德令哈两次大雨天气的雷达应用对比分析     

《青海气象》2013,(1)

利用德令哈X波段雷达站多普勒天气雷达资料、卫星云图、自动站及常规资料,对2012年6月5日德令哈市区和6月6日德令哈可鲁克湖的强降水天气过程的雷达回波特征及中小尺度系统进行了初步分析。分析表明:6月5日降水回波主要是暖平流下的积云层状云混合降水回波,此次强降水与对流单体不断生成并东移产生"列车效应"有直接关系。而6月6日降水回波主要是冷平流下的积云降水回波,并产生了"风暴"、"中气旋"、"雹云"等危险天气报警,具备中等到强垂直风切变环境中的多单体强风暴的特征。  相似文献   

台风山竹(1822)龙卷的双极化相控阵雷达特征          下载免费PDF全文

傅佩玲  胡东明  黄浩  张羽  田聪聪 《应用气象学报》2020,31(6):706-718

2018年9月17日台风山竹（1822）外围螺旋雨带中发生EF2级龙卷。在高湿度、高不稳定、强垂直风切变的环流背景下,龙卷在台风外围雨带上微型超级单体右后侧钩状回波顶端的弱回波区中发展起来。具有高时空分辨率的广州X波段双极化相控阵雷达,不仅观测到超级单体的发展过程,还呈现出龙卷涡旋演变特征:单体风暴尾端在右后方入流加强作用下,逐渐形成钩状回波形态,此时对流层中低层2~3 km高度附近的中气旋强度率先达到最大,随着旋转强度进一步加强和旋转中心高度逐步下降,低层强旋转特征越来越明显,当低层旋转速度达到峰值（超过21 m·s-1）,旋转直径收缩到1 km范围,地面出现EF2级以上龙卷,旋转速度对区域出现清晰的弱回波龙卷眼区特征。X波段双极化相控阵雷达在龙卷观测中优势显著,弥补了多普勒天气雷达观测的不足。  相似文献   

一种仿苏纪石材料的宝石学特征     

丛众  吴瑞华  王时麒  师伟 《地质科学译丛》2011,(1):16-20,42

采用宝石显微镜、偏光显微镜、电子探针、X射线粉末衍射仪和傅里叶变换红外光谱仪等测试方法对近期在北京珠宝市场上大量出现的一种仿苏纪石材料样品进行了常规宝石学、矿物学、谱学特征研究。结果表明,该仿苏纪石材料是以透闪石为主要矿物、石英为次要矿物的染色玉石;其与天然苏纪石的主要鉴别特征为：该仿苏纪石材料的密度较大,表面较粗糙以及特征的红外光谱。  相似文献   

用于有机废水处理的改性膨润土的制备新方法研究   总被引：2，自引：0，他引：2       下载免费PDF全文

凌辉  鲁安怀  王长秋 《岩石矿物学杂志》2011,30(1):135-140

提出一套不同于传统工艺的有机化膨润土制备方法,并首次采用COD(化学需氧量)与XRD(X射线衍射)双重指标衡量有机化膨润土的合成效果。COD测试表明,选择合适的改性剂种类和用量,是制备废水处理用有机化膨润土的两个前提。XRD分析说明,新工艺制备的有机化膨润土中蒙脱石的d001明显增大,有机改性剂长链分子已经插入蒙脱石矿物层间,合成效果良好。新的有机化膨润土合成工艺省去了过滤、洗涤、烘干、粉碎等步骤,能耗大大降低,成本优势明显,能够有力地促进有机化膨润土在废水处理领域的规模化应用。  相似文献   

Solar Impulsive Hard X-Ray Emission and Two-Stage Electron Acceleration     

Arjun Tan  Shi Tsan Wu 《中国天文和天体物理学报》2006,6(6):733-740

Heating and acceleration of electrons in solar impulsive hard X-ray (HXR) flares are studied according to the two-stage acceleration model developed by Zhang for solar 3He-rich events. It is shown that electrostatic H-cyclotron waves can be excited at a parallel phase velocity less than about the electron thermal velocity and thus can significantly heat the electrons (up to 40 MK) through Landau resonance. The preheated electrons with velocities above a threshold are further accelerated to high energies in the flare-acceleration process. The flare-produced electron spectrum is obtained and shown to be thermal at low energies and power law at high energies. In the non-thermal energy range, the spectrum can be double power law if the spectral power index is energy dependent or related. The electron energy spectrum obtained by this study agrees quantitatively with the result derived from the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) HXR observations in the flare of 2002 July 23. The total flux and energy flux of electrons accelerated in the solar flare also agree with the measurements.  相似文献   

The Multi-Wavelength Quasar Survey Ⅲ. Quasars in Field 836     

Yu Bai Yang Chen Xiang-Tao He Jiang-Hua Wu Qing-Kang Li Richard F.Green Wolfgang Voges 《中国天文和天体物理学报》2007,7(3):375-379

This is the third paper in a series connected with our Multiwavelength Quasar Survey. The survey is aimed to provide a quasar sample more complete than any previous survey by using a combined selection technique to reduce selection effects. We present the observational results for the X-ray candidates in field f836. We found 15 X-ray AGNs in this field of which eight are new discoveries. The X-ray data and optical spectra of these AGNs are given. We give the X-ray candidate selection criteria, which proved to be highly efficient in isolating X-ray AGNs.  相似文献   

Separation of Different Contributions to the Total X-ray Luminosity in Gamma-ray Loud Blazars     

Gustavo E.Romero 《中国天文和天体物理学报》2005,5(5):457-462

The relativistic beaming model has been successfully used to explain many of the observational properties of active galactic nuclei. In this model the total emission is formed by two components, one beamed, one unbeamed. However, the exact contribution from each component in unresolved sources is still not clear. In the radio band, the core and extended emissions are clearly separated. We adopt the method proposed by Kembhavi to separate the two contributions in the X-ray emissions in a sample of 19 gamma-ray loud blazars. It is clearly shown that the beamed emission dominates the X-ray flux and the unbeamed X-ray emission is correlated with the extended radio emission of the considered objects. We also find that the ratio of the beamed to the unbeamed X-ray luminosity is correlated with the X-ray spectral index, an effect that should be a consequence of the underlying X-ray emission mechanism.  相似文献   

吸积盘物理：稳定性和振动     

吴学兵 《云南天文台台刊》2003,(1):31-36

研究了环绕致密天体的吸积盘的稳定性质和振动模式。特别关注了在热致和粘滞扰动作用下稳定的对流起支配作用的盘外流。还研究了相对论性吸积盘的振动模式。一些在盘内的捕获的，非衰减的模式也许可以用来解释X射线双星和活动星系核中所观测到的准周期振动。  相似文献   

由对FRⅡ射电星系的X射线观测试预言射电噪活动星系核的X射线喷流     

白金明 《云南天文台台刊》2003,(1):19-25

在早期的文章中，基于耀变体（Blazar)的知识，我们预言了在射电噪活动星系核（AGN）中心10kpc范围内X射线喷流的存在。钱得拉（Chandra)卫星最近对低功率射电星系的X射线观测与我们的预言相一致。在本文中我们研究了kpc尺度喷流中的电子加速，并建议通过对强的FRⅡ射电星系中所预言的X射线喷流的钱得拉卫星的X射线的观测，来研究红的耀变体中的康普顿冷却以及在内部致密喷流和大尺度延伸喷流间环境的不同。以上的研究可以进一步检验我们的关于射电噪活动星系核中kpc尺度X射线喷流的模型。  相似文献   

Verification of Short-Term Predictions of Solar Soft X-ray Bursts for the Maximum Phase （2000-2001） of Solar Cycle 23     

Cui-Lian Zhu  Jia-Long WangNational Astronomical Observatories  Chinese Academy of Sciences  Beijing   《中国天文和天体物理学报》2003,3(6):563-568

We present a verification of the short-term predictions of solar Xray bursts for the maximum phase (2000-2001) of Solar Cycle 23, issued by two prediction centers. The results are that the rate of correct predictions is about equal for RWC-China and WWA; the rate of too high predictions is greater for RWC-China than for WWA, while the rate of too low predictions is smaller for RWC-China than for WWA.  相似文献