铜基等离子体喷涂钨涂层性能

阐述了钨涂层微观结构影响机理以及涂层性能。通过等离子体喷涂工艺参数及微观形貌分析涂层微观结构和参数对涂层性能的影响,工艺参数主要包括喷涂功率、喷涂距离、送粉气量等。结果显示钨涂层是由钨粒子熔融沉积平铺成"圆饼状"或"花瓣状"的单层叠加而成,单层呈现柱状晶微观结构,厚度约10μm、直径约50μm的"圆饼状"单层是状态比较好的涂层结构。钨粒子熔化状态、沉积速率以及喷涂环境决定了熔化粒子的沉积形貌;与大气喷涂相比,真空喷涂钨涂层气孔率低、传热性能和结合性能较好,适合作为面对等离子体材料的制备技术。     

送粉方式对等离子喷涂NiCrAlY/ Al2 O3涂层介电性能的影响

以内送粉和外送粉两种方式微弧等离子喷涂工艺制备了NiCrAlY/Al_2O_3复合涂层,分析了送粉方式对涂层相组成、微观结构和介电性能的影响。结果表明:与外送粉相比,内送粉方式沉积的涂层具有较高的沉积效率和较低的孔隙率。由于喷涂过程中α-Al_2O_3颗粒完全熔融,内送粉喷涂所得到涂层主要为γ/γ′和γ-Al_2O_3相,并且涂层结构致密,NiCrAlY颗粒分布均匀。介电性能测试表明,以外送粉方式制备的涂层复介电常数实部和虚部几乎不随频率发生变化。而以内送粉方式喷涂的涂层复介电常数实部和虚部随频率的增加而降低,呈现明显的频散现象。     

等离子体点火与助燃技术在航空发动机上的应用

等离子体点火与助燃技术是能源与动力领域的研究前沿。介绍了等离子体点火与助燃技术的研究背景和意义,分析了其基本原理,给出了常见的等离子体点火与助燃的类型,阐述了等离子体通过热强化、动力学强化与输运强化3种强化燃烧机制,利于点火助燃。针对国内外等离子体点火与助燃技术在航空发动机上的研究现状,提出了预燃式等离子体射流点火和旋转滑动弧助燃2种新型等离子体点火助燃方案,对等离子体点火与助燃技术在航空发动机上的实际应用进行了展望。     

利用栅网控制空间等离子体环境效应模拟中的等离子体参数

通常采用ECR等离子体源产生的等离子体的温度和密度都比较大，通过附加适当目数的栅网，并在栅网上加一定的偏置电位来对等离子体参数，尤其是温度，密度进行调整，满足空间等离子体环境模拟要求，本文利用14目，25目的栅网，对已有的地面实验室空间等离子体环境进行了改进，得到了更加接近空间等离子体参数的一个地面模拟环境。     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

An empirical model of the plasma environment around Mercury

Since the flyby observations by Mariner 10 in 1974 and 1975, Mercury has been one of the most interesting objects for space physics and planetary exploration. The MESSENGER and BepiColombo missions now plan to revisit this planet. In order to design plasma instruments for the BepiColombo mission, we have estimated electron and ion fluxes around Mercury with an empirical model, which has been developed for the Earth’s magnetotail. The solar wind data needed as input parameters are derived from Helios observations. The result shows that our predicted electron fluxes at aphelion agree well with the Mariner-10 data. It is also noted that ion instruments must cover a very wide dynamic range of proton fluxes. However, the applicability of the Earth’s magnetospheric model to Mercury is, in itself, an important issue for comparative magnetospheric studies.     

Understanding Substorms in the Magnetotail: Early Development and Recent Progress

This is a concise review of physics of the substorm in the magnetotail. It consists of two parts. The first part summarizes historical developments in the early days of the space age (1960--1975) when the basic concepts such as magnetotail and reconnection were established and the leading model of the substorm was introduced. The second part is an overview of the research conducted in recent years (1995--2010) when very significant advances have been achieved in understanding the substorm physics by virtue of several major satellites missions that addressed the magnetotail physics intensively.      

低轨道航天器高电压太阳电池阵电流泄漏效应分析计算

在一种简化的太阳电池阵结构模型基础上, 利用太阳电池阵电流收集经验模式,基于电流平衡, 建立了一种计算低轨道航天器高电压太阳电池阵在等离子体环境中电流泄漏的方法. 利用该方法, 对高电压太阳电池阵电流泄漏效应与低轨道等离子体环境、电池阵电压、电池阵裸露金属面积的关系进行了分析计算.结果表明, 随着轨道高度增加, 电流泄漏引起的电池阵功率损失迅速下降, 影响最严重的区域为电离层等离子体密度最高的300～400 km高度的轨道区域; 电流泄漏引起的功率损失与太阳电池阵电压呈指数关系, 电压越高功率损失越大; 200 V以下的电池阵功率损耗较小, 远低于电源系统总功率的1%;电流泄漏与太阳电池阵裸露金属导体的表面积呈正比关系, 因此, 通过减少太阳电池阵裸露面积, 可以降低电流泄漏的影响.      

减压直流非转移弧等离子体射流速度的静电探针测量

组建了一套利用静电探针诊断技术测量减压直流非转移弧等离子体射流速度的实验系统。对以纯氩为工质的等离子体,在气流量1．25×10^-1kg/s、弧电流80A、真空室压力165Pa的条件下,测量了射流的速度及其分布。结果表明射流在发生器出口处中心最高速度约为1200m／s,在半径20mm处减小到635m／s。沿射流轴线方向的速度梯度约为10（ms^-1）／mm。射流速度随着弧电流增加而缓慢单调增加;当真空室压力从165Pa提高到2kPa时,发生器出口轴线上的射流速度从1200m／s降至570m／s。     

2006年4月5日中等强度磁暴期间观测到的大经度范围等离子体泡

利用分布在70°E～210°E和20°S～40°N之间的GPS台站的数据,分析了2006年4月5日夜间(中等强度磁暴期间)观测到的电离层等离子体泡的特性.结果表明,本次事件中,等离子体泡大约发生在当地日落后1～1.5 h;空间范围为经度90°E～160°E,纬度12°S～33°N.这是第一次利用地基设备观测到如此大经度范围内的等离子体泡.等离子体泡在南半球出现较早,并且存活时间较长.在其产生的过程中,在约1100 km高度上,映射到磁赤道向上的运动速度约为300m/s,并且等离子体泡在高度上有倾斜.东向电场的存在,对激发等离子体泡起到了一定的作用.