GPS定位数据在海洋一号卫星中的应用与比较

简要介绍了海洋一号卫星星载GPS接收机的定位原理、流程和应用，探讨了一种在轨定位结果的确认和互验方法．借助于卫星工具包软件(STK)，利用NASA网站公布的HY-1卫星两行根数(TLE)进行卫星轨道推算，生成星下点位置，并与相应时刻星载GPS接收机实测数据得到的星下点位置进行比较，由此得到两种方法定位结果之间的偏差，用实际在轨数据验证了两者的位置符合程度．     

铝/ZN-1阻尼材料复合结构件的粘接技术研究

探讨了胶黏剂黏度、硬铝表面处理方式及硅烷偶联剂KH-560的使用方式等因素对硬铝板/ZN-1阻尼材料复合结构件的粘接性能的影响。研究表明：如果硬铝板表面采用砂纸打磨处理时，采用黏度较低的TC-1环氧树脂胶或者在黏度较高的J-22环氧树脂胶中添加2％的硅烷偶联剂KH-560可以获得优异的粘接效果；当硬铝板表面采用铬酸阳极化处理时，两种胶黏剂均能获得优异的粘接效果。     

测量机连续扫描控制系统设计

利用UCC1控制器作为核心,构建具有三维空间连续扫描功能的测量机控制系统的方法,并简要介绍了UCC1控制器的功能及控制系统硬件电路的设计。     

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.     

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.     

基于S1,S2流面理论的液体火箭发动机涡轮内部流场计算

应用S1,S2流面理论对某大型液氢/液氧火箭发动机涡轮泵的两级轴流式涡轮内部跨声速流场进行计算和分析。流面的求解采用流线曲率法。将混合平面法的思想用于流线曲率法的求解过程中,对动、静叶排之间的相互干扰进行处理,将复杂的非定常问题简化为定常问题,从而简化计算。粘性的影响通过几种损失系数进行修正。计算结果较好地描述了涡轮内部的流动情况,为进一步完善涡轮设计、提高涡轮性能提供了理论依据。     

基于三维裂纹尖端应力场的应力强度因子计算方法

提出一种基于无限大体裂纹尖端弹性应力场理论解的前几项多项式函数,对实际裂纹体弹性应力场有限元解进行拟合来计算应力强度因子的方法.该方法在计算应力强度因子时不需要预先假设裂纹尖端的应力应变状态,应力强度因子计算结果更符合三维裂纹体裂纹尖端实际的应力应变状态.首先基于二维无限大板中心穿透裂纹应力场理论解验证了方法的有效性,探讨了拟合确定应力强度因子需要的多项式应力函数的项数.然后分别以二维大板中心穿透裂纹、三维大体内埋圆裂纹和三维有限厚板中心穿透裂纹的应力强度因子计算为例,通过与无限大板和无限大体应力强度因子理论解以及基于位移外推法和1/4节点张开位移法的应力强度因子有限元解的对比分析,验证了该方法的有效性和合理性.研究表明该方法能够合理反映三维裂纹体裂纹尖端的实际应力应变状态,计算得到的应力强度因子数值更合理.