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Zusammenfassung Die Gesteine der Zone Sestri-Voltaggio im Hinterland von Genua stellen die Basis des Ligurikum dar. Diese Basis (Perm bis Oberjura) ist im Nordapennin normalerweise nicht aufgeschlossen. Lediglich in der Zone Sestri-Voltaggio wurde sie durch das Serpentinitmassiv der Gruppe von Voltri angeschleppt. Es lassen sich somit Vergleiche zwischen den mesozoischen Folgen der alpinen Gruppe von Voltri und der ligurischen Zone Sestri-Voltaggio anstellen. Diese Vergleiche zeigen, daß im Raum der Zone Sestri-Voltaggio von der Trias bis zur Kreide eine Faziesgrenze lag, deren Bedeutung durch den Intrusionsrand der Peridotite der Gruppe von Voltri und die Anlage der großen Randstörung der Linie SestriVoltaggio noch erhöht wurde. Die Alpen-Apenningrenze ist durchaus zu Redit in die Zone Sestri-Voltaggio zu legen.
The zone of Sestri-Voltaggio (near Genoa) represents the base of Liguricum. This Permian to Upper Jurassic base is not disclosed elsewhere in the Northern Apennines. Comparisons of the Mesozoic alpidic sequence of Voltri with the Ligurian zone mentioned above show a facies-boundary lasting from Triassic until Cretaceous times within the Sestri-Voltaggio-zone. This boundary seems to be underlined by the Voltri-peridotite-intrusive-border and by the situation of the border-fault of Sestri-Voltaggio. The boundary between the Alps and Apennines coincides with the Sestri-Voltaggio-zone.
Résumé Les roches de la zone Sestri-Voltaggio dans l'arrière-pays de Gênes représentent la base du Ligurikum. Cette base (Permien jusqu'au Jurassique supérieur) n'affleure pas normalement dans l'Apennin septentrional. C'est seulement dans la zone Sestri-Voltaggio qu'elle a été entraînée par le massif de Serpentine du groupe de Voltri. On peut ainsi faire des comparaisons entre la série mésozoïque du groupe alpine de Voltri et celle de la zone ligurique de Sestri-Voltaggio. Ces comparaisons montrent que dans le domain de la zone de Sestri-Voltaggio, il existe depuis le Triasique jusqu'au Crétacique une limitation du faciès, dont la signification est encore accentuée par la bordure intrusive de la péridotite du groupe de Voltri et la position de la grande dislocation de bordure de la ligne Sestri-Voltaggio. La limite Alpes-Apennin doit donc d'après cela, avec raison, se situer dans la zone Sestri-Voltaggio.
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P. Giese S. Ibbeken B. Baier K. Schulze-Frerichs 《International Journal of Earth Sciences》1990,79(3):567-579
Seismic refraction measurements were carried out along the DEKORP 2-N reflection line. Traveltime data have been inverted to velocity-depth distributions using x-t-inversion- und ray-tracing-methods. The velocity-model shows alternating layers of high and low velocity. High-velocity values range from 6.0 to 6.6 km/s in the upper crust and from 70 to 8.2 km/s in the lower crust. In low-velocity zones velocities do not exceed 6.25 km/s. The crust/mantle boundary lies in about 28–30 km depth. Correlations exist between the velocity-model of refraction seismics and the line drawing section of reflection seismics.
Zusammenfassung Entlang dem tiefenseismischen Reflexionsprofil DEKORP 2-Nord wurden seismische Refraktionsmessungen durchgeführt. Die Laufzeitdaten wurden mit Hilfe von x-t-Inversions- und Ray-Tracing-Verfahren in Geschwindigkeits-Tiefen-Verteilungen transformiert. Es treten alternierende Hoch- und Niedriggeschwindigkeitszonen auf. In der oberen Kruste treten hohe Geschwindigkeitswerte im Bereich von 6,0 bis 6,6 km/s auf und in der unteren Kruste Werte von 7,0 bis 8,2 km/s. Die Geschwindigkeitswerte in Niedriggeschwindigkeitszonen überschreiten 6,25 km/s nicht. Die Grenze zwischen Erdkruste und Erdmantel liegt in einer Tiefe von etwa 28 bis 30 km. Es bestehen Übereinstimmungen zwischen dem Geschwindigkeitsmodell der Refraktionsseismik und der Struktur der reflexionsseismischen Sektion.
Résumé Des mesures en sismique-réfraction ont été effectuées le long du profil de sismique réflexion DEKORP 2-N. On a réalisé une inversion des temps de propagation en distribution vitesse/profondeur par les méthodes de l'inversion x-t et du traçage de raie. Le modèle des vitesses fait apparaître des couches alternées à grandes et faibles vitesses. Les grandes vitesses sont de 6,0 à 6,6 km/sec dans la croûte supérieure et de 7,0 à 8,2 km/sec dans la croûte inférieure. Dans les zones à faible vitesse, celle-ci n'excède pas 6,25 km/sec. La profondeur du contact croûte/manteau est d'environ 28 à 30 km. Il existe une correspondance entre le modèle des vitesses de la sismique-réfraction et l'image fournie par la sismique-réflexion.
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The thermogravimetric measurements on fayalite reported by Nakamura and Schmalzried (1983) have been reassessed using the compound-energy model and computer calculations which eliminate much mathematical manipulation and subjective choice. The calculated phase field for fayalite differs somewhat from the one obtained by Nakamura and Schmalzried (1983) but there is satisfactory agreement in the experimental range. 相似文献
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The photo-sieving method enables the grain-size analysis of particles > 10 mm from unconsolidated openwork bedding surfaces. The accuracy is equal to the machine-sieving method. The sediment surface is photographed in the field using a camera stand. The enlarged print is digitized for computer processing by tracing the outlines of the pebbles. From the size and shape of the projection area of the individual pebble images the computer determines the ellipsoids of revolution, classifies these ellipsoids, and establishes their grain-size distribution in percentage by weight. Thus photo-sieving differs distinctly from point-counting techniques. With the aid of photo-sieving, the surface grain-size distributions of larger sedimentary systems may be regularly mapped. Alluvial fans, braided rivers, both onshore and offshore coasts or areas of relict sediments and manganese nodules are suitable for this method. 相似文献
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The Hanaupah-Fan Shoreline Deposit (HSD) is an as yet undescribed occurrence of shoreline sediments of late Pleistocene Lake Manly in Death Valley, California. It is located in the southern part of Death Valley, at the northeastern periphery of Hanaupah Fan. The HSD is a gently sloping, WSW-ENE elongated ridge, about 600 m long, 165 m wide and 8 m high. Its surface extends from -12 to +28 m in elevation, i.e. it has a vertical range of 40 m. We interpret the deposit as a sediment body that extended from the Hanaupah Fan east into the lake. Rising lake level, and waves approaching both from the north and south eroded fan materials, and produced a sediment body with a complex architecture. Fetch for waves approaching from either direction was about 40 km. The sedimentary inventory consists of cross-stratified gravel beds of various size ranges, dipping towards the north, south, and east, and of horizontal berm gravel beds, and horizontal silt layers. A discordant gravel layer covers the entire surface of the deposit, probably produced by wave action during the last phase of lake regression. This uniform gravel layer forms a surface that is distinctly different from the surrounding fan surfaces. It is relatively fine grained, much better sorted, and densely packed. Rock varnish is very well developed, and imparts a dark color to the surface, which makes it easily recognizable on aerial photographs. No absolute age date is available as yet, but circumstantial evidence places the formation of the deposit at the peak of marine isotope stage 2 (Wisconsinan/Weichsellian glacial maximum) 相似文献
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We applied new granulometric techniques to the various surfaces of the Hanaupah Fan, Death Valley, California, namely the Q1 surface, with an estimated age of 800–490 ka, the younger Q2 (170–105 ka) and Q3 (50–14 ka) surfaces, the <14 ka deposits of the incised channel, and to a (c. 14 ka) Lake Manly shoreline deposit at the northern periphery of the fan. We used these techniques to generate quantitative information on surface clast grain-size distributions, clast sphericity, roundness, and clast orientation to provide a data set that could be used to define fan-segment surfaces, and to help interpret fan genesis. Grain-size analyses were carried out by photo-sieving of 139 surface pictures, by petrographic identification of samples taken in the incised channel, and by identification and measuring of the largest clasts (1452 measurements) on the Q3 surface. The results show that all fan-segment surfaces, regardless of age, have similar size distributions, with a well-defined gravel mode of −2·3 to −3·0 phi, and are poorly to moderately sorted. Samples from the incised channel have distributions that are very similar to each other, regardless of distance from the apex, but display reduced sorting compared to the fan surfaces (which largely lack fines, perhaps from winnowing by secondary overland flow). Only the shoreline deposit is different from the other elements, showing a much narrower, well-defined gravel mode (−3·0 phi), and is moderately well sorted. Sphericity and roundness of clasts on all surfaces show only minor differences, similar to the other sedimentary parameters, indicating a remarkable homogeneity of the surfaces of the sediment body. In addition, measurements of the largest clasts (>100 cm long axis) on the Q3 surface showed no discernible trend either with radial distance or with rock type. These data suggest large depositional episodes that produce extensive sedimentary units without differentiation relative to distance from the source. Of the examined parameters, clast orientation is the best predictor of relative age of fan surfaces. Clast orientation in the main channel is bimodal, i.e. the long axes of clasts are either at right angles or parallel to transport direction. This bimodality disappears with increasing age, and the preferred orientation becomes unimodal (long clast axes normal to transport direction) on the Q1 surface. Although the causes of this change are still in debate, use of this parameter as a relative-age dating tool seems possible. © 1998 John Wiley & Sons, Ltd. 相似文献
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