基于神经网络的仿真输出数据的分布识别

分布识别在仿真输出数据的分析中有着重要的理论和实际价值，但长期以来一直没有很好解决，在研究和改进神经网络的基础上，提出用多层感知机ＢＰ网格进行分布识别，给出了基于ＮＮ的分布识别模型，并进行了实验检验，实验结果表明本方法识别效率高，并具有很高的可靠性，可以辅助分析者作出准确的判断。     

Intrinsic parameters of massive OB stars

We present the results of our observations of stars of type O5 and earlier and show that inclusion of the line blocking between 228 and 912 A solves the problem found by Herrero et al. (1992) in the determination of their stellar parameters. We study the influence of the line blocking and other effects on the mass and helium discrepancies and show that the first one is reduced by the use of spherical, non hydrostatic model atmospheres and that the second one is probably due to exposure of CNO material.The INT is operated on the island of La Palma by the RGO in the Spanish Observatorio de El Roque de los Muchachos of the Instituto de Astrofsica de Canarias     

典型隐身飞机的RCS起伏统计特性

雷达散射截面(RCS)起伏统计特性可以用来预测雷达的检测性能和评估飞机的散射特性。采用高频计算方法获取了6种典型隐身飞机在光学区8个频率点、两种极化方式、不同入射条件下的周向RCS统计数据。应用3种较新的起伏模型对统计数据进行拟合,通过对比分析各组数据的拟合效果,得出了各模型在数据拟合时存在的普遍规律:卡方(Chi-square)模型对概率密度分布曲线的峰值估计较为合理,对数正态模型容易将峰值高估,但在峰值之后卡方模型的拟合效果通常不如对数正态模型;统计数据均值的平方与方差之比越大(可达0.1~1.0),则卡方模型双自由度越大(可达1.1~1.5),拟合效果也越好,按Kolmogorov-Smirnov检验方法其误差在0.15~0.25范围内;统计数据的均值中值比越小(低至1.5~5.0),则对数正态模型拟合效果越好,误差在0.01~0.25范围内;在dB·m2单位制下,采用对数正态模型和勒让德多项式模型可以在更广的范围内更好地拟合各组数据,其拟合误差多在0.10以下。     

天/地基多平台空间目标光电观测时效性分析

针对如何部署光学探测设备才能更好实现对空间目标的高精度高频度监视问题,考虑光照条件、相对关系及探测性能,构建了天/地基空间目标探测与成像仿真模型;按照轨道特征选取了94颗LEO（Low Earth Orbit,低地球轨道）卫星、63颗GEO（Geosynchronous Earth Orbit,地球同步轨道）卫星和18颗大椭圆轨道卫星,选用春夏秋冬典型季节的特定时间长度,仿真分析了国内地基、南北极科考站、LEO卫星、准GEO卫星等多平台光电手段的位置探测和成像观测能力;比对分析地基平台纬度和季节、天基平台轨道高度和倾角对探测能力的影响得出：南北极科考站相比于国内站点可提高重点季节的探测时效性,98°倾角LEO平台对低轨目标成像时效性方面更具优势,等.在此基础上,提出了我国空间目标光电观测设备天地一体的布局构想.     

基于整数规划的终端区空域扇区划分研究

扇区划分是终端区空域规划的研究内容之一,划分后能覆盖不均匀的交通分布,缓解需求与容量的不平衡,从而提高空域系统的运行效率。将终端区扇区划分作为一个整数规划问题,在约束条件中考虑了间隔规则、飞行路径需求和机场跑道结构的几何约束等,根据最优解来生成终端区扇区。以某终端区算例,验证了整数规划模型的可行性。     

Performance evaluation of some rain rate conversion models for microwave propagation studies

An important characteristic of rainfall levels at a particular place is the statistical distribution of rainfall rate. In this paper, 5-min integration time rainfall data for the Northcentral region of Nigeria was obtained from the Tropospheric Data Acquisition Network (TRODAN), Anyigba, Nigeria. Also, 1-min integration time rainfall was measured at Minna, Nigeria. In order to obtain the optimal rain rate model suitable for this region, two globally recognised rain rate models were critically evaluated and compared with the 1-min measurements. These are the ITU-R P.837-7 and Lavergnat-Gole (L-G) models. The results obtained showed that the ITU-R P.837-7 and L-G models respectively underestimated the measured rain rate by 7.3 mm/h and 9 mm/h at time percentage exceedance of 0.1%, while they underestimated the measured rain rate by 23.4 mm/h and 13 mm/h respectively at 0.01%. At 0.001%, the measured rain rate was overestimated by the ITU-R P.837-7 and L-G models by 27.4 mm/h and 3 mm/h respectively. Further performance evaluation of the predefined models was carried out using different error metrics such as sum of absolute error (SAE), mean absolute error (MAE), root mean square error (RMSE), standard deviation (STDEV) and Spearman’s rank correlation. The results obtained adjudged the Lavergnat-Gole model as the best rain rate prediction model for this region.     

波音737NG飞机引气系统健康检查定制与专用设备的应用

介绍了波音737NG飞机引气系统健康检查项目的目标,采用波音C36001-44设备进行此项检查的具体实施方案,并介绍了国航自行研制的专用设备波音737NG引气系统健康诊断仪,及其与C36001-44在健康检查中的实际效果对比。3国航股份工程技术分公司贵阳维修基地4国航股份工程技术分公司重庆维修基地     

壁湍流等动量区对惯性颗粒分布的影响

对摩擦雷诺数为1000、颗粒Stokes数为1.0的含颗粒槽道湍流进行了直接数值模拟,采用高斯函数叠加法提取了等动量区的模态速度,对各等动量区内的颗粒分布进行了分析。发现在高动量的核心区,颗粒平均浓度高于非核心区,而浓度脉动低于非核心区。在等动量区界面上,流体速度和颗粒浓度变化剧烈,展向涡结构的出现导致了局部颗粒浓度较低。在等动量区的界面以下,在较高的壁面法向位置,存在大尺度的浓度幅值低而浓度脉动高的结构,其等值线分布与核心区/非核心区界面一致。     

Characteristics of solar particle events at Mars relative to Earth

While not specifically designed to detect solar energetic particle radiation, the Electron Reflectometer onboard Mars Global Surveyor (MGS/ER) collected such data from January 1999 through October 2006. Energetic protons (?25 MeV) and other ions penetrated the MGS/ER shielding and registered counts within the instrument’s electronics. During solar particle events (SPE’s), prolonged enhancements in the particle background were observed at Mars with time intensity profiles similar to Earth based SPE observations. Throughout the lifespan of MGS/ER, 85 distinct SPE’s were observed. Basic characteristics of Mars based SPE observations and the frequency of SPE occurrences at Mars are compared to corresponding Earth based observations. Approximately 22% of SPE’s that occurred during MGS/ER operation were observed at Earth but not Mars. Similarly, 19% of SPE’s were observed at Mars but not Earth. Time intensity profiles at Earth and Mars match predictions provided in the literature, based on the physical location of the detector with respect to the motion of the interplanetary shock wave. Note: The work described herein was largely conducted as part of a doctoral dissertation produced by the author.     

飞机轮胎溅水鸡尾流特性数值模拟

当飞机起落架的多轮经过涉水跑道时，除侧向溅水之外，在轮胎之间由于两股侧向水流汇聚，会形成类似公鸡尾的溅水形态，称之为鸡尾流。相比于轮胎的侧向溅水，鸡尾流成因复杂，且水量更大，溅水高度更高，可能对飞机安全造成更严重的危害。采用数值分析方法对飞机轮胎溅水产生的鸡尾流现象成型机理开展研究。根据轮胎几何结构特点建立飞机轮胎溅水模型，其中轮胎及跑道采用FEM方法建模，积水模型采用SPH法，给出了鸡尾流的形态和速度分布，通过与侧向溅水形态分布的分析与比较，揭示了鸡尾流溅水的形成机制，并研究了水深、轮胎间距、轮胎速度等因素对于鸡尾流形态以及速度分布的影响规律，初步验证了ESDU工程算法对于无翻边轮胎鸡尾流形态描述的可参考性。