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11.
In 1991, a deep seismic reflection line, MPNI-9101, was acquired in the southern North Sea from the Mesozoic Broad Fourteens Basin, across the West Netherlands Basin onto the London-Brabant Massif (LBM). The resultant section shows a strongly reflective lower crust beneath the area of Mesozoic basin development. This lower crustal reflectivity continues to be strong beneath the LBM. The travel time to the base of the reflective zone increases from approximately 11.0 s beneath the Mesozoic basins to 12.5 s beneath the LBM, suggesting a southward thickening of the crust (Rijkers et al., 1993). Based on these travel times and information from deep wells and refraction surveys. Moho depth is estimated to increase from about 31 km beneath the Mesozoic basins to about 38 km beneath the LBM. This difference in depth to the Moho can partly be explained by coaxial stretching of the crust beneath the Mesozoic basins. In comparison with the Mesozoic basins, the crust beneath the LBM was thickened during the Caledonian and Variscan orogenies.  相似文献   
12.
Telecommunications Synchronization and GPS   总被引:1,自引:0,他引:1  
Today, the Global Positioning System (GPS) is the technology most frequently selected for use in digital communication networks to meet the requirement for precision timing synchronization. The technological evolution of the telecommunications industry over the past 30 years has driven this constantly growing demand for higher performance and timing accuracy. Increased timing accuracy provides overall improvements in system performance, quality, and efficiency. In the United States and in many parts of the world, the telecommunications infrastructure uses the GPS signal as an integral and basic part of the system. The stability of GPS, ongoing health of the GPS constellation, and GPS signal quality can mpact telecommunications systems. ? 2001 John Wiley & Sons, Inc.  相似文献   
13.
Ted Munn founded Boundary-Layer Meteorology in 1970 and served as Editor for 75 volumes over a 25 year period. This short article briefly reviews Ted's scientific career with the Atmospheric Environment Service (of Canada), the International Institute for Applied Systems Analysis in Austria and with the Institute of Environmental Studies at the University of Toronto, and as editor of this journal.  相似文献   
14.
Zusammenfassung Die vorliegende Studie befaßt sich mit den meteorologischen Vorgängen in einer extrem stabil aufgebauten Kaltluft, wie sie sich in Strahlungsnächten in einem abgeschlossenen Becken mit ebener, horizontaler Talsohle von einigen Kilometern Ausdehnung und im wesentlichen einheitlichem Untergrund einer Moorlandschaft herausbildet.Untersucht wird in erster Linie das Eigenleben der so abgeschlossenen Luftmasse. Dabei zeigt sich, daß der Zustand eines ruhenden Kaltluftsees zumeist erst im Endstadium des nächtlichen Prozesses näherungsweise erreicht wird. Während des größten Teiles der Nacht kommen vielmehr überraschend lebhafte und weitreichende angenähert horizontale Bewegungen leicht zustande, die sich im thermischen Gefüge wie in der Windstruktur kundtun und in dem Verhalten der Nebel- und Dunstfelder sichtbar werden. Unter der Wirkung von Schwerkraft, Druckgefälle und Reibung entstehen einfache Gleitvorgänge, Schaukelbewegungen, fortschreitende Wellen und Seiches, die in einzelnen Beispielen beschrieben werden. Ähnlich wie in der Großraummeteorologie bilden sich durch das quantenhafte Verhalten der Energieumsätze Luftkörperindividuen, deren Deformation hier einfacheren Gesetzen folgt. Trotz ihrer sehr verschiedenen Größenordnung von einigen Dekametern bis zu mehreren Kilometern Ausdehnung bei geringer vertikaler Mächtigkeit zeigen sie auf ihrer Vorderseite einheitlich die Form des vonW. Schmidt in Modellversuchen gefundenen Böenkopfes.Der Einfluß höherer Luftschichten auf die stabilisierte Bodenkaltluft äußert sich in aufgeprägten Wellen und Frendlufteinschüben. Das Beispiel eines nächtlichen Wärmeeinbruchs aus der Höhe wird eingehend beschrieben.
Summary The present study deals with the meteorological processes in an extremely stable cold air, formed in clear nights in a confined basin with a plane, horizontal basis extended for some kilometres, and with an essentially uniform ground in a fen-country.In the first place the proper life of the so limited air is studied. It becomes evident, that the state of a resting lake of cold air generally is approximately reached but in the final phase of the night-time process. Moreover, for the greater part of the night surprising active and extended movements of nearly horizontal course easily occur, becoming evident in the structure of wind and temperature stratification and also visible in the behaviour of fog and haze fields. Produced by gravitation, pressure gradient and friction, simple gliding and swinging motions, proceeding waves and seiches result which are described in single examples. Corresponding to the large scale meteorology individual air bodies form by the quantum-like behaviour of energy transformations. Their deformation in this case however, takes course according to simpler laws. In spite of their much various magnitude of the dimensions of some decametres up to several kilometres, while being of small vertical extension they show in their fore part in all cases the shape of a Böenkopf as found byW. Schmidt by model experiments.The influence of upper atmospheric layers on the stable cold air near the ground manifests itself by impressed waves and by influxes of heterogeneous air. An example of a nocturnal invasion of warm air from aloft is described in detail.

Résumé Cette étude traite des processus météorologiques dans un air froid d'une stratification extrêmement stable, qui se développent pendant des nuits claires dans un bassin fermé, ayant une base plane et horizontale, d'une étendue de quelques km, et recouverte par le sol essentiellement homogène d'une région marécageuse.C'est surtout la «vie propre» de cette masse d'air limitée qui est étudiée. Il se trouve que, le plus souvent, l'état d'un «lac immobile d'air froid» n'est atteint approximativement qu'à la fin du processus nocturne. Pendant la plus grande partie de la nuit, se produisent au contraire facilement des mouvements presque horizontaux étonnamment actifs et étendus, qui se manifestent dans la structure thermique et du vent, et qui deviennent visibles par le comportement des couches de brouillard et de brume. De simples processus de glissement, des oscillations, des ondes progressives et des seiches se forment sous l'influence de la gravitation, du gradient de pression et du frottement; ils sont décrits par des exemples particuliers. Comme cela se produit dans la météorologie à grande échelle, il se forme des corps atmosphériques individuels à la suite du comportement en quanta des transformations d'énergie. Leur déformation a lieu cependant selon des lois plus simples. En dépit de leur étendue très variable allant de quelques decamètres à plusieurs km, et leur épaisseur peu considérable, ils montrent tous à leur partie antérieure la forme d'un «Böenkopf», pareil à celui queW. Schmidt a trouvé à la suite de ses expériences qu'il fit avec des modèles.L'influence des couches supérieures de l'atmosphère sur l'air froid stable au sol se manifeste par l'impression d'ondes et par des apports d'air étranger. On décrit ensuite en détail une invasion nocturne d'air chaud depuis les couches supérieures.


Mit 13 Textabbildungen.

Herrn Prof. Dr.W. Peppler, zum 70. Geburtstag.  相似文献   
15.
Classifying very fine-grained rocks through fabric elements provides information about depositional environments, but is subject to the biases of visual taxonomy. To evaluate the statistical significance of an empirical classification of very fine-grained rocks, samples from Devonian shales in four cored wells in West Virginia and Virginia were measured for 15 variables: quartz, illite, pyrite and expandable clays determined by X-ray diffraction; total sulfur, organic content, inorganic carbon, matrix density, bulk density, porosity, silt, as well as density, sonic travel time, resistivity, and -ray response measured from well logs. The four lithologic types comprised: (1) sharply banded shale, (2) thinly laminated shale, (3) lenticularly laminated shale, and (4) nonbanded shale. Univariate and multivariate analyses of variance showed that the lithologic classification reflects significant differences for the variables measured, difference that can be detected independently of stratigraphic effects. Little-known statistical methods found useful in this work included: the multivariate analysis of variance with more than one effect, simultaneous plotting of samples and variables on canonical variates, and the use of parametric ANOVA and MANOVA on ranked data.  相似文献   
16.
The rough‐sea reflection‐response varies (1) along the streamer (2) from shot to shot and (3) with time along the seismic trace. The resulting error in seismic data can be important for time‐lapse imaging. One potential way of reducing the rough‐sea receiver error is to use conventional statistical deconvolution, but special care is needed in the choice of the design and application windows. The well‐known deconvolution problem associated with the non‐whiteness of the reflection series is exacerbated by the requirement of an unusually short design window – a requirement that is imposed by the non‐stationary nature of the rough‐sea receiver wavelet. For a synthetic rough‐sea data set, with a white 1D reflection series, the design window needs to be about 1000 ms long, with an application window about 400 ms long, centred within the design window. Although such a short design window allows the deconvolution operator to follow the time‐variation of the rough‐sea wavelet, it is likely to be too short to prevent the non‐whiteness of the geology from corrupting the operator when it is used on real data. If finely spatial‐sampled traces are available from the streamer, the design window can be extended to neighbouring traces, making use of the spatial correlations of the rough‐sea wavelet. For this ‘wave‐following’ approach to be fruitful, the wind (and hence the dominant wave direction) needs to be roughly along the line of the streamer.  相似文献   
17.
The Morro Velho gold deposit, Quadrilátero Ferrífero region, Minas Gerais, Brazil, is hosted by rocks at the base of the Archean Rio das Velhas greenstone belt. The deposit occurs within a thick carbonaceous phyllite package, containing intercalations of felsic and intermediate volcaniclastic rocks and dolomites. Considering the temporal and spatial association of the deposit with the Rio das Velhas orogeny, and location in close proximity to a major NNW-trending fault zone, it can be classified as an orogenic gold deposit. Hydrothermal activity was characterized by intense enrichment in alteration zones of carbonates, sulfides, chlorite, white mica±biotite, albite and quartz, as described in other Archean lode-type gold ores. Two types of ore occur in the deposit: dark gray quartz veins and sulfide-rich gold orebodies. The sulfide-rich orebodies range from disseminated concentrations of sulfide minerals to massive sulfide bodies. The sulfide assemblage comprises (by volume), on average, 74% pyrrhotite, 17% arsenopyrite, 8% pyrite and 1% chalcopyrite. The orebodies have a long axis parallel to the local stretching lineation, with continuity down the plunge of fold axis for at least 4.8 km. The group of rocks hosting the Morro Velho gold mineralization is locally referred to as lapa seca. These were isoclinally folded and metamorphosed prior to gold mineralization. The lapa seca and the orebodies it hosts are distributed in five main tight folds related to F1 (the best examples are the X, Main and South orebodies, in level 25), which are disrupted by NE- to E-striking shear zones. Textural features indicate that the sulfide mineralization postdated regional peak metamorphism, and that the massive sulfide ore has subsequently been neither metamorphosed nor deformed. Lead isotope ratios indicate a model age of 2.82 ± 0.05 Ga for both sulfide and gold mineralization. The lapa seca are interpreted as the results of a pre-gold alteration process and may be divided into carbonatic, micaceous and quartzose types. The carbonatic lapa seca is subdivided into gray and brown subtypes. Non-mineralized, gray carbonatic lapa seca forms the hanging wall to the orebodies, and is interpreted as the product of extreme CO2 metasomatism during hydrothermal alteration. This dolomitic lapa seca ranges in composition from relatively pure limestone and dolomite to silty limestone and dolomite. The brown carbonatic and micaceous lapa secas are the host rocks to gold. These units are interpreted to correspond to the sheared and hydrothermal products of metamorphosed volcaniclastic and/or volcanic rocks of varying composition from dacitic to andesitic, forming various types of schists and phyllites. The high-grade, massive sulfide orebodies occur at the base of the gray carbonatic lapa seca. Both disseminated mineralization and quartz veins are hosted by micaceous lapa seca. The data are consistent with a model of epigenetic mineralization for the lapa seca, from a hydrothermal fluid derived in part from the Archean basement or older crust material.  相似文献   
18.
Binary coefficients: A theoretical and empirical study   总被引:1,自引:0,他引:1  
Binary coefficients can be assigned to several categories on the basis of algebraic and conceptual properties. The phi coefficient of association is related algebraically to the chi-square statistic for 2-by-2 contingency tables, and use of this coefficient in cluster analysis permits the objective, nonarbitrary partitioning of objects among groups on the basis of previously selected levels of significant, positive association. Similarity, matching, and distance coefficients possess neither conceptual nor operational statistical meaning for many geological data sets. The weighted pair group method and flexible clustering strategy may give an overly conservative partitioning of objects among groups. Clustering by the unweighted pair group method, using the phi coefficient, is recommended for the analysis of biostratigraphic and paleoecologic presence—absence data.  相似文献   
19.
The Kabanga Ni sulfide deposit represents one of the most significant Ni sulfide discoveries of the last two decades, with current indicated mineral resources of 23.23 Mt at 2.64% Ni and inferred mineral resources of 28.5 Mt at 2.7% Ni (Nov. 2008). The sulfides are hosted by a suite of ∼1.4 Ga ultramafic–mafic, sill-like, and chonolithic intrusions that form part of the approximately 500 km long Kabanga–Musongati–Kapalagulu igneous belt in Tanzania and Burundi. The igneous bodies are up to about 1 km thick and 4 km long. They crystallized from several compositionally distinct magma pulses emplaced into sulfide-bearing pelitic schists. The first magma was a siliceous high-magnesium basalt (approximately 13.3% MgO) that formed a network of fine-grained acicular-textured gabbronoritic and orthopyroxenitic sills (Mg# opx 78–88, An plag 45–88). The magma was highly enriched in incompatible trace elements (LILE, LREE) and had pronounced negative Nb and Ta anomalies and heavy O isotopic signatures (δ18O +6 to +8). These compositional features are consistent with about 20% contamination of primitive picrite with the sulfidic pelitic schists. Subsequent magma pulses were more magnesian (approximately 14–15% MgO) and less contaminated (e.g., δ18O +5.1 to +6.6). They injected into the earlier sills, resulting in the formation of medium-grained harzburgites, olivine orthopyroxenites and orthopyroxenites (Fo 83–89, Mg# opx 86–89), and magmatic breccias consisting of gabbronorite–orthopyroxenite fragments within an olivine-rich matrix. All intrusions in the Kabanga area contain abundant sulfides (pyrrhotite, pentlandite, and minor chalcopyrite and pyrite). In the lower portions and the immediate footwall of two of the intrusions, namely Kabanga North and Kabanga Main, there occur numerous layers, lenses, and veins of massive Ni sulfides reaching a thickness of several meters. The largest amount of high grade, massive sulfide occurs in the smallest intrusion (Kabanga North). The sulfides have heavy S isotopic signatures (δ34S wr = +10 to +24) that broadly overlap with those of the country rock sulfides, consistent with significant assimilation of external sulfur from the Karagwe–Ankolean sedimentary sequence. However, based partly on the relatively homogenous distribution of disseminated sulfides in many of the intrusive rocks, we propose that the Kabanga magmas reached sulfide saturation prior to final emplacement, in staging chambers or feeder conduits, followed by entrainment of the sulfides during continued magma ascent. Oxygen isotope data indicate that the mode of sulfide assimilation changed with time. The heavy δ18O ratios of the early magmas are consistent with ingestion of the sedimentary country rocks in bulk. The relatively light δ18O ratios of the later magmas indicate less bulk assimilation of the country rocks, but in addition the magmas selectively assimilated additional S, possibly through devolatization of the country rocks or through cannibalization of magmatic sulfides deposited in the conduits by preceding magma surges. The intrusions were tilted at ca. 1.37 Ga, during the Kibaran orogeny and associated synkinematic granite plutonism. This caused solid-state mobilization of ductile sulfides into shear zones, notably along the base of the intrusions where sulfide-hornfels breccias and lenses and layers of massive sulfides may reach a thickness of >10 m and can extend for several 10 s to >100 m away from the intrusions. These horizons represent an important exploration target for additional nickel sulfide deposits.  相似文献   
20.
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