机体弹性对起落架载荷影响分析

基于ADAMS软件建立了不同起落架布局的含弹性机体的全机多体动力学模型,进行了全机着陆仿真分析,研究了不同起落架布局的飞机机体弹性对起落架地面载荷的影响:对大多数机翼起落架布局的飞机,机体弹性减缓了起落架载荷;而对于机身起落架布局的飞机,考虑机体弹性后,起落架载荷有可能增大,也有可能减小.不同的飞机构型、不同的缓冲器参...     

基于磁链辨识的无轴承薄片电机轴向振动抑制策略

为了进一步提高BPMSM的悬浮性能,提出了一种基于磁链辨识的BPMSM轴向振动抑制策略,通过转子磁链的变化来估测转子轴向偏移量,然后将轴向偏移量转化为d轴电流分量参考值i*d,通过对i*d的调节来改善薄片转子的轴向恢复力,实现对轴向振动的有效抑制,从而有效改善电机的悬浮性能。试验结果表明:所提出的轴向振动抑制策略能够对薄片转子轴向振动进行有效抑制,提高系统的抗干扰能力,系统的运行性能得到了有效改善。     

Application of small-size antennas for estimation of angles of arrival of HF signals scattered by ionospheric irregularities

A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network.     

Thrusting maneuver control of a small spacecraft via only gimbaled-thruster scheme

The thrust vector control (TVC) scheme is a powerful method in spacecraft attitude control. Since the control of a small spacecraft is being studied here, a solid rocket motor (SRM) should be used instead of a liquid propellant motor. Among the TVC methods, gimbaled-TVC as an efficient method is employed in this paper. The spacecraft structure is composed of a body and a gimbaled-SRM where common attitude control systems such as reaction control system (RCS) and spin-stabilization are not presented. A nonlinear two-body model is considered for the characterization of the gimbaled-thruster spacecraft where, the only control input is provided by a gimbal actuator. The attitude of the spacecraft is affected by a large exogenous disturbance torque which is generated by a thrust vector misalignment from the center of mass (C.M). A linear control law is designed to stabilize the spacecraft attitude while rejecting the mentioned disturbance torque. A semi-analytical formulation of the region of attraction (RoA) is developed to ensure the local stability and fast convergence of the nonlinear closed-loop system. Simulation results of the 3D maneuvers are included to show the applicability of this method for use in a small spacecraft.     

L-band nighttime scintillations at the northern edge of the EIA along 95°E during the ascending half of the solar cycle 24

The characteristics of nighttime ionospheric scintillations measured at the L-band frequency of 1.575 GHz over Dibrugarh (27.5°N, 95°E, MLAT ～ 17°N, 43° dip) during the ascending half of the solar cycle 24 from 2010 to 2014 have been investigated and the results are presented in this paper. The measurement location is within or outside the zone of influence of the equatorial ionization anomaly depending on solar and geomagnetic activity. Maximum scintillation is observed in the equinoxes irrespective of solar activity with clear asymmetry between March and September. The occurrence frequency in the solstices shifts from minimum in the June solstice in low solar activity to a minimum in the December solstice in high solar activity years. A significant positive correlation of occurrence of scintillations in the June solstice with solar activity has been observed. However, earlier reports from the Indian zone (～75°E) indicate negative or no correlation of scintillation in June solstice with solar activity. Scintillations activity/occurrence in solstices indicates a clear positive correlation with Es recorded simultaneously by a collocated Ionosonde. In equinoxes, maximum scintillations occur in the pre-midnight hours while in solstices the occurrence frequency peaks just after sunset. The incidence of strong scintillations (S₄ ≥ 0.4) increases with increase in solar activity. Strong (S₄ ≥ 0.4) ionospheric scintillations accompanied by TEC depletions in the pre-midnight period is attributed to equatorial irregularities whereas the dusk period scintillations are related to the sporadic-E activity. Present results thus indicate that the current location at the northern edge of the EIA behaves as low as well as mid-latitude location.     

基于旋转高频信号注入法的内置式永磁同步电机低速段转子位置检测及其误差补偿

旋转高频信号注入法注入信号较为稳定,且位置估计过程不依赖电机参数,因而十分适用于内置式永磁同步电机(IPMSM)的零、低速转子位置检测。针对传统高频信号注入法无法辨别磁极的问题,用电压方波注入法检测磁极,结合有限元软件仿真,来合理选取方波电压幅值和时长,有效缩短了磁极判断耗时。分析了滤波器和信号离散化对位置估计精度的影响,提出在低速段可用线段拟合带通滤波器中心频率处的相频特性曲线,推导所需补偿角度与电机转速的关系。在理论分析的基础上,采用基于DSP28335的样机平台进行试验,结果表明磁极判断过程稳定,耗时较短,补偿后的位置估计值相比补偿前有明显改善,调速过程中系统动态性能良好。     

浅析民用飞机研制总体参数优化

分析了在概念设计阶段民用飞机总体设计工作内容和工作流程,并结合时下国外在用软件优缺点,构思了民用飞机总体设计参数综合优化的技术方案,包括优化设计架构、分析模型和优化算法等,为形成具有自主知识产权的民机总体设计综合分析和优化程序打下基础。     

Kink mode m = 1 in magnetic tube with discontinuous magnetic field

In this paper, we study conditions of realization and stability of kink modes with azimuthal wave numbers $m=\pm 1$ in cylindrical plasma flex with twisted magnetic field and homogeneous current along its axis. We assume permanent axial magnetic field both inside and outside the flex, surrounded by currentless plasma. Azimuthal magnetic field decreases inversely proportional to the distance from the boundary beyond the flex. We derived dispersion equations for stable and unstable modes in approximation of “thin” plasma flex. The analysis of equations has been provided for the case of discontinuous axial magnetic field on flex’s boundary. Conditions of propagation of wave modes have been defined. It was shown, that unstable modes can be implemented in certain interval of longitudinal wavenumbers. Results can be applied for the interpretation of solar magnetic tubes behavior, using measurements, provided by spacecrafts.