Parallelisierung des norddeutschen oberen Muschelkalks mit dem süddeutschen Hauptmuschelkalk anhand von Sedimentationszyklen

The interpretation of microfacial and geochemical sediment features resulted in a detailed sequence analysis of Upper Muschelkalk strata in the northern and middle parts of West-Germany. It is now possible to correlate columnar sections at far distances. The method allows to make a synthesis of basin evolution. In this way it also succeed to reconstruct the dynamic activities in an epicontinental sedimentation area. The Upper Muschelkalk strata shows a hierarchically nested development of stratification cycles. There are minor cycles of probably paleotectonic origin, which are only locally significant. The major cycles are basing probably on sea level changes and allow supraregional parallelizations of sections. Indicators of the sea level maximums are clay horizons. They are called »Tonhorizonte« in Southern Germany and could be proved also in the Upper Muschelkalk strata of Northern Germany. So the stratigraphic correlation of the two sedimentation areas, which were so different in paleotectonic views, is possible.     

Age and evolution of scheelite-hosting rocks in the Felbertal deposit (Eastern Alps): U-Pb geochronology of zircon and titanite

U-Pb isotope analyses of zircon and titanite extracted from different rocks of the Felbertal scheelite deposit yield the following information: (1) An age of 593±22 Ma (2) is obtained for zircon crystallization in the scheelite-bearing matrix of an eruption breccia in the western ore field. (2) Discordant zircons from an elongated, up to 8 m thick scheelite-rich quartzite body in the eastern ore field give an upper intercept age of 544±5 Ma. This quartzite contains a laminated, fine-grained scheelite mineralization. (3) Zircons from a small granitoid intrusion of the western ore field reveal an age of 336±16 Ma, and concordant titanites document an age of 282±2 Ma for Variscan amphibolite facies metamorphism. Both events, granitoid intrusion and later metamorphism caused ore re-mobilization, including the formation of yellowish fluorescent (molybdo-) scheelite porphyroblasts. (4) For a narrow lamprop-1hyric dike in the western ore field, a concordant titanite age of 283±7 Ma is obtained. This age is identical with the titanites from the amphibolite facies metamorphic intrusion. Tiny scheelite grains were tapped by the dike from pre-existing scheelite mineralizations in the truncated host rocks. (5) Alpine metamorphism at 31±4 Ma did not exceed lowermost amphibolite facies conditions, and it caused scheelite re-mobilization on a minor scale only, producing bluish fluorescent porphyroblasts in quartz veinlets and veins, as well as bluish fluorescent scheelite rims around older scheelite grains. Moreover, crosscutting Alpine fissure fillings show bluish fluorescent, inclusion-free scheelite. (6) The preservation of Variscan titanites, the absence of Alpine titanite growth, and the large degree of Variscan scheelite re-mobilization demonstrate that amphibolite facies metamorphism in the Felbertal area has a Variscan age. This result clearly documents Variscan tectono-metamorphism to be the dominant event, instead of the hitherto surmised Alpine metamorphism. This multi-stage evolution of the Felbertal ore bodies corroborates the view that tungsten deposits are conditioned by several succeeding thermal events, leading to a series of stages that ultimately produce high-grade scheelite concentrations. These high-grade ores predominately occur along shear zones of different age, accompanied by the formation of large volumes of low-grade scheelite mineralizations along host rock foliations and quartz veinlets and veins.     

Age,origin and geodynamic significance of a polymetamorphic felsic intrusion in the Ötztal Crystalline Basement,Tirol, Austria

Summary A multi-method approach was applied to derive the age and origin of an orthogneiss body located in the central Kaunertal, western Ötztal Crystalline Basement (ÖCB). The Tieftal orthogneiss body is an internally differentiated, polymetamorphosed epizonal intrusion, embedded in amphibolites. It comprises leucocratic hedenbergite-hornblende-, hornblende- and biotite-hornblende-gneisses, but also some melanocratic rock types. The leucocratic Tieftal gneisses are granitic, have a near eutectic melt composition and share some features of A-type granites, such as high Na₂O+K₂O(8.07 to 8.58wt%), Zr (379 to 554ppm) and Y (58 to 79ppm) contents. The REE-patterns are rather flat ((La/Yb)_N=2.4 to 3.7), with distinct negative Eu anomalies. Single zircon evaporation dating of two samples and Sm-Nd dating of relict magmatic titanite resulted in ages of 487±7, 484±3 and 487±5Ma, respectively. The weighted mean of 485±3Ma is interpreted as the primary crystallization age of the Tieftal orthogneiss body. Rb-Sr whole rock dating results in a well defined regression line, corresponding to an age of 411±9Ma. This age clearly documents at least a partial resetting of the whole rock Rb-Sr system, which is most probably due to subsequent metamorphic overprint. The leucocratic Tieftal gneisses are isotopically rather primitive with an Nd _CHUR ^{485 Ma} value of +1.7 and a calculated magmatic initial⁸⁷Sr/⁸⁶Sr ratio of 0.7047. These data suggest a major mantle contribution. Most probably, they originated through fractionation of the magmatic precursors of the accompanying tholeiitic metabasites. The more primitive isotopic composition of ÖCB metabasites and some late Archean/early Proterozoic and Cambrian inheritance in Tieftal gneiss zircons suggest some involvement of old crustal rocks, too. The amount of crustal contamination can be calculated to be in the range of 10 to 40%. The Tieftal gneisses and the accompanying metabasites are interpreted as remnants of igneous rocks related to an early Ordovician rifting and incipient formation of new oceanic crust, an event which can be traced throughout the central and western European Variscan and Alpine terranes.

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Alter, Genese und geologische Bedeutung einer polymetamorphen felsischen Intrusion im Ötztalkristallin, Tirol, Österreich

Zusammenfassung Ein Vielzahl von Methoden wurde angewandt, um das Alter und die Genese eines Orthogneiskörpers im mittleren Kaunertal, westliches Ötztalkristallin, abzuleiten. Der Tieftal-Orthogneiskörper ist eine in Amphiboliten eingeschaltete, intern differenzierte, polymetamorph überprägte, epizonale Intrusion. Er umfaßt sowohl leukokrate Hedenbergit-Hornblende-, Hornblende- und Biotit-Hornblende-Gneise als auch untergeordnet melanokrate Gesteine. Die leukokraten Tieftal-Gneise besitzen einen granitischen, beinahe einer eutektischen Schmelze entsprechenden Chemismus; einige Parameter wie hohe Na₂O+K₂O(8.07 bis 8.58Gew%), Zr(379 bis 554ppm) und Y(58 bis 79ppm) Gehalte weisen auf eine A-Typ Affinität hin. Die SEE-Spektren sind nur gering fraktioniert ((La/Yb)_N=2.3 bis 3.7) und weisen eine markante negative Eu-Anomalie auf. Einzelzirkon-Evaporationsdatierungen an 2 Proben und eine Sm-Nd Datierung von reliktischem magmatischem Titanit ergeben Alter von 487±7, 484±3 und 487±5Ma. Der gewichtete Mittelwert von 485±3Ma wird als das primäre magmatische Kristallisationsalter des Tieftal-Orthogneiskörpers interpretiert. Eine Rb-Sr Gesamtgesteinsdatierung ergibt eine gut definierte Regressionsgerade mit einem Alter von 411±9Ma. Dieses Alter beweist eine postmagmatische Störung des Rb-Sr Gesamtgesteinssystems, die durch die metamorphen überprägungen verursacht wurde. Die leukokraten Tieftal-Gneise besitzen eine relative primitive isotopische Zusammensetzung mit einem Nd _CHUR ^{485 Ma} a Wert von +1.7 und einem zurückgerechneten magmatischen⁸⁷Sr/⁸⁶Sr Initialverhältnis von 0.7047. Diese Daten machen eine große Beteiligung von Mantelmaterial wahrscheinlich. Am ehesten entstanden die leukokraten Tieftal-Gneise durch magmatische Fraktionierungsprozesse aus den Ausgangsgesteinen der begleitenden tholeiitischen Metabasite. Die noch primitivere isotopische Zusammensetzung der Metabasite im Ötztalkristallin und spätarchaische/frühproterozoische sowie kambrische Komponenten in den Zirkonen der leukokraten Tieftal-Gneise weisen aber auch auf die Beteiligung alten krustalen Materials hin. Der Anteil der krustalen Komponente liegt im Bereich von 10 bis 40%. Der Tieftal-Orthogneiskörper und die begleitenden Metabasite werden als Relikte magmatischer Gesteine, die während eines frühordovizischen Riftings und der beginnenden Bildung neuer ozeanischer Kruste entstanden sind, gedeutet. Zeugen dieses Vorganges sind in allen variszisch und alpidisch geprägten Gebieten Westund Mitteleuropas zu finden.

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With 13 Figures     

Zircon U/Pb and Pb/Pb geochronology of the Rastenberg granodiorite,South Bohemian Massif,Austria

Summary A combined zircon typology, zircon Pb-Pb evaporation, and conventional U-Pb study of the late- to post-tectonic Rastenberg granodiorite yields the following results: Typological investigations show two distinguishable zircon populations. Type l: subtype S24 ofPupin, colourless to slightly pink, clear to turbid, often with cores, few to abundant inclusions, long prismatic; type 2: subtype S4 ofPupin, colourless to reddish or slightly pink, clear to slightly turbid, no visible cores, abundant inclusions, tabular habit, short prismatic.At least 4 different zircon-forming events can be distinguished: Inherited cores with ages around 623±22Ma and single ages > 1206Ma from type 1 zircons imply the reworking of rocks derived from Cadomian and Proterozoic to Archean crust. Ages around 353±9Ma from type 1 zircons are interpreted as timing a first magma formation or the onset of a long-lasting magma-generating event during the Variscan plutonism in the South Bohemian pluton. The actual intrusion of the granodioritic magma into the middle crust took place around 338±2Ma (type 2 and rims of type 1 zircons).Only type 1 zircons are found as inclusions in large K-feldspar phenocrysts providing evidence that these phenocrysts have grown before the 338Ma event and may be as old as 353 Ma.[]

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Zirkon U/Pb und Pb/Pb Geochronologie des Rastenberger Granodiorits, südliche Böhmische Masse, Österreich

Zusammenfassung Zirkon-typologische Untersuchungen, Einzelzirkon Pb-Pb-Evaporations- und konventionelle U-Pb-Altersbestimmungen an Gesteinen des spät- bis postkinematischen Rastenberger Granodiorits geben folgende Resultate: Typologisch lassen sich zwei Zirkonpopulationen unterscheiden: Typ 1: S24 Subtyp vonPupin, farblos bis leicht rosa, klar bis getrübt, häufig mit Kernen, wenige bis viele Einschlüsse, lang prismatisch; Typ 2: S4 Subtyp vonPupin, farblos bis rötlich oder leicht rosa, klar bis leicht getrübt, keine sichtbaren Kerne, viele Einschlüsse, flachtafeliger Habitus, kurzprismatisch.Mindestens 4 unterschiedliche Altersgruppen lassen sich unterscheiden: Ererbte Kerne von Typ 1 Zirkonen mit Altern um 623±22Ma und einzelnen Altern > 1206Ma sprechen für die Aufarbeitung von Gesteinen, die von cadomischen und proterozoischen bis archaischen Gesteinen im Krustenbereich des Südböhmischen Plutons abstammen könnten. Alter um 353±9Ma von Typ 1 Zirkonen werden einer ersten magmatischen Phase oder dem Beginn der Krustenaufschmelzung im Zuge der Bildung der variszischen Plutonite zugeordnet. Die eigentliche Intrusion des Granodiorits um 338±2Ma wird mit Typ 2 und mit Randpartien von Typ 1 Zirkonen erfaßt.In den großen K-Feldspat-Phänokristallen finden sich nur Zirkone vom Typ 1. Dies deutet darauf hin, daß die Phänokristalle vor dem 338Ma Ereignis gebildet wurden, eventuell also bis 353Ma alt sein können.

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With 6 Figures     

Radial dependence of solar wind parameters in the ecliptic (1.1 R ⊙−61 AU)

The radial dependencies of four solar wind parameters (plasma density N, velocity V, temperature T, and magnitude of the interplanetary magnetic field B) are derived from remote sensing data of the solar corona and from in situ measurements in the heliosphere (Helios-1, 2, Pioneer-10, 11, and Voyager-1, 2). Using doubly logarithmic scaling (solar wind parameter vs radial distance from the Sun) one finds two distinct intervals in the ecliptic, i.e., an exponential section within, approximately, the inner heliosphere and a linear section - up to at least 61 AU - in the outer heliosphere.     

Polarized radiation diagnostics of magnetohydrodynamic models of the solar atmosphere

Solar magnetic elements and their dynamical interaction with the convective surface layers of the Sun are numerically simulated. Radiation transfer in the photosphere is taken into account. A simulation run over 18.5 minutes real time shows that the granular flow is capable of moving and bending a magnetic flux sheet (the magnetic element). At times it becomes inclined by up to 30° with respect to the vertical around the level ₅₀₀₀ = 1 and it moves horizontally with a maximal velocity of 4 km/s. Shock waves form outside and within the magnetic flux sheet. The latter cause a distinctive signature in a time series of synthetic Stokes V-profiles. Such shock events occur with a mean frequency of about 2.5 minutes. A time resolution of at least 10 seconds in Stokes V recordings is needed to reveal an individual shock event by observation.The National Center for Atmospheric Research is sponsored by the National Science Foundation     

Helium 10830 Å measurements of the Sun

Measurements of the Sun in the near-infrared He i 10830 Å absorption line were performed using the echelle spectrograph with a dispersion of 6.71 mÅ per pixel at the Vacuum Tower Telescope (German Solar Telescopes, Teide Observatory, Izaña, Tenerife, Spain) on May 26, 1993. These measurements were compared with full-disc soft X-ray images of the Sun (Japanese solar satellite Yohkoh), full-disc solar images in H (Big Bear Solar Observatory), full-disc solar images in the He i 10830 Å line (National Solar Observatory, Kitt Peak) and with full-disc microwave solar maps at 37 GHz (Metsähovi Radio Research Station). In the He 10830 Å line the Sun displays a limb darkening similar to that in the visible part of the spectrum. Active regions and H filaments show a strong absorption in the He 10830 Å line, whereas the absorption is weak in coronal holes.     

Talc-chlorite-amphibole felses of the KTB pilot hole,Oberpfalz, Bavaria: Protolith characteristics and phase relationships

Summary The metagabbro-amphibolite sequences in the KTB pilot hole contain intercalations of talc-chlorite-amphibole felses (or hosbachites), which show transitional contacts to the adjacent metagabbros. The hosbachites are characterized by relics of a primary igneous texture and still contain igneous minerals like clinopyroxene, biotite and pseudomorphs after olivine, while brown Ca-amphibole was presumably formed in a late-magmatic stage. The geological, textural, mineralogical and geochemical evidence indicates that the hösbachites were derived from ultramafic cumulates, differentiated from a basaltic magma, either in the inner parts of dolerite sills or in small gabbro intrusions. A pervasive metamorphic overprint under medium-pressure, amphibolite-facies conditions which was accompanied by penetrative deformation led to assemblages with green Ca-amphibole ± anthophyllite ± cummingtonite ± tremolite/actinolite + clinochlore + talc + olivine + ilmenite ± Cr-bearing spinel + sulfides. Phase relationships are consistent with a prograde P-T path leading to the formation of anthophyllite from olivine + talc at peak metamorphic temperatures of 640–700°C, at assumed pressures of 8-10 kbar, similar to those derived from mineral assemblages in the adjacent metabasites and metasediments. High-pressure relics locally present in coronitic metagabbros and retrograded eclogites of the KTB pilot hole were not recognized in the hosbachites. A retrograde overprint under greenschist-facies conditions led to the total replacement of igneous or metamorphic olivine by aggregates of antigorite + magnetite, chloritization of biotite and the formation of late tremolite/ actinolite.

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Zusammenfassung Talk- Chlorit-Amphibol-Felse der KTB-Vorbohrung, Oberpfalz: Eduktcharakteristik und Phasenbeziehungen Die Metagabbro-Amphibolit-Folge in der KTB-Vorbohrung enthält Einschaltungen von Talk-Chlorit-Amphibol-Felsen (Hosbachite), die graduelle Übergänge zu den benachbarten Metagabbros aufweisen. Die Hosbachite sind durch Relikte von primären magmatischen Gefügen gekennzeichnet and führen noch magmatische Mineralrelikte wie Klinopyroxen, Biotit and Pseudomorphosen nach Olivin, während brauner CaAmphibol wahrscheinlich spdtmagmatisch gebildet wurde. Verbandsverhältnisse, Reliktgefüge und Reliktminerale sowie Haupt- und Spurenelement-Geochemie sprechen dafür, daß die Hosbachite auf ultramafische Kumulate zurückgehen, die aus einem basischen Magma differenziert wurden, and zwar entweder im Innern von doleritischen Lagergängen oder in kleinen Gabbro-Intrusionen.Eine durchgreifende metamorphe Überprägung unter Bedingungen der Mitteldruck Amphibolitfazies, die von einer penetrativen Deformation begleitet war, fuhrte zu Mineralparagenesen mit grünern Ca-Amphibol ± Anthophyllit ± Cummingtonit + Tremolit/Aktinolith + Klinochlor + Talk + Olivin + Ilmenit + Cr-haltigem Spinell + Sulfiden.Die Phasenbeziehungen weisen darauf hin, daß sich im Zuge eines prograden P-TPfades Anthophyllit aus der Paragenese Olivin + Talk bildete. Als P-T-Bedingungen beim Hbhepunkt der Metamorphose können Temperaturen von 640–700°C in einem angenommenen Druckbereich von 8-10 kbar abgeschätzt wurden, ähnlich wie sie auch aus den Mineralparagenesen in den angrenzenden Metabasiten and Metasedimenten der KTB-Vorbohrung ableitbar sind. Hochdruckrelikte, die gelegentlich in koronitischen Metagabbros and retrograd überprägten Eklogiten der KTB-Vorbohrung auftreten, wurden in den Hösbachiten nicht gefunden. Eine retrograde Überprägung unter grünschieferfaziellen Bedingungen führte zu einer vollständigen Verdrängung von magmatischem und metamorphem Olivin durch Aggregate von Antigorit + Magnetit, zur Chloritisierung von Biotit und zur Bildung einer späten Generation von Tremolit/ Aktinolith.

     

Application of210Pb in soils

The spectroscopic measurement of soil samples is described.²¹⁰Pb data from a soil survey in western-Europe are briefly reviewed. The average²¹⁰Pb flux from the atmosphere, as determined from²¹⁰Pb _exc soil inventories, is 90 Bq m^–2a^–1. A simple one-dimensional box-chain model is described. The model simulates the vertical, post depositional transport of natural and fall-out radionuclides in the soil. Simulation of measured²¹⁰Pb _exc ,¹³⁴Cs,¹³⁷Cs, and²⁴¹Am soil profiles shows that mixing (bioturbation) is a very efficient transport mechanism. Lead seems to be strongly fixed to organic and clay particles. It is transported by the displacement of the organic and clay carrier substances. The mean residence time of lead, caesium, plutonium and americium in organic rich forest soils is in the order of 250–1000 years. An applicability study in investigate the use of²¹⁰Pb in erosion problems showed erosion rates from 60–180 g m^–2a^–1 on organic rich forest and meadow sites with 10°–25° slopes.This is the eighth of a series of papers to be published by this journal following the 20 ^th anniversary of the first application of²¹⁰Pb dating of lake sediments. Dr P. G. Appleby is guest editing this series.