Cross-Wavelet Analysis of the Arctic Oscillation and Climate Change in Northwest China     

GUO Qu  SUN Wei-guo  CHENG Bing-yan  DENG Ai-juan 《南京气象学院学报》2008,31(6)

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山东省气象通信网络系统简介     

曲军 《山东气象》2008,28(1):41-42

从通信网络、网络安全、视频系统、介绍了目前在实现气象信息收集、传输、方式。资料处理、信息共享等5个方面,信息共享方面的网络组成及通信  相似文献   

The causality between the rapid rotation of a sunspot and an X3.4 flare     

Xiao-Li Yan Zhong-Quan Qu Cheng-Lin Xu Zhi-Ke Xue De-Fang Kong 《中国天文和天体物理学报》2009,9(5)

Using multi-wavelength data of Hinode, the rapid rotation of a sunspot in ac-tive region NOAA 10930 is studied in detail. We found extraordinary counterclockwise rotation of the sunspot with positive polarity before an X3.4 flare. From a series of vector magnetograms, it is found that magnetic force lines are highly sheared along the neu-tral line accompanying the sunspot rotation. Furthermore, it is also found that sheared loops and an inverse S-shaped magnetic loop in the corona formed gradually after the sunspot rotation. The X3.4 flare can be reasonably regarded as a result of this movement. A detailed analysis provides evidence that sunspot rotation leads to magnetic field linestwisting in the photosphere. The twist is then transported into the corona and triggers flares.  相似文献   

东秦岭东段新发现的沙坡岭细脉浸染型钼矿地质特征、Re-Os同位素年龄及其地质意义   总被引：7，自引：0，他引：7  

苏捷  张宝林  孙大亥  崔敏利  屈文俊  杜安道 《地质学报》2009,83(10):1490-1496

豫西洛宁沙坡岭钼矿床位于华北克拉通南缘东秦岭钼矿带东段,是新近发现的赋存于太古宙太华群变质岩中的细脉浸染型钼矿床。本文对其地质特征进行了研究,并初步测定了1个辉钼矿样品的Re－Os同位素年龄,获得模式年龄为126.8±1.7Ma,表明沙坡岭钼矿形成于燕山期,接近金堆城、雷门沟钼矿的形成时代,Re同位素含量显示其地幔来源的特征。沙坡岭钼矿形成机制错综复杂,有待进一步研究,特别是深部钻孔工程验证工作,对于验证深部是否隐伏着与成矿相关的斑岩体、储量更大的斑岩型钼矿有着重要作用,找矿潜力巨大。  相似文献   

金川铜镍硫化物样品中锇同位素比值的高精度分析   总被引：11，自引：2，他引：9  

屈文俊  杜安道  李超  孙文静 《岩矿测试》2009,28(3):219-222

采用两种独立的190Os稀释剂、4个不同的化学流程,用等离子体质谱仪、TRITON热表面电离质谱仪和MAT-262固体质谱仪3种质谱仪器,在4个实验室分别对采自金川铜镍硫化物样品的187Os/188Os同位素比值进行分析,样品分析数量达到56个。4个实验室获得的结果分别为0.3356±0.0018(n=12,2s)、0.3363±0.0008(n=6,2s)、0.3363±0.0010(n=18,2s)和0.3353±0.0034(n=20,2s)。采用ISOPLOT软件对所得56个数据进行加权平均计算,得到187Os/188Os同位素比值为0.33602±0.00022(置信度95%)。两台TRITON热表面电离质谱仪测量的结果几乎完全一致,且精度高于MAT-262固体质谱仪和等离子体质谱仪。比较了碱熔和Carius管两种溶样方法,结果表明,对于所研究的样品,用Carius管溶矿方式可以将含锇矿物完全溶解。  相似文献   

藏西班公湖斑岩铜矿带成矿斑岩地球化学及Pb、Sr、Nd同位素特征   总被引：9，自引：1，他引：8  

辛洪波  曲晓明  王瑞江  刘鸿飞  赵元艺  黄玮 《矿床地质》2009,28(6):785-792

对班公湖铜矿带2个具有代表性的斑岩铜矿床--多不杂铜矿床和尕尔穷铜矿床进行了详细的岩石地球化学和Pb、Sr、Nd同位素特征研究表明,与冈底斯铜矿带相比,该铜矿带含矿斑岩大离子不相容元素的富集程度相对减弱,而高场强元素和重稀土元素的亏损程度明显减轻,轻、重稀土元素的分馏程度减弱,且具有Eu的弱正异常,岩石在氧化性上更强一些;从Pb、Sr、Nd同位素特征来看,班公湖铜矿带含矿斑岩更富含放射性成因铅,~(143)Nd/~(144)Nd比值明显降低,其源区更接近印度洋沉积物区域,表明该铜矿带含矿斑岩的岩浆源区更浅,有更多的地壳物质加入;班公湖铜矿带含矿斑岩形成的构造环境属于活动大陆边缘区域,而冈底斯铜矿带明显偏离了活动大陆边缘区域,表明班公湖斑岩铜矿带形成于碰撞后地壳隆升阶段,而冈底斯铜矿带则形成于碰撞后地壳伸展阶段.  相似文献   

西藏班公湖岛弧带含硫化镍超基性岩的源区性质与基底背景   总被引：5，自引：1，他引：4  

江军华  王瑞江  曲晓明  辛洪波 《矿床地质》2009,28(6):793-802

青藏高原班公湖一怒江成矿带上的超基性岩型硫化镍矿化是近年来在西藏地区发现的矿化新类型.文章根据成矿带西段班公湖地区含镍超基性岩体的岩石地球化学和Sr、Pb同位素分析结果,论述了含镍超基性岩浆的源区性质及生成条件,并根据锆石U-Pb LA-ICP-MS年龄测定结果,探讨了藏西北地区的基底背景.研究发现,班公湖地区的含镍超基性岩体以富集大离子不相容元素Rb、Th、U、Sr、Pb,亏损Ba、K为特点,高场强元素亏损Nb、Ti,富集Ta;稀士元素相对球粒陨石亏损强烈,但轻稀土元素相对富集.这些特点一致反映出含矿岩浆产生于受俯冲沉积物熔体交代的富集型岩石圈地幔源区.岩浆的生成深度较浅,为尖晶石二辉橄榄岩相,源区部分熔融程度较低,大体在10%左右.岩石中集中出现一批24.79亿年的残留锆石年龄,标志着当时班公湖中特斯洋盆沉积物的物源区较为单一,主要来自太古代末-元古代初的古老基底,并且推测太古代与元古代之交(25亿年)有可能是藏西北的一个古陆壳快速生长期.  相似文献   

安徽铜陵新桥Cu-Au-Fe-S矿床黄铁矿Re-Os定年及成矿意义   总被引：5，自引：0，他引：5       下载免费PDF全文

谢建成  杨晓勇  杜建国  杜小伟  肖益林  屈文俊  孙卫东 《地质科学》2009,44(1):183-192

安徽铜陵地区是长江中下游Cu-Au-Fe-S成矿带中的一个重要成矿区,新桥大型Cu-Au-Fe-S矿床为其重要的矿床之一.运用Re-Os同位素定年方法对该矿床中矿石的黄铁矿进行了精确定年测定,首次获得了黄铁矿的Re-Os等时线年龄为126±11Ma,初始OS值1.2±1.9（MSWD=2.6）,属早白垩世,代表了铁硫化物的成矿年龄.结合前人的精确同位素定年结果,认为铜陵地区存在两种成矿事件,一种是与Cu-Au-Mo矿有关的成矿事件,代表的铜钼金硫化物的成矿年龄为138.0～140.0 Ma;另一种与铁矿有关的成矿事件,代表的铁硫化物的成矿年龄为112.6～126 Ma.  相似文献   

A systematic study on energy dependence of quasi-periodic oscillation frequency in GRS 1915+105     

Shu-Ping Yan  Jin-Lu Qu  Guo-Qiang Ding  Peng Han  Li-Ming Song  Shu Zhang  Hong-Xing Yin  Cheng-Min Zhang  Jian-Min Wang 《Astrophysics and Space Science》2012,337(1):137-146

Systematically studying all the RXTE/PCA observations for GRS 1915+105 before November 2010, we have discovered three additional patterns in the relation between Quasi-Periodic Oscillation (QPO) frequency and photon energy, extending earlier outcomes reported by Qu et al. (Astrophys. J. 710:836, 2010). We have confirmed that as QPO frequency increases, the relation evolves from the negative correlation to positive one. The newly discovered patterns provide new constraints on the QPO models.  相似文献   

Morphological analysis on the coherence of kHz QPOs     

J. Wang  H. K. Chang  C. M. Zhang  D. H. Wang  L. Chen  J. L. Qu  L. M. Song 《Astrophysics and Space Science》2012,342(2):357-364

We take the recently published data of twin kHz quasi-period oscillations (QPOs) in neutron star (NS) low-mass X-ray binaries (LMXBs) as the samples, and investigate the morphology of the samples, which focuses on the quality factor, peak frequency of kHz QPOs, and try to infer their physical mechanism. We notice that: (1) The quality factors of upper kHz QPOs are low (2～20 in general) and increase with the kHz QPO peak frequencies for both Z and Atoll sources. (2) The distribution of quality factor versus frequency for the lower kHz QPOs are quite different between Z and Atoll sources. For most Z source samples, the quality factors of lower kHz QPOs are low (usually lower than 15) and rise steadily with the peak frequencies except for Sco X-1, which drop abruptly at the frequency of about 750 Hz. While for most Atoll sources, the quality factors of lower kHz QPOs are very high (from 2 to 200) and usually have a rising part, a maximum and an abrupt drop. (3) There are three Atoll sources (4U 1728-34, 4U 1636-53 and 4U 1608-52) of displaying very high quality factors for lower kHz QPOs. These three sources have been detected with the spin frequencies and sidebands, in which the source with higher spin frequency presents higher quality factor of lower kHz QPOs and lower difference between sideband frequency and lower kHz QPO frequency.  相似文献