D-最优试验设计在动力调谐陀螺测试中的应用

 为了提高动力调谐陀螺的静态漂移误差测试精度,针对简化静态漂移误差模型,并且考虑陀螺安装角误差的影响,依据D-最优试验设计理论以及正交设计的均匀分散性试验设计思路,设计了一种满足D-最优性质的正交八位置试验方案,并在整个正交空间内采用全局搜索的方法验证了其D-最优性。在相同试验环境下,采用力反馈位置试验法,以全正交空间预测误差平方和最小为评价准则,对该八位置试验方案和国军标GJB1183—91中的八位置试验方案进行比较与评价,试验结果表明该八位置试验方案优于国军标GJB1183—91中八位置试验方案。     

某型先进发动机燃油喷嘴雾化特性的试验研究及火焰筒头部数值模拟

使用相位多普勒粒子分析仪和激光多普勒粒子测速仪系统(PDPA/LDV)等设备测量了某型航空发动机喷嘴的雾化特性,主要包括:喷嘴流量特性,雾化粒度(SMD)和喷雾锥角。应用Fluent软件,对装用该喷嘴的燃烧室火焰筒进行了数值模拟。试验和计算结果得出了一些有价值的结论,对该发动机的燃油喷嘴和火焰筒头部温度场、速度场有深入了解,对其改进提供了重要依据。     

RTM成型聚酰亚胺复合材料研究

以苯乙炔封端聚酰亚胺树脂为基体,采用高温R1M工艺复合成型了T300碳布增强聚酰亚胺层合板,复合材料的Tg达351℃(DMA),材料在300℃弯曲强度保持率达90%以上,模量保持率达85%以上,层间剪切强度保持率达60%以上.     

RFI工艺成型两种环氧树脂基复合材料性能比较

采用RFI工艺分别成型了648和5228A环氧树脂基复合材料层合板,其增强材料为碳纤维无屈曲织物,铺层方式为[(0,90)/( 45)]s;测试了两组层舍板的拉伸性能、弯曲性能和层间剪切性能并做了比较分析;对破坏形式和机理进行了探讨.结果表明:5228A相对于648环氧树脂膜有较宽的低黏度区域,较长的凝胶时间;5228A与648层合板相比,拉伸强度高106%,拉伸模量、泊松比接近;弯曲强度高58%,弯曲模量高16%;层间剪切强度高62%.     

A Twin-CME Scenario for Ground Level Enhancement Events

Ground Level Enhancement (GLEs) events are extreme Solar Energetic Particle (SEP) events. Protons in these events often reach ～GeV/nucleon. Understanding the underlying particle acceleration mechanism in these events is a major goal for Space Weather studies. In Solar Cycle 23, a total of 16 GLEs have been identified. Most of them have preceding CMEs and in-situ energetic particle observations show some of them are enhanced in ICME or flare-like material. Motivated by this observation, we discuss here a scenario in which two CMEs erupt in sequence during a short period of time from the same Active Region (AR) with a pseudo-streamer-like pre-eruption magnetic field configuration. The first CME is narrower and slower and the second CME is wider and faster. We show that the magnetic field configuration in our proposed scenario can lead to magnetic reconnection between the open and closed field lines that drape and enclose the first CME and its driven shock. The combined effect of the presence of the first shock and the existence of the open close reconnection is that when the second CME erupts and drives a second shock, one finds both an excess of seed population and an enhanced turbulence level at the front of the second shock than the case of a single CME-driven shock. Therefore, a more efficient particle acceleration will occur. The implications of our proposed scenario are discussed.     

Study on Conceptual Selection for Provision of Trainers in Primary and Intermediate Training Stage

为了在初/中级教练机装备方案决策中体现出训练需求,选用质量功能展开的方法对其进行了分析.先利用比较矩阵确定训练需求重要度,建立训练需求与能力属性之间的QFD关系矩阵,得到不同能力属性的重要度,最后计算出个方案的能力属性值,通过线性加权计算将属性值反映到不同方案对于训练需求的满足程度上来,得出了量化分析的结果,为教练机装备决策方法研究提供了一个新思路.     

Track-before-detect for Infrared Maneuvering Dim Multi-target via MM-PHD

In this paper, we present a novel and efficient track-before-detect (TBD) algorithm based on multiple-model probability hypothesis density (MM-PHD) for tracking infrared maneuvering dim multi-target. Firstly, the standard sequential Monte Carlo probability hypothesis density (SMC-PHD) TBD-based algorithm is introduced and sequentially improved by the adaptive process noise and the importance re-sampling on particle likelihood, which result in the improvement in the algorithm robustness and convergence speed. Secondly, backward recursion of SMC-PHD is derived in order to ameliorate the tracking performance especially at the time of the multi-target arising. Finally, SMC-PHD is extended with multiple-model to track maneuvering dim multi-target. Extensive experiments have proved the efficiency of the presented algorithm in tracking infrared maneuvering dim multi-target, which produces better performance in track detection and tracking than other TBD-based algorithms including SMC-PHD, multiple-model particle filter (MM-PF), histogram probability multi-hypothesis tracking (H-PMHT) and Viterbi-like.     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

Family of constrained signal detectors for hyperspectral imagery

Generalized likelihood ratio tests (GLRTs) are derived for the problem of detecting targets in hyperspectral images. These detectors are derived under the assumptions that the signals from the materials in the image mix linearly and that the noise in the system is Gaussian. It is also assumed that the abundances of the signals from the various materials in a pixel must sum to one. This constraint models the fact that the material abundances in a pixel are just the fraction of the pixel that they occupy. Under these assumptions, detectors are derived which outperform the detectors derived without the sum-to-one constraint.