Stellar coronagraph using the principle of achromatic null-interferometer

In order to observe exoplanets we propose a space-based achromatic stellar coronagraph combined with a 0.8–1.5 m telescope. We develop an achromatic common path interferometer for observing an exoplanet (a faint off-axis source) on the background of a hoste star (bright axial source). An image of the star and its copy acquire an achromatic phase shift by 180° and interfere in antiphase. The achromatic phase shift is caused by geometric phase in the scheme of a three-dimensional interferometer. The interference process divides spatially the dark and light fields of the star image redirecting them to the opposite sides of a beam splitter. The interference process does not weaken the image of a planet, with equal intensities it is redirected to both sides of a beam splitter. The suggested scheme of common path interferometer ensures mechanical stability. The background signal is experimentally demonstrated to be reduced by six orders of magnitude.     

农村家庭资产配置与金融市场参与的实证研究——以浙江金华地区为例

通过金融深化增加农村家庭参与金融市场的机会，提高农村家庭的福利，让金融为广大农村家庭服务，改善其资源配置，解决农村金融抑制的问题，是当前金融改革与发展的一个重要内容。文章将农村家庭的实物资产分为生活型与生产投资型，将金融资产分为安全型和风险型，根据问卷调查获取的数据建立Logistic回归模型，对东部地区农村家庭实物资产配置和参与金融市场的决定因素进行研究，探讨当前农村的金融深化与金融发展路径。     

系统思想在航天企业全面风险管理实施中的应用

介绍了风险管理国际标准ISO31000的核心内容——风险管理框架,以及系统思想的基本理念;以系统观点和方法为基础,对国际标准在航天企业全面风险管理中的应用进行了探讨。通过对全面风险管理工作的系统分解与集成,并以其中的"环境"分系统建设为例,进一步细分工作内容,与现有业务管理工作相结合,探索出全面风险管理工作在航天企业落地的基本路径。     

线性调频半导体激光衍射光栅干涉仪

介绍一种以线性调频半导体激光为光源的衍射光栅干涉仪。激光与光栅上衍射的±１级衍射波会合，由于有光程差而发生光拍频，测量拍频信号的相位移则可测得光栅的位移。设计了一种克服激光波长漂移和空气折射率变化影响的对称差动光路，使这种方法达到实用化的程度，分辨力达到纳米级。此外，还介绍了应用于接触干涉仪的实验情况。     

二维三角晶格的Peierls相变前后的声子色散曲面的研究

利用晶格动力学理论计算了二维三角晶格的Peierls相变前后的声子能谱。并且在第一布里渊区绘制了声子色散曲面。通过对Peierls相变前后的声子能谱比较可知，随其对称性降低，声子能谱的简并度被破缺。二维三角晶格的Peierls相变前只有两支声频支声子能谱，Peierls相变后有两支声频支声子能谱与两支光频支声子能谱，并且声频支声子能谱与光频支声子能谱不相交，两支光频支声子沿ky轴平缓地变化。     

热-机耦合分析的有限元法及其应用

基于有限元分析的基本原理,建立了热-机耦合问题分析的有限元基本方程,并对工件挤压过程及摩擦制动问题进行了分析。算例表明,热-机耦合分析方法能很好地模拟受热结构的温度场和应力应变场,为结构设计和工艺设计提供依据。     

Current status and future plans for the general antiparticle spectrometer (GAPS)

We discuss current progress and future plans for the general antiparticle spectrometer experiment (GAPS). GAPS detects antideuterons through the X-rays and pions emitted during the deexcitation of exotic atoms formed when the antideuterons are slowed down and stopped in targets. GAPS provides an exceptionally sensitive means to detect cosmic-ray antideuterons. Cosmic-ray antideuterons can provide indirect evidence for the existence of dark matter in such form as neutralinos or Kaluza–Klein particles. We describe results of accelerator testing of GAPS prototypes, tentative design concepts for a flight GAPS detector, and near-term plans for flying a GAPS prototype on a balloon.     

温度翘曲应力对机场刚性道面寿命的影响

分析了目前中国民航机场刚性道面的设计过程,指出在设计过程中忽视温度应力的影响不合理。参照公路水泥混凝土路面温度应力计算方法并根据Miner定律研究了温度翘曲疲劳损耗对于机场刚性道面影响规律,即温度翘曲疲劳损耗随板厚、地基反应模量的增大而增大,随着混凝土设计强度的增加而降低。然后提出采用设计寿命的影响因子nt/Nt评价温度翘曲疲劳损耗对于机场刚性道面设计寿命影响的方法并提供了相应的机场刚性道面板厚度设计流程图。最后提供了一个考虑温度翘曲应力的刚性道面设计实例,为工程应用提供参考。     

The RadioAstron project: Measurements and analysis of basic parameters of space telescope in flight in 2011–2013

The results of a large number of the antenna radiometric measurements at bands of 92, 18, 6.2, 1.35, and 1.7-1.2 cm are presented by the data of the standard telemetry system of the Spektr-R spacecraft. Both special sessions of calibration object observations in the mode of a single space radio telescope (SRT) operation and numerous observations of researched sources in the mode of the ground-space interferometer were used. The obtained results agree with the first results of Kardashev et al. (2013), i.e., within 10–15% at bands of 92, 18, and 6.2 cm and 20–25% at the band of 1.35 cm. In the main, the measurements for the eight subbands at wavelengths of 1.7-1.2 cm indicate a monotonic increase in the spectral system equivalent flux density (SEFD) of noise radiation with a frequency consistent with the calculated estimates for the discussed model. The sensitivity of the ground-space interferometer for the five subbands at wavelengths from 1.35 to 1.7 cm can be higher by a factor of 1.5, and for the three subbands from 1.35 to 1.2 cm lower by a factor of 1.5 than at the band of 1.35 cm. The SRT contribution to the interferometer sensitivity proportional to the square root of SEFD is close to the design one at the bands of 92 and 18 cm and decreases the design sensitivity approximately by a factor of 1.5 and 2 at the bands of 6.2 and 1.35 cm, respectively. These differences of implemented values from the design ones were not significantly affected the scientific program implementation.     

Plasma convection model and generation of longitudinal currents in the earth's magnetosphere

The aim of this paper is to investigate processes in the magnetosphere and in particular the problems of the interaction of the solar wind with the Earth's magnetic field to produce large-scale convection, electric fields and longitudinal currents in the magnetosphere. The investigation is carried out in the frame of magnetic hydrodynamics. The reason for such an approach can be found in /1/. When calculating the transfer coefficients, the Böhm approximation is used, i.e. it is considered that the plasma in the near-equatorial part of the magnetosphere (quasiplanar geometry is used in the problem for simplification) is sufficiently turbulent that the condition ωτ ≈ 1 is valid (ω is the Larmor frequency of electrons, τ is effective time between two Quasi-collisions). The main subjects of investigation in this paper are the input near the equatorial boundary layer and the plasma layer of the magnetosphere tail.