基于联合滤波器的高精度卫星定姿系统设计

设计了由陀螺、GPS姿态敏感器、红外地平仪和太阳敏感器构成的太阳同步极轨卫星姿态确定系统。提出联邦滤波器结构和算法,推导了各子系统的量测方程和姿态确定系统的误差状态方程。为规避对量测值进行非相关处理,采用减小GPS姿态敏感器输出的姿态滤波值作为系统滤波器量测值的频率的方法。仿真结果表明,采用联邦滤波器对多敏感器卫星姿态确定系统进行信息融合,具有计算量小、精度高、可靠性好等优点。     

Research on a six-phase permanent magnet synchronous motor system at dual-redundant and fault tolerant modes in aviation application

With the development of more/all electrical aircraft technology,an electro-mechanical actuator (EMA) is more and more used in an aircraft actuation system.The motor system,as the crucial part of an EMA,usually adopts the redundancy technology or fault tolerance technology to improve the reliability.To compare the performances of these two motor systems,a 10-pole/ 12-slot six-phase permanent magnet synchronous motor (PMSM) is designed with the concentrated single-layer winding,which is able to operate at dual-redundant and fault tolerant modes.Furthermore,the position servo performances of the six-phase PMSM at dual-redundant and fault tolerant modes are analyzed,including the normal and fault conditions.In addition,a variable structure proportional-integral-derivative (PID) control strategy is proposed to solve the performance degradation problem caused by phase current saturation.Simulation and experimental results show that the fault tolerant PMSM has a better position servo performance than the dual-redundant PMSM,and the variable structure PID control strategy is able to improve the performance due to phase current saturation.     

Relativistic proton production at the Sun in the 20 January 2005 solar event

Based on the concept of multiple acceleration of solar energetic particles (SEP) we analyzed the super-event of 20 January 2005 by the data of ground level, balloon and spacecraft observations. The main characteristics of relativistic solar protons (energy spectra, anisotropy directions and pitch-angle distributions) are derived and their dynamics during the event is studied. It is shown that the flux of relativistic solar protons may consist of two distinct components, the so-called prompt and delayed ones. Within a two-source model of particle generation, one of which is associated with an expanding magnetic loop, we solved the transport equation in energy phase space, including adiabatic losses simultaneously with the stochastic acceleration process, and calculate the expected spectra of the delayed component at the source. The confrontation of experimental spectra with theoretical ones shows that the delayed component may be correctly described by stochastic acceleration, but not the prompt component. The required acceleration efficiencies turned out to be rather high, so that, for this particular event, adiabatic cooling is practically negligible. Our results provide a new support to the existence of two populations of relativistic solar protons in some SEP events.     

永磁同步电机新型单电阻电流重构技术研究

针对永磁同步电机在单电阻电流采样时,低调制区域和扇区边界区域难以进行电流重构的问题,提出了一种新型单电阻电流重构技术。首先,对三相电流重构技术原理进行研究,定义无法重构的区域为非观测区,对非观测区电流重构盲区进行分析。其次,使用脉冲宽度调制移相法对非观测区的电流进行重构,发现仍有部分非观测区只可测得一相电流,从而无法完成电流重构。针对这一问题,设计电流观测器,通过单相电流来估算三相电流,且不需要电机与负载参数,实现简单。试验验证表明,所提新型单电阻电流重构技术具有可行性和实用价值。     

多参仪器模糊自调谐离散滑模控制方法

针对多参数仪器的非线性高精度大动态控制问题, 提出对电机力矩脉动、摩擦扰动及其他未建模干扰等非线性因素,用两个独立的模糊自调谐回路进行自适应抑制衰减的方案,并进行了理论分析和建模仿真,表明该方案在宽速率范围内以及高动态仿真情况下,幅值误差小于5%,相位误差小于5°,并可在大动态宽速率范围内进行自适应调整,因此可改善多参数仪器在非线性复杂扰动情况下的工作性能。     

飞机主动侧杆的弹簧-阻尼系统力矩控制策略

主动侧杆(ASS)已成为目前的研究热点,可提供力反馈功能以模拟弹簧的作用,反馈的杆力随侧杆位移变化,且可自动回弹到中立位。针对飞机主动侧杆模拟弹簧控制问题,将主动侧杆等效为一个无质量的弹簧-阻尼系统,采用永磁同步电机作为力矩电机,其由PI电流环控制,根据位移-杆力特性曲线及阻尼特性得到交轴电流参考值,根据侧杆位移输出对应的转矩。并采用一种回中定位策略,根据侧杆不同的偏转角改变控制参考值。仿真和实验结果表明,该控制策略能够实现主动侧杆模拟弹簧功能,且杆力反馈具有较高的精度和稳定性,并可保证主动侧杆的快速精确回中。     

太阳同步冻结轨道星座保持与捕获

太阳同步冻结轨道卫星在经过同一星下点时光照特性和轨道高度相同,便于载荷观测及定标.由多颗太阳同步冻结轨道卫星组成的星座,需要实现星座成员轨道倾角、轨道高度、偏心率矢量和相对轨道幅角的同时保持.提出了基于切向单脉冲的最低燃耗轨道面内保持策略,证明了该策略的稳定性和燃料最优性,给出了太阳同步轨道地方时保持简单算法.仿真证明...     

一种新型的基于单电流调节器提高永磁同步电机系统负载与抗扰能力的算法

提出了一种根据永磁同步电机(PMSM)转速来调节交轴电压的最大转矩法。算法对电压极限矢量圆与电流极限矢量圆定量分析,找到电机稳定运行时的最大转矩点,通过在电压极限矢量圆补偿定子电阻压降修正最大转矩点。通过直接给定交轴电压的方式,充分利用修正最大转矩点的电磁转矩,提高电机的负载能力和抗干扰能力。仿真验证了该算法的有效性和可行性。对于最大转矩点的定量分析,使此模型具有良好的可移植性。     

Long-Term Fluences of Solar Energetic Particles from H to Fe

Data from ACE and GOES have been used to measure Solar Energetic Particle (SEP) fluence spectra for H, He, O, and Fe, over the period from October 1997 to December 2005. The measurements were made by four instruments on ACE and the EPS sensor on three GOES satellites and extend in energy from ∼0.1 MeV/nuc to ∼100 MeV/nuc. Fluence spectra for each species were fit by conventional forms and used to investigate how the intensities, composition, and spectral shapes vary from year to year.