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101.
102.
Ohne ZusammenfassungEine ausführliche Darstellung erscheint in Die Küste, Bd. 3, 1955.  相似文献   
103.
Analysis of extended plutons in the Coast Range of North Chile between 25°30′ and 26°35′ led to the recognition of a complex magmatic and structural evolution from the Upper Paleozoic to the Tertiary. The ascension of the intrusive bodies is dictated by deep-seated block tectonics. Generally the chemistry changes from S-type magmas in the Paleozoic to I-type magmas in the Mesozoic and Cainozoic. This is accompanied by a change in the structural geology of the continental margin which we present in six hypothetic phases (Devonian-Tertiary). We are only at the beginning of an encompassing synthesis of the genesis of the Andean orogen.  相似文献   
104.
Dense swarms of predominantly mafic dykes outcrop in the north Chilean Coast Range. These rocks are not lamprophyres. They mark channelways used by Jurassic-to-Lower Cretaceous extrusives.The dykes can be divided into three groups according to their petrography, major and trace element compositions. Rocks of the oldest group (series I) are essentially andesitic with high Na, K, Fe, Ti, Mn, P, V and low Al and Sr values. The rocks of series II are normal calc-alkaline basalts and andesites, whereas the rocks of series III are rhyodacites with calc-alkaline affinities.It is proposed that the series I dykes are genetically related to a continental fault system, whereas the dykes of series II and III are directly related to the post-Triassic evolution of the Andean active continental margin.
Zusammenfassung Die nordchilenische Küstenkordillere wird von einem dichten Netz vorwiegend mafischer Gänge durchzogen. Es sind dies keine Lamprophyre, sondern sie stellen Zufuhrsysteme effusiver Tätigkeit im Zeitraum Jura bis Unterkreide dar.Die Ganggesteine lassen sich petrographisch und aufgrund Haupt- und Spurenelementchemischer Charakteristika in drei Serien einteilen. Die ältere alkaline Serie I zeichnet sich durch erhöhte Na-, K-, Fe-, Ti-, Mn-, P-, V- sowie niedrige Al- und Sr-Gehalte aus. Die Basalte und Andesite der zweiten Serie hingegen zeigen eine normale kalkalkaline Entwicklung, die sich in den Rhyodaziten der dritten Serie fortsetzen dürfte.Während die Magmen der ersten Serie Affinitäten zu Basaltassoziationen kontinentaler Bruchsysteme aufzeigen, sind die kalkalkalinen Zusammensetzungen für die Magmenentwicklung des andinen, aktiven Kontinentalrandes seit dem Jura typisch.

Resumen La Cordillera de la Costa en el Norte de Chile es atravesada por una densa red de filones principalmente máficos. No se trata de rocas lamprofidicas sino representan sistemas de conductión de un volcanismo Jurásico/Cretácico Inferior.Basandose en sus caracteristicas petrográficas y geoquímicas las rocas filonianas se pueden dividir en tres series. La serie I, la más antigua, demuestra altas concentraciones de los elementos Na, K, Fe, Ti, Mn, P y V así como bajos contenidos de Al y Sr. Al contrario, las rocas basálticas y andesíticas de la serie II son caracterizadas por un desarollo calco-alcalino normal, lo cual habrá continuado en las rocas riodacíticas de la serie III.Mientras los magmas de la primera serie se pueden comparar con asociaciones basálticas de sistemas de fallas continentales, las series calco-alcalinas, por el contrario, son tipicas para un magmatismo que actuó en el borde continental activo andino desde el Jurásico.

- , , . , , . . . — 1 — Na, K, Fe, Mn, P, V . - ; . , - .


Prof. Dr. W. Zeil zum 65. Geburtstag gewidmet  相似文献   
105.
The otoliths of 200 postlarval spot (Leiostomus xanthurus) were marked by immersing the fish for 24 hr in a solution of 0.4 g tetracycline HCl l?1 of salt water (15 ‰). The resulting time-mark could later be identified under ultraviolet (UV) light with an epifluorescence microscope. Spot were held in the laboratory or in the field for up to 30 d. Two validation methods were employed to document daily increment formation. The total number of increments per otolith, or the number of increments formed after the time-mark, were regressed against days held in an experiment. The hypothesis of one increment per day would result in a regression coefficient not significantly different from 1.0. In the field both the total count method (b=1.05) and the time-mark method (b=0.90) supported a one-increment-per-day hypothesis and were not significantly different from each other (p>0.05). In the laboratory the total count method (b=0.56) and the time-mark method (b=0.36) were significantly different from 1.0 (p<0.05), and thus did not support the one-increment-per-day hypothesis. Failure to resolve a one-increment-per-day deposition rate in the laboratory was primarily attributed to food limitation in the experiments.  相似文献   
106.
Special issue on salt decay   总被引:1,自引:0,他引:1  
  相似文献   
107.
A representative suite of deformed, metamorphic rocks from the TRANSALP reflection seismic traverse in the Eastern Alps was studied in the laboratory with respect to elastic properties and whole-rock texture. Compressional wave (P-wave) velocities and their anisotropies were measured at various experimental conditions (dry, wet, confining pressure), and compared to the texture-related component of anisotropy. Here ‘texture’ refers to crystallographic preferred orientations (CPOs), which were determined by neutron texture goniometry. In gneisses and schists P-wave anisotropies are mainly controlled by the microcrack fabric. In marbles and amphibolites CPO contributes very significantly to anisotropy. At 200 MPa confining pressure the degree of anisotropy is between 5% and 15%, depending on rock composition and/or CPO intensity. Special emphasis was also put on discussing possible effects of fluids on seismic velocity and anisotropy. Distributions of water-filled microcracks and pores are distinctly anisotropic, with maximum contribution to bulk rock velocity mostly parallel to the foliation pole. Decreasing P-wave velocity and increasing anisotropy of immersed samples may be explained by crack-induced changes of the elastic moduli of bulk rock. The main conclusion regarding interpretation of TRANSALP data is that strong reflections in the deep Alpine crust are probably due to marble–gneiss and metabasite–gneiss contacts, although P-wave anisotropy and boundaries between zones of ‘dry’ or ‘wet’ series may contribute to reflectivity to some extent.  相似文献   
108.
International Journal of Earth Sciences - Systematic 40Ar/39Ar feldspar data obtained from the Sierras Pampeanas are presented, filling the gap between available high-...  相似文献   
109.
A high level of diversity has already been observed among the planets of our own Solar System. As such, one expects extrasolar planets to present a wide range of distinctive features, therefore the characterisation of Earth- and super Earth-like planets is becoming of key importance in scientific research. The Search (Spectropolarimetric Exoplanet AtmospheRe CHaracerisation) mission proposal of this paper represents one possible approach to realising these objectives. The mission goals of Search include the detailed characterisation of a wide variety of exoplanets, ranging from terrestrial planets to gas giants. More specifically, Search will determine atmospheric properties such as cloud coverage, surface pressure and atmospheric composition, and may also be capable of identifying basic surface features. To resolve a planet with a semi major axis of down to 1.4 AU and 30 pc distant Search will have a mirror system consisting of two segments, with elliptical rim, cut out of a parabolic mirror. This will yield an effective diameter of 9 m along one axis. A phase mask coronagraph along with an integral spectrograph will be used to overcome the contrast ratio of star to planet light. Such a mission would provide invaluable data on the diversity present in extrasolar planetary systems and much more could be learned from the similarities and differences compared to our own Solar System. This would allow our theories of planetary formation, atmospheric accretion and evolution to be tested, and our understanding of regions such as the outer limit of the Habitable Zone to be further improved.  相似文献   
110.
Abstract– The Moss meteorite is the first CO chondrite fall after a time period of 70 yr and the least terrestrially contaminated member of its group. Its cosmic‐ray exposure (CRE) age (T3 ~ 13.5 Ma; T21 ~ 14.6 Ma) is distinct among CO chondrites and, within witnessed falls is the shortest after Lancé, which we have reanalyzed. Gas retention ages are approximately 3.95 × 109 yr (U/Th‐He) and approximately 4.43 × 109 yr (K/Ar), respectively. Trapped Ar, Kr, and Xe are present in Moss in abundances typical for CO chondrites, with “planetary” elemental and isotopic compositions. Presence of HL‐xenon from presolar diamonds is observed in the stepwise release analysis of Lancé. It may also be present in Moss, but it is difficult to ascertain in single‐step bulk analyses. It follows from our new data combined with a survey of the literature that the abundance of trapped gases in CO chondrites is not a good indicator of their petrological subtype.  相似文献   
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