Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.     

基于放气控制的飞机轮胎自动充气装置设计

根据国内飞机轮胎充气工作的现状,设计了一种基于放气控制的飞机轮胎自动充气装置,介绍了基于此种方式的充气及检测控制过程,针对以往充气装置的不足,此控制方式能够提高轮胎充气及检测的精度。并通过实验证明系统设计合理,满足设计要求,且系统效率高、性能稳定、操作方便,具有较好的经济效益及社会效益。     

Solar Sources of Heliospheric Energetic Electron Events—Shocks or Flares?

Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks driven by coronal mass ejections (CMEs) with speeds ≳1000 km s⁻¹. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known several decades ago, but recent observations have presented a more complex picture. We review early and recent observational results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events; electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares. Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions for future work are given.     

新一代数据采集器模拟量采集插件设计技术

数据采集器是飞行试验关键的测试设备,它的性能与现代飞机飞行试验有很大的关系.为满足现代飞机设计定型的需求,新一代数据采集器设计大量采用了FPGA和DSP器件,大大提高了采集器测量参数的采样率、通道数、测量参数类型和使用的灵活性.本文介绍的新一代采集器模拟量采集卡设计技术,用数字信号处理技术来实现信号的放大、滤波及偏置修正,并提供了对采集卡各个部分进行设计的理论依据.     

三角翼大迎角绕流特性数值模拟的网格处理技术研究

研究网格对三角翼大迎角绕流特性数值模拟的影响.结果表明,网格的生成需要结合流动现象,对网格拓扑结构和网格点分布进行选择与搭配.C-H型网格适宜模拟尖前缘分离涡流态,法向网格在一定范围内应等距增长,沿流向逆压梯度较大的区域内适当增加网格点,尾迹区网格则应做上翘处理.Euler方程具有模拟三角翼旋涡及预测涡破裂特性的能力,但对二次涡等粘性引起的流动细节把握能力不足.利用层流假设的N-S方程,通过合适的网格,也可得到满意的计算结果,但对涡破裂后的强烈非定常湍流流动模拟能力不足.采用旋涡螺旋度可准确反映主涡与二次涡流动,描述旋涡的破裂现象.用轴向速度迅速减小并小于来流速度的点作为涡破裂判据似应更合理.     

某型先进发动机燃油喷嘴雾化特性的试验研究及火焰筒头部数值模拟

使用相位多普勒粒子分析仪和激光多普勒粒子测速仪系统(PDPA/LDV)等设备测量了某型航空发动机喷嘴的雾化特性,主要包括:喷嘴流量特性,雾化粒度(SMD)和喷雾锥角。应用Fluent软件,对装用该喷嘴的燃烧室火焰筒进行了数值模拟。试验和计算结果得出了一些有价值的结论,对该发动机的燃油喷嘴和火焰筒头部温度场、速度场有深入了解,对其改进提供了重要依据。     

Vibration Reduction of Open-chain Flexible Manipulators by Optimizing Independent Motions of Branch Links

In order to suppress vibration in flexible manipulators, a new type of manipulator mechanism with controllable local degrees of freedom is proposed. This mechanism consists of a main chain and some branch links. The main chain is of a flexible open-chain configuration with an end-effector installed at its tip, and the rigid branch links are able to perform active movements. It is proved by kinematics and dynamic analysis that, the branch links bear no direct kinematic relation to the main chain, but their independent motions can strongly affect the dynamic behavior and performance of the flexible manipulator. Then comes a new idea of suppressing vibration, in which independent motions of the branch links are used to suppress the undesired vibration of the flexible main chain through dynamic coupling. On this basis, an optimal method for reducing vibration of flexible manipulators is proposed. Finally, the effectiveness of this method is verified by numerical simulations.     

基于模拟退火算法与响应面模型的三维气动优化设计方法

提出了一套适用于高耗时三维气动设计问题的优化设计体系.其主要思想是采用改进拉丁超立方体试验设计选取样本点,应用自行开发的三维粘性流场求解程序进行流场计算建立数据库,采用二次响应面方法建立近似模型,再应用高效模拟退火算法进行全局寻优.以NASA rotor57为对象,在详细进行流场计算基础上采用所提出的优化体系对其进行了三维积叠优化设计.在对流量、效率加以严格约束的条件下,总压比可提高1.8%,对流场结构进行了分析.优化结果表明本优化方法省时,适于三维气动设计的特点.     

中国低价出口的成因分析

由于我国土地、资本以及劳动力要素价格本身较低,而企业承担的社会责任也较少,导致生产成本低廉,这是中国出口商品价格低廉的首要因素。同时,国内市场上产能过剩、进入壁垒较低等因素导致产业竞争加剧,企业被动寻求外销渠道。中国企业在研发能力、品牌以及国际化经营能力等核心竞争力方面的弱势,使得产品处在全球价值链末端,附加值较低,面对国际市场上同质产品的激烈竞争只能采用低价竞争策略。低价出口造成中国贸易条件的不断恶化及贫困化增长的不正常现象,因此,今后中国应加快经济增长方式的转变,实现对外贸易的持续发展。     

基于最小二乘支持向量机的普通高校招生人数预测研究

近年来普通高校的发展速度与规模,使社会大众兴起了对教育质量与总量的关注。普通高校招生数预测是制定教育政策的重要依据。针对中国文化教育的特征,在统计学习理论和结构风险最小化原理的基础上,建立了基于最小二乘支持向量机的时间序列预测模型。预测结果表明该模型具有较高的预测精度,为普通高校招生数预测提供了一条新的途径。