双馈型风电系统变流器控制参数对振荡模态的影响

研究双馈型风力发电系统变流器控制参数对振荡模态的影响。在MATLAB/Simulink中建立系统详细的小信号模型,利用特征值分析和相关因子分析,对机网相互作用振荡模态进行辨识和分类。通过改变变流器控制参数,研究振荡模态的变化特性。最后,在MATLAB/Simulink上进行仿真验证。研究表明,优化变流器控制参数,可有效抑制振荡。     

改进型滑模变结构电机控制的脉振电流注入法研究

为了提高永磁同步电机无位置传感器技术的控制性能,在电机动态品质优化的研究中,以滑模变结构控制器替代传统的PI控制器,采用新型趋近律函数改进滑模控制器的输出模型,削弱了传统滑模控制存在的抖振,提高了控制系统的抗干扰能力。在分析无位置传感器技术时,引入高通谐振滤波器,采用具备以高信噪比为特点的两相静止坐标系下高频脉振电流注入法。仿真结果表明,在带高通谐振滤波器的高频脉振电流注入法中运用滑模变结构控制器,提高了转子位置估计的精度,增强了控制系统的鲁棒性。     

被动射流旋涡对高速扩压叶栅气动性能的影响

提出了一种利用压力面与吸力面间压差产生射流旋涡的被动流动控制技术以改善压气机叶栅的气动性能,在进口马赫数Ma=0.67的高速扩压叶栅上验证了其有效性。结果表明,射流旋涡可有效增强吸力面附面层与主流间的能量交换,改变下游壁面涡的结构和尺寸,推迟流动分离,减小角区损失。当射流距分离线或端壁较近时,当地较厚的附面层使得旋涡上洗区的掺混损失增加;而射流距分离线或端壁过远时均会减弱下洗区能量注入对角区低能流体的影响;指向端壁的射流会增加壁面涡强度,而沿远离端壁方向过大的偏角则会减弱射流旋涡强度,从而减弱其控制效果。当射流轴向距叶片前缘xj/cx=40%、沿叶高距端壁h/H=15%、射流偏角β=60°时,其改善栅内流动的效果最佳,总压损失减小可达5.2%,而射流流量仅相当于主流的0.27‰。     

大型平台的惯性稳定与地理坐标系姿态跟踪

介绍了一种大型两轴稳定平台的惯性稳定和地理系姿态跟踪原理,建立了稳定平台俯仰框架和横滚框架的运动学模型和动力学模型,进行了稳定平台横滚通道的角速度回路和角位置回路设计,仿真分析了姿态角测量误差作用下的稳定平台姿态跟踪性能,与利用加速度计反馈实现调平的两轴阻尼稳定平台进行对比,比对结果验证了本文设计的控制系统在水平姿态跟踪速度和抗干扰能力上的优势.平台样机进行了姿态跟踪测试,结果验证了结合定位定向系统(POS)的稳定平台惯性稳定和姿态跟踪控制方法可行.     

利用机载GNSS-R的有效波高反演技术

采用自主研发的多源多宿GNSS-R(Global Navigation Satellite System-Reflections,全球导航卫星系统反射信号)海洋环境遥感探测系统,在天津渤海湾特定区域进行了3次机载校飞试验,获得了大量有效GNSS-R信号数据,对自然条件下的海面有效波高进行了反演处理。该系统通过对接收的GNSS直达信号和海面反射信号进行相关运算处理,可以获得DDM(Delay-Doppler Mapping,时延—多普勒映射)图谱,再利用DCF(Derivative of the Correlation Function,相关函数的导数)在DDM图谱基础上进行相关功率波形的计算,进而通过计算DCF的函数波形宽度得到海面有效波高,验证了该方法的可行性。该方法具有全天时、全天候、高分辨率、低成本等优点,对全球范围内中小尺度海洋状态和物理现象的监测具有重要意义。     

Observation of Terrestrial gamma-ray flashes in the RELEC space experiment on the <Emphasis Type="Italic">Vernov</Emphasis> satellite

The RELEС scientific payload of the Vernov satellite launched on July 8, 2014 includes the DRGE spectrometer of gamma-rays and electrons. This instrument comprises a set of scintillator phoswich-detectors, including four identical X-ray and gamma-ray detector with an energy range of 10 kev to 3 MeV with a total area of ~500 cm² directed to the atmosphere, as well as an electron spectrometer containing three mutually orthogonal detector units with a geometric factor of ~2 cm² sr. The aim of a space experiment with the DRGE instrument is the study of fast phenomena, in particular Terrestrial gamma-ray flashes (TGF) and magnetospheric electron precipitation. In this regard, the instrument provides the transmission of both monitoring data with a time resolution of 1 s, and data in the event-by-event mode, with a recording of the time of detection of each gamma quantum or electron to an accuracy of ~15 μs. This makes it possible to not only conduct a detailed analysis of the variability in the gamma-ray range, but also compare the time profiles with the results of measurements with other RELEC instruments (the detector of optical and ultraviolet flares, radio-frequency and low-frequency analyzers of electromagnetic field parameters), as well as with the data of ground-based facility for thunderstorm activity. This paper presents the first catalog of Terrestrial gamma-ray flashes. The criterion for selecting flashes required in order to detect no less than 5 hard quanta in 1 ms by at least two independent detectors. The TGFs included in the catalog have a typical duration of ~400 μs, during which 10–40 gamma-ray quanta were detected. The time profiles, spectral parameters, and geographic position, as well as a result of a comparison with the output data of other Vernov instruments, are presented for each of candidates. The candidate for Terrestrial gamma-ray flashes detected in the near-polar region over Antarctica is discussed.     

Designing corrections for the trajectory of the <Emphasis Type="Italic">Spektr-R</Emphasis> spacecraft in the event of immersions into the Moon’s sphere of influence

The results of updating the parameters of motion of the Spektr-R spacecraft at the end of 2016 have shown that, in January 2018, with a probability close to unity, the condition that a spacecraft stay in the Earth’s shadow is violated; however, in May of the same year, the ballistic life of the spacecraft will be terminated. Thus, in 2017, the question arose of how to design the correction of flight of this spacecraft using its onboard propulsion system. The correction was designed with allowance for the fact that, for the first time since it was launched, the spacecraft in the course of several years, beginning with 2017, repeatedly approaches the Moon, deeply immersing into its sphere of influence. This paper presents the technologically and organizationally convenient, allowable versions of upcoming correction of the Spektr-R spacecraft trajectory and justifies the particular scheme of its implementation.     

Estimating the accuracy of the technique of reconstructing the rotational motion of a satellite based on the measurements of its angular velocity and the magnetic field of the Earth

The paper has studied the accuracy of the technique that allows the rotational motion of the Earth artificial satellites (AES) to be reconstructed based on the data of onboard measurements of angular velocity vectors and the strength of the Earth magnetic field (EMF). The technique is based on kinematic equations of the rotational motion of a rigid body. Both types of measurement data collected over some time interval have been processed jointly. The angular velocity measurements have been approximated using convenient formulas, which are substituted into the kinematic differential equations for the quaternion that specifies the transition from the body-fixed coordinate system of a satellite to the inertial coordinate system. Thus obtained equations represent a kinematic model of the rotational motion of a satellite. The solution of these equations, which approximate real motion, has been found by the least-square method from the condition of best fitting between the data of measurements of the EMF strength vector and its calculated values. The accuracy of the technique has been estimated by processing the data obtained from the board of the service module of the International Space Station (ISS). The reconstruction of station motion using the aforementioned technique has been compared with the telemetry data on the actual motion of the station. The technique has allowed us to reconstruct the station motion in the orbital orientation mode with a maximum error less than 0.6° and the turns with a maximal error of less than 1.2°.     

航电系统安全性分析工具设计与研究

随着航电系统综合化程度的不断提高,传统的安全性分析方法过于依赖工程经验,难以保证失效模式的完备性。同时在系统迭代设计的过程中,由于系统的复杂性,会导致安全性分析工作量过大,增加了时间及经济成本。针对上述问题,设计了一种自动化安全性分析工具,基于Sys ML描述语言建立安全性数据模型,采用路径追溯的方法完成故障树自动建模,并对生成的故障树进行共模分析和区域安全性分析。以某系统为例的实验结果表明,该工具能够实现故障树自动建模与分析,提高了安全性分析的效率和完备性。