MIMO雷达中一种降维MUSIC的相干角度估计算法

研究单快拍下双基地多输入多输出（Multiple—InputMultiple-Output,MIMO）雷达中相干信源的离开角（Directionofdeparture,DOD）与到达角（directionofarrival,DOA）联合估计问题。利用单快拍下双基地MIMO雷达的接收信号构造一组Toeplitz矩阵,利用这组ToepIitz矩阵重构一个信号矩阵,提出一种基于降维多重信号分类（ReducedDimensionMultipleSignalClassification,RD-MUSIC）的DOD与DOA联合估计算法。提出的算法能够有效估计相干信源以及非相干信源的角度,实现角度的自动配对,并且角度估计性能远优于FBSS—ESPRIT算法以及ESPRIT-like算法。仿真结果验证了算法的有效性。     

Elemental Abundances in Coronal Structures

A great deal of evidence for elemental abundance variations among different structures in the solar corona has accumulated over the years. Many of the observations show changes in the relative abundances of high- and low-First Ionization Potential elements, but relatively few show the absolute elemental abundances. Recent observations from the SOHO satellite give absolute abundances in coronal streamers. Along the streamer edges, and at low heights in the streamer, they show roughly photospheric abundances for the low-FIP elements, and a factor of 3 depletion of high-FIP elements. In the streamer core at 1.5 R·, both high- and low-FIP elements are depleted by an additional factor of 3, which appears to result from gravitational settling. This revised version was published online in June 2006 with corrections to the Cover Date.     

一个方便实用的旋翼数据库

本文介绍了一个以EXCEL和EXCEL VB建立的旋翼数据库。并以一个分库为例介绍了建立和使用方法。     

模糊层次分析法在航空公司安全评估中的应用

在某航空公司安全评估指标体系的基础上,构建了其安全因素的模糊一致性判断矩阵,并通过权重分析获得各安全因素的影响程度;以人的因素为例进行综合评价,通过建立模糊隶属度矩阵从而得到了模糊综合评价矩阵,由此得出航空公司安全评估中人的风险值,方法为航空公司进一步加强管理提供了依据,因而具有一定的实用价值和经济效益。     

皖南机床数控龙门铣床用途与特点

黄山皖南机床生产的数控龙门铣床主要用于各种模具制造、各种基础大件、壳体件等多品种零件的加工,工件一次装夹后可自动高效、高精度地连续完成铣、镗、铰、攻丝等多种工序的加工.适用于汽车模具、重型机械、机车、造船、发电、机床、印刷、轻纺、航空航天等制造行业,配备多功能铣头后,可对工作进行五面体加工,以及对各种复杂型面进行三坐标加工.该机床主要有以下特点.     

先进复合材料在未来飞行器中的应用

复合材料在飞行器结构中的用量已经成为航空航天结构的先进性标志之一,其优越的综合性能非常适应未来飞行器的发展趋势.文章概述了先进复合材料在航空航天结构应用中的主要发展历程,结合未来飞行器的发展趋势,预测了先进复合材料在未来飞行器运用中可能带来的新挑战新机遇.     

A Cosmic-ray Composition Controlled by Volatility and a/q Ratio. snr Shock Acceleration of gas and Dust

The composition of Galactic Cosmic Ray Sources (GCRS) shows the following features: (i) an enhancement of the refractory elements relative to the volatile ones, and (ii) an enhancement of the heavier volatile elements relative to the lighter ones; this mass dependence should reflect a mass-to-charge (A/Q) dependence of the acceleration efficiency; among the refractory elements, there is only a very weak enhancement of heavier species, or none at all. We consider it fortuitous that the GCRS composition resembles that of the solar corona, which is biased according to first ionization potential. In a companion paper by Ellison et al. (1998, this issue), this GCRS composition is interpreted in terms of a supernova shock wave acceleration of interstellar and/or circumstellar (e.g., 22Ne-rich Wolf-Rayet wind) gas phase and especially dust grain material. These two papers summarize and complement the content of two papers that recently appeared in Astrophys. J. (Meyer et al., 1997; Ellison et al., 1997). This revised version was published online in June 2006 with corrections to the Cover Date.     

Galileo Probe Measurements of D/H and 3He/4He in Jupiter's Atmosphere

The Galileo Probe Mass Spectrometer measurements in the atmosphere of Jupiter give D/H = (2.6 ± 0.7) × 10-5 3He/4He = (1.66 ± 0.05) × 10-4These ratios supercede earlier results by Niemann et al. (1996) and are based on a reevaluation of the instrument response at high count rates and a more detailed study of the contributions of different species to the mass peak at 3 amu. The D/H ratio is consistent with Voyager and ground based data and recent spectroscopic and solar wind (SW) values obtained from the Infrared Spectroscopic Observatory (ISO) and Ulysses. The 3He/4He ratio is higher than that found in meteoritic gases (1.5 ± 0.3) × 10-4. The Galileo result for D/H when compared with that for hydrogen in the local interstellar medium (1.6 ± 0.12) × 10-5 implies a small decrease in D/H in this part of the universe during the past 4.55 billion years. Thus, it tends to support small values of primordial D/H - in the range of several times 10-5 rather than several times 10-4. These results are also quite consistent with no change in (D+3He)/H during the past 4.55 billion years in this part of our galaxy.     

碳纤维表面微观结构的定量化表征方法

通过使用Matlab编程处理日本东丽T300、国产GCF-1和GCF-2等3种碳纤维样品断面的扫描电镜照片,采用二值标签算法获得了碳纤维的直径及圆度等碳纤维物理特征定量数据。建立了采用直线方程切线法寻找并计算碳纤维表面沟槽的数量及尺度的方法,发现3种碳纤维样品的边缘沟槽的深度及宽度的分布均符合Weibull分布的特征。3种碳纤维的表面物理特征随温度变化的规律相同,说明其在结构上存在着一致性。经过不同温度热处理后3种碳纤维样品的圆度值变化不大,平均直径随着热处理温度的升高逐渐减小,并且表面沟槽的数量及分布的变化规律相同,说明其结构存在一致性。3种碳纤维的圆度等表面物理特征存在一定差异,T300的圆度小于国产GCF-1及GCF-2碳纤维。     

2219 铝合金搅拌摩擦焊缝匙孔形缺陷修补技术

采用固相填充+搅拌摩擦焊复合工艺进行了2219铝合金搅拌摩擦焊缝匙孔形缺陷的修补,焊后对接头的微观组织和力学性能进行了分析。结果显示:匙孔修补位置焊接接头焊核区呈现细小的等轴晶,热力影响区组织发生了较大程度的弯曲变形,接头抗拉强度≥335 MPa,延伸率≥8.0%,断裂机理为韧性断裂。