An FV-EE model to predict lean blowout limits for gas turbine combustors with different structures and sprays

The occurrence of Lean Blowout(LBO) is a disadvantage that endangers a stable operation of gas turbines. A determination of LBO limits is essential in the design of gas turbine combustors. A semiempirical model is one of the most widely used methods to predict LBO limits.Among the existing semiempirical models for predicting LBO limits, Lefebvre’s LBO model and the Flame Volume(FV) model are particularly suitable for gas turbine combustors. On the basis of Lefebvre’s and FV models, the concept o...     

Hierarchical model updating strategy of complex assembled structures with uncorrelated dynamic modes

In structural simulation and design, an accurate computational model directly determines the effectiveness of performance evaluation. To establish a high-fidelity dynamic model of a complex assembled structure, a Hierarchical Model Updating Strategy(HMUS) is developed for Finite Element(FE) model updating with regard to uncorrelated modes. The principle of HMUS is first elaborated by integrating hierarchical modeling concept, model updating technology with proper uncorrelated mode treatment, and...     

基于高轨导航接收机的自动化地面测试系统

高轨卫星导航接收机是实现高轨航天器自主定轨的核心设备。为在地面测试阶段对高轨卫星导航接收机进行充分高效的验证，亟需设计基于高轨卫星导航接收机的地面测试系统。设计了一种基于高轨卫星导航接收机的自动化地面测试系统，主要创新点如下：第一，本系统可对高轨卫星导航接收机实际在轨状态下接收到的导航星座信号进行仿真；第二，具有模拟包含北斗三号等多导航卫星星座信号的功能；第三，本系统充分考虑自动化、通用化与一体化设计。提出的基于高轨卫星导航接收机的自动化地面测试系统能够在地面测试阶段对高轨卫星导航接收机进行充分验证，并充分考虑测试实施，从自动化、通用化、一体化方面提升测试效率，减少人为操作失误导致的质量问题，解决人工判读带来的误判漏判问题。     

离心式压气机出口动态压力的关联维数特征分析

基于相空间重构理论,以800kW离心式压气机在不同工况下的出口动态压力为研究对象,分析了其时域、频域和关联维数特征,目的是实现喘振识别.结果表明:系统稳态时,动态压力幅值小且随机特性强,系统的混沌特征较为明显.此状态下的关联维数曲线波动很大,饱和关联维数也较大(8～20),并且部分时段不存在饱和关联维数.而随着系统经过...     

Study of aerodynamic and inertial forces of a experimental and numerical methods

The force-generation mechanism of a dovelike flapping-wing micro air vehicle was studied by numerical simulation and experiment. To obtain the real deformation pattern of the flapping wing, the digital image correlation technology was used to measure the dynamic deformation of the wing. The dynamic deformation data were subsequently interpolated and embedded into the CFD solver to account for the aeroelastic effects. The dynamic deformation data were further used to calculate the inertial forces...     

一种互相关法测量相位噪声理论及仿真分析

相位噪声测量是无线电计测领域的重要研究内容，随着信号源等各种信号仪器设备的不断发展，相位噪声测量技术方面也产生了更高的要求。介绍了互相关法测量相位噪声的理论与仿真分析方法，通过理论推导阐释了互相关法抑制干扰噪声的原理，在推论的基础上建立了基于MATLAB的仿真分析模型，仿真验证了不同互相关次数下，系统噪声底部的改善程度，并进一步分析了双通道相关性对互相关运算结果的影响，得到了对应的仿真验证结果，为相关的工程设计提供参考。     

On the time lag between solar wind dynamic parameters and solar activity UV proxies

The solar activity displays variability and periodic behaviours over a wide range of timescales, with the presence of a most prominent cycle with a mean length of 11 years. Such variability is transported within the heliosphere by solar wind, radiation and other processes, affecting the properties of the interplanetary medium. The presence of solar activity–related periodicities is well visible in different solar wind and geomagnetic indices, although their time lags with respect to the solar cycle lead to hysteresis cycles. Here, we investigate the time lag behaviour between a physical proxy of the solar activity, the Ca II K index, and two solar wind parameters (speed and dynamic pressure), studying how their pairwise relative lags vary over almost five solar cycles. We find that the lag between Ca II K index and solar wind speed is not constant over the whole time interval investigated, with values ranging from 6 years to $～$1 year (average 3.2 years). A similar behaviour is found also for the solar wind dynamic pressure. Then, by using a Lomb-Scargle periodogram analysis we obtain a 10.21-year mean periodicity for the speed and 10.30-year for the dynamic pressure. We speculate that the different periodicities of the solar wind parameters with respect to the solar 11-year cycle may be related to the overall observed temporal evolution of the time lags. Finally, by accounting for them, we obtain empirical relations that link the amplitude of the Ca II K index to the two solar wind parameters.