直升机高次谐波主动抑振技术

从控制的观点阐述高次谐波控制（ＨＨＣ）基本原理,提出ＨＨＣ旋翼数学模型;机体振动数学模型;ＨＨＣ参数辨识;控制律设计以及数字仿真验证     

Characteristics of equatorial nighttime spread F – An analysis on season-longitude,solar activity and triggering causes

To understand global variability and triggering mechanisms of ionospheric nighttime equatorial spread F (ESF), we analyzed measurements from satellite and a ground-based GPS station for the years between 2010 and 2017. In this study we present seasonal-longitudinal as well as monthly variability of ESF occurrence for solar minimum and yearly variations of ESF occurrence for solar maximum and minimum periods. One of the long standing open questions in the study of ESF is what exactly initiates the Rayleigh-Taylor (RT) plasma instability growth. This question is the focus of the present work. Zonal background eastward electric field and E × B upward plasma drift speed patterns are found to be critically important in understanding plasma irregularity formation. In addition to particular patterns observed on these parameters, the background plasma density in the local evening hours just before the onset of ESF occurrence is very important. Stronger plasma densities just before the onset of irregularities resulted in stronger plasma irregularities, while relatively less dense plasma just before the onset of irregularities resulted in relatively lower plasma irregularities. Seasonal variations in ESF activity between March and September equinox seasons with comparable plasma densities can be defined in terms of the rate of change of solar flux F10.7 (dF10.7/day) index. Strongest ESF occurrence and strongest dF10.7/day are measured in the same month out of all other months in 2016 and 2017. Longitudinal variations of ESF activity in our measurements are related to longitudinal variations of plasma densities. We also found that ESF occurrence is better correlated with rate of change of F10.7 index for months in equinox seasons than for months in solstice seasons for the years between 2013 and 2016.     

区域安全性分析在飞机总装过程中的应用探索

区域安全性分析(ZSA)是指为降低飞机机载系统在整机装配、维护等物理性集成时引起的飞机系统、飞机整机工作过程中的功能性风险,而在传统飞机物理样机阶段提前开展的结构与系统、系统与系统间协调性、技术符合性的分析检查工作.随着数字化设计模式的引入,部分区域安全性分析也尝试在设计阶段基于设计数字样机开展.在民用飞机设计领域,国...     

Low latitude ionospheric scintillation and zonal irregularity drifts observed with GPS-SCINDA system and closely spaced VHF receivers in Kenya

In this study we have used VHF and GPS-SCINDA receivers located at Nairobi (36.8°E, 1.3°S, dip −24.1°) in Kenya, to investigate the ionospheric scintillation and zonal drift irregularities of a few hundred meter-scale irregularities associated with equatorial plasma density bubbles for the period 2011. From simultaneous observations of amplitude scintillation at VHF and L-band frequencies, it is evident that the scintillation activity is higher during the post sunset hours of the equinoctial months than at the solstice. While it is noted that there is practically no signatures of the L-band scintillation in solstice months (June, July, December, January) and after midnight, VHF scintillation does occur in the solstice months and show post midnight activity through all the seasons. VHF scintillation is characterized by long duration of activity and slow fading that lasts till early morning hours (05:00 LT). Equinoctial asymmetry in scintillation occurs with higher occurrence in March–April than in September–October. The occurrence of post midnight VHF scintillation in this region is unusual and suggests some mechanisms for the formation of scintillation structure that might not be clearly understood. Zonal drift velocities of irregularities were measured using cross-correlation analysis with time series of the VHF scintillation structure from two closely spaced antennas. Statistical analyses of the distribution of zonal drift velocities after sunset hours indicate that the range of the velocities is 30–160 m/s. This is the first analysis of the zonal plasma drift velocity over this region. Based on these results we suggest that the east–west component of the plasma drift velocity may be related to the evolution of plasma bubble irregularities caused by the prereversal enhancement of the eastward electric fields. The equinoctial asymmetry of the drift velocities and scintillation could be attributed to the asymmetry of neutral winds in the thermosphere that drives the eastward electric fields.     

Temperature variability in the tropical mesosphere during the northern hemisphere winter

Temperature observations at 20–90 km height and 5°N–15°N during the period of December 1992–March 1993 from the WINDII and MLS experiments on the UARS satellite are analysed together with MF radar winds and UKMO assimilated fields of temperature and zonal and meridional winds. The correlation between the different datasets at the tropics and zonal mean wind data at mid latitudes is examined for period February–March 1993, when series of stratospheric warming events were observed at middle and high latitudes. Wavelet analysis is applied to investigate coupling between stationary and travelling planetary waves in the stratosphere and the upper mesosphere. Planetary waves m = 1 with periods of 4–7 days, 8–12 days and 13–18 days are found to dominate the period. Westward 7- and 16–18 day waves at the tropics appear enhanced by stationary planetary waves during sudden stratospheric warming events.     

后掠机翼横流驻波及其谐波研究

使用Mack方法求解三维不可压Orr-Sommerfeld方程（忽略曲率影响）,得到模型在风洞最佳实验条件下空间最大放大率展向波长为4mm。以此为基础,选择大于此波长的具有代表性的展向扰动波长6mm与7mm,计算了这两个驻波及其谐波空间的放大率。研究在整个层流区主导流动的扰动波长及其发展趋势。使用丝网印刷的方式,在后掠机翼前缘添加粗糙带,人工引入6mm与7mm驻波,通过升华法验证了计算与理论分析。     

某型飞机短舱辐射换热计算

针对某飞机地面慢车工况,进行了短舱内复合换热数值计算研究,分别运用球谐函数法、离散坐标法和蒙特卡洛法计算辐射换热.结果显示:不同计算方法所得结果总体上趋于一致,热辐射与自然对流耦合作用明显.与单纯自然对流的计算结果相比,舱内温度显著升高,各区域温度值上升7%~30%.考虑空气介质对不同波段热辐射的选择性吸收后,短舱内各计算点温度进一步上升.综合分析表明:地面条件下飞机短舱换热分析过程中热辐射的影响不可忽略.      

液体火箭发动机燃烧室声腔建模方法研究

基于数值模拟技术及有关振动理论,提出了一种建立液体火箭发动机燃烧室声腔模型的方法。为验证方法的可行性,建立了用于带声腔燃烧室全场数值模拟的分区解法,利用这两种方法对同一过程进行的计算表明建模方法是可行的     

The post sunset equatorial F- region zonal drift variability and its linkage with equatorial spread F onset and duration over Indian longitudes

The seasonal and solar activity variation of the post sunset F- region zonal plasma drift, at the magnetic equatorial region over Indian longitudes is analyzed using the Republic of China Satellite-1 data from January 2000 to April 2004. The post sunset F- region zonal drifts are observed to be higher in the years of high solar activity in comparison with low solar activity, while seasonally the drifts are minimum in summer with much higher values in other seasons. The seasonal and solar activity variations of zonal plasma drift are attributed to the corresponding variations in the neutral winds. The dependences of the F region peak vertical drift on the zonal plasma drift at 18.5 IST (Indian Standard Time) and the time difference of the conjugate points sunset times, are quantitatively analyzed. Further an integrated parameter (incorporating the above mentioned two independent factors), which is able to predict the peak vertical drift and growth rate of Rayleigh Taylor instability is proposed. The other major outcome of the study is the successful prediction of the Equatorial Spread F (ESF) onset time and duration using the new integrated parameter at 18.5 IST. ESF irregularities and associated scintillations adversely affect communication and navigation systems. Hence, the present methodology for the prediction of the characteristics of these nocturnal irregularities becomes relevant.     

计及高次谐波影响的高密度永磁同步电机铁耗计算

在经典Bertotti三项式常系数铁耗计算模型的基础上,基于谐波分析原理,引入涡流损耗、磁滞损耗和附加损耗补偿系数,提出了一种计及高次谐波影响的高密度永磁同步电机(PMSM)铁耗计算模型。该模型中的补偿系数均随磁密幅值、频率和畸变率变化,能较好地反映基波及谐波磁场对铁耗的影响。为了验证该模型的有效性及准确性,以48槽/8极内转子和36槽/48极外转子两台PMSM为研究对象,将模型的计算值、有限元仿真结果和试验数据进行对比分析。结果表明,铁耗计算模型有较高的精度,特别适用于磁密幅值与频率变化范围大的场合。