反步法与神经网络融合的平流层飞艇轨迹鲁棒控制方法

针对平流层飞艇水平轨迹控制面临外部风场扰动和模型参数不确定的特点,提出一种反步法与RBF神经网络融合的非线性鲁棒轨迹控制方法.该方法采用Lagrange动力学模型,通过反步法直接求解推力和力矩的控制律,采用RBF神经网络动态优化调整反步法的控制增益参数.仿真结果表明,新的控制方法可实现平流层飞艇对直线/圆组合式参考轨迹...     

小子样下导电滑环磨损失效仿真的可靠性评估研究

针对滑环失效数据较少的特点，构建导电滑环磨损失效模型，结合小子样数据处理法和随机性理论对滑环摩擦副进行可靠性评估研究。首先，考虑滑环摩擦副在热力电多场耦合环境下的特点，应用传热学、赫兹理论、能量守恒定律量化多场耦合对滑环摩擦副的影响，再结合Archard模型理论构建导电滑环摩擦副磨损失效模型。然后，采用小子样数据的虚拟增广法和Boot-strap法对仿真数据进行扩展，根据滑环磨损特征量分布规律分别得到随机失效阈值与固定阈值下的可靠度函数曲线，以某厂制造的导电滑环为例，进行滑环摩擦副可靠性评估，实验结果表明随机失效阈值下的可靠度与实际更接近。研究表明所构建的磨损模型和方法可以有效地对导电滑环进行可靠性评估，避免了传统的必须依赖大量试验数据的方法，解决了缺少滑环试验数据而难以进行可靠性评估的问题，填补了导电滑环可靠性研究的空白。     

天宫号目标飞行器氢镍蓄电池压力-容量充电控制研究简

作为在轨管理的关键部分,良好的充电控制是保证蓄电池长寿命的重要因素.对于氢镍蓄电池,压力-容量充电控制是最理想的充电控制方式,但存在压力检测难度大、控制策略复杂等困难.天宫一号目标飞行器氢镍蓄电池通过大量的压力测量地面可靠性试验,解决了压力传感器的测量稳定性及一致性问题;同时提出柔性充电控制策略,给出了压力-容量标准曲线、不同荷电态下的充电电流及压力控制点修正系数.在轨数据表明,天宫一号目标飞行器氢镍蓄电池压力-容量充电控制稳定,满足设计要求.     

Solution of the five-layer beam bending problem using the calculus of variation

The paper deals with the problem of lateral bending for the five-layer panel with the lightweight filler that is reduced to the bending problem of a beam fixed at the end sections. To solve the differential equations describing the beam bending, the Euler-Lagrange variational principle is used.     

Formation of programmed spatial flight trajectories of unmanned aerial vehicles

In this paper, we introduce a concept of coordinated turn that means the application of the lifting force being perpendicular to the UAV velocity vector and parallel to the surface on which the exact point target is located. Analytical solutions of the corresponding differential equations of the coordinated turn are derived.     

The effect of detuning of the partial frequency of MEMS gyros sensing elements on the amplitude-frequency response

The effect of detuning the partial frequencies of MEMS gyroscopes on its amplitudefrequency response is investigated. The formulated mathematical model allows defining requirements for the tolerances on gyros parameters, which determine the values of gyros partial frequencies, at the design stage of the sensor.     

The 3D Computational Investigation of Film Cooling Effectiveness for Turbine Nozzle Vanes with “Meridian Constriction” and Shaped Film-Cooling Holes

Active influence dimension of film cooling along the blade profile is investigated with using the Spalart–Allmaras turbulence model. The cooling effectiveness of vane platforms and vane fillets is studied with the use of perforation holes on the leading edge.     

Determination of Slag Retention Ability of Gating Systems

The paper highlights results of analyzing the gating systems in terms of assurance of slag retention at the stage when the mold cavity is filled up with the melt. Quantitative values of parameters as to assessment of slag retention were obtained that can be applied in selecting the gating system type for a casting.     

Reusable Space Transportation System

We present a design lay-out diagram of the reusable space transportation system that consists of an aerospace transformed vehicle that is injected into an orbit by means of the first and second stages. Some starting configurations of such system with the first and second stages are considered.     

Old-Aged Primary Distance Indicators

Old-aged stellar distance indicators are present in all Galactic structures (halo, bulge, disk) and in galaxies of all Hubble types and, thus, are immensely powerful tools for understanding our Universe. Here we present a comprehensive review for three primary standard candles from Population II: (i) RR Lyrae type variables (RRL), (ii) type II Cepheid variables (T2C), and (iii) the tip of the red giant branch (TRGB). The discovery and use of these distance indicators is placed in historical context before describing their theoretical foundations and demonstrating their observational applications across multiple wavelengths. The methods used to establish the absolute scale for each standard candle is described with a discussion of the observational systematics. We conclude by looking forward to the suite of new observational facilities anticipated over the next decade; these have both a broader wavelength coverage and larger apertures than current facilities. We anticipate future advancements in our theoretical understanding and observational application of these stellar populations as they apply to the Galactic and extragalactic distance scale.