任意铺层复合材料加筋板屈曲/后屈曲行为的解析解

给出了一种求解任意铺层复合材料加筋板屈曲/后屈曲问题的解析方法。首先将加筋板简化为受弹簧约束的层合板,而后通过构造位移函数,并利用伽辽金法得到了加筋板压缩、剪切和压剪载荷下的屈曲/后屈曲解析解。求解中引入了无量纲参数,使得结果更具一般性;在后屈曲行为中考虑了初始缺陷和由耦合刚度引起的前屈曲挠度,使得结果更加准确。通过与有限元结果的比较,讨论了几何参数、弹簧刚度等对解的影响。最后将该方法应用于T形加筋对称铺层复合材料加筋板的屈曲/后屈曲分析中,考虑T形筋对复合材料层板粘结区的刚度增强作用,采用刚度平均化方法引入增强效果,并与两种T形筋刚度简化模型以及有限元结果进行了比较,验证刚度平均化方法对计算加筋板屈曲/后屈曲行为的有效性。     

大型整体壁板成形技术

 大型整体壁板是现代先进民用飞机的重要结构件,大型整体壁板成形技术是整机研制过程中所必须要解决的重大关键技术。从大型整体壁板的结构特点出发,介绍了整体壁板的结构形式和分类,重点阐述了整体带筋壁板喷丸成形技术和时效成形技术的国外研究应用进展及发展趋势,分析了国内现有整体壁板成形技术的基础和存在问题,特别介绍了国内在ARJ21新支线飞机研制中所取得的最新进展。最后针对中国大飞机研制的紧迫需求,提出了尽快开展大飞机机翼和机身整体壁板成形技术研究的建议和对策。     

多段翼型分析和反设计位流计算

本文采用第二代低阶面元法给出了多段翼型分析和反设计位流计算方法。按照曲率变化情况划分板块可很好地提高计算效率。     

外挂物投放 发射过程数值仿真中的非均匀流场计算

本文介绍了用面元法计算外挂物投放/发射过程中的非均匀流场问题。理论分析表明三角形奇点分布形态在非均匀流场计算中具有其独特的优越性。本文还阐述了伍德沃德程序中机翼线性变化源分布中法向扰动速度公式的错误。数值结果表明,理论计算与实验值吻合较好。     

Particle acceleration and kinematics in solar flares – A Synthesis of Recent Observations and Theoretical Concepts (Invited Review)

We review the physical processes of particle acceleration, injection, propagation, trapping, and energy loss in solar flare conditions. An understanding of these basic physical processes is inexorable to interpret the detailed timing and spectral evolution of the radiative signatures caused by nonthermal particles in hard X-rays, gamma-rays, and radio wavelengths. In contrast to other more theoretically oriented reviews on particle acceleration processes, we aim here to capitalize on the numerous observations from recent spacecraft missions, such as from the Compton Gamma Ray Observatory (CGRO), the Yohkoh Hard X-Ray Telescope (HXT) and Soft X-Ray Telescope (SXT), and the Transition Region and Coronal Explorer (TRACE). High-precision energy-dependent time delay measurements from CGRO and spatial imaging with Yohkoh and TRACE provide invaluable observational constraints on the topology of the acceleration region, the reconstruction of magnetic reconnection processes, the resulting electromagnetic fields, and the kinematics of energized (nonthermal) particles. This revised version was published online in June 2006 with corrections to the Cover Date.     

Composition of anomalous cosmic rays and implications for the heliosphere

We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the Voyager 1 and 2 spacecraft during the period 1994/157-313 to determine several parameters of interest to heliospheric studies. We estimate that the strength of the solar wind termination shock is 2.42 (–0.08, +0.04). We determine the composition of ACRs by estimating their differential energy spectra at the shock and find the following abundance ratios: H/He = 5.6 (–0.5, ⁺0.6), C/He = 0.00048 ± 0.00011, N/He = 0.011 ± 0.001, O/He = 0.075 ± 0.006, and Ne/He = 0.0050 ± 0.0004. We correlate our observations with those of pickup ions to deduce that the long-term ionization rate of neutral nitrogen at 1 AU is 8.3 × 10^–7 s^–1 and that the charge-exchange cross section for neutral N and solar wind protons is 1.0 × 10^–15 cm² at 1.1 keV. We estimate that the neutral C/He ratio in the outer heliosphere is 1.8(–0.7, +0.9) × 10^–5. We also find that heavy ions are preferentially injected into the acceleration process at the termination shock.     

飞机整体壁板战伤修理研究

 为飞机整体壁板战伤应急胶接修理提出了波纹板补强方案,该方案改善了补片与其周围壁板间的刚度匹配,使被修复壁板承载能力得以提高,且无须改变原有的胶接修理工艺及胶粘剂。     

水轰五飞机大型整体壁板的设计与制造

 本文介绍水轰五飞机大型整体壁板的结构设计和经济效果及其数控加工,喷丸成形和毛坯扁挤压制造工艺特点。     

卫星太阳阵展开的动力学方程

研究了卫星太阳阵展开的动力学问题，将卫星太阳阵的结构视为树形多体系统，利用给出的自由形式树形多刚体系统运动微分方程建立太阳阵系统的动力学方程，应用为该系统动力学方程编制的计算程序，可对太阳阵展开过程中卫星本体姿态的改变量以及太阳帆板在展开过程中的运动参数进行数值计算。     

Coronal Dynamics and the AIA on SDO

We provide a brief overview of present-day studies of inner corona dynamics, with examples of mass ejections (CME), flares and active region dynamics. While the names of the topics have not changed in several decades, the internal details and the language used to express the nature of the problem have changed considerably. We conclude with a short discussion of the contribution to studies of coronal dynamics to be expected from the Atmospheric Imager Assembly (AIA) on the Solar Dynamics Observatory.