一种基于数据融合的加速度传感器的静态模型辨识方法

通过对现有加速度传感器静态模型参数辨识方法进行分析,指出传统的算术平均值法在实现加速度传感器静态模型参数辨识中存在的缺陷,提出了数据融合方法,并对其进行了讨论。数据融合方法是将来自同一目标的多源数据加以智能化合成,从而产生比单一数据源更精确更完全的估计和判决。通过分析表明,采用数据融合方法进行参数辨识得到的参数的离散度小于传统的算术平均值法所求参数的离散度,使模型参数的精度有明显提高。因此数据融合方法优于传统的算术平均值法,特别适合于加速度传感器静态模型参数的辨识。该方法的提出为控制系统的实时补偿提供了良好的条件。     

ARINC629航空数据总线研究

从ARINC629总线系统的发送机制、消息格式和个性化表3个方面介绍了ARINC629总线系统.     

The Progress of the Taiwan Oscillation Network Project

We describe the present status of the project of the Taiwan Oscillation Network (TON) and discuss a scientific result using the TON data. The TON is a ground-based network to measure solar intensity oscillations for the study of the solar interior. Four telescopes have been installed in appropriate longitudes around the world. The TON telescopes take K-line full-disk solar images of diameter 1000 pixels at a rate of one image per minute. The data has been collected since October of 1993. The TON high-spatial-resolution data are specially suitable for the study of local properties of the Sun. In 1997 we developed a new method, acoustic imaging, to construct the acoustic signals inside the Sun with the acoustic signals measured at the solar surface. From the constructed signals, we can form intensity map and phase-shift map of an active region at various depths. The direct link between these maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximation. This technique of acoustic imaging has been used to image the far-side of the Sun that could provides information on space weather prediction. The TON Team includes: Antonio Jimenez (Instituto Astrofisica de Canarias, Spain); Guoxiang Ai and Honqi Zhang (Huairou Solar Observing Station, P.R.C.); Philip Goode and William Marquette (Big Bear Solar Observatory, U.S.A.); Shuhrat Ehgamberdiev and Oleg Ladenkov (Ulugh Beg Astronomical Institute, Uzbekistan) This revised version was published online in August 2006 with corrections to the Cover Date.     

基于手眼视觉的测量与定位方法的研究与实现

机器视觉对机器人克服工作环境中的不确定性具有重要意义。针对空间遥操作机器人面对的是危险不确定环境，文中提出一种基于手眼视觉的测量与定位方法，可为判断示知目标物体是否可抓持以及进行抓持规划提供有效依据。在重复定位的任务中，该方法可以利用目标物质的先验信息快速定位从而避免频繁移动手臂。文章首先给出了该方法的原理，然后通过实验实现了此方法，并对误差进行了分析，实验结果表明了该方法具有较高的精度。     

Tong检测算法性能分析及参数设置

Tong检测算法是常用的信号检测算法,但在其统计性能以及算法参数设置等方面仍缺少全面的结论.针对这些问题,运用统计和递推分析方法对信号搜索单元滞留次数的均值及方差进行了较为详细的理论分析,给出了相应表达式,根据3西格玛原则,提出了一种最大滞留次数限定方法.分析了检测概率、噪声搜索单元和信号搜索单元平均滞留次数与算法中计数器初值和最大值以及预检测信噪比之间的关系.分析结果表明Tong检测算法参数的设置需依据信号强弱和搜索方式,并折衷考虑对检测概率与噪声搜索单元或信号搜索单元平均滞留次数的影响.      

单框架控制力矩陀螺系统的运动奇异及回避

为满足航天器姿态三轴控制的要求,通常在姿态控制系统中采用3个或以上的单框架控制力矩陀螺(SGCMG).当多个SGCMG协调工作时,系统会出现奇异现象.在研究SGCMG系统的运动奇异机理及零运动的基础上,提出了一种判别奇异状态可回避性的新方法.该方法把对奇异状态可回避性的判别转化为对一组非线性常微分方程的定性研究.以某4-SGCMG系统为例,验证了上述方法的可行性.      

Probing Solar Subsurface Magnetic Fields

Helioseismology uses solar p-mode oscillations to probe the structure of the solar interior. The modifications of p-mode properties due to the presence of solar magnetic fields provide information on the magnetic fields in the solar interior. Here we review some of results in helioseismology on the magnetic fields in the solar convection zone. We will also discuss a recent result on the magnetic fields at the base of the convection zone. This revised version was published online in August 2006 with corrections to the Cover Date.     

Sensitivity analysis of dual-satellite geolocation

An analytic solution is presented for the linearized estimation problem arising from the dual-satellite geolocation of the source of a narrowband signal using time- and frequency-difference-of-arrival (TDOA and FDOA, respectively) observations and an altitude constraint. This solution is used to analyze the covariance matrix of the resultant source location estimate, along with the sensitivity of its mean to errors in the presumed source altitude and velocity, and the measured or predicted positions and velocities of the satellites. Following the practice of differential Global Positioning System, the technique of differential calibration is used to reduce or eliminate various sources of solution bias which would otherwise require tight, and consequently expensive, individual calibration     

Determination of epsomite-hexahydrite equilibria by the humidity-buffer technique at 0.1 MPa with implications for phase equilibria in the system MgSO4-H2O

Epsomite (MgSO(4).7H(2)O) and hexahydrite (MgSO(4).6H(2)O) are common minerals found in marine evaporite deposits, in saline lakes as precipitates, in weathering zones of coal and metallic deposits, in some soils and their efflorescences, and possibly on the surface of Europa as evaporite deposits. Thermodynamic properties of these two minerals reported in the literature are in poor agreement. In this study, epsomite-hexahydrite equilibria were determined along four humidity-buffer curves at 0.1 MPa and between 25 and 45 degrees C. Results obtained for the reaction epsomite = hexahydrite + H(2)O, as demonstrated by very tight reversals along each humidity buffer, can be represented by ln K(+/- 0.012) = 20.001 - 7182.07/T, where K is the equilibrium constant, and T is temperature in Kelvin. The derived standard Gibbs free energy of reaction is 10.13 +/- 0.07 kJ/mol, which is essentially the same value as that calculated from vapor pressure measurements reported in the literature. However, this value is at least 0.8 kJ/mol lower than those calculated from the data derived mostly from calorimetric measurements.     

考虑框架伺服特性时SGCMG系统操纵律设计

在单框架控制力矩陀螺(SGCMG)系统操纵律的设计中,通常假定框架伺服系统具有理想的伺服跟踪性能.然而,框架伺服系统有限的带宽和实际存在的各种扰动力矩都会使其跟踪性能下降.为抑制SGCMG框架伺服特性对操纵性能的影响,设计了一种新型操纵律.该操纵律综合考虑了SGCMG系统运动学和动力学特性,可以根据航天器姿态控制给出的角动量(或力矩)指令,直接计算出每个SGCMG框架驱动系统所需的控制力矩.由于操纵律没有算法奇异,在SGCMG系统不出现运动奇异的情况下,可使操纵误差指数收敛至零.同时,操纵律形式简单,易于实现.应用在航天器上的某4-SGCMG系统的仿真结果表明,上述操纵律是可行的.