基于数值定容弹方法的推力室阻尼特性研究

为确定推力室的声学振型频率及其阻尼特性，给出推力室最容易激发声学振型和最难衰减声学振型，建立了基于数值定容弹和半带宽法的推力室声学振型及其阻尼特性的数值模拟方法。对小推力姿轨控发动机推力室进行近圆周壁面的定容弹激励仿真，激发出了多模态的声学振型，其中，一阶切向振型为最容易激发振型，而一阶纵向振型为最难衰减振型。进一步讨论了推力室构型参数对其阻尼特性的影响，结果表明：随推力室内径增大，纵向振型得到抑制，而切向振型变得不易衰减；随推力室收缩比增加，一阶切向振型半带宽先增大后保持不变；随推力室圆柱段长度增加，各振型半带宽没有明显的变化趋势。     

等压差条件下多斜孔综合冷效实验研究

为了研究不同进气条件对多斜孔气膜冷却的影响规律,采用实验方法,从等压差和等冷气量两个角度分别探讨了孔径d为0.5mm～1mm,开孔率op为0.0245～0.0383,流向倾角α为20°～45°的变化对综合冷效的影响规律。实验结果表明:综合冷效沿流向方向逐渐增大。开孔率和流向倾角不变时,孔径减小,在等单位面积冷气量下,综合冷效显著增加;在等压差条件下,孔径越小,单位面积冷气量越小,综合冷效仍然随之增加。孔径和流向倾角不变,两种进气条件下,综合冷效随开孔率的增加而增加,但等压差条件下增大幅度更高。孔径和开孔率不变,在等冷气量条件下,20°流向倾角综合冷效最高;在等压差条件下,30°流向倾角综合冷效最高。     

Ionospheric perturbations due to earthquakes as determined from VLF and GPS-TEC data analysis at Agra,India

Employing SoftPAL receiver, amplitude variations of VLF transmitter signals NWC (19.8?kHz) and NPM (21.4?kHz) are analyzed at Agra station in India (Geograph. lat. 27.2°N, long. 78°E) ±15?days from five major earthquakes of magnitude M?=?6.9–8.5 occurred in Indian subcontinent during the years 2011–2013. We apply nighttime fluctuation (NF) method and show that in almost all cases the trend decreases and dispersion and NF increase on the same days corresponding to each earthquake about 11–15?days prior to the main shock. Assuming that the ionospheric perturbations are caused by atmospheric gravity waves (AGW), we also calculate AGW modulation index for each case and find its values increased on the days amplitude fluctuations take place. Its value is decreased in one case only where the perturbations may be attributed to penetration of seismogenic electric field.In order to support the above results we also present GPS-TEC data analyzed by us corresponding to three of the above earthquakes. We study the TEC anomalies (unusual enhancements) and find that in one case the precursory period is almost the same as that found in NF method.     

On the stabilizing effect of Solar Radiation Pressure in the Earth-Moon system

Solar sails change the natural dynamics of systems: Trajectories that are driven by gravitational forces can be displaced and changed because of the effect of Solar Radiation Pressure (SRP). Moreover, if the lightness number of the sail is large enough, the instability of certain orbits can be diminished and even removed. In this paper we modify two models for the motion of a probe in the Earth-Moon system that include the effect of Sun’s gravity to take also into account the effect of SRP. These models, the Bicircular Problem (BCP) and the Quasi-Bicircular Problem (QBCP), are periodic perturbations of the Earth-Moon Restricted Three Body Problem (RTBP). The models are modified to consider the effect of the SRP upon a solar sail. We provide examples of periodic orbits that are stabilized (or made less unstable) due to the effect of SRP.     

基于自适应修正曼哈顿距离的室内定位方法

在室内WiFi环境下,针对常见指纹匹配算法所忽略的信号波动问题,提出了一种基于自适应修正曼哈顿距离和AP选择的指纹匹配算法,并结合加权K近邻方法实现定位。首先采用AP选择算法获取部分受干扰程度小和出现频率高的AP,在指纹匹配时仅使用该部分AP的接收信号强度进行计算;在分析WiFi信号传播衰减公式和信号波动的基础上,提出了将自适应修正曼哈顿距离作为指纹匹配的度量距离,使用该距离旨在平滑信号波动对指纹相似度计算的影响;最后采用加权K近邻方法估计测试点的坐标。实验结果表明,在加权K近邻方法的框架下,基于自适应修正曼哈顿距离的定位算法在定位精度上优于基于欧氏距离、曼哈顿距离、余弦距离和Sorensen距离的定位算法。     

叶片前缘旋流和常规冲击对比数值研究

为了寻求更好的叶片前缘内冷结构,对旋流冲击和常规冲击的流动和传热特性进行了数值模拟,对比研究了二者的涡流结构、传热强度、流动阻力、综合传热性能和热均匀性,研究了通道Re数和冲击间距对这些参数的影响。结果表明旋流冲击形成的旋涡有利于传热的增强和热均匀性的提高。在所研究的Re数（2×104~7.78×104）和冲击间距（3.3~5倍直径）范围内,旋流冲击与常规冲击相比平均传热增强18%~34%,增幅随Re数和冲击间距的增大而增大;流阻增大10%~26%,增幅随Re数和冲击间距的增大而减小;综合传热性能增强20%左右;热均匀性提高60%左右。     

轴流压气机转子叶片表面静压分布实验

在低速轴流压气机转子叶片吸力面50%叶高沿轴向埋入5个Kulite动态压力传感器,并采用固定在压气机转轴上一种新型可存储的数据采集器记录数据,对近设计点和2 kr/min转速不同流量工况条件下转子叶片表面静压进行了实验测量,并与CFD数值模拟结果进行了对比。结果表明,除近失速点外,叶片表面静压实验测量值与计算结果吻合较好,说明所采用的的测量方法是成功的,测量结果是可靠的;在近失速工况,实验值与计算结果差值较大,主要是由试验台振动所引起的实验误差和CFD数值计算对近失速点工况流场模拟得不够准确所导致的。     

涡轮级内非定常流场的数值研究

对涡轮级内非定常流动进行了数值研究,探讨了转子和静子叶片之间的非定常相干的机理。结果表明,高频振动对整个流场的非定常性没有太大的影响,1倍频处的波动幅度占据主导地位,可用正弦函数近似表示叶片上力随时间脉动,时均效应和1倍频效应的影响是统一的。静叶尾迹中波动最强烈的区域正好撞击到动叶通道中央,非定常脉动影响主要出现在前缘附近。     

Design of an FPGA-based electronic flow regulator (EFR) for spacecraft propulsion system

This paper describes a scheme for electronically regulating the flow of propellant to the thruster from a high-pressure storage tank used in spacecraft application. Precise flow delivery of propellant to thrusters ensures propulsion system operation at best efficiency by maximizing the propellant and power utilization for the mission. The proposed field programmable gate array (FPGA) based electronic flow regulator (EFR) is used to ensure precise flow of propellant to the thrusters from a high-pressure storage tank used in spacecraft application. This paper presents hardware and software design of electronic flow regulator and implementation of the regulation logic onto an FPGA.