静电场仪校准系统的设计及仿真研究

静电场仪的精确校准对提高卫星在轨电场探测精度、保障卫星安全发射升空、精确预测雷电等具有重要意义。针对电场仪校准的需要,设计了平行极板电容式静态电场仪校准装置。利用三维电磁场仿真软件CST对标准静电场发生装置进行数值仿真,研究了校准箱内部及边缘处的静电场分布特点,分析标准极板直径和间距对边缘效应的影响,结合极板平行度对电场均匀性的影响分析,确定了校准过程中电场仪探头的最佳位置,实现静电场仪校准装置的最优化设计。     

压电周期板中耦合禁带影响规律分析

近年来,利用周期结构中弹性波禁带特性减振的研究思路受到了广泛关注。针对以往周期结构难以实现宽频且可调禁带的问题,设计了一种含电路网络的压电周期结构。该结构中的弯曲波和电路网络中的电波通过压电效应可以产生一个较宽的耦合禁带,且通过调整电路参数就可以达到调节禁带位置的目的。首先,为了高效计算该结构的波动特性,开发了适用于压电周期结构的减缩波有限元算法,该算法可以在保证结果准确性的基础上节约90%以上的计算时间。利用该算法研究了压电材料尺寸和形状对耦合禁带性能的影响。结果表明:相同电学参数下,随着压电片尺寸的增大,耦合禁带向低频移动,且禁带带宽增加;相同面积下含圆形和方形压电片的机电系统内耦合禁带差异较小,即形状对耦合禁带的分布影响不大。其次,针对不同尺寸和形状的机电系统,设计了电学参数使得在同一频率附近产生耦合禁带,并分析了其性能差异。最后,为了证明耦合禁带的减振效果,设计了一种有限压电周期板模型,其强迫响应的结果证明了耦合禁带对结构内弹性波可以进行有效调控。      

环氧树脂基复合材料加筋板结构吸湿行为研究

环氧树脂基复合材料的性能对湿热环境敏感,掌握该材料所组成结构的吸湿行为对其实际应用具有重要意义。通过以碳纤维环氧树脂基复合材料层合板的non-Fickian吸湿模型为基础,建立环氧树脂基复合材料加筋板结构的non-Fickian吸湿模型,在70℃/85% RH湿热条件下开展加筋板结构的吸湿实验,对所建立模型进行验证,并与已有的加筋板吸湿模型进行对比,通过所建立模型给出了加筋板沿厚度方向的吸湿量分布规律。结果表明:所建立加筋板non-Fickian吸湿模型的计算结果与实验结果吻合良好,在整个吸湿阶段相对误差小于5%,模型的预测精度高于传统Fick模型。所建立的加筋板non-Fickian吸湿模型可用于环氧树脂基复合材料加筋板层合结构吸湿量的准确预测。      

Scientific objectives and payloads of Tianwen-1, China’s first Mars exploration mission

This paper describes the scientific objectives and payloads of Tianwen-1, China’s first exploration mission to Mars. An orbiter, carrying a lander and a rover, lifted-off in July 2020 for a journey to Mars where it should arrive in February 2021. A suite of 13 scientific payloads, for in-situ and remote sensing, autonomously commanded by integrated payload controllers and mounted on the orbiter and the rover will study the magnetosphere and ionosphere of Mars and the relation with the solar wind, the atmosphere, surface and subsurface of the planet, looking at the topography, composition and structure and in particular for subsurface ice. The mission will also investigate Mars climate history. It is expected that Tianwen-1 will contribute significantly to advance our scientific knowledge of Mars.     

Spacecraft survivability in the natural debris environment near the stable Earth-Moon Lagrange points

The theoretical analysis of the motion of natural space debris near the stable Earth-Moon Lagrange Points, $L_4$ and $L_5$, is presented with a focus on the potential debris risks to spacecraft operating near these points. Specifically, the research formulates a debris propagation model using four-body dynamics, then applies candidate probabilistic survivability models to a notional spacecraft operating at the $L_4$ and $L_5$ Lagrange points to quantify the collision risks to the spacecraft from natural debris particles. Of the survivability models implemented, the natural debris collision risks to spacecraft survivability are found to be incredibly low, but mitigation strategies to reduce the risk further are identified in this study. Overall, research into stable Lagrange point natural debris propagation improves understanding of the collision risks posed by the naturally occurring Kordylewski clouds and enhances operational planning for Lagrange point space missions.     

Solar sail trajectories with piecewise-constant steering laws

Solar sails have much attracted the interest of the scientific community as an advanced low-thrust propulsion means capable of promoting the reduction of mission costs and the feasibility of missions that are not practically accessible via conventional propulsion because of their large ΔV requirements. To reduce the overall flight time, a given mission is usually analyzed in the framework of a minimum time control problem, with the employment of a continuous steering law. The aim of this paper is to investigate the performance achievable with a piecewise-constant steering law whose aim is to substantially reduce the complex task of reorienting the sail over the whole mission. Unlike previous studies based on direct approaches, here we use an indirect method to optimally select the sail angle within a set of prescribed values. The corresponding steering law translates the results available for continuous controls to the discrete case, and is able of producing trajectories that are competitive in performance with the optimum variable direction program.     

基于ANSYS的同面多电极电容传感器仿真研究

同面多电极电容传感器是一种新的飞机复合材料构件损伤检测技术,该检测技术的正问题中敏感场分布函数的计算要涉及到静电场中电容计算问题。在仿真研究中,电容要通过场的数值计算方法来求得。本文介绍了如何使用ANSYS有限元分析计算同面多电极电容传感器中的各电极对之间的电容,对检测材料发生异常及传感器参数改变时电容的变化进行了分析,为损伤检测的特征提取和逆问题图像重构提供了仿真数据。     

翼尖装置优化设计研究

使用面元法气动分析软件VSAERO对机翼与翼梢小翼组合体模型进行数值模拟,并采用Steve Smith提出的诱导阻力优化方法对翼梢小翼的定位进行优化设计。结果表明,能够有效地预测出翼梢小翼的最优定位,在翼梢小翼优化设计中具有很好的适用性。     

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.     

由混合特征对构造对称三对角矩阵

文章考虑一类由混合特征对构造对称三对角矩阵,文中给出了解的存在性和唯一性的充分必要条件,并且给出相应的算法和数值算例。