一种燃油箱绿色惰化系统地面惰化性能分析

在描述一种采用催化燃烧产生惰气来降低油箱气相空间氧体积分数的新型绿色惰化工作原理基础上,设计了绿色惰化系统流程,通过一定的假设和简化建立了其数学模型并进行了求解.将结果与采用中空纤维膜产生富氮气体的机载惰化系统进行了比较,结果显示:当绿色惰化系统中抽吸气的流量与中空纤维膜惰化所产生富氮气体流量一致时,前者惰化效果远好于后者.同时,还研究了催化反应器效率和预热气体抽取比例对绿色惰化系统的影响,结果表明:提高反应器效率可有效缩短达到安全氧体积分数所需的时间,且最终油箱气相空间氧体积分数会降低,而选取合适的预热气体抽取比例可以减少系统能耗.      

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。     

考虑条件风险价值的含多风电场电力系统经济调度

针对单一Copula函数在描述风速相关性时的限制性,通过引入mixCopula函数获取具有相关性的多维风速样本。引入条件风险价值理论,将风电功率的不确定性以经济性考量,建立了一种含多风电场的电力系统经济调度模型,协调经济性和安全性的问题。采用场景化理论对目标函数进行处理,使得计算得以简化。以含2个风电场的IEEE30节点系统为算例,分析风速相关性和置信水平对优化结果的影响,验证模型的合理性及有效性。     

一种卡尔曼滤波器的永磁同步电机无速度传感器

针对滑模观测器的永磁同步电机参数误差容易造成估算误差和反电动势中存在高频纹波分量的缺点,使用低通滤波器不能有效消除高频纹波,提出在滑模观测器前端引入卡尔曼滤波器来消除高频纹波,使得永磁同步电机的控制系统具有更好的稳态效果和动态响应。依据设计仿真搭建MATLAB平台,对提出新方法进行验证。试验结果表明增加卡尔曼滤波环节后的滑模观测器不仅鲁棒性强,而且在一定程度上有效抑制了抖振,在系统快速性及稳态性能上都有较好的效果。     

可折叠铍青铜弹性豆荚杆焊接成型工艺

可折叠铍青铜豆荚杆的焊接成型是该类豆荚杆研制的难点之一,本文对铍青铜豆荚杆的储能点焊工艺进行了研究,分析了工艺参数及热处理对焊接接头名义剪切强度的影响,给出了优选的工艺参数为焊接电压180 V、保压7 s。在最佳工艺条件下成型并经过340℃/2 h时效处理后,焊接接头的名义剪切强度由52 MPa提高到68 MPa。铍青铜焊接接头的名义剪切断口随着焊接电压的增大,从焊接接头区域向热影响区转移。     

高性能产品(零件)制造技术特征现状的研究分析

系统分析各类高性能制造以注重零件的几何尺寸精度所带来的问题,即在具备超精密、高精度加工能力后,由"合格的高精度零件"装配出的产品至今依然还是合格率低、参数稳定性差的本质内因.首次从零件制造微观角度提出了产品生产合格率低、参数稳定性差是由零件表面微观特征与产品技术特征非匹配性导致的,提出了全新的产品制造理念,从注重零件的几何尺寸精度向关注零件制造微观工艺特征与产品技术特征的匹配性和符合性转变.形成和建立起我国自主创新的高性能产品制造思想和产品制造工艺技术体系,才能从根本上解决产品生产制造合格率低、参数稳定性差等问题,才能形成有继承性、可持续、稳定的产品制造技术体系,而这一切是工业4.0制造模式无法解决的.     

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°.