气膜内冷通道高度对气膜孔流量系数的影响

以一种基于旋流增益的强化换热技术为研究对象,对狭小受限的气膜孔内冷通道中气膜孔的流量系数开展了试验研究.试验中通过改变气膜孔雷诺数Re(4800～26000)、吹风比M(0.36～2.74)、无量纲冷却通道高度h/d(0.33～2.0)等参数,研究了狭小空间的几何结构、流动参数等对单排气膜孔平均流量系数Cd的影响,并得...     

脉冲周期介质阻挡放电作用的PIV实验研究

静止大气下,对施加脉冲周期介质阻挡放电,半顶角为10°的圆锥前体进行了PIV实验研究。采用总平均和相位锁定平均方法对脉冲周期放电进行了分析;对比了不同占空比和不同相位角沿θ=90°半径上的切向速度和轴向涡量分布,得到了在圆锥表面等离子体诱导的最大速度和最大涡量;分析了脉冲周期放电的动量转移特性。实验结果表明：脉冲周期放电引发动量转移的主要机制是涡的增强而非气流的加速;当激励器处于脉冲放电间歇时,相位锁定平均的最大速度和最大涡量不为零,存在流动滞后效应,有利于节省能耗。     

高频脉冲微细电火花加工放电通道形成过程

研究了微细电火花加工中,高频电磁场形成的强磁力箍缩效应对加工过程中放电通道扩张及放电通道位形变化的影响.计算了高频电磁场作用下,放电通道中带电粒子所受洛伦兹力的变化情况.通过理论分析与实验研究,推测了放电通道的形成过程,认为在高频电磁场中,放电通道在强磁力箍缩效应作用下产生的通道直径减小、能量密度增大等变化是微细电火花加工表面出现的一系列特殊现象的重要原因.     

电容放电式火工品点火电路参数设计与仿真

文章介绍了火工品电容放电式点火电路,阐述了电容充放电原理和充放电电路的参数计算方法;仿真分析了充电电压和储能电容等参数对点火电路放电性能的影响。通过仿真分析得出,合理选择储能电容和充电电压能够获得较好的点火性能。     

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.     

One-to-one relationship between low latitude whistlers and conjugate source lightning discharges and their propagation characteristics

One-to-one relation with its causative lightning discharges and propagation features of night-time whistlers recorded at low-latitude station, Allahabad (geomag. lat. 16.05°N, L = 1.08), India, from continuous observations made during 1–7 April, 2011 have been studied. The whistler observations were made using the Automatic Whistler Detector (AWD) system and AWESOME VLF receiver. The causative lightning strikes of whistlers were checked in data provided by World-Wide Lightning Location Network (WWLLN). A total of 32 whistlers were observed out of which 23 were correlated with their causative lightnings in and around the conjugate location (geom. lat. 9.87°S) of Allahabad. A multi-flash whistler is also observed on 1 April with dispersions 15.3, 17.5 and 13.6 s^1/2. About 70% (23 out of 32) whistlers were correlated with the WWLLN detected causative lightnings in the conjugate region which supports the ducted mode of propagation at low latitude. The multi-flash and short whistlers also propagated most likely in the ducted mode to this station.     

介质阻挡放电等离子体的温度测量

在空气介质阻挡放电中,利用氮分子振动谱线和氮分子离子的转动谱线,研究了振动温度和转动温度在两极板间的分布情况。结果表明：越靠近极板振动温度越小,中间振动温度最高;而转动温度在两极板间基本保持不变。     

液体火箭可贮存推进剂泄出速度影响因素分析

为提高液体火箭可贮存推进剂泄出速度，缩短泄出时间，通过分析泄出过程中推进剂流动状态及能量变化，建立了推进剂泄出速度的数学模型，按照实际设定参数计算了泄出量，计算结果与实际泄出吻合，并依据模型分析了相关因素对泄出速度的影响程度。结果表明：泄出转接波纹软管管径是影响泄出速度的主要因素，增加软管管径可显著缩短泄出时间；同时，贮箱气枕压力对泄出速度同样具有明显的影响。     

高空低气压下电晕放电电磁脉冲辐射特性模拟实验

为研究高空低气压下飞行器表面电晕放电电磁脉冲辐射特性,以尖端导体电晕放电为研究对象,进行了低气压下电晕放电电磁脉冲辐射特性模拟实验,给出了辐射电场幅值与气压的关系表达式,并基于气体放电和电磁场理论总结了电晕放电电磁脉冲辐射特性随电压极性、气压以及测试距离的变化规律。结果表明:电晕放电电磁脉冲辐射电场时域波形呈衰减振荡形式,持续时间约为600 ns,首脉冲方向随电压极性的不同而不同,且辐射电场分量主要集中在与放电针相同的极化方向;辐射电场频谱主要分布在500 MHz以内,在35 MHz和170 MHz处出现稳定的波峰;在气压为4~30 kPa范围内,随着气压的降低,放电电磁脉冲辐射电场增强;随着测试距离的增加,电晕放电电磁脉冲辐射电场逐渐衰减。该研究结论可为低气压下飞行器电晕放电电磁脉冲辐射特性研究提供有益参考。     

空间真空环境下密封电磁继电器的触点失效研究

密封电磁继电器有其固有的漏率,在应用于空间真空环境下由于气体泄漏使得其内部气体压力逐渐降低,导致继电器的触点在低气压环境下工作失效（负载切换时）。文章选择国产继电器样品对上述机理进行了试验验证,并对继电器内部气体压力与触点电弧失效的规律进行了研究。