新疆北山构造带西段小长山南超单元花岗岩特征

小长山南超单元花岗岩是新疆北山构造带中重要的地质体 ,为华力西中期第 2序次岩浆侵入活动的产物 ,包括 5个单元 ,出露面积 132 .9km2 ,其中第 4单元同位素地质年龄 32 0 .2Ma±2 3Ma(锆石 ,Pb -Pb法 )。岩石系列属钙碱性 ,为明显同源岩浆演化序列 ,微量元素指示其具大陆弧背景下成熟弧花岗岩和I型花岗岩特征。综合分析后认为小长山南超单元花岗岩属北山克拉通裂谷闭合期岩浆强力就位产物     

广州“5.7”高空槽后和“5.14”槽前大暴雨过程对比分析

利用常规观测资料和雷达资料,对广州2010年5月7日槽后大暴雨和2010年5月14日槽前大暴雨过程进行对比分析。结果表明：＂5.7＂大暴雨主要受500hPa高空槽后西北气流和850hPa切变线的共同作用,与典型的华南前汛期暴雨形势不同的是槽后冷空气叠加在低层暖湿气流上,对层结不稳定起到增幅作用;＂5.14＂大暴雨过程主要受高空槽前的西南气流、切变线和地面弱冷空气共同影响。两次大暴雨过程都是由带有超级单体的飑线引发的,前者飑线长度更长,强回波范围更大,超级单体更多,降水强度和累积降水量更大;飑线维持和发展的机制不同,前者通过补充合并两广交界处不断新生对流单体,后者则是通过吸收合并其移动前方沿近地层辐合带新生单体,得以维持和发展。     

The Cretaceous Turn of Geological Evolution: Key Evidence from East Asia

this work focuses on one of the critical points of Earth’s history when the Solar System passed through the most distant point of its galactic orbit. During this event, Earth may have suffered from maximum extension, associated with its relative proximity to the Sun at that time, followed by long-term contraction related to its later distancing. This paper is based on generalized data on the Cretaceous evolution of the Earth as a whole and of East Asia in particular. The evidence suggests that major geological processes at this time may be interpreted as transitional changes in the state of Earth. A liquid nature of its core may have reacted to the gravitational and electromagnetic transformations. When the cosmic changes took place at 135-120 Ma, more turbulent flows in the outer core would have favoured the rise of voluminous magmatic plumes and associated fluid flows. These would substantially transform the mantle, crust, hydrosphere, biosphere and atmosphere. In particular, plume-related melting of overlying subducting slabs and lower continental crust could have initiated numerous adakitic melts that formed the East Asian Adakitic Province. These and associated juvenile events produced numerous metallic ore, coal, gas and oil deposits. The Cretaceous is one of the most significant resource-producing periods.     

上海二次温室大棚区强尘卷风的成因分析

尘卷风是近地面气层中的小旋风,使沙尘或其他细小物体随风卷起而形成的一种天气现象。2011年10月27日11时10分和2015年9月13日11时12分发生于上海地区的两次强尘卷风天气过程(北京时,下同)均造成了不同程度的灾害。两次尘卷风均发生在温室大棚区,其下垫面性质和干旱区裸露地面和水泥沥青城市地面极不相同,因此了解其发生原因很有必要。本文利用常规天气图、温度对数压力图、100 m以下5层铁塔风和温度、微波辐射仪以及温室大棚基地自动气象站等资料对这两次尘卷风过程进行了分析。发现.在常规探空都未探测到明显的超绝热现象,但在铁塔观测的地表面层温度垂直廓线结合微波辐射仪及自动气象站等资料揭示了尘卷风发生时近地面气层都具备了超绝热条件。尘卷风发生前后10∶00—12∶00的10～70 m温度垂直递减率γ平均达1.58℃/100 m,极大值达2.33℃/100 m,为干绝热递减率的两倍还多。上海地区10座铁塔测风网获得的10、30、50、70 m近地层风场的旋转和辐合特征揭示了尘卷风旋转的角动量来源。通过分析500、700、850 hPa天气形势探讨了有利于发生尘卷风的大尺度环流条件为尘卷风预报提供参考。最后对这两次尘卷风发生在温室大棚区域而不是自然农田的机理提出了初步看法供进一步讨论。     

Trimble S6超站仪在大比例尺地形图检验中的应用研究

超站仪是将全站仪与GNSS整合在一起的新型测量设备,使用超站仪测量,无须控制点,利用CORS系统和似大地水准面精化模型,采用GNSS RTK技术获取测站点坐标和高程,并按全站仪功能进行地形要素采集。本文以Trimble S6超站仪为研究对象,在大比例尺地形图测绘成果质量检验应用中提高了检验效率,实现了检验智能化。     

Development of a New Method of Extraction of Interstitial Water from Low‐Porosity Consolidated Sediments Recovered During Super‐Deep Drilling Projects

During the Integrated Ocean Drilling Program (IODP) Expedition 338, several methods were tested for the extraction of interstitial water in consolidated, low‐porosity deep‐sea sediments from Site C0002 in the Kumano Basin. On the basis of those tests, we propose a modified ground rock interstitial normative determination (GRIND) method of extraction of interstitial water. In separate runs of the new method, sediment samples were ground in a ball mill with either ultrapure water or a solution of HNO₃. The interstitial water was then extracted with a conventional squeezer. Sufficient solution was extracted by this method to analyse most major and a few minor components of interstitial water that were comparable to those previously reported for samples extracted by the conventional squeezing method. The new method requires much smaller amounts of sediment than that of the conventional method and will be useful for analysis of samples recovered during super‐deep drilling programmes.     

小波超分辨率重建算法及其在SPOT影像中的应用

影像超分辨率重建就是从一系列质量较差、分辨率较低的图像来重建图像质量更好、空间分辨率更高的影像的算法.在将所有低分辨率影像纳入同一参考格网中考虑的情况下,低分辨率数据相当于一非规则采样的交错采样数据.本文在多分辨率分析的基础上对基于小波的影像超分辨率重建理论进行介绍,并将现有的小波超分辨率重建算法推广到更一般的运动模型,以充分利用交错采样数据的内在规律性和结构特征,同时针对SPOT影像的特点,分析SPOT影像的调制传送函数,对SPOT重建影像进行包括去噪与解卷积的复原后处理.最后给出基于小波的SPOT影像超分辨率重建结果,表明遥感影像的超分辨率重建在应用中取得进展.     

调制结构矿物晶体的单晶X射线衍射特征

调制结构广泛存在于天然矿物中,利用具有照相特点的CCD平面高灵敏探测器单晶X射线衍射仪,对公度和非公度调制结构的单晶衍射特征进行了研究,根据倒易点的分布规律和晶胞特点提出了超结构的分类方法和非公度调制结构的高维指标化方法。     

Variability and evolution in various classes of post‐AGB stars

We aim to compare properties of early‐type post‐asymptotic giant‐branch (post‐AGB) stars, including normal first‐time B‐type post‐AGB stars, and extreme helium stars (EHes). Hipparcos photometry for 12 post‐AGB stars and 7 EHe stars has been analyzed; 5 post‐AGB stars are clearly variable. The Hipparcos data are not sufficiently sensitive to detect variability in any of the EHes. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

特大型银矿床地质特征及找矿方向

特大型银矿床在资源占有量上占举足轻重的地位,使之已经成为近年来重要的研究课题之一.从已知的国内外特大型银矿床入手,在成矿时间、空间以及成矿特征方面进行了深入的研究.提出了特大型银矿床的主要成矿地质特征、矿床类型划分方案及在我国的找矿方向.概括如下:(1)已知特大型银矿床均分布于环太平洋成矿带内,主要受控于中生代、新生代的火山岩带和裂谷带之中,多数矿床与中酸性-酸性岩浆活动有关;(2)特大型银矿床以成矿系列为主要线索,划分为浅成低温热液型、斑岩型、矽卡岩型和5元素型;(3)中国在中新生代火山岩及裂谷发育地区,如大兴安岭-太行山带等,具有特大型银矿床的成矿潜力.