单平台多任务电子载荷的射频与信号处理管理

介绍了侦察、对抗和打击一体化系统在现代战争中的地位与作用,分析了单个平台内多任务使命电子载荷发展的趋势在于射频和信号处理综合管理,并对综合管理面临的挑战、可行性和实现途径等进行了研究,在此基础上得出几点启示。     

冷却速度对TG6钛合金均温区组织性能的影响

通过焊接热模拟试验研究冷却速度对TG6钛合金焊接热模拟均温区组织性能的影响。结果表明:在空冷状态下均温区达到最佳的性能,随着冷却速度的增大,均温区的抗拉强度稍有提高,拉伸延伸率及断面收缩率没有明显变化;冲击韧性空冷达到最大值,水冷稍有下降;显微硬度随冷却速度增大而增加。     

抑制恒压变量柱塞泵压力低频振荡方法的研究

为解决恒压变量柱塞泵出口压力出现低频振动的问题,阐述了恒压变量机构的原理,从理论上分析了影响出口压力的因素,并指出产生振荡的原因,提出在泵装配过程中,采用工艺关键要点控制的方法可抑制压力低频振荡。试验表明,该方法有效地减小了泵出口压力的低频振荡,使产品装调合格率大大提高。     

深层地质数据监测系统的设计

本系统以STM32处理器芯片为主控制器,采用MSP430单片机挂载多个传感器执行多点数据采集,CAN总线实现数据通信。另配有SD存储卡,键盘,TFT彩屏,具有存储,显示等功能。本系统可以监测深层地质数据,具有超低功耗、高可靠性等优点,可以适应野外各种复杂环境下连续的长时间工作,具有广泛的应用前景。     

火星车转移坡道柔顺性优化设计及动力学分析

对一种抽展式火星车转移坡道开展柔顺性优化设计和动力学分析。首先,分析火星车与存在异面角的坡道的挤压几何原理。然后,设计坡道的间隙机构和限位机构,并计算出机构关键设计参数的最优值,以自适应调整两侧坡道的距离,〖JP2〗减小火星车与坡道护栏之间的相互作用力。最后,对坡道下落过程和火星车在坡道上的行驶过程进行动力学仿真,验证坡道柔顺性优化设计的效果。结果表明：优化后的坡道柔顺性大幅提高,坡道可以自适应调整两侧的距离;使用优化后的坡道,可以有效降低火星车与坡道护栏的作用力,实现火星车在坡道上的安全行驶。     

液氢贮箱停放过程中的力热分析

为了寻找到运载火箭长时间停放过程中液氢贮箱的最经济液位,用于制定合理的发射流程以及紧急处置方法,采用计算流体力学(CFD)技术,对某型运载火箭停放期间液氢贮箱的力、热情况进行了仿真计算和分析。计算选用了VOF(Volume-of-fluid)两相流模型以及Lee相变模型,为了提高Lee模型在不同压力情况下对相变过程的模拟精度,采用安托因方程修正了该模型。修正后的模型首先由试验数据校验了其精确性,随后开展的液氢贮箱停放过程仿真结果表明：贮箱的竖直方向与径向均存在温度分层的现象,液相内会形成大的漩涡,该漩涡会使得冷热流体不断进行热交换,并导致贮箱内部的液氢出现气化。贮箱停放期间蒸发率最大值超过2 m 3/h,发生在停放4 h左右;而贮箱液位充填至37 m 3以上或17 m 3以下时蒸发率较低,最小值接近1 m 3/h。     

An improved numerical method for constructing Halo/Lissajous orbits in a full solar system model

An improved numerical method that can construct Halo/Lissajous orbits in the vicinity of collinear libration points in a full solar system model is investigated. A full solar system gravitational model in the geocentric rotating coordinate system with a clear presentation of the angular velocity relative to the inertial coordinate system is proposed. An alternative way to determine patch points in the multiple shooting method is provided based on a dynamical analysis with Poincare′sections. By employing the new patch points and sequential quadratic programming, Halo orbits for L_1, L_2, and L_3 points as well as Lissajous orbits for L_1 and L_2 points in the EarthMoon system are generated with the proposed full solar system gravitational model to verify the effectiveness of the proposed method.     

油液冷却航空湿式摩擦离合器热特性分析

为了研究航空高功率密度湿式摩擦离合器在油液冷却作用下的温度特性,基于计算流体动力学（computational fluid dynamics,CFD）方法建立了华夫槽湿式摩擦离合器的热特性分析模型;研究了湿式摩擦离合器中摩擦副上热流密度的计算方法和施加方式;运用热流耦合方法,考虑了油液的散热作用,分析了离合器内各对摩擦副上的油液分布及温度分布。研究结果表明:钢片上和摩擦片上的油液分布不均造成钢片和摩擦片上温度分布不均;不同钢片和摩擦片上的温度分布受片上油液分布及该片热传导性能的影响,呈现出不同的温度分布规律。      

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

Using the radial basis function neural network to predict ionospheric critical frequency of F2 layer over Wuhan

Neural networks (NNs) have been applied to ionospheric predictions recently. This paper uses radial basis function neural network (RBF-NN) to forecast hourly values of the ionospheric F₂ layer critical frequency(f_oF₂), over Wuhan (30.5N, 114.3E), China. The false nearest neighbor method is used to determine the embedding dimension, and the principal component analysis (PCA) is used to reduce noise and dimension. The whole study is based on a sample of about 26,000 observations of f_oF₂ with 1-h time resolution, derived during the period from January 1981 to December 1983. The performance of RBF-NN is estimated by calculating the normalized root-mean-squared (NRMSE) error, and its results show that short-term predictions of f_oF₂ are improved.