高超声速尾迹雷达散射湍流场研究

为给高超声速再入尾迹亚密湍流雷达散射分析提供所需的脉动背景场参数 ,本文提出计算非平衡再入湍流尾迹脉动等离子体场的理论方法。在研究高超声速尾迹流动特征的基础上 ,推导、使用包括化学组份浓度脉动强度的k ε g湍流模型 ,用以封闭高超声速尾迹雷诺平均控制方程 ,并用全隐式有限差分求解。以M∞ =2 1 .2 6、Re∞D =1 .33× 1 0 6的小钝锥体流动为例 ,得到的结果说明 :流场的流向和径向参数分布合理 ;在转捩点后较近距离内湍流脉动影响较大 ,随着向下游流动脉动影响迅速减弱 ;本文计算尾迹湍流脉动等离子体场的方法是可行的     

K417合金缓进磨削烧伤表面形貌及形成机理

本文在严格控制的实验条件下,建立了磨削弧区温度同试件表面烧伤色之间的对应关系;并以扫描电镜(SEM)、电子探针(EPA)等较为先进的测试仪器为手段详细研究了K417镍基铸造高温合金缓进磨削中表面为正常、淡黄、黄褐、紫褐以及紫黑等深浅不同的色斑时诸试件表面形貌特征和对应的砂轮表面形貌特征,揭示了K417材料缓磨中表面形貌的变化特征及其形成机理。测试结果表明,K417材料缓磨表面出现烧伤色斑时,磨粒与试件材料之间存在粘结现象;试件表面出现粘结滞留的涂覆物。随表面烧伤色层次的加深,磨粒与试件材料之间的粘结越普遍、越严重,试件表面涂覆程度亦越强烈。当出现紫黑色斑时,表面还伴有微裂纹出现。     

非麦氏电子分布对霍尔推力器等离子体与壁面相互作用的影响

为深入分析霍尔推力器放电通道的非麦氏电子分布对等离子体与壁面相互作用的影响,采用一维非稳态鞘层动力学模型,统计了等离子体与壁面相互作用的重要物理量。结果表明,非麦氏电子分布函数和麦氏电子分布函数下等离子体与壁面相互作用存在很大差异,电子服从非麦氏电子分布时入射电子在壁面上的能量沉积,以及二次电子对主流区电子的冷却作用都明显弱于电子服从麦氏分布的情形。     

高超声速钝体尾流的积分电子密度与尺寸度律

本文提出了一个高超声速非烧蚀钝体化学非平衡尾流流场的简化模型和简化的空气化学模型。应用该模型计算尾流的积分电子密度。计算结果与实验数据符合得很好。在此基础上,以P_∞D_N=375mmHg·mm为例,初步论证了尾流双尺度律的适用程度与范围,为弹道靶模型实验提供正确的导向。     

太阳同步轨道电子探测器的多方向设计研究

为实现观测电子投掷角分布的目标,本文讨论了太阳同步轨道三轴稳定卫星电子观测的多方向设计。分析了磁层电子投掷角分布特征,并根据太阳同步轨道卫星的轨道参数,计算得到卫星运行轨迹上,三个探测器常用安装面正入射粒子的投掷角。在此基础上,进行电子探测器的探测方向设计,结果表明探测器要在任何安装面都满足投掷角观测要求,至少需要在0°、10°、20°、25°、35°、45°、70°、80°和90°共9个方向上设计探测窗口。     

Night-time total electron content enhancements at equatorial anomaly region in China

This paper presents small scale (duration ?1 h, ΔTEC ? 1TECU) night-time total electron content (TEC) enhancements observed at the equatorial anomaly region in China, for the first time. The data is from a GPS receiver chain established in 2005 by Institute of Center for Space Science and Applied Research, Chinese Academy of Sciences and a GPS receiver of International GPS Service (IGS), located between Fuzhou (26.1°N, 119.3°E) and Nanning (22.8°N, 108.3°E). Two other GPS observations of IGS taken at higher latitude were also used to investigate the localization of such phenomenon. The characteristics of the night-time TEC enhancement are examined with two case studies. The TEC increases about 1–3TECU, intermittently. While the night-time TEC enhancement mainly occurs at the equatorial anomaly region, it can be observed at middle latitude as well. The spatial size of the enhancement region is less than 5° in longitude. The primary statistical study shows that the TEC enhancement is more often observed in spring and autumn, but rarely in summer. It has no dependence on geomagnetic activity. The enhancement can occur both before and after midnight.     

The effect of total solar eclipse of October 3, 2005, on the total electron content over Europe

GPS observations from EUREF permanent GPS network were used to observe the response of TEC (Total Electron Content) to the total solar eclipse on October 3, 2005, under quiet geomagnetic conditions of the daytime ionosphere. The effect of the eclipse was detected in diurnal variations and more distinctly in the variations of TEC along individual satellite passes. The trough-like variations with a gradual decrease and followed by an increase of TEC at the time of the eclipse were observed over a large region. The depression of TEC amounted to 3–4 TECU. The maximum depression was observed over all stations located at the maximum path of the solar eclipse. The delay of a minimum level of TEC with respect to the maximum phase of the eclipse was about 20–30 min.     

RPC-MIP: the Mutual Impedance Probe of the Rosetta Plasma Consortium

The main objective of the Mutual Impedance Probe (MIP), part of the Rosetta Plasma Consortium (RPC), is to measure the electron density and temperature of Comet 67P/Churyumov-Gerasimenko’s coma, in particular inside the contact surface. Furthermore, MIP will determine the bulk velocity of the ionised outflowing atmosphere, define the spectral distribution of natural plasma waves, and monitor dust and gas activities around the nucleus. The MIP instrumentation consists of an electronics board for signal processing in the 7 kHz to 3.5 MHz range and a sensor unit of two receiving and two transmitting electrodes mounted on a 1-m long bar. In addition, the Langmuir probe of the RPC/LAP instrument that is at about 4 m from the MIP sensor can be used as a transmitter (in place of the MIP ones) and MIP as a receiver in order to have access to the density and temperature of plasmas at higher Debye lengths than those for which the MIP is originally designed.     

基于CHC算法的无人机航迹规划方法

利用改进的遗传算法——跨世代异物种重组大变异(CHC, Cross generation Heterogeneous recombination Cataclysmic mutation)算法提出了一种无人机的航迹规划方法.初始种群即初始航线集利用具有启发式信息的搜索算法产生;适应度函数为距离指标与威胁指标的组合形式;选择操作群体为当前群体与上世代群体的群体总和,由于大个体群操作,可以更好地保持遗传多样性;交叉操作采用单点交叉方法,交叉点取为2条航线中距离最近的2个点;变异操作的步骤是:首先在航线中搜索出2个点,然后算出这2个点之间的直线距离与实际航线距离的比值,如果这个比值小于某一阈值则以这2个点为端点重新规划一条航线.由于考虑到了无人机约束条件的限制,从而避免了盲目性且加快了收敛速度.仿真结果表明该方法比基本遗传算法要快而且满足最优条件.      

电子束固化环氧树脂的引发和增长反应速率

对二苯基碘 鎓 六氟磷酸盐引发的环氧树脂电子束(EB)辐射固化反应动力学进行了研究,应用环氧树脂乙腈溶液推导出引发剂辐射分解速率常数和引发、增长反应速率.动力学研究结果表明,二苯基碘 鎓六氟磷酸盐引发剂经电子束辐射分解产生质子酸的过程是二级反应,在辐射反应过程中,环氧树脂体系的引发速率和增长速率分别迅速达到最大值后逐渐减小.