基于能量法的刷式密封刷丝颤振流固耦合研究

为了研究刷式密封刷丝颤振特性,采用能量法及双向流固耦合与动网格技术,建立了刷式密封刷丝颤振特性瞬态流固耦合求解模型,将数值模型结果与理论模型和实验结果分别进行验证;在此基础上,从非定常气动力做功角度分析刷丝的变形规律,研究了刷式密封结构参数对刷丝颤振特性的影响。结果表明:非定常气动力做功与刷丝变形运动随时间均呈振荡变化趋势;后挡板保护高度从2.1~3.6mm,刷丝长度从4.0~5.5mm以及刷丝直径从0.13~0.19mm非定常气动力做功减少,有利于抑制颤振的发生;刷丝间隙及刷丝束与后挡板轴向间隙的变化对刷丝颤振影响不大。     

兰姆波频散方程的分析及数值迭代算法

根据兰姆波运动规律的时间简谐波因子与频散曲线的物理特性,用数值迭代法在实数域内求解频散方程.给出了铝板中兰姆波相速度和群速度的解.研究表明:该法可较易获得频散曲线,无需方程分段求解,具一定的参考价值.     

Shock waves in water foams

Propagation of shock waves in tubes filled with water foams is studied using pressure gauges. Low amplitude shock waves consist of a precursor which propagates at a velocity slightly less than the acoustic velocity in the gas, and of a main compression wave which propagates slower than the precursor. Stronger shock waves have a single front. Maximum pressure rise in the incident and reflected shock waves cannot be calculated using one-dimensional conservation equations at the shock front. It is suggested that the flow of the liquid in foam cells has to be taken into account in order to predict the behavior of shock waves in foams. The nature of the gas which fills the cells is shown to have a strong effect on the quenching of blast waves in foams.     

Longitudinal variations of geomagnetic and ionospheric parameters in the Northern Hemisphere during magnetic storms according to multi-instrument observations

We present a joint analysis of longitude-temporal variations of ionospheric and geomagnetic parameters at middle and high latitudes in the Northern Hemisphere during the two severe magnetic storms in March and June 2015 by using data from the chains of magnetometers, ionosondes and GPS/GLONASS receivers. We identify the fixed longitudinal zones where the variability of the magnetic field is consistently high or low under quiet and disturbed geomagnetic conditions. The revealed longitudinal structure of the geomagnetic field variability in quiet geomagnetic conditions is caused by the discrepancy of the geographic and magnetic poles and by the spatial anomalies of different scales in the main magnetic field of the Earth. Variations of ionospheric parameters are shown to exhibit a pronounced longitudinal inhomogeneity with changing geomagnetic conditions. This inhomogeneity is associated with the longitudinal features of background and disturbed structure of the geomagnetic field. During the recovery phase of a storm, important role in dynamics of the mid-latitude ionosphere may belong to wave-like thermospheric disturbances of molecular gas, propagating westward for several days. Therefore, it is necessary to extend the time interval for studying the ionospheric effects of strong magnetic storms by a few days after the end of the magnetospheric source influence, while the disturbed regions in the thermosphere continues moving westward and causes the electron density decrease along the trajectories of propagation.     

Feasibility,and Contribution to Ocean Circulation Studies,of Ocean Bottom Pressure Determination

An assessment is presented of the probable magnitude of ocean signals causing aliasing in ocean bottom pressure measurements from the GRACE satellite mission. Even after modelling as much of the high frequency signal as possible, variability between 1 mbar (in quiet ocean regions) and 10 mbar (on some shelves) is likely to remain. Interpretation of the resulting retrievals will therefore rely on the facts that the satellite sampling will average the aliasing signal to some extent, and that the spatial patterns of aliased signal and true signal will be different. To this end, a theoretical argument is given, and supported by model diagnostics, suggesting that observable bottom pressure signals will be strongly constrained by the shape of the ocean floor. The modelled magnitudes offer the prospect of significant detectable signals and, while the model accuracy can be called into question, there are hints from Earth rotation and satellite orbit measurements that significant mass redistributions occur in the ocean. It seems certain that we will learn something new about the oceans from GRACE. This revised version was published online in August 2006 with corrections to the Cover Date.     

轰炸机的发展历程和前景

介绍了轰炸机在各历史阶段发挥的重要作用，分析了轰炸机从诞生到第二次世界大战中发展成熟，以及在冷战时期轰炸机发展的3个阶段。描述了在每个时期不同战场环境下对轰炸机的不同要求，以及由此而产生不同的气动布局形式，进而分析了未来轰炸机发展的3个方向和美国当前可能的型号选择。     

高速热流下薄壁结构声振响应分析及寿命预估

现代飞行器飞行过程中发动机薄壁结构受高速热流冲击面临着极为严酷的工作环境,使结构产生大挠度动力学响应以及疲劳损伤破坏现象。为获取难以实测的热流冲击下结构声振响应规律及疲劳破坏时间,采用耦合有限元/边界元的方法进行数值模拟分析与热声疲劳试验相结合的方法,根据载荷效果构建与试验件尺寸完全一致的数值仿真模型,对热声载荷下薄壁结构进行仿真计算。采用功率谱密度（PSD）法分析频率响应峰值随声载荷变化规律,并通过改进的雨流计数法对声振响应数据进行统计分析,得到疲劳寿命时间。并对比声振响应仿真计算结果与试验结果发现误差小于2%,验证了数值仿真的可靠性。在此基础上,对高速热流冲击作用下薄壁结构进行数值仿真分析,通过分析频率响应峰值随温度和流速的变化规律获取不同温度各流速下结构声振响应及疲劳寿命变化规律,并阐述造成这种变化的原因。本文完成的工作可对高速热流环境下薄壁结构响应分析和寿命预估提供参考依据。     

基于CFD的某减速器飞溅润滑仿真分析与验证

为评估飞溅润滑减速器的储油结构是否合理,基于计算流体动力学方法,建立了包含机匣、螺旋锥齿轮等构件的某减速器飞溅润滑动态仿真模型,开展了气液两相流飞溅润滑流体仿真计算与分析,获得了减速器内部的滑油运动轨迹及分布云图。通过仿真分析可以发现:输入端油兜收集到的滑油量为531 mL,大于输出端收集到的滑油量65 mL;4号油兜收集到的滑油量为0 mL,结构设计存在不合理之处,并进行了飞溅润滑试验验证。仿真分析结果与试验结果的趋势一致,验证了仿真分析方法的准确性,为飞溅润滑减速器储油结构设计提供了指导。     

盘一盘螺栓连接结构模态频率分析

基于ANSYSWorkbench软件,采用层单元法和多点约束技术,模拟了盘一盘螺栓连接结构的螺栓预紧力,对其进行了模态分析,并与试验结果进行了比较。研究表明：采用层单元法模拟螺栓预紧力的模态结果与试验结果吻合较好,为在预紧力作用下螺栓连接结构模态频率的有限元计算提供了1种有效方法。     

Time delays in the nonthermal radiation of solar flares according to observations of the <Emphasis Type="Italic">CORONAS-F</Emphasis> satellite

In 2001–2003, the X-ray and microwave observations of ten solar flares of M- and X-classes were carried out by the CORONAS-F orbital station, the RSTN Sun service, and Nobeyama radio polarimeters. Based on these observations, a correlation analysis of time profiles of nonthermal radiation was performed. On average, hard X-ray radiation outstrips the microwave radiation in 9 events, i.e., time delays are positive. The appearance of negative delays is associated with effective scattering of accelerated electrons in pitch angles, where the length of the free path of a particle is less than the half-length of a flare loop. The additional indications are obtained in favor of the need to account for the effect of magnetic mirrors on the dynamics of energetic particles in the coronal arches.