A fast arc fault detection method for AC solid state power controllers in MEA

Arc fault detection is desperately required in Solid State Power Controllers (SSPC) in addition to their fundamental functions because arcs will provoke growing harm and threat to aircraft safety. Experimental study has been done to obtain the faulted current data. In order to improve the detection speed and accuracy, two fast arc fault detection methods have been proposed in this paper with the analysis of only half cycle data. Both Fast Fourier Transform (FFT) and Wavelet Packets Decomposition (WPD) have been adopted to distinguish arc fault currents from normal operation currents. Analysis results show that Alternating Current (AC) arcs can be effectively and accurately detected with the proposed half cycle data based methods. Moreover, experimental verification results have also been provided.     

New insights into SNR evolution revealed by the discovery of recombining plasmas

We report the discovery of recombining plasmas in three supernova remnants (SNRs) with the Suzaku X-ray astronomy satellite. During SNR’s evolution, the expanding supernova ejecta and the ambient matter are compressed and heated by the reverse and forward shocks to form an X-ray emitting hot plasma. Since ionization proceeds slowly compared to shock heating, most young or middle-aged SNRs have ionizing (underionized) plasmas. Owing to high sensitivity of Suzaku, however, we have detected radiative recombination continua (RRCs) from the SNRs IC 443, W49B, and G359.1–0.5. The presence of the strong RRC is the definitive evidence that the plasma is recombining (overionized). As a possible origin of the overionization, an interaction between the ejecta and dense circumstellar matter is proposed; the highly ionized gas was made at the initial phase of the SNR evolution in dense regions, and subsequent rapid adiabatic expansion caused sudden cooling of the electrons. The analysis on the full X-ray band spectrum of IC 443, which is newly presented in this paper, provides a consistent picture with this scenario. We also comment on the implications from the fact that all the SNRs having recombining plasmas are correlated with the mixed-morphology class.     

飞机刹车系统接地保护功能研究

分析了目前飞机刹车系统接地保护功能,提出了一种安全可靠的飞机接地保护功能的实现方法.这种方法彻底改变现有飞机接地保护功能弊端,避免了飞机带压着陆,拖胎、爆胎事故发生,最大可能的缩短地面刹车距离.     

空投舱体着陆冲击仿真与分析

针对空投物资方式中物资的安全着陆问题,采用舱体结构对空投救生装备进行缓冲保护.本文在对舱体空投问题进行了力学分析的基础上,采用显式非线性动力学分析有限元软件ANSYS/LS-DYNA对空投舱体着陆冲击进行模拟计算,根据仿真计算所得的舱体在冲击过程中的动态响应,来确定舱体结构设计方案的可行性,体现了设计的先进性.     

舰载无人机横侧向着舰控制律设计

舰载无人机横侧向控制一直是着舰控制律设计的难点。为了解决着舰横侧向控制的难题,针对舰载无人机的非线性模型采用了反演控制器设计方法,为解决传统反演的计算膨胀问题,引入了指令滤波方法,同时只设计了一个Lyapunov函数证明了稳定性;由于舰载机动力学模型不能精确获得,采用了自适应方法对其进行估计。设计的横侧向着舰控制器,能较好地解决横侧向控制器设计过程中的耦合问题,并且和传统PID进行了仿真对比,证明了所设计的控制律满足了对参考信号跟踪的性能要求。     

自动油门控制技术在舰载机上的应用

着舰技术是舰载机应用的一项高难技术,自动油门控制作为一项有效的着舰辅助手段,通过进场动力补偿,可有效提高舰载机着舰轨迹稳定性,进而显著提升着舰精度及着舰成功率。介绍了自动油门控制技术的起源、着舰需求、基本组成和控制原理,并对其未来发展前景进行了展望。     

国产着色渗透探伤剂主要性能的普查

本文对国产大部分着色渗透剂、清洗剂、显像剂的主要性能进行了测试，提出了存在的问题，供用户在使用过程中，对探伤剂的性能要求及监督引起重视。     

Numerical study on flow control of ship airwake and rotor airload during helicopter shipboard landing

A numerical study on flow control of ship airwake during shipboard landing is carried out to address the effect of flow control devices on helicopter rotor airload. The in-house Reynolds Averaged Navier-Stokes (RANS) based solver Rotorcraft AeroDynamics and Aeroacoustics Solver (RADAS), with combination of momentum source approach is employed to conduct the helicopter shipboard landing simulation. The control effects of three aerodynamic modifications of ship superstructure, i.e. ramp, notch and flap, in different Wind-Over-Deck (WOD) conditions are discussed. From the steady simulation results, the effect of spatial variation of ship airwake on rotor airloads is concluded. The aerodynamic modifications reduce the strength of shedding vortex and increase rotor normal force through delaying and relieving flow separation, and therefore are beneficial to alleviate the limitation of control inputs. By contrast, the perturbation of unsteady ship airwake can cause the serious oscillation of rotor forces during shipboard landing. The unsteady simulations show that the turbulence intensity of ship airwake and oscillatory rotor airloading, represented by Root-Mean-Square (RMS) loading, can be remarkably reduced by the ramp and notch modifications, while the flap modification has adverse effect. It means that flow control devices have large potential benefits to alleviate the pilot’s workload and improve the shipboard landing safety, but they should be well designed to avoid the introduction of more vortex, which leads to increase in disturbance of flow field.     

FUZZY IDENTIFICATION METHOD BASED ON A NEW OBJECTIVE FUNCTION

Many fuzzy models on modeling and controlmethods have been developed since Takagi-Sugeno model was proposed[1] .The main prob-lems of the fuzzy identifying method based on T-S model appear in the following two aspects:　　 1 It is important what heuristic knowledgeis chosen to acquire the premise structure of theT- S model.This problem is related to the opti-mal partition of input space of premise part andmodeling accuracy.　　 2 Itis crucial whatidentifying method is u-tilized to estimate …     

The damping of small-amplitude oscillations in quiescent prominences

The presence of small-amplitude oscillations in prominences is well-known from long time ago. These oscillations, whose exciters are still unknown, seem to be of local nature and are interpreted in terms of magnetohydrodynamic (MHD) waves. During last years, observational evidence about the damping of these oscillations has grown and several mechanisms able to damp these oscillations have been the subject of intense theoretical modelling. Among them, the most efficient seem to be radiative cooling and ion-neutral collisions. Radiative cooling is able to damp slow MHD waves efficiently, while ion-neutral collisions, in partially ionised plasmas like those of solar prominences, can also damp fast MHD waves. In this paper, we plan to summarize our current knowledge about the time and spatial damping of small-amplitude oscillations in prominences.