光学遥感器微晶玻璃镜头组件空间低温模拟试验技术

文章介绍了光学遥感器微晶玻璃镜头组件在空间环境下的低温模拟试验技术与试验方法。分别从试验设备的开发、试验技术指标的实现进行了分析和阐述;对关键参数进行了详细的计算;重点解决了低温实现过程中的低温传导、低温辐射下试件温度水平的控制问题,为空间低温热试验提供了具有参考价值的新型手段。     

三维空间拦截的前置追踪变结构制导律(英文)

This article aims to develop a head pursuit （HP） guidance law for three-dimensional hypervelocity interception, so that the effect of the perturbation induced by seeker detection can be reduced. On the basis of a novel HP three-dimensional guidance model, a nonlinear variable structure guidance law is presented by using Lyapunov stability theory. The guidance law positions the interceptor ahead of the target on its tlight trajectory, and the speed of the interceptor is required to be lower than that of the target, A numerical example of maneuvering ballistic target interception verifies the rightness of the guidance model and the effectiveness of the proposed method.     

科学发展观与和谐劳资关系的构建

构建和谐劳资关系必须坚持以科学发展观所倡导的“以人为本、可持续发展和统筹兼顾”作为指导思想,需要资本所有者与经营者、劳动者、政府三方的共同努力。资本所有者与经营者要充分意识到劳动和劳动力持续供给的重要性,在追求自身全面发展的同时,充分重视劳动者的各项权益,使劳动者不仅忠于职守而且在感情上与企业融为一体,通过劳资双方的合作共同为社会创造更多的物质财富。劳动者在维护企业发展大局的同时,要通过参加培训等各种方式不断提高自身的素质和在谈判中的竞争能力,并借助工会组织的力量,通过集体谈判等方式积极主动地维护自身的权益。国家要坚持统筹兼顾的原则,既不能为了维护劳动者的权益而消灭资本,也不能为了鼓励资本的发展而漠视劳动者的权益,而是通过制度建设、通过德治与法治的治国方略等来维护劳资双方的权益,化解劳资双方的矛盾和冲突。     

Observational study of magnetic chirality of solar active regions

We present the evolution of magnetic field and relationship with the magnetic (current) helicity in solar active regions from a series of photospheric vector magnetograms obtained at Huairou Solar Observing Station near Beijing, and also longitudinal magnetograms by MDI of SOHO, white light and 171 Å images by TRACE and soft X-ray images by Yohkoh.The conclusions in the analysis of the formation process of complex and delta magnetic configuration in some super active regions are the following: (1) The magnetic shear and gradient provide the non-potentiality of the magnetic field of active regions reflecting the existence of electric current. (2) Some of large-scale delta active regions could be due to the emergence of highly sheared non-potential magnetic flux bundles from the subatmosphere with amount of magnetic helicity, in addition to the emergence of twisted magnetic ropes. (3) We also present some results on the study of the magnetic (current) helicity in solar active regions.     

基于主题模型的结构化Web服务发现机制

提出了基于主题模型(topic model)的结构化Web服务发现机制.利用LDA(Latent Dirichlet Allocation)生成概率模型,将Web服务(Web service)建模为结构化文本文档.一个文档视作主题的概率分布,主题又由关键词的概率分布组成,从而提供基于主题的Web服务检索.同时,利用Web服务的结构化特性,将Web服务描述文档表示为有向无环图,利用n阶谱核测量Web服务文档的相似度,实现Web服务结构化信息的发现.通过实验分析对比,基于主题模型的结构化Web服务发现机制有效提高了Web服务发现的效率和精确率.      

谈二外日语教学中学生跨文化交际能力的培养

长期以来,我国二外日语教学受传统的教学方式的影响,存在着不可忽视的问题,本文提出了以学生为主体的跨文化交际能力培养的解决方法。     

Power-law spectra of energetic electrons in solar flares from the maximum entropy and dimensional considerations

The maximum entropy formalism and dimensional analysis are used to derive a power-law spectrum of accelerated electrons in impulsive solar flares, where the particles can contain a significant fraction of the total flare energy. Entropy considerations are used to derive a power-law spectrum for a particle distribution characterised by its order of magnitude of energy. The derivation extends an earlier one-dimensional argument to the case of an isotropic three-dimensional particle distribution. Dimensional arguments employ the idea that the spectrum should reflect a balance between the processes of energy input into the corona and energy dissipation in solar flares. The governing parameters are suggested on theoretical grounds and shown to be consistent with solar flare observations. The flare electron flux, differential in the non-relativistic electron kinetic energy E, is predicted to scale as $E^{-3}$. This scaling is in agreement with RHESSI measurements of the hard X-ray flux that is generated by deka-keV electrons, accelerated in intense solar flares.     

匀速及加速行驶时带后视镜轿车气动噪声的研究

应用计算流体力学软件FLUENT对带后视镜简化直背式轿车外部流场及车外某接收点处的气动噪声进行了数值计算和分析.脉动流场计算采用大涡模拟湍流模型,动量方程的离散格式采用有限中心差分格式.分别对两种匀速运动情况和一种加速运动进行了计算,由此研究不同车速、匀速和加速运动对接收点处脉动流场和气动噪声的影响.对于匀速运动,车速越大,接收点处流速越大,压力越小,脉动压力的脉动幅度越大,在每个频率上所对应的声压级基本上越大,总声压级也越大;在同一行驶速度下,加速运动比匀速运动在接收点处的流速要大,压力要小,在每个频率上所对应的声压级基本上要大,总声压级要大,声压级随频率的变化情况与匀速运动一样.      

Large-scale waves in the solar corona: The continuing debate

Ten years after the first observation of large-scale wave-like coronal disturbances with the EIT instrument aboard SOHO, the most crucial questions concerning these “EIT waves” are still being debated controversially – what is their actual physical nature, and how are they launched? Possible explanations include MHD waves or shocks, launched by flares or driven by coronal mass ejections (CMEs), as well as models where coronal waves are not actually waves at all, but generated by successive “activation” of magnetic fieldlines in the framework of a CME. Here, we discuss recent observations that might help to discriminate between the different models. We focus on strong coronal wave events that do show chromospheric Moreton wave signatures. It is stressed that multiwavelength observations with high time cadence are particularly important, ideally when limb events with CME observations in the low corona are available. Such observations allow for a detailed comparison of the kinematics of the wave, the CME and the associated type II radio burst. For Moreton-associated coronal waves, we find strong evidence for the wave/shock scenario. Furthermore, we argue that EIT waves are actually generated by more than one physical process, which might explain some of the issues which have made the interpretation of these phenomena so controversial.     

太阳同步轨道真空紫外光电倍增管的高能粒子屏蔽方法研究

空间辐射环境是导致光电倍增管性能衰变甚至失效的主要原因, 由于空间辐射环境的复杂性以及飞行器在空间活动的轨道、设计寿命和光电倍增管的类型不同, 光电倍增管需要的抗辐射屏蔽要求不同. 以太阳同步轨道高能粒子辐射环境为例, 对真空紫外光电倍增管进行了辐射屏蔽的Monte-Carlo计算, 在此基础上提出了运行于该轨道上的真空紫外光电倍增管的高能粒子屏蔽优化组合. 模拟计算表明, 采用Al-W-Al三层结构的屏蔽组合形式, 其中Al层厚2mm, W厚 0.5mm,可将辐射剂量从原本的9.98× 106rad (Si)降低到 8.41× 102rad (Si), 能较好地满足实际使用要求.