Zur Reinigung organisch verschmutzter Abwässer im Stabilisierungsteichsystem Warnitz     

G. P. Schmidt  S. Schwarz 《洁净——土壤、空气、水》1976,4(4):345-351

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Improvement of the geoid in local areas by satellite gradiometry     

K. P. Schwarz  J. Kryński 《Journal of Geodesy》1977,51(3):163-176

Summary Satellite gradiometry is studied as a means to improve the geoid in local areas from a limited data coverage. Least-squares collocation is used for this purpose because it allows to combine heterogeneous data in a consistent way and to estimate the integrated effect of the attenuated spectrum. In this way accuracy studies can be performed in a general and reliable manner. It is shown that only three second-order gradients contribute significantly to the estimation of the geoidal undulations and that it is sufficient to have gradiometer data in a 5°×5° area around the estimation point. The accuracy of the geoid determination is strongly dependent on the degree and order of the reference field used. An accuracy of about ±1 m can be achieved with a reference field of (12, 12). There is an optimal satellite altitude for each reference field and this altitude may be higher than 300 km for a field of low degree and order. The influence of measuring errors is discussed and it is shown that only gradiometer data with accuracies better than ±0.05 E will give a significant improvement of the geoid. Finally, some results on the combination of satellite gradiometry and terrestrial gravity measurements are given. The proposed method seems to be well suited for local geoid determinations down to the meter range. It is especially interesting for unsurveyed and difficult areas because no terrestrial measurements are necessary. Furthermore, it has the practical advantage that only a local data coverage is needed.  相似文献   

Sedimentationszyklen und stratigraphisch-fazielle Probleme der Randfazies des Unteren Muschelkalkes (Kernbohrung Mersch/ Luxemburg)     

Hans -Ulrich Schwarz 《International Journal of Earth Sciences》1977,66(1):34-61

Zusammenfassung Ausgehend von einem Vergleich randnaher Normprofile und der faziellen Analyse eines vollständigen Bohrprofils wird für die Randfazies des Unteren Muschelkalkes ein Sedimentationsmodell entwickelt, das auf der Basis klimatisch und epirogenetisch bedingter Untergliederungen des Profils neue Parallelisierungsmöglichkeiten mit beckenwärtigen Faziesbereichen eröffnet.Hervorstechendste Merkmale des Bohrprofils sind rhythmisches Auftreten von Magnesit — der als sedimentäre Bildung bislang nur in Zusammenhang mit chloridischen Evaporiten bekannt war —, eine sedimentologisch und geochemisch begründete zyklische Gliederung sowie intensive Bioturbation und zugleich durchgehende Vergipsung.Die Zyklen sind formal gekennzeichnet durch Koppelung von tonigem Sandstein mit geringen Eisen- und hohen Magnesiumgehalten einerseits und von rotem Ton und Silt mit hohen Eisen- und niedrigen Magnesiumwerten andererseits. Die Zyklen werden als Wechselfolge von litoralen Sedimentationsphasen in subtropischem Klima und Abschnürungsphasen mit Hungersedimentation in aridem Klima interpretiert. Der syndiagenetisch gebildete Magnesit ist dabei Tonsedimentationsphasen genetisch zugeordnet. Anhand der Verteilung der vier nicht-detritischen Hauptminerale Dolomit, Gips, Anhydrit und Magnesit wird der Diageneseablauf rekonstruiert.Nach einer Diskussion der Bildungsumstände und der Korrelierbarkeit bieten sich die Werksteinzone der Randfazies und die Spiriferinabank der Beckenfazies als sedimentologische Zeitmarke an.

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A depositional model of the marginal facies of the Lower Muschelkalk (Middle Triassic) is developed by comparison of near-marginal profiles and a facies analysis of a complete drilling record. It is based upon climatologically and epirogenetically caused partitions of the profile and opens new possibilities of correlation with basinal areas.Significant features of the drilling record are rhythmic occurrences of magnesite in sediments only known in connection with chloridic evaporites, a cyclic deposition based on sedimentological and geochemical criteria, and intensive bioturbation with a gypsification throughout.The cycles are formally marked by the correlation of clayey sandstone with low iron and high magnesium contents at the one hand and of red clay and silt with high iron and low magnesium values at the other hand. The cycles are interpreted as an alternation of littoral sedimentation under a subtropical climate and of stages of lagoonal conditions or emersion under an arid climate. The magnesite syndiagenetically formed is genetically attached to stages of clay sedimentation. The process of diagenesis is reconstructed studying the distribution of four main non-detrital minerals: dolomite, gypsum, anhydrite, and magnesite.After discussion of the depositional conditions and the possibilities of correlation, the Werkstein-Zone of the marginal facies and the Spiriferina-Bank of the basinal facies are thought to be sedimentological time markers.

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Résumé Une conception de la formation du facies marginal du Muschelkalk inférieur est développée sur la base d'une comparaison entre les profils normés de la région de sondage Mersch/Luxembourg et l'analyse facielle du profil complet de la carotte de ce sondage. A partir des divisions en partie causées par les climats et par des mouvements épirogénétiques, cette conception donne une nouvelle possibilité de corrélation avec le facies situé plus au centre du bassin sédimentaire.Le forage étudié est caractérisé par la présence rythmique de magnésite, qui, jusqu'à présent, était seulement connu en tant que formation sédimentaire, avec des évaporites, par une répartition cyclique basée sur des observations sédimentologiques et géochimiques et par une bioturbation intensive ainsi qu'une gypsification générale.Les cycles sont caractérisés formellement par le couplage d'un grès argileux à faible teneur en fer et à forte teneur en magnésium d'une part et d'argile rouge à forte teneur en fer et à faible teneur en magnésium d'autre part. Les cycles sont interpretés comme une séquence alternante comprenant une sédimentation littorale en climat subtropical et une sédimentation lagunaire ou d'émersion en climat aride. La magnésite formée syndiagénétiquement est donc coordonnée à une phase sédimentaire argileuse. Le cours de la diagénèse est reconstruit à partir de l'étude de la répartition des quatre minéraux principaux non-détriques: dolomite, gypse, anhydrite et magnésite.A la suite de la discussion des conditions de formation et des possibilités de corrélation la « Werkstein-Zone » du facies marginal et la « Spiriferina-Bank » du facies central apparaissent comme des indicateurs sédimentologiques chronostratigraphiques.

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SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h     

P. Rodríguez-Gil  B. T. Gänsicke  H.-J. Hagen  S. Araujo-Betancor  A. Aungwerojwit  C. Allende Prieto  D. Boyd  J. Casares  D. Engels  O. Giannakis  E. T. Harlaftis  J. Kube  H. Lehto  I. G. Martínez-Pais  R. Schwarz  W. Skidmore  A. Staude  M. A. P. Torres 《Monthly notices of the Royal Astronomical Society》2007,377(4):1747-1762

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The use of FFT techniques in physical geodesy   总被引：20，自引：0，他引：20  

K. P. Schwarz  M. G. Sideris  R. Forsberg 《Geophysical Journal International》1990,100(3):485-514

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Swift observations of the X-ray and UV evolution of V2491 Cyg (Nova Cyg 2008 No. 2)     

K. L. Page  J. P. Osborne  P. A. Evans  G. A. Wynn  A. P. Beardmore  R. L. C. Starling  M. F. Bode  A. Ibarra  E. Kuulkers  J.-U. Ness  G.J. Schwarz 《Monthly notices of the Royal Astronomical Society》2010,401(1):121-130

We present extensive, high-density Swift observations of V2491 Cyg (Nova Cyg 2008 No. 2). Observing the X-ray emission from only one day after the nova discovery, the source is followed through the initial brightening, the super-soft source phase and back to the pre-outburst flux level. The evolution of the spectrum throughout the outburst is demonstrated. The UV and X-ray light curves follow very different paths, although changes occur in them around the same times, indicating a link between the bands. Flickering in the late-time X-ray data indicates the resumption of accretion. We show that if the white dwarf (WD) is magnetic, it would be among the most magnetic known; the lack of a periodic signal in our later data argues against a magnetic WD, however. We also discuss the possibility that V2491 Cyg is a recurrent nova, providing recurrence time-scale estimates.  相似文献   

大兴安岭中南段中生代成矿物质的深部来源与背景   总被引：19，自引：3，他引：16  

邵济安  牟保磊  朱慧忠  张履桥 《岩石学报》2010,26(3):649-656

大兴安岭是我国北方一个重要的多金属成矿带。本文从成矿的物质来源和构造作用两方面讨论大兴安岭的成矿系统。Sr、Nd、O、Pb同位素的研究显示大兴安岭成矿物质的深部来源,大兴安岭晚中生代壳幔混熔花岗质岩石组成及其构造环境的研究,表明它们是在板内非造山的伸展环境下形成的A型花岗岩。与南岭花岗岩及其成矿作用的对比研究,将加深对大兴安岭中生代成矿特征的认识。深部构造特征也进一步印证了大兴安岭的成岩-成矿的背景。  相似文献   

40Ar‐39Ar step‐heating of impact glasses from the Nördlinger Ries impact crater—Implications on excess argon in impact melts and tektites     

Winfried H. Schwarz  Hans J. Lippolt 《Meteoritics & planetary science》2014,49(6):1023-1036

Seven impact melts from various places in the Nördlinger Ries were dated by ⁴⁰Ar‐³⁹Ar step‐heating. The aim of these measurements was to increase the age data base for Ries impact glasses directly from the Ries crater, because there is only one Ar‐Ar step‐heating spectrum available in the literature. Almost all samples display saddle‐shaped age spectra, indicating the presence of excess argon in most Ries glass samples, most probably inherited argon from incompletely degassed melt and possibly also excess argon incorporated during cooling from adjacent phases. In contrast, moldavites usually contain no inherited argon, probably due to their different formation process implying solidification during ballistic transport. The plateau age of the only flat spectrum is 14.60 ± 0.16 (0.20) Ma (2σ), while the total age of this sample is 14.86 ± 0.20 (0.22) Ma (isochron age: 14.72 ± 0.18 [0.22] Ma [2σ]), proofing the chronological relationship of the Ries impact and moldavites. The total ages of the other samples range between 15.77 ± 0.52 and 20.4 ± 1.0 Ma (2σ), implying approximately 2–40% excess ⁴⁰Ar (compared to the nominal age of the Ries crater) in respective samples. Thus, the age of 14.60 ± 0.16 (0.20) (2σ) (14.75 ± 0.16 [0.20 Ma] [2σ], calculated using the most recent suggestions for the K decay constants) can be considered as reliable and is within uncertainties indistinguishable from the most recent compilation for the age of the moldavite tektites.  相似文献   

Coeval argon‐40/argon‐39 ages of moldavites from the Bohemian and Lusatian strewn fields     

Winfried H. Schwarz  Hans J. Lippolt 《Meteoritics & planetary science》2002,37(12):1757-1763

Abstract— ⁴⁰Ar/³⁹Ar ages of four tektites (moldavites) from southern Bohemia (near ?eské Budějovice, Czech Republic) and a tektite from Lusatia (near Dresden, Germany) have been determined by 11 step‐degassing experiments. The purpose of the study was to enlarge the ⁴⁰Ar/³⁹Ar data base of moldavites and to check the age relations of the Bohemian and Lusatian samples. The mean plateau‐age of the Bohemian samples, which range from 14.42 to 14.70 Ma, is 14.50 ± 0.16 (0.42) (2σ) Ma (errors in parentheses include age error and uncertainty of standard monitor age). The plateau age of the Lusatian sample of 14.38 ± 0.26 (0.44) (2σ) Ma confirms the previously published ⁴⁰Ar/³⁹Ar age of 14.52 ± 0.08 (0.40) (2σ) Ma, and demonstrates that the fall of Lusatian and Bohemian tektites were contemporaneous. Because of their geochemistry and their ages there is no doubt that the Lusatian tektites are moldavites. Accepting that moldavites are ejecta from the Nördlinger Ries impact, the new ages also date the impact event. This age is slightly younger (about 0.2–0.3 Ma) than the age suggested by earlier K‐Ar determinations.  相似文献   

The magnetic properties of Quaternary and Tertiary sediments in the southern North Sea     

R. Thompson  T. D. J. Cameron  C. Schwarz  K. A. Jensen  V. Van Maenhaut Lemberge  L. P. Sha 《第四纪科学杂志》1992,7(4):319-334

Cores from boreholes penetrating late Quaternary, glacial, interglacial and postglacial sediments and the underlying late Cenozoic delta complex of the southern North Sea have been examined for their magnetic properties. A magnetic polarity stratigraphy has been established as an aid to biostratigraphic dating of the sediments; the Kaena-Gauss and Gauss—Matuyama transitions and the base and top of the Olduvai subchron have been identified. The strength and stability of laboratory-induced isothermal remanent magnetisation display clear magneto-petrological variations, which match lithostratigraphic changes in the cores. Principal component analysis has picked out a basin-wide and palaeoenvironmental consistency in the magnetic data. Large, multi-domain magnetite grains predominate in the post-deltaic and fluvio-deltaic sediments, whereas smaller greigite or titanomagnetite grains are concentrated in the intertidal and marine deltaic facies. Since heavy mineral analysis indicates that most of the deltaic detritus derived from common source areas, the differences in magnetic mineralogy have probably been caused by the sediment transport processes operating within the delta complex.  相似文献