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卫星故障诊断的最优奇偶向量法 总被引:5,自引:0,他引:5
提供一种卫星故障诊断方法以提高 GPS导航的完整性。该方法利用最优奇偶向量来检测和诊断卫星故障以提高卫星故障诊断的准确性。仿真结果显示,在故障幅值较小的情况下最优奇偶向量方法相比广义似然比方法可以提高故障的正确检测率和正确诊断率。该方法还可以缩短检测斜坡型故障的时间,从而提高了系统的可靠性。 相似文献
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针对传统RAIM算法很难检测微小伪距偏差的问题,可以通过对多个历元的统计检验量进行归一化处理,增大统计检验量的非中心化参数,提高对微小故障的检测率.Kalman新息检测法可以对卫星的故障进行独立检测,具有运算量小、在少星情况时仍能进行故障检测和识别的优点,但是对微小伪距偏差不敏感.针对两种方法的优点提出了基于Kalman滤波和奇偶矢量法的综合RAIM算法.仿真结果表明,该方法不仅可以提高对微小伪距偏差的检测率,同时减少了对可见卫星数的要求,验证了该算法应用于接收机自主完好性检测的可行性和正确性. 相似文献
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由于惯性导航系统和卫星导航系统具有良好的互补性与北斗导航系统的迅速发展,惯性/卫星紧组合导航系统得到广泛应用。但卫星导航系统的时变、易受干扰等特性,极易污染整个组合导航系统。因此,研究了一种新型的惯性/北斗紧组合导航系统的故障检测算法,在传统的卡方故障检测算法基础上,利用新息动态变化特性来识别故障星,并对故障星进行隔离,从而保证整个导航系统的稳定性与精度。最后基于嵌入式PC104平台,利用Qt Creator软件开发了多线程惯性/北斗紧组合导航系统,对所研究的算法进行了可靠验证。实验结果表明,所研究的故障检测算法能够有效地检测出卫星信号故障,能及时剔除故障星,大大降低了漏检、错检的概率,提高了整个导航系统的可靠性与精度。 相似文献
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为使惯性冗余系统达到故障检测与识别的功能,本文对惯性冗余系统的奇偶向量在有、无故障的不一致情况进行了研究,介绍了单自由度惯性仪表和双自由度惯性仪表广义似然比故障检测与隔离方法,通过对奇偶向量的分析及仿真,给出了最优化故障检测与隔离算法,该结果表明,采用奇偶向量法确实可以提高冗余惯性系统的故障检测与识别的性能,可以解决其软故障的检测能力。 相似文献
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针对多颗微小卫星合作接管失效卫星姿态运动的问题,研究了考虑微小卫星控制约束的多星合作博弈策略学习与协同控制方法。首先,建立了微小卫星合作博弈模型,给出了能够处理微小卫星控制约束的多星合作博弈帕累托最优策略显式表达式。其次,针对微小卫星合作博弈策略学习需求,通过过去与当前时刻数据的并行使用,设计了基于并行学习的策略迭代方法,该方法放松了神经网络(NN)权值矢量学习对持续激励条件的要求。给出了为确保神经网络权值矢量估值收敛,所使用的过去时刻数据所需满足的条件,并通过Lyapunov方法分析了神经网络权值矢量估计误差的一致最终有界性。之后,采用并行学习策略迭代方法进行了微小卫星合作博弈帕累托最优策略数值解的逼近。所获得的合作博弈策略具有反馈控制形式,在进行神经网络权值矢量学习后,各微小卫星能够通过合作博弈策略的独立计算实现失效卫星姿态运动接管过程中的闭环协同控制。所设计方法避免了传统姿态控制方法所需进行的力矩分配,消除了微小卫星数量对其控制计算复杂度的影响。最后,通过数值仿真对所设计方法的有效性进行了验证。 相似文献
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给出了一种非线性系统传感器的故障诊断方法。该方法将T-S 模糊模型、全解耦奇偶方程和参数估计相结合,同时对非线性系统的多个传感器的故障进行检测、隔离与识别。设计出用于产生残差的线性系统全解耦奇偶方程,并给出了全解耦奇偶向量的存在条件,全解耦奇偶方程产生的残差仅对一个传感器故障敏感,而对系统状态、扰动输入和其它传感器输出解耦。引入T-S 模型将全解耦奇偶方程推广到非线性系统中得到了模糊奇偶方程。传感器的故障模型表示为刻度因子和偏差的形式,根据残差信息应用卡尔曼估计方法可识别出故障模型的参数。最后给出了某型号飞机控制系统传感器的故障诊断仿真实例。 相似文献
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全电推进卫星星上自主变轨,是全电推进卫星重要的发展方向。为了获得运算量小、计算简单、可以星上计算且变轨时间最短的小推力变轨策略,研究了Lyapunov反馈制导律和推力矢量分段固定法两种方法。基于Lyapunov反馈制导律的变轨策略,权重系数在地面进行优化,推力指向星上实时计算,在标称任务工况下变轨时间比理论最优解加长8.18%。推力矢量分段固定法变轨策略更为简单,每10天星上对两个关键控制参数Ψ1,Ψ2进行修正,推力指向变化规律恒定,变轨时间比理论最优解加长7.43%。两种方法都具有任务适应性好和计算简单的优点,Lyapunov反馈制导律对姿态控制能力要求较高,推力矢量分段固定法姿态控制要求容易满足,后者更适合于卫星应用。 相似文献
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针对近地低轨三轴稳定卫星在轨管理后期,除磁强计外其他姿态敏感器都无效情况下的姿态异常问题,分析了三轴稳定卫星失去姿态基准后,星体自旋状态下三轴磁强计测量数据的特点,提出了使用磁强计测量数据的矢量信息,以找到能够获取卫星状态的方法,从而建立了磁强计测量矢量与卫星自旋轴的几何关系,给出了处于自旋状态下的卫星自旋轴确定方法。通过此种辨识方法,获得了某气象卫星姿态异常翻转状态下的自旋矢量方向和自旋角速度,从而证明了该辨识方法快速、有效,可以作为姿态异常卫星自旋状态的辨识手段,为恢复卫星姿态提供了重要信息,具有一定的工程应用价值。 相似文献
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编队飞行小卫星空间状态测量方法研究 总被引:1,自引:0,他引:1
介绍了编队飞行小卫星特点,提出了小卫星空间状态测量方案。着重论述了星间相对状态自主测量方法,计算了伪码和载波相位跟踪环路、时钟基准频差以及测量设备延迟带来的星间相对距离测量误差,讨论了降低误差的方法。在对误差项进行综合分析后,得出相对距离测量误差可达到厘米级的结论。 相似文献
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Investigation into navigation satellite on board clock frequency references and performance are reported. The focus is on the stability of the clocks aboard the NAVSTAR GPS (Global Positioning System) and GLONASS satellites as well as those used by their respective maser control stations and associated time scales. Allan-variance techniques have been applied to determine the long-term time-domain behavior of satellite clocks in an attempt to identify different regions of power spectral density. Coupled with analysis of relative-frequency drift over a period of many weeks, this behavior allows the type of satellite onboard standard to be tentatively identified. The known nature of the GPS clocks has shown that the different types of clocks aboard the satellites (crystal, rubidium, and cesium) are distinguishable given a sufficient sample time. The same approach has been applied to the GLONASS satellites, and a comparison of the results obtained from GPS has allowed conjecture on the type of clock used by the GLONASS satellites. It appears that GLONASS has used clocks of the quality of rubidium atomic oscillators since at least 1986, and that the quality and performance of onboard standards have increased steadily with time. Some current satellites perform well enough in terms of frequency drift, flicker FM noise floor, and long-term stability to compare favorably with the cesium beam standards carried on NAVSTAR GPS satellites launched in 1983-84 相似文献
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Low-Earth-Orbit(LEO) formation-flying satellites have been widely applied in many kinds of space geodesy. Precise Relative Orbit Determination(PROD) is an essential prerequisite for the LEO formation-flying satellites to complete their mission in space. The contribution of the BeiDou Navigation Satellite System(BDS) to the accuracy and reliability of PROD of LEO formation-flying satellites based on a Global Positioning System(GPS) is studied using a simulation method. Firstly, when BDS is added to GPS, the mean number of visible satellites increases from9.71 to 21.58. Secondly, the results show that the 3-Dimensional(3 D) accuracy of PROD, based on BDS-only, GPS-only and BDS + GPS, is 0.74 mm, 0.66 mm and 0.52 mm, respectively. When BDS co-works with GPS, the accuracy increases by 29.73%. Geostationary-Earth-Orbit(GEO) satellites and Inclined Geosynchronous-Orbit(IGSO) satellites are only distributed over the Asia-Pacific region; however, they could provide a global improvement to PROD. The difference in PROD results between the Asia-Pacific region and the non-Asia-Pacific region is not apparent. Furthermore, the value of the Ambiguity Dilution Of Precision(ADOP), based on BDS + GPS, decreases by 7.50% and 8.26%, respectively, compared with BDS-only and GPS-only. Finally, if the relative position between satellites is only a few kilometres, the effect of ephemeris errors on PROD could be ignored. However, for a several-hundred-kilometre separation of the LEO satellites, the SingleDifference(SD) ephemeris errors of GEO satellites would be on the order of centimetres. The experimental results show that when IGSO satellites and Medium-Earth-Orbit(MEO) satellites co-work with GEO satellites, the accuracy decreases by 17.02%. 相似文献
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卫星接收机自主完好性监测是指根据用户接收机的多余观测值监测用户定位结果的完好性,其目的是在导航过程中检测出发生故障的卫星,并保障导航定位精度。针对卫星接收机自主完好性监测算法可用性不足的问题,结合机载实际导航系统配置,提出了一种基于气压高度表辅助的机载自主完好性监测算法。综合利用卫星导航系统及气压高度表观测信息,建立联合系统的观测模型,推导了基于多解分离的完好性监测及保护级别计算方法。仿真结果表明,相比于传统的接收机自主完好性监测算法,该算法在可见星为5颗时仍能识别故障卫星。该算法具有更好的故障检测能力及可用性,能有效提高卫星导航系统的完好性监测性能,从而保证卫星导航系统的精度和可靠性。 相似文献
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B. A. Smith G. A. Briggs G. E. Danielson A. F. Cook II M. E. Davies G. E. Hunt H. Masursky L. A. Soderblom T. C. Owen C. Sagan V. E. Suomi 《Space Science Reviews》1977,21(2):103-127
The overall objective of this experiment is exploratory reconnaissance of Jupiter, Saturn, their satellites, and Saturn's rings. Such reconnaissance, at resolutions and phase angles unobtainable from Earth, can be expected to provide much new data relevant to the atmospheric and/or surface properties of these bodies. The experiment also has the following specific objectives:Observe and characterize the global circulation of the atmospheres of Jupiter and Saturn;Determine the horizontal and vertical structure of the visible clouds and establish their relationship to the belted appearance and dynamical properties of the planetary atmospheres;Determine the vertical structure of high, optically-thin, scattering layers on Jupiter and Saturn;Determine the nature of anomalous features such as the Great Red Spot, South Equatorial Belt disturbances, etc.;Characterize the nature of the colored material in the clouds of Jupiter and Saturn, and identify the nature and sources of chromophores on Io and Titan;Perform comparative geologic studies of many satellites at less than 15-km resolution;Map and characterize the geologic structure of several satellites at high resolution (1 km);Investigate the existence and nature of atmospheres on the satellites;Determine the mass, size, and shape of many of the satellites by direct measurement;Determine the direction of the spin axes and periods of rotation of several satellites, and establish coordinate systems for the larger satellites;Map the radial distribution of material in Saturn's rings at high resolution;Determine the optical scattering properties of the primaries, rings, and satellites at several wavelengths and phase angles;Search for novel physical phenomena, e.g., phenomena associated with the Io flux tube, meteors, aurorae, lightning, or satellite shadows.Team leader.Deputy team leader. 相似文献
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针对2012年5月21日某低轨卫星受到月影干扰导致控制系统工作异常的问题,分析了月影现象产生原理,结合月影期间影响卫星安全的异常原因,系统分析了卫星平台能源预警机制与驱动控制系统中的太阳帆板控制方案,提出了某型号低轨卫星应对月影现象安全运行的处置方法和后续同类型卫星能源管理修改建议.该方法分别在2012年11月9日、2013年5月10日得到应用,在月影期,该卫星太阳阵输出电流从4.5A下降到2A,太阳帆板对日转动正常,能源管理系统未出现报警.应用结果说明,该方法能够有效地解决同类型卫星月影干扰的问题. 相似文献
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天基测控模式是航天器测控发展的必然趋势.天基测控模式与地基测控模式有着本质的区别,如何实现天基测控是我国航天领域目前研究的重点课题之一.本文在分析天基测控技术和我国现有条件的基础上,提出了实现航天器天基测控的方法,分析研究了与航天器天基测控中心相关的关键技术。 相似文献