应用ART1神经网络仿真车间分组

阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。     

Expectations for Infrared Spectroscopy of 9P/Tempel 1 from Deep Impact

The science payload on the Deep Impact mission includes a 1.05–4.8 μm infrared spectrometer with a spectral resolution ranging from R∼200–900. The Deep Impact IR spectrometer was designed to optimize, within engineering and cost constraints, observations of the dust, gas, and nucleus of 9P/Tempel 1. The wavelength range includes absorption and emission features from ices, silicates, organics, and many gases that are known to be, or anticipated to be, present on comets. The expected data will provide measurements at previously unseen spatial resolution before, during, and after our cratering experiment at the comet 9P/Tempel 1. This article explores the unique aspects of the Deep Impact IR spectrometer experiment, presents a range of expectations for spectral data of 9P/Tempel 1, and summarizes the specific science objectives at each phase of the mission.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

波音737NG飞机平尾内梁下蒙皮裂纹的修理

介绍了水平安定面内梁下蒙皮裂纹的成因以及发现裂纹后的修理方法，结合定检维修经验对裂纹损伤修理方案和经常出现的问题进行了分析总结，并给出了修理工期控制的建议。     

基于B/S的空管自动化综合航迹显示系统的设计与实现

提出一种基于B/S的综合航迹显示系统,该系统通过解析空管自动化系统的综合航迹实现了在IE浏览器上对区域内的航迹的监视。系统实现主要包括三部分:一是综合航迹的接收,主要通过对同步串口卡的数据读取;二是对数据的数据库处理;三是对综合航迹的显示。系统实现了对MH4008003类数据的解析以及对空管自动化系统的地图解析,并且在IE界面上提供了航迹态势显示以及用户交互接口。     

Atmospheric reentry hemisphere prediction for prograde orbits using logical disjunction

A unique logic-based algorithm for atmospheric reentry hemisphere prediction is presented for spacecraft in low-eccentricity, prograde low Earth orbits at altitudes of 300 km and lower. Using two-line element (TLE) data for initial orbit conditions, coupled with coarse estimates for spacecraft aerodynamic characteristics, the algorithm relies on logical disjunction operations based on a dual analysis of histogram and two-weighted Gaussian probability density function (PDF) fits of predicted reentry latitude data. The algorithm requires the execution of a series of parametric simulations to determine the reentry hemisphere for variations in spacecraft aerodynamic coefficients and drag reference area. When implemented, the algorithm yields accurate hemisphere predictions on average 15 days from reentry as demonstrated by historical reentry cases from 1979 to 2018. All reentry cases were selected to demonstrate the algorithm’s ability to deliver accurate reentry hemisphere predictions for spacecraft with varying physical size and mass, and reentering during different periods of solar cycle activity.     

DME Interference mitigation for L-DACS1 based on system identification and sparse representation

L-band digital aeronautical communication system 1 (L-DACS1) is a promising candi-date data-link for future air-ground communication, but it is severely interfered by the pulse pairs (PPs) generated by distance measure equipment. A novel PP mitigation approach is proposed in this paper. Firstly, a deformed PP detection (DPPD) method that combines a filter bank, correlation detection, and rescanning is proposed to detect the deformed PPs (DPPs) which are caused by mul-tiple filters in the receiver. Secondly, a finite impulse response (FIR) model is used to approximate the overall characteristic of filters, and then the waveform of DPP can be acquired by the original waveform of PP and the FIR model. Finally, sparse representation is used to estimate the position and amplitude of each DPP, and then reconstruct each DPP. The reconstructed DPPs will be sub-tracted from the contaminated signal to mitigate interference. Numerical experiments show that the bit error rate performance of our approach is about 5 dB better than that of recent works and is closer to interference-free environment.     

均匀化处理对TiAl 合金铸造组织的影响

研究了均匀化处理对两种含B的铸造TiAl合金铸造组织的影响。研究发现1 370℃/5 min/OQ+1150℃/6 h/AC均匀化热处理能有效消除B2相,将b稳定化元素固溶到基体中,实现成分均匀化;1 370℃/5 min/OQ+1 150℃/24 h/AC均匀化热处理后可使粗大的铸造片层组织分解转变为细晶近g组织,平均晶粒直径50mm。     

会议筹备的多目标规划

针对会议筹备的三个问题即预订宾馆、会议室安排、租车问题建立优化模型。对于预订宾馆问题、建立目标函数和约束条件、利用Lingo求解,将会议室安排和租车问题的各方面因素综合考虑建立模型并求解。     

TA2/Ni+Nb中间层/1Cr18Ni9Ti扩散焊接头的组织与性能

采用50μm纯Ni箔+10μm纯Nb箔复合中间层,在焊接温度840℃,880℃和920℃,压力4MPa以及保温时间60min的工艺下,对工业纯钛TA2和1Cr18Ni9Ti不锈钢进行了真空扩散焊实验,测试了接头的抗拉强度,并利用光学显微镜(OM)、扫描电镜(SEM)、能谱(EDS)和X射线衍射(XRD)对接头的组织结构、元素分布以及断口形貌和相组成进行了分析。结果表明:Ni+Nb复合中间层的存在成功阻止了Fe,Ti互扩散,实现了TA2与1Cr18Ni9Ti的可靠连接,接头的拉伸强度达到261MPa,该强度主要受剩余Ni箔控制,且焊接温度的变化对其影响不大。接头所生成反应层自不锈钢一侧起分别为FeCrNi固溶体、剩余Ni,Ni3Nb,剩余Nb以及TiNb魏氏体。