Experimental investigation of cavitation instabilities in inducer with different tip clearances

To investigate the effect of tip clearance size on cavitation characteristics in a turbopump inducer, a series of experiments have been conducted in a newly developed visualization test facility using room temperature water as working fluid. The pressure fluctuations near the tip region were collected, and the cavity structures under various conditions were documented by a high-speed camera. It is found that large tip clearance distinctly reduces both the non-cavitation and cavitation performance. Three cavitation instabilities, super-synchronous rotating cavitation, synchronous rotating cavitation and cavitation surge have been carefully identified through combination of cross-correlation analysis of pressure signals and visualization results. Large tip clearance displays a remarkable stabilization effect on pressure fluctuation, cavitation surge totally disappears, and the range of occurrence of synchronous rotating cavitation becomes smaller for the large tip clearance, whereas super-synchronous rotating cavitation only occurs in the large tip clearance. The cavitation areas are smaller at large tip clearance, while the flow channels are more seriously choked when cavitation occurs heavily in comparison with those at small tip clearance, which may be responsible for the worse cavitation performance.     

主惯导速度误差短周期波动对子惯导传递对准影响分析

随着激光陀螺技术的发展,旋转调制式激光陀螺惯性导航系统逐渐成为舰载主惯导系统,舰载机、舰载武器系统需要旋转调制式激光惯导系统提供的姿态、速度和位置信息进行对准,即主子惯导的传递对准。由于旋转调制式系统中的姿态、速度和位置具有随旋转的短周期波动问题,势必会影响对准时间较短的子惯导对准精度。为了保证传递对准的快速性,一般采用速度匹配方法。定量分析了主子惯导传递对准过程中主惯导速度误差短周期波动对子惯导系统对准精度的影响,首先进行了数字仿真,之后利用双轴激光陀螺惯导、纯捷联光纤陀螺惯导数据进行了半实物仿真,验证了主惯导速度误差的一次项系数与子惯导初始对准水平姿态误差呈线性关系,二次项系数与子惯导初始对准航向误差呈线性关系。     

某型液压伺服机构系统压力脉动特性分析

对某型伺服机构系统压力脉动量大的原因进行分析,确认为油泵、高压管路、溢流阀之间存在频率特性的耦合现象,激发溢流阀发生谐振.针对频率耦合的特性,提出在高压管路上安装节流块的措施,试验验证表明方案简单有效,系统压力脉动量由改进前的4MPa降低至0.8MPa左右.     

锥形旋流器内燃料分布对模型燃烧室近贫熄状态的影响

针对近贫熄状态,研究锥形旋流器内燃料分布对模型燃烧室燃烧稳定的影响。在不同空气流量下对头部燃料分布A和B分别进行了锥形旋流器模型燃烧室的贫熄状态实验。结果表明:同样的进气条件下,分布B在贫熄时刻的过量空气系数是分布A的4倍以上,并在可比较的实验流量范围内保持明显的优势;分布B的火焰可以由锥形旋流器外缩入锥形旋流器内熄灭,而分布A的火焰不能缩入旋流器内部,只能在锥形旋流器外部以整团火焰的形态熄灭;锥形旋流器头部中心轴线上引入的少量燃料对燃烧室近贫熄状态的压力脉动有极大影响,分布B的压力波动幅值比分布A降低90%以上,压力波动主频从88Hz减小到50Hz。结合数值模拟计算,从切向涡量角度分析了近贫熄火焰前端稳定在不同位置的原因,比较了两种燃气分布下局部流场物理参数分布的差异,有助于理解与认识锥形旋流器内燃料分布对燃烧稳定性的影响。     

压气机转子叶片表面动态压力测量的探索

将一个Kulite动态压力传感器埋入轴流压气机转子叶片50%叶高、25%轴向弦长位置,对该点吸力面动态压力进行了试验测量,并与CFD(计算流体动力学)数值模拟结果进行了对比,为今后进一步测量转子表面静压分布和动态压力脉动积累了丰富的经验.试验中数据采集系统固定在压气机转轴上随其一起旋转,可以对压力信号直接进行采集、放大并存储.结果表明:①叶片表面静压试验测量值与计算结果吻合较好,说明测量结果是可信的;②可以成功地捕捉到转子叶片表面的非定常压力脉动,测量点非定常压力脉动的周期与转子转动周期相同.      

Morphological studies on ionospheric VHF scintillations over an Indian low latitude station during a solar cycle period (2001–2010)

The amplitude scintillations data recorded at 244 MHz from the geostationary satellite, FLEETSAT (73°E) at a low latitude station, Waltair (17.7°N, 83.3°E) during the ten year period of high to low solar activity from 2001 to 2010 is considered to study the occurrence characteristics of the VHF scintillations. A close association between the intense scintillations on VHF signals during pre-midnight hours, associated with range type of spread-F on ionograms and a relatively weak and slow fading scintillations during post-midnight hours associated with frequency type of spread-F is observed during the relatively high sunspot years from 2001 to 2004, whereas during the low sunspot years from 2005 to 2010 the scintillation activity as well as spread-F activity are found to be minimum. During both the high and low sunspot years, it is observed that the maximum scintillation activity occurs during equinoctial months followed by winter with the minimum occurrence during summer months. The annual mean percentage occurrence of scintillations is found to be clearly associated with the variations in the annual mean sunspot number. The nocturnal variations in the occurrence of scintillations show the onset of scintillation activity starts from 19:00 h LT with maximum of occurrence around 21:00 h LT. A clear semiannual variation in the occurrence of scintillations is observed during pre-midnight hours with two peaks in equinoctial months of March/April and September/October. The number of scintillation patches observed is found to be more during pre-midnight hours compared to those during post-midnight hours. The most probable scintillation patch duration lies around 30 min. Further, it is also found that the number of scintillation patches with durations of 60 min and more decreases with the increase in the patch duration. It is also observed in general that the scintillation activity is inhibited during geomagnetic disturbed days.     

用电子束荧光技术研究高超声速边界层中的扰动现象

利用电子束荧光技术对高超声速平板边界层中的扰动现象进行实验研究,实验在炮风洞中进行,自由流马赫数为7．8,单位长度雷诺数为3．5×107/m,测量了平均密度分布、脉动密度分布,并获得了湍流密度脉动的互相关分布和频谱分布。实验结果表明在过渡区中有序与随机现象并存。     

一种用于热流脉动测量的宽频带热电模拟网络

本文简述设计对数模拟网络的方法和预计网络频域和时域特性的理论分析,并给出按其设计制作的频宽为0.04HZ～200kHz 的九节热电模拟网络。与其它设计方法相比,它具有精度高,元件少,成本低,制作简便等优点。     

Fading in the HF ionospheric channel and the role of irregularities

It is well known that the ionosphere affects radio wave propagation especially in the high frequency (HF) range. HF radio waves reflected by the ionosphere can reach considerable distances, often with changes in amplitude, phase, and frequency. The ionosphere is a dispersive in frequency and time, bi-refractive, absorbing medium, in which multipath propagation due to traveling irregularities is very frequent. The traveling irregularities undulate the reflecting ionospheric layer, introducing variations in signal amplitude (fading). In this multipath time variant channel fading is mainly considered, even though it is not the sole effect. Echo signals from a single reflection, as in ionospheric vertical sounding (VIS) techniques, are affected by a certain degree of variability even in quiet ionospheric conditions. In this work the behavior of the ionospheric channel is studied and characterized by observing the power variation of received echoes using the VIS technique. Multipath fading was analyzed quantifying the power variation of the signal echo due to irregularities on a temporal scale from 0.5 to 256 s. An experimental set-up derived from an ionosonde was implemented and the analysis was performed employing a special numerical algorithm operating off-line on the acquired time sequence of the signal. The gain-loss of the irregularity shapes are determined in some special cases.