"龙王"(LONGWANG)台风过程湿位涡的诊断分析   总被引：8，自引：2，他引：8       下载免费PDF全文

赖绍钧  何芬  赵汝汀  沈桐立  吴启树 《气象科学》2007,27(3):266-271

本文应用MM5V3中尺度数值模式对0519号台风“龙王”过程进行了数值模拟,利用模拟结果计算了台风过程湿位涡(Moist Potential Vorticity,MPV)的演变,从湿位涡的角度研究了台风过程大暴雨的产生机制。结果表明:倾斜涡度发展是“龙王”台风在福建沿海产生大暴雨的重要机制之一,湿位涡能够对暴雨落区的预报有较强的指示性作用,暴雨产生在θse线陡立的对流层中低层MPV1等值线密集带中零线附近,对流层中高层的MPV2负值区可以作为暖湿气流或涡旋活动的示踪;另外,对流层中高层中高纬度冷空气扩散南下与台风的东南暖湿空气在福建沿海交汇,加剧了气旋性涡度发展,对暴雨的发生发展也有巨大的作用。  相似文献   

南秦岭勉县─略阳结合带蛇绿岩与岛弧火山岩地球化学及其大地构造意义   总被引：31，自引：1，他引：30  

赖绍聪  张国伟  杨永成  陈家义 《地球化学》1998,(3)

南秦岭勉县-略阳结合带中超基性岩类主要为方辉橄榄岩和纯橄榄岩,稀土特征为轻稀土亏损,铕富集型;辉绿岩均为轻稀土富集型。变质火山岩可区分为两种组合：一为轻稀土亏损的洋脊拉斑玄武岩,其Ti／V．Th／Ta、Th／Yb、Ta／Yb表明其为MORB型玄武岩,代表本区消失了的洋壳岩石,指示本区晚古生代一早中生代期间的一个古洋盆。另一类为岛弧火山岩组合,除岛弧拉斑玄武岩外,甚至还有大量中、酸性岛弧火山岩,它们并非洋壳的物质组成,而是大陆弧岩浆活动的产物。这表明勉略洋盆在晚古生代-早中生代期间曾经经历过一个较完整的有限洋盆的发生、发展与消亡过程,这期间秦岭已成为一独立的岩石圈微板块,其南缘具有活动大陆边缘的构造属性,秦岭并非华北与扬子陆块之间的简单碰撞产物。  相似文献   

利用变参数回归方法反演泥质岩裂缝密度     

赖生华  刘文碧  李德发  周文  彭军 《沉积与特提斯地质》1998,18(3):50-54

本文利用变参数回归分析建立了多口井的泥质岩储层裂缝密度模型。该模型的平均相对误差为１３．５％,较常系数回归分析、ＢＰ网络模型进行裂缝预测的精度高（平均相对误差分别为３８．７％、１７．９％）。通过实际资料处理认为该油田在纵向上随时代变老,深度加深,裂缝密度降低。即从Ｎ２２、Ｎ１２到Ｎ１,平均裂缝密度从０．７８条／ｍ、０．５条／ｍ降低到０．３条／ｍ。在平面上,沿构造轴部裂缝最发育,平均裂缝密度Ｎ２２、Ｎ１２、Ｎ１层分别为０．５８条／ｍ、０．６条／ｍ、０．３条／ｍ。  相似文献   

Geochemical Features and Tectonic Settings of Upper Ordovician Marine Volcanic Rocks on North Margin of Qaidam     

Lai Shaocong  Deng Jinfu  Zhao Hailing 《中国地质大学学报(英文版)》1998,9(2)

ＩＮＴＲＯＤＵＣＴＩＯＮＡＮＤＢＲＩＥＦＧＥＯＬＯＧＩＣＡＬＤＥＳＣＲＩＰ┐ＴＩＯＮＳＴｈｅＵｐｐｅｒＯｒｄｏｖｉｃｉａｎｍａｒｉｎｅｖｏｌｃａｎｉｃｒｏｃｋｓｏｎｔｈｅｎｏｒｔｈｍａｒｇｉｎｏｆＱａｉｄａｍｈａｖｅｂｅｅｎｒｅｐｅａｔｅｄｌｙｄｉｓ...  相似文献   

中上扬子地区五峰组沉积环境分析   总被引：4，自引：0，他引：4  

蔡俊  何幼斌  张来  邱子瑶  甘永年 《海洋地质前沿》2010,26(6)

关于中上扬子地区五峰组的沉积环境是深水沉积还是浅水沉积,这两种观点一直存在较大争议,其焦点主要是关于对观音桥段介壳化石的不同认识。在数十年的学术讨论中,双方都试图从不同方面来证明各自的观点,但至今依然没有得到令人非常信服的结论。通过对古生态学、沉积速率、海平面变化、砾屑灰岩成因讨论等方面的综合分析,认为五峰组为深水沉积的观点更为合理。  相似文献   

Triangulated spherical splines for geopotential reconstruction     

M. J. Lai  C. K. Shum  V. Baramidze  P. Wenston 《Journal of Geodesy》2009,83(8):695-708

We present an alternate mathematical technique than contemporary spherical harmonics to approximate the geopotential based on triangulated spherical spline functions, which are smooth piecewise spherical harmonic polynomials over spherical triangulations. The new method is capable of multi-spatial resolution modeling and could thus enhance spatial resolutions for regional gravity field inversion using data from space gravimetry missions such as CHAMP, GRACE or GOCE. First, we propose to use the minimal energy spherical spline interpolation to find a good approximation of the geopotential at the orbital altitude of the satellite. Then we explain how to solve Laplace’s equation on the Earth’s exterior to compute a spherical spline to approximate the geopotential at the Earth’s surface. We propose a domain decomposition technique, which can compute an approximation of the minimal energy spherical spline interpolation on the orbital altitude and a multiple star technique to compute the spherical spline approximation by the collocation method. We prove that the spherical spline constructed by means of the domain decomposition technique converges to the minimal energy spline interpolation. We also prove that the modeled spline geopotential is continuous from the satellite altitude down to the Earth’s surface. We have implemented the two computational algorithms and applied them in a numerical experiment using simulated CHAMP geopotential observations computed at satellite altitude (450 km) assuming EGM96 (n _max = 90) is the truth model. We then validate our approach by comparing the computed geopotential values using the resulting spherical spline model down to the Earth’s surface, with the truth EGM96 values over several study regions. Our numerical evidence demonstrates that the algorithms produce a viable alternative of regional gravity field solution potentially exploiting the full accuracy of data from space gravimetry missions. The major advantage of our method is that it allows us to compute the geopotential over the regions of interest as well as enhancing the spatial resolution commensurable with the characteristics of satellite coverage, which could not be done using a global spherical harmonic representation. The results in this paper are based on the research supported by the National Science Foundation under the grant no. 0327577.  相似文献   

深圳市闪电定位资料误差分析及其优化     

曾庆锋  张其林  赖鑫  徐栋璞  王皓 《气象科技》2015,43(3):530-536

利用场地误差优化模式对深圳地区的地闪定位资料进行优化处理。首先对深圳市闪电定位系统进行简单介绍,然后利用改进的传输线模式对真实地表环境下的闪电辐射电磁场进行计算,以分析深圳市闪电定位系统的场地误差,最后基于定位误差和场地误差模式对闪电定位数据进行定位误差订正。结果表明不同方位角上的不规则地形对继后回击电磁场波形具有不同影响,随着表征地形粗糙程度的高度均方根的增加,电场的峰值下降,波形的上升沿时间增加。同时,电场波形上升沿时间也会随着方位角的变化而变化,这可能会给时间到达法的定位带来一定误差。为了验证该算法的合理性,对该系统覆盖的区域进行了闪电定位数据优化精度的时空分布分析和评估。结果表明这种优化方案是可行的、可靠的,优化后的闪电定位精度明显提高。  相似文献   

柳州夏季一次雨夹冰雹的天气过程分析     

覃艳秋  赖雨薇  刘蕾 《气象研究与应用》2015,36(1)

利用常规地面观测、柳州地面自动站、FY-2C卫星、柳州和河池的多普勒天气雷达观测资料,对2014年7月22日夏季柳州发生的一次短暂的雨夹冰雹天气过程的环境条件和雷达产品特征进行分析,主要结果如下:受副高和台风外围气流影响,柳州全市出现了37℃以上大范围的高温天气,天气尺度和中尺度的上升运动较弱,局地性质的加热作用导致大气的不稳定度加强而诱发对流云系进一步发展造成的;雷达显示的冰雹云的最大基本反射率因子为65d BZ,强回波区面积小;风速的切变和辐合上升运动小,0℃层高度较高,不利于对流系统的发展和维持。  相似文献   

Characteristics of convection and overshooting in RGB and AGB stars     

Xiang-Jun Lai    Yan Li  National Astronomical Observatories/ Yunnan Observatory  Chinese Academy of Sciences  Kunming  China  Key Laboratory for the Structure  Evolution of Celestial Objects  China Graduate University of Chinese Academy of Sciences  Beijing  China. 《中国天文和天体物理学报》2011,(10)

Based on the turbulent convection model (TCM) of Li & Yang, we have studied the characteristics of turbulent convection in the envelopes of 2 and 5M⊙ stars at the red giant branch and asymptotic giant branch phases. The TCM has been successfully applied over the entire convective envelopes, including the convective unstable zone and the overshooting regions. We find that the convective motions become progressively stronger when the stellar models are located farther up along the Hayashi line. In the convect...  相似文献   

A note on the discovery of a 2M_⊙ pulsar     

Xiao-Yu Lai  Ren-Xin Xu School of Physics  State Key Laboratory of Nuclear Physics  Technology  Peking University  Beijing  China 《中国天文和天体物理学报》2011,(6)

It is conventionally thought that the state equation of dense matter softens and thus cannot result in high maximum mass if pulsars are quark stars and that a recently discovered 2M⊙ pulsar (PSR J1614-2230) may make pulsars unlikely to be quark stars. However, this standard point of view would be revisited and updated if quark clustering could occur in cold quark matter because of the strong coupling be- tween quarks at realistic baryon densities in compact stars. It can be argued that the state equation of...  相似文献