Experimental,analytical and numerical investigation on tensile behavior of twisted fiber yarns

Stitched composite materials are emerging as a promising material due to their high interlaminar strength, combined performance and light weight. The mechanical properties of stitch yarns are very essential for stitched composite structures. In this study, the tensile behaviors of the twisted fiber yarn in stitched composites were investigated experimentally, analytically and numerically. Two kinds of cross-sectional area of twisted yarn are proposed and discussed. The paper presents an intersecting circle model to describe the cross-section of twisted fiber yarns, and a physics-based theoretical model to predict the effective tensile moduli. The numerical models take into account the cross-sectional characteristic and the twist architecture. The investigation shows that: the sum of each fiber area should be used for experimental analysis; and the cross-sectional area surrounded by the yarn profile should be used for theoretical predictions and finite element (FE) simulations. The relative errors of the prediction method and the FE simulation are less than 2% and 1%, respectively. The friction between the fibers is derived, and the effect of friction on mechanical properties is discussed. The investigation method will serve as a fundamental component of twisted fiber bundle/yarn analysis.     

Transient thermal behavior of stratospheric balloons at float conditions

The prediction of the thermal behavior of stratospheric balloons under varying environmental conditions is one of the key issues in the design and flight test of balloons. In this paper, a three-dimensional transient thermal model is developed to predict the thermal behavior of spherical stratospheric balloons. The diurnal variations of the skin and lifting gas temperatures at float conditions are discussed in detail. The further studies on the thermal behavior of stratospheric balloons are presented also.     

The dynamic heliosphere,solar activity,and cosmic rays

This brief review addresses the relation between solar activity, cosmic ray variations and the dynamics of the heliosphere. The global features of the heliosphere influence what happens inside its boundaries on a variety of time-scales. Galactic and anomalous cosmic rays are the messengers that convey vital information on global heliospheric changes in the manner that they respond to these changes. By observing cosmic rays over a large range of energies at Earth, and with various space detectors, a better understanding is gained about space weather and climate. The causes of the cosmic ray variability are reviewed, with emphasis on the 11-year and 22-year cycles, step modulation, charge-sign dependent modulation and particle drifts. Advances in this field are selectively discussed in the context of what still are some of the important uncertainties and outstanding issues.     

浅析歼八飞机机体结构设计的四个问题

对歼八飞机结构设计中出现的4个难点问题（机翼四梁接头耳片、原型机腹鳍、减速板、机尾罩尾尖）做一探讨性浅析。     

创业氛围与环境优化

创业环境的优化是一个内外协同演进的共生过程,培育一定的创业氛围是其中至关重要的中间环节。创业环境包括两个组成部分：内生决定的创业氛围和外部影响的创业条件。现阶段,决定我国创业水平的环境因素是创业氛围,它表现为显在与潜在的创业者行为方式,是一种主观的生态环境。不同区域创业环境优化的政策思路应当有别,落后的中西部地区创业环境建设的关键在于形成一定的创业氛围,否则,客观的创业条件再怎么改善也很难有效刺激创业活动。     

SiO2-水纳米流体在波壁管内流动特性的实验研究

实验研究了不同质量分数的SiO2-水纳米流体在波壁管内的流动特性,由于波壁管自身的结构特点,使流体在较小雷诺数下达到湍流状态,可以方便测出流体在层流、过渡流、湍流区的流动特性.研究发现:相同温度条件下,纳米流体的粘度随着质量分数的提高而增大;流动可视化照片显示纳米流体中由于内部纳米粒子的微运动促使流体均匀性更好;沿程阻力测试表明在层流区内摩擦系数随纳米流体质量分数的增加而增大,在过渡流和湍流区内摩擦系数随质量分数增加变化不大.     

考虑组织因素的航空维修差错产生机理分析

为有效防范航空维修差错的发生,从组织因素角度对航空维修差错产生机理进行分析,在对组织因素影响维修差错作用关系分析的基础上,建立了组织因素导致维修差错的成因机理分析模型,从差错产生的潜伏阶段、发生阶段、纠正或扩展阶段和致灾阶段4个阶段对差错产生的演化过程进行了分析,进一步构建了组织层面的维修差错防控体系,为维修差错的系统...     

氯离子和温度对铝合金在冷却液中腐蚀的影响

分别采用了动电位极化法、电化学阻抗法研究了不同温度下、不同氯离子浓度下防锈铝在模拟冷却液中的腐蚀行为,采用金相显微镜和扫描电镜对极化后防锈铝的表面特征进行了观察和记录。结果表明,氯离子吸附在防锈铝氧化膜表面,对氧化膜表面造成破坏。在一定温度下（30℃）,当氯离子浓度超过0.01mol/L时,中间产物吸附作用就会增强,阻抗谱中低频区出现感抗弧,点蚀萌生。随着氯离子浓度增高（超过0.01mol/L）,防锈铝的腐蚀加剧,耐腐蚀性能下降。随着温度的升高,阴极和阳极反应阻力变小,阳极金属铝的溶解和阴极氧还原速度增大,腐蚀速度增大。温度升高的同时,溶解氧含量下降,阴极反应受到抑制。与此同时扩散过程在整个腐蚀反应过程中的支配性降低,中间产物在氧化膜表面的吸附作用增强,从而导致低频容抗弧的出现。温度对点蚀形貌的影响主要体现在影响单个点蚀坑的几何大小,促进点蚀坑的生长。      

Statistical properties of the IMF clock angle in the solar wind with northward and southward interplanetary magnetic field based on ACE observation from 1998 to 2009: Dependence on the temporal scale of the solar wind

Utilizing ACE satellite observations from 1998 to 2009, we performed the elaborate study on the properties of the clock angle θ_CA (arctan(By/Bz) (?90° to 90°) of the interplanetary magnetic field (IMF) in the solar wind at 1?AU. The solar wind with northward IMF (NW-IMF) and southward IMF (SW-IMF) are analyzed, independently. Statistical analysis shows that the solar wind with SW-IMF and NW-IMF has similar properties in general, including their durations, the IMF Bz and By components, and the IMF θ_CA. Then, the solar wind with NW-IMF (SW-IMF) is classified into five different temporal scales according to the duration of the NW-IMF (SW-IMF), i.e., very-short wind of 10–30?min, short-scale wind of 0.5–1?h, moderate-scale wind of 1–3?h, long-scale wind of 3–5?h, and super-long wind >5?h. Our analysis reveals that the IMF θ_CA has a distinct decrease with increase of the temporal scale of the solar wind. Next, the solar wind is classified into two groups, i.e., the high-speed solar wind (>450?km/s) and the low-speed solar wind (<450?km/s). Our analysis indicates that the IMF θ_CA depends highly on the solar wind speed. Statistically, high-speed solar wind tends to have larger IMF θ_CA than low-speed solar wind. The evolutions of the solar wind and IMF with the solar activity are further studied, revealing no clear solar variation of the IMF θ_CA. Finally, we analyze the monthly variation of the IMF θ_CA. Superposed epoch result strongly suggests the seasonal variation of the IMF θ_CA.     

Solar Activity and the Climate of Prebaikalia

This paper presents convincing evidence for the reality of manifestations of solar variability in climate characteristics of the Prebaikalia. A numerical estimate is obtained of this influence on ground air temperature. It is shown that the main meaningful variations in air temperature in the region for the period1881-1960 were caused by solar activity. Since the 1960s till the present, with the influence of solar variability continuing, a clear-cut influence of another factor has been observed, the role of which has been steadily increasing, and in the hst decade it has now exceeded the contribution of solar variability. Research results on the variations in hydrological characteristics of Lake Baikal and the Angara river and their connection with solar activity are presented. It is shown that these characteristics are closely correlated with the duration of solar cycles.