用于导弹系统性能统计分析的统计线性化伴随法

本文在研究ＳＬＡＭ方法基础上，进行了理论推导和计算方法方面的改进，并将此方法应用于导弹系统性能的统计分析，计算机仿真结果表明该方法与采用ＣＡＤＥＴ方法的结果完全一致。     

大型太阳帆板展开状态动态特性研究

利用有限元技术及自编的 FORTRAN程序计算了单翼太阳帆板约束模态的振型和频率 ,计算结果和实验结果比较表明 ,计算精度在工程上是可以接受的。在此基础上 ,以飞船带有双翼对称太阳帆板为模型 ,计算了太阳帆板在转动和不转动情况下非约束模态的振型和频率。上述计算结果为研究带有挠性太阳帆板的航天器的动力学与控制问题打下了基础     

5GAT 靶机 RCS 特性仿真计算与分析

为对5GAT 靶机的RCS特性进行分析,采用外形逆向建模和RCS仿真计算的方法,对UHF~X波段该靶机单站和双站RCS进行了仿真计算。仿真结果表明:通过采用综合外形隐身设计手段,该靶机在高频的C和 X波段处于较低的散射水平,头向和侧向和RCS均值随频率升高呈迅速递减的趋势。通过几何特性相似的设计手段,该型靶机能在一定程度上模拟五代机的RCS 特性。     

Vertical and radial metallicity gradients in high latitude galactic fields with SDSS

We used the ugr magnitudes of 1437467 F-G type main-sequence stars with metal abundance $-2?[\mathrm{Fe}/\mathrm{H}]?+0.2$ dex and estimated radial and vertical metallicity gradients for high Galactic-latitude fields, $50°<b?90°$ and $0°<l?360°$, of the Milky Way Galaxy. The radial metallicity gradient $d[\mathrm{Fe}/\mathrm{H}]/\mathit{dR}=-0.042\pm 0.011$ dex kpc^?1 estimated for the stars with $1.31<z\le 1.74$ kpc is attributed to the thin-disc population. While, the radial gradients evaluated for stars at higher vertical distances are close to zero indicating that the thick disc and halo have not undergone a radial collapse phase at least at high Galactic latitudes. The vertical metallicity gradients estimated for stars with three different Galactic latitudes, $50°<b?65°,65°<b?80°$ and $80°<b?90°$ do not show a strong indication for Galactic latitude dependence of our gradients. The thin disc, $0.5<z?2$ kpc, with a vertical metallicity gradient $d\left[\mathrm{Fe}/\mathrm{H}\right]/\mathit{dz}=-0.308\pm 0.018$ dex kpc^?1, is dominant only in galactocentric distance interval $6<R?10$ kpc, while the thick disc ($2<z?5$ kpc) could be observed in the intervals $6<R?10$ and $10<R?15$ kpc with compatible vertical metallicity gradients, i.e. $d\left[\mathrm{Fe}/\mathrm{H}\right]/\mathit{dz}=-0.164\pm 0.014$ dex kpc^?1 and $d\left[\mathrm{Fe}/\mathrm{H}\right]/\mathit{dz}=-0.172\pm 0.016$ dex kpc^?1. Five vertical metallicity gradients are estimated for the halo ($z>5$ kpc) in three galactocentric distance intervals, $6<R?10,10<R?15$ and $15<R?20$ kpc. The first one corresponding to the interval $6<R?10$ kpc is equal to $d\left[\mathrm{Fe}/\mathrm{H}\right]/\mathit{dz}=-0.023\pm 0.006$ dex kpc^?1, while the others at larger galactocentric distances are close to zero. We derived synthetic vertical metallicity gradients for 2,230,167 stars and compared them with the observed ones. There is a good agreement between the two sets of vertical metallicity gradients for the thin disc, while they are different for the thick disc. For the halo, the conspicuous difference corresponds to the galactocentric distance interval $6<R?10$ kpc, while they are compatible at higher galactocentric distance intervals.     

隐身飞行器电磁散射特性分析

为对隐身飞行器的探测手段进行研究和指导隐身飞行器的研制,研究其电磁散射特性。采用外形逆向建模、理论预估和散射测量、强散射源减缩相结合的手段,对隐身飞行器的隐身性能进行预估。该方法具有精度高、速度快的优点,适合在隐身飞行器研制方案设计阶段使用。     

基于序优化理论的同步轨道入轨优化

基于序优化理论的多目标遗传(GA)算法,对小推力同步轨道卫星入轨控制方案设计与优化进行了研究.针对直接法中优化参数搜索范围大的缺点,提出了一种基于序优化理论的参数选定算法.给出了远地点变轨轨道控制优化方案,并利用序优化理论确定优化参数初始区间与约束关系.仿真结果表明:采用序优化算法可明显加快收敛速度,提高计算效率.对相同的GA参数设置,用序优化算法有可能得到比原来性能更好的子代,获得更理想的目标函数值.     

低轨卫星多普勒频移特性的快速计算

地面站利用低轨卫星进行通信时,地面接收站接收信号存在明显的多普勒频移现象。为描述多普勒频移特性,首先分析卫星轨道偏心率对多普勒特性曲线的影响,分析表明：轨道偏心率越大,地面站接收信号多普勒变化率越大。其次,推导了卫星多普勒频移的计算表达式,并讨论了低轨卫星多普勒频移特性曲线的快速计算。仿真计算结果表明,该算法可以很好地描述任意低轨道卫星多普勒频移特性,并明显缩短了精确算法的计算时间,对于10 000km轨道高度卫星,算法置信度可达99%以上。     

Rainfall retrieval over Indian land and oceanic regions from SSM/I microwave data

Present study focuses on the estimation of rainfall over Indian land and oceanic regions from the Special Sensor Microwave/Imager (SSM/I) on the Defense Meteorological Satellite Program (DMSP) F-13. Based on the measurements at 19.35, 22.235 and 85.5 GHz channels of SSM/I Satellite, scattering index (SI) has been developed for the Indian land and oceanic regions separately. These scattering indices were co-located against rainfall from Precipitation Radar (PR) onboard Tropical Rainfall Measuring Mission (TRMM) to develop a new regional relationship between the SI and the rain rate for the Indian land and oceanic regions. A non-linear fit between the rain rate and the SI is established for rain measurement. In order to have confidence in our method, we have also estimated rainfall using the global rainfall and scattering index relationship developed by Ferraro and Marks [Ferraro, R.R., Marks, G.F. The development of SSM/I rain rate retrieval algorithms using ground based radar measurements. J. Atmos. Ocean. Technol. 12, 755–770, 1995]. The validation with the rain-gauge shows that the present scheme is able to retrieve rainfall with better accuracy than that of Ferraro and Marks (1995). Further intercomparison with TRMM-2A12 and validation with rain-gauges rainfall showed that the present algorithm is able to retrieve the rainfall with reasonably good accuracy.     

基于PWM的挠性航天器分力合成主动振动抑制方法

分力合成主动振动抑制方法可以有效抑制挠性振动. 其利用几个相同或相似的随时间变化的分力, 按一定的规律沿时间轴排列合成为合力作为系统输入, 此合力可以在保证完成规定刚体运动的同时抑制掉指定的任意阶振动谐波. 对于使用常幅值力矩喷气执行机构的航天器, 应用脉宽调制(PWM)技术将符合分力合成方法的时间最优机动控制指令变化为常幅值力矩形式, 设计出常幅值的时间最优大角度机动策略. 数值仿真结果证实了方法的有效性.      

基于人工势场法的移动机器人最优路径规划

提出一种解决人工势场法目标不可达问题的方法.分析了传统人工势场法中的固有缺陷:目标不可达;在障碍物附近或通过狭小通道时的抖动问题.通过选取适当的增益系数解决了目标不可达问题,使机器人快速到达目标点.用拉紧法去除路径的冗余节点并用极坐标下对称多项式优化出圆滑的最优路径.仿真结果证实了所提方法的正确性和有效性.