Finite Larmor radius effects in the magnetosphere

This article reviews theories and observations related to effects produced by finite (and large) Larmor radii of charged particles in the magnetosphere. The FLR effects depend on =r _H /L, wherer _H is the Larmor radius andL is the spatial scale for field/plasma inhomogeneity. The parameter is a basic expansion parameter for most equations describing plasma dynamics in the magnetosphere. The FLR effects enter naturally the drift approximation for particle motion and represent also non-ideal MHD terms in the fluid formalism. The linear and higher order terms in lead to charge separation, energization of particles, and produce viscosity without collisions. The FLR effects introduce also important corrections to the dispersion relations for MHD waves and drift instabilities. Expansion of plasma into magnetic field leads to filamentation of the plasma boundary and to creation of structures with thickness less than an ion gyroradius. Large Larmor radius effects (1) in curved magnetic field geometry lead to stochastic behaviour of particle trajectories and to deterministic chaos. The tiny scale of the electron and ion gyroradii does not necessarily mean that FLR/LLR phenomena have negligible effect on the macroscopic dynamics and energetics of the whole magnetosphere. On the contrary, the small scale gyro-effects may provide the physical mechanism for gyroviscous coupling between the solar wind and the magnetosphere, the mechanism for triggering disruption of the magnetotail current layer, and the mechanism for parallel electric field that accelerate auroral particles.     

新一代引射式跨音速风洞（IDT）高要求指标的研究

 本文介绍了北京航空航天大学IDT-1甲型引射式前导性跨音速风洞的研究工作,包括风洞实验段动态气流品质及引射效率（G_T/G_j）等方面。在采取了多种技术措施后,表征实验段脉动压力的参数值达到或接近Lowson公式和Mabey准则所给出的值,使风洞这类性能进入世界同类研究的先进行列。引射效率和气流的湍流度也达到相当好的水平。实验研究还表明引射驱动方式应用于跨音速风洞具有光明的前景。     

爪型泵转子理论型线计算机模拟研究

本文针对爪型泵转子的理论型线进行了分析研究。运用计算机手段对转子的理论型线进行了计算与模拟，通过程序计算出型线的点坐标值，并运用计算机动画模拟仿真了转子的旋转啮合过程。     

电磁继电器转换电压测试方法的研究与应用

研究了一种新的电磁继电器转换电压的测试方法,这种测试方法引入了自反馈控制的原理,对于提高电磁继电器的测试速度,简化测试引线,减小测试误差都具有突破性的意义,更有利于电磁继电器的可靠性质量保证工作。     

航天用系列行波型超声波电机的研制

简述了超声波电机在航天领域的应用情况，并介绍了所研制的系列行波型超声波电机（直径分别为80mm、60mm、45mm和30mm）的结构形式、摩擦材料、粘结工艺、温度特性、机械特性和瞬态特性，提出了神经元自适应PID算法实现高精度的速度和位置控制。结果表明其具有良好的特性，适用于空间机器人、登月车、太阳能帆板、CCD等空间机构的驱动，并结合航天领域的应用要求，提出了下一步的研究重点。     

二阶中立型方程周期解的存在性

利用Ｆｏｕｒｉｅｒ级数理论研究二阶常第数线性中立型方程的周期解，得到了在｜ｃ｜＝１的条件下，二阶中立型方程周期解存在的充要条件；在｜ｃ｜＝１条件下，方程周期解存在的充分条件，并给出了具有特殊时滞的方程周期解存在的充分条件。     

大功率微波部件多载波无源互调分析与实验验证

无源互调是通信系统不可避免的问题，随着卫星载荷技术向更高功率、宽频段、高灵敏度接收方向发展，无源互调对通信系统造成的影响更加严重。常用的双载波分析评价无源互调已经不能适用于现代复杂载荷通信系统，提出确定多载波无源互调分布类型分析与计算方法，采用非线性模型计算多载波无源互调功率电平。通过对TNC双阴连接器的分析计算可得到接收频带内产生3个互调频率点，对比非线性模型计算的互调功率电平与多载波实验测量的互调功率电平，3个互调频率点最大误差小于5dB。分析方法有助于大功率微波部件多载波无源互调分析，可为多载波无源互调测量提供参考和依据。     

量块的电脑化测试装置

接触式干涉仪是计量部门测试三等量块的法定仪器。本文介绍了一种基于接触式干涉仪的量块自动测试系统，它以光电探测替代目视估测，免除操作人员的视力疲劳，并能自动处理数据。软件系统以最新的国家检定标准编制，易学好用。     

焊接工艺对钛合金焊接接头冲击韧性的影响

介绍了俄罗斯对钛及其钛合金焊接接头冲击韧性最大值的影响因素的研究工作,以对相关航空研究作参考作用。     

A study on radio-loud interacting/non-interacting CMEs-associated SEPs and solar flares

We have established a data set of 58 major hybrid SEP events associated with meter-to-decahectometer wavelength (m-to-DH) type II bursts, solar flares, and radio-load CMEs during the period of 1997–2014. The main focus of our study is to address the following two questions: Does the interaction of CMEs play a role in the enhancement of SEP intensity? Is there any difference in the seed population, and parent eruptions in the SEP events with and without CME interactions? Hence, the sample of 58 events is classified into two sets: (i) 35 non-interacting-CME-associated SEP events; (ii) 23 interacting-CME-associated SEP events. All the characteristics of SEPs, their associated CMEs/flares and the relationships between them are statistically analyzed and compared. Some of the basic attributes and relative elemental abundances (Fe/O ratios) of the both the sets are also compared. The results indicate that the seed particles in non-interacting-CME-associated SEP events are mostly from solar wind/coronal materials. But in the case of interacting-CME-associated SEP events, it may be associated with both flare material from preceding flares and coronal materials from solar wind/preceding CMEs. The correlation studies reveal that there are clear correlations between logarithmic peak intensity of SEP events and properties of CMEs (space speed: cc?=?0.56) and solar flares (peak intensity: cc?=?0.40; integrated flux: cc?=?0.52) for non-interacting-CME-associated SEP events. But these correlations are absent for the interacting-CME-associated events. In addition, the results suggest that interaction of primary CMEs with their preceding CMEs plays an important role in the enhancement of peak intensity of SEPs at least for a set of m-to-DH type II bursts associated SEP events.