空间站新型渐开弧面齿轮传动理论及试验研究

针对因空间站大型对日定向装置传动末端齿轮副尺寸大导致的中心距偏移及倾斜偏差问题，提出具有中心距可分性的新型渐开弧面齿轮，具备中心距补偿能力，有效解决末端齿轮传动中心距偏差问题;依据对末端传动指标要求及约束条件，采用渐开弧面齿轮传动技术对齿轮副进行设计、强度校核及仿真分析;设计并开展等比例方案下多套产品研制及多轮次齿轮副寿命试验研究工作，测试传动效率并观察齿轮齿面状态，以验证新型齿轮传动的中心距补偿能力及可行性。研究内容为大型传动机构齿轮副方案设计奠定基础，并为新型渐开弧面齿轮的研制提供参考。     

Bifurcation analysis of dual-sidestay landing gear locking performance considering joint clearance

Sidestay lock mechanism is an important part of landing gear system, and the locking performance can be analyzed based on changes in its stability. However, during numerical continuation analysis of fully-rigid dual-sidestay landing gear without clearance, it has been found that the appearance of bifurcation points does not necessarily imply that both sidestay links can be locked synchronously. This problem reveals the limitations of fully-rigid model with ideally-articulated in solving dual-sid...     

导引头伺服机构消隙齿轮系统动力学特性分析

消隙齿轮广泛应用于导引头伺服机构惯性稳定平台传动系统中，用于消除回程误差，提高传动精度。目前，对消隙齿轮传动系统的动力学分析大多采用数值方法，然而在求解含时变啮合刚度和间隙的强非线性系统时耗时较长。本文利用集中质量法建立考虑时变啮合刚度的消隙齿轮系统动力学模型，通过对模型的无量纲及归一化处理，运用分段的增量谐波平衡法对消隙齿轮传动系统进行分析，并利用四阶Runge-Kutta法进行数值验证，研究了不同参数对消隙齿轮系统动力学特性的影响规律。结果表明:随扭簧刚度的提高，系统谐振频率也提高，且共振幅值降低;随内部激励的增加、阻尼比的减小，系统由周期运动逐渐变为混沌运动，且共振幅值增大。     

1-D dusty photo-ionization models of WR planetary nebulae NGC 2452 and IC 2003

We report dusty photo-ionization models for two Planetary Nebulae NGC 2452 and IC 2003, which have [WR] type central stars, using 1D photo-ionization code Cloudy17.02. We used the medium resolution optical spectra and archival IRAS photometry to constrain our models. The physical size of the ionized nebula derived using accurate distance measurements and absolute H$\beta$ flux available in the literature were used as additional constrains. We examine the importance of photo-electric heating and found that models with and without considering photo-electric heating do not make significant difference for both PNe for the MRN grain size distribution considered in this study. We derive the nebular elemental abundances of these PNe by the empirical method as well as by making dusty photo-ionization models. The values of N/O ratios for both PNe obtained from our models are lower than their respective values arrived using empirical methods. The central stars are assumed to be black bodies and the photospheric temperatures derived respectively for NGC 2452 and IC 2003 from their best fit models are 182 kK and 155 kK and their respective luminosities are 630$L_{\odot }$ and 1015$L_{\odot }$. We propose that both the PNe were resulted from low-mass progenitors of mass $?$2.8 M_⊙.     

基于时空数据模型的障碍物数据集数据查询与应用研究

障碍物数据集是国际民航组织在航空情报管理（AIM）体系下提出的一种基于航空信息交换模型（AIXM）规范的航空情报数据集，该数据集中障碍物的查询将直接影响机场净空评估与飞行程序设计。在分析障碍物数据集的时间与空间属性基础上，利用时空数据模型与航空信息交换模型规范，提出一种基于时间点和空间位置的障碍物数据集查询方法， 用于解决障碍物数据集的查询问题；构建障碍物查询与可视化系统，并通过设计随机实验和实例应用对该方法的可行性和可靠性进行验证。结果表明：该障碍物数据集查询方法能够提取出对机场净空与飞行程序设计有影响的障碍物，增强了飞行程序设计人员对机场障碍物分布的情景意识。