一种基于虚拟页地址映射的NAND Flash管理算法

本文提出了一种基于虚拟页地址映射的NAND Flash管理算法.该算法通过定义坏块表、对应表等结构，以及设计的坏块替换策略和虚拟页地址到实际物理页地址的转换算法，实现上层软件采用虚拟地址对NAND Flash的无坏块连续页地址访问.该算法是一种高效的地址映射算法，能高效地对数据进行索引，占用SRAM空间较少，使系统达到高性能，并使得闪存使用的更加稳定持久.     

光纤通道在基于MIL-STD-1553的航空电子系统网络中的应用

光纤通道作为新一代的航空电子系统通信网络技术,具有传输速度高、延时低、传输距离远和可靠性高等特性,高达4G bps的数据传输带宽,为其上层通信协议提供了一种通用的高速率的数据传输通道。FC-1553作为光纤通道上层通信协议之一,对MIL-STD-1553通信协议具有完全的兼容性,它继承了传统MIL-STD-1553通信协议的基本特征,实现了向光纤通道链路层的映射,从而扩展了通信网络的结构,提高了网络的通信能力。本文首先介绍MIL-STD-1553和光纤通道的基本特性,然后描述在光纤通道中对1553通信协议的映射,最后,提出了基于光纤通道和MIL-STD-1553的航空电子系统通信网络结构。     

虚拟现实系统中三维视觉几何建模

三维视觉建模是建立虚拟现实系统的基础,文中主要研究了虚拟现实系统中对象形状的建造方法、纹理映射的数学建模,并对其常用算法进行了比较分析。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

基于总线式集成框架的本体构建及映射研究

通过本体的构建及相应的本体映射策略,可以很好地解决信息集成过程中出现的语义异构问题。是实现异构数据源语义解析的基础。在已有研究成果总线式信息集成框架的基础上,针对目前本体构建过程存在的不足,提出了基于共享词汇表的全局本体构建技术和基于UML的局部本体构建技术,使所构建的本体元素间关系更加准确完备,具有良好的一致性。提出了基于综合相似度的本体映射策略,大大提高了本体映射的精度。     

Nonlinear dynamic modeling of a helicopter planetary gear train for carrier plate crack fault diagnosis

Planetary gear train plays a significant role in a helicopter operation and its health is of great importance for the flight safety of the helicopter. This paper investigates the effects of a planet carrier plate crack on the dynamic characteristics of a planetary gear train, and thus finds an effec-tive method to diagnose crack fault. A dynamic model is developed to analyze the torsional vibra-tion of a planetary gear train with a cracked planet carrier plate. The model takes into consideration nonlinear factors such as the time-varying meshing stiffness, gear backlash and viscous damping. Investigation of the deformation of the cracked carrier plate under static stress is performed in order to simulate the dynamic effects of the planet carrier crack on the angular displacement of car-rier posts. Validation shows good accuracy of the developed dynamic model in predicting dynamic characteristics of a planetary gear train. Fault features extracted from predictions of the model reveal the correspondence between vibration characteristic and the conditions (length and position) of a planet carrier crack clearly.     

国内外行星表面巡视器自主导航技术研究

作为航天技术发展的前沿和趋势,深空探测是人类历史上最为复杂的系统工程之一.星球巡视器是在星球表面移动作业的无人探测系统,能够对星球表面进行大面积、近距离和接触式的考察,是地外星球着陆探测作业的主要手段.星球巡视器导航技术是研究星球巡视器的关键技术之一,其导航自主性能直接影响星球探测计划能否顺利进行.本文首先概述了星球巡...     

航天测控系统自主运行的关键技术

航天事业发展趋势和未来需求指明,航天测控系统应该向以自主运行能力为代表特征的智能化方向发展。基于此,提出了标准化的支持与服务、映射现实的体系架构、实时响应的运行模式、服务化的基础平台等4项关键技术。通过将测控系统和卫星系统之间的接口、测控系统和用户系统之间的接口标准化,从而在此基础上建立最优化的操作逻辑。通过在计算机中映射现实系统的思想方法,从而产生稳定性和灵活性兼备的、支持自主运行的,并具有良好进化性能的系统架构。通过实时响应的运行模式可以很好满足全时段和突发性等具有挑战性的测控服务需求。通过大数据和云计算技术构建基础计算服务平台实现基础层与业务层分离,有利于整个系统的持续改进,提高服务质量改善的速度,建立竞争力优势。由此说明,在当前技术条件下实现自主运行的航天测控系统是可行的。     

封闭式行星轮系功率流判别的键合图法

为更简单清晰地对封闭式行星轮系的功率流情况进行判别,利用键合图能量守恒和功率流动的特点,将键合图理论应用于该类轮系的功率流分析中.以功率汇流型、回流型2种形式的封闭式行星轮系为例,根据轮系的传动关系,利用绝对速度法建立轮系的键合图模型,根据提出的功率流向判别依据对轮系进行功率流向判别,得到整个轮系及其转换机构的功率流情况,为轮系的效率计算提供了基础.该方法适用于其它复杂轮系的功率流判别中,比传统方法更具直观性、系统性.     

一种用于运动目标捕获的行星轮差动式欠驱动臂

为解决运动目标捕获过程中的碰撞问题,采用欠驱动自适应原理研制了具有碰撞能量吸收能力的机械臂。三自由度的机械臂由2个电机驱动:基关节由单个电机驱动;中关节和末关节由一个单输入双输出行星轮组完成动力分配。在机械臂捕获运动目标过程中,碰撞产生的部分冲击能量通过欠驱动行星轮组传递到末关节,转化为关节动能。依靠欠驱动机械系统完成对碰撞的响应,解决了控制系统因时延而无法快速对碰撞进行响应的难题。为完成对目标的抓取,基于阻抗控制提出了机械臂运动目标捕获控制算法。运动目标捕获实验验证了机械臂对碰撞的快速响应能力及运动目标捕获控制算法的可行性。