黎曼流形的Delaunay三角化和Voronoi图

主要研究黎曼空间中Delaunay三角化和Voronoi图.首先,分析和讨论了黎曼流形的Delaunay三角化和Voronoi图的存在性和生成算法.然后,在分析已有研究成果基础上,给出了黎曼流形Delaunay三角化和Voronoi图的一些性质和证明,并提出了采用黎曼流形描述问题的必要性和使用坐标卡研究黎曼流形的优势和意义.最后,以二维流形为例,介绍了将模型初始数据解释为黎曼流形的算法,包括建立坐标卡,定义流形函数等.在黎曼流形定义的基础上,详细描述了基于坐标卡生成模型的Delaunay三角化和Voronoi图的算法,并给出具体实例.     

磁流体力学的共面黎曼问题

MHD黎曼问题的求解对分析行星际扰动演化趋势和激波相互作用具有重要意义。本文基于MHD共面间断可以分解为前后向快慢激波、中心简单波和接触间断的假定,提出MHD共面黎曼问题的一种三参数迭代解法,运用该解法实现纯法向速度间断的分解,并初步探讨该解法的适用范围。      

空间成像光谱信息的处理与分析

信息处理和分析是空间成像光谱技木中涉及最终取得地物目标识别结果的两个重要步骤。按照信息处理流程,阐述了存档处理、数据压缩、检索处理、辐射与几何校正等关键技术;并在评述图像恢复与增强处理及多光谱数据信息分析方法的基础上,对成像光谱数据人工目视解译与计算机分析解译技术进行了研究与探讨。     

几何量检测专家系统设计

几何量检测专家系统是以机械制造中最常见的参数、最常用的测量方法为研究对象，综合计算机在几何量测试技术、测试误差理论与修正技术、测量数据处理技术等方面的应用于一体，在一定程度上替代专家，解决检测时可能遇到的各种问题并提供所需的服务。论述了几何量检测专家系统的主要功能、组成及测量过程模型。     

从ACCV‘95看计算机视觉技术的发展

介绍了第二届亚洲计算机视觉会议（ＳＥＣＯＮＤ ＡＳＩＡＮ ＣＯＮＦＥＲ－ＥＮＣＥ ＯＮ ＣＯＭＰＵＴＥＲ ＶＩＳＩＯＮ，ＡＣＣＶ’９５）的一些情况；回顾了在该领域及相关学科的研究成果，讨论了当前计算机视觉所面临的理论与实际应用问题，并对中国空间技术研究院这一学科的发展提出看法。     

CT导航混联医疗机器人灵活性研究

总结了目前医疗机器人灵活性的分析方法,基于服务球的数值法,对5R串联机器人和4H并联机器人进行了灵活度计算,得到了各自的任务灵活度.针对9-DOF冗余度串并混联医疗机器人运动学的复杂性以及难以获得逆解的解析解的状况,给出了串联部分、并联部分的位移流形,推导了混联机器人的位移流形.提出了混联机器人的灵活性分析方法,即基于位移流形(黎曼流形)的方法,并定义了混联机器人灵活度的通用解析表达式.基于黎曼曲面外接椭球面的面积计算,得到混联机器人的灵活度超过了CT导航手术所需的灵活度,满足手术要求,为微创外科混联机器人灵活性分析和度量提供了新的参考.      

无人直升机自主着舰的计算机视觉算法

通过理论分析和计算机半实物仿真研究了一种应用于无人直升机自主着舰的计算机视觉系统及相关计算机视觉技术.从工程实践的角度研究了计算机视觉技术在无人直升机自主着舰过程中的应用,并提出了可靠实用的一系列算法.通过精心设计,整套算法达到了无人直升机自主着舰的实时性和实用性要求,为工程样机的研制做好了理论上的准备.     

视觉导航下基于H2/H∞的航迹跟踪

为了从理论上研究视觉导航系统的特性,首先在物理上将视觉导航系统划分为传感器(摄像头、激光测距仪)和视觉处理计算机。针对视觉处理计算机,建立视觉位置测量模型。将视觉位置测量模型的不确定性分为参数不确定性和输入干扰2种。然后通过仿真详细分析了视觉位置估计针对不同模型不确定性的敏感程度。最后在引入视觉位置测量模型不确定性的基础上研究H₂/H_∞混合鲁棒控制在航迹跟踪上的应用,并给出了保证航迹控制系统稳定性和跟踪性能情况下的视觉位置测量模型摄动范围,对计算机视觉算法的研究具有一定的指导意义。     

关于磁层中磁力线几何结构的研究

磁层磁场的几何结构是空间物理中的重要研究内容.本文采用曲率半径分析方法,结合Cluster立体探测的相关知识和背景,利用Cluster立体探测的优势,通过对Cluster 2001年的立体探测数据的研究,分析了磁层各区域的磁力线结构,包括背阳面、Cusp区以及昏侧,得出各区域中磁力线的曲率半径大小,曲率矢量以及磁力线密切面的法线矢量的方向.利用这些参量直接确定出该区域中磁力线的空间几何构型,进而揭示了该区域磁场的三维立体结构.所得结果也验证了曲率半径分析方法的正确性.在科学探测数据完备的情况下,将这一研究方法应用到磁层中其他所有区域,可以得到整个磁层的详细三维结构模型,这具有重要的科学意义.      

基于类脑模型与深度神经网络的目标检测与跟踪技术研究

目标检测与跟踪技术广泛应用于交通、医疗、安保和航天等领域.目前，目标检测与跟踪技术面临目标微弱、背景复杂、目标被遮挡等挑战.同时，随着脑科学研究的不断深入，人们对人脑视觉系统的理解逐渐透彻，利用类脑计算解决复杂背景下高精度目标检测与跟踪问题成为相关领域的重要研究方向.本文结合神经工程导向的类脑模型和计算机工程导向的深度神经网络(Deep Neural Networks, DNNs)，提出多种基于类脑模型与深度神经网络的目标检测与跟踪算法，包括：基于演算侧抑制的目标检测算法，基于结构 对比度(Structure Contrast, SC)视觉注意模型的弱小目标检测算法和基于记忆机制与分层卷积特征的目标跟踪算法.实验结果表明，将类脑模型和深度神经网络应用于目标检测和跟踪领域，有利于实现复杂条件下的高精度目标检测和鲁棒性目标跟踪.     

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.     

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.     

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.     

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.     

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.