Ionospheric scintillations at Guilin detected by GPS ground-based and radio occultation observations

The occurrence of ionospheric scintillations with S4 ? 0.2 was studied using GPS measurements at Guilin, China (25.29°N, 110.33°E; geomagnetic: 15.04°N, 181.98°E), a station located near the northern crest of the equatorial anomaly. The results are presented for data collected from January 2009 to March 2010. The results show that nighttime amplitude scintillations only took place in February and March of the considered years, while daytime amplitude scintillations occurred in August and December of 2009. Nighttime amplitude scintillations, observed in the south of Guilin, always occurred with phase scintillations, TEC (Total Electron Content) depletions, and ROT (Rate Of change of TEC) fluctuations. However, TEC depletions and ROT fluctuations were weak during daytime amplitude scintillations, and daytime amplitude scintillations always took place simultaneously for most of the GPS satellites which appeared over Guilin in different azimuth directions. Ground-based GPS scintillation/TEC observations recorded at Guilin and signal-to-noise-ratio (SNR) measurements obtained from GPS-COSMIC radio occultation indicate that nighttime and daytime scintillations are very likely caused by ionospheric F region irregularities and sporadic E, respectively. Moreover, strong daytime amplitude scintillations may be associated with the plasma density enhancements in ionospheric E region caused by the Perseid and Geminid meteor shower activities.     

The geomagnetic solar flare effect identified by SIIG as an indicator of a solar flare observed by GOES satellites

This paper studies the efficiency of geomagnetic solar flare effects (gsfe) in X solar flare detection; so during the period 1999–2007 a comparison between solar flare (sf) observed by satellites of the Geostationary Operational Environmental Satellite (GOES) programme and gsfe published by the Service International des Indices Geomagnetiques (SIIG) is made.     

一类隔离驱动电路的“剩余驱动”问题

讨论直流变换器中将脉宽调制器（PWM）输出与受控MOS管栅极连接的一类开关驱动电路.专注于分析它在PWM电路关闭后对栅极产生的驱动信号,被命名为＂剩余驱动＂.描述这类剩余驱动的电气特性,说明它对变换器造成的危险,提出改进这类驱动电路以消除这些危险的4种方法.     

GPS姿态测量的载波相位整周模糊度快速解算

 根据 ARCE方法可以将模糊度搜索空间从所观测到的 m颗卫星的 m -1维降为 3维独立整周模糊度搜索空间,结合整数高斯变换及基线长度约束减小模糊度搜索空间,利用 Cholesky分解提高模糊度搜索效率,实验结果证明该方法能够快速解算整周模糊度适于实时姿态确定等应用。     

一种消除GPS模糊度相关性的新算法

 通过分析几种典型的整周模糊度去相关处理的方法 ,提出了一种简单快速消除GPS模糊度相关性的算法 ,介绍了算法中排序、整数LDLT 分解和模糊度筛选的处理过程 ,比较了该算法与其它算法性能上的差异 ,最后通过计算说明该算法的高效、可靠。     

基于Euler／N—S方程的跨音速非线性静气动弹性问题研究

在C-H网格的基础上,采用Jameson的中心差分有限体积法求解Euler/N-S方程,采用结构影响系数法计算结构的弹性变形,用三角元面积加权法和常体积转换法(CVT)实现流固耦合,计算了弹性后掠机翼在跨音速状态的静气动弹性问题     

基于离散曲率计算的三角网格模型优化调整

采用面积夹角加权的三角网格模型顶点法矢及三角片质心权值对Taubin的三角网格模型离散曲率计算方法进行了改进,在此基础上提出了一种新的三角网格模型优化调整方法。用该方法调整三角网格模型,在模型上曲率变化较平缓的平坦区域及曲率变化较剧烈的特征区域都能取得较好的调整效果。     

C/SiC-W复合材料的制备与表征

采用化学气相渗透(CVI)结合溶液浸渍法制备C/SiC-W多元基复合材料,利用XRD和SEM对材料的物相组成及微观结构进行表征,并对制备过程的反应机理进行初步探讨.结果表明,W在复合材料中成颗粒团聚状,它不仅能渗入到复合材料的纤维束间,还渗入到纤维束内.制得C/SiC-W复合材料的密度为4.1g/cm3,开气孔率为12%.     

The Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First Results

The Grain Impact Analyser and Dust Accumulator (GIADA) onboard the ROSETTA mission to comet 67P/Churyumov–Gerasimenko is devoted to study the cometary dust environment. Thanks to the rendezvous configuration of the mission, GIADA will be plunged in the dust environment of the coma and will be able to explore dust flux evolution and grain dynamic properties with position and time. This will represent a unique opportunity to perform measurements on key parameters that no ground-based observation or fly-by mission is able to obtain and that no tail or coma model elaborated so far has been able to properly simulate. The coma and nucleus properties shall be, then, clarified with consequent improvement of models describing inner and outer coma evolution, but also of models about nucleus emission during different phases of its evolution. GIADA shall be capable to measure mass/size of single particles larger than about 15 μm together with momentum in the range 6.5 × 10⁻¹⁰ ÷ 4.0 × 10⁻⁴ kg m s⁻¹ for velocities up to about 300 m s⁻¹. For micron/submicron particles the cumulative mass shall be detected with sensitivity 10⁻¹⁰ g. These performances are suitable to provide a statistically relevant set of data about dust physical and dynamic properties in the dust environment expected for the target comet 67P/Churyumov–Gerasimenko. Pre-flight measurements and post-launch checkouts demonstrate that GIADA is behaving as expected according to the design specifications. The International GIADA Consortium (I, E, UK, F, D, USA).     

基于两相法的机翼结构几何优化设计

针对机翼结构的几何优化问题,提出了一种基于两相法的几何优化设计新方法。采用参数化命令流文件进行有限元建模,利用复合形法进行位置优化,利用MSC/NASTRAN进行尺寸优化,并将尺寸优化结果传递给复合形法作为复合形法进行操作的依据。算例表明,本文所提方法可行,所得结果可信度高。