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41.
为了消除舰尾流对载机着舰过程产生的影响,同时完成低动压状态下飞行速度与高度的解耦工作,基于定量反馈理论/总能量控制理论(QFT/TECS)设计了纵向着舰控制系统。针对着舰过程中数学模型所具有的不确定因素及舰尾流对下滑航迹的影响,以载机高度变化率为控制对象,使用定量反馈理论结合推力补偿系统进行了内回路鲁棒控制律设计。外回路控制律设计是以总能量控制理论为基础,通过粒子群优化算法对待调控制参数进行寻优,进而实现了对高度、速度等参数的精确控制,完成了载机纵向着舰轨迹与速度的解耦工作。仿真结果表明,该控制律在拥有较强的鲁棒性的基础上具有良好的解耦控制能力,实现了载机着舰段的高度与速度的解耦控制,明显提高了载机对着舰轨迹的跟踪能力,可满足不确定条件下载机的着舰要求。 相似文献
42.
I.S. Batista M.A. Abdu Paulo A.B. Nogueira R.R. Paes J.R. de Souza B.W. Reinisch V.H. Rios 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
This study reports on ionospheric disturbances that occurred in the early morning hours in the South American–Atlantic sector during a few intense/super storm events. The events were observed at latitudes close to the southern crest of the equatorial ionization anomaly (EIA) as an unusual intensification of the F region electron density peak at local times when the EIA is not usually developed. All the events were observed at pre dawn-morning hours, under conditions of northward interplanetary geomagnetic field. Large scale traveling ionospheric disturbances that are launched during highly disturbed conditions and/or equatorward surges in the thermospheric meridional winds seem to be the most probable causes of the observed disturbances. 相似文献
43.
P.V.S. Rama Rao K. VenkateshD.S.V.V.D. Prasad K. Niranjan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Indian sector encompasses the equatorial and low latitude regions where the ionosphere is highly dynamic and is characterized by the equatorial ionization anomaly (EIA) resulting in large latitudinal electron density gradients causing errors and uncertainties in the estimation of range delays in satellite based navigation systems. The diurnal and seasonal variations of standard deviations in the TEC data measured during the low sunspot period 2004–2005 at 10 different Indian stations located from equator to the anomaly crest region and beyond are examined and presented. The day-to-day variability in TEC is found to be lowest at the equatorial station and increases with latitude up to the crest region of EIA and decreases beyond. 相似文献
44.
GPS广域增强系统电离层延迟网格修正算法的研究 总被引:5,自引:0,他引:5
建立了一种广域增强系统地面监测网对电离层延迟的观测数据生成网格修正值算法,并在天津,长春,西安三地通过用双频接收机同时采集的电离层延迟实测数据,对广域增强系统的电离层网格修正法的修正精度进行验证,并与一般用户目前采用的Klobuchar模型修正法进行了比较,结果表明,电离层延迟网格修正法的修正精度普遍大于80%,优于Klobuchar模型修正法,是一种精度较高的电离层实时修正法。 相似文献
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将最大熵动态互普方法用于高频多普勒台阵数据处理,从覆盖太阳活动高、低年份的高频多普勒台阵观测数据中,得出了中国中部地区电离层声重波扰动的传播方向、时空尺度等参量之间的统计分布特性,进而探讨了有关扰动源的情况,结果表明,极区源和局地源两种不同的激发源所激发的声波,分别反映了电离层扰动的全球传播和地区特性两种不同的特征。 相似文献
47.
Fengsi Wei Xueshang Feng Xu Ya Quanlin Fan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2363-2367
A so-called “ISF” prediction method for geomagnetic disturbances caused by solar wind storms blowing to the Earth is suggested. The method is based on a combined approach of solar activity, interplanetary scintillation (I) and geomagnetic disturbance observations during the period 1966–1982 together with the dynamics of solar wind storm propagation (S) and fuzzy mathematics (F). It has been used for prediction tests for 37 geomagnetic disturbance events during the descending solar activity phase 1984–1985, and was presented in 33rd COSPAR conference. Here, it has been improved by consideration of the three dimensional propagation characteristics of each event, the search for the best radio source and the influence of the southward components of interplanetary magnetic fields on the geomagnetic disturbances. It is used for prediction tests for 24 larger geomagnetic disturbance events that produced space anomalies during the period 1980–1999. The main results are: (1) for the onset time of the geomagnetic disturbance, the relative error between the observation, Tobs, and the prediction, Tpred, ΔTpred/Tobs 10% for 45.8% of all events, 30% for 78.3% and >30% for only 21.7%; (2) for the magnetic disturbance magnitude, the relative error between the observation, ∑Kp,obs, and the prediction, ∑Kp,pred, Δ∑Kp,pred/∑Kp,obs 10% for 41.6% of all events, 30% for 79% and 45% for 100%. This shows that the prediction method described here has encouraging prospects for improving predictions of large geomagnetic disturbances in space weather events. 相似文献
48.
BD2系统广域差分格网电离层模型研究与应用 总被引:1,自引:0,他引:1
电离层延迟误差是影响BD2卫星导航系统定位测速精度的关键因素,如何减少电离层误差是当前卫星导航定位领域研究的热点问题.常见的电离层模型包括广域差分格网模型和Klobuchar模型,已有研究主要关注Klobuchar模型,对BD2广域差分格网模型的研究较少.本文分析比较了广域差分格网电离层模型和Klobuchar模型对电离层延迟误差的影响,并进行了真实环境下的评测.实验结果表明,使用广域差分格网电离层模型修正电离层延迟可以减小电离误差,从而提高单频接收机导航定位精度. 相似文献
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50.
Mikhail E. Gushchin Sergey V. KorobkovAlexander V. Kostrov Mikhail V. StarodubtsevAskold V. Strikovsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Modulation of whistler waves in a plasma with time-dependant magnetic field perturbations was investigated experimentally. The experiments were performed on large “Krot” device, which was specially designed to study space plasma physics phenomena. It is shown that magnetic field variations on the wave propagation path can lead to splitting of initially continuous whistler wave into the sequence of bursts, whose repetition rate corresponds to magnetic field perturbation period. The frequency inside each burst is changing from its front edge to the back edge. Relative shift of the wave frequency can be as large as the relative magnetic disturbance. Distortion of whistler wave frequency spectrum after its passing through magnetically disturbed areas can be used as a diagnostics for low-frequency magnetic field variations. The applicability of our laboratory results to space plasma is discussed. 相似文献