Geochemical facies model of ore formation in the Grythyttan-Hällefors area,Bergslagen, Central Sweden

The different iron and manganese ore deposits of the Grythyttan-Hällefors area display an arrangement that reflects a systematic change in redox conditions from oxidic banded iron formation into highly reduced graphite-bearing slates. This phenomenon is explained by a facies model. The different environmental conditions are also held to be responsible for the geochemical differentiation of base metal deposits into Cu ores associated with minerals of Bi, Co, Mo, As, Zn, Pb, Au, and Pb-Zn-Ag ores associated with minerals of Sb, Mn, As, Sn, Cu. Spatial relationships between deposits of these two groups and certain iron and manganese deposits point to a common source of all metals, possibly connected with exhalative derivates from basic volcanism.

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Zusammenfassung Die verschiedenen Eisen- und Manganerz-Bildungen des Grythyttan-Hällefors-Gebietes zeigen Verhältnisse auf, die einem systematischen Wechsel der Redoxbedingungen wiedergeben, von oxidischer Bändereisenerzbildung bis hin zu stark reduzierten graphitführenden Schiefern. Dieses Phänomen wird durch ein Fazies-Modell erklärt. Die unterschiedlichen Milieu-Bedingungen werden auch als Ursache für die geochemische Diferentiation unedler Metall-Ablagerungen in Cu-Erze angesehen, die mit Mineralien assoziiert sind, die Bi, Co, Mo, As, Zn, Pb, Au führen und in Pb-Zn-Ag-Erze in Verbindung mit Sb-, Mn-, As-, Sn- und Cu-führenden Mineralien. Die räumlichen Beziehungen zwischen Ablagerungen dieser zwei Gruppen und gewissen Eisen- und Mangan-Bildungen weisen auf eine gemeinsame Quelle aller Metalle hin, die möglicherweise mit exhalativen Derivaten eines basischen Vulkanismus in Verbindung steht.

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Résumé Les différents gisements de minerais de Fe et Mn de la région de Grythyttan-Hällefors montrent une disposition qui réflète un changement systématique dans les ernolitions de réduction des formations rubanées de fer oxydé en phyllades graphiteux. Ce phénomène s'explique suivant un modèle faciétal. Les différentes conditions de l'environnement sont ainsi rendues responsables de la différentiation géochimique des gisements métallifères de base en minerais de Cu associés à des minéraux de Bi, Co, Mo, As, Zn, Pb, Au et des minerais de Pb-Zn-Ag associés à des minéraux de Sb, Mn, As, Sn, Cu. Des relations spatiales entre les gisements de ces deux groupes et certains gisements de Fe et Mn indiquent une source commune pour tous les métaux, en liaison possible avec des émanations du volcanisme basique.

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Grythyttan-Hällefors , - : , , - . . , , Bi, , Mo, As, Zn, Pb, Au, , — , Sb, Mn, As, Sn, . , , , .

     

Properties of Components in Contact Systems

A new sample of contact systems, consisting of more than 100 stars, was created for binaries for which the physical parameters have been determined using both photometric light curves and radial velocity measurements of both components. Properties of components are discussed including their evolutionary status.     

Estimating the extent of the spraying zone on a sea-going ship

The maximum extent of ship spraying for a medium-sized fishing trawler (MFV) of Soviet type has been considered. A simple geometrical model for generating the spray due to ship-wave collisions has been applied to determine the maximum height of the spray source above the ship deck. The maximum height of the spray source has been assumed to depend on the ship speed relative to the moving waves and an empirical constant specific to a given type of ship. A unique field data set (Kuzniecov et al., 1971) of the height of the upper limit of ice accretion on the foremast of an MFV has been used to determine the value of the empirical constant for this vessel. For documented air-sea and ship motion parameters, the trajectories of droplets hitting the upper parts of the accretion on the foremast have been calculated using the equation of droplet motion for each reported icing event.The heights of the spray source computed by the trajectory method for each case of icing were compared with the heights of the spray source determined by a correlation involving the ship speed relative to the waves and the vertical extent of spray. The best fit was obtained for an empirical constant value of 0.535.The model performance was tested using an independent data set (Sharapov, 1971) on the spraying zone of an MFV. The tests showed that this model predicts the extent of the spraying zone over the ship with satisfactory accuracy and suggest that it should be incorporated into an integrated ship icing model.Finally, the model was run for several ship speeds, headings and wind speeds to examine the effect of these parameters on the maximum height of the spray hitting the ship's foremast. It was found that this height increases with wind speed and ship speed and is maximum for ship headings of 120–130°.     

Production of gas from coal seams in the Upper Silesian Coal Basin in Poland in the post-injection period of an ECBM pilot site

A pilot site for CO₂ storage in coal seams was set-up in the Upper Silesian Coal Basin in Poland in the scope of the RECOPOL project, funded by the European Commission. About 760 tons CO₂ were injected into the reservoir from August 2004 to June 2005. Breakthrough of the injected CO₂ was established, which resulted in the production of about 10% of the injected CO₂ in this period. This paper reports on activities performed under the European Commission project MOVECBM that aimed at the assessment of the storage performance of the reservoir in the follow-up period, i.e. whether the injected CO₂ was adsorbed onto the coal or whether it was still present as free gas in the pore space. The injection well was used for this purpose, as the production well had to be abandoned for permitting reasons. Several operational periods can be defined between the last injection in June 2005 and the abandonment of the well in October 2007. In the first period the well was shut-in to observe the pressure fall-off, from about 15.0 MPa at the wellhead after the last injection until about 4.5 MPa at the end of 2005. This pressure fall-off curve showed that the reservoir permeability was very low. This seemed to confirm the observed swelling of the coal during the injection period. In the first months of 2006 the pressure at the wellhead was decreased by releasing gas in a controlled way. The amount and composition of the gas were measured. As a result of the pressure reduction, the well flooded with water. A production pump was placed on the former injection well, enabling active production from the coal from March to September 2007. Results of these operations showed that whereas the gas production rates were as expected based on the experience with the production well, the water production was remarkably low. This could be related to permeability issues or, alternatively, indicate a drying effect of the CO₂ in the reservoir. Further, the gas composition showed a predominance of CO₂ over CH₄ during the gas release that changed gradually into a predominance of CH₄ over CO₂ during the production phase. Although stabilization was not reached within the given production period, the composition approached a 60% methane, 40% CO₂ ratio. This indicates that the exchange of these gases is more complex than often envisaged. After removal of the pump the well was filled with water, which ceased the gas release. This indicates that the pressure in the reservoir was back to its original, hydrostatic, state. As the total volume of CO₂ produced was only a fraction of the amount that was injected, it can be concluded that the CO₂ was taken up by the coal and is currently adsorbed. This gives confidence in the long-term stability of the injected CO₂.     

The Spatial Distribution of W UMa-Type Stars

The aim of this project is to study the spatial distribution of contact binaries and to compare the sample from the project of study the W UMa-type stars, with existing databases such as Hipparcos, GCVS or ASAS (ESA, 1997; GCVS, 2005; Pojmanski, 2002).     

The W UMa-type Stars Program: First Results, Current Status and Perspectives

We present the results of a statistical investigation of the period-color and period-bolometric magnitude relations using a carefully selected sample of 120 contact systems with known physical parameters.