引导场对无碰撞电流片低频电磁不稳定性的影响

通过数值求解无碰撞电流片中可压缩磁流体力学模型下得到的一般形式的色散关系,讨论了无碰撞电流片中引导场对低频电磁波不稳定性的影响.结果表明,平衡态磁场中的引导场,对于三维扰动传播的波不稳定性有很强的影响.(1)在电流片中间平面上(z=0),无引导场时,没有不稳定性发生,但若存在引导场,不稳定性便发生,并随着引导场的增强,不稳定性明显增强,不稳定的波模可能是低混杂模.(2)在中间平面附近(z=0.2),电流片是不稳定的.随着引导场的增强,不稳定性增长率明显地增强,不稳定的波模从平行和反平行两个方向传播变为反平行方向一个方向传播,并且是斜传播的,具有低频哨声模或低混杂模的特征.(3)在电流片边缘附近(z=0.8),引导场对不稳定的波模和增长率没有明显影响,不稳定的波模都是准平行的哨声波.      

直流电弧等离子体炬数值模拟与诊断

直流电弧等离子体炬内部物理过程复杂且具动态性,较难对其进行准确描述与深入研究,且其工作温度较高,其状态参数难以使用常规方式测量。针对直流电弧等离子体炬,建立流动、传热和电磁相互耦合的数值模型,基于Fluent软件对直流电弧等离子体炬进行三维数值模拟和特性分析,设计并搭建了一套热焓探针实验系统,完成对直流电弧等离子体炬射流参数的测量分析。结果表明:建立的数值模型模拟结果与实验测量结果吻合较好,误差在10%以内;炬内温度与速度最大值与工作气流量呈正相关,均出现在靠近阴极区域,且沿轴线逐渐降低;等离子体炬内高温区与高电流密度区重合。     

黄海气象海况对海上发射运载火箭的影响

海上发射运载火箭的实施过程会受到气象海洋环境的影响和制约,气象海洋环境会直接影响海上发射窗口期的选择及发射安全。为避免海上发射在复杂气象海况条件下发生设备重大损坏、窗口长期延后和人员安全事故等问题,通过分析黄海海域波浪场、风场、温度场及降水场的分布特征及变化规律,对基于季节变化特征的海上发射实施阶段及季节性预防趋势进行分析总结,为以后在不同季节极端天气下海上发射运载火箭提供参考。     

比例式变推力固体姿控发动机非稳态特性研究

为了研究比例式变推力固体姿控发动机的内流场非稳态特性,建立了比例针栓推力器的二维轴对称计算模型,基于动网格技术模拟入口压强随喉部面积变化而变化的推力器工作模式,得到了内流场各性能参数的变化规律。结果表明:在非稳态工作过程中,内流场会出现典型的亚音速回流区、斜激波和流动分离等特征,入口压强、针栓壁面及喷管壁面压强均随针栓靠近喉部而增大,推力器推力逐渐上升,实现了推力连续调节。开关频率会加剧针栓前进过程中头部压强波动。针栓头部收敛角越大,其头部回流区越小。当喉部面积一定时,燃速压强指数越高,发动机压强与推力变化范围越大,为实现预设的推力调节范围,需要选择合适的燃速压强指数。     

Flow field characteristics,mixing and emissions performance of a lab-scale rich-quench-lean trapped-vortex combustor utilizing a quench orifice plate combined with a bluff-body

In this study, the low emission combustion technology of Rich-Quench-Lean (RQL) has been applied in Trapped-Vortex Combustor (TVC), and the combinative RQL-TVC shows a promising low emissions performance. By utilizing a quench orifice plate combined with a bluff-body, a lab-scale RQL-TVC was designed. The flow fields of RQL-TVC were measured by 2-D PIV and predicted by 3-D numerical simulation. Flow structures, radial profiles of normalized mean axial velocity, turbulence intensity and mixing level of the quench zone were analyzed. Results reveal that the dual-vortex and the single-vortex flow patterns both exist in cavities and quench zone of RQL-TVC, and the turbulence intensity is strong in the quench zone with some reverse flows. The spiral vortex was discussed by 3-D streamlines and the detail flow structures of the quench zone were analyzed based on the numerical results. The mixing level of the quench zone was determined, and results show that the quench device enhances the mixing level compared with TVC. Combustion efficiency and emissions performance were investigated experimentally, and results demonstrate that RQL-TVC has relatively higher combustion efficiency and lower emission index of CO, UHC and NO_x than the same size lab-scale TVC in present work.     

某型发动机进口压力畸变实验研究与分析

发动机进口流场畸变是影响发动机稳定性的一个很关键的降稳因子,而进口压力场周向分布不均匀对燃气涡轮发动机的稳定工作范围有很大影响.通过对某型涡喷发动机进行进口压力畸变模拟实验,探讨了发动机进口流场压力畸变的实验程序和方法,通过对实验数据的分析和处理,确定了该型发动机的稳定性对进气压力畸变的敏感程度.     

直升机附件舱温度场的数值模拟

为考查某型直升机附件舱的热控制能力,采用有限元软件分析了其在强制冷却和自然冷却情况下的温度场分布.应用非结构化网格和有限体积法进行计算区域和控制方程的离散,采用标准k-ε模型封闭湍流控制方程.针对3种冷却系统设计方案,分析了不同冷却气流进口尺寸、相对位置以及不同附件散热量对附件舱温度分布的影响,计算了自然冷却情况下附件舱密闭时的温度场.计算和试验结果均表明,所采用的冷却方案可以满足附件舱冷却的需要.      

单一压力容器镍氢电池组几何参数对其温度场的影响

 针对实际空间用单一压力容器(IPV)镍氢电池组的传热特点,建立其瞬态热分析的数学物理仿真模型。通过设计改变电池组几何参数,包括电池组底板厚度、套筒高度和厚度,采用有限差分法,对比模拟研究电池组在飞船实际运行条件下几何参数对其温度场的影响。结果表明：套筒厚度对电池组温度场的影响最为敏感,增大套筒厚度可明显缩短电池组热系统达到平衡态的响应时间;其次是套筒高度;改变底板厚度对电池组温度场变化影响不明显。该研究为镍氢电池组的结构优化和热控制研究提供理论基础。     

温度对磁屏蔽霍尔推力器磁场构型的影响研究

霍尔推力器磁路设计主要通过常温静态磁场仿真得到，并实测推力器非工作状态常温磁场进行复核。大功率霍尔推力器将面临更为严峻的热问题，推力器工作时磁路系统受高温影响，因此在常温下仿真得到的磁场位形会因温度升高而产生偏移，不能反映推力器真实工作时的磁场情况。为研究霍尔推力器工作时热量对磁路系统的影响，通过热磁耦合仿真对10kW磁屏蔽霍尔推力器的热态磁场分布进行研究，并对热态、常温仿真结果进行了对比，发现在阳极附近的径向磁感应强度Br的差异比放电室出口更大。常温设计的磁屏蔽构型在热态时偏离磁屏蔽，磁场和壁面最大不符合度达到13%，通过陶瓷出口型面修正后重新获得磁屏蔽效果，使最大不符合度降低到4.8%以下。合理热设计有助于降低热载荷，热仿真得到磁路系统最高温度低于500℃，低于0.78倍的居里温度Tc磁性急剧转变点，不会出现磁性能急剧下降，但热量对磁屏蔽霍尔推力器磁场构型的影响是应该考虑的。     

Observations of the local interstellar medium with the Extreme Ultraviolet Explorer

Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm^–3 while the H II density ranges between 0.0 and 0.14 cm^–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm^–3 K, a factor of 2 to 3 above previous estimates.