基于QPSO算法的自抗扰控制器设计及参数整定

提出了一种基于量子粒子群(QPSO)的自抗扰控制器(ADRC)设计及参数整定方法.利用自抗扰控制器抗于扰能力强、鲁棒性好、对模型参数变化适应能力强的特点,设计了自抗扰纵向飞行控制器以提高飞行控制性能.针对所设计的自抗扰控制器参数多,需要依靠专家经验或试凑进行整定的问题,应用QPSO算法进行控制器参数整定.仿真结果表明,...     

Effects of Atomic Oxygen Irradiation on Transparent Conductive Oxide Thin Films

作为一种功能薄膜,透明导电氧化物(TCO)薄膜在飞行器的抗原子氧(AO)涂层和太阳能电池领域有着巨大的应用价值。ZnO:Al(ZAO)和In2O3:Sn(ITO)薄膜是目前研究和应用最广泛的TCO。本文对ITO薄膜和ZAO薄膜进行了不同通量的AO辐照。通过对辐照前后样品的X射线衍射、扫描电镜及霍耳效应的表征及测试,研究了AO辐照对这两种TCO薄膜的结构、性能及电学特性的影响。研究表明AO辐照对ZAO薄膜表面有明显的侵蚀作用,但对其结构和导电性能没有明显影响。对于ITO薄膜,随着AO通量的增大,其载流子浓度逐渐下降从而导致了电阻率的提高,电阻率的最大变化达到了21.7%。     

Model Development and Adaptive Imbalance Vibration Control of Magnetic Suspended System

对星载磁悬浮单框架控制力矩陀螺,建立其转子的平动与转动的动力学方程。所建模型反映了转子的动、静不平衡特性,以及转子运动与框架、星体运动的耦合关系。模型是主动磁悬浮控制与动框架效应分析的基础。对动、静不平衡量未知的转子,设计了自适应对中控制器。在分散PD、比例交叉反馈控制器与高低通滤波器的基础上,通过动、静不平衡量的辨识与补偿控制,使转子绕其惯量主轴旋转,衰减角动量交换执行机构高速转子因不平衡而对基座产生的干扰力,消除星上主要颤振源,达到降低卫星姿态抖动的目的。     

基于角加速度的陀螺框架伺服系统干扰观测器

磁悬浮控制力矩陀螺(MSCMG,Magnetically Suspended Control Moment Gyro)是大型航天器姿态控制的关键执行机构,影响MSCMG输出力矩准确度的一个关键因素是其框架伺服系统的控制精度.为提高MSCMG框架伺服系统的抗干扰能力和控制精度,提出了一种基于角加速度的干扰观测器.其设计思想是:卡尔曼滤波器利用角位置估计出角速度并送往状态观测器以获取准确的角加速度,角加速度和电流作为干扰观测器的输入以获得补偿电流,补偿电流加到电流环的输入端以补偿各种干扰.干扰观测器结构简单,抗干扰能力强.实验表明:该方法有效地提高了MSCMG框架伺服系统的角速度精度与稳定度.     

基于LADRC的无人直升机轨迹跟踪

无人直升机轨迹控制系统是对多输入/多输出强耦合非线性系统进行解耦控制的系统。为解决无人直升机轨迹控制效果依赖于直升机物理参数的测量和辨识精度以及外部扰动大小问题,提出了一种基于线性自抗扰控制(LADRC)的多回路无人直升机轨迹控制系统。首先建立无人直升机X-Cell的飞行动力学模型,并引入风切变、大气紊流和突风模型以更加准确模拟真实飞行环境;然后对X-Cell进行配平计算以验证动力学模型和配平算法的准确性,并选取一组配平值作为轨迹控制仿真的初始状态和操纵量;随后根据被控量的动力学方程阶次选取对应的一阶和二阶LADRC基本控制器,并结合时间尺度原理,自内向外依次构建无人直升机的姿态、速度和位置控制回路,将三回路串联从而建立了无人直升机轨迹控制系统;而后进行了稳定性分析,特征根计算结果表明轨迹控制系统镇定了X-Cell开环系统不稳定的动态特性;最后将该控制系统应用于各种扰动下直升机轨迹跟踪仿真,结果表明本文无人直升机轨迹控制系统能很好地实现带爬升率的"8"字形轨迹跟踪,且相比于基于比例积分和微分(PID)控制的轨迹控制系统,该控制系统具有更优的鲁棒性和抗扰性。     

激光技术在高技术国防战争中的应用

介绍激光技术的基本含义以及激光技术在新军事应用中的分类,并结合我军的军事战略,从激光侦查技术、激光对抗与激光干扰技术、激光模拟训练技术以及激光武器四个方面对激光技术在高技术国防战争中的应用进行分析,最后结合装甲装备,介绍激光技术在观瞄系统中的具体应用。     

Compensation of time-variable magnetic moments for a precise attitude control in nano- and micro-satellite missions

Theses days, many nano- and micro-satellites are applied to several astronomy and remote sensing missions. In order to achieve mission requirements, these satellites must control the attitude precisely. A magnetic disturbance is one of the dominant sources of attitude disturbances. Therefore, this disturbance should be canceled in-orbit or on the ground to achieve the attitude strict requirements. This paper presents the effect of the magnetic disturbance to the attitude in nano- and micro-satellite missions and the sources of the residual magnetic moment of the satellites, which causes the magnetic disturbance. Then, the paper proposes a method to compensate the residual magnetic moment both in-orbit and in the design phase of the satellites. The research also focused on a time-varying residual magnetic moment. Finally, the method is applied to a micro-astrometry satellite as an example.     

Study of the ionosphere during a magnetospheric storm using data on the ground and in space

For the magnetospheric storm of May 14–16, 1997 geophysical data of satellites DMSP and IMP-8 are compared with data of radio propagation on the high-latitude HF radio path of Heiss Island – St. Petersburg and data from European ionosondes. Peculiarities of variations of the operational frequencies range MOF–LOF (maximum and lowest observed frequencies) on the path were considered. The range has been determined by the method of oblique ionospheric sounding (OIS). The latter is more informative for observations during a magnetic storm compared to the vertical sounding method. Nevertheless, an analysis of variations of the critical frequency of the ionospheric F2 layer from the chain of European ionosondes was carried out. For interpretation of results, data of magnetospheric parameters, AE-indexes and riometer data were used. The variations of both frequency range on the path and critical frequencies of the F2 layer through the ionosondes chain during the disturbed period had certain regularities of behaviour. These regularities are being explained from the physical point of view. The analysis of the satellite DMSP data has showed that a magnetospheric disturbance causes displacement equatorward of precipitation and some growth of its width and energy.     

Study of TEC changes during geomagnetic storms occurred near the crest of the equatorial ionospheric ionization anomaly in the Indian sector

GPS satellites data obtained at Bhopal (23.16° N, 77.36° E, geomagnetic latitude 14.23° N) India were analyzed to study the TEC changes during several geomagnetic storms (−300 nT < Dst < −50 nT) occurred in 2005–2007. We had segregated the storms according to the Dst value, i.e. moderate storms (−100 nT < Dst ? −50 nT), strong storms (−150 nT < Dst < −100 nT), and severe storms (Dst less than −150 nT). Total of 21 geomagnetic storms (10 moderate, 9 strong, 2 severe) are considered for the present study. Deviation in vertical total electron content (VTEC) during the main phase of the storm was found to be associated with the prompt penetration of electric field originated due to the under-shielding and over-shielding conditions for almost all geomagnetic storms discussed in this paper. For most of the storms VTEC shows the positive percentage deviation during the main phase while it shows positive as well as the negative deviation during the recovery phase of the storms. The −80% deviation in VTEC was found for geomagnetic storm occurred on July 17, 2005 and the negative trend continued for recovery phase of the storm. This was mainly due to the thermospheric composition changes by Joule heating effect at auroral latitudes that generate electric field disturbance at low latitudes. Traveling ionospheric disturbances (TIDs) were responsible for the formation of wave like nature in VTEC for the storms occurred on May 15, 2005, whereas it was not observed for storm occurred on August 24, 2005.     

一种加速度干扰下的稳定被动定位跟踪算法

在研究一种具有误差自动解耦的观测域滤波的目标跟踪算法和自适应渐消EKF算法的基础上,提出一种匀速运动模型下,基于观测域的自适应目标跟踪算法。使用实测GPS导航数据进行数字仿真,结果表明：观测域的自适应目标跟踪算法在加速度扰动下,稳定性优于观测域滤波算法。