卫星介质深层充电相关的辐射带高能电子环境的主要特征和规律,建立了相应的高能电子环境模式及软件,并运用该模式针对某飞行器的深层充放电危险性进行了分析和评估。结果表明该模式相对于AE8模式更好地反映了高能电子环境的动态特征,与欧空局建立的FLUMIC模式符合较好。该模式与深层充电分析模型相结合,可用于对航天器的充放电异常进行在轨诊断,以及在工程上针对深层充电进行防护设计。     

有源相控阵中场测量中的空间误差研究

由于中场监测设备量少,且测量效率高,所以是有源相控阵雷达阵面测量的重要方法之一,在工程中得到了广泛应用。其系统误差包括监测方法误差和测量设备误差,其中测量方法误差非常关键,而测量设备误差与所采用的具体设备有关。在中场测量中,探头的位置偏移导致的空间误差是其特有的测量方法误差。本文对空间误差进行了理论分析,并以x波段有源相控阵的中场测量为例,给出了空间误差的计算结果和实验结果。计算结果表明,空间幅度误差很小;空间相位误差与被测阵面口径、测量距离和探头位置偏移有关。实验结果进一步验证了这种计算结果。分析结果为中场测量的实施提供了参考,具有一定的工程意义。     

国外深空探测态势特点与启示（上）

通过对国外主要航天大国在深空探测领域发展过程的梳理,重点分析了各国在无人深空探测技术、载人深空探测技术和地面测控通信技术三个方面的技术发展特点,并从总体角度对其主要技术特征和关键技术进行了深入剖析,从中提炼出对我国深空探测活动的启示,以期对我国深空探测的开展有所借鉴和推动。     

国外深空探测态势特点与启示（下）

通过对国外主要航天大国在深空探测领域发展过程的梳理,重点分析了各国在无人深空探测技术、载人深空探测技术和地面测控通信技术三个方面的技术发展特点,并从总体角度对其主要技术特征和关键技术进行了深入剖析,从中提炼出对我国深空探测活动的启示,以期对我国深空探测的开展有所借鉴和推动。     

空天飞机全C／SiC复合材料机身襟翼的静力试验研究与失效分析

针对全C／SiC复合材料机身襟翼再人过程中受到强烈的气动载荷作用的受力状况,进行了静力试验考核。对静力试验方法进行了讨论与探索,通过验证性的试验,确定了传统的贴帆布带加载的静力试验方案。并通过有限元建模计算明晰了机身襟翼结构的静力试验的危险区域。静力试验中,襟翼试件在未达到试验设计载荷的情况下,出现了提前破坏。通过对试件的传力路线的分析以及损伤部位的观察和研究,找出了失效的原因是由于角盒工艺上的缺陷造成的,并提出了工艺上改进的方法。     

Application of support vector machine combined with K-nearest neighbors in solar flare and solar proton events forecasting

The support vector machine (SVM) combined with K-nearest neighbors (KNN), called the SVM-KNN method, is new classing algorithm that take the advantages of the SVM and KNN. This method is applied to the forecasting models for solar flares and proton events. For the solar flare forecasting model, the sunspot area, the sunspot magnetic class, and the McIntosh class of sunspot group and 10 cm solar radio flux are chosen as inputs; for the solar proton event forecasting model, the inputs include the longitude of active regions, the flux of soft X-ray, and those for the solar flare forecasting model. Detailed tests are implemented for both of the proposed forecasting models, in which the SVM-KNN and the SVM methods are compared. The testing results demonstrate that the SVM-KNN method provide a higher forecasting accuracy in contrast to the SVM. It also gives an increased rate of ‘Low’ prediction at the same time. The ‘Low’ prediction means occurrence of solar flares or proton events with predictions of non-occurrence. This method show promise for forecasting models of solar flare and proton events.     

Human response to high-background radiation environments on Earth and in space

The main long-term objective of the space exploration program is the colonization of the planets of the Solar System. The high cosmic radiation equivalent dose rate represents an inescapable problem for the safe establishment of permanent human settlements on these planets. The unshielded equivalent dose rate on Mars ranges between 100 and 200 mSv/year, depending on the Solar cycle and altitude, and can reach values as high as 360 mSv/year on the Moon. The average annual effective dose on Earth is about 3 mSv, nearly 85% of which comes from natural background radiation, reduced to less than 1 mSv if man-made sources and the internal exposure to Rn daughters are excluded. However, some areas on Earth display anomalously high levels of background radiation, as is the case with thorium-rich monazite bearing sand deposits where values 200–400 times higher than the world average can be found. About 2% of the world’s population live above 3 km and receive a disproportionate 10% of the annual effective collective dose due to cosmic radiation, with a net contribution to effective dose by the neutron component which is 3–4 fold that at sea level. Thus far, epidemiological studies have failed to show any adverse health effects in the populations living in these terrestrial high-background radiation areas (HBRA), which provide an unique opportunity to study the health implications of an environment that, as closely as possibly achievable on Earth, resembles the chronic exposure of future space colonists to higher-than-normal levels of ionizing radiation. Chromosomal aberrations in the peripheral blood lymphocytes from the HBRA residents have been measured in several studies because chromosomal damage represents an early biomarker of cancer risk. Similar cytogenetic studies have been recently performed in a cohort of astronauts involved in single or repeated space flights over many years. The cytogenetic findings in populations exposed to high dose-rate background radiation on Earth or in space will be discussed.     

载体姿态无扰的自由漂浮空间机器人运动学特性研究

针对载体姿态无扰的自由漂浮空间机器人的运动学问题,引入具有非完整特性的载体 姿态无扰约束方程,推导了载体姿态无扰的自由漂浮空间机器人广义雅可比矩阵。采用等效 杆的概念,分析了普通状态的自由漂浮空间机器人和载体姿态无扰的自由漂浮空间机器人可 达工作空间;基于载体姿态无扰的自由漂浮空间机器人广义雅可比矩阵所得到的奇异方程, 研究了载体姿态无扰的自由漂浮空间机器人动力学奇异性。仿真结果验证了普通状态的自由 漂浮空间机器人与载体姿态无扰的自由漂浮空间机器人运动学问题的差异性。研究结果为载 体姿态无扰的自由漂浮空间机器人运动规划及控制研究奠定了理论基础。
     

双臂空间机器人关节运动的一种增广自适应控制方法

讨论了载体位置、姿态均不受控制情况下,具有未知参数的自由漂浮双臂空间机器人系统的自适应控制问题.由于此类机器人系统具有结合系统动量及动量矩守恒关系得到完全能控形式的系统动力学方程,以及系统惯性参数不符合惯常的线性函数关系的特点,因而地面机器人的控制方法在此难以直接推广应用.为了克服上述难点,仅将系统动量守恒关系耦合到系统动力学方程当中,而不耦合系统动量矩守恒关系,结果得到一组欠驱动形式的系统动力学方程.该系统动力学方程的优点是关于一组组合惯性参数能保持惯常的线性函数关系.以此为基础,并借助增广变量法,针对双臂空间机器人末端爪手所持载荷参数未知的情况,设计了关节空间轨迹跟踪的自适应控制方案.该控制方案的显著优点为,不需要测量、反馈双臂空间机器人漂浮基的位置、移动速度和移动加速度.系统的数值仿真,证实了方法的有效性.      

基于X射线脉冲星的深空探测器自主导航方案

X射线脉冲星自主导航系统可以为深空探测器提供位置、速度、时间和姿态等丰富且自主的导航信息,以X射线脉冲星测得的信息作为量测量,结合轨道动力学方程,对航天器的轨道进行自主估计确定。论文阐述了该方案的导航原理,在借鉴现有航天器导航系统的基础上,提出了基于X射线脉冲星导航的方案,介绍了方案的硬件组成、系统结构,并针对方案中导航敏感器多冗余的特征,给出了基于多传感器组合导航技术的结构,最后用仿真资料对方案做了性能概算和精度估计。