J2轨道模型对月地激光通信预瞄准精度影响研究

基于J_2轨道预测模型,设计了不同倾角和轨道高度圆轨道月球卫星,通过将J_2轨道预测模型预瞄准仿真结果与直接积分RKF7(8)法仿真结果相对比,研究了不同类型月球卫星轨道对-Y面卫星舱板激光通信终端瞄准精度的影响。仿真结果表明,J_2轨道预测模型可以满足月球极地卫星月地激光通信要求,当轨道高度为1 000 km和2 000 km的时候,10 min方位角偏差不超过40μrad,而俯仰角偏差仅为7μrad时,在一定程度上J2轨道预测模型可以满足月地激光通信预瞄准要求。     

一种应用于实时深空干涉测量的电离层时延修正方法

针对"嫦娥4号"中继星任务S频段信标信号的高精度实时干涉测量需求,结合深空测控干涉测量系统采用的稀疏标校工作模式,研究验证了一种面向测控模式实时干涉测量的电离层时延修正方法。首先分析了电磁波经电离层传播的延迟机理及特性;基于深空站历史观测数据,通过自相关函数分析验证了天顶向TEC的周日特性;在此基础上,结合深空干涉测量中心数据处理设备软件系统,讨论了电离层时延修正方法;通过任务期间的实测数据处理分析,验证了所提方法可以将实时测量精度提升1～3 ns,对低仰角跟踪弧段,该技术方法优势更为明显。该方法为后续深入推进深空测控干涉测量系统在任务中的实时应用提供了技术储备。     

“龙江2号”月球轨道微卫星定轨分析

微纳卫星深空探测任务中,通常所分配的测控资源有限,因此有必要对有限测控资源条件下微纳卫星的定轨精度进行分析。以微纳卫星深空探测为背景,采用"龙江2号"微卫星的轨道测量数据对其定轨精度进行了分析。"龙江2号"微卫星只有USB轨道测量数据,且环月段测控资源相对紧张,每天有两站跟踪,共约3～4 h的轨道测量数据。首先介绍了"龙江2号"微卫星飞行任务及其飞行过程中影响测定轨的因素;其次给出了定轨的动力学模型,对微卫星地月转移段的定轨精度进行了分析;最后通过分析摄动力、动量轮卸载以及数据弧段长度的影响,给出了微卫星环月阶段所使用的定轨策略,并通过重叠弧段比较的模式,给出了微卫星环月段的定轨精度。研究结论可以为后续微纳卫星深空探测任务提供有益参考。     

基于光纤耦合金刚石NV色心系综磁强计的电路诊断方法

为考查应用新型磁强计——金刚石氮空穴(nitrogen-vacancy,NV)色心系综磁强计进行电路诊断的可行性和可靠性,从金刚石NV色心系综磁强计的基本原理出发,搭建了一套光纤耦合金刚石NV色心系综磁强计测试实验系统,将探头紧贴于电路导线外壳,通过测量磁强计处磁场信号的变化实现对电路的诊断.实验结果表明,金刚石NV色...     

载人航天器密封系统漏率设计方法

载人航天器密封舱为航天员提供在轨生活、工作的环境,对密封舱及其环控生保系统、热控制系统、推进控制系统等中各管路的密封性能有严格要求。文章提出了一种漏率设计方法,建立了相应的漏率检测系统,并依据该方法制定了密封舱体和各管路的漏率设计和指标分配的流程。本流程可用作载人航天器舱体密封系统、管路密封系统的漏率设计,对保证载人航天器在轨安全可靠运行有重要参考价值。     

航空发动机第1级风扇叶片鸟撞研究

针对目前对鸟体撞击风扇部位影响分析不全的问题,计算了鸟体飞向叶片不同部位和穿过支板间隙的概率,在此基础上分析了鸟体撞击旋转状态第1级风扇叶片不同位置的概率。基于数值模拟技术,建立了鸟体撞击叶片的有限元模型,模拟鸟撞击风扇叶片叶尖、叶中、叶根部位,在分析引起叶片不同位置塑性变形的基础上,进一步确定了风扇损伤最大的位置。针对4种不同的鸟体撞击速度,对发动机第1级风扇叶片鸟体撞击部位损伤进行了分析。得到鸟体穿过叶尖部位支板间隙的概率约为50%,撞击叶尖部位概率约为16.7%,是最容易撞击的部位,受到的损伤也较大。计算结果可以为确定发动机风扇叶片鸟体撞击损伤提供参考。     

无人自转旋翼机建模与控制方法研究

以500kg级无人自转旋翼机为研究对象,研究了样例无人旋翼机的建模和自动飞行控制技术.首先,基于解析形式叶素积分法给出自转旋翼机的建模方法,并给出了样例旋翼无人机的数学模型;然后,设计了无人旋翼机的俯仰和滚转控制律,并在此基础上设计了速度、高度及侧偏控制律.最后,通过飞行试验验证了模型的准确性及控制律的有效性.     

Study of ionospheric D region changes during solar flares using MF radar measurements

During solar flares, the X-ray radiation suddenly increases, resulting in an increase in the electron density of the atmospheric D region and a strong absorption of short-wave radio waves. Based on Langfang medium frequency (MF) radar, this paper analyzed the variation characteristics of D region in the lower ionosphere from 62 km to 82 km. The analysis focused on multiple C-level and M-level solar flare events before and after the large-scale flare event at 11:53 (UT) on September 6, 2017. The results show that it is difficult to detect the electron density over 70 km in Langfang during solar flares, but the electron density value can be obtained as low as 62 km, and the stronger the flare intensity, the lower the detectable electron density height. Besides, the equal electron density height, the received power of X and O waves will also be significantly reduced during the flares, and the reduction of equal electron density height has a weak linear relationship with flare intensity.     

超细CL‑20的可控批量制备及降感技术

为了批量制备低感度超细六硝基六氮杂异伍兹烷(CL-20),用作固体推进剂的高能添加剂,以氧化锆球(0.8 mm或0.3 mm)为研磨介质,采用HLG-05型粉碎设备制备了两种超细类球形CL-20。用激光粒度仪、扫描电子显微镜(SEM)、X射线衍射(XRD)、傅里叶红外光谱(FTIR)和拉曼光谱(Raman)对CL-20样品进行了相应的表征;用差示扫描量热(DSC)研究了样品的热分解性能;测试了样品的撞击、摩擦和静电火花感度。结果表明:制备的微米级和亚微米级CL-20平均粒径分别为3.43μm和320 nm,表面光滑,类球形;其晶型不变,无质杂峰;超细CL-20的分解峰温稍有下降,活化能降低,其静电火花感度略有提高,但撞击感度分别降低了24.6%和108.4%,摩擦感度下降了8%和20%;机械感度降低效果明显,在高能固体推进剂中有较大的应用前景。     

Ground experiments of Chang’e-5 lunar regolith penetrating radar

The Lunar Regolith Penetrating Radar (LRPR) is an Ultra-Wideband (UWB) array-based Ground penetrating radar (GPR) onboard the lander of Chang’e-5 (CE-5) mission. The primary scientific objectives of the LRPR are to probe the thickness and structure of lunar regolith of the landing site, and support the drilling and sampling process. In order to evaluate the performance of the LRPR, a series of ground experiments are performed using the LRPR prototype mounted on a CE-5 lander model. The performance of the LRPR is evaluated by comparing the experimental data with the simulated data. Data processing and imaging method are verified, and the interferences from the lander and other aspects are analyzed. The results of the ground experiments and simulation demonstrate that the LRPR is able to meet the design requirement of 2-m detection depth. They also indicate that the upper and lower interfaces of the stratified structure in the lunar regolith can be well distinguished by the LRPR when the dielectric constant difference is greater than 0.3, and the imaging effect of the location under the dense antennas is better than that of other positions. However, the identification capability of the LRPR to the independent blocky objects is relatively poor mainly due to the clutters caused by the lander, the sparsity of the antenna elements compared to the size of the basalt block, the limited aperture of the antenna array, and the tail of the transmitted waveform.