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41.
Four magma series are distinguished in the northeastern TroodosExtrusive Series: (A) a Lower Low-Ti Series (Lo-LTS) of basalticandesites, (B) a High-Ti Series (HTS) of basaltic andesitesto rhyodacites, (C) a Low-Ti Series(DLTS), the last two beingof basaltic andesite. Trace-element characteristics vary systematicallyfrom Series A to D and are interpreted in terms of a variablecontribution of three major source components (SCs). LILE-enrichedwater-rich fluids (SCI) derived from dehydration of a subductedlithosphere slab were continuously added to the overlying mantlewedge. Increasing LILE/HFSE and LILE/REE ratios and decreasingabsolute HFSE and REE concentrations from Series A to Dindicateprogressive depletion of the actual mantle source (SCII). Anegative Ta anomaly in the lavas decreases from Series A toD and is interpreted to have resulted from partial melting ofthe lower crust (SCII) where Ta-Nb-Ti may be fractionated byTi-rich accessory phases. The contribution of SCIII decreaseswhen the eruptive sites successively move away from the centralaxial zone and the temperature of the lower crust decreases,preventing partial melting of the lower crust. Chemical compositionsof fresh glass separates and phenocrysts indicate a change ofmajor petrogenetic processes from series A to D. Lo-LTS andIITS lavas are intrepreted to be directly related by open-systemfractional crystallization in crustal magma chambers. Removalof observed phenocryst phases clinopyroxene, orthopyroxene,plagioclase, and magnetite, and repeated subsequent mixing ofdacitc to rhyodacitic magmas with batches of replenshing basalticandesites are the major processes, possibly induced by vesicleformation in the mafic layer after a period of some crystallization.LTS and DLTS magmas were directly fed to the surface withoutstagnating at crustal levels, with feeder dykes positioned marginalto the central rift zone and thus by-passing the central magmachambers. These magmas apparently experienced only limited fractionalcrystallization of 10–15 wt.% olivine+clinopyroxene+chromite,probably at the mantle-crust boundary.  相似文献   
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寒武纪早期是地球海洋环境与生命演化的关键时期,但目前扬子东南缘深水相区的早寒武纪地层尚缺乏系统、精确 的地层对比工作。该文选取湖南省怀化地区会同钻孔剖面(深水相区) 的留茶坡组硅质岩、小烟溪组黑色页岩为研究对 象,进行了高分辨的有机碳同位素(δ13Corg) 地层对比,结果在会同剖面自下而上识别出四个正漂移(P1、P2、P3和P4) 与两个负漂移(N1和N2),结合其他剖面的生物化石记录和锆石U-Pb年龄资料,将会同剖面有机碳同位素与湖南其他 剖面,以及和云南和三峡等地浅水相区剖面的有机碳、无机碳同位素曲线进行对比,认为扬子东南缘埃迪卡拉系-寒武 系界线在湖南深水相区可放置于留茶坡组上部较大的有机碳同位素负漂移(Basal Cambrian Carbon isotope Excursion, BACE) 出现的位置,但由于钻孔深度不够,所以该负漂移未在会同剖面获得,而P1、P2和P3分别对应于寒武系的ZHUCE (ZHUjiaqing Carbon isotope Excursion,第二阶)、CARE (Cambrian Arthropod Radiation isotope Excursion,第三阶) 和MICE(MIngxinsi Carbon Isotope Excursion,第四阶) 正漂移,N1 和N2 分别对应于寒武系的SHICE (SHIyantou Carbon isotope Excursion,第二阶) 和AECE(Archaeocyathid Extinction Carbon isotope Excursion,第四阶) 负漂移,因此会同剖面留茶坡组顶部至小烟溪组底部属于寒武系第二阶,小烟溪组下部属于寒武系第三阶,而小烟溪组中-上部属于寒武系第四阶,而顶 部是否达到第四阶顶部尚无法确认。碳同位素的负漂移可能是海侵时期上升流水体将底层富含12C还原水体带至浅水地区所 致,并分别与埃迪卡拉动物群、小壳化石动物群和古杯动物的灭绝密切相关;而在生物繁盛时期,海洋初级生产力升高, 有机质埋藏增加,导致碳同位素的正漂移。  相似文献   
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Abstract

This paper presents an expert system to help select the best method to estimate design flood flows for civil engineering works based upon the procedures available, the nature and characteristics of the basin and existing hydrological records. The system presents the user with a list of possible methods ranked in descending grade order and optionally presents explanations which support the selected choices. Ordering is achieved using the knowledge base provided by the expert. The system recommends procedures for both preliminary estimates and final designs. The system also constitutes a valuable aid for junior engineers and experienced hydrologists in the selection of methods. Its conceptual structure can be easily generalized to treat other problems of a similar nature in the field of hydrology and water resources.  相似文献   
46.
Approximately 30% of the land surface is arid, having desert or semi-desert conditions. Aerosol originating from these regions plays a significant role in climate and atmospheric chemistry of the atmosphere. Retrieving aerosol properties from space-borne platforms above desert conditions, where the surface reflectance is usually very bright, is a challenging task. The proportion of the surface to top of atmosphere (TOA) reflectance can reach values over 90%, especially for wavelength above 500 nm. For these reasons detailed knowledge of aerosol and surface optical properties from these regions is required to separate atmosphere from intrinsically bright surfaces.
An approach to retrieve aerosol properties over arid and semi-arid regions based on the Bremen Aerosol Retrieval (BAER) has been developed and validated within the Dust Aerosol Retrievals from Space-Born Instruments (DREAMS) Project, which is part of the Saharan Mineral Dust Experiment ( SAMUM, 2006 ). Combining measurements of the backscattered radiation from the Medium Resolution Imaging Spectrometer (MERIS) instrument aboard Environmental Satellite (ENVISAT) and ground-based measurements in Morocco in radiation closure experiments yields the aerosol optical properties of mineral dust at selected locations.  相似文献   
47.
The present study examines sedimentation rates in the eastern Gotland Basin using a variety of methods that reveal considerable heterogeneity in the rates, both spatially and temporally. High-resolution seismic recordings and correlation with long sediment cores indicate increased thickness of strata and higher sedimentation rates (0.75 mm a -1 ) in the eastern part of the basin than in the western part (0.23 mm a -1 ) since the Littorina transgression some 8000 14 C years BP. This difference is apparently a consequence of a counterclockwise near-bottom circulation in the basin with periodically high current speeds that cause winnowing on the steep SE slope of the basin and differential settling of sediments in areas of low current speeds. On shorter time scales, recent sediment accumulation rates based on radiometric dating ( 210 Pb) are in general twice as high as those observed 25 years ago using the same method. The higher modern rates, compared to those of the 1970s, may partly be due to increased eutrophication, as more carbon is buried in the sediment, and partly due to increased erosion in shallow water areas. However, strong lateral variations are evident. The average sediment accumulation rates vary between 119 and 340 g m -2 a -1 (corresponding to sedimentation rates of 2.1-2.5 mm a -1 ) in the deepest part of the basin. Very high rates (6100 g m -2 a -1 , corresponding to sedimentation rates of 30 mm a -1 ) are observed on an intraslope basin site (offshore Latvia) at a water depth of only 70 m. The radiometrically determined sediment accumulation rates are up to three times higher than those estimated from average water column concentrations of suspended matter and from sediment trap flux rates. The discrepancy suggests that sedimentation in the deep basin may have a substantial contribution from near-bottom lateral transport.  相似文献   
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MEIN  P.  MEIN  N.  MALHERBE  J.-M.  HEINZEL  P.  KNEER  F.  VON UEXKULL  M.  STAIGER  J. 《Solar physics》1997,172(1-2):161-170
A small flare was observed at the Teide Observatory on October 5, 1994. Simultaneous data were obtained at the German Vacuum Tower Telescope (VTT) with the MSDP spectrograph providing high-resolution imaging spectroscopy in two chromospheric lines, and the Gregory Coudé Telescope (GCT) providing information about the magnetic field. Basic flare characteristics are:The area of the flare kernel ( 2 x 2 arc sec) is similar in H and Caii 8542 Å.The early phase of the flare is characterized by a blue asymmetry in H and a red one in Caii 8542 Å line.The evolutions of line profiles are different; the red asymmetry observed in the Caii line is detected a few seconds later in H.The maximum asymmetry of the Caii line does not coincide with the maximum brightness.The flare occurs in a region of a strong horizontal gradient of the line-of-sight component of the magnetic field.Brightness and asymmetry in H and Caii are discussed in the context of standard flare models and velocity fields. Our observations suggest that a magnetic reconnection could occur at low levels of the solar atmosphere.  相似文献   
50.
Geological significance of Coorong dolomites   总被引:2,自引:0,他引:2  
Microcrystalline dolomite and related carbonate minerals have been forming throughout the Quaternary in shallow ephemeral alkaline lakes on the coastal plain of the Coorong area in southern Australia. These Coorong dolomites differ significantly from sabkha-type dolomites. They form in areas where evaporation rates during summer months exceed groundwater inflow rates to a series of alkaline lakes. This results in the lakes becoming desiccated during summer months. Brines resulting from this drying phase are then refluxed out of the system into seaward-flowing groundwaters of an unconfined coastal aquifer. Dolomites and other fine-grained carbonates remain behind, whilst saline and sulphate evaporite minerals are flushed out of the system. Progressive restriction by sedimentation in and around the Holocene coastal dolomite lakes results in an upward-shoaling sedimentary cycle. Basal sediments which formed in a restricted marine environment pass upwards to lacustrine dolomites or magnesites exhibiting desiccation and groundwater resurgence structures such as mudcracks and teepees. The upper Proterozoic Skillogallee Dolomite Formation, an early rift basin unit of the Adelaide Supergroup, contains dolomites which show many of the features characteristic of the peculiar groundwater hydrology which plays an important role in Coorong dolomite genesis. These features include aphanitic dolomites which lack relict saline or sulphate evaporite minerals. The Skillogallee Dolomite Formation in some areas overlies an earlier dolomitic unit, informally named the Callanna Beds, typified by abundant pseudomorphs after sulphate minerals. Sabkha style dolomites characterizing the Callanna Beds are replaced up-section by the Coorong-type dolomite of the Skillogallee Dolomite Formation. This implies the development of an increasingly more active groundwater regime. The ultimate source and mode of concentration of the necessary Mg required to form both the modern and ancient dolomites remain imperfectly understood.  相似文献   
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