用电离层特性参量提取等效风场信息

导出了利用中低纬电离层特性参量获取电离层F层峰区高度上等效风场（包含电场和风场信息在内）的基本方程，并尝试用该方法从电离层特性参量（峰高和临频）提取等效风场信息，利用武汉站DGS-256电离层数字测高仪数据及由美国Massachusetts Lowell大学最新版的剖面反演程序换算得到F层峰高，获得了武汉地区夏季至日点附近，冬季至日点附近，冬季地磁特别宁静的九天和冬季平均等效风场的初步特征，并利用Fejer经验电场模式计算冬季电场引起的垂直漂移，估计电场和风场对武汉地区的垂直等效风场的贡献大小，结果表明：等效风场呈现出白天与夜晚幅度和方向的差异。至日点附近冬季与夏季白天的幅度差异以及明显的凌晨凹陷现象；平均情况下，垂直等效风场幅度和方向的变化主要是由中性风引起，受电场的影响不大。     

Mathematical modeling of plasma drifts over equatorial low latitude regions

This paper presents a mathematical model to simulate ionospheric plasma drifts at equatorial low latitude regions by coupling of E- and F-regions. The governing non-linear differential equations (of elliptic and parabolic nature) are solved numerically through finite-difference schemes and obtained neutral winds and electric fields. The temperature and electron density profiles are generated utilizing MSIS-86 atmospheric model. The continuity equation is employed to obtain night-time E-region density profile using measured ionograms at Trivandrum (India). The computed vertical and zonal plasma drifts are comparable with measured Jacamarca plasma drifts with little variations during noon and evening times. The plasma drifts at Trivandrum (8.5° N, 76.5° E, dip 0.5° N) are compared with those of Jicamarca (12° S, 76.9° W, dip 2° N). Neutral wind simulations of present model agree well with those of horizontal wind model (HWM-93). The post-sunset enhancement and its reversal are also discussed.     

Space observations of comets during solar flares: A possible explanation for comet brightness outbursts

Problems connected with mechanisms for comet brightness outbursts as well as for gamma-ray bursts remain open. Meantime, calculations show that irradiation of a certain class of comet nuclei, having high specific electric resistance, by intense fluxes of energetic protons and positively charged ions with kinetic energies more than 1 MeV/nucleon, ejected from the Sun during strong solar flares, can produce a macroscopic high-voltage electric double layer with positive charge in the subsurface zone of the nucleus, during irradiation times of the order of 10–100 h at heliocentric distances around 1–10 AU. The maximum electric energy accumulated in such layer will be restricted by the electric discharge potential of the layer material. For comet nuclei with typical radii of the order of 1–10 km the accumulated energy of such natural electric capacitor is comparable to the energy of large comet outbursts that are estimated on the basis of ground based optical observations. The impulse gamma and X-ray radiation together with optical burst from the comet nucleus during solar flares, anticipated due to high-voltage electric discharge, may serve as an indicator of realization of the processes above considered. Multi-wavelength observations of comets and pseudo-asteroids of cometary origin, having brightness correlation with solar activity, using ground based optical telescopes as well as space gamma and X-ray observatories, during strong solar flares, are very interesting for the physics of comets as well as for high energy astrophysics.     

离子液体电喷推力器的关键技术及展望

首先介绍离子液体电喷推力器的工作原理和分类，通过与其他相同推力量级的电推力器对比进一步分析了其特点，然后总结了离子液体电喷推力器的国内外研究现状，在此基础上重点梳理了微尺度下带电粒子的产生与加速、微细制造与精密装配、推进剂贮存和供给、高升压比微功率电源处理单元以及比冲和推力测试等离子液体电喷推力器研制过程中涉及的关键技术，最后展望了小型化、模块化与推力密度提升的发展趋势并提出离子液体电喷推力器的发展构想。     

有磁场时电子在航天器光电子鞘层中的漂移运动

采用二级漂移近似理论，研究了在航天器光电子鞘层中与电流收集有关的电子在磁场中的运动轨道和收集电子有关的磁瓶结构，结果表明当磁场越强，航天器表面电势越弱，磁瓶在无穷远处横截面积就越小。在光电子鞘层中，势垒对电流收集影响较大，磁瓶的横截面积在略远于垫垒处有极大值，磁瓶在无穷远处的横截面积并非随着势垒距航天器距离的远近而单调变化。     

电机瞬态转速测试

介绍了一种利用单片机和光电转速传感器来测量电机瞬态转速及电机转速变化过程的方法。该方法简单、反应时间快、准确度高。     

航天用电连接器的解体失效分析

航天用电连接器在使用过程中由于结构不可靠造成解体，是危及整个系统工程成败的致命失效。总结并分析了近年来出现的多起解体失效案例，在阐明解体失效模式和失效机理的基础上，提出针对性的检验和防止解体失效的措施。     

专业音响配置中应注意的几个问题

要使专业音响达到优良效果，在配置时应按照建筑声学的要求，计算出音箱电功率，保证音箱与功率放大器匹配，同时要考虑声场带来的影响，做到准确定位，充分发挥出设备的最大功能。     

碳纳米管阵列推力器放电特性的数值模拟研究

基于直接蒙特卡洛(DSMC)算法、浸入式有限元算法(IFE)、粒子云及蒙特卡洛碰撞(PIC-MCC)算法以及Ammosov-Delone-Krainov(ADK)隧穿电离模型建立了碳纳米管阵列推力器工质气体和CNT场电离过程的三维仿真模型。利用文献中的实验数据对本文仿真模型的有效性进行了验证,结果表明本文仿真模型与实验结果基本一致。针对碳纳米管阵列推力器的放电特性进行了研究,并重点分析了离子与原子碰撞过程对碳纳米管阵列推力器放电特性的影响。结果表明CNT可以极大地增强局部电场,稳态时场增强因子约为1308;与原子的碰撞使得离子在CNT附近更加集中,降低了局部电场,进而降低了其场增强能力。     

惯性静电约束推力器放电过程数值模拟研究

为了研究惯性静电约束推力器(Inertial Electrostatic Confinement Thruster,IECT)的放电原理和工作机制,采用漂移-扩散流体模拟方法,基于圆柱形惯性静电约束推力器的结构,研究不同栅网线直径、栅网个数、推力器尺寸条件下等离子体放电情况和阴极电压、背景气压对推力器放电的影响。结果表明:在所研究条件下,保证阴极必要的几何透过率的同时,适当增加推力器栅网个数可以提高喷射离子密度,减小羽流发散角;随着阴极电压和背景气压的增大,推力器喷射的等离子体密度增大。但是,压强继续增大会达到临界值,等离子体被约束在推力器内部无法喷出,即喷射模式无法运行,故阴极电压与背景气压对IECT均有较大影响。