排序方式： 共有9条查询结果，搜索用时 241 毫秒
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在低精度MEMS-IMU和GPS组合导航中,由于IMU的精度问题,无法通过传统的解析方法实现方位失准角的粗对准,造成了大方位失准角问题,从而导致系统的强非线性。通过变换状态量,用方位失准角的两个三角函数代替方位失准角作为状态量,建立了新的线性系统方程。用改进奇异值分解法对新对准系统进行可观测度分析,完成了车载导航试验,结果表明：本初始对准方案在低精度的组合导航中具有很好的对准精度和对准速度。 相似文献
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This study explored the impact of coastal radar observability on the forecast of the track and rainfall of Typhoon Morakot(2009)using a WRF-based ensemble Kalman filter(EnKF)data assimilation(DA)system.The results showed that the performance of radar EnKF DA was quite sensitive to the number of radars being assimilated and the DA timing relative to the landfall of the tropical cyclone(TC).It was found that assimilating radial velocity(Vr)data from all the four operational radars during the 6 h immediately before TC landfall was quite important for the track and rainfall forecasts after the TC made landfall.The TC track forecast error could be decreased by about 43% and the 24-h rainfall forecast skill could be almost tripled.Assimilating Vr data from a single radar outperformed the experiment without DA, though with less improvement compared to the multiple-radar DA experiment.Different forecast performances were obtained by assimilating different radars, which was closely related to the first-time wind analysis increment, the location of moisture transport, the quasi-stationary rainband, and the local convergence line.However, only assimilating Vr data when the TC was farther away from making landfall might worsen TC track and rainfall forecasts.Besides, this work also demonstrated that Vr data from multiple radars, instead of a single radar, should be used for verification to obtain a more reliable assessment of the EnKF performance. 相似文献
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将星载时钟钟差增广为状态向量,根据非线性系统的可观性秩条件判据,从理论上证明了利用X射线脉冲星进行同步定位/授时是可观的,为X射线脉冲星自主导航的工程应用提供了理论依据。 相似文献
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当前的重力卫星任务除了本身特有的观测方式外，都采用了高低卫卫跟踪的观测方式。为研究高低卫卫跟踪观测系统的时变行为和获取重力场信息的能力，文中运用描述时变系统的状态空间模型方法，根据附加参数的类型，建立了3种状态空间模型，并对系统的可观测性从解析法的角度进行了分析。结果表明，对于单一的高低卫卫跟踪观测系统，引力系数的可观测性实际上是不成立的，根据一次任务只能建立引力系数的一组约束条件。 相似文献
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Kalman filtering for stochastic dynamic tidal models, is a hyperbolic filtering problem. The questions of observability and stability of the filter as well as the effects of the finite difference approximation on the filter performance are studied. The degradation of the performance of the filter, in case an erroneous filter model is used, is investigated. In this paper we discuss these various practical aspects of the application of Kalman filtering for tidal flow identification problems. Filters are derived on the basis of the linear shallow water equations. Analytical methods are used to study the performance of the filters under a variety of circumstances. 相似文献
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We systematically surveyed the orbits of short-period (SP) comets that show a large change of perihelion distance (q) between 1–2 AU (visible comets) and 4–5 AU (invisible comets) during 4400 years. The data are taken from Cosmo-DICE (Nakamura and Yoshikawa 1991a), which is a long-term orbital evolution project for SP comets. Recognizing that q is the most critical element for observability of comets, an invisibility factor (f), defined as the ratio of unobservable time span to observable span during 4400 years, is calculated for each of the large-q-change comets. A detection limit for each comet is obtained from the heliocentric distance at discovery and/or the absolute magnitude at recent apparitions. A mean f value for 35 SP comets with 2.9 J (J is the Tisserand's invariant) is found to be 19.8. This implies that for each visible SP comet of this J-range, at every epoch of time, there exist about 20 invisible comets near the capture orbits by Jupiter, under the assumptions of steady-state flux and ergodicity for the SP-comet population. 相似文献
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