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  • 1990-1994  (11)
  • 1960-1964
  • 1994  (10)
  • 1991  (1)
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  • 1990-1994  (11)
  • 1960-1964
Year
  • 1
    Electronic Resource
    Electronic Resource
    s.l. ; Stafa-Zurich, Switzerland
    Materials science forum Vol. 175-178 (Nov. 1994), p. 1009-1014 
    ISSN: 1662-9752
    Source: Scientific.Net: Materials Science & Technology / Trans Tech Publications Archiv 1984-2008
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Abstract Crust formation ages inferred on the basis of Nd model age, U-Pb zircon and Pb-Pb data for granulites from central Sri Lanka, and the late Archean Lewisian (Scotland) and Nuk (south-western Greenland) high-grade gneisses are comparable, and in the range 2.2–3.0 Ga and 2.8–3.0 Ga respectively. The time interval between crust formation and high-grade metamorphism (with its attendant depletions of incompatible and heat-producing elements) is in the order of ∼ 2 Ga for the ∼ 0.6 Ga Highland granulites of Sri Lanka, but are less than ∼ 0.1–0.2 Ga for the Lewisian and Nuk gneisses. Severe depletions of U and Th produced the distinctive unradiogenic present-day Pb ratios of the Lewisian and Nuk gneisses. The Sri Lanka granulites, in contrast, preserve a record of an extended residence in a high U/Pb, high Th/Pb environment and display radiogenic »upper crustal« — like present-day isotope ratios. Relative to primitive mantle compositions, the Pb isotopes identify the Lewisian and Nuk terrains as crustal reservoirs depleted in Th and U (relative to Pb), whereas the Highland granulites are enriched. The global Pb isotope mass balance requires the existence of low U/Pb, low Th/Pb and high Th/U reservoir(s) for successful solutions, and the lower crust is a likely candidate for this reservoir. High-grade terrains like Sri Lanka show depletions of measured U and Th abundances relative to Pb, but do not show Pb isotope signatures of »model bulk lower crust«. Archean high-grade gneisses display the appropriate combination of retarded Th/Pb and U/Pb although their absolute compositions are much less radiogenic than those of »model bulk lower crust« predicted from simple mass balance calculations.
    Abstract: Résumé Les âges modèles de formation de la croûte, estimés à partir des méthodes Nd, U-Pb (zircon) et Pb-Pb, pour les granulites du Sri Lanka central d'une part et les gneiss de degré élevé lewisiens (Archéen sup.) d'Ecosse et de Nuk (sud-ouest du Groenland) d'autre part, sont comparables et se situent respectivement dans les intervalles de 2,2–3,0 Ga et 2,8–3,0 Ga. L'intervalle de temps qui sépare la formation de la croûte et le pic du métamorphisme (accompagné de pertes d'éléments incompatibles et producteurs de chaleur) est de l'ordre de ± 2 Ga pour les granulites du Sri Lanka, âgées de ± 0,6 Ga, mais n'excède pas 0,1 à 0,2 Ga pour le Lewisien et les gneiss de Nuk. Des pertes sévères en U et en Th sont responsables des rapports Pb actuels peu radiogéniques dans le Lewisien et les gneiss de Nuk. Par contre, les granulites du Sri Lanka se sont maintenues dans des conditions de rapports U/Pb et Th/Pb élevés et fournissent des rapports isotopiques analogues à ceux de la croûte supérieure actuelle. Par rapport aux compositions mantéliques primitives, les isotopes du Pb identifient le Lewisien et les formations de Nuk comme des réservoirs crustaux appauvris en Th et en U (par rapport au Pb), tandis que les granulites du Sri Lanka ont été enrichies. Le bilan de masse des isotopes du Pb à l'échelle globale requiert l'existence d'un ou de plusieurs réservoirs à faible U/Pb, faible Th/Pb et haut Th/U; la croûte inférieure pourrait constituer ce réservoir. Des formations très métamorphiques comme celles du Sri Lanka présentent un appauvrissement des teneurs en U et en Th par rapport au Pb, mais ne montrent pas les signatures isotopiques du Pb correspondant à un modèle de croûte inférieure globale. Les gneiss archéens de degré élevé possèdent la combinaison adéquate des rapports Th/Pb et U/Pb déprimés, bien que leurs compositions absolues soient moins radiogéniques que celle de la »croûte inférieure type« prévue par les bilans de masse.
    Notes: Zusammenfassung Nd-Modellalter, U-Pb-Zirkondaten sowie Pb-Pb-Alter weisen auf vergleichbare Krustenbildungsalter von 2.2–3.0 Ga für den zentralen Granulitgürtel Sri Lankas bzw. 2.8–3.0 Ga für die spätarchaischen Granulitgebiete der Lewisian-(Schottland) und Nuk-Komplexe (südwestliches Grönland) hin. Die extrem lange Zeitspanne von ca. 2 Ga zwischen Krustenbildung und hochgradiger Metamorphose und die daraus resultierende Verarmung an hochinkompatiblen Elementen unterscheidet jedoch die ca. 0.6 Ga alten Granulite der Highland- und Südwest-Gruppe Sri Lankas von den Lewisian- und Nuk-Gneisen. Hier erfolgte die Granulitmetamorphose verhältnismäßig bald nach der Krustenbildung (≤ 0.1–0.2 Ga), und die frühe signifikante Verarmung an U und Th ist verantwortlich für die heutige, wenig radiogene Pb-Isotopie in diesen Gesteinen. Im Gegensatz dazu zeigen Konzentrationsmessungen an den Granuliten Sri Lankas zwar eine Verarmung von U und Th relativ zu Pb, was aber aus der hochradiogenen Pb-Isotopie nicht ersichtlich ist. Der Grund hierfür ist, daß dieser Krustenkomplex eine sehr lange Zeit zur kontinentalen Oberkruste gehörte, mit entsprechend hohen U/Pb- und Th/Pb-Verhältnissen und dem daraus entstandenen Zuwachs an radiogenem Blei. Die terrestrische Massenbilanz des Bleis erfordert, daß die zeitintegrierten erhöhten U/Pb-, Th/Pb- und erniedrigten Th/U-Werte sowohl der Oberkruste als auch fast aller Mantel-derivate durch ein Reservoir, wie z.B. die Unter-kruste, mit langfristig erniedrigtem U/Pb und Th/ Pb und erhöhtem Th/U kompensiert werden muß. Krustenkomplexe wie Sri Lanka, die erst in jüngster Zeit in die Unterkruste versenkt wurden, kommen dafür nicht in Frage. Archaische Granulitgebiete, jedoch, zeigen das entsprechende Th/Pb und U/Pb, wenn auch ihre absolute Zusammensetzung deutlich weniger radiogen ist als es die Modellunterkruste verlangt.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Solar physics 153 (1994), S. 1-17 
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Discussion on the preflare state held at the Ottawa Flares 22 Workshop focused on the interpretation of solar magnetograms and of Hα filament activity. Magnetograms from several observatories provided evidence of significant build up of electric currents in flaring regions. Images of X-ray emitting structures provided a clear example of magnetic relaxation in the course of a flare. Emerging and cancelling magnetic fields appear to be important for triggering flares and for the formation of filaments, which are associated with eruptive flares. Filaments may become unstable by the build up of electric current helicity. Examples of heliform eruptive filaments were presented at the Workshop. Theoretical models linking filaments and flares are briefly reviewed.
    Type of Medium: Electronic Resource
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  • 4
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Through coordinated observations made during the Max'91 campaign in June 1989 in Potsdam (magnetograms), Debrecen (white light and Hα), and Meudon (MSDP), we follow the evolution of the sunspot group in active region NOAA 5555 for 6 days. The topology of the coronal magnetic field is investigated by using a method based on the concept of separatrices - applied previously (Mandriniet al., 1991) to a magnetic region slightly distorted by field-aligned currents. The present active region differs by having significant magnetic shear. We find that the Hα flare kernels and the main photospheric electric current cells are located close to the intersection of the separatrices with the chromosphere, in a linear force-free field configuration adapted to the observed shear. Sunspot motions, strong currents, isolated polarities, or intersecting separatrices are not in themselves sufficient to produce a flare. A combination of them all is required. This supports the idea that flares are due to magnetic reconnection, when flux tubes with field-aligned currents move towards the separatrix locations.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 372 (1994), S. 63-68 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Many hitherto puzzling features of the isotope and trace-element geochemistry of the Earth's mantle and crust can be explained if Earth history is punctuated by episodes of enhanced exchange between the lower and upper mantle. Such episodes would replenish the upper mantle with trace elements, and ...
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Inflammation research 43 (1994), S. 79-81 
    ISSN: 1420-908X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Type of Medium: Electronic Resource
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  • 7
    ISSN: 1432-1831
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Abstract Immunodominant proteins are variable in molecular and antigenic structure among different genospecies of Borrelia burgdorferi sensu lato. We have recently developed an immunoblot using five recombinant antigens: the chromosomal-encoded B. burgdorferi proteins p 100, the flagellin and an internal flagellin fragment thereof, and the plasmid-encoded outersurface proteins A (OspA) and C (OspC). In the present study the same antigens (derived from strain PKo, genospecies B. afzelii) were compared with the homologous recombinant proteins from strain B31 (genospecies B. burgdorferi sensu stricto) and with OspA, OspC and the internal flagellin fragment from strain PBi (genospecies B. garinii). Patients with neuroborreliosis (n=28) and patients with acrodermatitits chronica atrophicans (n=20) were investigated in the IgG immunoblot; the IgM immunoblot was performed only in patients with neuroborreliosis. There was a small increase in the detection rate of OspA-specific IgG or IgM antibodies using the different variants of recombinant OspA; however, OspA remained an insensitive antigen for antibody detection in Lyme borreliosis. The same was true to OspC-specific IgG antibodies. The sensitivity of OspC, which is the immunodominant antigen for IgM antibody detection, could not be increased using recombinant antigens derived from different strains. However, some sera which were negative in the recombinant immunoblot reacted with OspC in the conventional immunoblot using B. burgdorferi whole cell lysate as antigen. The most unexpected finding was the high degree of immunological heterogeneity of the internal flagellin fragments: IgG antibodies were detected in 18 of 48 patients using B31 fragments, in 25 of 48 using PKo fragments, in 23 of 48 using PBi fragments versus 33 of 48 when the three recombinant proteins were combined. PKo-derived fragments were more sensitive for antibody detection in patients with acrodermatitis chronica atrophicans, B31- and PBi-derived fragments for antibody detection in patients with neuroborreliosis. This is in agreement with the fact that isolates from patients with neuroborreliosis are predominantly belonging to the genospecies B. burgdorferi sensu stricto and B. garinii. For detection of IgM antibodies in sera from patients with neuroborreliosis, recombinant internal fragments derived from strains B31 and PBi were more sensitive than the PKo-derived fragment. The best discrimination between neuroborreliosis sera and control sera was achieved when the IgM blot was performed using recombinant internal flagellin fragments derived from strains PKo and PBi and OspC derived from B31 or PKo.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Fresenius' Zeitschrift für analytische Chemie 350 (1994), S. 642-644 
    ISSN: 1618-2650
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology
    Notes: Abstract Isotope dilution measurements of geological reference materials are described using a newly developed multi-ion counting (MIC) system for a spark source mass spectrometer. Compared with the conventional photoplate detection system, there are considerably improved analytical features of the MIC system, especially the high sensitivity which leads to short measuring times of 1 min to 1 h for trace element analysis on the μg/g — ng/g level.
    Type of Medium: Electronic Resource
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  • 9
    ISSN: 1573-4803
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Notes: Abstract The interaction of PAN-based T800H type carbon fibres, which had been coated with (i) pyrocarbon and (ii) pyrocarbon+SiC protective layers, was studied by means of SEM, energy-dispersive X-ray analysis and Auger electron spectroscopy. The interaction occurred during the pressure infiltration process at temperatures from 898 to 908 K and at contact times of 4–30 s. As detected by AES measurements, both Mg and Li penetrated throughout the carbon fibres, and Li2C2 was formed without remarkable reaction zone occurrence, which led to carbon fibre degradation. The pyrocarbon layer (about 50 nm thick) demonstrated a good protective efficiency and the corresponding metal-matrix composite exhibited satisfying strength characteristics; nevertheless, the influence of processing variables (temperature, time) was obvious. On the other hand, the double-coated pyrocarbon+SiC carbon fibres were strongly affected by Li2C2 formation.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Hyperfine interactions 89 (1994), S. 221-242 
    ISSN: 1572-9540
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Positronium formation (Ps) cross sections for positrons impinging on atomic hydrogen were measured in the impact energy range from 13 to 255 eV at the High Intensity Positron (HIP) beam at Brookhaven National Laboratory (BNL). The Ps-formation cross section was found to rise rapidly from the threshold at 6.8 eV to a maximum value of (2.98±0.18) ×10−16 cm2 for ∼15 eV positrons. By 75 eV it drops below the detection limit of 0.17×10−16 cm2 which is the present level of statistical uncertainty. A more elaborate data analysis was performed leading to somewhat smaller cross sections than originally published [1]. During the course of this experiment further relative data on impact-ionization cross sections were accumulated.
    Type of Medium: Electronic Resource
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