机载分布式系统的透明性设计

在分析国外分布式系统和ASAAC标准的基础上指出,分布式系统的透明性主要体现在8个方面,即访问透明、位置透明、并发透明、备份透明、故障透明、迁移透明、性能透明和扩充透明,并对实现这8种透明性所采用的理论和技术进行了阐述,目的在于把握分布式系统的设计方向和获取一些设计经验.     

俯仰振荡翼型推阻力转变滞后机制数值研究

扑翼产生的反卡门涡街被认为是一种推力型尾迹,但已有研究指出,随着斯特劳哈尔数(St)增大,低雷诺数下俯仰振荡翼型的净推力产生明显滞后于反卡门涡街的出现。为探究该现象背后的物理机制,对NACA0012翼型在雷诺数1 000条件下作简谐俯仰运动的流场进行了数值模拟。采用翼型表面积分方法和基于有限控制体的气动力估计方法分别研究了翼面分布力特性和尾迹流场特性变化对阻力-推力转变临界点的影响。翼面分布力积分结果表明,当翼型振荡参数进入对应反卡门涡街尾迹形态区域时,翼面压力分布产生的推力分量无法克服剪切层的黏滞阻力,是造成俯仰翼型推力产生滞后于反卡门涡街出现的主要原因。对尾迹流场及相应的推阻力特性变化的分析表明,尽管反卡门涡街会产生"喷流效应",但在St较小时,其产生的动量诱导推力无法克服反卡门涡自身的涡致阻力和尾迹流场压力损失引入的附加阻力,因此即使存在反卡门涡街也不能产生净推力,进而从流场分析的角度进一步解释了这一滞后现象的发生机制。     

嫦娥五号月球轨道交会对接远程导引轨道设计与飞行实践

结合月球轨道交会对接任务的特殊性和中国探月工程的实际工程约束,介绍了嫦娥五号任务月球轨道交会对接远程导引轨道设计,包括轨道器调相和上升器远程导引两方面内容,重点介绍了月球轨道交会对接远程导引多脉冲调相轨道方案的选择、标称轨道优化设计、轨控策略和误差分析结果以及实际飞行轨道控制的情况。飞行实践数据分析表明:嫦娥五号任务月球轨道交会对接远程导引轨道设计是正确合理的,实际飞行的速度增量满足推进剂预算的要求,全飞行过程测控条件良好,交班点控制精度完全满足转自主控制的要求,有力保障了交会对接和样品转移的顺利完成。     

Pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method

In order to shorten the data update period and further improve the accuracy, a pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method is proposed. The asynchronous overlapping observation method partially overlaps the two adjacent observation periods, so that the data update period depends on the minimum pulsar observation period rather than the maximum like the other algorithms. The number of sampling points is also reduced to 2, which will effectively reduce the calculation burden. The proposed pre-correction extended Kalman filter uses observation data of adjacent sampling points to achieve a two-fold correction and makes up for the problem of insufficient observations on some sampling points caused by the observation method. Finally, simulations show that the proposed algorithm reduces the position and velocity errors by 21.55% and 19.13% compared to the EKF based on asynchronous observation method when using three detectors to observe the corresponding pulsars simultaneously. At the same time, the running time of one data update calculation is only 6.6% more than that of the EKF algorithm based on synchronous observation method.     

具有SGCMG系统的挠性卫星姿态机动控制及验证

针对挠性卫星在轨姿态快速机动的需求，开展了星体姿态机动控制方法及控制实现研究。基于建立的挠性卫星姿态跟踪控制误差方程，给出了PD控制与补偿控制相结合的姿态跟踪控制器形式；考虑系统实现的时延影响，利用经典频率分析方法选择了兼顾系统稳定性及宽带控制的控制参数；在控制具体实现中，采用一种新型的基于力矩矢量调节奇异规避操纵策略，克服常规鲁棒奇异规避操纵存在的框架“锁死”现象，在解决奇异规避的同时避免激发挠性振动。所提出方法的有效性通过了在轨验证。     

A MARS-based method for estimating regional 2-D ionospheric VTEC and receiver differential code bias

The geometry-free linear combination of dual-frequency GNSS reference station ground observations are currently used to build the Vertical Total Electron Content (VTEC) model of the ionosphere. As it is known, besides ionospheric delays, there are differential code bias (DCB) of satellite (SDCB) and receiver (RDCB) in the geometry-free observation equation. The SDCB can be obtained using the International GNSS Service (IGS) analysis centers, but the RDCB for regional and local network receivers are not provided. Therefore, estimating the RDCB and VTEC model accurately and simultaneously is a critical factor investigated by researchers. This study uses Multivariate Adaptive Regression Splines (MARS) to estimate the VTEC approximate model and then substitutes this model in the observation equation to form the normal equation. The least squares method is used to solve the RDCB and VTEC model together. The research findings show that this method has good modeling effectiveness and the estimated RDCB has good reliability. The estimated VTEC model applied to GPS single-frequency precise point positioning has better positioning accuracy in comparison to the IGS global ionosphere map (GIM).     

Three-Dimentional Surface Light Irradiance Reconstruction in Bioluminescence Tomography

Reconstruction of 3D surface irradiance distribution using multiple views captured by charged coupled device(CCD)camera is the basis of solving the light source in bioluminescence tomography(BLT).A simple and convenient mapping technique based on the pin-hole imaging model and Lambert′s cosine law was presented to establish the relationship between gray levels and irradiance intensities.Compared with previous integrating sphere camera calibration used in BLT,the proposed method can effectively avoid heavy burden of simulation experiment to obtain the corresponding relationship of gray levels and irradiance intensities.The accuracy and feasibility of the proposed method are validated with no more than 1mm location error by different types of phantom experiments.The mapping approach is also applicable to other noncontact optical imaging system.     

A prediction model of short-term ionospheric foF2 based on AdaBoost

In this paper, the AdaBoost-BP algorithm is used to construct a new model to predict the critical frequency of the ionospheric F2-layer (foF2) one hour ahead. Different indices were used to characterize ionospheric diurnal and seasonal variations and their dependence on solar and geomagnetic activity. These indices, together with the current observed foF2 value, were input into the prediction model and the foF2 value at one hour ahead was output. We analyzed twenty-two years’ foF2 data from nine ionosonde stations in the East-Asian sector in this work. The first eleven years’ data were used as a training dataset and the second eleven years’ data were used as a testing dataset. The results show that the performance of AdaBoost-BP is better than those of BP Neural Network (BPNN), Support Vector Regression (SVR) and the IRI model. For example, the AdaBoost-BP prediction absolute error of foF2 at Irkutsk station (a middle latitude station) is 0.32 MHz, which is better than 0.34 MHz from BPNN, 0.35 MHz from SVR and also significantly outperforms the IRI model whose absolute error is 0.64 MHz. Meanwhile, AdaBoost-BP prediction absolute error at Taipei station from the low latitude is 0.78 MHz, which is better than 0.81 MHz from BPNN, 0.81 MHz from SVR and 1.37 MHz from the IRI model. Finally, the variety characteristics of the AdaBoost-BP prediction error along with seasonal variation, solar activity and latitude variation were also discussed in the paper.     

自然形高空气球上升过程形状预测

为研究高空气球在上升过程中的形状变化以及蒙皮应力分布情况，并给气球的结构设计以及强度设计提供一定依据，本文建立了气球上升过程中的热力学模型，同时基于高空气球蒙皮材料具有非线性、黏弹性、各向异性和不能抗压等特点，通过简化气球几何模型，采用最小势能法预测自然形高空气球上升过程中的形状，并分析了气球上升过程中的应力分布情况，气球的应力极值出现在气球顶部和底部，而经向应力的数量级远大于纬向应力；还对比了不同充气量下、不同时刻下气球形状及应力分布情况，为气球设计及工程应用提供了有效计算 方法。     

多维磁悬浮隔振系统动力学模型与控制策略

磁悬浮隔振系统具有非线性、强耦合、高响应、宽频带等特点，系统的隔振控制目标与其定子和浮子之间的位置约束相互制约，这对系统的精密控制提出了较大的挑战。为解决该问题，建立了面向控制的六自由度磁悬浮隔振系统非线性动力学模型，并提出了双闭环控制策略，使系统在低频到中高频带内实现隔振控制，在极低频带内实现跟踪控制。采用PD定点控制算法，在MATLAB/Simulink环境中开发了控制系统仿真程序，通过分析不同扰动频率下浮子的绝对运动响应以及定子与浮子之间的相对运动响应，获得了系统的隔振控制与跟踪控制仿真结果。搭建了磁悬浮隔振平台样机测试系统，验证了动力学模型的正确性和控制策略的有效性。