用二次子结构法对过盈螺纹进行应力分析

针对过盈螺纹的疲劳寿命估算进行了工作,求解应力是寿命估算的第一步。为减少求解自由度,节省机时,提高效率,文章根据螺纹配合的特点,提出二次子结构法,消去内部节点,只留下配合点、加载点和边界约束点。 文章推导了子结构公式及过盈配合公式,给出了程序流程图及有限元计算结果,由结果可知,随过盈量增加,齿间应力差减小;而随过盈量增加,危险点相当应力增大。这些结果,对过盈量的选择也有参考价值。     

Chromospheric line emission in seismically active flares

Some flares are known to drive seismic transients into the solar interior. The effects of these seismic transients are seen in helioseismic observations of the Sun’s surface thousands of km from their sources in the hour succeeding the impulsive phase of the flare. Energetic particles impinging from the corona into the chromosphere are known to drive strong, downward-propagating shocks in active region chromospheres during the impulsive phases of flares. H observations have served as an important diagnostic of these shocks, showing intense emission with characteristic transient redshifts. In most flares no detectable transients penetrate beneath the active region photosphere. In those that do, there is a strong correlation between compact white-light emission and the signature of seismic emission. This study introduces the first known H observations of acoustically active flares, centered in the core of the line. The morphology of line-core emission H in the impulsive phase of the flare is similar to that of co-spatial line-core emission in NaD₁, encompassing the site of seismic emission but more extended. The latter shows a compact red shift in the region of seismic emission, but a similar feature is known to appear in a conjugate magnetic footpoint from which no seismic emission emanates. Radiative MHD modelling based on the profiles of chromospheric line emission during the impulsive phases of flares can contribute significantly to our understanding of the mechanics of flare acoustic emission penetrating into the solar interior and the conditions under which it occurs.     

液体镜头技术应用于空间探测的初步探讨

文章介绍了一种方兴未艾的镜头技术——液体镜头技术，分析了几种典型液体镜头的工作原理和控制方法，并初步探讨了其在空间探测领域应用的可能性。     

多因素组合下发射载体出管速度偏差预估方法

运用极限偏差、合成标准差、统计分析、蒙特卡洛仿真等多种预估方法,对发射载体出管速度偏差进行对比分析。分析结果表明,极限偏差法工程应用成熟,但预估结果偏于保守,适用于影响因素尚未认知完全的工程型号;对于影响因素比较明确的系统,运用统计分析法、合成标准差法得到的发射载体出管速度预估值一致性好,方法简单,且具有较高的准确性;蒙特卡洛法计算过程复杂,可通过大量仿真计算获取出管速度的分布特性,得到对应不同指标的分布概率,相比其他几种方法,计算结果更加科学、合理。工程型号应用时,可根据实际需要组合使用上述方法进行发射载体出管速度偏差预估分析。     

Quasi-biennial oscillations in the cross-correlation of properties of macrospicules

Jets, whatever small (e.g. spicules) or large (e.g. macrospicules) their size, may play a key role in momentum and energy transport from photosphere to chromosphere and at least to the low corona. Here, we investigate the properties of abundant, large-scale dynamic jets observable in the solar atmosphere: the macrospicules (MS). These jets are observationally more distinct phenomena than their little, and perhaps more ubiquitous, cousins, the spicules. Investigation of long-term variation of the properties of macrospicules may help to a better understanding of their underlying physics of generation and role in coronal heating. Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory, a new dataset, with several hundreds of macrospicules, was constructed encompassing a period of observations over six years. Here, we analyse the measured properties and relations between these properties of macrospicules as function of time during the observed time interval. We found that cross-correlations of several of these macrospicule properties display a strong oscillatory pattern. Next, wavelet analysis is used to provide more detailed information about the temporal behaviour of the various properties of MS. For coronal hole macrospicules, a significant peak is found at around 2-year period. This peak also exists partially or is shifted to longer period, in the case of quiet Sun macrospicules. These observed findings may be rooted in the underlying mechanism generating the solar magnetic field, i.e. the global solar dynamo.     

Equilibrium positions on stationary orbits and planetary principal inertia axis orientations for the Solar System

We present a qualitative analysis in a phase space to determine the longitudinal equilibrium positions on the planetary stationary orbits by applying an analytical model that considers linear gravitational perturbations. We discuss how these longitudes are related with the orientation of the planetary principal inertia axes with respect to their Prime Meridians, and then we use this determination to derive their positions with respect to the International Celestial Reference Frame. Finally, a numerical analysis of the non-linear effects of the gravitational fields on the equilibrium point locations is developed and their correlation with gravity field anomalies shown.     

凸轮检测方法的误差分析

对发动机凸轮检测方法的原理误差、检测系统误差、测头制造及安装误差、凸轮偏心误差、阿贝误差及检测方法总误差等进行了比较全面的分析     

The damping of small-amplitude oscillations in quiescent prominences

The presence of small-amplitude oscillations in prominences is well-known from long time ago. These oscillations, whose exciters are still unknown, seem to be of local nature and are interpreted in terms of magnetohydrodynamic (MHD) waves. During last years, observational evidence about the damping of these oscillations has grown and several mechanisms able to damp these oscillations have been the subject of intense theoretical modelling. Among them, the most efficient seem to be radiative cooling and ion-neutral collisions. Radiative cooling is able to damp slow MHD waves efficiently, while ion-neutral collisions, in partially ionised plasmas like those of solar prominences, can also damp fast MHD waves. In this paper, we plan to summarize our current knowledge about the time and spatial damping of small-amplitude oscillations in prominences.     

Solar Isotopic Composition as Determined Using Solar Energetic Particles

Solar energetic particles (SEPs) provide a sample of the Sun from which solar composition may be determined. Using high-resolution measurements from the Solar Isotope Spectrometer (SIS) onboard NASA’s Advanced Composition Explorer (ACE) spacecraft, we have studied the isotopic composition of SEPs at energies ≥20 MeV/nucleon in large SEP events. We present SEP isotope measurements of C, O, Ne, Mg, Si, S, Ar, Ca, Fe, and Ni made in 49 large events from late 1997 to the present. The isotopic composition is highly variable from one SEP event to another due to variations in seed particle composition or due to mass fractionation that occurs during the acceleration and/or transport of these particles. We show that various isotopic and elemental enhancements are correlated with each other, discuss the empirical corrections used to account for the compositional variability, and obtain estimated solar isotopic abundances. We compare the solar values and their uncertainties inferred from SEPs with solar wind and other solar system abundances and find generally good agreement.     

将日本文化融入到二外日语教学的始终

每一种语言的形成和发展都与其社会环境密切相连，语言同时反映出一个国家和民族的历史和文化。从这个层面上说，教授语言同时也是在教授文化，学习语言的同时也是在学习文化。一个科学的语言教学体系，必须将文化教学紧密融入到语言的教学当中。鉴于当前的高校二外日语教学中鲜有独立开设日本文化课的情况，将日本文化融入到二外日语教学的始终，将会有效帮助学生在有限的学习时间里取得良好的学习效果。本文针对现阶段高校二外日语教学的特点，探讨了在日本文化背景下进行二外日语教学的重要性，并提出了一些文化导入的内容与方法。