A Twin-CME Scenario for Ground Level Enhancement Events

Ground Level Enhancement (GLEs) events are extreme Solar Energetic Particle (SEP) events. Protons in these events often reach ～GeV/nucleon. Understanding the underlying particle acceleration mechanism in these events is a major goal for Space Weather studies. In Solar Cycle 23, a total of 16 GLEs have been identified. Most of them have preceding CMEs and in-situ energetic particle observations show some of them are enhanced in ICME or flare-like material. Motivated by this observation, we discuss here a scenario in which two CMEs erupt in sequence during a short period of time from the same Active Region (AR) with a pseudo-streamer-like pre-eruption magnetic field configuration. The first CME is narrower and slower and the second CME is wider and faster. We show that the magnetic field configuration in our proposed scenario can lead to magnetic reconnection between the open and closed field lines that drape and enclose the first CME and its driven shock. The combined effect of the presence of the first shock and the existence of the open close reconnection is that when the second CME erupts and drives a second shock, one finds both an excess of seed population and an enhanced turbulence level at the front of the second shock than the case of a single CME-driven shock. Therefore, a more efficient particle acceleration will occur. The implications of our proposed scenario are discussed.     

Nonclassical Transport and Particle-Field Coupling: from Laboratory Plasmas to the Solar Wind

Understanding transport of thermal and suprathermal particles is a fundamental issue in laboratory, solar-terrestrial, and astrophysical plasmas. For laboratory fusion experiments, confinement of particles and energy is essential for sustaining the plasma long enough to reach burning conditions. For solar wind and magnetospheric plasmas, transport properties determine the spatial and temporal distribution of energetic particles, which can be harmful for spacecraft functioning, as well as the entry of solar wind plasma into the magnetosphere. For astrophysical plasmas, transport properties determine the efficiency of particle acceleration processes and affect observable radiative signatures. In all cases, transport depends on the interaction of thermal and suprathermal particles with the electric and magnetic fluctuations in the plasma. Understanding transport therefore requires us to understand these interactions, which encompass a wide range of scales, from magnetohydrodynamic to kinetic scales, with larger scale structures also having a role. The wealth of transport studies during recent decades has shown the existence of a variety of regimes that differ from the classical quasilinear regime. In this paper we give an overview of nonclassical plasma transport regimes, discussing theoretical approaches to superdiffusive and subdiffusive transport, wave–particle interactions at microscopic kinetic scales, the influence of coherent structures and of avalanching transport, and the results of numerical simulations and experimental data analyses. Applications to laboratory plasmas and space plasmas are discussed.     

Nanofillers modification of Epocast 50-A1/946 epoxy for bonded joints

Epocast 50-A1/946 epoxy was primarily developed for joining and repairing of composite aircraft structural components. The objective of the present work is to modify the Epocast epoxy resin by different nanofillers infusion. The used nanofillers include multi-walled carbon nanotubes（MWCNTs）, SiC and Al2O3 nanoparticles. The nanofillers with different weight percentages are ultrasonically dispersed in the epoxy resin. The sonication time and amplitude for MWCNTs are reduced compared to Al2O3 and SiC nanoparticles to avoid the damage of MWCNTs during sonication processes. The fabricated neat epoxy and twelve nanocomposite panels were characterized via standard tension and in-plane shear tests. The experimental results show that the nanocomposites materials with 0.5wt% MWCNTs, 1.5wt% SiC and 1.5wt% Al2O3 nanoparticles have the highest improvement in the tensile properties compared to the other nanofiller loading percentages.The improvements in the shear properties of these nanocomposite materials were respectively equal to 5.5%, 4.9%, and 6.3% for shear strengths, and 10.3%, 16.0%, and 8.1% for shear moduli. The optimum nanofiller loading percentages will be used in the following papers concerning their effect on the bonded joints/repairs of carbon fiber reinforced composites.     

虹桥机场障碍物碰撞风险分析

研究了最后进近及复飞阶段航空器与地面障碍物之间的碰撞风险的计算方法,结合航空资料汇编中上海虹桥机场的相关信息,利用碰撞风险模型对机场的主要障碍物进行了碰撞风险计算,并分析了障碍物宽度、障碍物高度、障碍物X位移和Y位移等四个参数的变化对碰撞风险的影响。结果表明虹桥机场的障碍物碰撞风险小于安全目标水平,超障高满足要求;在一定范围内,碰撞风险随障碍物高度增大而增加,但当宽度到一个临界值后不再增加;随障碍物宽度增大而增加;随X位移增大而减小;当Y位移为0时,碰撞风险值最大。     

航空铝合金LC4在酸性介质中的在线腐蚀监测

根据航空铝合金LC4进行阳极化和封孔处理后在不同浓度醋酸溶液中电容的变化进行在线腐蚀监测.阳极化铝合金LC4在醋酸溶液中的电容变化可分为三个阶段,缓慢增长期,快速增长期和大幅振荡期.结合SEM截面观察结果,在缓慢增长期,氧化膜致密耐蚀;在快速增长期,氧化膜变得疏松;大幅振荡期的出现标志着铝合金表面的阳极氧化膜已经被完全腐蚀掉.同时还研究溶液浓度和封孔对电容变化规律的影响.结果表明,可以通过阳极化铝合金LC4在醋酸溶液中的电容变化规律进行腐蚀状况的在线评价.另外,通过LCR数字电桥测得的阻抗-频率图谱与传统测量得到的电化学阻抗谱相比,在变化规律上具有较好的一致性.     

航空发动机过渡态全局寻优控制方法研究

为了对发动机的动态过程进行控制, 提出了一种基于SQP的全局寻优控制方法.每一步寻优过程分为长程优化和短程优化两个阶段.根据长程优化结果, 重构了关联目标函数, 在此基础上, 进行了短程优化修正, 并利用修正结果进行控制.将这种方法应用于某型航空发动机的过渡态控制中, 得到了理想的控制结果.仿真结果表明该方法能较好地解决一般局部优化方法在有纯延迟、模型失配等情况下的优化控制效果下降的问题.      

燃气轮机滚动轴承故障模式及延寿方法

分析了燃气轮机滚动轴承常见的10种故障模式及其产生原因,研究了相应的延寿方法及其延寿机理。     

基于CPLD的动态频率信号测量装置的设计与实现

提出了一种基于单周期测频原理的动态频率信号测量方法,给出了动态频率信号测量装置的设计方案及其具体实现。该装置能够很好地跟踪频率信号的动态变化,且工作稳定可靠;同时还具有体积小、功耗低、便于携带等优点。     

基于非下采样轮廓波变换的红外和SAR图像融合算法

针对现有红外和合成孔径雷达(Synthetic Aperture Radar,SAR)图像的融合算法融合质量差、边缘轮廓不清晰、效率低下、可视性差,目标检测效率低等问题,提出一种基于非下采样轮廓波变换的融合算法。首先采用非下采样轮廓波变换对预处理的红外和SAR图像进行分解,获得各自低频和带通方向图像,接着根据红外和SAR图像的特征选取其含重要目标信息的频带进行低频图像和带通方向图像融合。为了检验本文所提出算法性能的优越性,采用两组红外和SAR图像进行融合实验,与其他图像融合算法进行对比,并对融合图像进行目标检测,证明了该融合算法能有效提高多源图像目标检测率。     

Space–Time Structure of Energetic Electron Precipitations according to the Data of Balloon Observations and Polar Satellite Measurements on February 1–6, 2015

Cosmic Research - The results of an analysis of the space–time characteristics and dynamics of precipitations of magnetospheric electrons with energies in the range from 0.1 to 0.7 MeV are...