一种基于切比雪夫插值的联想记忆系统

提出了一种基于切比雪夫插值的高阶联想记忆系统(TI-AMS),能提供对任意阶多变量多项式函数的无误差逼近.切比雪夫插值的近似于最优一致逼近的性质从理论上保证了对任意连续函数的全局逼近精度.特别在对一些不连续函数(如矩形脉冲函数)的逼近中也有其它AMS无法比拟的优势.理论分析和数值模拟表明,该系统具有计算简单、学习精度高、收敛速度快、总的存储单元空间较小等优点.可广泛应用于图像压缩、模式识别、及高精度实时智能控制等领域.      

Effect of non-uniform basic temperature gradient on the onset of Marangoni convection in a fluid with suspended particles

The effect of a non-uniform basic temperature gradient on the onset of convection driven by surface tension in a horizontal layer of a Boussinesq fluid with suspended particles confined between an upper free, constant heat flux boundary and a lower rigid isothermal boundary is considered. The microrotation is assumed to vanish at the boundaries. A linear stability analysis is performed. The Rayleigh–Ritz technique is used to obtain the eigenvalues. The influence of various parameters on the onset of convection has been analyzed. Six different non-uniform basic state temperature profiles are considered and their comparative influence on onset is discussed. It is observed that the fluid layer with suspended particles heated from below is more stable compared to the classical fluid layer without suspended particles. The problem has possible applications in microgravity situations.     

一种改进的FMCW SAR RD成像算法

FMCWSAR将调频连续波与合成孔径成像技术结合于一体,是一种新近被提出来的成像雷达体制,它以其体积小、重量轻、成本低、分辨率高等一系列优点,引起越来越多的关注。然而,在FMCWSAR系统中,雷达连续不断地发射信号,调制信号周期相对较长,停一走（STOP AND GO）近似不再成立,所以要用合适的算法来实现成像。针对FMCW SAR的特点,详细推导了停一走近似失效时FMCW SAR的信号模型及处理过程,提出了一种改进的RD算法。此方法是通过补偿连续运动引入的多普勒频移,消除连续运动的影响。     

L-可积函数的逼近定理

通常所说的函数逼近,或者是在C—范数拓扑下连续函数的多项式逼近,或者是在L~p—范数拓扑下L~p函数的多项式逼近,或者是在Sobolev范数(‖·‖_(H~(m,p)(Ω)))拓扑下用C~∞(Ω)(或C~∞(Ω))对于Sobolev空间H~(m,p(Ω))的逼近。而对于有界L—可积函数的多项式a·e(即几乎处处)逼近,至今未见有任何文献。本文则借助于实变函数的性质与连续函数多项式逼近的技巧来处理这一工作,而文中的主要结果(即定理1—3)正反映了这一尚未有过的工作。确切地说,本文首先利用L—可测函数的重要定理,把L—可测函数转化为连续函数,使(用多项式)a·e逼近成为可能;而后,再对连续函数将广义Jackson算子逼近的已知结果与相应技巧应用上去,得到一系列刻划逼近程度(即逼近阶)的渐近估计。     

电磁式跟踪器磁场畸变的姿态校正技术

电磁式跟踪器可以测量物体的位置和姿态,但其测量精度也容易受金属环境干扰。本文根据电磁跟踪器的工作原理,给出了电磁式跟踪器姿态校正的模型,讨论了两种不同的姿态校正实现方法:插值法和拟合法,比较了两种方法的优缺点。最后,对某一金属环境进行了畸变姿态校正的试验,给出了3个不同的姿态实际值和在此金属环境下的畸变和校正结果。试验结果表明本文提出的姿态校正算法能很好地补偿金属环境引起的电磁式跟踪器姿态的畸变。     

多项式系统几何性质的注记

证明：在研究多项式系统的几何性质时，多项式系统应当定义成射影空间中奇点集之余维数至少为2的线场。在这个定义中，多项式系统的次数与通常的次数，在概念上不同相同，通常的n 1次退化系统属于这里的n次系统。值得注意的是，本给出的定义与坐标系的选取无关，在这种定义下，多项式系统的某些几何性质变得非常明显。     

GPS接收机中码相位测量精化方法的研究

精确的码相位测量是保证GPS接收机得到精确伪距值进而进行精确定位的一个重要前提。在已有码相位测量精化方法的基础之上提出了两种新的码相位测量精化的方法,讲述了两种方法的原理与具体实现方法,并利用蒙特卡洛方法进行了仿真实验,得到了码相位结果均值、码相位结果均值方差等一系列实验结果,对几种方法的精化效果从精确性、稳定性和跟踪性能等几个方面进行了比较分析,得出了相应的结论。与三角匹配法和二次曲线插值精化法相比,二阶最小二乘拟合精化法和广义延拓逼近精化法有明显优势;广义延拓逼近精化法的精化精度最高、跟踪精度最高,而二阶最小二乘拟合精化法的稳定性最好。     

地形匹配系统中各项误差的等效噪声分析

本文提出了把航迹、航速和航向误差等效为附加的测量噪声的方法。用两种统计参数估计方法估计了等效测量噪声的均值和标准差。求出了这些数字特征与地形的起伏标准差、粗糙度以及航速、航向误差之间的定量变化关系,为工程设计提供参考和依据。     

热防护系统的硅纤维隔热层复合传热数值计算

鉴于热防护系统的硅纤维隔热层是各向异性的非灰体材料，其复合传热计算是复杂且耗时的，提出了一种简便方法用于硅纤维这类各向异性非灰体材料的复合传热计算。该方法借鉴了医学领域断层摄影法（局部X射线检测法）中对光沿各向异性散射介质传播分析的思路，得到了各向异性扩散的热辐射方程（RTE—D）并把该方程用于求解非灰体半透明介质的辐射热通量。计算结果与文献中基于辐射传递方程（RTE）求得辐射热流的复合传热数值结果相比较，其最大相对误差为1．5％，并且其计算时间也由Pentium Ⅱ的3297．66分钟缩短为PentiumⅣ的约5分钟。最后，该方法被用于真实热环境下刚性隔热瓦L1900（高空隙率硅纤维隔热材料）的复合传热计算，计算结果与实验数据有较高吻合度。数据结果表明，各向异性的扩散近似被用于求解非灰体半透明介质的辐射热通量的方法用在热防护系统的硅纤维隔热层复合传热数值计算中是简便高效的。     

On the validity of the aluminum equivalent approximation in space radiation shielding applications

The origin of the aluminum equivalent shield approximation in space radiation analysis can be traced back to its roots in the early years of the NASA space programs (Mercury, Gemini and Apollo) wherein the primary radiobiological concern was the intense sources of ionizing radiation causing short term effects which was thought to jeopardize the safety of the crew and hence the mission. Herein, it is shown that the aluminum equivalent shield approximation, although reasonably well suited for that time period and to the application for which it was developed, is of questionable usefulness to the radiobiological concerns of routine space operations of the 21st century which will include long stays onboard the International Space Station (ISS) and perhaps the moon. This is especially true for a risk based protection system, as appears imminent for deep space exploration where the long-term effects of Galactic Cosmic Ray (GCR) exposure is of primary concern. The present analysis demonstrates that sufficiently large errors in the interior particle environment of a spacecraft result from the use of the aluminum equivalent approximation, and such approximations should be avoided in future astronaut risk estimates. In this study, the aluminum equivalent approximation is evaluated as a means for estimating the particle environment within a spacecraft structure induced by the GCR radiation field. For comparison, the two extremes of the GCR environment, the 1977 solar minimum and the 2001 solar maximum, are considered. These environments are coupled to the Langley Research Center (LaRC) deterministic ionized particle transport code High charge (Z) and Energy TRaNsport (HZETRN), which propagates the GCR spectra for elements with charges (Z) in the range 1 ? Z ? 28 (H–Ni) and secondary neutrons through selected target materials. The coupling of the GCR extremes to HZETRN allows for the examination of the induced environment within the interior of an idealized spacecraft as approximated by a spherical shell shield, and the effects of the aluminum equivalent approximation for a good polymeric shield material such as generic polyethylene (PE). The shield thickness is represented by a 25 g/cm² spherical shell. Although, one could imagine the progression to greater thickness, the current range will be sufficient to evaluate the qualitative usefulness of the aluminum equivalent approximation. Upon establishing the inaccuracies of the aluminum equivalent approximation through numerical simulations of the GCR radiation field attenuation for PE and aluminum equivalent PE spherical shells, we further present results for a limited set of commercially available, hydrogen rich, multifunctional polymeric constituents to assess the effect of the aluminum equivalent approximation on their radiation attenuation response as compared to the generic PE.