GPS scintillation and TEC depletion near the northern crest of equatorial anomaly over South China

This study presents a statistical analysis of GPS L-band scintillation with data observed from July 2008 to March 2012 at the northern crest of equatorial anomaly stations in Guangzhou and Shenzhen of South China. The variations of the scintillation with local time, season, solar activity and duration of scintillation patches were investigated. The relationship between the scintillation and TEC depletion was also reported. Our results revealed that GPS scintillation occurred from 19:30 LT (pre-midnight) to 03:00 LT (post-midnight). During quiet solar activity years, the scintillation was only observed in pre-midnight hours of equinox months and patches durations were mostly less than 60 min. During high solar activity years, more scintillation occurred in the pre-midnight hours of equinox and winter months; and GPS scintillation started to occur in the post-midnight hours of summer and winter. The duration of scintillation patches extended to 180 min in high solar activity years. Solar activity had a larger effect to strong scintillations (S₄ > 0.6) than to weak scintillations (0.6 ? S₄ > 0.2). Strong scintillations were accompanied by TEC depletion especially in equinox months. We also discussed the relationship between TEC depletion and plasma bubble.     

The detection of “magnetic element” – Why we need a one-meter Space Solar Telescope

The nature of a magnetic element, the elemental structure of the solar magnetic field, is one of the most important mysteries in solar physics. In this paper, we will discuss the requirements of magnetic element detection, such as spatial resolution and magnetic sensitivity. By these discussions, we conclude that it is almost impossible to detect magnetic element with currently used ground-based telescopes and techniques. The proposed Space Solar Telescope, a one-meter Chinese space project, can match these requirements.     

基于连续性条件的体PIV后处理技术

对粒子图像测速技术(PIV,Particle Image Velocimetry)体空间内三维速度场的后处理技术进行研究,引入不可压缩连续性方程的约束对实验测得流场进行修正,使得修正后流场严格满足差分形式的连续性方程.通过流场修正的后处理技术实现拉格朗日乘数法求解全流场修正速度场二范数的极小值.理论推导严格证明了修正后的速度场在数学上更接近满足连续性方程的真实流场.对解析流场引入高斯噪音来进行人工模拟的测试,其结果进一步验证了修正后流场能更趋近于真实流场,对流场中出现的PIV常见的高斯分布噪音有一定的消弱作用.该技术被成功应用于实验数据的后处理,结果表明其能改善测量速度场的平滑度.     

基于简化误差修正的卫星姿态确定算法

针对典型的星敏感器/陀螺姿态卫星确定算法运算复杂这一问题,提出了一种基于简化误差修正的星敏感器/陀螺卫星姿态确定算法.通过对陀螺角速度进行简化修正,减少了滤波器的状态变量,降低滤波器的复杂性.仿真结果表明：该算法在保证姿态确定精度的条件下,能够减少运算量,提高算法的实时性.     

EXPERIMENTAL INVESTIGATION ON THE TURBULENT COHERENT STRUCTURES OF LAMINAR SEPARATION FLOW OVER A BACKWARD FACING STEP

ＥＸＰＥＲＩＭＥＮＴＡＬＩＮＶＥＳＴＩＧＡＴＩＯＮＯＮＴＨＥＴＵＲＢＵＬＥＮＴＣＯＨＥＲＥＮＴＳＴＲＵＣＴＵＲＥＳＯＦＬＡＭＩＮＡＲＳＥＰＡＲＡＴＩＯＮＦＬＯＷＯＶＥＲＡＢＡＣＫＷＡＲＤＦＡＣＩＮＧＳＴＥＰＷａｎｇＪｉｎｊｕｎ；ＬｉａｎＱｉｘｉａｎｇ...     

环境水质远程监测技术研究

在监测现场采用ADAM5510数据采集器,将PH值、溶解氧、温度和浊度等分析测试仪器的数据通过MODBUS现场总线采集并储存,主监控室通过电话线或卫星实现与各个监测现场ADAM5510数据采集器的通讯,完成各个流域不同监测端面的水质数据的记录、曲线显示、查询、报表和打印,同时,主监控室可对某些现场检测设备远程操作。     

复合材料中、长寿命区S-N曲线方程

提出一种新的基于两个假设条件下,用于复合材料层压板中、长寿命区S-N曲线构造的四参数模型。与其它方法相比,此方法不用考虑疲劳机理,只是根据疲劳试验数据,用纯数学方法来确定S-N曲线方程。算例结果表明:本文提出的方法不仅具有良好的拟合效果,而且具有较强的适用范围,因而具有潜在的工程应用价值。     

在三维湍流边界层中摩擦应力的测量研究

本文给出了V形壁面热膜测量物面摩擦应力的方法研究。实验表明该技术对三维湍流边界层中的摩阻测量是一类有效的方法。从本实验的数据可以看到,壁面热膜在二维湍流边界层中得到的校测函数能够直接用于三维湍流边界层的摩擦应力测量。     

复合式气冷涡轮叶片内流动和换热计算

本文给出了复合式气冷涡轮叶片内冷气流量分配、温增加和换热系数迭代求解方法和计算实例 ,还讨论了转动效应对冷气流动和换热和影响。并成功地应用于高性能推进系统气冷叶片的设计 ,同时也可用于气冷涡轮叶片改型和模底分析、验算     

混杂纤维复合材料混杂效应的理论估算与实验

 对碳纤维、玻璃纤维混杂复合材料的层间、层内及夹芯结构试样在拉伸试验中混杂效应的理论估算与实验研究,揭示出了混杂比、分散度对混杂效应的影响规律,建立了估算混杂效应的经验公式,其计算结果与实验结果较为一致。