Eocene high pressure metamorphism in the Penninic units of the Tauern Window (Eastern Alps): evidence from40Ar−39Ar dating and petrological investigations

The⁴⁰Ar-³⁹Ar degassing spectra of white micas and amphiboles from three tectonic units of the central Tauern Window (Pennine basement and cover in the Eastern Alps) have been measured. White micas are classified as (1) pre-Alpine low-Si relic micas with an age value of 292 Ma, variously disturbed by the Alpine metamorphism; (2) Alpine phengitic micas of variable composition with an age between 32 and 36 Ma; (3) Alpine low-Si micas with a maximum age of 27 Ma. We attribute the higher Alpine ages to a blueschist facies event, whereas the lower age reflects the late cooling of the nappe pile. Blueschist facies phengites from the basement (Lower Schieferhülle) and the tectonic cover (Upper Schieferhülle) crystallized at a temperature below the closure temperature (T _c) for argon diffusion in white mica and record ages of 32 to 36 Ma. At the same time a thin, eclogite facies unit (Eclogite Zone) was thrust between the Lower and the Upper Schieferhülle and cooled from eclogite facies conditions at about 600°C at 20 kbar to blueschist facies conditions at 450°C or even 300°C at >10 kbar. Eclogite facies phengites closed for argon diffusion and record cooling ages, coinciding with the crystallization ages in the hanging and the footwall unit. Amphibole age spectra (actinolite, glaucophane, barroisite) are not interpretable in terms of geologically meaningful ages because of excess argon.     

Die tektonische Evolution der Erde von Pangäa zur Gegenwart ein plattentektonisches Modell

Zusammenfassung Das hier vorgestellte Modell basiert auf der Annahme, daß sich unter großen Landmassen, wie Pangäa zum Beispiel, in tektonischen Ruheperioden Wärme aus dem Erdinneren anstaut. Infolgedessen entwickelte sich vom Perm bis zur Kreide ein weites Konvektionstumorsystem; Pangäa zersplitterte und die kontinentalen Platten bewegten sich vom afrikanischen Zentrum weg. Die ozeanischen Rücken des Atlantiks und Indiks folgten den abwandernden Platten wie sich »öffnende Ringe«. Panthalassa, der Eo-Pazifik, wurde von allen Seiten überdriftet. Es muß einen Gegenstrom vom Pazifik im Mantel geben, welcher für die Auffüllung der zwischen den Pangäabruchstücken entstehenden ozeanischen Räume mit Mantelmaterial sorgt. Auch die ozeanischen Platten des Pazifiks bewegen sich vom zentralen »Darwin-Rise« weg. Der ostpazifische Rükken folgte der Bewegung und bildet heute einen ausgedehnten ostwärts gekrümmten Bogen. In den ozeanischen »Außenbögen« bildeten sich infolge der Dehnung Querrifts. Die Transformstörungen sind in beiden Systemen radial angeordnet. Die Terrains an Nordamerikas Westküste können nur östlich eines ostpazifischen Rückens aus ihrer ursprünglichen Position im zentralen Pazifik herausgewandert sein, also synchron mit dem sich öffnenden Pazifik. Die Kontinente bewegen sich möglicherweise solange von ihrer ursprünglichen Position weg, bis erneut eine große Landmasse zusammengedriftet ist. Unterhalb einer solchen »Neogäa« könnte sich wieder ein Konvektionstumor infolge von Wärmestau entfalten. Das findet vielleicht in Intervallen von einigen hundert Millionen Jahren statt und könnte die WILSON-Zyklen der Erdgeschichte erklären.

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The tectonic evolution of the earth from Pangea to the present a plate tectonic model

The model proposed here is based on the assumption that beneath giant landmasses (e.g. Pangea) heat from the inner earth is stored up and accumulated during periods of tectonic inactivity. Consequently below Pangea a huge convection bulge system developed from the Permian to the Cretaceous; Pangea split up and the continental plates moved away from the African centre. The oceanic ridges of the Atlantic and the Indic also followed the movement of the withdrawing continents like »opening rings«. The oceanic ridges always maintained their position in the middle of the spreading oceans above unidirectional flows in the upper mantle. Panthalassa which surrounded Pangea, was over-drifted from all sides. Since the »expansion« of Pangea is continuing even today, there must be a counter current of mantle material from the Pacific area, compensating the gaps between the fragments of Pangea. Consequently at the subduction zones a suction should exist, which pulls the Pacific plates under the advancing plates of the former Pangean continent. In the centre of Panthalassa another bulge from the upper mantle developed simultaneously with the bulge under Pangea. The Pacific oceanic plates moved away outwards from this central »Darwin rise«. The Eastpacific ridge also followed this movement eastwards and forms today a wide, ringlike arc. In the outer arcs of the Pangean and Pacific spreading ocean systems transverse ridges developed as a result of the extension of the older oceanic crust. The transform faults are radial structures in both »expanding« systems. The hotspot spurs of the Hawaii and Polynesian islands can be explained as the result of material derived from an independent slowly ESE moving deeper part of the mantle. The terrains on North Americas West cost moved away from their original position in the central Pacific ocean synchronously with the opening ocean on the east side of the advancing East Pacific ridge.The energy which drives the whole system is residual plus radioactive heat. Kinetic movements compensate the heat surplus of the earth. The continental plates of the Pangean system are moving away from their original position until a new giant landmass is formed by collision. Below such a stationary »Neogea« a heat bulge can develop again. This may take place perhaps in intervals of hundred of million years, explaining the WILSON-cycles in earth history.

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Résumé Le modèle présenté ici est basé sur l'hypothèse qu'endessous des grandes masses continentales — comme la Pangée p.ex. - il s'accumule, pendant les périodes de calme tectonique, de la chaleur d'origine interne. En conséquence, depuis le Permien jusqu'au Crétacé, un vaste système de convection s'est développé; la Pangée s'est morcelée et les plaques continentales se sont éloignées du centre africain. Les dorsales océaniques circum-africaines ont suivi le mouvement de ces plaques à la manière d'»anneaux concentriques«. La Panthalassa, précurseur du Pacifique, a été chevauchée de tous les côtés. Il doit s'être établi, dans le manteau, à partir du Pacifique, un contre-courant qui compense l'ouverture des océans en formation entre les fragments de la Pangée. Le Pacifique a donné lieu, lui aussi, à une expansion centrifuge; la dorsale est-pacifique a suivi le mouvement et forme aujourd'hui un arc bombé vers l'est. Dans les arcs océaniques extérieurs, l'expansion a provoqué la formation de dorsales transverses. Les failles transformantes montrent, dans les deux systèmes, des dispositions radiales. Les terrains de la côte W de l'Amérique du N ne peuvent provenir que d'une région située à l'Est de la dorsale est-pacifique dans sa position d'origine. Les continents s'éloigment et forme aujourd'hui un arc bombé vers l'est. Dans les arcs océaniques extérieurs, l'expansion a provoqué la forSous une telle »Néogée«, une nouvelle cellule de convection pourrait ensuite se développer. Ces phénomènes pourraient se dérouler dans un intervalle de quelques centaines de millions d'années, expliquant ainsi les cycles de Wilson dans l'histoire de la Terre.

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Der Eiswinter 1983/84 im deutschen Küstengebiet zwischen Ems und Trave

Ohne Zusammenfassung     

Holes in the Hα Eruptive Prominence Structure

The eruptive prominence observed on 27 May 1999 in H at Ondejov Observatory is analyzed using image-processing techniques. To understand the physical processes behind the prominence eruption, heated structures inside the cold H prominence material are sought. Two local minima of intensity (holes), the first above and the second below the erupting H prominence, have been found in the processed H images. A comparison of H images with the SOHO/EIT and Yohkoh/SXT images showed: (a) the cold H prominence is visible as a dark feature in the EIT images, (b) the upper local minimum of intensity in the H image corresponds to a hot structure seen in EIT, (c) the lower minimum corresponds to a hot loop observed by SXT. The physical significance of the H intensity minima and their relation to the hot structures observed by EIT and SXT is discussed. The time sequence of observed processes is in favor of the prominence eruption model with the destabilization of the loop spanning the prominence. For comparison with other events the velocities of selected parts of the eruptive prominence are determined.     

Ice core evidence for secular variability and 200-year dipolar oscillations in atmospheric circulation over East Antarctica during the Holocene

Two Holocene ice core records from East Antarctica (Vostok and EPICA-Dome C) were analysed for dust concentration and size distribution at a temporal resolution of 1 sample per ~50 years. A series of volcanic markers randomly distributed over the common part of the ice cores (from 9.8 to 3.5 kyear BP) ensures accurate relative dating (±33 years). Dust-size records from the two sites display oscillations structured in cycles with sub-millennial and secular scale frequencies that are apparently asynchronous. The power spectra of the composite sum (Σ) of the two dust-size records display spectral energy mostly for 150- to 500-year periodicities. On the other hand, the 200-year band is common to both records and the 200 year components of the two sites are out-of-phase (100-year lead or lag) over ~5.5 kyear, a phenomenon also reflected by a significant (>99% conf. lev.) band in the power spectra of the composite difference (Δ) of the two size records. During long-range transport, mineral dust originating from the Southern Hemisphere continents is graded to a variable extent depending on the altitude and duration of atmospheric transport. Relatively coarse dust is associated with air mass penetration from the middle–lower troposphere and conversely relatively fine dust with upper troposphere air masses or the influence of subsidence over the Antarctic plateau, a hypothesis already proposed for the changes that occurred during the Last Glacial Maximum to Holocene transition (Delmonte et al. 2004b). Moreover, we assume that the overall fluctuation of air mass advection over Antarctica depends on the meridional pressure gradient with respect to low latitudes, i.e. the Antarctic Oscillation (AAO). We therefore suggest a regional variability in atmospheric circulation over East Antarctica. The 150–500 year power spectrum of the composite (Σ) parameter represents the long term variability of the AAO, imprinted by secular internal oscillations probably related to the southern ocean-climatic system. On the other hand, the Δ dust composite parameter suggests a persistent atmospheric dipole over East Antarctica delivering coarser (finer) dust particles alternatively to Vostok and Dome C regions with a bi-centennial periodicity. Indeed, a seesaw phenomenon in dust size distribution was already observed at three East Antarctic sites during the last deglaciation (Delmonte et al. 2004b) and was interpreted as a progressive reduction of the eccentricity of the polar vortex with respect to the geographic south pole. Interestingly, the Δ parameter shows a pronounced 200-year oscillation mode, throwing new light on the unresolved question of a possible relationship between climate and solar activity.     

The world''s large lake basins as denudation-accumulation systems and implications for their lifetimes

The mechanical denudation rates of 81 large lake basins (lake area > 500 km²) were determined from long-term river loads and erosion maps. Using the drainage area/lake area ratios the mean sedimentation rates of the lakes were calculated for a porosity of 0.3. The mean sedimentation rates of different lake types vary between 0.1 mm/a (glacial lakes, lowland) and 5.4 mm/a (mostly sag basin lakes). The calculated lifetimes of the lakes are based on the lake volumes and mean sedimentation rates, assuming steady-state conditions and solely clastic material. On average, glacial lakes in highlands and fault-related lakes show the shortest lifetimes (c. 70 ka), glacial lakes in lowlands and rift lakes have the longest lifetimes (c. 1 Ma). Some lakes remain unfilled for very long time spans due to rapid subsidence of their basin floors. The calculated lifetimes are compared with those derived from sediment core studies. Most core studies indicate lower mechanical sedimentation rates than the calculated ones because a major part of the incoming sediment is trapped in deltas. However, a number of lakes (e.g., the Great Lakes of North America) show the opposite tendency which is largely caused by extensive shoreline erosion and resuspension. The lifetimes of large glacial lakes often exceed the duration of interglacials. Hence, their lifetimes are restricted by glaciation and not by sediment infill. Rift lakes persist for long time periods which exceed the calculated lifetimes in some cases. Time-dependent subsidence, basin extension, as well as the impact of climate change are briefly described.     

Location and height of intertidal bars on macrotidal ridge and runnel beaches

Previous studies devoted to the morphology and hydrodynamics of ridge and runnel beaches highlight characteristics that deviate from those initially postulated by King and Williams (Geographical Journal, 1949, vol. 113, 70–85) and King (Beaches and Coasts, 1972, Edward Arnold). Disagreements on the morphodynamics of these macrotidal beaches include the position of the ridges relative to the mean neap and spring tide levels, the variation in the height of the ridges across the intertidal profile and, most importantly, whether the ridges are formed by swash or surf zone processes. The morphological characteristics of ridge and runnel beaches from three locations with varying wave, tidal and geomorphic settings were investigated to address these disagreements. Beach profiles from each site were analysed together with water‐level data collected from neighbouring ports. It was found that the ridges occur over the entire intertidal zone. On one site (north Lincolnshire, east England), the ridges are uniformly distributed over the intertidal beach, whereas on the two other sites (Blackpool beach, northwest England, and Leffrinckoucke beach, north France) there is some indication that the ridges appear to occur at preferential locations. Most significantly, the locations of the ridge crests were found to be unrelated to the positions on the intertidal profile where the water level is stationary for the longest time. It was further found that the highest ridges generally occur just above mid‐tide level where tidal non‐stationarity is greatest. These findings argue against the hypothesis that the ridges are formed by swash processes acting at stationary tide levels. It is tentatively suggested that the ridges are the result of a combination of swash and surf zone processes acting across the intertidal zone. Elucidation of the morphodynamic roles of these two types of processes, and other processes such as strong current flows in the runnels, requires further comprehensive field measurements complemented by numerical modelling. Copyright © 2001 John Wiley & Sons, Ltd.