一种有效的消波装置

对无限长渠道中小振幅入射波通过两块间距为ｌ,透水性能不同的多孔透水板的反射和透射进行了研究。应用分离变量法得到了反射波和透射波的波形。结果表明,当ｌ为入射波半波长的倍数时,反射波和透射波振幅最大,消波效果差,最佳消波率为５０％。当ｌ为入射波１／４波长加半波长的倍数时,反射波和透射波振幅最小,消波效果好,最佳消波率大于５０％。此外,还得到了无反射波的条件。     

CDAS 自动化监控管理系统

指令与数据获取站监控管理系统吸取了国内外先进的集散控制系统的优点,综合运用了现代计算机管理先进技术。文章介绍了该监控管理系统的方案、系统功能模块、系统结构和应用软件的设计,实现了系统管理的高效自动化,确保系统运行的可靠、安全。     

Ada动态测试中遗传算法的参数编码方法

介绍了将遗传算法应用在Ada程序结构测试中,被测单元参数按照遗传算法的运算规则进行编码的原则与方法.首先,介绍了包括枚举类型和变长数组的基本数据类型的参数编码方法.由于Ada语言允许使用动态数据结构类型的参数,如何在一个较高自动化的动态测试工具中实现对动态数据结构的自动测试,成为首要关注的问题.因此文中着重介绍了Ada程序的动态数据结构在遗传算法中的编码方法.     

基于控制力矩陀螺的水下运载器动力学与仿真

为弥补水下运载器(AUV,Autonomous Underwater Vehicle)中传统舵面控制机构的低速控制的不足,改善其操纵性能,引入单框架控制力矩陀螺(SGCMG,Single Gimbal Control Moment Gyro)作为控制机构进行姿态稳定与控制.把AUV简化为刚体,加入SGCMG,考虑水下环境的特点,建立基于SGCMG的AUV动力学模型,并仿真分析AUV的动力学、姿态运动、SGCMG的框架运动以及环境之间的相互作用.仿真结果说明:基于SGCMG控制的AUV的姿态机动快速、准确,低速性能理想,为操纵律设计及姿态控制算法研究提供基础.     

Influence of lunar topography on simulated surface temperature

The surface temperature of the Moon is one of the essential parameters for the lunar exploration, especially to evaluate the Moon thermophysical features. The distribution of the temperature is heavily influenced by the Moon topography, which, however, is rarely studied in the state-of-art surface temperature models. Therefore, this paper takes the Moon topography into account to improve the surface temperature model, Racca model. The main parameters, such as slopes along the longitude and latitude directions, are estimated with the topography data from Chang’E-1 satellite and the Horn algorithm. Then the effective solar illumination model is then constructed with the slopes and the relative position to the subsolar point. Finally, the temperature distribution over the Moon surface is obtained with the effective illumination model and the improved Racca model. The results indicate that the distribution of the temperature is very sensitive to the fluctuation of the Moon surface. The change of the surface temperature is up to 150 K in some places compared to the result without considering the topography. In addition, the variation of the surface temperature increases with the distance from the subsolar point and the elevation, along both latitude and longitude directions. Furthermore, the simulated surface temperature coincides well with the brightness temperature in 37 GHz observed by the microwave sounder onboard Chang’E-2 satellite. The corresponded emissivity map not only eliminates the influence of the topography, but also hints the inherent properties of the lunar regolith just below the surface. Last but not the least, the distribution of the permanently shadowed regions (PSRs) in the lunar pole area is also evaluated with the simulated surface temperature result.     

Flow Stability Model for Fan/Compressors with Annular Duct and Novel Casing Treatment

A three-dimensional compressible flow stability model is presented in this paper, which focuses on stall inception of multi-stage axial flow compressors with a finite large radius annular duct configuration for the first time. It is shown that under some assumptions, the stability equation can be obtained yielding from a group of homogeneous equations. The stability can be judged by the non-dimensional imaginary part of the resultant complex frequency eigenvalue. Further more, based on the analysis of the unsteady phenomenon caused by casing treatment, the function of casing treatment has been modeled by a wall impedance condition which is included in the stability model through the eigenvalues and the corresponding eigenfunctions of the system. Finally, some experimental investigation and two numerical evaluation cases are conducted to validate this model and emphasis is placed on numerically studying the sensitivity of the setup of different boundary conditions on the stall inception of axial flow fan/compressors. A novel casing treatment which consists of a backchamber and a perforated plate is suggested, and it is noted that the open area ratio of the casing treatment is less than 10%, and is far smaller than conventional casing treatment with open area ratio of over 50%, which could result in stall margin improvement without obvious efficiency loss of fan/compressors.     

神经网络在高空长航时无人机翼型多点优化中的应用

NSGAII算法在翼型多点设计中有着广泛的应用价值,然而其巨大的计算资源和计算成本限制了它的使用。为了解决这个问题,本文引入具有较强非线性映射能力的神经网络代理模型,采用实验设计结合BP法训练神经网络响应面来代替N-S方程求解翼型的性能。在实验点的数值模拟中,为了进一步节省计算资源,提高计算效率,采用网格的变形代替网格的重新划分,使得计算网格的更新速度提高了约50%。在翼型的参数化过程中,采用改进的PARSEC方法,用较少的参数实现了翼型的精确控制。为了增强神经网络的泛化能力,采用12-7-4-3-1的隐层结构。对NLF1015翼型的多点优化算例表明,此方法不仅显著降低了整个优化过程的计算量,而且对翼型的气动性能预测也具有较高的可信度,在高空长航时无人机的翼型设计中具有一定的潜力。     

4种DGPS模块动态定位精度测试与分析

采用RTK-DGPS为参照,对GARMIN GPS15L、Ublox LEA-4S、Gstar GS-87和Gstar GS-89m-J共4种DGPS模块在单机模式、地面伪距差分模式和卫星差分模式下的动态定位精度进行了测试和分析.结果表明:(1)对于GARMIN GPS15L 和Ublox LEA-4S,单机定位精度为米级,使用地面伪距差分定位可分别提高动态定位精度20%和87%;(2)总体上看,DGPS模块的地面伪距差分定位精度优于卫星差分定位,卫星差分定位精度优于单机定位;(3)在视野狭窄地段,无论单机定位、伪距差分定位还是卫星差分定位,动态定位精度都受到一定影响,和视野开阔地段相比,精度明显下降.     

Global Hybrid Simulation of Magnetic Reconnection in the Magnetosheath

A three-dimensional (3-D) global hybrid simulation is carried out for the generation and structure of magnetic reconnection in the magnetosheath due to interaction of an interplanetary Tangential Discontinuity (TD) with the bow shock and magnetosphere. Runs are performed for solar wind TDs possessing different initial half-widths. As the TD propagates through the bow shock toward the magnetopause, it is greatly narrowed by a two-step compression processes, a "shock compression' followed by a subsequent ``convective compression'. In cases with a relatively thin solar wind TD, 3-D patchy reconnection is initiated in the transmitted TD, forming magnetosheath flux ropes. Multiple components of ion particles are present in the velocity distribution in the magnetosheath merging, accompanied by ion heating. For cases with a relatively wide initial TD, a dominant single X-line appears in the subsolar magnetosheath after the transmitted TD is narrowed. A shock analysis is performed for the detailed structure of magnetic reconnection in the magnetosheath. Rotational Discontinuity (RD)/Time-Dependent Intermediate Shock (TDIS) are found to dominate the reconnection layer, which and some weak slow shocks are responsible for the ion heating and acceleration.      

一种稀疏阵列下的二维DOA估计方法

研究了稀疏阵列下二维波达方向（DOA）的估计问题,提出一种基于不动点迭代的空间谱估计（FPC-MUSIC）算法。首先建立基于矩阵填充的DOA估计信号模型,并验证该信号模型满足零空间性质（NSP）,其次通过不动点迭代算法将稀疏阵列信号恢复为完整信号,最后利用恢复信号估计二维DOA。该算法可在稀疏阵列下大幅度降低谱估计平均副瓣,在大幅度降低阵元数的同时具有较高的估计精度。计算机仿真表明：FPC-MUSIC算法可在稀疏阵列下准确估计二维DOA,验证了该算法的有效性和优越性。