Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

对接口匹配的航天器双主动最优交会研究

研究了两航天器协同轨道机动（双主动）完成近距离交会任务的最优控制问题。在考虑航天器姿态变化、对接口位置及路径约束的情况下,构建了完整的6自由度、26状态的双主动最优交会数学模型。利用高斯伪谱法分别将燃料总消耗最少和交会时间最短两种最优问题离散为大型非线性规划问题,而后应用SNOPT软件包进行了求解。在此基础上通过大量数值计算分析总结了不同初始参数对最小燃料消耗和最短交会时间的影响规律,并与主被动交会形式进行了对比。结果表明,当两航天器质量接近时,双主动交会通常可明显减少燃料消耗,或缩短交会时间;而当质量差距较大时,双主动最优交会逐渐退化为主被动最优交会。     

Global ionospheric scintillations revealed by GPS radio occultation data with FY3C satellite before midnight during the March 2015 storm

Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively.     

光学基片表面软质抛光胶体粒子的激光清洗

介绍了光学基片表面软质抛光胶体粒子激光清洗的基本方法、原理和实验装置,并通过对含有污染微粒的基片表面进行激光清洗,获得了高洁净表面的光学基片.     

大气层内模型预测静态规划拦截中制导

在临近空间机动目标拦截中,拦截器的初始动力段对中制导段乃至末端拦截性能具有重要影响。在模型预测静态规划（MPSP）理论基础上提出了一种初、中制导联合规划制导方法,旨在解决多阶段、快速、最优拦截轨迹规划和制导问题。首先,提出了一种改进的模型预测静态规划方法,该方法不仅可以满足终端约束,还可以生成最优初始状态,并在性能指标中考虑状态变量相关函数。其次,基于等效阻力模型建立了包含动力段与非动力段的两段规划模型,通过采用分段离散以及构建关机点变分关系的方法,避免了内点约束的引入,使MPSP算法可直接求解该两段规划问题。最后,结合提出的MPSP算法以及两段规划模型,实现了终端速度最优的拦截轨迹规划,结合目标预测方法,实现了对机动目标的预测拦截。仿真结果表明,本文方法可提高制导精度和终端速度,且能更好满足对机动目标的拦截需求。     

不同载荷方式下MDYB-3有机玻璃的变形与破坏行为

 为了理解和评价MDYB-3定向有机玻璃的力学行为,采用CSS44100电子万能试验机,分离式Hopkinson技术和MTS液压伺服试验机分别进行了5种不同类型的力学试验。这些试验包括力学各向异性试验、穿孔试验、应变率从0.001 s^-1到 2 000 s^-1和初始温度从218 K 到 373 K的单轴拉、压试验、等幅应力控制下不同应力集中系数的双边缺口试样疲劳试验。同时采用光学显微镜对变形试样的破坏和断裂进行了观察和分析。结果表明：①MDYB-3定向有机玻璃呈现明显的各向异性性能;②沿板面法线方向MDYB-3定向有机玻璃具有更高的硬度和强度,在穿孔或冲击条件下它以脆性分层破裂和散落为破坏形式;③MDYB-3定向有机玻璃的力学响应强烈地依赖于应变率和温度,且在拉伸和压缩加载下表现出很大的强度非对称性;④双边带有缺口试样的S-N曲线表明,最大应力幅值较低时,MDYB-3定向有机玻璃的疲劳寿命对缺口不敏感。在循环载荷下裂纹起源与微层特性及层间强度有关,它起源于层间可处在缺口中段部位,最后文中对变形与破坏机理也进行了分析和讨论。     

金属橡胶减振器用于发动机安装减振的研究

 为减小发动机传递至飞机机身结构的振动,设计了金属橡胶减振器用于航空发动机安装。对该金属橡胶减振器进行了动力学建模研究,采用有限元技术对安装减振器前后的飞机全机结构进行了仿真分析,初步表明了该设计对结构频率影响较小,但能引入较大阻尼,降低响应水平。在理论分析基础上,进一步将设计制造的金属橡胶减振器安装于某型飞机,进行地面开车,实测了应用减振安装前后飞机的动力学响应。结果证明了发动机减振安装的可行性与有效性。     

低碳硅锰系TRIP钢热处理工艺的研究

仅含碳、硅、锰合金元素的结构钢,采用临界区等温淬火热处理工艺,得到铁素体、贝氏体和残余奥氏体三相组织。该钢在 Ｍｓ（马氏体转变开始温度）～Ｍｄ（马氏体转变终止温度）ｄ温度之间形变,应变诱导相变,相变诱发塑性──ＴＲＩＰ,其力学性能指标大大提高。本文通过显微组织观察,力学性能结果分析,对这种低碳硅锰系ＴＲＩＰ钢三种不同的热处理工艺制度进行了研究。     

涡轴发动机尾气静电监测信号影响因素分析

 针对某型航空涡轴发动机试车台实验所获得的尾气静电监测信号,结合发动机台架试车状态和性能数据,分别在两个时间尺度上展开分析研究。研究发现发动机的工作状态和健康状态均对尾气静电信号产生重要影响。在小时间尺度上的分析发现,无故障情况下影响尾气静电信号变化的主要因素为燃油供给量,尾气静电信号能量随燃油供给量的增加近似按指数规律上升;而在大时间尺度上的分析发现,在一定的燃油供给和恒定的自由涡轮转速条件下,尾气静电信号能量随着发动机性能的缓慢衰退而逐渐上升。实测尾气静电信号所反映的趋势与初步的理论分析结果相一致,为建立涡轴发动机尾气静电信号的健康"基线",进而用于气路状态监测及故障识别提供了初步的依据。研究还发现,静电监测技术不仅能够为突发性故障提供预警信息,而且能够反映发动机整机性能衰退,进一步拓展了静电传感器的监测能力及其在航空发动机健康管理中的应用。