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61.
This paper deals with the regional and structural framework of the Cretaceous rocks in the Afikpo Basin located in the southeastern part of the Lower Benue Trough. Results from regional tectonics are presented together with those of the microtectonic analysis of microfaults in the Owutu-Afikpo-Adadama area in the basin. The Owutu-Afikpo-Adadama ridge at the north-central part of the basin marks the boundary between the Late Cenomanian-Turonian-Conianian sediments and the Campanian-Maastrichtian sandstones. This ridge trends N45°E on average and is faulted in three main directions, namely: (1) N-S normal faults; (2) NE-SW strike-slip faults; and (3) NW-SE strike-slip faults. The faulted rocks along these brittle discontinuities are mainly cataclastics with internal fracture cleavage and sigmoidal quartz mosaics that are reminiscent of extensional deformation. The cataclasites often bear slickenside striations.  相似文献   
62.
Petrographic and geochemical analyses of three Cretaceous lithostratigraphic sandstone units were undertaken to constrain their provenance and tectonic setting. Petrographic analysis showed that there are differences in composition between the three sandstone bodies, which can be attributed to differences in provenance relief, transport distance and geology of the terrain. Composition of the three lithostratigraphic sandstone bodies fall within the craton interior field.
Framework mode and chemical features indicated their derivation from basaltic volcanics, source rocks during the early rifting stage, and felsic, intermediate and mafic igneous source rocks located at the southeast basement complex terrain, with minor sedimentary components from the uplifted and folded older Cretaceous strata.
The chemical composition of the sandstones is mainly related to source rocks, chemical weathering conditions and transport agents. The source rocks were derived mainly from the southeastern Precambrian basement of Nigeria. Through examination of the sandstones, the tectonic setting was modeled. The Benue Trough belongs to a continental sedimentary basin of the passive margin type.
The tectonic evolution from Albian to Maastrichtain of the trough is contributed to the difference in framework mode and chemical composition of the sandstones. The evolution of the basin was reconstructed in terms of sandstone petrology and geochemistry. The tectonic evolution can be subdivided into three stages from the petrology and geochemistry data. The first stage covers Albian; the second stage the Turonian-Coniacian, and the third stage the Campanian-Maastrichtain. These are the three mega discontinuities in the sandstone composition among these three stages. These three discontinuities signify the influence of tectonism.  相似文献   
63.
64.
Discrete Markov chain models (DMCs) have been widely applied to the study of regional income distribution dynamics and convergence. This popularity reflects the rich body of DMC theory on the one hand and the ability of this framework to provide insights on the internal and external properties of regional income distribution dynamics on the other. In this paper we examine the properties of tests for spatial effects in DMC models of regional distribution dynamics. We do so through a series of Monte Carlo simulations designed to examine the size, power and robustness of tests for spatial heterogeneity and spatial dependence in transitional dynamics. This requires that we specify a data generating process for not only the null, but also alternatives when spatial heterogeneity or spatial dependence is present in the transitional dynamics. We are not aware of any work which has examined these types of data generating processes in the spatial distribution dynamics literature. Results indicate that tests for spatial heterogeneity and spatial dependence display good power for the presence of spatial effects. However, tests for spatial heterogeneity are not robust to the presence of strong spatial dependence, while tests for spatial dependence are sensitive to the spatial configuration of heterogeneity. When the spatial configuration can be considered random, dependence tests are robust to the dynamic spatial heterogeneity, but not so to the process mean heterogeneity when the difference in process means is large relative to the variance of the time series.  相似文献   
65.
The burial metamorphism of the Andean geosynclinal deposits of Central Chile is studied. The stratigraphic units under consideration, Lower Jurassic to Upper Cretaceous and/or Lower Tertiary in age, have an accumulated thickness of 15,000 to 28,000 m, cover an area of nearly 2,500 km2, and consist predominantly of basic and acid lavas, ignimbrites and volcanic-clastic sediments, deposited in marine and continental environments. Unconformities break up the sequence into several stratigraphic-structural units.A specific burial metamorphic pattern, or series, characterizes each of the units. Each series consists of a succession of mineral assemblages, the metamorphic grade increasing downwards. The isograds are essentially parallel to the bedding planes. The grade range in each series covers different intervals between the zeolite and greenschist facies. Each unconformity corresponds to a mineralogie break in the alteration, higher grade assemblages generally overlying lower grade assemblages. The downward increase in metamorphic grade as well as the mineralogie breaks seem to be unrelated to the volcanic versus sedimentary character and to the continental versus marine depositional environment of the rocks.The repeated pattern of burial metamorphism between unconformities suggests a history consisting of several burial metamorphic episodes, each taking place prior to a folding period and leaving unaffected the underlying units, which were apparently sealed up by the previous episode. This mechanism provides an explaination for the presence of such low-grade burial metamorphic facies at the bottom of a stratigraphic column as thick as that of the Andean Geosyncline.
Zusammenfassung Die Auswirkungen der Versenkungsmetamorphose auf die Ablagerungen der andinen Geosynklinale in Mittel-Chile wurden untersucht. Die betrachteten stratigraphischen Einheiten, unterer Jura bis obere Kreide und/oder unteres Tertiär, haben eine kumulative Mächtigkeit von 15 000 bis 28 000 m; sie bedecken ein Gebiet von fast 2500 km2 und bestehen in der Hauptsache aus basischen und sauren Laven, Ignimbriten und vulkanoklastischen Sedimenten, die unter marinen und kontinentalen Bedingungen abgelagert wurden. Diskordanzen unterteilen die Abfolge in mehrere stratigraphisch-strukturelle Einheiten.Jede Einheit ist in einer besonderen, für die Versenkungsmetamorphose typischen Abfolge von Mineralgesellschaften geprägt. Der Grad der Metamorphose steigt mit zunehmender Tiefe. Die Isograden verlaufen im wesentlichen parallel zu den Schichtflächen. Die Bandbreite jeder der metamorphen Mineralgesellschaften bedeckt verschiedene Intervalle zwischen der Zeolith- und Grünschiefer-Fazies. Jeder Diskordanz entspricht auch ein Sprung in der mineralogischen Zusammensetzung, wobei die höhergradigen Mineralgesellschaften in der Regel die tiefergradigen überlagern. Der mit der Tiefe zunehmende Grad der Metamorphose und die Sprünge in der mineralogischen Zusammensetzung scheinen von dem vulkanischen bzw. sedimentären Charakter der Gesteine ebenso unabhängig zu sein wie von deren marinen bzw. kontinentalen Bildungsbedingungen.Die sich wiederholenden Muster der Versenkungsmetamorphose zwischen den Diskordanzen lassen vermuten, daß mehrere Metamorphosen stattfanden, wobei jede einzelne Umwandlung vor einer Faltungsperiode ablief und die unterlagernden Einheiten unverändert ließ, die anscheinend durch die vorangegangene Metamorphose versiegelt wurden. Dieser Mechanismus liefert eine Erklärung für die niedriggradigen Fazies der Versenkungsmetamorphose im Liegenden einer so mächtigen stratigraphischen Abfolge wie der der andinen Geosynklinale.

Resumen En este trabajo se describe el metamorfismo de sepultamiento en los depósitos del Geosinclinal Andino. Las unidades estratigráficas estudiadas son de edad jurásica inferior a cretácica superior y/o terciaria inferior, tienen un espesor acumulado de 15.000 a 28.000 m, cubren un area de aproximadamente 2.500 km2 y consisten predominantemente de lavas básicas y ácidas, ignimbritas y rocas sedimentario-volcánicas, depositadas en ambiente marino y continental.Cada una de las unidades estratigráficas está caracterizada por una serie metamórfica de sepultamiento específica. Cada serie consiste de una sucesión de asociaciones minerales con un grado de metamorfismo que aumenta hacia abajo. Las isogradas son esencialmente paralelas a los planos de estratificación. El rango de grado metamórfico de cada serie abarca diferentes intervalos entre las facies de zeolita y esquistos verdes. Cada discordancia corresponde a una discontinuidad mineralógica en la alteración en la que generalmente las asociaciones de mayor grado metamórfico cubren asociaciones de menor grado. El aumento de grado hacia abajo, lo mismo que las discontinuidades mineralógicas, parecen ser independientes tanto del carácter sedimentario o volcánico como del ambiente continental o marino de la depositación.La repetición de series metamórficas de sepultamiento entre discordancias, indica varios episodios metamórficos, cada uno de ellos anterior al plegamiento de la unidad afectada; al mismo tiempo, cada episodio metamórfico dejó sin afectar las unidades subyacentes, las que aparentemente habrían sido selladas por el episodio anterior.Este mecanismo explicaría la presencia de una facies metamórfica tan baja como la que existe en el fondo de una columna estratigráfica tan potente como la del Geosinclinal Andino.

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66.
We propose a method to remove the mass-sheet degeneracy that arises when the mass of galaxy clusters is inferred from gravitational shear. The method utilizes high-redshift standard candles that undergo weak lensing. Natural candidates for such standard candles are type Ia supernovae (SNe Ia).
When corrected with the light-curve shape (LCS), the peak magnitude of SNe Ia provides a standard candle with an uncertainty in apparent magnitude of Δ m ≃0.1–0.2. Gravitational magnification of a background SN Ia by an intervening cluster would cause a mismatch between the observed SN Ia peak magnitude compared with that expected from its LCS and redshift. The average detection rate for SNe Ia with a significant mismatch of ≥2Δ m behind a cluster at z ≃0.05–0.15 is about 1–2 supernovae per cluster per year at J , I , R ≲25–26.
Since SNe are point-like sources for a limited period, they can experience significant microlensing by massive compact halo objects (MACHOs) in the intracluster medium. Microlensing events caused by MACHOs of ∼10−4 M⊙ are expected to have time-scales similar to that of the SN light curve. Both the magnification curve by a MACHO and the light curve of a SN Ia have characteristic shapes that allow us to separate them. Microlensing events caused by MACHOs of smaller mass can unambiguously be identified in the SN light curve if the latter is continuously monitored. The average number of identifiable microlensing events per nearby cluster ( z ≲0.05) per year is ∼0.02 ( f /0.01), where f is the fraction of the cluster mass in MACHOs of masses 10−7< M macho/M⊙<10−4.  相似文献   
67.
The Thellier method for paleointensity determinations has been applied to prepared samples containing magnetites whose mean particle sizes range from single domain, SD, to multidomain, MD. Linear (ideal) PNRM-PTRM curves are obtained for samples containing SD and submicron magnetite particles. However, for MD particles non-linear (concave-up) PNRM-PTRM curves are observed such that a linear approximation to the lower blocking-temperature data leads to apparent paleointensities that are higher than the actual paleofield; however, the ratio of the end-points, NRM/TRM, yields the correct (laboratory) intensity. The non-linear (concave-up) PNRM-PTRM curves for the MD particles are explained in terms of the lack of symmetry of the domain-wall movements during the two heatings of the Thellier experiment. Low stabilities with respect to alternating fields and with respect to temperature cycles below magnetite's isotropic temperature are diagnostic in detecting samples most likely to exhibit non-linearities due to the MD effect.  相似文献   
68.
A study was made of the effect of low-temperature thermal fatigue on the generation of regular and irregular fractures in olivine-rich terrestrial rocks. The results appear to confirm the influence of thermal actions in the metamorphism of stony meteorites and lunar rocks.  相似文献   
69.
Felsenstein  Daniel  Elbaum  Eilat  Levi  Tsafrir  Calvo  Ran 《Natural Hazards》2021,105(1):21-45
Natural Hazards - Building damage probabilities are invaluable for assessing short-term losses from natural hazards. In many countries however, the individual building level data required for...  相似文献   
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