南通地区新构造运动特征   总被引：4，自引：0，他引：4  

范迪富  徐雪球 《江苏地质》2002,26(1):7-12

从盆地沉积及其演变特征入手，总结了该区新构造运动特征；运用新构造运动理论对海岸线的变迁、长江的迁移及旋扭变形现象进行了探讨，并提出建立第四系各年代的地层沉降速率数学模型、用升降运动速率划分和对比第四纪地层的见解。  相似文献   

Fall vs flow activity during the 1991 climactic eruption of Pinatubo Volcano (Philippines)     

M. Rosi  M. Paladio-Melosantos  A. Di Muro  R. Leoni  T. Bacolcol 《Bulletin of Volcanology》2001,62(8):549-566

Six years after the 1991 Mt. Pinatubo eruption, deep erosion incisions into the pyroclastic deposits accumulated around the volcano enabled us to investigate the stratigraphy of the climactic deposits both in valley bottoms and on contiguous ridges. Stratigraphic relationships between fall, flow, and surge deposits in the Marella drainage system indicate that during the climactic eruption a progressive shift occurred from an early convective regime, to a transitional regime feeding both the plinian convective column and mostly dilute density currents, to a fully collapsing regime producing mostly dense pyroclastic flows. Syn-plinian dilute density currents (surges) propagated up to ~10 km from the crater, both along valley bottoms and on contiguous ridges of the Marella Valley, whereas post-plinian pyroclastic flows had greater runout (~13 km), were confined to valleys and were not associated with significant surges. Stratigraphic study and grain-size analyses allow the identification of three types of intra-plinian deposits: (a) lower and often coarse-grained surge deposits, emplaced during the accumulation of the coarsest portion of the fallout bed at time intervals of ~16-24 min; (b) upper fine-grained surge deposits, interstratified with the fine-grained portion of the fall bed and emplaced at shorter time intervals of ~3-13 min; and (c) small-volume, channel-confined, massive pumiceous flow deposits interbedded with the upper surges in the upper fine-grained fall bed. Maximum clast size isopleths of 1.6 and 0.8 cm for lithics (ML) and 2.0 and 4.0 cm for pumices (MP) show almost symmetrical distribution around the vent, indicating that the passing of the typhoon Yunya during the climactic eruption had little effect on trajectories of high-Reynold-number clasts. Significant distortion was, however, observed for the 3.2-cm ML and 6.0-cm MP proximal isopleths, whose patterns were probably influenced by the interaction of the clasts falling from column margins with the uprising co-ignimbrite ash plumes. Application of the Carey and Sparks (1986) model to the undisturbed isopleths generated by the umbrella cloud yields a maximum column height of ~42 km, in good agreement with satellite measurements. Systematic stratigraphic and vertical grain-size studies of the plinian fall deposit in the Marella Valley, combined with satellite data and eyewitness accounts, reveal that the carrying capacity of the convective column and related fallout activity peaked in the early phase of the eruption, beginning slightly before 13:41 and gradually declined until its cessation 3 h later. Most of the pumiceous pyroclastic flow deposits were emplaced after the end of the fallout activity at ~16:30 but before the summit caldera collapse at approximately 19:11. Only a small volume of pumiceous flow deposits accumulated after the final caldera collapse. In contrast to the previous reconstruction of Holasek et al. (1996), which interpreted the progressive lowering of the column, documented by satellite data, as due to a decreasing mass eruption rate, we suggest that a progressive shift from a plinian column to a large co-ignimbrite column could also account for such a variation.  相似文献   

MAPGIS下重磁数据直接成图的实现及意义   总被引：3，自引：4，他引：3  

敖文波  周蒂  胡光道 《物探化探计算技术》2001,23(3):281-285

作者在文中介绍了通过编制QBASIC小程序实现两种常见格式重磁数据直接生成MAPGIS图形文件的方法，为其它类似格式数据在MAPGIS下成图及建库提供可借鉴的思路和途径。  相似文献   

基于计算机视觉的专题图读取系统     

林宗坚  卢健  邸凯昌 《武汉大学学报(信息科学版)》1992,(2)

本文提出了一种基于计算机视觉的专题图读取系统方案。该系统用CCD相机获取专题图影象,通过线划跟踪、弧段矢量化、拓扑结构形成、数据压缩、几何纠正与拼接等步骤,实现专题图的自动读取,继而进行各种几何量算和统计,建立专题信息库  相似文献   

关于火山岩型铀矿床成矿规律中一些问题的讨论   总被引：5，自引：2，他引：5  

俞时清  邸瑞姞 《铀矿地质》1993,(2)

火山岩型铀矿常位于大的地质构造单元界线附近,特别是稳定区与活动区之间的过渡带上。矿区的基底不仅需有较高的成熟度而且是在火山岩形成前或长期处于隆起状态者。负向火山构造,上叠式或拗凸型上叠式火盆是铀矿田的有利构造形式。红盆对成矿的作用不是古气候方面的而是构造方面的。火山岩型铀矿成矿深度可以较大,而且在垂向上不只一个富集高峰。铀及其主要伴生组份不是来源于赋矿围岩,而是来自基底或更深处。  相似文献   

Analysis of the vortivity and divergence of the thermal wind in pure geostrophic flow     

Felice Di Benedetto 《Meteorology and Atmospheric Physics》1957,10(1):20-28

By applying the horizontal del operator to the thermal wind equation in vectorial form and considering only horizontal geostrophic motion, expressions are found for the vorticity and divergence of thermal wind. It is shown that vorticity, in the case of pure geostrophic flow at all levels, depends upon four factors, namely: latitude, horizontal distribution of temperature, temperature lapse rate and divergence of horizontal temperature gradient. The divergence of the thermal wind, on the other hand, depends only upon the orientation of the mean isotherms of an isobaric layer relative to the parallel circles. These terms are evaluated and it is shown that the latitude term and the lapse rate term are far greater than the remaining terms of the vorticity equation for geostrophic flow. A criterion is then given which enables to determine the conditions for irrotational horizontal motion with vertical geostrophic wind shear.

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Zusammenfassung Durch Anwendung des horizontalenNabla-Operators auf die thermische Windgleichung in vektorieller Form und bei ausschließlicher Berücksichtigung der geostrophischen Horizontalbewegung lassen sich Ausdrücke für die vorticity und die Divergenz des thermischen Windes herleiten. Es wird gezeigt, daß die vorticity im Falle einer rein geostrophischen Strömung in allen Niveaus von folgenden vier Faktoren bedingt ist: Breite, horizontale Temperaturverteilung, vertikaler Temperaturgradient und Divergenz des horizontalen Temperaturgradienten. Andrerseits hängt die Divergenz des thermischen Windes nur von der Orientierung der mittleren Isothermen einer in Bezug auf die Parallelkreise isobaren Schicht ab. Diese vier Terme werden ausgewertet und es wird gezeigt, daß das Breitenglied und der Term für den Vertikalgradienten viel größer sind als die übrigen Terme der vorticity-Gleichung für geostrophische Strömung. Schließlich wird ein Kriterium entwickelt, das gestattet, die Bedingungen für rotorfreie Horizontalbewegung mit vertikaler geostrophischer Windscherung zu bestimmen.

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Résumé On peut déduire des équations sur la rotationelle et la divergence du vent thermique en appliquant l'opérateur nabla horizontal à l'équation du vent thermique sous une forme vectorielle et en ne considérant que le mouvement géostrophique horizontal. On démontre que la rotationelle, dans le cas d'un courant géostrophique pur, dépend dans tous les niveaux des quatre facteurs suivants: latitude, répartition horizontale de la température, gradient vertical de la température et divergence du gradient horizontal de température. D'autre part, la divergence du vent thermique ne dépend que de l'orientation des isothermes moyennes d'une couche isobare par rapport aux parallèles. En évaluant ces quatre termes, on montre que les termes relatifs à la latitude et au gradient vertical sont beaucoup plus grands que les autres termes de l'équation de la rotationelle pour un courant géostrophique. Pour terminer, l'auteur développe un critère qui permet de déterminer les conditions pour un mouvement horizontal irrotationel mais avec un cisaillement vertical géostrophique du vent.

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The Ethiopian Rift Valley (between 7° 00′ and 8° 40′ lat. north)     

G. M. Di Paola 《Bulletin of Volcanology》1972,36(4):517-560

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Analysing Lava Risk for the Etnean Area: Simulation by Cellular Automata Methods     

Crisci  G. M.  Di Gregorio  S.  Rongo  R.  Spataro  W.  Nicoletta  F. 《Natural Hazards》1999,20(2-3):215-229

The model SCIARA, based on the Cellular Automata paradigm, is a versatile instrument whose scope is to analyse volcanic risk from lava flows.The possible fields of intervention are:[(a)] Long term forecasting of the flow direction at various eruption rates and points of emission by locating potential risk areas and permitting the creation of detailed maps of risk;[(b)] The possibility to follow the progress of an event and predict its evolution;[(c)] The verification of the possible effects of human intervention on real or simulated flows in stream deviation.A risk scenario has been developed for the Etnean territories of the towns of Nicolosi, Pedara and S. Alfio, simulating possible episodes with different vent locations along the fracture opened in the 1989 eruption and successively activated in the 1991–1993 eruption.The main characteristics of lava flows, that might be dangerous to the inhabited areas, have been analysed on the basis of the carried out Cellular Automata.  相似文献   

Short Term and Short Range Seismicity Patterns in Different Seismic Areas of the World     

R. Console  F. Di Luccio  M. Murru  M. Imoto  G. Stavrakakis 《Natural Hazards》1999,19(2-3):107-121

The aim of this work is to quantitatively set up a simple hypothesis for occurrence of earthquakes conditioned by prior events, on the basis of a previously existing model and the use of recent instrumental observations. A simple procedure is presented in order to determine the conditional probability of pairs of events (foreshock-mainshock, mainshock-aftershock) with short time and space separation. The first event of a pair should not be an aftershock, i.e., it must not be related to a stronger previous event. The Italian earthquake catalog of the Istituto Nazionale di Geofisica (ING) (1975–1995, M 3.4), the earthquake catalog of the Japan Meteorological Agency (JMA) (1983–1994, M 3.0) and that of the National Observatory of Athens (NOA) (1982–1994, M 3.8) were analyzed. The number of observed pairs depends on several parameters: the size of the space-time quiescence volume defining nonaftershocks, the inter event time, the minimum magnitude of the two events, and the spatial dimension of the alarm volume after the first event. The Akaike information criterion has been adopted to assess the optimum set of space-time parameters used in the definition of the pairs, assuming that the occurrence rate of subsequent events may be modeled by two Poisson processes with different rates: the higher rate refers to the space-time volume defined by the alarms and the lower one simulates earthquakes that occur in the nonalarm space-time volume. On the basis of the tests carried out on the seismic catalog of Italy, the occurrence rate of M 3.8 earthquakes followed by a M 3.8 mainshock within 10 km and 10 days (validity) is 0.459. We have observed, for all three catalogs, that the occurrence rate density for the second event of a couple (mainshock or aftershock) of magnitude M₂ subsequent to a nonaftershock of magnitude M₁ in the time range T can be modeled by the following relationship: (T, M₂) = 10^{a + b(M1 - M2)} with b varying from 0.74 (Japan) to 1.09 (Greece). The decrease of the occurrence rate in time for a mainshock after a foreshock or for large aftershocks after a mainshock, for all three databases, obeys the Omori's law with p changing from 0.94 (Italy) to 2.0 (Greece).  相似文献   

Mantle source heterogeneity in the Campanian Region (South Italy) as inferred from geochemical and isotopic features of mafic volcanic rocks with shoshonitic affinity   总被引：6，自引：0，他引：6  

M. D'Antonio  L. Civetta  P. Di Girolamo 《Mineralogy and Petrology》1999,67(3-4):163-192

Summary Major, trace element and Sr-Nd-isotopic data on mafic volcanic rocks with shoshonitic affinity from the islands of Procida and Ventotene (Campanian Region, South Italy) are reported. Within-suite chemical and isotopic variations are interpreted in terms of open system differentiation processes held responsible for enrichment in a number of trace elements and for radiogenic Sr observed in both Procida and Ventotene volcanic sequences. Conversely, trace element contents and Sr-Nd-isotopic compositions of the least-evolved among the investigated samples are thought to reflect source region characteristics with only negligible crustal contamination of the primary magmas.The data support an origin from distinct source regions for the primary magmas. In the case of Ventotene, the source would have been asthenospheric and/or lithospheric mantle with features similar to transitional mid-ocean ridge basalts (T-MORB), modified by enriching agents made up mainly of subducted slab-released components coming from marly sediments (about 7%) similar to cherts from Tuscan Apennines plus a limestone contribution. In the case of Procida, the source would have been asthenospheric and/or lithospheric mantle with a slightly more enriched T-MORB-like feature with respect to Ventotene, modified by slab-derived enriching agents, likely represented by a small amount of sediments (about 2.5%) of oceanic nature (mostly terrigenous/pelagic). These differences are constrained by lower Zr/Nb, Y/Nb, Sc/Nb, V/Nb, LILE/HFSE, LREE/HFSE and⁸⁷Sr/⁸⁶Sr, higher Ba/La and¹⁴³Nd/¹⁴⁴Nd ratios, as well as by the lack of a detectable negative Eu anomaly, in the least-evolved volcanic rocks of Procida, with respect to those of Ventotene, which show conversely a significant negative Eu anomaly. Thus, a sharp heterogeneity exists in the mantle beneath the Campanian Region. It is thought to be the consequence of two different slabs which are in contact along the Volturno River Plain tectonic line: a continental slab, seismically inactive, descending beneath the Latium Region, and an oceanic slab, seismically active, descending beneath the Calabria, up to the Campanian Region.

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Résumé De nouvelles analyses géochimiques d'éléments majeurs et en traces ainsi que des rapports isotopiques du Sr et du Nd sont été obtenues sur des roches volcaniques mafiques à affinité shoshonitiques provenant des îles de Procida et Ventotene (Région Campanienne, Italie du Sud). Les variations géochimiques et isotopiques observées au sein des séries volcaniques de ces deux îles sont interprétées en terme de processus de différenciation en système ouvert, tenu pour responsable d'un enrichissement d'un certain nombre d'éléments en traces et de leur composition en Sr radiogénique. Cependant, les teneurs en éléments traces et les compositions isotopiques en Sr et Nd des échantillons les moins évolués parmi ceux étudiés reflètent les caractéristiques de leur source, avec une contamination crustale très négligeable des magmas primitifs.Ces données démontrent que des sources distinctes sont à l'origine des magmas primitifs. Pour Ventotene, cette source doit être un manteau asthénosphérique et/ou lithosphérique dont la signature est similaire à celle de basaltes transitionnels de dorsale océanique (T MORB), légèrement enrichie en éléments dérivants d'une croûte plongeant dans une subduction comme des sédiments mameux (pour environ 7%) analogues aux cherts des Appenins de Toscane et comportant un apport en calcaire. Dans le cas de Procida, cette source doit être un manteau asthénosphérique et/ou lithosphérique montrant une signature de type T-MORB légèrement plus enrichie qu' à Ventotene, également modifiée par un apport venant d'une croûte en subduction, probablement une faible quantité (environ 2.5%) de sédiments de nature océanique (principalement terrigène/pélagique). Ces différences sont attestées par des rapports Zr/Nb, Y/Nb, Sc/Nb, V/Nb, LILE/HFSE, LREE/HSFE and⁸⁷Sr/⁸⁶Sr plus bas et des rapports Ba/La et¹⁴³Nd/¹⁴⁴Nd plus harts, ainsi que par l'absence d'une anomalie en Eu dans les compositions des roches volcaniques les moins évoluées de Procida par rapport à celles de Ventotene, qui elles, au contraire, montrent une anomalie en Eu significative.Ainsi, une importante hétérogénéité du manteau existe sous la Campanie. Cette hétérogénéité doit être la conséquence de la nature différente des croûtes en subduction et qui sont en contact le long de la ligne tectonique de la plaine de la rivière Volturno: an Nord-Ouest, une croûte continentale, sismiquement inactive, plonge sous le Latium alors qu'au Sud-Est, une croûte océanique, sismiquement active, plonge sous la Calabre et jusque sous la Campanie.

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With 9 Figures  相似文献