两种导风方法在台风路径分析中的 应用比较研究   总被引：2，自引：1，他引：1  

李峰  王振会  官莉  河惠清 《气象科学》2009,29(3):330-334

基于云导风使用的最大相关法（已经广泛应用）和TCFM法（傅立叶相位分析法和最大相关法相结合）两方法的原理,开发了利用FY-2C静止气象卫星30min间隔卫星云图资料获得云迹风的可视化导风实验系统。利用该系统处理2005年夏季麦莎、卡努、龙王等3个台风期间的卫星云图,对得到的云迹风进行台风路径反演分析。结果表明,TCFM导风方法得到的结果优于最大相关法。  相似文献   

Numerical study of a downslope windstorm in Northwestern Greece     

I. Koletsis  K. Lagouvardos  V. Kotroni  A. Bartzokas 《Atmospheric Research》2009,94(2):178-193

This paper describes the leeside wind storm of 25–26 March 1998, the most intense wind storm of the last decade in Northwestern Greece. This wind storm produced wind gusts of  30 m s^− 1 that resulted in tree uprooting, roof damaging, electric power network disruption and flooding in the lake-side areas of Ioannina city in Northwestern Greece. With the aim to identify the role of Mountain Mitsikeli near the city of Ioannina on the windstorm and to investigate the physical mechanisms responsible for such orographically induced weather events, numerical simulations with MM5 model have been performed. The model results showed that a resolution of 2-km resolution is necessary in order to reproduce the localized character of the wind storm. The analysis revealed that a synergistic combination of the cross-barrier northeasterly flow, the stable layer above the mountain top and the presence of a critical level, led to the intensification of the lee side winds during the studied wind event. Sensitivity experiments with modified topography, further supported the important role of mountain Mitsikeli that stands as an isolated obstacle, on the modification of the wind field during the observed windstorm.  相似文献   

Accreting white dwarfs as supersoft X‐ray sources     

M. Kato 《Astronomische Nachrichten》2010,331(2):140-145

I review various phenomena associated with mass‐accreting white dwarfs (WDs) in the view of supersoft X‐ray sources. When the mass‐accretion rate is low (Ṁ_acc < a few × 10^–7 M⊙yr^–1), hydrogen nuclear burning is unstable and nova outbursts occur. A nova is a transient supersoft X‐ray source (SSS) in its later phase which timescale depends strongly on the WD mass. The X‐ray turn on/off time is a good indicator of the WD mass. At an intermediate mass‐accretion rate an accreting WD becomes a persistent SSS with steady hydrogen burning. For a higher mass‐accretion rate, the WD undergoes “accretion wind evolution” in which the WD accretes matter from the equatorial plane and loses mass by optically thick winds from the other directions. Two SSS, namely RX J0513‐6951 and V Sge, are corresponding objects to this accretion wind evolution. We can specify mass increasing WDs from light‐curve analysis based on the optically thick wind theory using multiwavelength observational data including optical, IR, and supersoft X‐rays. Mass estimates of individual objects give important information for the binary evolution scenario of type Ia supernovae (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

The study of proto-magnetar winds     

Yan-Jun Chen  Ye-Fei Yuan 《中国天文和天体物理学报》2010,10(3)

The velocity profiles and properties of proto-magnetar winds are investigated.It is found that the corotation of wind matter with magnetic field lines significantly affects r-process nucleosynthesis and could lead to long duration γ-ray bursts and hyper-energetic supernovae.  相似文献   

DEVELOPING AND NON-DEVELOPING TROPICAL CYCLONES AS REVEALED BY HIGH DENSITY CLOUD MOTION WINDS   总被引：1，自引：0，他引：1  

方翔  许健民  张其松 《热带气象学报(英文版)》2001,7(1):80-85

An algorithm for computation of cloud motion winds has been developed at the National Satellite Meteorological Center in China. Since 1997, it has been applied to calculate the cloud motion winds for a 1.25 lat. 1.25 long. mesh over the northwest Pacific region with the satellite data from GMS-5. The development of the tropical cyclones is studied. It shows that the tropical cyclone is usually intrigued by the westerly jet streams at the upper levels of the troposphere, which may be caused by mid-latitude troughs well extending into the tropics. During the prime season of summer, the westerly flowing equatorward of the TUTT may also be a cause for the generation of typhoons.  相似文献   

近地质时期岩石圈板块构造运动的力学分析     

程学友 《地质与勘探》1995,31(5):15-22

运用相对运动的地球动力学理论，把软流圈以上的岩石圈和软流圈以下的地球内圈，作为两个独立的运动单元来考察它们随地球自转时所发生的变化和各自的运动状态。完整的岩石圈碎裂成岩石块之后，它们各自作为独立的单元，在纬向西漂力、经向离极力和洋底扩张力联合作用下，产生相对运动。  相似文献   

Vector magnetic analysis within the southern Ayu Trough, equatorial western Pacific   总被引：2，自引：1，他引：2  

Sang-Mook Lee  Seung-Sep Kim 《Geophysical Journal International》2004,156(2):213-221

  相似文献   

Divergent evolution in fluviokarst landscapes of central Kentucky     

Jonathan D. Phillips  Linda L. Martin  Viva G. Nordberg  William A. Andrews 《地球表面变化过程与地形》2004,29(7):799-819

Central Kentucky is characterized by a mixture of karst and ?uvial features, typically manifested as mosaic of karst‐rich/channel‐poor (KRCP) and channel‐rich/karst‐poor (CRKP) environments. At the regional scale the location and distribution of KRCP and CRKP areas are not always systematically related to structural, lithological, topographic, or other controls. This study examines the relationship of KRCP and CRKP zones along the Kentucky River gorge area, where rapid incision in the last 1·5 million years has lowered local base levels and modi?ed slopes on the edge of the inner bluegrass plateau. At the scale of detailed ?eld mapping on foot within a 4 km² area, the development of karst and ?uvial features is controlled by highly localized structural and topographic constraints, and can be related to slope changes associated with retreat of the Kentucky River gorge escarpment. A conceptual model of karst/?uvial transitions is presented, which suggests that minor, localized variations are suf?cient to trigger a karst–?uvial or ?uvial–karst switch when critical slope thresholds are crossed. Copyright © 2004 John Wiley & Sons, Ltd.  相似文献   

An Idealized Mean Wind Profile for the Atmospheric Boundary Layer     

John D. Wilson  Thomas K. Flesch 《Boundary-Layer Meteorology》2004,110(2):281-299

We test a flexible, idealized mean wind profile for the loweratmosphere that can easily be matched to whatever windobservations may be available. Its intended function is to providea `best guess' wind profile from limited observations, e.g., foruse in dispersion models, and to this end, following earlierauthors, we have matched a Monin–Obukhov layer to a baroclinic Ekman layer.To demonstrate the flexibility of the two-layer wind profile, weoptimize its free parameters to provide best interpolative fits toa sample of multi-level wind profiles. These include model windprofiles extracted from the Canadian Global EnvironmentalMulti-scale weather model (GEM), as well as experimental profilesfrom the Wangara experiment, and from an over-ocean dispersionexperiment (LROD). In most cases the two-layer profile fit issatisfactory.  相似文献   

多普勒雷达估算降水和反演风在不同初值方案下对降水预报影响的数值研究   总被引：7，自引：6，他引：7  

王叶红  赵玉春  崔春光 《气象学报》2006,64(4):485-499

基于有限区域中尺度暴雨预报模式AREM,利用常德、荆州、宜昌3部多普勒雷达及武汉数字化天气雷达联合反演的1h降水量资料和宜昌、荆州多普勒雷达反演的水平风场资料,采用3种不同的初值方案:Grapes-3DVAR同化方案、Barnes客观分析法及Barnes-3DVAR同化方案,对2002年7月22日20:00—23日20:00发生在长江流域的一次大暴雨过程进行了多普勒雷达估算降水和反演风场在不同初值方案下对降水预报影响的数值试验,结果表明:(1)采用相同资料源(探空 T213L31分析场),3种初值方案降水模拟效果差别显著。整体而言,融合了Barnes和3DVAR两种方案的Barnes-3DVAR初值方案降水模拟效果最好:雨带模拟完整,位置与实况完全一致;降水中心中尺度结构清晰,位置、强度与实况接近。(2)Barnes-3DVAR同化方案与Grapes-3DVAR同化方案都能同化雷达降水和风场资料,但两者降水预报结果相差很大。Barnes-3DVAR方案下的降水模拟结果明显好于Grapes-3DVAR同化方案。(3)Grapes-3DVAR同化方案下,在控制试验的基础上增加雷达降水资料的同化,24h降水模拟效果有所改善;增加雷达风场资料的同化,仅部分改善模拟效果,某些地方效果反而变差;同时增加雷达降水和风场资料的同化,降水模拟效果反而明显变差。Barnes-3DVAR同化方案则不然,无论雷达降水资料和风场资料单独同化还是两种资料同时同化,降水模拟效果都有不同程度的改进,特别是对雷达降水和风场资料同时同化的模拟结果是各种试验中效果最好的。(4)融合Barnes客观分析方法和Grapes-3DVAR同化方案的Barnes-3DVAR同化方案,是同化雷达降水和风场资料的一种新的、有效的初值方案。  相似文献