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91.
为了研究空间微小碎片碰撞对航天器的影响,国内外研制了各种类型的微小碎片加速器。文章简要介绍了一种很有前景的静电式微小碎片加速器及其关键部件的工作原理、结构特点及适用范围等。 相似文献
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以惠普尔(Whipple)防护屏结构为例,通过实验研究了铝合金柱状弹体以第一门槛值附近速度斜撞击LY12合金防护屏的特点,研究了不同速度下,不同撞击角度下,防护屏损伤的变化规律,对于速度在第一门槛值附近的斜撞击,以斜撞击存在一个临界入射角度,当入射角度大于临界入射角度时,发生滑弹现象,入射角度越大,产生的滑弹碎片数量就越多。 相似文献
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Bao-Jun Pang Dong-Fang Wang Wei-Ke Xiao Bin-Bin Lu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(8):2274-2281
The availability of engineering models to estimate the risk from space debris is essential for space missions. According to current research, cumulative flux calculation is mostly carried out based on the equal-width interval discretization. The method discretizes the volume around the Earth into cells defined in earth centered inertial coordinates. The resulting debris flux onto a target object is shown to depend on the chosen size of the cells. To avoid a discretization error, this must be accounted for. In order to present reliable flux predictions for space mission, the algorithm improvement is an ongoing topic for the related research field. The aim of this study was to examine the discretization error during the cumulative flux determination process. Both the effect of interval step length and the orbital boundary are under investigation. Several typical orbits are selected as examples here and the 2018/01/03 TLE (Two Line Element) data published by the US Space Surveillance Network is used as the debris background in this paper. Furthermore, the Interval Distance-Based method for Discretization (IDD) is adopted in this paper. A position-centered flux determination method is introduced based on the IDD method. According to the example analysis, the IDD used in the flux calculation process provides results which are less affected by the interval step-size setup; and the orbital boundary has no effect on the calculation process. In other words, the discretization error is significantly reduced. The position-centered method provided a possible suggestion for the improvement of space debris environment models. 相似文献
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在卫星/惯性(GNSS/INS)组合导航系统中,针对基于残差检测的完好性监测算法对于缓变误差检测效果不佳,以及自主完好性监测外推(AIME)法存在检测时延的缺陷,提出了一种基于抗差估计改进的完好性监测方法.该方法在AIME法的基础上,通过定义标准化残差,引入三段权函数抗差估计对AIME法进行改进,并设计了一种调节准则,实现在不同情况下采用不同的检测方式.最后通过搭建仿真平台对所提方法进行验证,仿真结果表明,该方法可有效降低组合导航系统完好性监测的误警率和告警时间,提高卡尔曼滤波估计精度和组合导航系统对缓变误差的检测性能. 相似文献
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Ershen Wang Chaoying Jia Gang Tong Pingping Qu Xiaoyu Lan Tao Pang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(5):1260-1272
The receiver autonomous integrity monitoring (RAIM) is one of the most important parts in an avionic navigation system. Two problems need to be addressed to improve this system, namely, the degeneracy phenomenon and lack of samples for the standard particle filter (PF). However, the number of samples cannot adequately express the real distribution of the probability density function (i.e., sample impoverishment). This study presents a GPS receiver autonomous integrity monitoring (RAIM) method based on a chaos particle swarm optimization particle filter (CPSO-PF) algorithm with a log likelihood ratio. The chaos sequence generates a set of chaotic variables, which are mapped to the interval of optimization variables to improve particle quality. This chaos perturbation overcomes the potential for the search to become trapped in a local optimum in the particle swarm optimization (PSO) algorithm. Test statistics are configured based on a likelihood ratio, and satellite fault detection is then conducted by checking the consistency between the state estimate of the main PF and those of the auxiliary PFs. Based on GPS data, the experimental results demonstrate that the proposed algorithm can effectively detect and isolate satellite faults under conditions of non-Gaussian measurement noise. Moreover, the performance of the proposed novel method is better than that of RAIM based on the PF or PSO-PF algorithm. 相似文献
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