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81.
Maurits Lindström Johan Ekvall Stefan E. Hagenfeldt Brigitta Säwe Erik F. F. Sturkell 《International Journal of Earth Sciences》1991,80(1):201-204
The Lockne impact crater south of Östersund formed in the early Middle Cambrian with a diameter of 7 km. It is identified by its rim wall of crushed Precambrian basement granite, by fragments of impact melt, and by grains of shocked quartz. The exceptional preservation, in particular of the rim wall, is due to a complicated geological history, the first stage of which consisted of burial by marine sediments. This stage lasted until the Middle Ordovician, or over 50 million years. An early Caradoc lowering of the sea-level may have induced debris flows that stripped the rim wall of much of its sedimentary cover. Because normal marine sedimentation recommenced soon after this event, the structure was not seriously damaged, as it was buried again. The Caledonian orogeny emplaced an overthrust nappe as ultimate protection, which was removed by a recent erosion episode from all but the center of the structure.Structures formed by the impact of extraterrestrial bodies are very rare throughout much of Europe, because such structures are neither well preserved nor displayed in young mountain belts or sedimentary basins. However, northern Europe has several ascertained structures of this kind (Svensson &Wickman, 1965;Svensson, 1968;Bruun &Dahlman, 1982;Kala et al., 1984;Flodén et al., 1986;Wickman, 1988). Unfortunately, the hitherto known structures are either poorly preserved or hidden by younger deposits. We are reporting the discovery of a well-preserved exposed and accessible impact structure that has escaped the notice of geologists although important features of it have been described and puzzled over by generations of researchers (Wiman, 1900;Hadding, 1927;Thorslund, 1940;Lindström et al., 1983).The structure is located in the Lockne area to the south of Östersund in central Sweden. It has a diameter of 7 km and its center is near Tramsta on the northwest shore of Lake Locknesjön (Fig. 1). Its middle is covered by folded Lower to Middle Ordovician Orthoceratite Limestone with the sheared Lower Ordovician Töyen Shale at its base. This local expanse of deformed rock is the remainder after erosion of an extensive nappe of overthrust rocks emplaced during the Caledonian orogeny. The good preservation of the impact structure is due to the nappe cover, which had to be removed before erosion could attack the underlying structures.The rim of the impact crater is outlined by a wall of strongly shattered fragments of Proterozoic crystalline rocks (Fig. 2), which formed the local bedrock (Strömberg et al., 1984) at the time of impact. The rim wall is best preserved along the western part of the structure. It was referred to as »arkose-like breccia« byThorslund (1940), who interpreted it as the result of continental weathering, but the components rather show evidence of intense crushing than of weathering (Simon, 1987a). The »arkose-like breccia« does not contain components derived from the lower Palaeozoic deposits of the area. 相似文献
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The concept of essential fish habitats (EFHs) is widely accepted for conservational and management purposes. EFHs are often considered as high quality habitats for fisheries species and subsequently of high values for society. In this study, fish and Substrate-Associated Prey (SAP) were sampled during the productive summer season 1998 (fish) and 2003 and 2004 (SAP) in shallow coastal rocky- and soft-bottom habitats on the Swedish west coast. The aim was to study the spatial and monthly variation of SAP as well as abundance and biomass of fish, and to examine if food items found in the diet of the fish assemblage were derived from SAP. We also examined if the diet of Ctenolabrus rupestris, a resident and abundant fish species in the shallow coastal habitats, and the diet of four seasonally abundant and commercially important fish species (Gadus morhua, Pleuronectes platessa, Salmo trutta and Scomber scombrus) were derived from SAP. There were significantly higher mean species number and abundance of the SAP assemblage on rocky compared to soft bottoms and the highest values were found on the rocky bottoms in August and in the shallowest (0–3 m) depth strata. There were no significant differences in number of fish species caught in the two habitats, although mean number of fish and mean biomass were significantly higher on rocky bottoms. Both habitats showed the same seasonal variation and the highest values of number of fish species, abundance and biomass were observed in June. On rocky bottoms, gastropods and amphipods were the most frequent food items in the diet of the entire fish assemblage and these items were also the most abundant SAP in this habitat. The dominant food items of the soft-bottom fish assemblage were decapods and fish, which were not common SAP. However, except for S. scombrus, the diet of the selected fish species showed a strong association to the SAP availability. Gadus morhua displayed the strongest association to SAP on rocky bottoms and P. platessa and C. rupestris to SAP on soft bottoms. Further, for C. rupestris, multivariate statistical analysis showed a significant association to the SAP assemblage on both rocky and soft bottoms. These results provide vital new information for the management and conservation of Essential Fish Habitats on the Swedish west coast. 相似文献
84.
Simulations of subtropical marine low clouds and their radiative properties by nine coupled ocean-atmosphere climate models
participating in the fourth assesment report (AR4) of the intergovernmental panel on climate change (IPCC) are analyzed. Satellite
observations of cloudiness and radiative fluxes at the top of the atmosphere (TOA) are utilized for comparison. The analysis
is confined to the marine subtropics in an attempt to isolate low cloudiness from tropical convective systems. All analyzed
models have a negative bias in the low cloud fraction (model mean bias of −15%). On the other hand, the models show an excess
of cloud radiative cooling in the region (model mean excess of 13 W m−2). The latter bias is shown to mainly originate from too much shortwave reflection by the models clouds rather than biases
in the clear-sky fluxes. These results confirm earlier studies, thus no major progress in simulating the marine subtropical
clouds is noted. As a consequence of the combination of these two biases, this study suggests that all investigated models
are likely to overestimate the radiative response to changes in low level subtropical cloudiness. 相似文献
85.
C. Johan Masreliez 《Astrophysics and Space Science》2010,326(2):281-291
The phenomenon of inertia is modeled by a new process, which semi-discretely changes the metrical scale of spacetime. This
process explains inertia as a curved spacetime phenomenon, since all accelerating trajectories take place on geodesics of
general relativity. By this approach inertial reference frames are Minkowskian manifolds imbedded in a five-dimensional space.
It would imply a revised interpretation of special relativity, which preserves a universal temporal reference. If acceleration
curves spacetime, it would also imply the existence of an energy-momentum tensor with net energy, which under certain conditions
could become negative. 相似文献
86.
Eduardo Zorita Anders Moberg Lotta Leijonhufvud Rob Wilson Rudolf Brázdil Petr Dobrovolný Jürg Luterbacher Reinhard Böhm Christian Pfister Dirk Riemann Rüdiger Glaser Johan Söderberg Fidel González-Rouco 《Climatic change》2010,101(1-2):143-168
Two European temperature reconstructions for the past half-millennium, January-to-April air temperature for Stockholm (Sweden) and seasonal temperature for a Central European region, both derived from the analysis of documentary sources and long instrumental records, are compared with the output of climate simulations with the model ECHO-G. The analysis is complemented by comparisons with the long (early)-instrumental record of Central England Temperature (CET). Both approaches to study past climates (simulations and reconstructions) are burdened with uncertainties. The main objective of this comparative analysis is to identify robust features and weaknesses in each method which may help to improve models and reconstruction methods. The results indicate a general agreement between simulations obtained with temporally changing external forcings and the reconstructed Stockholm and CET records for the multi-centennial temperature trend over the recent centuries, which is not reproduced in a control simulation. This trend is likely due to the long-term change in external forcing. Additionally, the Stockholm reconstruction and the CET record also show a clear multi-decadal warm episode peaking around AD 1730, which is absent in the simulations. Neither the reconstruction uncertainties nor the model internal climate variability can easily explain this difference. Regarding the interannual variability, the Stockholm series displays, in some periods, higher amplitudes than the simulations but these differences are within the statistical uncertainty and further decrease if output from a regional model driven by the global model is used. The long-term trend of the CET series agrees less well with the simulations. The reconstructed temperature displays, for all seasons, a smaller difference between the present climate and past centuries than is seen in the simulations. Possible reasons for these differences may be related to a limitation of the traditional ‘indexing’ technique for converting documentary evidence to temperature values to capture long-term climate changes, because the documents often reflect temperatures relative to the contemporary authors’ own perception of what constituted ‘normal’ conditions. By contrast, the amplitude of the simulated and reconstructed inter-annual variability agrees rather well. 相似文献
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The Upper Tertiary inter-andean tectonic trough of the Salar de Punta Negra is being filled mainly through sporadic flash-floods by denudation products from the East (Andes). Borehole records up to 430 m deep suggest depositional conditions similar to the actual ones.Block tectonic movements with N-S and NNE-SSW directions from Upper Tertiary through Pleistocene affected the normal morphology of the fans.Gravity survey has corfirmed a tectonic origin of the basin. East of the Salar, a buried graben with an alluvial fill of 550–750 m thickness was found, which may contain a groundwater reservoir.
Zusammenfassung Der jungtertiäre intra-andine Graben des Salars Punta Negra wurde durch sporadische Flutfächer vorwiegend aus dem Osten (Hochkordillere) gefüllt. Bohrungen bis 430 m Tiefe zeigen ähnliche Fanglomerate, wie sie heute entstehen.Verwerfungen mit N-S- und NNE-SSW-Richtungen zwischen Jungtertiär und Pleistozän beeinflussen die Morphologie der Schuttfächer.Gravimetrische Messungen ergaben, daß die Depression tektonisch angelegt ist. Östlich des heutigen Salars liegt ein verschütteter Graben mit einer alluvialen Füllung von mindestens 550–750 m Dicke. Hier könnte ein Grundwasser-Reservoir liegen.
Resumen El graben intra-andino del Salar de Punta Negra de edad Terciario Superior ha sido esporádicamente rellenado por conos aluviales. Estos vienen principalmente del este desde la Alta Cordillera. Perforaciones que han llegado hasta 430 m de profundidad muestran fanglomerados semejantes a los que se forman actualmente.Una tectónica de bloques de dirección N-S y NNE-SSW entre el Terciario Superior y el Pleistoceno afectan la morfología de los conos aluviales.Mediciones gravimétricas permiten concluir que la depresión tiene origen tectónico. Al oriente del Salar aparece un graben relleno de materiales aluviales con una potencia entre 550–750 m. Este graben puede contener acuíferos profundos de utilidad local.
Résumé Le graben intra-andin Cénozoïque Supérieur du Salar de Punta Negra se comble par des courants torrentueux sporadiques de produits de dénudation venant surtout de l'Est (Haute Cordillère). Des forages atteignant 430 m de profondeur suggèrent des conditions de dépôt similaires aux actuelles.Des failles N-S et NNE-SSW actives depuis le Cénozoïque Supérieur jusqu'au Pléistocène ont affecté la morphologie des cônes de déjection.Les mesures gravimétriques confirment l'origine tectonique du bassin de Punta Negra. A l'Est du Salar est situé un graben totalement enfoui de dépôts alluviaux d'une puissance d'environ 550–750 m, où des nappes aquifères exploitables sont susceptibles d'exister à grande profondeur.
- Salars Punta Negra , . 430 , . - -- — -- . , , . Salars , 550–750 . .相似文献
90.