昆明上空电离层D区电子密度季节变化的首次观测分析

通过分析2008年8月至2009年7月昆明站(25.6°N, 103.8°E) 中频(MF)雷达观测数据, 研究了太阳活动低年电离层D区电子密度的季节变化特性,发现D区电子密度主要呈现半年变化特征, 即在春秋季电子密度较大, 而在夏冬季则较小, 这与国际参考电离层(IRI)预测的年变化趋势不一致, 但与昆明站电离层测高仪的最低回波频率f_min的观测结果相符. 同时比较了D区电子密度半年变化与纬向风半年变化的关系, 发现二者之间保持了非常一致的变化趋势并对这种一致性的内在原因进行了分析.     

Dark Matter Particle Explorer:The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

The Dark Matter Particle Explorer (DAMPE) mission is one of the five scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Science (CAS) approved in 2011. The main scientific objective of DAMPE is to detect electrons and photons in the range of 5GeV-10TeV with unprecedented energy resolution (1.5% at 100GeV) in order to identify possible Dark Matter (DM) signatures. It will also measure the flux of nuclei up to above 500TeV with excellent energy resolution (40% at 800GeV), which will bring new insights to the origin and propagation high energy cosmic rays. With its excellent photon detection capability, the DAMPE mission is well placed for new discoveries in high energy-ray astronomy as well.      

A-100钢电子束熔丝成形件超声相控阵检测应用初探

初步研究了超声相控阵检测技术在A-100钢电子束熔丝成形制件中的应用.结果表明:超声相控阵检测技术在A-100钢电子束熔丝成形制件微裂纹检测和大厚度制件检测中有较好的应用效果;与成形路径等因素相关的微观组织结构对检测技术的应用有较大影响;超声波入射方向和角度选择对微裂纹的识别非常关键;制件内部微裂纹存在与平行于逐层生长方向的某端面呈现小倾角或近似平行的断续拐弯状的分布趋势.     

TA15钛合金电子束焊平行焊缝形貌及显微组织研究

对TA15钛合金厚板电子束焊接均匀焊缝即熔合线近似平行的焊缝的电子束焊接工艺进行了研究,获得了一系列均匀焊缝的焊接工艺方法。选用加速电压为140kV、焊接速度600mm/min,聚焦电流318mA和338mA,电子束流43mA和50mA的工艺条件获得了2种形状的焊缝。研究结果表明,电流越大,焊缝显微组织越粗大,热影响区越宽,接头显微硬度曲线也越平滑。     

TC4-DT合金电子束焊接接头低周疲劳性能研究

通过对TC4-DT钛合金母材、电子束焊接接头显微组织的分析及焊接接头不同位置疲劳性能的测试,研究了焊接接头显微组织特点,比较了母材与焊接接头不同位置处的低周疲劳性能,讨论了不同应变水平下接头的断口形貌.结果表明,当疲劳应变幅△εt/2小于0.6％时,TC4-DT钛合金母材与接头的疲劳寿命2Nf基本相同,当疲劳应变幅△ε...     

薄壁TC4钛合金电子束焊接应用研究

针对某薄壁TC4钛合金零件的电子束焊接,设计了焊接工装夹具,保证了焊接变形要求。通过工艺试验,确定了合理的焊接方案,成功的实现了该零件的电子束焊接。同时,针对其成功应用的研究过程,从焊接工艺及加工方案上总结出经验,为薄壁类钛合金零件的电子束焊接提供了借鉴依据。     

Coupling plasma plume of a low-power magnetically shielded Hall thruster with a hollow cathode

The coupling region of a Hall thruster with a hollow cathode is the region between the cathode and the thruster plume. The characteristics of plasma in that region are complicated and strongly associated with the thruster working conditions and the cathode position. In this paper,a laboratory 100 W class magnetically shielded Hall thruster was coupled with a hollow cathode.Optical imaging and electrostatic probe were employed to monitor and scan the plasma plume.Plume characteristics in the coup...     

基于背散射电子的电子束加工过程在线观测系统研制

为了在高真空、高温、高金属蒸气的电子束加工过程中获得清晰的观测效果,采用四极板背散射电子接收传感器、高频信号放大电路、高频数据采集卡、高频偏转扫描系统等,研制了一套基于背散射电子的在线观测系统.通过试验验证,所研制系统可以有效观测100mm×100mm范围内的工件,图像分辨率为512像素×512像素,图像处理帧数可以达...     

Loop Models from SOHO Observations

The Coronal Diagnostic Spectrometer (CDS) on SOHO is a grazing/normal incidence spectrograph, aimed to produce stigmatic spectra of selected regions of the solar surface in six spectral windows of the extreme ultraviolet from 150 Å to 785 Å (Harrison et al. 1995). In the present work, CDS, EIT, MDI and Yohkoh observations of active region lops have been analyzed. These observations are part of JOP 54. CDS monochromatic images from lines at different temperatures have been co-aligned with EIT and MDI images, and loop structures have been clearly identified using Fe XVI emission lines. Density sensitive lines and lines from adjacent stages of ionization of Fe ions have been used to measure electron density and temperature along the loop length; these measurements have been used to determine the electron pressure along the loop and test the constant pressure assumption commonly used in loop modeling. The observations have been compared with a static, isobaric loop model (Landini and Monsignori Fossi 1975) assuming a temperature-constant heating function in the energy balance equation. Good agreement is found for the temperature distribution along the loop at the coronal level. The model pressure is somewhat higher than obtained from density sensitive line ratios.     

On the uncertainties in the measurement of absolute (true) TEC over Indian equatorial and low latitude sectors

The Indian sector encompasses the equatorial and low latitude regions where the ionosphere is highly dynamic and is characterized by the equatorial ionization anomaly (EIA) resulting in large latitudinal electron density gradients causing errors and uncertainties in the estimation of range delays in satellite based navigation systems. The diurnal and seasonal variations of standard deviations in the TEC data measured during the low sunspot period 2004–2005 at 10 different Indian stations located from equator to the anomaly crest region and beyond are examined and presented. The day-to-day variability in TEC is found to be lowest at the equatorial station and increases with latitude up to the crest region of EIA and decreases beyond.