高旋转数下不同通道转角梯形带肋回转通道的换热特性

为研究截面形状和旋转效应对高压涡轮动叶内部冷却通道换热的影响,对雷诺数为10000～50000,旋转数为0~209,通道转角为0°、225°、45°的带直肋双流程梯形截面通道换热特性进行了实验研究。结果表明:静止状态下,在第一通道,梯形通道后缘换热强于前缘;在第二通道,前、后缘换热区别不大,后缘的换热略强于前缘。旋转状态下,对0°通道转角,随旋转数的增大,第一通道的后缘面换热仍强于前缘面和外侧面,且差异更明显;第二通道前缘换热相对后缘增强。在较高旋转数（旋转数大于1）时,0°通道转角工况的换热最强,45°转角最弱。      

旋转涡轮叶片前缘热色液晶测温技术研究

建立了基于频闪拍照和液晶测温技术的旋转态全环涡轮叶片前缘外壁面温度场测量系统,研究了不同旋转状态下前缘外壁面温度场特性。实验结果表明:该系统能够获取旋转状态下全环涡轮叶片前缘外壁面温度分布,并具有足够的分辨率和精度;随着旋转数的增加,前缘气膜冷却效率整体呈下降趋势,且加剧了压力面和吸力面气膜冷却效率的不均衡。      

介质阻挡放电等离子体的温度测量

在空气介质阻挡放电中,利用氮分子振动谱线和氮分子离子的转动谱线,研究了振动温度和转动温度在两极板间的分布情况。结果表明：越靠近极板振动温度越小,中间振动温度最高;而转动温度在两极板间基本保持不变。     

民用运输类飞机最大可用速率抬前轮试飞技术研究

最大可用速率抬前轮试飞是验证抬前轮速度与起飞安全速度的重要依据,也是难度较大、风险较高的试验项目。以起飞动力学分析为基点,得出最大可用速率抬前轮试飞可能达到的最大迎角,并结合相应的适航审定条款,分析了影响该科目试飞的主要因素,给出了最大可用速率抬前轮试飞技术分析和数据处理方法。     

电机瞬态转速测试

介绍了一种利用单片机和光电转速传感器来测量电机瞬态转速及电机转速变化过程的方法。该方法简单、反应时间快、准确度高。     

锚固站数量及布局对导航星座自主定轨影响分析

针对导航星座自主定轨中的星座整体旋转问题,采用增设少量地面锚固站的方法可有效解决该问题。通过推导星地距离对卫星轨道升交点赤经的偏导数,证明了星地距离对卫星轨道升交点赤经可观。仅考虑在我国大陆范围内布设锚固站的条件下,仿真分析了锚固站数量以及布局对导航星座自主定轨精度的影响。仿真实验结果表明:采用3个以上的锚固站,即可有效控制星座整体旋转,在14d的仿真时段内卫星自主定轨精度保持4m以内;锚固站数量越多,自主定轨精度越高,但随着锚固站数量的增加,自主定轨精度改善程度越来越小;在保持4个锚固站的情形下,采用不同的锚固站布局方案,自主定轨精度并无明显差别。     

Mechanism of error propagation from the subdaily Universal Time model into the celestial pole offsets estimated by VLBI

Within the analysis of space geodetic observations, errors of the applied subdaily Earth rotation model can induce systematic effects in different estimated parameters. In this paper, we focus on the impact of the subdaily Universal Time (UT1) model on the celestial pole offsets (CPO) estimated from very long baseline interferometry (VLBI) observations. We provide a mechanism that describes the error propagation from the subdaily UT1 into the daily CPO.In typical 24-h VLBI sessions the observed quasars are well distributed over the sky. But the observations, if looked at from the Earth-fixed frame, are not homogeneously distributed. The amount of observations performed in different terrestrial directions shows an irregularity which can be roughly compared to the case where the observations are collected in only one Earth-fixed direction. This peculiarity leads to artefacts in VLBI solutions, producing a correlation between the subdaily variations in UT1 and the position of the celestial pole. As a result errors in diurnal terms of the subdaily UT1 model are partly compensated by the estimated CPO. We compute for each 24-h VLBI session from 1990 until 2011 the theoretical response of the CPO to an error in the subdaily UT1 by setting up a least-squares adjustment model and using as input the coordinates of the observed quasars and observation epochs. Then real observed response of the estimated CPO derived from the VLBI session solutions is compared to the predicted one. A very good agreement between the CPO values estimated from VLBI and the predicted values was achieved. The presented model of error propagation from the subdaily UT1 into the daily CPO allows to predict and explain the behaviour of CPO estimates of VLBI solutions computed with different subdaily Earth rotation models, what can be helpful for testing the accuracy of different subdaily tidal models.     

VHF/UHF振幅闪烁和VHF快速法拉弟旋转起伏

本文利用1988年9月至1989年5月在武昌(114.4°E,30.6°N)同时接收日本ETS-Ⅱ卫星(130.0°E)发出的VHF(136MHz)信标信号和苏联静止站-T卫星(99.0°E)发出的UHP(714MHz)广播电视信号时获得的观测记录,对夜间出现的双频(VHF/UHF)闪烁和VHF快速(每分钟大于5次的起伏)法拉弟旋转起伏(以下用FRF表示法拉弟旋转起伏)进行了统计分析,结果发现在临近太阳黑子最大年份观测到的双频夜间闪烁主要为急始型,呈赤道特性,且在临近二分点的月份里有最大出现率,秋季更为明显;伴随VHF振幅闪烁出现的快速FRF常与UHF振幅闪烁共存,以及产生这种现象的不规则体由西向东漂移,东-西向的漂移速度分量,在子夜前为140m/s,在子夜后为90m/s。      

涡轮泵转子工作转速的模糊可靠性确定方法及其应用

针对涡轮泵转子共振失效的特点,分析了转子工作状态超界的隶属函数,详细讨论了隶属函数中有关参数的确定方法,建立了转子工作转速模糊可靠性计算模型,推导出工作转速的计算公式,并与常规的工作转速确定法进行了比较。