基于窄带雷达RCS序列的空间目标尺寸估计

从窄带雷达横截面积(RCS)序列中提取目标尺寸特征对空间目标的分类识别具有重要价值. 本文在研究椭球体RCS序列特性的基础上, 提出了一种空间目标形状估计方法, 并进一步研究了空间目标尺寸估计问题, 提出了一种新的尺寸估计方法. 实测数据的验证表明, 该方法能有效估计卫星、碎片等空间目标的形状和二维尺寸.      

仿真输出非平均性能测度的Bayes估计

考虑离散事件仿真中一个非平均性能测度－－比例的估计问题，在对有关比例的已有估计方法的概述和分析的基础上，提出了一种比例的Ｂａｙｅｓ估计方法和贝塔分布的区间估计方法，从实验上对这些方法进行了研究和比较，从而证明了Ｂｅｙｅｓ方法能合理地给出比例的估计，而且仿真精度在大样本情形比已有方法略有提高，在小样本情形有明显的改进。     

基于比例积分强跟踪滤波器的故障估计

研究了线性系统执行机构和敏感器的故障估计方法．基于比例积分观测器具有同时估计系统状态和故障大小的能力,将比例积分观测器和强跟踪滤波器相结合,组成比例积分强跟踪滤波器来估计执行机构和敏感器故障,这种方法增强了对突变故障的快速跟踪能力．在系统发生故障时,比例积分强跟踪滤波器不仅能够快速检测、定位故障,而且还能估计出故障的大小．以某卫星为例,将此方法应用于推力器和陀螺的故障估计,并通过仿真验证了这种方法的有效性．     

伴飞航天器轨道修正点状态的最小二乘估计

研究了近圆轨道航天器长期伴随飞行在轨道修正时刻相对状态的最小二乘估计方法。针对长期伴飞航天器在固定时刻进行轨道修正的特点,提出采用最小二乘估计方法对轨道修正时刻的相对位置状态进行估计,并基于模型误差特点提出对该算法进行改进的加权最小二乘估计算法。算法具有计算相对简单、算法灵活等特点。仿真结果表明,对于固定时刻的状态估计,这种加权最小二乘估计算法和扩展卡尔曼滤波算法的效果相当,能够满足在轨长期伴随飞行在轨道修正时刻的相对状态估计精度要求。     

基于STLS的卫星惯量矩阵在轨估计

提出了一种采用结构总体最小二乘（Structured total least squares, STLS）进行卫星惯量矩阵在轨估计的方法,与当前估计方法相比,该方法在考虑敏感器测量噪声时能获得一致估计。首先由动量守恒定律得到估计方程,针对该方程的特点定义了惯量矩阵的STLS估计,并使用结构总体最小范数（Structured total least norm, STLN）算法进行求解。证明了当噪声为高斯分布时该STLS估计为极大似然估计,给出了该STLS估计具有一致性的充分条件,仿真结果验证了文章所提估计方法的有效性。     

量子科学实验卫星微振动地面测试与估计方法

介绍了卫星微振动地面测试和信号估计方法.根据量子科学实验卫星特点,对动量轮运行状态下光学载荷的微振动线位移及角位移进行估计.通过地面微振动测试系统,测量了动量轮运行下光学载荷的微振动加速度;应用小波积分方法,精确估计了卫星结构敏感点的振动线位移和振动角位移.通过工程实测证明了微振动测试与估计方法的有效性.研究结果对于高精度科学实验卫星微振动地面试验具有一定工程应用意义.      

机载目标状态估计器

研究基于空载雷达测量下的机动目标状态估计器的设计问题。通过建立直角坐标状态方程和选取一种伪测量量，并采用测量模型线性化的方法，建立起了估计器的基本结构，在此基础上增加距离通道的冗余滤波，进一步提高距离通道的估计精度，最后将估计器联入整个综合火力／飞行控制系统中，进行了Ｍｏｎｔｅ Ｃａｒｌｏ仿真，仿真结果表明，设计的目标状态估计器具有很好的跟踪估计性能。     

基于多模型滚动时域估计的卫星故障诊断

研究了卫星姿态控制系统故障诊断问题, 将滚动时域估计与交互式多模型(IMM)方法相结合, 利用滚动时域估计方法对系统状态进行估计, 系统转换概率也相应地利用了一个时间段的估计误差作为依据, 而不是只考虑一个时刻的估计误差, 因此有效减少了大噪声以及个别错误测量对诊断结果的影响. 最后的仿真结果证明了该算法的有效性.      

基于瞬时相位的BPSK信噪比估计算法

通过对加性高斯白噪声条件下正弦型信号瞬时相位分布情况进行研究,提出了一种新的BPSK(Binary Phase Shift Keying)信噪比估计方法.含噪信号瞬时相位的方差与信噪比之间存在近似线性的一一对应关系,以此为基础通过将含噪信号的估计方差与理论值相比较获得信噪比估计值.该方法直接对基带过采样信号进行处理,不需要事先进行符号定时与同步.使用计算机仿真测试了算法的估计性能,并与高阶累积量方法和子空间分解方法进行了比较,结果表明该算法具有更高的估计精度.      

基于多源图像弱监督学习的3D人体姿态估计

3D人体姿态估计是计算机视觉领域一大研究热点,针对深度图像缺乏深度标签,以及因姿态单一造成的模型泛化能力不高的问题,创新性地提出了基于多源图像弱监督学习的3D人体姿态估计方法。首先,利用多源图像融合训练的方法,提高模型的泛化能力;然后,提出弱监督学习方法解决标签不足的问题;最后,为了提高姿态估计的效果,改进了残差模块的设计。实验结果表明:改善的网络结构在训练时间下降约28%的情况下,准确率提高0.2%,并且所提方法不管是在深度图像还是彩色图像上,均达到了较好的估计结果。      

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

基于LuGre模型的电液加载系统摩擦补偿

为了提高电液加载系统控制精度,针对摩擦问题提出了基于LuGre摩擦模型的前馈补偿方法.建立了用于摩擦仿真分析和补偿器设计的电液加载系统数学模型;通过实验获取并分析了相关的摩擦数据;基于实验数据进行LuGre模型参数辨识,把LuGre模型和辨识结果引入电液加载系统数学模型,并进行仿真结果与实际摩擦数据的对照,证明了LuGre摩擦模型的准确性.设计前馈补偿器,进行了实验对比,实验结果表明前馈补偿器可将摩擦产生的控制误差有效地降至未补偿时的30%左右.      

Concept options for the aerial survey of Titan

Various aerial platforms intended for long endurance survey of the Titan surface are presented. A few novel concepts are introduced, including a heated methane balloon and a balloon with a tethered wind turbine. All the concept options are predicted to have lower scientific payload fractions than the Huygens probe. It is concluded that the selection of the best aerial platform option depends on more accurate mass estimates and a clear decision on whether, or not, in situ surface composition measurements are required in conjunction with aerial remote sensing.     

Heterogeneous solid/gas chemistry of organic compounds related to comets,meteorites, Titan,and Mars: Laboratory and in lower Earth orbit experiments

To understand the evolution of organic molecules involved in extraterrestrial environments and with exobiological implications, many experimental programs in the laboratory are devoted to photochemical studies in the gaseous phase as well as in the solid state. The validity of such studies and their applications to extraterrestrial environments can be questioned as long as experiments conducted in space conditions, with the full solar spectrum, especially in the short wavelength domain, have not been implemented. The experiments that are described here will be carried out on a FOTON capsule, using the BIOPAN facility, and on the International Space Station, using the EXPOSE facility. Vented and sealed exposition cells will be used, which will allow us to study the chemical evolution in the gaseous phase as well as heterogeneous processes, such as the degradation of solid compounds and the release of gaseous fragments.     

CoRoT and Kepler results: Solar-like oscillators

The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars.     

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

Radioactivity of the Moon and planets

In this report the main results of the study of radioactivity of the solar sistem bodies are considered. The radioactivity of the Moon and planets was measured by means of vehicles in situ. The radioactivity of the lunar samples, brought to the Earth was studied with laboratory equipment.     

The ESA scientific programme

The ESA scientific programme has, so far, provided several significant astrophysics experiments and further important missions are scheduled for execution during the next decade. These missions are briefly summarised together with several astrophysics investigations presently under study.     

直尺反转组合法测量直线度的理论分析

对直尺反转组合法的测量原理进行了较为深入的理论分析，指出测量的准确性受测头误差、采样点定位误差、直尺尺面斜率、直尺再定位误差、直尺各点直线度误差的变化率等五个方面共同作用。其中，采样点定位误差和直尺安装斜率影响直线度测量准确度这一结论，将适用于其他的直尺直线度测量方法，因而具有普遍的指导意义。     

一种提高螺栓联接强度的新方法

根据山本晃教授对螺栓，螺母，螺纹牙受力及其变形研究的成果，导出了该理论条件下受拉螺栓在等载荷受力状态下，当螺栓螺纹采用标准尺寸，螺母螺纹的螺旋线形状，并依据实用性，从螺母螺纹加工方便考虑，提出了近似等负荷螺纹。