酿酒葡萄冻害原因的初步分析及防御对策   总被引：5，自引：0，他引：5  

常绪正张慧  康永义 《沙漠与绿洲气象(新疆气象)》2004,27(4):27-30

通过对酿酒葡萄冻害的调查研究分析指出：初霜冻的早晚和冬季的极端低温不是造成酿酒葡萄冻害的主要原因。品种间差异和栽培管理不同也不是造成酿酒葡萄冻害的主要原因，10月份的强降温、气温明显偏低(气温≤-5．2℃)才是酿酒葡萄树体冻害的主要原因。引种抗冻能力较强酿酒葡萄品种、选择适应的生长环境和掌握适宜的埋土时间，是防御酿酒葡萄冻害防御的主要对策。  相似文献   

1885~2000年长江中下游梅雨特征量的统计分析   总被引：22，自引：3，他引：22       下载免费PDF全文

魏凤英  张京江 《应用气象学报》2004,15(3):313-321

该文分析了1885~2000年长江中下游梅雨特征量的基本统计特征及其相互关系，在此基础上研究了梅雨较长时间尺度的变化特征。结果发现:①梅雨量的大小与梅雨期的长短和出梅日期的早晚为显著的正相关；②梅雨的主要周期为3 a、6 a和8 a，它们分别与低纬100 hPa高度场、热带系统以及全球陆地温度的变化有关；③控制入梅、出梅和梅雨期6 a左右周期的气候因素是相同的，而3 a左右的周期可能受到不同气候因素的影响；④长江中下游梅雨在近116年期间，经历了6个不同的气候阶段。  相似文献   

辽西地区中侏罗世海房沟组火山岩地球化学特征及其地质意义   总被引：4，自引：0，他引：4  

武广  李之彤  王文武 《岩石矿物学杂志》2004,23(2):97-108

辽西地区中侏罗世海房沟组火山岩的岩石共生组合为粗安岩粗面岩安山岩英安岩 ,属于高钾钙碱性钙碱性火山岩系 ,全岩Rb_Sr等时线年龄为 177.2± 2 8.0Ma。岩石总体上反映出高Al高Na特点 ,SiO2 ≥ 5 6 .99% ,Al2 O3 ≥ 15 .4 5 % ,Na2 O/K2 O≥ 1.35。稀土元素分馏明显 ,(La/Yb) N≥ 14 .80 ,(Ho/Yb) N≥ 1.15 ,贫Yb、Y(Yb≤ 1.4 2× 10 -6,Y≤ 15 .18× 10 -6) ,基本无Eu负异常 (0 .86～ 1.0 3) ,明显亏损Rb、Nb、Zr、Ti,而Sr、Ba、K及LREE富集 ,Rb/Sr值均小于 0 .1,地球化学特征与埃达克岩十分类似 ,属埃达克质岩。Sr、Pb和Nd同位素资料反映出这套火山岩的源岩较深 ,可能为古老的下地壳中基性变质岩部分熔融产物。研究表明 :海房沟组火山岩形成于板内环境 ,与太平洋板块俯冲没有直接关系 ;辽西地区中生代构造应力场的重大转换、广泛的岩浆活动和大规模断陷盆地群的形成与岩石圈拆沉作用密切相关。海房沟组埃达克质岩的确认对探讨辽西地区火山岩浆起源、壳幔相互作用及大陆动力学背景具有重要意义。  相似文献   

Petrology and Geochemistry of Early Cretaceous Bimodal Continental Flood Volcanism of the NW Etendeka, Namibia. Part 1: Introduction, Mafic Lavas and Re-evaluation of Mantle Source Components   总被引：9，自引：4，他引：9  

EWART  A.; MARSH  J. S.; MILNER  S. C.; DUNCAN  A. R.; KAMBER  B. S.; ARMSTRONG  R. A. 《Journal of Petrology》2004,45(1):59-105

The bimodal NW Etendeka province is located at the continentalend of the Tristan plume trace in coastal Namibia. It comprisesa high-Ti (Khumib type) and three low-Ti basalt (Tafelberg,Kuidas and Esmeralda types) suites, with, at stratigraphicallyhigher level, interstratified high-Ti latites (three units)and quartz latites (five units), and one low-Ti quartz latite.Khumib basalts are enriched in high field strength elementsand light rare earth elements relative to low-Ti types and exhibittrace element affinities with Tristan da Cunha lavas. The unradiogenic²⁰⁶Pb/²⁰⁴Pb ratios of Khumib basalts are distinctive, most plottingto the left of the 132 Ma Geochron, together with elevated ²⁰⁷Pb/²⁰⁴Pbratios, and Sr–Nd isotopic compositions plotting in thelower ¹⁴³Nd/¹⁴⁴Nd part of mantle array (EM1-like). The low-Tibasalts have less coherent trace element patterns and variable,radiogenic initial Sr (  相似文献   

Crustal Growth by Magmatic Accretion Constrained by Metamorphic P-T Paths and Thermal Models of the Kohistan Arc, NW Himalayas   总被引：2，自引：0，他引：2  

YOSHINO  TAKASHI; OKUDAIRA  TAKAMOTO 《Journal of Petrology》2004,45(11):2287-2302

Magmatic accretion is potentially an important mechanism inthe growth of the continental crust and the formation of granulites.In this study, the thermal evolution of a magmatic arc in responseto magmatic accretion is modeled using numerical solutions ofthe one-dimensional heat conduction equation. The initial andboundary conditions used in the model are constrained by geologicalobservations made in the Kohistan area, NW Himalayas. Takingconsideration of the preferred intrusion locations for basalticmagmas, we consider two plausible modes of magmatic accretion:the first involves the repeated intrusion of basalt at mid-crustaldepths (‘intraplate model’), and the second evaluatesthe simultaneous intrusion of basalt and picrite at mid-crustaldepths and the base of the crust respectively (‘double-platemodel’). The results of the double-plate model accountfor both the inferred metamorphic P–T paths of the Kohistanmafic granulites and the continental geotherm determined frompeak P–T conditions observed for granulite terranes. Thedouble-plate model may be applicable as a key growth processfor the production of thick mafic lower crust in magmatic arcs. KEY WORDS: thermal model; magmatic underplating; P–T path; granulite; lower crust  相似文献   

Gravity anomalies and associated tectonic features over the Indian Peninsular Shield and adjoining ocean basins     

D.C. Mishra  K. Arora  V.M. Tiwari 《Tectonophysics》2004,379(1-4):61-76

A combined gravity map over the Indian Peninsular Shield (IPS) and adjoining oceans brings out well the inter-relationships between the older tectonic features of the continent and the adjoining younger oceanic features. The NW–SE, NE–SW and N–S Precambrian trends of the IPS are reflected in the structural trends of the Arabian Sea and the Bay of Bengal suggesting their probable reactivation. The Simple Bouguer anomaly map shows consistent increase in gravity value from the continent to the deep ocean basins, which is attributed to isostatic compensation due to variations in the crustal thickness. A crustal density model computed along a profile across this region suggests a thick crust of 35–40 km under the continent, which reduces to 22/20–24 km under the Bay of Bengal with thick sediments of 8–10 km underlain by crustal layers of density 2720 and 2900/2840 kg/m³. Large crustal thickness and trends of the gravity anomalies may suggest a transitional crust in the Bay of Bengal up to 150–200 km from the east coast. The crustal thickness under the Laxmi ridge and east of it in the Arabian Sea is 20 and 14 km, respectively, with 5–6 km thick Tertiary and Mesozoic sediments separated by a thin layer of Deccan Trap. Crustal layers of densities 2750 and 2950 kg/m³ underlie sediments. The crustal density model in this part of the Arabian Sea (east of Laxmi ridge) and the structural trends similar to the Indian Peninsular Shield suggest a continent–ocean transitional crust (COTC). The COTC may represent down dropped and submerged parts of the Indian crust evolved at the time of break-up along the west coast of India and passage of Reunion hotspot over India during late Cretaceous. The crustal model under this part also shows an underplated lower crust and a low density upper mantle, extending over the continent across the west coast of India, which appears to be related to the Deccan volcanism. The crustal thickness under the western Arabian Sea (west of the Laxmi ridge) reduces to 8–9 km with crustal layers of densities 2650 and 2870 kg/m³ representing an oceanic crust.  相似文献   

Lu–Hf and U–Pb isotope systematics of zircons from the Storgangen intrusion, Rogaland Intrusive Complex, SW Norway: implications for the composition and evolution of Precambrian lower crust in the Baltic Shield     

Tom Andersen  William L Griffin   《Lithos》2004,73(3-4):271-288

The Storgangen orebody is a concordantly layered, sill-like body of ilmenite-rich norite, intruding anorthosites of the Rogaland Intrusive Complex (RIC), SW Norway. 17 zircon grains were separated from ca. 5 kg of sand-size flotation waste collected from the on-site repository from ilmenite mining. These zircons were analysed for major and trace elements by electron microprobe, and for U–Pb and Lu–Hf isotopes by laser ablation microprobe plasma source mass spectrometry. Eight of the zircons define a well-constrained (MSWD=0.37) concordant population with an age of 949±7 Ma, which is significantly older than the 920–930 Ma ages previously reported for zircon inclusions in orthopyroxene megacrysts from the RIC. The remaining zircons, interpreted as inherited grains, show a range of ²⁰⁷Pb/²⁰⁶Pb ages up to 1407±14 Ma, with an upper intercept age at ca. 1520 Ma. The concordant zircons have similar trace element patterns, and a mean initial Hf isotope composition of ¹⁷⁶Hf/¹⁷⁷Hf_{949 Ma}=0.28223±5 (_Hf=+2±2). This is similar to the Hf-isotope composition of zircons in a range of post-tectonic Sveconorwegian granites from South Norway, and slightly more radiogenic than expected for mid-Proterozoic juvenile crust. The older, inherited zircons show Lu–Hf crustal residence ages in the range 1.85–2.04 Ga. One (undated) zircon plots well within the field of Hf isotope evolution of Paleoproterozoic rocks of the Baltic Shield. These findings indicate the presence of Paleoproterozoic components in the deep crust of the Rogaland area, but do not demonstrate that such rocks, or a Sveconorwegian mantle-derived component, contributed significantly to the petrogenesis of the RIC. If the parent magma was derived from a homogeneous, lower crustal mafic granulite source, the lower crustal protolith must be at least 1.5 Ga old, and it must have an elevated Rb/Sr ratio. This component would be indistinguishable in Sr, Nd and Hf isotopes from some intermediate mixtures between Sveconorwegian mantle and Paleoprotoerzoic felsic crust, but it cannot account for the initial ¹⁴³Nd/¹⁴⁴Nd of the most primitive, late Sveconorwegian granite in the region, without the addition of mantle-derived material.  相似文献   

Pressure State in Deep Crust and Formation Depth of UHP Metamorphic Rocks     

Lü Guxian 《中国地质大学学报(英文版)》2004,15(2):135-144

INTRODUCTIONSincethediscoveryofeclogiteswithcoesiteanddia mondinclusionsrelatedtothecontinent continentcollision orogenyenvironment,theultrahigh pressuremetamorphism(UHPM )intheDabie Suluhasarousedgreatinterestinmanygeologists (Liouetal .,1994 ;Xuetal.,1992 ) .Experimentalstudieshaveprovedthatsuchmineralsasdia mond ,coesiteandomphaciteoccurredat 2 - 5GPa (andatthecorrespondingtemperatures) (Stevenetal.,1982 ;MirwaldandMasonne ,1980 ) .However,itdoesnotmeanthatthemetamorphicrockscanbe…  相似文献   

Granulite and pyroxenite xenoliths from the Deccan Trap: insight into the nature and composition of the lower lithosphere beneath cratonic India     

A.G. Dessai  A. Markwick  H. Downes 《Lithos》2004,78(3):263-290

Granulite and pyroxenite xenoliths in lamprophyre dykes intruded during the waning stage of Deccan Trap volcanism are derived from the lower crust beneath the Dharwar craton of Western India. The xenolith suite consists of plagioclase-poor mafic granulites (55% of the total volume of xenoliths), plagioclase-rich felsic granulites (25%), and ultramafic pyroxenites and websterites (20%) with subordinate wehrlites. Rare spinel peridotite xenoliths are also present, representing mantle lithosphere. The high Mg #, low SiO₂/Al₂O₃ and low Nb/La (<1) ratios suggest that the protoliths of the mafic granulites broadly represent cumulates of sub-alkaline magmas. All of the granulites are peraluminous and light rare-earth element-enriched. The felsic granulites may have resulted from anatexis of the mafic lower crustal rocks; thus, the mafic granulites are enriched in Sr whereas the felsic ones are depleted. Composite xenoliths consisting of mafic granulites traversed by veins of pyroxenite indicate intrusion of the granulitic lower crust by younger pyroxenites. Petrography and geochemistry of the latter (e.g. presence of phlogopite) indicate the metasomatised nature of the deep crust in this region.Thermobarometric estimates from phase equilibria indicate equilibration conditions between 650 and 1200 °C, 0.7-1.2 GPa suggestive of lower crustal environments. These estimates provide a spatial context for the sampled lithologies thereby placing constraints on the interpretation of geophysical data. Integration of xenolith-derived P-T results with Deep Seismic Soundings (DSS) data suggests that the pyroxenites and websterites are transitional between the lower crust and the upper mantle. A three-layer model for the crust in western India, derived from the xenoliths, is consistent with DSS data. The mafic nature of this hybrid lower crust contrasts with the felsic lower crustal composition of the south Indian granulite terrain.  相似文献   

Geometry of extensional faults developed at slow-spreading centres from pre-stack depth migration of seismic reflection data in the Central Atlantic (Canary Basin)     

T. J. Reston  C. R. Ranero  O. Ruoff  M. Perez-Gussinye  J. J. Dañobeitia 《Geophysical Journal International》2004,159(2):591-606

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