高超声速钝头体边界层转捩试验

为研究高超声钝头体边界层转捩以及头部钝度对转捩的影响,在FD-14和FD-14A两座激波风洞中开展了热流、压力扰动和高速纹影显示等综合测量。试验结果表明,转捩雷诺数关于钝度雷诺数的变化显示出转捩反转的趋势。压力扰动的功率谱密度（PSD）分析结果以流向离散分布云图形式显示,边界层高速纹影图像显示了第二模态波的发展、湍流的生成和熵层对边界层结构的显著影响。大头部钝度带来的强熵梯度熵层流动对边界层压力扰动频谱特性和流动结构影响显著,在转捩反转机理中起到重要作用。此外,马赫数对转捩的影响不容忽视。     

仿真转台周期性干扰抑制的研究

提出采用加速度反馈方案,在无需加大系统带宽的情况下提高系统的动态刚度,从而提高了系统对周期性干扰的抑制能力。仿真结果表明,与传统PID控制相比,采用加速度反馈确实能够较好地抑制系统中的周期性干扰。     

基于扩张状态观测器的永磁同步电机自抗扰无源控制

针对传统永磁同步电机滑模控制存在的抖振以及系统抗扰动鲁棒性差问题,提出一种基于扩张状态观测器的永磁同步电机自抗扰无源控制方法。转速外环设计自适应滑模控制器,采用扩张状态观测器对系统干扰项进行观测,用其进行前馈补偿。电流内环将无源控制与自抗扰控制相融合,得到dq旋转坐标系下的电压给定。新型控制方法可有效抑制系统抖振,增强系统鲁棒性。试验结果验证了所提控制方法的有效性和实用性。     

基于自适应方法的多无人机编队队形控制

针对"长机-僚机"近距编队队形因风场扰动而不能保持期望队形的问题,首先,提出了一种自适应队形保持控制的方法,该方法可用于抵消因风场不确定性对无人机的横侧向和前行方向所产生的距离误差,同时能够保持无人机编队稳定飞行。其次,由于风场的不确定性会引起"长机-僚机"之间的动力学发生变化,因此设计了一种基于"长机-僚机"相对运动模型的自适应控制律用以估计风场在3个方向的大小,进而控制无人机之间的相对运动以消除风场不确定性所产生的距离误差并保持速度的一致性,最终实现保持期望的队形。再次,通过构建合理的李雅普诺夫函数,证明无人机编队在风场干扰下能够保持编队稳定飞行,同时"长机-僚机"之间相对横向、横侧向以及纵向的距离误差均接近零。最后,通过仿真验证：所提出的自适应控制方法具有良好的鲁棒性,这为工程实践提供理论依据。     

Anomalous enhancement of electric field derived from ionosonde data before the great Wenchuan earthquake

The seismo-ionospheric coupling is a hot topic of modern scientific research. One of the most reasonable mechanisms is the hypothesis of quasistatic electric field. With a preliminary analytical method, electric field in F2-region before Wenchuan earthquake was derived from the five lower latitude ground-based ionosondes: Lhasa (29.63°N, 91.17°E), Chongqing (29.50°N, 106.40°E), Kunming (25.00°N, 102.70°E), Guangzhou (23.15°N, 113.35°E) and Haikou (23.15°N, 110.35°E). The results show that there was an anomalous enhancement of electric field in F2-region close to the epicenter with maximal amplitude ∼2 mV/m (about 10 times of the background) at 15:00 LT on 9 May, which is in line with the amplitudes of anomalous electric field related to some previous earthquakes observed by satellites.     

Cosmic ray anisotropy based on Yakutsk station in real time

The method has been developed to calculate galactic cosmic ray anisotropy parameters by using on-line data of the neutron monitor 24-NM-64 and muon telescope at the Yakutsk station. The preliminary analysis shows that characteristic changes in the anisotropy parameters caused by the first spherical harmonics of cosmic ray angular distribution are observed 1–2 days before the onset of the most part of large-scale geophysical disturbances on the Earth. There is reason to believe that the attraction of data of geophysical observations of other kinds will allow to develop the forecast methods for the arrival of large-scale interplanetary disturbances at the Earth.     

舰尾流环境中载机纵向QFT/TECS控制系统设计

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。     

Early morning enhancement in ionospheric electron density during intense magnetic storms

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.     

我国中部地区电离层扰动时空尺度的统计分析

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。     

Prediction tests by using “ISF” method for the geomagnetic disturbances

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, T_obs, and the prediction, T_pred, ΔT_pred/T_obs  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, ∑K_p,obs, and the prediction, ∑K_p,pred, Δ∑K_p,pred/∑K_p,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.