碟式飞行器复合控制的共栖现象研究

借用生物学概念,首次提出了复合控制的共栖现象概念,并对碟式飞行器复合控制中产生的两类共栖现象进行了仿真研究,比较了复合控制中共栖现象与生物共栖现象的相似点,指出了共栖现象的研究意义和应用前景。     

定常流场中二维激波反射迟滞现象研究进展

为深入理解超声速飞行器和动力系统流场中存在的激波反射迟滞现象,对近年来有关定常激波反射迟滞文献资料进行了调研和总结。回顾了定常激波反射迟滞现象的提出与证实过程,介绍了改变入射激波形状、改变下游波系结构等可引起激波反射出现迟滞的实现方式,并对粘性效应、三维效应和动态效应等影响激波反射迟滞现象的因素进行了探讨,对激波反射迟滞现象的研究热点和难点问题进行了分析与总结。     

变结构控制系统中的混沌现象

应用相轨迹、功率谱等方法,证实了一类变结构控制系统中存在混沌现象,分析了产生混沌现象的原因并给出不同条件下的混沌图形。     

某型飞机脚蹬反弹故障原因分析

某型飞机在外场飞行、滑跑、供压、试车过程中,脚蹬多次出现撞击式反弹现象,通过对故障现象的模拟、确认、故障定位,深入分析了该故障的原因,为类似故障的查找和分析提供了参考。     

进气道内激波/边界层干扰及控制研究进展

进气道作为高速航空航天飞行器的重要气动部件,对飞行器的气动力特性、结构重量、隐身性能等有显著影响。激波/边界层干扰现象是高速进气道内普遍存在的一类流动现象,对进气道的性能有突出的影响。发生于进气道内的激波/边界层干扰现象主要可分为正激波/边界层干扰、斜激波/边界层干扰以及三维激波/边界层干扰几类,由于受到侧壁壁面和进气道内背景波系的影响,这些干扰现象偏离了传统基于简化模型的研究结果,具有显著的耦合干扰特征,干扰区间内三维特征明显。概述了发生于进气道内的激波/边界层干扰特性及相关研究进展,并对目前进气道内激波/边界层干扰现象的控制方法进行了总结。     

空间发动机系统关机过程水击现象理论分析

对空间发动机系统关机过程进行了数值仿真分析,讨论了关机过程中系统管路内的水击现象,以及多推力室发动机系统工作状态、阀门响应特性等因素对水击现象的影响。     

碟式飞行器复合控制的共栖现象

借用生物学概念,首次提出了复合控制的共栖现象概念,并对碟式飞行器复合控制中产生的两类共栖现象进行了仿真研究,比较了与生物共栖的相似点,指出了共栖现象的研究意义和应用前景。     

某型飞机液压油箱漏油故障分析

某型飞机液压油箱在外场使用中出现油液渗漏现象,通过对故障现象确认、机理分析、故障验证,找到了故障根源,提出改进措施,在实际应用中具有借鉴和指导意义。     

挤压油膜阻尼器结构参数对气穴现象影响的实验研究

在实验的基础上, 研究了挤压油膜阻尼器的结构参数诸如偏心率、油膜的径向间隙比和承载长度等对气穴现象的影响。上述结构参数保持不变时, 借助高速摄影机观察了不同转速工况的气穴现象, 归纳出两种不同成份组成的气穴。同时, 还测试和分析了气穴现象对挤压油膜压力分布的影响。以上结果对建立新挤压油膜阻尼器理论模型具有重要参考和利用价值。      

应用分支和突变理论对飞机空间机动稳定性的研究

 本文应用分支和突变理论,研究了飞机空间机动全局稳定性,导出了求解滚转速率临界稳定值的解析公式,分析了非线性跳跃现象和周期性振荡现象,并找出了这两种现象产生的原因。     

Doppler scintillation measurements of the heliospheric current sheet and coronal streamers close to the Sun

Prominent enhancements in Doppler scintillation lasting a fraction of a day (solar source several degrees wide) and overlying the neutral line represent the signature of the heliospheric current sheet and the apparent interplanetary manifestation of coronal streamers near the Sun. This first detection of coronal streamers in radio scintillation measurements provides the link betweenin situ measurements of the spatial wavenumber spectrum of electron density fluctuations beyond 0.3 AU and earlier measurements deduced from radio scintillation and scattering observations inside 0.3 AU. Significant differences between the density spectra of fast streams and slow solar wind associated with the heliospheric current sheet near the Sun reinforce the emerging picture that high- and low-speed flows are organized by the large-scale solar magnetic field, and that while the contrast between solar wind properties of the two flows is highest near the Sun, it undergoes substantial erosion in the ecliptic plane as the solar wind expands.     

Effects of two-way decorrelation on radar detection inscintillation

A 3 dB gain in average signal-to-noise ratio of a monostatic radar operating in scintillation has recently been established both theoretically and observationally. The statistics of two-way scintillation are derived here for the case where the uplink and downlink both experience Rayleigh fading and where there is arbitrary correlation between the scintillation on the two paths. These statistics are then used to compute radar detection curves. A surprising result is obtained. The probability of detection is only weakly dependent (for P _D in the range 0.1 to 0.9) on the degree of uplink-downlink correlation in the scintillation when the average (nonfading) signal-to-noise ratio is constant and when proper account is taken of the change in mean power between the monostatic and bistatic cases. Much larger differences are seen in the detection curves with scintillation compared with nonfading curves (for P_D equal to 0.7 this scintillation loss is about 7 dB). Thus the difference in detection performance of monostatic and bistatic radars is determined primarily by the difference in the radar cross section (RCS) of the target for the two cases     

The Impact of Strong Scintillation on Space Based Radar Design I: Coherent Detection

Electromagnetic signals which propagate through strongly disturbed regions of the ionosphere can experience angular scattering, causing appreciable amplitude and phase scintillation and angle-of-arrival fluctuations. The performance of a space based radar (SBR) subject to degradation due to signal propagation through a highly disturbed ionospheric channel is considered here. Pertinent characteristics of the disturbed channel and the received radar signal are described. The effects of the propagation path are investigated and the differences between monostatic and bistatic operation are presented. Results are presented which show the effect of severe scintillation on the coherent target detection performance of an SBR. It is shown that coherent detection performance can be seriously degraded in a scintillation environment if scintillation effects are not considered in the radar design.     

Interplanetary scintillation of radio sources during August 1972

The observations of interplanetary scintillation of radio sources in early August 1972 are reviewed. Three-site measurements of solar wind speed were made at University of California, San Diego (73.8 MHz) and at Nagoya University, Toyokawa (69.3 MHz). Single-site measurements of scintillation index were made at Mullard Radio Astronomy Observatory, Cambridge (81.5 MHz) and at University of Adelaide (111.5 MHz). The enhancements in solar wind speed and scintillation index associated with three shock waves were detected. The extent in both longitude and latitude of the shock wave associated with the solar flare on 7 August, the anisotropic expansion of shock waves and the detection of the corotating high-speed streams are main results deduced from the observations.     

‘Good’ events selection efficiency of the scintillation time-of-flight system of the Gamma-1 telescope in the 30–300 MeV energy range

The scintillation time-of-flight triggering system of the Gamma-1 gamma-ray telescope provides for both the time-of-flight discrimination and the pulse height discrimination of the secondary particles. The paper gives some experimental results for energy dependence of the instrument efficiency in 30–300 MeV energy range for different trigger logics.     

Angular Accuracy of the Binary Moving Window Radar Detector

The angular accuracy of a search radar depends on the extraction technique. For the case of a binary moving window extractor, the accuracy is evaluated in different operational conditions including target scintillation. A beam-splitting technique that was devised to improve the accuracy is also evaluated and compared with the binary moving window.     

Deducing turbulence parameters from transionospheric scintillation measurements

The theoretical framework and experimental methodology used to interpret observations of ionospheric scintillations in terms of geophysical processes are reviewed and recent experimental observations of ionospheric scintillations are discussed in this paper. During the past 15 years significant progress has been made in several areas. In particular, significant advances have been made in theoretical understanding of the strong scintillation regime and the effects of short-term temporal variations of the scintillation producing irregularities on observations made with spaced-receiver geometries in both weak and strong scintillations. This improved understanding of the scintillation process has significantly increased the utility of the technique particularly in the equatorial latitudes where geometrical effects are least important.     

The Impact of Strong Scintillation on Space Based Radar Design II: Noncoherent Detection

Electromagnetic signals that propagate through strongly disturbed regions of the ionosphere can experience scattering which can cause significant amplitude, phase, and angle-of-arrival fluctuations. This paper considers the performance of a space based radar (SBR) that must operate through a highly disturbed propagation environment such as might occur during a barium release or after a high altitude nuclear detonation. A brief summary of the propagation channel characteristics is given in terms of quantities that are important to SBR design issues. Results are then given showing the effect of noncoherent integration on target detection performance. Both coherent and noncoherent detection performance can be seriously degraded by scintillation if scintillation is not adequately considered in the radar design.     

大气湍流对APD直接检测接收机抗噪声性能影响

针对以往分析湍流信道对系统抗噪声性能影响的不足,给出了一种基于APD直接检测接收机的湍流噪声的处理方法.在APD直接检测接收机模型的基础上,推导了其信噪比和曼彻斯特编码系统的差错概率,并详细分析了湍流对接收机的抗噪声性能影响.结果表明,增大接收天线孔径可以减弱湍流的影响,但在天线孔径较小时,增加发射功率并不能有效地提高...     

Interplanetary scintillation

The use of interplanetary scintillations for probing otherwise inaccessible regions of the solar wind is reviewed. A comparison with space-craft observations in the ecliptic is used as a calibration for the scintillation observations. Recent observations at high latitudes and near the Sun are discussed from this viewpoint. A new analysis which uses both scintillation and angular scattering observations to estimate the electron density spectrum is introduced. The spectrum appears to have a high frequency cutoff which varies slowly with solar distances and may also have a relatively flat region just below the cutoff frequency.