变结构航天器模糊神经网络滑模控制器设计

变结构航天器是目前航天领域的重要发展方向,航天器结构的变化将导致质量分布发生明显变化,这对航天器动力学建模和控制器设计都提出新的问题。针对这种情况,采用混合坐标法和拉格朗日方程建立了航天器刚柔耦合动力学模型,利用几种典型工况的参数近似得到变结构过程中动力学参数的变化规律。设计滑模控制器对航天器变结构过程进行姿态控制,为提高滑模控制器的适应性,设计模糊神经网络（FNN）自适应调节滑模控制器参数,并利用径向基函数（RBF）神经网络逼近动力学模型,得到控制力矩与姿态变化之间的近似关系,用于FNN的优化。通过仿真得到航天器变结构期间无控、滑模控制和模糊神经网络滑模控制的姿态变化,仿真结果对比验证了模糊神经网络滑模控制对于滑模控制的优势,证明了其在变结构航天器姿态控制方面的有效性。     

基于摄动模型的挠性航天器姿态控制系统设计

为了完成挠性航天器高精度姿态控制任务,首先采用摄动法分析了挠性航天器动力学方程,得到相应的0阶和1阶动力学系统.针对0阶非线性时不变系统,同时考虑到转动惯量不确定性和干扰,对已有的非线性直接自适应控制律进行改进,设计PI(Propor-tional-Integral)型参数自适应律,以提高姿态控制精度,同时给出了稳定性证明.针对1阶系统设计PI控制器及PPF(Positive Position Feedback)控制器,以有效抑制挠性结构振动.仿真结果表明,在采用摄动法对动力学方程分析的基础上设计姿态控制系统,可以有效完成挠性航天器高精度姿态控制任务.     

带VSCMGs的航天器姿态稳定及功率补偿控制

基于变速控制力矩陀螺群动力学模型建立其复合控制方程和分系统解耦约束方程,用矩阵投影方法同步设计得到航天器姿态与能量一体控制复合操纵律,利用Lyapunov方法分析了转子轴向惯量误差对姿态控制分系统的影响.根据飞轮转子轴向惯量与功率输出之间的误差关系设计出功率控制补偿器.复合操纵律中的力矩和功率两解形式相同,约束方程使得姿态与能量控制两分系统解耦,便于进行考虑执行机构特性的闭环控制系统性能分析.考虑飞轮转子轴向惯量误差时,姿态控制分系统的输出耗散特性使其能够保持稳定,而功率控制分系统输出误差与转子轴向惯量误差成比例关系,经过补偿后功率输出能满足控制要求.     

采用变速控制力矩陀螺的航天器姿态跟踪研究

研究了以变速控制力矩陀螺(VSCMG)作为执行机构的航天器姿态跟踪问题.建立了以VSCMG为执行机构的航天器姿态动力学模型, 引入一阶稳定的线性角速度滤波方程, 同时, 根据Lyapunov稳定性定理, 设计了闭环系统的控制律. 利用加权的最小范数解得到VSCMG的姿态控制输入矢量. 提出了表征VSCMG构型的新奇异度量, 在其基础上利用梯度法构建了VSCMG的零运动, 以回避VSCMG的构型奇异, 并使转子转速趋于期望值. 以四陀螺金字塔构型为例进行仿真,仿真结果验证了该算法的可行性和有效性.      

柔性隔振结构影响下控制力矩陀螺的动力学建模与仿真#br#

近年来,控制力矩陀螺逐渐广泛应用于航天器姿态控制中.为了减小动量轮的高速旋转引起的振动对星体的影响,需要在控制力矩陀螺于航天器之间安装隔振装置.但是隔振装置的引入对控制力矩陀螺内部机构的动力学特性造成了影响.基于此,本文建立了柔性隔振机构耦合作用下的控制力矩陀螺动力学模型.本文通过欧拉角变换建立了陀螺内部各机构的运动学关系,使用能量方法建立了陀螺内部各结构的动力学特性.并在Matlab中进行了数值仿真与分析.通过仿真发现了隔振结构对陀螺的输出力矩产生了影响,在柔性支撑下的陀螺力矩存在明显波动,且波动范围随动量轮转速的增加而增加.同时,柔性隔振机构的引入还导致了干扰力矩的产生,该干扰力矩对控制力矩陀螺框架电机的控制存在较大影响.     

在轨发动机射流的电离层效应

卫星等航天器在轨运行期间,通过喷气实现姿态控制、轨道调整等特定需求.喷气射流与电离层相互作用,能够引起电离层环境改变,对星载设备产生重要影响.通过研究航天器在轨发动机喷气射流在电离层中的动力学及化学反应过程,建立射流的电离层效应物理模型,模拟了不同射流量及高度条件下喷气射流的运动过程、密度分布及电离层扰动效应.仿真结果表明,相同高度下,随着射流量增加,电离层扰动效应逐渐增强;相同射流量条件下,随着高度增加,电离层扰动效应逐渐减弱,扰动区域逐渐扩大.      

基于深度神经网络的航天器姿态控制系统故障诊断与容错控制研究

针对传统航天姿控系统故障诊断与容错控制诊断精度及控制分配效率较低的问题,提出了一种基于深度神经网络的航天器姿态控制系统故障诊断与容错控制方法。以控制力矩陀螺为执行机构的航天器发生执行机构故障工况时,所提出的方法可保证鲁棒的姿态控制。首先,利用三个异构深度神经网络实现传统容错控制器的故障诊断、姿态控制和力矩分配等功能,建立了全神经网络的智能自适应容错控制器架构。然后,对三个神经网络的网络层数、神经元数目和激活函数等参数进行优化调整,对比分析了神经网络参数对控制器性能的影响。最后,对所提出的新型控制器在控制力矩陀螺发生故障时的控制精度和鲁棒性进行了仿真验证。仿真结果表明,对于具有冗余控制力矩陀螺的航天器,提出的方法不仅能在单一陀螺故障下实现高精度的容错控制,也能在发生多陀螺故障时保证一定的姿态稳定控制。     

组合体航天器姿态的智能自适应控制方法

研究了交会对接后组合体航天器构型变化带来的姿态控制问题,对执行机构在控制量受限时的控制能力进行了分析,应用基于特征模型的智能自适应控制方法,设计了能适用于不同构型的姿态控制器,分别对组合体在直线构型和L构型对接情况下进行了数学仿真,仿真结果验证了智能自适应控制方法可行并且具有一定的优越性。     

控制力矩陀螺框架谐波减速驱动系统建模与仿真

摘要： 控制力矩陀螺是航天器姿态控制系统的重要执行机构,它具有输出力矩大、速度响应快、功率消耗低、寿命长等优点,可以完成高速率的姿态机动控制.综合考虑谐波减速器的齿隙模型、非线性刚度、减速器效率等因素,对CMG框架驱动组件用谐波减速器进行精细建模.针对低速下谐波减速器的刚度较低、传动误差较大这一缺陷,建立考虑传动误差的减速器模型;与传统的不考虑传动误差的模型相比可更准确地描述谐波减速器在低速下的输出速度曲线.根据建立的CMG框架驱动系统模型,在低速下采用PID闭环控制对输出转速误差进行抑制,使输出转速误差降低了50%以上.最后分析其对谐波减速器刚度和阻尼对框架系统性能的影响.     

Scaling analysis and model estimation of solar corona index

A monthly average solar green coronal index time series for the period from January 1939 to December 2008 collected from NOAA (The National Oceanic and Atmospheric Administration) has been analysed in this paper in perspective of scaling analysis and modelling. Smoothed and de-noising have been done using suitable mother wavelet as a pre-requisite. The Finite Variance Scaling Method (FVSM), Higuchi method, rescaled range (R/S) and a generalized method have been applied to calculate the scaling exponents and fractal dimensions of the time series. Autocorrelation function (ACF) is used to find autoregressive (AR) process and Partial autocorrelation function (PACF) has been used to get the order of AR model. Finally a best fit model has been proposed using Yule-Walker Method with supporting results of goodness of fit and wavelet spectrum. The results reveal an anti-persistent, Short Range Dependent (SRD), self-similar property with signatures of non-causality, non-stationarity and nonlinearity in the data series. The model shows the best fit to the data under observation.     

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.     

Development of a gas chromatography compatible Sample Processing System (SPS) for the in-situ analysis of refractory organic matter in martian soil: preliminary results

In the frame of the 2009 Mars Science Laboratory (MSL) mission a new sample preparation system (SPS) compatible with gas chromatography–mass spectrometry (GC–MS) has been developed for the in situ analysis of complex organic molecules in the Martian soil. The goal is to detect, if they exist, some of the key compounds that play an important role in life on Earth including carboxylic acids, amino acids and nucleobases.     

Learning in an immersive digital theater

The Houston Museum of Natural Science, in collaboration with Rice University has an outreach program taking portable digital theaters to schools and community sites for over five years and has conducted research on student learning in this immersive environment. By using an external independent evaluator, the effectiveness of NASA-funded Education and Public Outreach (EPO) projects can be assessed. This paper documents interactive techniques and learning strategies in full-dome digital theaters. The presentation is divided into Evaluation Strategies and Results and Interactivity Strategies and Results. All learners from grades 3–12 showed statistically significant short-term increase in knowledge of basic Earth science concepts after a single 22-min show. Improvements were more significant on items that were taught using more than one modality of instruction: hearing, seeing, discussion, and immersion. Thus immersive theater can be an effective as well as engaging teaching method for Earth and Space science concepts, particularly those that are intrinsically three-dimensional and thus most effectively taught in an immersive environment. The portable system allows taking the educational experience to rural and tribal sites where the underserved students could not afford the time or expense to travel to museums.     

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.      

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.     

Return to Europa: Overview of the Jupiter Europa orbiter mission

Missions to explore Europa have been imagined ever since the Voyager mission first suggested that Europa was geologically very young. Subsequently, the Galileo spacecraft supplied fascinating new insights into this satellite of Jupiter. Now, an international team is proposing a return to the Jupiter system and Europa with the Europa Jupiter System Mission (EJSM). Currently, NASA and ESA are designing two orbiters that would explore the Jovian system and then each would settle into orbit around one of Jupiter’s icy satellites, Europa and Ganymede. In addition, the Japanese Aerospace eXploration Agency (JAXA) is considering a Jupiter magnetospheric orbiter and the Russian Space Agency is investigating a Europa lander.     

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.     

基于最小值原理的冗余度机器人动力学控制

为了解冗余度机器人全局法优化中数值求解的困难,本文讨论了动力学方程的建立,无约束和有约束最优控制问题之间的内在联系,重点分析了求解最优控制问题的数值方法,文中提出了双向异步积分迭代的求解正则方程组的直接迭代法,较好解决了状态方程和协态方程稳定相逆给求解两点这值问题带来的困难。     

基于GPS载波相位的微卫星姿态算法研究

GPS姿态系统是利用GPS载波相位测量来确定载体的航向和姿态角。本文对微卫星的GPS姿态系统进行了研究。重点解决短基线的GPS状态算法，讨论了姿态价格函数的了小化方法。测试结果表明，所提的算法对小于1m的基线是有效的。