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  • 1
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Boring -- Congresses. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (374 pages)
    Edition: 1st ed.
    ISBN: 9783540687788
    DDC: 550
    Language: English
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  • 2
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Cryptoexplosion structures -- Congresses. ; Geology, Structural -- Congresses. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (570 pages)
    Edition: 1st ed.
    ISBN: 9783540275480
    Series Statement: Impact Studies
    DDC: 551.3/97
    Language: English
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  • 3
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Cryptoexplosion structures--Chesapeake Bay (Md. and Va.). ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (528 pages)
    Edition: 1st ed.
    ISBN: 9783642189005
    Series Statement: Impact Studies
    Language: English
    Note: Impact Studies -- The Chesapeake Bay Crater -- Copyright -- Preface -- Acknowledgments -- Contents -- 1 Introduction -- 2 Geological Framework of Impact Site -- 3 Geophysical Framework of Impact Site -- 4 The Primary Crater -- 5 Secondary Craters -- 6 Synimpact Crater-Fill Deposits -- 7 Initial Postimpact Deposits -- 8 Age of Chesapeake Bay Impact Crater -- 9 Geological Consequences of Chesapeake Bay Impact -- 10 Comparisons with Other Impact Craters -- 11 Comparisons Between lmpactites -- 12 Implications for Impact Models -- 13 Biospheric Effects of Chesapeake Bay Impact -- 14 Residual Effects of Chesapeake Bay Impact -- 15 Summary and Conclusions -- Appendix -- References -- Index.
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  • 4
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Cryptoexplosion structures. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (360 pages)
    Edition: 1st ed.
    ISBN: 9783642554636
    Series Statement: Impact Studies
    DDC: 551.3/97
    Language: English
    Note: Impact Studies -- Impact Markers in the Stratigraphic Record -- Copyright -- Preface -- Contents -- List of Contributors -- The Stratigraphic Record of Impact Events: A Short Overview -- Application of stratigraphic nomenclature to terrestrial impact-derived and impact-related materials -- Main Geochemical Signatures Related to Meteoritic Impacts in Terrestrial Rocks: A Review -- Impact Decompression Melting: A Possible Trigger for Impact Induced Volcanism and Mantle Hotspots ? -- Displacement of Target Material During Impact Cratering -- Obscure-bedded Ejecta Facies from the Popigai Impact Structure, Siberia: Lithological Features and Mode of Origin -- Biostratigraphic Indications of the Age of the Boltysh Impact Crater, Ukraine -- Ejecta of the Boltysh Impact Crater in the Ukrainian Shield -- Stratigraphy and Sedimentology of Coarse Impactoclastic Breccia Units within the Cretaceous-Tertiary Boundary Section, Albion Island, Belize -- New Geochemical Insights from Electron-Spin- Resonance Studies of Mn2+ and SO3 - in Calcites: Quantitative Analyses of Chicxulub Crater Ejecta from Belize and Southern México with Comparison to Limestones from Distal Cretaceous-Tertiary-Boundary Sites -- Petrography and Geochemistry of a Deep Drill Core from the Edge of the Morokweng Impact Structure, South Africa -- Stratigraphy, Paleomagnetic Results, and Preliminary Palynology across the Permian-Triassic (P-Tr) Boundary at Carlton Heights, Southern Karoo Basin (South Africa) -- Search for an Extraterrestrial Component in the Late Devonian Alamo Impact Breccia (Nevada): Results of Iridium Measurements -- The Osmussaar Breccia in Northwestern Estonia - Evidence of a ~475 Ma Earthquake or an Impact?.
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  • 5
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Planetology. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (391 pages)
    Edition: 1st ed.
    ISBN: 9783540257363
    Series Statement: Impact Studies
    DDC: 577.2
    Language: English
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  • 6
    ISSN: 1365-3121
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: In a recent article in Terra Nova, Kristan-Tollmann and Tollmann (1994) suggested that the Biblical Flood can be explained by seven fragments of a comet that impacted the ocean at seven locations on Earth at 03.00h (C.E.T.) on 23 September, 9545 yr BP. We demonstrate that all the ‘geological proofs’ that allegedly support their conclusions are not supported by the available data on impact cratering. Their hypothesis is based on insufficient and ambiguous data, selective citation, and incomplete comprehension of previous research.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 378 (1995), S. 17-18 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] DIAMONDS have long caused excitement not only among the general public, which appreciates them mainly for their beauty and value, but also among geologists. The latter use diamonds in a not very glam-orous way as probes of the properties of the Earth's mantle, which is otherwise rather ...
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 79 (1990), S. 327-335 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Abstract The major and trace element geochemistry of magnesite and dolomite samples from alternating rock masses at the Oberdorf/Laming (Styria, Austria) mineralization has been studied. The rare earth elements (REE) are considered to be of importance for the discussion of the origin of sparry magnesite deposits. The Al and REE contents are positively correlated, indicating a clay component as the main source for REE in the magnesites and their precursor rocks. Our data support the view that the Oberdorf and probably other magnesite mineralizations in the Eastern Alps have been formed by metasomatism. Through this process calcite (which was deposited by sedimentation in a marine environment) underwent dolomitization. Subsequently, Mg-rich solutions circulating through the rock masses formed the magnesite bodies. During the formation of the dolomites and the conversion to magnesites, the REE patterns of the original carbonates remained unchanged. The magnesites exhibit patterns that are very similar to sedimentary carbonates (which contain a REE-bearing clay component). Magnesites of purely sedimentary origin, formed in a predominantly evaporitic environment, should have lower total REE contents and different patterns due to the short residence times of these elements in seawater. Analyses of talc pseduomorphs after magnesite indicate as well that the REE patterns are not significantly altered during the talcification. The Mg-rich solutions that led to the formation of the magnesites have probably been derived from serpentinites below the gneiss complexes of eastern Styria and the South Penninic units of the Tauern window.
    Abstract: Résumé Cette note présente les résultats d'une étude géochimique des éléments majeurs et en trace d'échantillons de magnésite et de dolomite qui se présentent en masses alternées dans la mine de magnésite de Oberdorf/Laming (Steiermark, Autriche). Une attention particulière a été apportée aux terres rares, considérées comme fournissant des arguments importants dans la discussion de l'origine des gisements. Les teneurs en Al et en terres rares montrent une corrélation positive, ce qui permet de rapporter à un composant argileux la source principale des terres rares. Les résultats obtenus plaident en faveur d'une origine métasomatique des minéralisations en magnésite d'Oberdorf et d'autres endroits des Alpes orientales. Au cours de ce processus, la calcite, d'origine sédimentaire marine, a été le siège d'une dolomitisation avec, subséquemment, formation de corps de magnésite grâce à la circulation de solutions riches en Mg. Au cours de la métasomatose, la distribution des terres rares des carbonates originels n'est pas modifiée: les magnésites montrent des répartitions très semblables à celles des carbonates sédimentaires (lesquels renferment un constituant argileux porteur des terres rares). Des magnésites d'origine purement sédimentaires, formées en milieu évoporitique, doivent présenter un contenu total en terres rares moins élevé et une distribution différente de ces éléments, eu égard à la brièveté de leur séjour dans l'eau de mer. Des analyses de pseudomorphoses de magnésite en talc montrent de même que la distribution des terres rares n'est pas modifiée de manière significative au cours de la talcification. Les solutions riches en Mg responsables de la formation de la magnésite sont probablement dérivées de serpentines situées sous les complexes gneissiques de Styrie et les unités penniques méridionales de la fenêtre des Tauern.
    Notes: Zusammenfassung Die Haupt- und Spurenelementgeochemie von Magnesit- und Dolomitproben, die aus alternierenden Gesteinsstöcken in der Magnesitmine von Oberdorf/Laming (Steiermark, Österreich) stammen, wurde untersucht. Besonderes Augenmerk wurde dabei auf die Geochemie der Seltenen Erdelemente (REE) gelegt, da diese für Aussagen über die Entstehung der Magnesitlagerstätten von besonderer Bedeutung sind. Eine positive Korrelation zwischen den Al und REE-Gehalten deutet darauf hin, daß der Hauptteil der REE einer Tonkomponente entstammt. Die Daten unterstützen eine metasomatische Entstehung der Spatmagnesite der Oberdorfer Lagerstätte und anderer Ostalpiner Lagerstätten. Sedimentär angelegter Kalzit wird dabei über Dolomit mit Mg-reichen Lösungen in Magnesit umgewandelt. Während der Metasomatose bleiben die chondritnormierten REE-Verteilungen der Ausgangskarbonate relativ unverändert erhalten. Die so entstandenen Spatmagnesite weisen Verteilungsmuster auf, die jenen der sedimentären Karbonate, aus denen sie entstanden sind, entsprechen. Rein sedimentär entstandene Magnesite werden praktisch nur in evaporitischem Milieu gebildet und sollten infolge der kurzen Verweilzeit dieser Elemente im Meerwasser wesentlich niedrigere REE-Gehalte und andere Verteilungsmuster aufweisen. Analysen einer Talkpseudomorphose zeigen, daß sich die REE-Verteilungsmuster auch bei der metasomatischen Talk-bildung nicht wesentlich ändern. Die Mg-reichen Lösungen, die zur Bildung der Magnesite notwendig waren, entstammen vermutlich tiefliegenden Sepentiniten, auf die es Hinweise im Untergrund der oststeirischen Gneisskomplexe und des südpenninischen Tauernfensters gibt.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 85-86 (1999), S. 179-200 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Classical science fiction films have been depicting space voyages, aliens, trips to the moon, the sun, Mars, and other planets, known and unknown. While it is difficult to critique the depiction of fantastic places, or planets about which little was known at the time, the situation is different for the moon, about which a lot of facts were known from astronomical observations even at the turn of the century. Here we discuss the grade of realism with which the lunar surface has been depicted in a number of movies, beginning with George Méliés' 1902 classic Le Voyage dans la lune and ending, just before the first manned landing on the moon, with Stanley Kubrick's 2001: A Space Odyssey. Many of the movies present thoughtful details regarding the actual space travel (rockets), but none of the movies discussed here is entirely realistic in its portrayal of the lunar surface. The blunders range from obvious mistakes, such as the presence of a breathable atmosphere, or spiders and other lunar creatures, to the persistent vertical exaggeration of the height and roughness of lunar mountains. This is surprising, as the lunar topography was already well understood even early in the 20th century.
    Type of Medium: Electronic Resource
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  • 10
    ISSN: 1573-0794
    Keywords: History ; impact craters ; lunar craters ; lunar maps
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The origin of lunar craters has been discussed for centuries,since they were discovered by Galilei in 1609. The majority of researchers were of the opinion that they are volcanic structures, but a variety of “exotic” explanations that included tidal forces, circular glaciers, and coral atolls was also considered. The meteorite impact hypothesis had been discussed a few times, starting with Hooke in 1665, and formulated in more detail by Proctor in 1873 and Gilbert in 1893. However, this theory only gained momentum early in the 20th century, after the identification of Meteor Crater in Arizona as an impact structure, and after specific and plausible physical models for impact craters formation were devised by Öpik in 1916, Ives in 1919, and Gifford in 1924. Nevertheless, despite growing evidence for the interpretation that most craters formed by impact, proponents of the volcanic theory impact were still vociferous as late as 1965, just four years before the first samples were brought back from the moon. Important lessons could have been learned for the study of impact craters on the Earth, especially in view of evidence that large impactevents had some influence on the geologic and biologic evolution of the Earth.
    Type of Medium: Electronic Resource
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