阳极层霍尔推力器内轮辐效应不稳定性研究

为研究圆柱形阳极层霍尔推力器内轮辐效应的不稳定性,利用高速相机和静电探针得到1-2-1模式、1-2-3-1模式和1-2-3-2-1模式的轮辐分裂与合并现象。随着磁感应强度由205Gs增加到225Gs,轮辐个数m由1增加到3。轮辐的分裂与合并模式增多,且轮辐的旋转频率随之由25kHz提高到40kHz～50kHz。轮辐效应的存在是电子密度分布函数的宏观体现,动理论方程中力F的波动引起了轮辐的分裂,随着轮辐个数m的增加,电子分布的低频大幅度波动逐渐演变为小幅度高频率的波动。电子密度分布函数的波动引起的轮辐效应产生了角向分布的电场强度与磁场共同作用,增强了电子轴向漂移运动。     

Effect of the seed perturbation amplitude on the equatorial spread F initiation during solar minimum

The contribution of gravity wave (GW) to the initiation/development of spread F during a solar minimum year was investigated through the comparison of the observed precursory parameters and characteristics of the corresponding equatorial spread F (ESF) events. The ionospheric parameters were recorded at the magnetic equatorial station Sao Luis (2.3°S, 44°W, dip latitude 2°S) during March and October 2010. These data were used to estimate the influence of the relative gravity wave amplitude and the ambient ionospheric condition on the diurnal variation of the spread F initiation. The vertical velocity drift indicated a clear control and defines the threshold for the seasonal variability of the ESF occurrence. However, it was insufficient to solely determine or predict the day to day variation of ESF occurrence. Thus, few days with contrasting ambient ionospheric condition and magnitude of GW amplitude were analysed in order to investigate the role of the different precursory factors in the observed diurnal variation of the plasma irregularity development. The density scale length and gravity wave amplitude were shown to immensely contribute to the linear instability growth rate, especially during the days with a low post-sunset rise. Thus, the experimental observations have demonstrated the strong inter-dependence between the precursory factors and they have also highlighted the probable control of the ESF morphology.     

喷嘴式隔板与纵向肋式隔板阻尼效应分析

利用声学模型和单喷嘴声学模拟试验研究了喷嘴式隔板的耗散机理;用数值方法分析了纵向肋式隔板周围的涡流;用声学理论研究了纵向肋式隔板的声场。研究结果表明:选取合适的管间隙将会使喷嘴式隔板具有更好的稳定性作用;肋片周围是涡流产生的主要区域;肋高对燃烧室声学特性的影响远大于肋长。     

Low-cost precise measurement of oscillator frequency instability based on GNSS carrier observation

Global navigation satellite systems (GNSS) receivers can be used in time and frequency metrology by exploiting stable GNSS time scales. This paper proposes a low-cost method for precise measurement of oscillator frequency instability using a single-frequency software GNSS receiver. The only required hardware is a common radio frequency (RF) data collection device driven by the oscillator under test (OUT). The receiver solves the oscillator frequency error in high time resolution using the carrier Doppler observation and the broadcast ephemeris from one of the available satellites employing the onboard reference atomic frequency standard that is more stable than the OUT. Considering the non-stable and non-Gaussian properties of the frequency error measurement, an unbiased finite impulse response (FIR) filter is employed to obtain robust estimation and filter out measurement noise. The effects of different filter orders and convolution lengths are further discussed. The frequency error of an oven controlled oscillator (OCXO) is measured using live Beidou-2/Compass signals. The results are compared with the synchronous measurement using a specialized phase comparator with the standard coordinated universal time (UTC) signal from the master clock H226 in the national time service center (NTSC) of China as its reference. The Allan deviation (ADEV) estimates using the two methods have a 99.9% correlation coefficient and a 0.6% mean relative difference over 1–1000 s intervals. The experiment demonstrates the effectiveness and high precision of the software receiver method.     

Self-similar flow of a rotating dusty gas behind the shock wave with increasing energy, conduction and radiation heat flux

A self-similar solution is obtained for one dimensional adiabatic flow behind a cylindrical shock wave propagating in a rotating dusty gas in presence of heat conduction and radiation heat flux with increasing energy. The dusty gas is assumed to be a mixture of non-ideal (or perfect) gas and small solid particles, in which solid particles are continuously distributed. It is assumed that the equilibrium flow-condition is maintained and variable energy input is continuously supplied by the piston (or inner expanding surface). The heat conduction is expressed in terms of Fourier’s law and the radiation is considered to be of the diffusion type for an optically thick grey gas model. The thermal conductivity K and the absorption coefficient α_R are assumed to vary with temperature only. In order to obtain the similarity solutions the initial density of the ambient medium is assumed to be constant and the angular velocity of the ambient medium is assumed to be decreasing as the distance from the axis increases. The effects of the variation of the heat transfer parameters and non-idealness of the gas in the mixture are investigated. The effects of an increase in (i) the mass concentration of solid particles in the mixture and (ii) the ratio of the density of solid particles to the initial density of the gas on the flow variables are also investigated.     

基于流动显示的翼尖涡不稳定频率测量

翼尖涡涡核振荡频率的准确测量是翼尖涡控制技术得以有效实施的重要前提。采用流动显示方法,研究了椭圆机翼翼尖涡在低雷诺数条件下的不稳定特性。分别采用单点谱分析和动力学模态分解技术,从流动显示图像序列中提取了涡核振荡的短波不稳定模态的频率,2种方法得到的频率相对误差最大不超过5%。研究结果表明:涡对的空间运动通常展现出长波与短波模态的耦合,涡核的高频短波振荡耦合在低频长波摆动中,以前者为主要含能模态;短波不稳定性的无量纲振荡频率随雷诺数的增大而增大、随机翼攻角的增大而减小。      

窄条翼导弹俯仰机动中滚转失稳及其控制过程

窄条翼布局导弹通常具有复杂的横向气动特性,在大迎角飞行及快速机动中很容易诱发出现滚转非指令偏离和连续振荡,可能导致飞行失控,影响落点精度。为了研究窄条翼导弹俯仰快速机动对滚转失稳的诱发过程及滚转失稳对俯仰机动控制效果的影响,并验证三通道解耦控制方法的有效性,针对典型俯仰机动过程,分别利用2.4 m跨声速风洞虚拟飞行试验平台和耦合气动/运动/控制的一体化数值计算方法开展了相关研究。结果表明,风洞试验和数值模拟均成功预测了俯仰拉起和保持过程中的滚转自激失稳运动及其引起的纵、横向耦合运动,针对该机动过程,三通道解耦控制方法能够有效抑制滚转运动,保持姿态稳定。     

液体火箭发动机诱导轮旋转汽蚀分析

超同步旋转汽蚀和次同步旋转汽蚀是液体火箭发动机诱导轮旋转汽蚀现象的两种类型。为了揭示它们之间的差异,完成了Tsujimoto旋转汽蚀计算模型的理论求解,开展了旋转汽蚀现象的数值计算。结果表明,旋转汽蚀两种类型发生时,质量流量增益系数M都发生周期性变化。当超同步旋转汽蚀发生时,M>0;而当次同步旋转汽蚀发生时,M值的变化范围更广。由于在设计工况点附近,通常有M>0,因此在多数情况下很难观测到次同步旋转汽蚀。     

基于升华法实验研究后掠翼三维边界层的转捩

在西北工业大学的低湍流度风洞,采用升华法研究不同雷诺数下后掠翼上表面的转捩现象。实验发现雷诺数较低时,后掠翼上的转捩由流向不稳定触发,转捩位置在最小压力点之后,转捩分界为一条直线;当雷诺数足够大时,转捩由横流驻波不稳定触发,转捩提前到最小压力点之前,转捩分界呈现尖楔形状。该结果表明升华法不但能够较准确地分辨出后掠翼上的转捩位置,还能够区分不同的转捩机理,判断转捩是由流向不稳定还是横流驻波不稳定触发。此外,实验中还发现在横流驻波不稳定增长较大时,升华法能够提供转捩上游区域边界层内的横流不稳定信息;当横流驻波不稳定进一步增强时,该不稳定受模型表面粗糙度的影响较大,萘的喷涂有可能会影响到升华法的结果。     

氢喷射温度对氢氧火箭发动机燃烧稳定性的影响

应用CFD方法对氢氧火箭发动机中高频燃烧不稳定性进行了数值模拟,研究分析了不同工况条件下氢喷射温度对燃烧振荡的影响规律,得出了压力振荡频率变化规律及稳定性极限图。结果表明：在一定的氢喷射温度范围内会发生不稳定燃烧,且随着混合比的增大,发生不稳定燃烧的氢喷射温度上限增大;不稳定燃烧振荡主频呈倍频关系,且在氢喷射温度（70K～110K）内,振荡主频最大。