民用飞机复合材料结构制造工艺变化的等效性验证

高性能复合材料已经大量应用于民用运输飞机结构,并以飞机主制造商协同供应商的方式进行复合材料飞机结构的制造。介绍了航空器适航审定对复合材料结构制造的适航要求,引出了复合材料结构制造工艺变化的等效性验证方法。目前,复合材料结构制造工艺变化的等效性验证是通过所制造复合材料物理的、化学和基本力学的性能试验,并对试验结果进行统计分析来实现的。最后提供了等效性验证的接受准则。所述内容,对国内民用飞机复合材料结构在不同供应商处制造以及制造过程中工艺变化如何满足航空器适航审定要求提供借鉴;对其它行业复合材料结构制造的质量控制也有借鉴意义。     

运输类飞机结构设计安全系数的探讨

中国民用航空规章运输类飞机适航标准25.303要求采用1.5的安全系数,该要求同其他相关适航条款,例如25.307"结构符合性的证明"、25.603"材料"、25.605"制造方法"、25.613"材料的强度性能和材料的设计值"等,共同保证了飞机结构的高可靠性。理论上,当材料、载荷、分析等方面的不确定性降低,采用低于1.5的安全系数可以保证结构具有同等的高可靠性;另一方面,当材料、载荷、分析等方面的不确定性大于目前适航规章所允许的水平,通过采用大于1.5的安全系数也可以保证结构具有等同的高可靠性。为了在民用运输类飞机的适航取证/审定过程中,在保证结构可靠性的前提下,能够根据具体情况适当调整结构安全系数,在综合研究中国民用航空规章第25部《运输类飞机适航标准》相关条款内在联系的基础上,探讨了载荷、材料性能、分析方法等不确定性对飞机结构安全系数的贡献。研究结果表明,目前1.5的飞机结构安全系数,用于考虑载荷、材料性能、分析方法等不确定性的系数分量分别为1.2、1.12、1.116.     

复合材料工艺的适航审定

阐述并解析了运输类飞机适航规章对结构制造方法的内在要求,介绍了复合材料工艺适航审查的流程、验证级别、验证所需考虑的要素,以及为表明对适航规章的符合性,复合材料工艺规范应包含的必要组成部分以及各部分的编制要求。     

Stability analysis of an aeroelastic system with friction

In this paper, harmonic balance method, exact formulation and numerical simulation method are adopted to study the effects of different friction stiffness on the stability of 1.5 degrees of freedom aeroelastic system. On this basis, the expressions of input energy and dissipated energy are deduced, and the energy method is used to reveal the mechanisms of the stable boundary and unstable boundary existing in the system and the effects of different friction stiffness on the stability of the system. Studies have shown that the stability region and the critical aerodynamic damping ratio of the system rise with the increase of the friction stiffness, while the friction stiffness has little effect on the stability boundary. In the analysis of the stability of system, the results of harmonic balance method, exact formulation and Newmark of numerical simulation method are in good agreement. Compared with exact formulation and numerical simulation method, the concept and conclusion of harmonic balance method are simple in the system stability analysis.     

航天飞行器中舷窗温度场及换热的研究：外部界面处于第三类非线性边界条件

本文采用控制容积法,光线踪迹法结合谱带模型,研究航天飞机返回大气层时舷窗硅玻璃的非稳态复合换热。文章给出了界面S_2处于第三类非线性边界条件下,舷窗硅玻璃内部的温度场和进入机舱内部的热流密度。计算结果表明,如不考虑硅玻璃内部的辐射作用,对温度场影响不太大,但对进入机舱内的热流密度将会产生很大的误差。     

用高速纹影摄影技术观测自由面微物质的喷射

本文介绍了适于爆轰实验研究的透射式高速纹影仪。该设备具有较高的测试灵敏度。应用它观测了铅和钢样品自由面的微物质喷射现象,取得了好的结果。     

高教机天线布局影响通讯距离研究与改进

某型高级教练机在试飞中,出现空地通讯距离不满足战技指标要求的问题。经过分析发现,由于超短波电台天线作为单极天线,其安装布局未满足天线本身要求,即接地面尺寸过小、近场区环境复杂等,导致天线辐射性能受到影响。本文对天线阻抗和方向性系数进行了研究分析,并根据飞机情况制定相应的改进方案。     

民用飞机静气动弹性载荷计算方法研究

以某大型客机为例,根据气动外形利用有限元软件PANTRAN建立高阶气动面元,利用ZONAIR静气动弹性方法,分析了其弹性载荷,包含气动力系数、过载、迎角,并与刚性载荷进行了对比。此方法合理可靠,可用于民用飞机的弹性载荷设计分析。     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

大口径远程榴弹气动力-外弹道综合优化设计

在大口径远程榴弹设计中,在保证弹丸具有足够的威力,飞行稳定性和发射强度的前提下,使弹丸具有最大射程是一个很有意义的问题。本文给出了大口径远程榴弹气动力一外弹道综合优化设计数学模型,本文还首次涉及了底部排气弹外形优化问题。