混合动力学中一种综合控制指标

本文从环境流体力学角度，结合混合动力学机理，导出了一种新混合综合控制指标。     

中国空间大功率微波部件微放电抑制表面处理技术最新进展

材料表面的二次电子发射会触发和维持空间高功率射频器件的共振雪崩放电现象,这种现象又被称为微放电效应。微放电效应是限制空间大功率微波部件应用的关键问题之一。从微放电作用的机理出发,首先介绍了两种微放电类型（单表面与双表面）的基本物理机理;然后总结了当前主流的微放电抑制方法并给出各自应用于空间大功率微波部件时的限制。针对空间大功率微波部件微放电抑制的特殊问题,综述了国内近5年来在表面处理法抑制微放电领域的研究成果并预测了微放电抑制技术的发展趋势。     

电动式磁悬浮动量球电磁场耦合分析

本文针对电动式磁悬浮动量球(Electrodynamic suspension reaction sphere, EDSRS)的电磁场耦合进行分析，采用定子绕组的感应电动势评判耦合强度，提出了耦合强度评判指标，作为EDSRS的结构设计约束，以降低电磁场耦合的影响。首先，结合EDSRS的具体结构特点，对多定子之间的电磁场耦合问题进行分析，采用定子电磁场在另一个定子绕组中产生的感应电动势评判耦合强度。然后，对感应电动势产生规律进行分析，提出了耦合强度评判指标，并基于所提评判指标，建立了耦合约束验证流程，作为EDSRS的结构设计约束，最后，通过有限元仿真和实验验证了上述电磁场耦合分析。     

微阴极真空电弧点火起弧及加速机理研究综述

微阴极真空电弧推力器具有结构简单、重量轻、功耗低、比冲高等优点，因而在航天推进领域有着广阔应用前景.当前推力器设计研制、可靠性和寿命的提高等方面遇到的一些关键问题均与微阴极真空电弧放电过程的基本物理问题密切相关.对微阴极电弧推力器运行中涉及的电子发射、电极间起弧过程、阴极斑点形成及特点、烧蚀和形貌变化、电极间等离子体射流加速过程进行了梳理，相关认识可以为今后进一步开展微阴极电弧推力器的设计优化、性能提高奠定基础.     

失效概率矩独立全局灵敏度分析的高效算法

失效概率矩独立全局灵敏度分析对指导可靠性优化至关重要，本文从乘法降维及Edgeworth级数展开的角度提出一种失效概率矩独立全局灵敏度指标分析的高效算法。所提算法通过Edgeworth级数展开将失效概率矩独立全局灵敏度指标的求解转化为输出无条件及条件前四阶整数矩的求解。对于输出的无条件及条件四阶矩的计算，基于乘法降维的思想，本文推导了重复利用计算输出的无条件矩的输入输出样本来计算条件矩以及外层关于输入变量一维积分的计算公式，使得仅需重复利用输出无条件前四阶矩求解产生的积分网格内的数据即可同时求得输出的前四阶条件矩以及外层关于输入变量的一维积分。所提算法大大提高了失效概率矩独立全局灵敏度的分析效率。航空发动机涡轮盘以及汽车前轴的分析结果验证了所提算法的高效性及准确性。     

L-band nighttime scintillations at the northern edge of the EIA along 95°E during the ascending half of the solar cycle 24

The characteristics of nighttime ionospheric scintillations measured at the L-band frequency of 1.575 GHz over Dibrugarh (27.5°N, 95°E, MLAT ～ 17°N, 43° dip) during the ascending half of the solar cycle 24 from 2010 to 2014 have been investigated and the results are presented in this paper. The measurement location is within or outside the zone of influence of the equatorial ionization anomaly depending on solar and geomagnetic activity. Maximum scintillation is observed in the equinoxes irrespective of solar activity with clear asymmetry between March and September. The occurrence frequency in the solstices shifts from minimum in the June solstice in low solar activity to a minimum in the December solstice in high solar activity years. A significant positive correlation of occurrence of scintillations in the June solstice with solar activity has been observed. However, earlier reports from the Indian zone (～75°E) indicate negative or no correlation of scintillation in June solstice with solar activity. Scintillations activity/occurrence in solstices indicates a clear positive correlation with Es recorded simultaneously by a collocated Ionosonde. In equinoxes, maximum scintillations occur in the pre-midnight hours while in solstices the occurrence frequency peaks just after sunset. The incidence of strong scintillations (S₄ ≥ 0.4) increases with increase in solar activity. Strong (S₄ ≥ 0.4) ionospheric scintillations accompanied by TEC depletions in the pre-midnight period is attributed to equatorial irregularities whereas the dusk period scintillations are related to the sporadic-E activity. Present results thus indicate that the current location at the northern edge of the EIA behaves as low as well as mid-latitude location.     

高校委托工程审计的质量控制与评价指标体系构建

委托工程审计质量关系到高校工程审计职能的发挥和投资建设目标的实现.结合高校工程审计实践,探讨高校委托工程审计质量控制关键路径,并据此构建质量评价指标体系,以实现高校委托工程审计质量有效控制和科学评价.     

1992年10月27日耀斑的多波段观测和分析

利用１９９２年１０月２７日耀斑极为完整的高质量观测资料,通过对可见光、软Ｘ射线和硬Ｘ射线图像和光谱的综合分析,诊断耀斑过程中的热与非热性质,结果表明,在这个事件中,热与非热过程并存且在时空演化上呈现不同的特征     

复杂产品研制项目标准化效益评估模型

旨在量化计算标准化工作的效益,凸显标准化工作的重要作用.通过分析复杂产品研制项目标准化工作的特点,确定标准化工作权重计算方法,建立了复杂产品研制项目标准化工作项目体系及效益指标体系.深入研究复杂产品研制项目标准化效益评估模型的构建方法,编制总效益调研问卷,收集有关型号标准化工作效果数据,构建了复杂产品研制项目标准化效益评估模型.运用本方法建立了航空领域复杂产品研制项目标准化效益评估模型,并以某型飞机研制项目的真实数据验证了模型的准确度.     

Structure of the Program of Short-term Prediction of Powerful Solar Flares

Input data of the system are two-dimensional images and one-dimensional distributions of total and polarized solar emission at 5.2 cm wavelength obtained with SSRT. Together with photoheliograms, magnetograms, Hα-filtergrams and characteristics of active regions received from other sources, they form the initial database. The first stage includes superimposing the images, identifying microwave sources with active regions, assigning NOAA numbers to the sources, and determining for each active region the heliolatitude, extent, and inclination angle of the group's axis to the equator. These data are used to calculate the boundaries of longitude zones for each active region. A next stage involves determining the brightness temperatures of microwave sources less than the polarization distribution, the degree of polarization, and microwave emission flux, as well as calculating the parameters of microwave sources. Each parameter is assigned its own value of the weight factor, and the sum of values is used to draw the conclusion about the flare occurrence probability in each active region and on the Sun in general.