一种微波关联成像的新方法

将强度关联量子成像理论引入到雷达成像技术中,提出了一种全新的微波关联成像方法。向目标发射多个幅度、相位可控的单元信号,同时记录各个信号的状态并结合距离信息制作＂成像底版＂,通过对回波信号和＂成像底版＂的关联结果进行数理统计后可实现雷达高分辨成像。     

环形腔室径向宽度对加力燃油泵内流及性能影响

对某加力燃油泵内部非定常流动开展了系统的数值模拟,研究了不同环形腔室径向宽度条件下泵的外特性和内流特征.计算结果表明,缩小径向宽度可有效提高泵在不同流量下的扬程,且小流量工况增幅显著高于大流量,明显改善了小流量工作的不稳定性.对于大流量工况,环形腔室截面变小导致腔室内循环流量降低、沿程损失明显减小,是泵出口扬程提高的主要因素;而对于小流量工况,环形腔室截面变小使得扩散管主流贴近环形腔室,显著降低了叶轮流道扬程损失,有效提升了泵出口扬程.      

大飞机风切变探测告警系统

介绍了国内外在机载风切变告警系统方面的研究进展,通过对比国内外的研究情况,发现由于国内的需求不足,使得在具体产品的研究进展上与国外存在较大差距。由于中国大飞机研究项目的全面展开．也必然为包括机载风切变告警系统在内的、与大飞机有关的各种机载产品的发展提供了很好的机会。指出为了尽快弥补国内研究的差距,需在风切变建模、风切变探测及风切变告警系统的试飞验证方面做出进一步努力。     

条形碳化硅纤维的制备与性能

使用异形喷丝板通过熔融纺丝制备出条形聚碳硅烷原纤维,然后经不熔化及高温烧成得到条形碳化硅纤维。通过X射线衍射仪分析了条形碳化硅纤维的构成、强度及电磁性能。结果表明,条形碳化硅纤维主要由β-SiC和无定形SiC组成,纤维的当量直径为20~31μm,拉伸强度为0.8~2.4 GPa,介电常数实部ε′为6.2~6.8,虚部ε″为2.5~3.3。条形碳化硅纤维可用作结构吸波材料。     

基于LabVIEW的空间碎片高速撞击数据采集系统设计与实现

利用声发射传感器对空间碎片的撞击数据进行实时采集监测,用以对航天器在轨安全防护提供预警。该系统基于LabVIEW虚拟仪器技术,采用图形化编程语言实现了高速数据的采集。具有数据采集、实时波形显示、数据存储等功能,编程简捷、精度高、稳定性好,且人机界面友好。     

基于双驱调制的高速光电探测器频响自校准表征

针对当前高速光电探测器频率响应测试的问题,提出了基于双驱调制的高速光电探测器频响自校准表征方法。该方法通过设置双驱调制频率为近似相等关系克服了电-光响应器件不平坦响应的额外校准,实现了光电探测器频率响应的自校准表征。同时,通过采用双驱调制频率的和频与差频拍频边带的相对功率来获得光电探测器的频率响应,摆脱了双驱马赫-曾德尔调制器偏置漂移的影响并扩展了两倍以上的测试带宽。相比于全光激励法,提高了测量精度与动态范围;与传统电光激励法相比,克服了强度调制器偏置漂移的影响和额外校准的难题;优于先前的双音调制法,简化了测试系统和降低了测量成本。光电探测器频率响应的实验测量结果与强度噪声法测量结果以及与该光电探测器出厂数据的一致性验证了该方法的正确性。     

On the early phase of relativistic solar particle events: Are there signatures of acceleration mechanism?

Many physical processes precede and accompany the solar energetic particles (SEP) occurrence on the Earth’s orbit. Explosive energy release on the Sun gives rise to a flare and a coronal mass ejection (CME). X-ray and gamma emissions are believed to be connected with flares. Radio emission is signature of disturbances traveling through the corona and interplanetary space. Particles can gain energy both in the flare and the accompanying wave processes. The beginning of the SEP events has the advantage of being the phase most close to the time of acceleration. Influence of interplanetary transport is minimal in the case of first arriving relativistic solar protons recorded by ground based neutron monitors in so called ground-level enhancements (GLE). The early phase of the SEP events attracts attention of many scientists searching for the understanding of particle acceleration. However, they come to the opposite conclusions. While some authors find arguments for coronal mass ejections as a sole accelerator of SEPs, others prove a flare to be the SEP origin. Here, the circumstances of SEP generation for several GLEs of the 23rd solar cycle are considered. Timing of X-ray, CME, and radio emissions shows a great variety from event to event. However, the time of particle ejection from the Sun is closer to maximum of X-ray emission than to any other phenomena considered. No correlation is found between the particle fluxes and the CME characteristics.     

The dust content of clusters of galaxies

We have statistically investigated the infrared luminosity of clusters of galaxies in comparison with the known tracers of the cluster mass like the X-ray luminosity and the cluster richness (e.g. the number of member galaxies). Our results show that there is a clear positive correlation of the infrared luminosity with the cluster mass. Quantitatively speaking, the infrared luminosity is on average 20 times higher than the X-ray luminosity. Moreover, the infrared luminosity increases with the redshift. This probably shows that a major part of this infrared luminosity is due to star formation in the member galaxies. Another possible contribution would be the thermal emission from dust particles in the diffuse intracluster medium. However our method does not allow us to infer conclusions about this second hypothesis. Depending on their size and abundance, such particles would contribute to the infrared luminosity of galaxy cluster and have an impact on the cooling function of the baryons and thus on the formation of the large scale structures. This is an important cosmological question which still remains open.     

Experimental Investigation into Characteristics of Plasma Aerodynamic Actuation Generated by Dielectric Barrier Discharge

This article carries out synthetic measurements and analysis of the characteristics of the asymmetric surface dielectric barrier discharge plasma aerodynamic actuation.The rotational and vibrational temperatures of an N2 (C3Пu) molecule are measured in terms of the optical emission spectra from the N2 second positive system.A simplified collision-radiation model for N2(C) and N2+(B) is established on the basis of the ratio of emission intensity at 391.4 nm to that at 380.5 nm and the ratio of emission intensity at 371.1 nm to that at 380.5 nm for calculating temporal and spatial averaged electron temperatures and densities.Under one atmosphere pressure,the electron temperature and density are on the order of 1.6 eV and 1011cm-3 respectively.The body force induced by the plasma aerodynamic actuation is on the order of tens of mN while the induced flow velocity is around 1.3m/s.Starting vortex is firstly induced by the actuation;then it develops into a near-wall jet,about 70 mm downstream of the actuator.Unsteady plasma aerodynamic actuation might stimulate more vortexes in the flow field.The induced flow direction by nanosecond discharge plasma aerodynamic actuation is not parallel,but vertical to the dielectric layer surface.     

天线系数变化对电场辐射发射测量的影响

介绍了天线系数的有关特性。阐述了天线系数变化对电场辐射发射测量的影响。最后分析了天线系数变化的原因。