High Angular Resolution Studies of Coronal Structures with SOHO

Since January 1996, the Solar and Heliospheric Observatory (SOHO)has been providing unprecedented views of the extended solar coronato heliocentric distances of up to 32 solar radii. During the past threeyears we carried out studies of the morphology and dynamical evolutionof various structures in the solar corona using two instruments on boardSOHO: the Large Angle Spectrometric Coronagraph (LASCO) and the ExtremeUltraviolet Imaging Telescope (EIT). We have applied advanced image resolutionenhancement techniques to explore in detail the characteristics of thesmall-scale structures and/or the low contrast structures in the solarcorona. We describe here the results from these high-angular resolutionstudies, including of the kinematics of several Coronal Mass Ejections andpolar jets.     

Der Mechanismus der dreimonatigen Oszillation des Großen Roten Flecks auf dem Jupiter

The present paper is a test to explain the three-month oscillation of the Great Red Spot on Jupiter as a solution of the NAVIER-STOKES equation which is coupled with a nonlinear equation of oscillation. Since several parameters resp. functions are unknown it is difficult to find quantitative solutions.     

Uranium (-nickel-cobalt-molybdenum) mineralization along the Singhbhum copper belt,India, and the problem of ore genesis

Uranium mineralization is present at many places along the 200 km long Singhbhum copper belt, but the mineralization is relatively concentrated at the central part of it. The belt is characterized by many shear zone features, such as mylonites, phyllonites, and L-S type of structures and of course, copious metasomatism. Country rocks are basic schists, metapelites, quartzose rocks and albite schist/gneiss (Soda Granite). Orebodies are sheet-like, conformable with the pervasive planar structures in the host rocks. No pronounced wall rock alteration accompanied the mineralization. Grade of the ore is low (<0.1% U₃O₈). The principal uraniferous mineral uraninite occurs as dissemination. Other uranium-bearing minerals include pitchblende, allanite, xenotime, davidite, clarkeite, autunite (-metaautunite), torbernite, schoepite (-metaschoepite) and uranophane. Uranium is also present in a number of refractory phases either as inclusion of uraninite or in the crystal structure. Additionally, nickel, cobalt and molybdenum are present at Jaduguda-Bhatin in the form of millerite, gersdorffite, melonite, nickel-bearing pyrite, molybdenite etc. Dominance of uraninite over pitchblende and the larger cell-edge of uraninite, development of hematite-bearing quartz and Na-oligoclase at places in the ore zone, association of uranium mineralization with Ni-Co-Mo(-S-As) mineralization at Jaduguda-Bhatin and continuation of the orebodies to considerable depths, suggest that the uranium mineralization along the Singhbhum belt belongs to moderate to high temperature vein type. The age obtained by Pb²⁰⁷/Pb²⁰⁶ ratio and the concordia method suggest that the uranium mineralization in Singhbhum took place 1500–1600 Ma ago and this age is not far different from the age of formation of uranium-vein deposits in many other Precambrian shields of the world. The following two mechanisms of the formation of the deposits are discussed: 1) uranium precipitated in the Dhanjori basal sediments was mobilized during deformation and metamorphism into ore deposits, 2) the hydrodynamic system that leached out copper from the metabasic rocks to form the copper deposits at an earlier stage, could, in one of the oxidised pulses leach out uranium from the basal sediments and precipitate it in the favourable situations. Subsequent small-scale redistribution is possible. Constituents of the Ni-Co-(-S-As) mineralization appear to have been contributed by the volcanic-sedimentary pile.     

Mass-independent isotope effects in Archean (2.5 to 3.8 Ga) sedimentary sulfides determined by ion microprobe analysis

We report sulfur isotope anomalies with Δ³³S, the deviation from a mass-dependent fractionation line for the three-isotope system (³⁴S/³²S vs. ³³S/³²S), ranging up to ±2‰ within individual Archean sedimentary sulfides from a variety of localities. Our measurements, which are made in situ by multicollector secondary ion mass spectrometry, unequivocally corroborate prior bulk measurements of mass-independent fractionations (MIF) in sulfur and provide additional evidence for an anoxic atmosphere on the Earth before ∼2 Ga. This technique also offers new opportunities for exploring ancient sulfur metabolisms preserved in the rock record. The presence of MIF sulfur in sulfides from a >3.8-Ga Fe-rich quartzite from Akilia (island), West Greenland, is consistent with a marine sedimentary origin for this rock.     

Use of Geomorphological Information in Indirect Landslide Susceptibility Assessment

The objective of this paper is to evaluate the importance of geomorphological expert knowledge in the generation of landslide susceptibility maps, using GIS supported indirect bivariate statistical analysis. For a test area in the Alpago region in Italy a dataset was generated at scale 1:5,000. Detailed geomorphological maps were generated, with legends at different levels of complexity. Other factor maps, that were considered relevant for the assessment of landslide susceptibility, were also collected, such as lithology, structural geology, surficial materials, slope classes, land use, distance from streams, roads and houses. The weights of evidence method was used to generate statistically derived weights for all classes of the factor maps. On the basis of these weights, the most relevant maps were selected for the combination into landslide susceptibility maps. Six different combinations of factor maps were evaluated, with varying geomorphological input. Success rates were used to classify the weight maps into three qualitative landslide susceptibility classes. The resulting six maps were compared with a direct susceptibility map, which was made by direct assignment of susceptibility classes in the field. The analysis indicated that the use of detailed geomorphological information in the bivariate statistical analysis raised the overall accuracy of the final susceptibility map considerably. However, even with the use of a detailed geomorphological factor map, the difference with the separately prepared direct susceptibility map is still significant, due to the generalisations that are inherent to the bivariate statistical analysis technique.     

Trans-Atlantic correlation of eruptive sequences and individual silicic volcanic units within the Paraná-Etendeka igneous province

The Mesozoic volcanic rocks of the Serra Geral Formation in the Paraná Basin, South America, and of the Etendeka Group in northwestern Namibia were erupted shortly before the opening of the South Atlantic. The major widespread silicic volcanic units in the Etendeka Group are interpreted as rheoignimbrites (Milner et al., 1992) and are interbedded with tholeiitic basalts and basaltic andesites.The southern portion of the Etendeka Group is subdivided into a basal Awahab Formation which is overlain disconformably by the Tafelberg Formation. Both formations contain silicic and mafic units. Bulk composition, initial ⁸⁷Sr/⁸⁶Sr ratios, phenocryst assemblages and mineral compositions are used to correlate silicic units of the Awahab Formation with the basal units of the Palmas silicic volcanic rocks in the southern Paraná Basin. Silicic units of the Tafelberg Formation can similarly be correlated with silicic units in the upper portion of the Palmas succession, which are also disconformable on the units below them. Not all silicic units in these successions are present in both the Etendeka and Paraná areas, but where correlation of individual units is possible, then this is found to be consistent with the overall stratigraphic sequence.Silicic units in the Awahab Formation were erupted from the Messum Igneous Complex in Namibia and their correlation into Brazil indicates that individual eruptive units must have travelled over 340 km from their source. Serial changes in the composition of silicic units in the Awahab Formation and their correlatives indicates that they were erupted from a single magma system from which a total of ˜ 8600 km³ of material was erupted.     

The Hinode Spectro-Polarimeter

The joint Japan/US/UK Hinode mission includes the first large-aperture visible-light solar telescope flown in space. One component of the Focal Plane Package of that telescope is a precision spectro-polarimeter designed to measure full Stokes spectra with the intent of using those spectra to infer the magnetic-field vector at high precision in the solar photosphere. This article describes the characteristics of the flight hardware of the Hinode Spectro-Polarimeter, and summarizes its in-flight performance.