Attitude control system of the first Russian nanosatellite <Emphasis Type=Italic>TNS-0 no. 1</Emphasis>

The results of designing the attitude control system of the first Russian nanosatellite TNS-0 no. 1 providing orientation of its longitudinal axis along the local geomagnetic field induction vector are presented. The system consists of a permanent magnet and two sets of hysteresis rods. The magnetic and geometric parameters of the magnet and rods are calculated. The influence of the permanent magnet field on the hysteresis rods and mutual influence of the rods in the case of compact satellite packaging are analyzed. Examples of calculations of transient processes and steady-state angular satellite motion are presented.     

三相谐振直流环节逆变器的控制策略

本文针对三相谐振直流环节逆变器提出了三种电流调节方案,并对这三种调节方案进行了分析比较。电流调节△调制方案是零滞环的,它使得三相电流总是流向正确的方向,具有良好的动态特性,但谐波特性较差;相邻模态电流调制方案使逆变器在相邻的开关模态或零开关模态之间进行切换,谐波特性很好,动态特性不够好,而滞环控制电流调制器根据逆变器的实际情况选择开关模态(包括零模态),具有良好的动态特性和谐波特性,适用于三相谐振直流环节逆变器。文中给出了三种方案下的仿真波形,仿真结果的比较也于文后给出。     

基于双时相遥感影像差异信息的深度学习滑坡检测

目前利用高分辨率卫星影像进行滑坡等地质灾害识别逐渐成为研究热点,滑坡目视解译依赖于解译人员的经验,耗时费力且提取精度低,而传统的滑坡自动识别方法易将滑坡和道路、裸地、建筑等多种具有相似光谱信息的地物混淆。针对以上问题,文章使用一种双时相高分辨率卫星影像差异信息的深度学习滑坡检测算法,获取时序影像各个波段和归一化植被指数（Normalized Difference Vegetation Index,NDVI）的差异影像作为深度学习的输入特征。为充分挖掘滑坡前后影像多种信息差异特征,采用了U-net网络模型耦合空洞空间金字塔池化和嵌入注意力机制模块相结合进行滑坡特征提取的方法,该方法增强了滑坡边界信息的保存,能够有效地提取滑坡边界信息和发生剧烈变化的区域。利用上述方法对恩施市和九寨沟进行了滑坡检测,实验结果显示,所取得的综合评价指标值（F1-Score）分别为88.4%和90.53%,误差较小、精度较高。表明该方法能够准确检测出高分卫星数据的滑坡边界,且能保持滑坡的完整性。     

表面处理和胶瘤对航天器结构用铝合金胶接剥离强度的影响

针对工程实践中铝合金的胶接剥离强度数据差异大、胶接可靠性急需提升的现状,开展了常温常压环境下铝合金金属对金属,以及蜂窝夹层结构胶接剥离强度的测试验证,分析了试片表面处理工艺和试样周围有/无胶瘤对胶接剥离强度的影响。结果表明,在试样周围保留0.5～1 mm宽的胶瘤有利于提高试样的剥离强度;仅用有机溶剂清洁试片胶接面,试样的剥离强度最低且数据离散性大;对试片胶接面进行砂纸打磨后再清洁,试样的剥离强度有较大提高,但数据离散性仍然偏大;对试片胶接面进行磷酸阳极化氧化处理可使试样的剥离强度提高最多。所得结果可为胶接工艺优化提供参考。     

基于分布式星群的全相参雷达低副瓣波束形成设计方法

不同于地面稀布阵相参阵列雷达,分布式星群平台具有高速运动特性,相应地全相参合成效率受限于星间的空时频同步误差、波束指向误差等系统误差约束。提出了一种基于分布式星群的全相参雷达低副瓣波束形成设计方法。首先,从星群系统规模、星间安全距离、远场条件、探测链路等因素入手推导了有效探测距离区间。接着,给出了同步误差、波束指向误差以及卫星高速运动特性对全相参合成效率的定量影响评估方法。最后,利用空时频多维联合方法实现了低副瓣稳健波束形成,可有效增加无模糊视场范围,适用于实际星群规模有限的应用场景。仿真结果验证了所提算法的有效性。     

分数阶控制器实现方法研究

研究了分数阶控制器的模拟和数字实现方法,其中数字实现是重点。数字实现是通过构造一个新的IIR型数字滤波器来对函数的分数阶微积分计算进行近似求解,然后对该滤波器进行连分式展开来完成的。以PID控制为例进行的数值仿真结果表明,用此方法设计的离散分数阶PID控制器比传统离散整数阶PID控制器具有更优的控制性能,同时也验证了该数字实现方法的正确性与可行性。     

Relaxation of electron and proton radiation belts of the earth after strong magnetic storms

During strong magnetic storms in July and November of 2004 the fluxes of trapped particles (protons and electrons of MeV energies) in the Earth’s radiation belts have increased by orders of magnitude and then decreased remaining on an enhanced level for several months. These enhancements allowed us to study the processes of relaxation of the radiation belts. Measurements of energetic particles by low-altitude satellites Coronas-F and Servis-1 have shown that predictions of the theory about the rate of pitch-angle diffusion are not always correct, giving both overestimated and underestimated values for the lifetime of energetic particles.     

Electrodynamic stabilization of earth-orbiting satellites in equatorial orbits

A satellite with electrodynamic stabilization system is considered. Based on the method of Lyapunov functions, sufficient conditions of the asymptotic stability of direct equilibrium position of this satellite in the orbital coordinate system under perturbing action of a gravitational moment are obtained. These conditions allow one to ensure a rational choice of parametric control coefficients depending on parameters of the satellite and its orbit.     

Activation of the tail open part during the magnetospheric storm

In each polar cap (PC) we mark out “old PC” observed during quiet time before the event under consideration, and “new PC” that emerges during the substorm framing the old one and expanding the PC total area. Old and new PCs are the areas for the magnetosphere old and new tail lobes, respectively. The new lobe variable magnetic flux Ψ₁ is usually assumed to be active, i.e. it provides the electromagnetic energy flux (Poynting flux) ɛ′ transport from solar wind (SW) into the magnetosphere. The old lobe magnetic flux Ψ₂ is supposed to be passive, i.e. it remains constant during the disturbance and does not participate in the transporting process which would mean the old PC electric field absolute screening from the convection electric field created by the magnetopause reconnection. In fact, screening is observed, but far from absolute. We suggest a model of screening and determine its quantitative characteristics in the selected superstorm. The coefficient of a screening is the β = Ψ₂/Ψ₀₂, where Ψ₀₂ = const is open magnetic flux through the old PC measured prior to the substorm, and Ψ₂ is variable magnetic flux through the same area measured during the substorm. We consider three various regimes of disturbance. In each, the coefficient β decreased during the loading phase and increased at the unloading phase, but the rates and amplitudes of variations exhibited a strong dependence on the regime. We interpreted decrease in β as a result of involving the old PC magnetic flux Ψ₂, which was considered to be constant earlier, in the Poynting flux ɛ′ transport process from solar wind into the magnetosphere. Transport process weakening at the subsequent unloading phase creates increase in β. Estimates showed that coefficient β during each regime and the computed Poynting flux ɛ′ varied manifolds. In general, unlike the existing substorm conception, the new scenario describes an unknown earlier of tail lobe activation process during a substorm growth phase that effectively increases the accumulated tail energy for the expansion and recovery phases.