基于改进伪谱反馈控制的远程变轨闭环制导

利用最优反馈控制和轨迹快速重构技术,设计一种有限推力空间远程变轨自适应闭环制导方法。首先给出了最优反馈控制的求解原理和必要条件。将空间变轨动力学模型特点和伪谱法相结合,设计基于状态量缩减的计算效率改进策略以提高轨迹优化的实时性。基于改进伪谱法进行逐次轨迹快速重构,利用开环最优解形成闭环反馈,从而保证制导指令的实时更新,并通过引入控制逻辑改进制导算法。远程交会仿真表明,该闭环制导方法在保证任务指标具有一定最优性的同时,可以有效抑制多种参数不确定性和外界干扰的影响,具有较高的制导精度、自适应性和鲁棒性。     

An introduction to the lunar and planetary science activities in Korea

Korea is planning a series of lunar space programs in 2020 starting with a lunar orbiter and a lander with a rover. Compared to other countries, Korea has a relatively brief history in space and planetary sciences. With the expected Korean missions on the near-term horizon and the relatively few Korean planetary scientists, Korea Institute of Geoscience and Mineral Resources (KIGAM) has established a new planetary research group focusing on development of prospective lunar instruments, analysis of the publicly available planetary data of the Moon, organizing nationwide planetary workshops, and initiating planetary educational programs with academic institutions. Korea has also initiated its own rocket development program, which could acquire a rocket-launch capability toward the Korean lunar mission. For the prospective Korea’s lunar science program, feasibility studies for some candidate science payloads have been started since 2010 for an orbiter and a lander. The concept design of each candidate instrument has been accomplished in 2012. It is expected that the development of science payloads may start by 2014 as Phase A. Not only developing hardware required for the lunar mission but also educational activities for young students are high priorities for Korea. The new plan of the Korean lunar mission can be successfully accomplished with international cooperative outreach programs in conjunction with internationally accessible planetary data system (PDS). This paper introduces the KIGAM’s international cooperative planetary research and educational programs and also summarizes other nationwide new developments for Korean lunar research projects at Kyung Hee University and Hanyang University.     

某型飞机襟副翼交点同轴度分析

通过某型飞机襟副翼在实际装配中出现的交点同轴度问题，从工装、零件、工艺方法、容差分配等多角度进行了分析、论述，并采取一系列措施，使问题得以解决，为以后类似机型的设计、生产积累了经验。     

颗粒尺寸对Fe-Si-Al 电磁与吸波性能的影响

为阐明吸收剂的颗粒尺寸与吸波材料电磁、吸波性能之间的关系,以气雾化球状Fe-Si-Al粉末为原料,通过筛分获得不同颗粒尺寸的Fe-Si-Al合金,以硅橡胶为基体制备了Fe-Si-Al吸波材料。借助振动样品磁强计和矢量网络分析仪分别研究了颗粒尺寸对Fe-Si-Al粉末和吸波材料的比饱和磁化强度、电磁参数和吸波性能的影响。结果表明:随着颗粒尺寸的减小,Fe-Si-Al粉末的比饱和磁化强度增加;吸波材料的复磁导率增加,复介电常数减小;3 mm厚的Fe-Si-Al吸波材料随其颗粒尺寸的减小,匹配频率向低频移动。减小吸收剂的粒径有助于提高其磁性能和吸波材料的低频吸收效果。     

量子科学实验卫星的多维数据立方体方法研究

科学实验卫星以科学目标为任务战略导向,需要任务团队结合实际业务运行情况制定阶段实验计划.这些实验计划以任务运行数据为依据,由科学卫星任务各分系统数据分析获得的策略集合综合得到.量子科学实验卫星在轨运行期间会产生大量运行数据,如何有效利用这些数据给不同决策层提供辅助是当前面临的一大难题.目前主流方式主要借助值班日志统计和...     

锥形预混火焰羽流脱落过程的实验诊断

为了研究锥形预混火焰的羽流脱落特性,以丙烷-空气预混火焰为实验对象,通过粒子图像测速技术对锥形预混火焰的羽流速度场进行了实验研究,动态模态分解法对得到的速度场进行了模态分解和主要特征重构还原。同时采用光电倍增器对火焰热释放强度信号进行实时采集,采用双热电偶法对然后热气体的温度进行了重建。结果表明在浮力诱导下燃尽气体与周围环境空气相互剪切形成剪切层（BSL）, BSL 的 KH 不稳定性诱导产生了涡,涡作用于燃尽区附近的流场,扰动传至火焰面附近区域,与火焰剪切层（FSL）的 DL 不稳定性耦合,表现为火焰面的脉动和火焰热释放率的脉动。通过近红外自发光成像得到的热气体自发光强度与温度信号有较强的相关性,热气体呈现出与速度场相似的周期性传播模式,为研究预混火焰的羽流脱落特性提供了新的思路。     

改性羰基铁粉/ 硅橡胶材料的制备及其力学性能

以微米级改性羰基铁粉为填充剂,甲基乙烯基硅橡胶为基体,制备了高温硫化的羰基铁粉/硅橡胶复合材料.研究了偶联剂种类、用量及羰基铁粉填充量对复合材料力学性能的影响,利用扫描电镜对硫化胶断面的微观结构进行了观察.结果表明,采用硅烷偶联剂KH570、KH151改性羰基铁粉都能提高复合材料的拉伸强度,其中KH151的改性效果要优于KH570;KH151的最佳用量为羰基铁粉质量的1%;在一定范围内随着改性羰基铁粉体积分数的增加,复合材料的拉伸强度增大.羰基铁粉体积分数超过60%后,混炼困难.     

Critical Issues on Magnetic Reconnection in Space Plasmas

The idea of expedient energy transformation by magnetic reconnection (MR) has generated much enthusiasm in the space plasma community. The early concept of MR, which was envisioned for the solar flare phenomenon in a simple two-dimensional (2D) steady-state situation, is in dire need for extension to encompass three-dimensional (3D) non-steady-state phenomena prevalent in space plasmas in nature like in the magnetosphere. A workshop was organized to address this and related critical issues on MR. The essential outcome of this workshop is summarized in this review. After a brief evaluation on the pros and cons of existing definitions of MR, we propose essentially a working definition that can be used to identify MR in transient and spatially localized phenomena. The word “essentially” reflects a slight diversity in the opinion on how transient and localized 3D MR process might be defined. MR is defined here as a process with the following characteristics: (1) there is a plasma bulk flow across a boundary separating regions with topologically different magnetic field lines if projected on the plane of MR, thereby converting magnetic energy into kinetic particle energy, (2) there can be an out-of-the-plane magnetic field component (the so-called guide field) present such that the reconnected magnetic flux tubes are twisted to form flux ropes, and (3) the region exhibiting non-ideal MHD conditions should be localized to a scale comparable to the ion inertial length in the direction of the plasma inflow velocity. This definition captures the most important 3D aspects and preserves many essential characteristics of the 2D case. It may be considered as the first step in the generalization of the traditional 2D concept. As a demonstration on the utility of this definition, we apply it to identify MR associated with plasma phenomena in the dayside magnetopause and nightside magnetotail of the Earth’s magnetosphere. How MR may be distinguished from other competing mechanisms for these magnetospheric phenomena are then discussed.This revised version was published online in July 2005 with a corrected cover date.