Inertia and a fifth dimension—special relativity from a new perspective     

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   

European temperature records of the past five centuries based on documentary/instrumental information compared to climate simulations     

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   

Redefining the trophic importance of seagrasses for fauna in tropical Indo-Pacific meadows   总被引：2，自引：1，他引：1  

Jan Arie Vonk  Marjolijn J.A. Christianen  Johan Stapel 《Estuarine, Coastal and Shelf Science》2008,79(4):653-660

Fauna species living in seagrass meadows depend on different food sources, with seagrasses often being marginally important for higher trophic levels. To determine the food web of a mixed-species tropical seagrass meadow in Sulawesi, Indonesia, we analyzed the stable isotope (δ¹³C and δ¹⁵N) signatures of primary producers, particulate organic matter (POM) and fauna species. In addition invertebrates, both infauna and macrobenthic, and fish densities were examined to identify the important species in the meadow. The aims of this study were to identify the main food sources of fauna species by comparing isotopic signatures of different primary producers and fauna, and to estimate qualitatively the importance of seagrass material in the food web. Phytoplankton and water column POM were the most depleted primary food sources for δ¹³C (range −23.1 to −19.6‰), but no fauna species depended only on these sources for carbon. Epiphytes and Sargassum sp. had intermediate δ¹³C values (−14.2 to −11.9‰). Sea urchins, gastropods and certain fish species were the main species assimilating this material. Seagrasses and sedimentary POM had the least depleted values (−11.5 to −5.7‰). Between the five seagrass species significant differences in δ¹³C were measured. The small species Halophila ovalis and Halodule uninervis were most depleted, the largest species Enhalus acoroides was least depleted, while Thalassia hemprichii and Cymodocea rotundata had intermediate values. Fourteen fauna species, accounting for 10% of the total fauna density, were shown to assimilate predominantly (>50%) seagrass material, either directly or indirectly by feeding on seagrass consumers. These species ranged from amphipods up to the benthic top predator Taeniura lymma. Besides these species, about half of the 55 fauna species analyzed had δ¹³C values higher than the least depleted non-seagrass source, indicating they depended at least partly for their food on seagrass material. This study shows that seagrass material is consumed by a large number of fauna species and is important for a large portion of the food web in tropical seagrass meadows.  相似文献   

Regional Flow in the Baltic Shield During Holocene Coastal Regression   总被引：2，自引：0，他引：2  

Clifford I. Voss  Johan Andersson 《Ground water》1993,31(6):989-1006

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Floodfan sedimentation and gravitational anomalies in the Salar de Punta Negra,Northern Chile     

Ronald A. van Overmeeren  Johan H. Staal 《International Journal of Earth Sciences》1976,65(1):195-211

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.

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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.

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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.

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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.

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- Salars Punta Negra , . 430 , . - -- — -- . , , . Salars , 550–750 . .

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The significance of mafic nodules in the ultra-potassic rocks from central Italy - discussion     

Johan C. Varekamp 《Journal of Volcanology and Geothermal Research》1983,16(1-2)

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La parapierrotite,un nouveau minéral thallifère d'Allchar (Yougoslavie)     

Dr. Z. Johan  Dr. P. Picot  Dr. J. Hak  Dr. M. Kvaček 《Mineralogy and Petrology》1975,22(3-4):200-210

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Paleomagnetism in deep-sea core A179-15     

Nils-Axel Mörner  Johan Lanser 《Earth and Planetary Science Letters》1975,26(1):121-124

Core A179-15 from the southern North Atlantic exhibits one of the best paleoclimatic records for the last 25,000 years. This is because it is a high-sedimentation rate core and because it has been analysed at 1 cm intervals by Ericson and Wollin. The core has been used by Mörner for global climatic correlations. The magnetic measurements show a fairly drastic declination excursion at 12,350 B.P., i.e. exactly at the same age as the end of the Gothenburg Magnetic “Flip”. Therefore, the declination excursion in core A179-15 probably represents the end of the Gothenburg Magnetic “Flip” and Excursion. The excursion and a lithologic boundary verify the chronology earlier applied by Mörner.  相似文献   

Evolution paragénétique de la minéralisation uranifère de Chaméane (Puy-de-Dôme), France: chaméanite,geffroyite et giraudite,trois séléniures nouveaux de Cu,Fe, Ag et As     

Dr. Z. Johan  Dr. P. Picot  Dr. F. Ruhlmann 《Mineralogy and Petrology》1982,29(3):151-167

Résumé Trois séléniures nouveaux ont été découverts dans la minéralisation unranifère à séléniures et sulfures de Chaméane, France. Geffroyite, (Cu, Fe, Ag)₉(Se, S)₈, cubique,Fm3m,a=10.889 ,Z=4; structure type pentlandite. Densité calculée 5.39 g/cm³. Les raies les plus intenses du diagramme de poudre sont: 9 3.282 (311); 9 3.145 (222); 6 2.094 (511;333); 10 1.925 (440); 5 1.660 (533); 6 1.112 (844). Microdureté Vickers 70 kg/mm². Brun crème en lumière réfléchie, réflectances: 19.0 (420), 27.5 (500), 30.1 (540), 33.6 (600), 35.8 (660), 36.9 (700 nm). Chaméanite. Les analyses à la microsonde correspondent à (Cu_3.46Fe_0.52)_3.98 (As_0.94 Sb_0.02)_0.96(Se_3.72S_0.34)_4.06, formule idéale (Cu, Fe)₄As(Se, S)₄. Le rapport Cu/Fe varie de 6 à 13. Cubique,I---,a=11.039 ,Z=8, densité calculée 6.17 g/cm³. Raies les plus intenses du diagramme de poudre: 10 3.187 (222); 9 1.951 (440); 8 1.665 (622); 4 1.381 (800); 6 1.266 (662); 7 1.127 (844); 5 1.062 (10.2.2; 666). Microdureté Vickers 265 kg/mm². Gris foncé en section polie, plages à zonage complexe dû à des variations de Cu/Fe. Réflectances maximales: 27.1 (420), 26.6 (500), 27.1 (540), 27.7 (600), 28.2 (660); 28.7 (700 nm). Giraudite, (Cu, Zn, Ag)₁₂(As, Sb)₄(Se, S)₁₃. Cubique ,a=10.578 ,Z=2; structure type tétraédrite. Analogue arsénié de la hakite. Densité calculée 5.75 g/cm³. Raies les plus intenses du diagramme de poudre: 10 3.050 (222); 5 2.497 (411; 330); 6 1.932 (521); 9 1.868 (440); 7 1.593 (622). Microdureté Vickers 293 kg/mm². Gris clair, réflectances: 32.2 (420), 31.6 (500), 31.7 (540), 31.7 (600), 31.5 (660), 30.8 (700 nm).Trois épisodes minéralisants, séparés par des mouvements tectoniques, forment la paragenèse de Chaméane, comportant: barytine, pechblende, hématite, löllingite, mispickel, pyrite, chalcopyrite, clausthalite, tétraédrite, tennantite, bukovite, athabascaïte, umangite, berzelianite, klockmannite, eucaïrite, geffroyite, chaméanite, giraudite, eskebornite.

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Paragenetic evolution of the uranium mineralization rich in selenides at chaméane (Puy-de Dôme), France: Chaméanite, geffroyite and giraudite, three new selenides of Cu, Fe, Ag and As

Summary Three new selenides occur in the uranium mineralization rich in selenides and sulphides at Chaméane, France. Geffroyite, (Cu, Fe, Ag)₉(Se, S)₈, cubic,Fm3m,a=10.889 ,Z=4; pentlandite-like structure. Calculated density 5.39 g/cm³. The strongest lines in the X-ray powder pattern are: 9 3.282 (311); 9 3.145 (222); 6 2.094 (511; 333); 10 1.925 (440); 5 1.660 (533); 6 1.112 (844). Vickers microhardness 70 kg/mm². In reflected light, it has a brown colour with a cream tint. Reflectances: 19.0 (420), 27.5 (500), 30.1 (540), 33.6 (600), 35.8 (660), 36.9 (700 nm). Chaméanite. Microprobe analyses gave (Cu_3.46Fe_0.52)_3.98(As_0.94Sb_0.02)_0.96(Se_3.72S_0.34)_4.06; ideal formula is (Cu, Fe)₄As(Se, S)₄. The Cu/Fe ratio varies from 6 to 13. CubicI---,a=11.039 ,Z=8, calculated density 6.17 g/cm³. Strongest lines in the powder pattern: 10 3.187 (222); 9 1.951 (440); 8 1.665 (622); 4 1.381 (800); 6 1.266 (622); 7 1.127 (844); 5 1.062 (10.2.2; 666). Vickers microhardness 265 kg/mm². Dark grey in reflected light. Some grains exhibit irregular zoning due to variations of Cu/Fe ratio. Maximum reflectances: 27.1 (420), 26.6 (500), 27.1 (540); 27.7 (600), 28.2 (660), 28.7 (700 nm). Giraudite, (Cu, Zn, Ag)₁₂(As, Sb)₄(Se, S)₁₃. Cubic, ,a=10.578 ,Z=2; member of tetrahedrite series. Arsenian analogue of hakite. Calculated density 5.75 g/cm³. Strongest lines in the powder pattern: 10 3.050 (222); 5 2.497 (411; 330); 6 1.932 (521); 9 1.868 (440); 7 1.593 (622). Vickers microhardness 293 kg/mm². Light grey in reflected light, reflectances: 32.2 (420), 31.6 (500), 31.7 (540), 31.7 (600), 31.5 (660), 30.8 (700 nm). The mineralization of the Chaméane deposit consists of three cycles separated by tectonic movements. The minerals found are: barite, pitchblende, hematite, löllingite, arsenopyrite, pyrite, chalcopyrite, clausthalite, tetrahedrite, tennanite, bukovite, athabascaite, umangite, berzelianite, klockmannite, eucairite, geffroyite, chaméanite, giraudite and eskebornite.

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Avec 5 Figures  相似文献   

Siltation by sediment-induced density currents     

Johan C.?WinterwerpEmail author  Thijis?van Kessel 《Ocean Dynamics》2003,53(3):186-196

This paper describes the results of numerical experiments with a three-dimensional hydrodynamic and mud transport model in which sediment–fluid interaction is taken into account through the effects of hindered settling, buoyancy destruction in the turbulence k– model and sediment-induced barocline pressure gradients in the momentum equations. The model was applied to a schematic case representing a coastal area with a tidal river, navigation channel and harbour basin, and a real-world case, viz. Rotterdam harbour area in The Netherlands. The results show that the sediment transport into the harbour area, and subsequent siltation rates, increase by a factor 3 to 5 due to the sediment–fluid interaction. It is shown that the larger contribution stems from an increase in vertical gradients in suspended sediment.Responsible Editor: Jens Kappenberg  相似文献