编队卫星姿态的自适应协同控制

研究了无向信息交互条件下的多卫星姿态同步和跟踪问题,分别在模型参数精确已知和存在模型参数不确定性的情形下设计分散式协同控制算法。当模型参数精确已知时,基于滑动模态变量设计的协同控制力矩,实现了编队卫星姿态的同步机动,即保证编队卫星姿态的同步,并同时跟踪期望的时变参考姿态轨迹。当在轨卫星存在模型参数不确定性和常值未知扰动力矩时,提出了一种自适应协同控制律,仍能实现多卫星姿态的同步机动。基于Lyapunov-Krasovskii的分析表明,当星间链路存在任意未知的定常通讯时延时,本文设计的控制器有效。数值仿真算例验证了本文提出的控制算法。     

Ionospheric Effects of Geomagnetic Storms in Different Longitude Sectors

This paper analyzes the state of the ionosphere during two geomagnetic storms of a different intensity evolving in different sectors of local time in different seasons. There were used the data from a network of ionospheric stations located in the opposite longitudinal sectors of 80°-150° E and 250°-310° E.This analysis has permitted us to conclude that the detected differences in the variations of the disturbances are likely to be determined by the local time difference of the geomagnetic storm development, its intensity and by the different illumination conditions of the ionosphere.      

Magnetic Field Fluctuations in the Solar Wind, Foreshock and Magnetosheath： Cluster Data Analysis

46 magnetosheath crossing events from the two years (2001.2-2003.1) of Cluster magnetic field measurements are identified and used to investigate the characters of the magnetic field fluctuations in the regions of undisturbed solar wind, foreshock, magnetosheath. The preliminary results indicate the properties of the plasma turbulence in the magnetosheath are strongly controlled by IMF orientation with respect to the bow shock normal. The amplitude of the magnetic field magnitude and direction variations behind quasi-parallel bow shock are larger than those behind quasi-perpendicular bow shock. Almost purely compressional waves are found in quasi-perpendicular magnetosheath.     

扩展近似时间最优伺服控制及其试验验证

针对带有惯性阻尼环节的典型伺服系统,提出一种能实现大范围快速定点运动的控制方案。控制方案首先利用时间最优控制律进行快速目标追踪,当系统速度下降到一定范围内时平滑切换成线性控制律。采用线性控制区内的闭环极点阻尼系统和自然频率作为设计参数,给出了全参数化的控制律。基于Lyapunov理论分析了控制系统的闭环稳定性。将该控制方案用于一个直流伺服电机的位置-速度环的定点位置控制,并进行了MATLAB数字仿真和基于TMS320F28335 DSC的试验研究。结果表明:所设计的控制系统可以对大范围的给定目标进行快速和准确的跟踪,且对扰动和系统参数差异具有较好的鲁棒性。     

基于最小二乘法的磁力计误差补偿与校准

磁力计在行人自主导航系统中用于提供绝对航行信息,而航向的精度直接决定着系统定位的精度。针对目前磁力计标定方法中存在磁干扰等问题,提出了一种基于最小二乘法和"8"字校准法对磁力计零偏进行实时校准的方法。该方法先利用最小二乘法修正磁力计零偏,再根据磁力计的模值大小及方差作为磁干扰的判断条件,用"8"字旋转方式进行实时校准。通过仿真和实验验证,新的方法有效地解决了磁力计误差补偿问题,证明了改进误差补偿算法的可行性和有效性。     

Fundamental (f) oscillations in a magnetically coupled solar interior-atmosphere system – An analytical approach

Solar fundamental (f) acoustic mode oscillations are investigated analytically in a magnetohydrodynamic (MHD) model. The model consists of three layers in planar geometry, representing the solar interior, the magnetic atmosphere, and a transitional layer sandwiched between them. Since we focus on the fundamental mode here, we assume the plasma is incompressible. A horizontal, canopy-like, magnetic field is introduced to the atmosphere, in which degenerated slow MHD waves can exist. The global (f-mode) oscillations can couple to local atmospheric Alfvén waves, resulting, e.g., in a frequency shift of the oscillations. The dispersion relation of the global oscillation mode is derived, and is solved analytically for the thin-transitional layer approximation and for the weak-field approximation. Analytical formulae are also provided for the frequency shifts due to the presence of a thin transitional layer and a weak atmospheric magnetic field. The analytical results generally indicate that, compared to the fundamental value ($\omega =\sqrt{\mathit{gk}}$), the mode frequency is reduced by the presence of an atmosphere by a few per cent. A thin transitional layer reduces the eigen-frequencies further by about an additional hundred microhertz. Finally, a weak atmospheric magnetic field can slightly, by a few percent, increase the frequency of the eigen-mode. Stronger magnetic fields, however, can increase the f-mode frequency by even up to ten per cent, which cannot be seen in observed data. The presence of a magnetic atmosphere in the three-layer model also introduces non-permitted propagation windows in the frequency spectrum; here, f-mode oscillations cannot exist with certain values of the harmonic degree. The eigen-frequencies can be sensitive to the background physical parameters, such as an atmospheric density scale-height or the rate of the plasma density drop at the photosphere. Such information, if ever observed with high-resolution instrumentation and inverted, could help to gain further insight into solar magnetic structures by means of solar magneto-seismology, and could provide further insight into the role of magnetism in solar oscillations.     

Midlatitude ionospheric F2-layer response to eruptive solar events-caused geomagnetic disturbances over Hungary during the maximum of the solar cycle 24: A case study

In our study we analyze and compare the response and behavior of the ionospheric F2 and of the sporadic E-layer during three strong (i.e., Dst?<??100nT) individual geomagnetic storms from years 2012, 2013 and 2015, winter time period. The data was provided by the state-of the art digital ionosonde of the Széchenyi István Geophysical Observatory located at midlatitude, Nagycenk, Hungary (IAGA code: NCK, geomagnetic latitude: 46.17° geomagnetic longitude: 98.85°). The local time of the sudden commencement (SC) was used to characterize the type of the ionospheric storm (after Mendillo and Narvaez, 2010). This way two regular positive phase (RPP) ionospheric storms and one no-positive phase (NPP) storm have been analyzed. In all three cases a significant increase in electron density of the foF2 layer can be observed at dawn/early morning (around 6:00 UT, 07:00 LT). Also we can observe the fade-out of the ionospheric layers at night during the geomagnetically disturbed time periods. Our results suggest that the fade-out effect is not connected to the occurrence of the sporadic E-layers.     

Kink mode m = 1 in magnetic tube with discontinuous magnetic field

In this paper, we study conditions of realization and stability of kink modes with azimuthal wave numbers $m=\pm 1$ in cylindrical plasma flex with twisted magnetic field and homogeneous current along its axis. We assume permanent axial magnetic field both inside and outside the flex, surrounded by currentless plasma. Azimuthal magnetic field decreases inversely proportional to the distance from the boundary beyond the flex. We derived dispersion equations for stable and unstable modes in approximation of “thin” plasma flex. The analysis of equations has been provided for the case of discontinuous axial magnetic field on flex’s boundary. Conditions of propagation of wave modes have been defined. It was shown, that unstable modes can be implemented in certain interval of longitudinal wavenumbers. Results can be applied for the interpretation of solar magnetic tubes behavior, using measurements, provided by spacecrafts.     

抗扰动复合非线性伺服控制器的设计与应用

针对典型的电机伺服系统,提出了一种鲁棒复合非线性伺服控制器的离散域设计方案。把系统的扰动和不确定性归结为一个斜坡信号(其变化率恒定),设计一个降维线性扩展状态观测器,对系统未测量状态和未知扰动加以估计。把设计的控制律应用于永磁同步伺服电机,先在MATLAB上进行仿真分析,随后基于TMS320F28335DSC进行试验测试。结果表明系统在各种类型扰动作用下,对目标位置都能实现快速、平稳和准确的跟踪,具有较好的鲁棒性。     

考虑系统扰动的永磁同步电机复合控制策略

提出一种结合滑模速度控制和扩展滑模扰动观测器的永磁同步电机复合控制策略。滑模速度控制采用新型趋近律设计,扩展滑模扰动观测器对系统内部参数摄动以及外部负载干扰进行准确估计。所设计的复合控制器通过系统扰动估计环节对控制系统中的综合扰动项进行实时估计,用以对速度控制环节进行前馈补偿,实现控制系统自抗扰控制。试验结果验证了所提出控制策略的有效性和可行性。