介质阻挡体放电对甲烷扩散火焰CH*自发辐射影响实验研究

为分析非平衡等离子体对空气/甲烷扩散火焰的助燃效果,实验以发射中心谱线430nm的激发态自由基CH*表征火焰燃烧状态,采用同轴圆柱构型激励器在高频交流模式下激发等离子体,分析了火焰CH*自发辐射图像、火焰高度、CH*径向分布和燃烧释热速率等火焰特性在不同空气流量和当量比下随放电电压的变化规律。结果表明：等离子体激励在空气流量较低时,会显著增强火焰上游甲烷燃烧,从而降低CH*空间分布高度和火焰高度;空气流量增大后,有利于促进甲烷充分燃烧,增大火焰下游CH*辐射强度和分布范围。在火焰上游区域,等离子体气动效应可有效扩展甲烷径向分布,实现剪切层更宽范围燃烧,其活化效应会明显提高剪切层燃烧强度,并随电压增大作用效果逐渐增强。此外,等离子体激励会使燃烧器喷嘴出口附近火焰释热速率显著增大,该现象在空气-甲烷动量比较大时更容易发生。     

Possible evidence for small-scale wave seeding of equatorial plasma bubbles

The small-scale wave-like structure (SSWS) of F region bottomside plasma density was proposed to be an important seeding for equatorial plasma bubble (EPB) generation, and employed in theoretical simulations of EPBs in recent years. The seeding role of SSWS, however, is waiting to be demonstrated by observation. Here we present two cases of SSWS and EPB observed by the Fuke all-sky airglow imager (19.3°N, 109.1°E; dip latitude 14.3°N). For each case, the results show that two large-scale wave-like structures (LSWSs) initially appeared around sunset in the longitude regions separated by 3–4°, but EPB irregularities were only generated in one of the LSWSs where SSWSs were seen riding on LSWS. For the other LSWS, no SSWS and EPB irregularities were seen. Considering that the two LSWSs were situated closely in longitude where the amplitude of pre-reversal enhancement of background eastward electric field should be similar, the observation that EPB was only generated in the longitude with simultaneous LSWS and SSWS could provide supporting evidence for SSWS seeding of EPB.     

航空装备综合诊断的现状与发展设想

综合诊断是伴随着装备的发展和对装备保障能力的要求不断提高而产生和发展的,为此将国外航空装备综合诊断技术的发展历程以及各综合诊断系统的具体组成进行了对比,阐述了当前我国航空装备故障诊断的情况,分析了综合诊断的支撑技术和发展趋势,提出在我国航空装备的维修保障中实施综合诊断的必要性,并对我国建立面向多机型、多专业、以网络为中...     

高阶矩谱分析与空间等离子体非线性相互作用识别

利用高阶矩统计分析方法对ＡＵＲＥＯＬ－３卫星观测数据进行分析处理，所涉及的信号分别为ＥＬＦ频率范围内的电场扰动Ｅｈ（ｔ）和等离子体密度波动δＮｅ／ｎｅ（ｔ），处理结果表明：利用高阶矩谱分析方法可以很好地识别空间等离了波－粒相互作用过程中的非线性成分     

用于合成金刚石薄膜的微波等离子体CVD系统

研制了一套功率容量大、结构合理、工作稳定的微波等离子体ＣＶＤ系统。描述了系统的基本结构和性能，讨论了它的特点。作者利用该系统，在单晶Ｓｉ等衬底材料上成功地合成了金刚石薄膜。     

The energy release of substorm and magnetic storm: Its present state and future improvements by KuaFu mission

Considering the KuaFu mission, state of the energy release of substorm and storm is simply presented and it’s improvements by KuaFu mission are investigated. The KuaFu mission will provide us an opportunity to improve our understanding of the energy release during the storm and the substorms. The two KuaFu-B satellites flying in 180° phase-lagged formation in a polar orbit will allow synoptic observations of the auroral oval, central plasma sheet, ring current and other regions. It can monitor the polar region 24/7 continuously. The advantage of the KuaFu mission is to provide the data during all phases of storm and substorm time that can be used to study the global energy release during all phases continuously. The data from auroral imager and other in-situ instruments on board KuaFu-B can be used to study the auroral dynamics and Joule heating during a storm and substorm. The data from the neutral atom imager instrument can be used to study the dynamics and the energy release in the ring current region from sudden commencement to complete storm recovery. Furthermore the data from KuaFu-A, which is around L1 point, can be used to study the interplanetary conditions along with the data from the plasma sheet to study the triggering process and energy release during a substorm. So, KuaFu mission with its continuous time monitoring facilities would enable us to make much progress towards solving the underlying problems.     

NS-DBD激励控制非细长三角翼前缘涡仿真研究

通过在三角翼前缘施加纳秒脉冲介质阻挡放电（NS-DBD）激励唯象学模型,进行了47°后掠角钝前缘三角翼流动控制的仿真。分析了不同迎角下升力和阻力系数的变化、流场结构的变化、以及激励诱导旋涡的演化过程。研究表明:施加无量纲激励频率F+=1.44的NS-DBD激励后,可明显提高三角翼失速前后的升力系数;同时阻力系数也有所增加,变化趋势与实验结果一致。激励在前缘分离剪切层处诱导产生流向涡,改变了前缘剪切层结构,使其向内卷吸;激励后时均流场形成了明显的负压峰值,前缘涡附着线外移,吸力面回流区减小。      

两种翼型螺旋桨ARA-D和S1223的等离子体增效实验研究

文章首先基于雷诺相似理论,在地面螺旋桨实验平台上开展ARA-D翼型螺旋桨微秒脉冲等离子体增效三维实验,结果表明,等离子体对螺旋桨拉力增效效果随着脉冲频率增加而减弱,而螺旋桨转矩受等离子体影响随拉力增效效果增加而减弱,拉力、效率最大增幅分别达到10.79%、11.56%。而后基于雷诺相似理论及叶素理论,在低湍流度风洞开展S1223翼型螺旋桨叶素微秒脉冲等离子体增效二维实验,结果表明等离子体激励提高了翼型各叶素拉力,其中根部与尖部叶素表现尤为明显。二维实验结果可为三维实验激励器展向排布方案提供理论依据。2种实验结果均表明,等离子体射流可以有效抑制翼型表面流动分离。     

TiAl合金粉末射频等离子体球化过程数值模拟

采用数值模拟的方法对TiAl合金粉末的射频(radio frequency)等离子体球化过程进行研究,分析速度场和温度场对不同粒径TiAl合金粉末的运动轨迹及质量变化的影响。结果表明:粉体颗粒在等离子体的高温作用下温度急剧升高,表面蒸发导致粒径降低,太小的颗粒很快蒸发消失掉;在冷却塔下端,不同粒径颗粒的运动轨迹存在较大差异,小颗粒倾向于随气流进入气流出口,大颗粒落到冷却塔底部被收集;增大气流量会提高球化系统中的气流速度,导致在气流出口能被气流带走的颗粒粒径变大,收粉率降低;模拟得到TiAl合金粉末球化后的粉末粒径分布、平均粒径及收粉率等参数与实验结果比较接近,模型能够较好地符合实际球化过程。