巍山火山村地区中低温热液型铅锌多金属矿     

胡文奎  尹银寿  孙贵荣  董建春 《云南地质》2009,28(2):161-165

矿体产于灰岩与泥岩间接触处的灰岩构造裂隙中为受褶皱内部构造裂隙带控制的中低温热液型矿床,通过地质勘查工作,认为矿区外围具备进一步的找矿地质条件。  相似文献   

2008年6—8月T639、ECMWF及日本模式中期预报性能检验   总被引：2，自引：0，他引：2  

蔡芗宁 《气象》2008,34(11):111-116

为更好地应用T639模式中期预报产品,对2008年6-8月T639 模式进行天气学检验,并与ECMWF、日本模式进行了对比分析.结果表明:3种模式均对亚洲中高纬环流形势的调整和演变具有较好的预报性能.综合来看,ECMWF模式对各系统及要素的预报最接近实况;日本模式和T639模式稍差,稳定性不如ECMWF模式;特别是T639模式对0808号台风凤凰(FUNG-WONG)路径及强度的预报与实况差异较大,而ECMWF及日本模式预报相对准确.  相似文献   

不同对流参数化方案和初值场组合对四川两次暴雨影响的数值模拟   总被引：6，自引：3，他引：3  

何光碧  曹杰 《高原气象》2008,27(4)

针对2004年9月2~6日四川盆地东北部一次持续性暴雨过程和2004年6月30日成都地区暴雨过程,利用MM5中尺度数值模式,进行了Grell、Kuo、KF及BM四种积云对流参数化方案与T213模式分析值及NCEP再分析值两种初始值组合的数值试验,分析了不同积云方案和初值组合的模拟性能。比较结果表明,MM5模式较好地再现了这两次强降水过程。在同一模式中,不同对流参数化方案和不同初值组合在降水落区和强度模拟上存在一定程度的差异。初步模拟表明NCEP资料模拟的降水强度较T213资料模拟的降水强度偏弱,但降水落区较T213资料模拟的更接近实况,T213资料模拟的降水空报现象较严重。以T213资料模拟得到的高度、温度场都较NCEP资料更有利于影响系统的加强,模拟的湿度场、散度场和垂直运动场都较NCEP资料更有利于强降水的发生。相对而言,NCEP资料模拟结果更接近实况,Kuo和Grell方案对初值表现出更为敏感。  相似文献   

T213数值预报产品在白银市盛夏中雨以上降水中的释用技术     

景怀玺  徐科展  石圆圆  白虎志 《干旱气象》2008,26(1):83-88

基于MICAPS系统,利用T213数值预报格点资料、预报关键区34个站点的高空资料以及市内4县区不同时次的本站气压和日降水量资料,通过分析白银市中雨以上降水的天气特征,归纳出中雨以上降水的天气形势,并据此进行客观定量化分型;选取对白银市中雨以上降水具有明显物理意义的消空指标和预报因子,利用PP数值释用方法,建立了白银市盛夏中雨以上降水的短期预报模型。对2007年6～8月进行试报,预报准确率平均达66.7%,预报效果较好。  相似文献   

T213L31全球模式云和对流参数化方案改进试验     

陈起英  李泽椿  管成功  佟华  王雨  Peter Bechtold 《气象学报》2009,67(2):227-240

针对中国业务中期数值预报模式T213对中雨量级以上的降水预报空报比较明显的问题,文中对此模式预报的降水进行了诊断分析。发现T213模式预报的总降水分布主要是由可分辨尺度降水决定的,且在降水偏多最明显的地区,可分辨尺度的降水即超过或达到了观测的总降水,表明降水空报的主要原因在于可分辨尺度降水偏多。可分辨尺度降水偏多的可能原因有：土壤湿度初始化、云变量的初始化和直接产生降水的云与对流参数化方案存在一定的缺陷。鉴于前两者是目前国际上的难点,文中针对第3个方面的可能原因进行了分析和相应的改进。包括在对流方案之前增加一次云方案的调用;对流参数化方案的闭合由“动力型”改为对流有效位能调整闭合;更复杂的对流触发机制;改进冰沉降和降水通量计算。改进的主要目的是使对流参数化方案更活跃,从而减少格点尺度对流的发生。采用改进的方案,进行了敏感性试验和2005年夏季的连续滚动同化预报试验,并与中国区域400个标准站的降水观测和GPCP的全球降水观测进行了比较。结果表明,改进的方案无论是对中国区域还是全球夏季平均的降水分布预报都好于业务,但四川省和赤道东太平洋降水偏多的问题依然存在。中国区域的降水统计检验还表明,除小雨外,其他量级在大部分时效上降水的TS评分增加,预报偏差降低。  相似文献   

2009年3—5月T639、ECMWF及日本模式的中期预报性能检验   总被引：2，自引：0，他引：2  

马杰  王蕾  秦宝国 《气象》2009,35(8):112-117

为更好地应用T639模式中期预报产品,对2009年3-5月T639模式进行天气学检验,并与ECMWF和日本模式进行了对比分析.结果表明:T639和ECMWF模式及日本模式预报性能均较好,相对地,ECMWF对中高纬大气环流的演变及850hPa温度有较强的预报能力.选取2009年4月23-25目的沙尘天气个例,T639模式对于引发此次沙尘天气的地面强风的中期预报指示意义最好,日本模式次之.  相似文献   

Effect of the chemical composition of the crust on the metamorphic evolution of orogenic wedges   总被引：4，自引：0，他引：4  

B. Goffé  R. Bousquet  P. Henry  X. Le Pichon 《Journal of Metamorphic Geology》2003,21(2):123-141

Petrological data provide a good record of the thermal structure of deeply eroded orogens, and, in principle, might be used to relate the metamorphic structure of an orogen to its deformational history. In this paper, we present two‐dimensional thermal modelling of various subduction models taking into account varying wedge geometry as well as variation of density and topography with metamorphic reactions. The models clearly show that rock type accreted in the wedge has important effects on the thermal regime of orogenic wedges. The thermal regime is dominated by radiogenic heat production. Material having high radioactive heat production, like the granodioritic upper crust, produces high temperature metamorphism (amphibolitic conditions). Material with low radioactive heat production results in low temperature metamorphism of greenschist or blueschist types depending on the thickness of the wedge. Application of this model to seemingly unrelated areas of the Central Alps (Lepontine Dome, Grisons) and Eastern Alps (Tauern Window) explains the coexistence and succession of distinct Barrovian and blueschist facies metamorphic conditions as the result of a single, continuous tectonic process in which the main difference is the composition of the incoming material in the orogenic wedge. Accretion of the European upper continental crust in the Lepontine and Tauern Domes produces Barrovian type metamorphism while accretion of oceanic sediments results in blueschist facies metamorphism in the Valaisan domain.  相似文献   

Contrasting metamorphic evolution of metasedimentary rocks from the Çine and Selimiye nappes in the Anatolide belt, western Turkey   总被引：1，自引：0，他引：1  

J. L. Régnier  U. Ring  C. W. Passchier  K. Gessner  T. Güngör 《Journal of Metamorphic Geology》2003,21(7):699-721

Abstract P–T conditions, mineral isograds, the relation of the latter to foliation planes and kinematic indicators are used to elucidate the tectonic nature and evolution of a shear zone in an orogen exhumed from mid‐crustal depths in western Turkey. Furthermore, we discuss whether simple monometamorphic fabrics of rock units from different nappes result from one single orogeny or are related to different orogenies. Metasedimentary rocks from the Çine and Selimiye nappes at the southern rim of the Anatolide belt of western Turkey record different metamorphic evolutions. The Eocene Selimiye shear zone separates both nappes. Metasedimentary rocks from the Çine nappe underneath the Selimiye shear zone record maximum P–T conditions of about 7 kbar and >550 °C. Metasedimentary rocks from the overlying Selimiye nappe have maximum P–T conditions of 4 kbar and c. 525 °C near the base of the nappe. Kinematic indicators in both nappes are related to movement on the Selimiye shear zone and consistently show a top‐S shear sense. Metamorphic grade in the Selimiye nappe decreases structurally upwards as indicated by mineral isograds defining the garnet‐chlorite zone at the base, the chloritoid‐biotite zone and the biotite‐chlorite zone at the top of the nappe. The mineral isograds in the Selimiye nappe run parallel to the regional S_R foliation, parallel the Selimiye shear zone and indicate that the Selimiye shear zone formed during this prograde greenschist to lower amphibolite facies metamorphic event but remained active after the peak of metamorphism. ⁴⁰Ar/³⁹Ar mica ages and the tectonometamorphic relationship with the Eocene Cyclades–Menderes thrust, which occurs above the Selimiye nappe in the study area, suggests an Eocene age of metamorphism in the Selimiye nappe. Metasedimentary rocks of the Çine nappe 20–30 km north of the Selimiye shear zone record maximum P–T conditions of 8–11 kbar and 600–650 °C. An age of about 550 Ma is indicated for amphibolite facies metamorphism and associated top‐N shear in the orthogneiss of the Çine nappe. Our study shows that simple monophase tectonometamorphic fabrics do not always indicate a simple orogenic development of a nappe stack. Preservation in some areas and complete overprinting of those fabrics in other areas apparently occur very heterogeneously.  相似文献   

Metamorphic petrology and zircon geochronology of high-grade rocks from the central Mozambique Belt of Tanzania: crustal recycling of Archean and Palaeoproterozoic material during the Pan-African orogeny   总被引：7，自引：0，他引：7  

H. Sommer  A. Kröner  C. Hauzenberger  S. Muhongo  M. T. D. Wingate 《Journal of Metamorphic Geology》2003,21(9):915-934

New data on the metamorphic petrology and zircon geochronology of high‐grade rocks in the central Mozambique Belt (MB) of Tanzania show that this part of the orogen consists of Archean and Palaeoproterozoic material that was structurally reworked during the Pan‐African event. The metamorphic rocks are characterized by a clockwise P–T path, followed by strong decompression, and the time of peak granulite facies metamorphism is similar to other granulite terranes in Tanzania. The predominant rock types are mafic to intermediate granulites, migmatites, granitoid orthogneisses and kyanite/sillimanite‐bearing metapelites. The meta‐granitoid rocks are of calc‐alkaline composition, range in age from late Archean to Neoproterozoic, and their protoliths were probably derived from magmatic arcs during collisional processes. Mafic to intermediate granulites consist of the mineral assemblage garnet–clinopyroxene–plagioclase–quartz–biotite–amphibole ± K‐feldspar ± orthopyroxene ± oxides. Metapelites are composed of garnet‐biotite‐plagioclase ± K‐feldspar ± kyanite/sillimanite ± oxides. Estimated values for peak granulite facies metamorphism are 12–13 kbar and 750–800 °C. Pressures of 5–8 kbar and temperatures of 550–700 °C characterize subsequent retrogression to amphibolite facies conditions. Evidence for a clockwise P–T path is provided by late growth of sillimanite after kyanite in metapelites. Zircon ages indicate that most of the central part of the MB in Tanzania consists of reworked ancient crust as shown by Archean (c. 2970–2500 Ma) and Palaeoproterozoic (c. 2124–1837 Ma) protolith ages. Metamorphic zircon from metapelites and granitoid orthogneisses yielded ages of c. 640 Ma which are considered to date peak regional granulite facies metamorphism during the Pan‐African orogenic event. However, the available zircon ages for the entire MB in East Africa and Madagascar also document that peak metamorphic conditions were reached at different times in different places. Large parts of the MB in central Tanzania consist of Archean and Palaeoproterozoic material that was reworked during the Pan‐African event and that may have been part of the Tanzania Craton and Usagaran domain farther to the west.  相似文献   

Peculiarities of the UV continuum energy distribution for T Tauri stars     

A. S. Kravtsova  S. A. Lamzin 《Astronomy Letters》2003,29(9):612-620

In the UV spectra of BP Tau, GW Ori, T Tau, and RY Tau obtained with the Hubble Space Telescope, we detected an inflection near 2000 Å in the F _λ ^c (λ) curve that describes the continuum energy distribution. The inflection probably stems from the fact that the UV continuum in these stars consists of two components: the emission from an optically thick gas with T<8000 K and the emission from a gas with a much higher temperature. The total luminosity of the hot component is much lower than that of the cool component, but the hot-gas radiation dominates at λ<1800 Å. Previously, other authors have drawn a similar conclusion for several young stars from low-resolution IUE spectra. However, we show that the short-wavelength continuum is determined from these spectra with large errors. We also show that, for three of the stars studied (BP Tau, GW Ori, and T Tau), the accretion-shock radiation cannot account for the observed dependence F _λ ^c (λ) in the ultraviolet. We argue that more than 90% of the emission continuum in BP Tau at λ>2000 Å originates not in the accretion shock but in the inner accretion disk. Previously, a similar conclusion was reached for six more classical T Tau stars. Therefore, we believe that the high-temperature continuum can be associated with the radiation from the disk chromosphere. However, it may well be that the stellar chromosphere is its source.  相似文献