Metal concentrations, fluxes, inventories and chronologies in sediments from Sepetiba and Ribeira Bays: A comparative study

Three sediment cores were sampled at Sepetiba Bay and four cores at Ribeira Bay, Rio de Janeiro State, Brazil. Sediment accumulation rates and chronologies were obtained from ²¹⁰Pb activity-depth profiles. Sediment accumulation rates in Ribera Bay ranged from 1.2 mm y⁻¹ in the inner bay to 2.6 mm y⁻¹ close to its entrance. In Sepetiba Bay two sediment accumulation rates were observed: a lower rate of 0.35 cm y⁻¹ before the 1960s and 0.76 cm y⁻¹ since then. The cause of this change is due to the construction of the Santa Cecília impoundment (1955) that brings water from the Paraíba do Sul Basin into the Guandu River, which increased its flow from the original 20 m³ s⁻¹ to 160 m³ s⁻¹. Concentration of 44 elements was obtained by ICP-MS after total dissolution of samples from two selected cores. The relative differences between the concentrations of crustal elements, such as Al, Fe and Ti are only about 20% (p < 0.05). Cd and Zn are 15 and four times larger in Sepetiba Bay than in Ribeira Bay, respectively. Other major and minor elements show lower statistically significant differences. The enrichment factors and metal inventories show that Sepetiba Bay can be considered polluted with Bi, Cd, Cr, Cu, Sb and Zn. Particularly, Cd and Zn present concentrations three and four times higher than the Brazilian existing limits.     

Dual-energy computerized tomography in compacted soil

This paper describes an alternative nondestructive technique for bulk density and water content determination in soils using dual-energy computerized tomography. A first generation tomographic system (STAC-1) was used in the analysis of the specimens. The system used ¹³⁷Cs (662 keV), ¹⁹²Ir (316 keV) and ²⁴¹Am (60 keV) as radiation sources and a Sodium Iodine crystal (NaI(Tl)) with photomultiplier tube as the detector. The specimens of soil tested were from different regions, one from São Paulo, and the other from Rio de Janeiro. The bulk density and the water content were determined point by point, in a transverse section of the soil specimens, using a computational algorithm that generated images of bulk density and water content. By utilizing the average pixel values of linear attenuation coefficient in these images, for each specimen, a characteristic curve could be built for each soil. The linear attenuation coefficient values agreed with the expected data. The compaction curves presented good agreement between the tomographic technique and the standard geotechnical method.     

A multi-scale approach to study the lithospheric structure of the southern Upper Rhine Graben: from seismic tomography through reflection seismics to surface geology

This paper integrates the results of different techniques—local and regional travel time tomography, reflection seismics, and surface geology. With this integration of different techniques, working on different scales, it is possible to derive a comprehensive picture of the present-day structures in the lithosphere of the Upper Rhine Graben. It is shown that the stucture of the lithosphere is dominated by structures related to the Variscan orogeny. Late stage strike-slip reactivation of the internal faults of the Rhine Graben is observed in the field. This reactivation is of dominant influence on the geomorphology in the southern end of the Upper Rhine Graben.     

Impact craters on Titan

Five certain impact craters and 44 additional nearly certain and probable ones have been identified on the 22% of Titan’s surface imaged by Cassini’s high-resolution radar through December 2007. The certain craters have morphologies similar to impact craters on rocky planets, as well as two with radar bright, jagged rims. The less certain craters often appear to be eroded versions of the certain ones. Titan’s craters are modified by a variety of processes including fluvial erosion, mass wasting, burial by dunes and submergence in seas, but there is no compelling evidence of isostatic adjustments as on other icy moons, nor draping by thick atmospheric deposits. The paucity of craters implies that Titan’s surface is quite young, but the modeled age depends on which published crater production rate is assumed. Using the model of Artemieva and Lunine (2005) suggests that craters with diameters smaller than about 35 km are younger than 200 million years old, and larger craters are older. Craters are not distributed uniformly; Xanadu has a crater density 2-9 times greater than the rest of Titan, and the density on equatorial dune areas is much lower than average. There is a small excess of craters on the leading hemisphere, and craters are deficient in the north polar region compared to the rest of the world. The youthful age of Titan overall, and the various erosional states of its likely impact craters, demonstrate that dynamic processes have destroyed most of the early history of the moon, and that multiple processes continue to strongly modify its surface. The existence of 24 possible impact craters with diameters less than 20 km appears consistent with the Ivanov, Basilevsky and Neukum (1997) model of the effectiveness of Titan’s atmosphere in destroying most but not all small projectiles.     

Metropolitan deconcentration, socio-political fragmentation and extended suburbanisation: Brazilian urbanisation in the 1980s and 1990s

The aim of this paper is to discuss the phenomena of socio-political fragmentation of urban space, extended suburbanisation and metropolitan deconcentration, which have been important features of Brazilian urbanisation since the 1980s (metropolitan deconcentration partly since the 1970s). At the beginning it profiles the recent evolution of the country's economy, in order to make sense of the worsening situation in terms of exclusion and violence in big Brazilian cities since the 1980s. Against this background, recent trends both in terms of socio-spatial segregation and social conflict within cities (formation of enclaves dominated by drug trafficking organisations and self-segregation of the élites as a response to this) and in terms of the growing attractiveness of areas outside the biggest metropolises (extended suburbanisation and metropolitan deconcentration) are analysed. The main focus is the socio-political dimension of Brazilian urbanisation in the 1980s and 1990s, which has been undervalued by analysts.