带孔件成形过程试验研究

本文采用坐标网目法对带孔件成形过程进行了试验研究。试验所获应变分布表明,带孔件在变形过程中存在拉深和翻边两种变形趋向性,在模具参数和工艺条件完全相同的情况下,其可能的变形趋势与孔的尺寸有关。本文的研究结果可为带孔件成形过程中的变形趋向性分析乃至变形过程控制提供理论依据。     

夫兰克—赫兹实验中影响曲线形状的因素分析

夫兰克－赫兹实验是近代物理的实验之一，对物理学有深远影响。本文介绍在夫兰克－赫兹实验中影响IA－UGK曲线的几种重要因素，得出了这些因素变化时的实验曲线变化规律，详细分析了原因，并总结出为减小测量误差应选择的实验参数的范围。     

甲烷/氧气双组元微型推力室的实验研究

为研究微小推力室的工作特点,建立了双组元微小推力室的地面实验装置和数据采集系统。在内径为4mm,喉部直径为0.4mm的微小推力室内,采用氧气和甲烷气体作为推进剂进行了点火热试车,实时测量燃烧室压力和壁面的温度分布。实验结果表明,在富燃工况下,随着混合比的升高,燃烧温度和燃烧室压力逐渐升高;当混合比一定时,随着总流量的增加,燃烧室压力增加,微小推力室的推力和比冲也在升高。微小推力室的真空推力达到120mN,真空比冲达到了240s。     

惯性组合导航系统的实时多级景象匹配算法

 针对景象匹配辅助惯性组合导航系统需要快速准确获取飞行器位置、航向偏差的要求,提出一种实时多级景象匹配算法。算法分为两级,第一级粗匹配中提出了中心点4邻域的抗变形算法,能抗旋转和小尺度变化的影响,使定位精度达到像素级;第二级精匹配中提出了基于分支特征点,应用最小二乘法原理精确匹配定位出两幅图像间的最优相似变换参数,即飞行器的精确位置和航向偏差的算法。仿真分析表明,提出的实时多级算法能满足景象匹配辅助惯性组合导航系统实时性、精确性和鲁棒性的要求。     

Time delay of ionospheric TEC storms to geomagnetic storms and pre-storm disturbance events in East Asia

Using the TEC data at Beijing (39.61°N, 115.89°E)/Yakutsk (62.03°N, 129.68°E) stations of East Asia regions and relevant geomagnetic data from 2010 to 2017, we have studied the time delay of ionospheric storms to geomagnetic storms and compare it with our previous results of Taoyuan (25.02°N, 121.21°E) station (Zhang et al., 2020). The data shows a well-known local time dependence of the time delay, and seasonal dependences are different at these stations. In addition, there is no correlation between the time delay and the magnetic storm intensity /solar activity, except the time delay of negative storms has weakly negative dependence on the solar activity. Comparing with the results of Taoyuan station which is located at EIA region in East Asia, we find that the time delay increases nonlinearly as the latitude decreases due to different ionospheric backgrounds at these places. Moreover, the pre-storm disturbance events are found to have similar statistical characteristics as the pre-storm enhancement in Europe middle latitudes (Bure?ová and La?tovi?ka, 2007). By subtracting the common features of the pre-storm disturbance events, we preliminarily infer that auroral activity might be main driver of the pre-storm disturbance events.     

Polysaccharide from Loquat Leaves to Prepare Hierarchical Porous Carbon as a Matrix for Active Sulfur

Fossil fuel exhaustion and overdevelopment usually lead to a recession,which is worsened by the environmental pollution.So it is of high priority to develop high-efficiency energy storage device.Here,agreen and environment-friendly strategy is devised to fabricate carbon materials from biomass.By water extraction and alcohol precipitation,polysaccharide is extracted from loquat leaves.After calcining under high temperature,hierarchical porous carbon materials(HPCM)are obtained,possessing a variety of macropores,mesopores and micropores.Such ample and hierarchical pores enable the electrolyte infiltration and the buffering of the volume expansion of sulfur in repeated electrochemical reactions.The structure stability of the entire electrode can thus be well maintained.When evaluated as the scaffold for sulfur,the electrochemical performance of carbon/sulfur composite was tested.Even after 500 cycles,the reversible capacity is retained as high as 485.4 mA·h/g at the current density of 1.6 A/g.It also offers a notable rate capability,attaining the discharge capacity of 700.7 mA·h/g at 2 C.All the electrochemical performance results prove the feasibility of the proposed strategy.     

Statistical study of energetic electrons in Jupiter’s inner magnetosphere by Juno/JEDI

The Juno spacecraft made the first in-situ observations of energetic particles in the polar region of Jupiter’s magnetosphere. After Jupiter Orbit Insertion (JOI) in July 2016, data from ~20 Juno perijoves (PJs) obtained by Juno/JEDI are accumulated, providing an excellent opportunity to study the long term spatio-temporal distribution of energetic particles in Jupiter’s radiation belt. We transform Juno’s position from a Cartesian to a magnetic coordinate system by tracing magnetic field lines based on a fourth order Runge-Kutta method. Then the fluxes of energetic electrons from PJ1 to PJ14 sorted by different locations in magnetic coordinate space and the data are well organized by the L-shell parameter. The variation of electron flux increases with L-shell. The deviation (the ratio of the 75th percentile to the 25th percentile) of 0.51 MeV electron flux varies from a factor of 1.23 near L = 9.5 to 27.57 near L = 15.5. However, the mean flux decreases by about one order of magnitude in the same region. The electron spectra at larger L-shells are softer than that at smaller L-shells. On the other hand, the electron flux decreases more rapidly with increased L-shell when the location is off the equator. Along an L-shell, the electron flux decrease at first and then increase again from equator to mid-latitude region. In addition, we compare the statistical results with the widely used GIRE2 model. JEDI data correspond well with the GIRE2 model when the L-shell is > 14.75. GIRE2 underestimate the electron flux for L-shell smaller than 13.25. These results of this analysis are applicable to estimate the effects of the radiation environment in Jupiter’s magnetosphere.     

量子计算及其在空气动力学中的应用前景综述

量子计算是最重要的后摩尔计算技术之一，拥有经典计算机无可比拟的超强计算能力，未来能够对各行业应用产生颠覆性的影响。针对量子计算给空气动力学带来的机遇和挑战，详细综述了量子计算机、量子算法、量子底层软件栈等方面的研究进展。结合空气动力学领域常用的基础方法，在综述量子计算线性方程组求解、插值操作、数值积分、优化搜索等最新进展的基础上，结合典型量子算法深入分析了量子计算在空气动力学领域的应用前景，并指出了需要重点关注的研究方向。     

基于受摄轨道模型的小卫星轨道摄动分析研究

小卫星在实际运行中受到多种摄动力的作用,这会对其轨道造成不同程度的影响,因此在小卫星的轨道设计与控制中,摄动是必须考虑的重要因素。本文以500km高的小卫星太阳同步轨道为研究对象,运用轨道摄动的基本理论,估计了地球非球形引力、大气阻力、太阳光压及第三体引力的量级并进行比较;建立小卫星轨道摄动分析模型,并在此模型的基础上,利用计算机仿真技术,对小卫星轨道摄动问题展开仿真研究,验证了几种主要摄动力的量级估计的结果,分析比较了几种主要摄动力对小卫星运行轨道的影响程度及规律,本文结果对小卫星轨道设计与控制具有很好的参考价值。     

基于脉冲星的空间飞行器自主导航技术研究

研究了利用X射线脉冲星实现空间飞行器自主导航的原理,指出通过测量脉冲星发射的脉冲到达航天器与到达太阳系质心的时间差可以确定该航天器的位置。给出了两种适合用于处理脉冲星观测量的方法,即基于最小二乘(LS)的方法和基于卡尔曼滤波(KF)的方法。通过数值仿真验证了X射线脉冲星自主导航技术的可行性,并且说明采用KF算法能够有效利用卫星轨道运动方程中包含的导航信息,从而获得更高的导航精度。