基于Kalman滤波的GPS/INS接收机自适应干扰抑制方法

 考虑到惯导信息辅助GPS(GPS/INS)接收机对干扰抑制实时性的要求,提出一种基于Kalman滤波的GPS/INS接收机自适应干扰抑制方法。自适应广义旁瓣相消(GSC)多采用低复杂度最小均方(LMS)算法更新权矢量,收敛速率较低,严重时会导致接收机定位中断。首先利用Householder变换构建GSC下支路的阻塞矩阵,用于阻塞任意二维阵型阵列接收的期望信号;再用Kalman滤波自适应更新下支路权矢量,从而有效提高阵列输出信干噪比(SINR)。理论分析和仿真结果说明本文方法可有效抑制干扰对接收机的影响,且具有实时性高的特点。     

非均匀来流下等压力梯度曲面压缩系统的试验研究

根据激波和膨胀波理论,设计了Ma=5.3等压力梯度曲面压缩系统。在Ma=3.85和Ma=5.3的小高超风洞完成均匀来流试验,并利用风洞壁面自然发展的附面层进行非均匀来流等压力梯度曲面压缩系统性能试验。试验发现:均匀来流下,试验模型壁面压力均按照等压力梯度规律分布,但来流马赫数Ma=5.3时出口流场均匀性较差;非均匀来流下,大量的附面层吸入不仅影响壁面压力不再呈等压力梯度分布,而且对出口流场均匀性影响也极大。      

民用航空发动机拐点温度的计算方法

影响民航飞机飞行安全的因素众多,其中动力装置性能为一主要因素。针对国内外民机主力机型A320系列飞机的航空发动机CFM56-5B的拐点温度进行研究。阐释高涵道比发动机拐点温度的定义,统计分析CFM56-5B系列发动机拐点温度值及影响因素。分析其对飞机实施假设温度减推力起飞的意义及实施方法,飞机运行高温高原机场的性能要求以及拐点温度对发动机实施健康评估保障飞行安全的作用。应用最小二乘法对起飞数据进行处理,分别采用平均值法和正切法计算实际拐点温度,并与理论值验证得正切法可行。     

直升机起落架虚拟静力试验方法研究

基于LMS Virtual.Lab多体动力学仿真平台,建立了某型直升机起落架虚拟静力试验方法。基于修正的Craig-Bampton固定界面模态综合法,通过求解各构件的Craig-Bampton模态信息,建立了直升机起落架试验系统的刚柔耦合动力学模型。通过动力学仿真,分析了不同工况下监测点位移随载荷变化规律,考察了夹具柔性对仿真结果的影响。仿真结果表明:对虚拟静力试验系统中的与起落架直接连接夹具加以柔性化处理,其起落架结构的最大位移与试验结果吻合较好;夹具柔性对仿真结果有较大影响。     

基于CFD的变后掠翼单速度最优后掠角预测模型

为延长飞行器续航时间,探索变后掠翼飞行器控制规律,根据新型变后掠翼飞行器模型,探究了通过飞行器速度及迎角来控制弹翼后掠角度,以达到最优气动性能,从而使该飞行器获得更长续航力.选取飞行马赫数为0.4～0.8、前缘后掠角度为15°～45°内的39个关键点,在迎角为0°～14°范围内进行CFD仿真,将仿真结果在不同数学模型下...     

大型客机后缘襟翼滑轨整流罩气动外形设计方法

大型客机后缘襟翼机构伸出机翼下表面会带来气动损失,必须设计相应整流罩。整流罩的外形尺寸对气动力影响较大,会直接影响飞机的气动特性。设计整流罩时应该遵循整流罩外形设计要求,使其引起的高速巡航阻力尽可能小。在查阅相关文献、对比研究大量整流罩图片、分析研究计算机辅助设计(CAD)中NURBS曲面曲线描述方法的基础上,建立了一套详细的大型客机后缘襟翼滑轨整流罩外形设计方法,该方法在满足整流罩包裹住机构、减小气动损失等基本要求的同时,缩短了整流罩设计周期。     

带VSCMGs的航天器姿态稳定及功率补偿控制

基于变速控制力矩陀螺群动力学模型建立其复合控制方程和分系统解耦约束方程,用矩阵投影方法同步设计得到航天器姿态与能量一体控制复合操纵律,利用Lyapunov方法分析了转子轴向惯量误差对姿态控制分系统的影响.根据飞轮转子轴向惯量与功率输出之间的误差关系设计出功率控制补偿器.复合操纵律中的力矩和功率两解形式相同,约束方程使得姿态与能量控制两分系统解耦,便于进行考虑执行机构特性的闭环控制系统性能分析.考虑飞轮转子轴向惯量误差时,姿态控制分系统的输出耗散特性使其能够保持稳定,而功率控制分系统输出误差与转子轴向惯量误差成比例关系,经过补偿后功率输出能满足控制要求.     

Research on constellation refueling based on formation flying

A new scheme for refueling satellite constellation is proposed in this paper. Compared with the traditional research, where the satellite refueling is implemented through spacecraft rendezvous and docking, the new pattern studied here is based on formation flying, and it is more feasible, safer and more reliable. On the grounds of the proposed pattern, two refueling strategies are studied. The first is called single supplier refueling (SSR) based on formation flying. In this scenario, one fuel-sufficient satellite called a supplier, departs from its parking orbit, and after a series of orbit maneuvers, arrives at the target constellation that consists of multiple fuel-deficient satellites called workers. It then transfers equal fuel to each worker within the prescribed mission time. The second strategy is called double suppliers refueling (DSR) based on formation flying. This time two suppliers take charge of refueling half of the workers respectively in the same way as SSR. Using a genetic algorithm, the orbit of a supplier with a minimum consumption of fuel can be obtained once the mission time is fixed. Simulation results indicate that DSR is superior to SSR and that this dominance will be more distinct as the number of workers increases and the mission time decreases.     

Global Properties of Solar Flares

This article broadly reviews our knowledge of solar flares. There is a particular focus on their global properties, as opposed to the microphysics such as that needed for magnetic reconnection or particle acceleration as such. Indeed solar flares will always remain in the domain of remote sensing, so we cannot observe the microscales directly and must understand the basic physics entirely via the global properties plus theoretical inference. The global observables include the general energetics—radiation in flares and mass loss in coronal mass ejections (CMEs)—and the formation of different kinds of ejection and global wave disturbance: the type II radio-burst exciter, the Moreton wave, the EIT “wave”, and the “sunquake” acoustic waves in the solar interior. Flare radiation and CME kinetic energy can have comparable magnitudes, of order 10³² erg each for an X-class event, with the bulk of the radiant energy in the visible-UV continuum. We argue that the impulsive phase of the flare dominates the energetics of all of these manifestations, and also point out that energy and momentum in this phase largely reside in the electromagnetic field, not in the observable plasma.     

脉冲周期介质阻挡放电作用的PIV实验研究

静止大气下,对施加脉冲周期介质阻挡放电,半顶角为10°的圆锥前体进行了PIV实验研究。采用总平均和相位锁定平均方法对脉冲周期放电进行了分析;对比了不同占空比和不同相位角沿θ=90°半径上的切向速度和轴向涡量分布,得到了在圆锥表面等离子体诱导的最大速度和最大涡量;分析了脉冲周期放电的动量转移特性。实验结果表明：脉冲周期放电引发动量转移的主要机制是涡的增强而非气流的加速;当激励器处于脉冲放电间歇时,相位锁定平均的最大速度和最大涡量不为零,存在流动滞后效应,有利于节省能耗。