柔性航天器高精度隔振与定向研究

随着大型航天器柔性越来越大,结构越加复杂,导致低频柔性模态密集,但同时需要极高的定向精度及姿态稳定度, 这就对航天器姿态控制系统提出了更高的要求。本文采用拉格朗日法建立了柔性航天器姿态轨道耦合动力学模型,并设计了大角度机动航天器的姿态控制器。Lyapunov定理给出闭环系统的稳定性,在0.03Nm均方根的白噪声扰动下,大角度机动姿态角误差小于0.02°,均方根误差0.003°, 为了抑制姿态抖振,设计了复合控制器,采用Stewart平台对敏感载荷局部高精度主动隔振和定向,局部控制后敏感载荷的定向误差小于0.0001°,均方根误差0.000036°。鲁棒 Η ∞ 控制器对Stewart平台主动镇定时,姿态抖振小于0.000002°,均方根误差小于 0.0000008° ,姿态稳定度优于0.00001°/s。     

基于TDICCD相机有源低通滤波器的优化研究

文章通过分析低通滤波器的特性,指出航天TDICCD相机中有源低通滤波器的重要性,提出优化实现的可行性,并给出了具体原理电路及仿真结果。     

Recent advances in film cooling enhancement: A review

Film cooling is an indispensable scheme in the design of highly-efficient cooling configurations to satisfy the thermal protection requirement of turbine hot section components. During the last few decades, vast efforts have been paid on the discrete-hole film cooling enhancement. In this paper, some of the recent literatures related to the passive strategies (such as shaped film cooling holes, upstream ramps, shallow trenches, mesh-fed slots) and the active strategies (such as the use of pulsation modulating device or plasma actuator) for film cooling enhancement are surveyed, with the aim at presenting an updated overview about the state of the art in advanced film cooling. In addition, some challenging issues are also outlined to motivate further investigations in such a broad topic.     

Active vibration control of piezoelectric bonded smart structures using PID algorithm

Thin-walled structures are sensitive to vibrate under even very small disturbances. In order to design a suitable controller for vibration suppression of thin-walled smart structures, an electro-mechanically coupled finite element(FE) model of smart structures is developed based on first-order shear deformation(FOSD) hypothesis. Considering the vibrations generated by various disturbances, which include free and forced vibrations, a PID control is implemented to damp both the free and forced vibrations. Additionally, an LQR optimal control is applied for comparison.The implemented control strategies are validated by a piezoelectric layered smart plate under various excitations.     

主动重心控制功能仿真建模与应用

减小飞行阻力、节省燃油消耗,是主动重心控制功能的重要收益之一,对功能方案的迭代和优化设计具有重要影响。基于主动重心控制技术原理和方案,耦合飞控系统模型、自动飞控系统模型、燃油系统模型、气动力模型、发动机模型和飞机六自由度（6-DOF）模型,建立某型飞机主动重心控制功能仿真模型。该模型计及燃油消耗引起的重心变化的影响,在...     

空间机器人主从遥操作的自抗扰控制

目前基于模型的控制方法是空间机器人遥操作控制的主流方法,但该方法不可避免地会引入运动的累积误差,甚至造成控制失稳。针对这一问题,基于自抗扰控制方法为空间机器人主从遥操作设计了一类单关节控制器,并采用计算机仿真方法研究了其基本性能,结果表明所设计的自抗扰控制器能够实现稳定的遥操作控制,且具有良好的抗扰性和鲁棒性。特别是由于自抗扰控制方法不依赖于机器人的数学模型,因此十分适合作为现行基于模型控制的有益补充。     

150座级商用发动机控制技术对比分析

主要对现役150座级商用发动机CFM56-5B、CFM56-7B、V2500以及下一代150座级商用发动机LEAP X、GTF的控制技术进行初步分析,包括对FADEC系统组成、燃油系统、各项控制技术及超转保护的分析,并对现役及下一代150座级商用发动机控制技术进行对比分析,初步分析出其各项技术的差异,最后给出分析结论并...     

An active debris removal parametric study for LEO environment remediation

Recent analyses on the instability of the orbital debris population in the low Earth orbit (LEO) region and the collision between Iridium 33 and Cosmos 2251 have reignited interest in using active debris removal (ADR) to remediate the environment. There are, however, monumental technical, resource, operational, legal, and political challenges in making economically viable ADR a reality. Before a consensus on the need for ADR can be reached, a careful analysis of its effectiveness must be conducted. The goal is to demonstrate the need and feasibility of using ADR to better preserve the future environment and to explore different operational options to maximize the benefit-to-cost ratio. This paper describes a new sensitivity study on using ADR to stabilize the future LEO debris environment. The NASA long-term orbital debris evolutionary model, LEGEND, is used to quantify the effects of several key parameters, including target selection criteria/constraints and the starting epoch of ADR implementation. Additional analyses on potential ADR targets among the existing satellites and the benefits of collision avoidance maneuvers are also included.     

宽带有源巴伦的仿真设计

文章重点研究基于分立PHEMT器件和HMIC工艺的有源巴伦,该成果可以进一步用于MMIC的设计。在1～2 GHz频率范围内,通过ADS软件对该有源巴伦进行仿真设计,其幅度差在0.17 dB之内,相位差在0.9°之内。利用AutoCAD软件生成PCB版图,采用Rogers4003基片加工。测试结果与仿真比较一致。     

High resolution spectroscopy of Seyfert warm absorbers with XMM-Newton

We present results from the analysis of an XMM-Newton observation of the Seyfert 1 galaxy NGC 7469, the first high resolution X-ray spectrum of this source. The Reflection Grating Spectrometer (RGS) spectrum has several narrow absorption and emission lines of O, N, C and Ne, originating from gas at a range of ionisation parameters, from log ξ1.6 to log ξ−2 (where ξ has the units erg cm s⁻¹). We demonstrate that the ionisation state of the warm emitter is consistent with that of the high-ionisation phase of the warm absorber, and compare the warm absorber in this object with those in other sources.