RN-FD型固体氡气源的稳定性及应用分析

对测氡仪器进行精确校准是氡测量工作中的重要环节,固体氡气源的稳定性、可靠性在校准中则显得至关重要。本文通过分析RN-FD型固体氡气源对闪烁室K值的稳定性实验结果,认为:RN-FD型固体氡气源标称的浓度值与实际浓度值不一致,标称浓度值只是理论浓度值而不是实际浓度值,需重新刻度才能使用;RN-FD型固体氡气源抽气循环时间不同则浓度不同,但抽气循环时间固定,观测结果比较稳定;对于没有α检查源的台站,RN-FD型固体氡气源可用于氡观测仪器坪区检查。     

高温环境下大尺度薄壁结构的电性能优化设计

考虑温度引起的热变形和材料电磁参数变化对天线罩电性能的影响,基于口径积分-表面积分法(AI-SI)和有限元法(FEM),提出了高温环境下天线罩电性能分析方法;进而基于粒子群算法(PSO),建立了计及热效应的天线罩结构电性能优化流程。分别选取常温环境、均匀高温环境和非均匀高温环境三种典型工况,对比研究了温度对天线罩电性能的影响规律,并对天线罩电性能进行了优化,研究结果表明:高温会引起天线罩透波系数的下降和瞄准误差的上升,在天线罩优化设计中应重视温度对电性能的影响;计及热效应的天线罩结构电性能优化方法能显著提升天线罩的透波系数、降低瞄准误差,具有良好的优化效果。     

同步误差条件下的空间目标双基地ISAR自聚焦算法

以空间目标为研究对象，针对双基地雷达时间、空间及频率同步误差导致的逆合成孔径雷达图像散焦问题，提出基于离散多项式相位变换的自聚焦算法。算法首先将目标平动、转动及同步误差导致的相位项统一建模为高阶多项式，利用离散多项式相位变换方法估计高阶多项式系数并据此构建补偿相位项，完成高阶相位补偿。最后进行方位压缩得到高聚焦度的二维ISAR像。算法通过选取合适的延时参数及成像积累时间可得到高精度参数估计及相位补偿，理论分析和仿真校验了算法性能优于常用的非参数化自聚焦算法。     

一种GPS抗干扰及干扰DOA估计工程集成方法

卫星导航干扰对消技术和干扰测向技术是卫星导航干扰对抗的两个典型方向,并逐渐成为当前卫星导航抗干扰装备的标配功能。如何实现干扰对消和干扰测向的高效集成成为制约工程实现的主要瓶颈之一。提出一种GPS抗干扰及DOA估计的工程集成方法,通过优化噪声子空间估计工程实现,实现了高性能抗干扰和高精度干扰测向的高效集成,与抗干扰模块和干扰测向模块相比,集成模块极大降低了工程实现资源。测试结果表明该方法可以有效对抗干信比60dB的干扰,并提供2度的测向精度。     

一种适用于封闭场景下的遥测信号接收方法

常规的遥测信号接收多是在开阔场景进行,被测对象除了在起飞或降落时短暂低仰角,大部分时间其信号是视距传输,其遥测信道近似于高斯白噪声信道。随着遥测应用场景的逐步扩展,封闭场景下的遥测需求逐步被提出,应用模式和信道条件发生了巨大变化。针对某封闭场景,分析常规遥测接收方法存在的一些问题,提出一种双天线加盲均衡的分集合成和接力接收方案,有效解决了封闭场景下的遥测信号中断问题。方案成功应用于某测试系统,实测结果表明,方案能够极大提升遥测系统的健壮性。     

航天器近距离交会的固定时间终端滑模控制

针对航天器近距离交会段的位置姿态耦合控制问题，假设航天器受外界干扰且目标航天器存在空间自由翻滚情形时，基于固定时间概念设计了一种六自由度位姿终端滑模自适应控制器，通过引入显含正弦函数的切换项来避免奇异问题。此外所设计的控制器含双幂次项，不仅能全局提高姿态和位置的跟踪速度及精度，还能估计系统稳定所需的时间上界，且该上界与状态初始值无关。基于Lyapunov方法分析了闭环系统的固定时间稳定性。仿真结果表明，该控制器能快速实现对航天器近距离交会时相对位置和姿态的控制，具有较高的精度和良好的干扰抑制能力。     

环雄安新区康养人才培养模式探讨

康养产业在国内尚属于新型的一个产业,而中国的康养产业发展迅速,显示出了勃勃的生机和巨大的发展潜力,但同时也出现了很多问题,其中人才培养是重要的一个环节。当前高等院校在康养行业专业人才培养方面,已经进行了许多探索和尝试,但就整体而言,我国康养行业高校人才培养还存在诸多问题。本文通过分析国内康养人才培养的现状,同时结合雄安新区的实际情况,提出环雄安新区康养人才培养的策略。     

The Kumtag meteorite strewn field

The Kumtag meteorite strewn field was found in the Kumtag desert, 132 km south of Hami city in the Xinjiang province, China. It is an ellipse of 2.5 × 7.9 km, with a long axis extending along the northeast-southwest direction. The largest individual meteorite of the strewn field weighs about 10 kg; the smallest individual has a mass of only 27 g. In total, more than 100 individuals with a total mass of more than 180 kg were collected. The location and the distribution of the fragments suggest that the Kumtag meteoroid entered the atmosphere in the direction Northeast-Southwest. All meteorites collected in this strewn field are samples from the same unique meteorite shower. The Kumtag meteorite is an H5 ordinary chondrite with a shock stage S2, and a weathering grade W2. The cosmic ray exposure age of Kumtag is 6.7 ± 0.8 Ma, which is rather typical for H chondrites and which indicates that Kumtag was derived from the massive impact event on its parent body ~7 Ma ago. A significant amount of He has been lost during certain unknown processe(s) before the Kumtag meteorite was ejected from its parent body.     

Orbit determination and prediction of GEO satellite of BeiDou during repositioning maneuver

In order to establish a continuous GEO satellite orbit during repositioning maneuvers, a suitable maneuver force model has been established associated with an optimal orbit determination method and strategy. A continuous increasing acceleration is established by constructing a constant force that is equivalent to the pulse force, with the mass of the satellite decreasing throughout maneuver. This acceleration can be added to other accelerations, such as solar radiation, to obtain the continuous acceleration of the satellite. The orbit determination method and strategy are illuminated, with subsequent assessment of the orbit being determined and predicted accordingly. The orbit of the GEO satellite during repositioning maneuver can be determined and predicted by using C-Band pseudo-range observations of the BeiDou GEO satellite with COSPAR ID 2010-001A in 2011 and 2012. The results indicate that observations before maneuver do affect orbit determination and prediction, and should therefore be selected appropriately. A more precise orbit and prediction can be obtained compared to common short arc methods when observations starting 1 day prior the maneuver and 2 h after the maneuver are adopted in POD (Precise Orbit Determination). The achieved URE (User Range Error) under non-consideration of satellite clock errors is better than 2 m within the first 2 h after maneuver, and less than 3 m for further 2 h of orbit prediction.