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1.
Progradational and backstepping shoreface deposits in the Ladinian to Early Norian Snadd Formation of the Barents Sea 下载免费PDF全文
Tore G. Klausen Alf Ryseth William Helland‐Hansen Helge K. Gjelberg 《Sedimentology》2016,63(4):893-916
Shoreface sandstone deposits within the Early Carnian part of the Snadd Formation of the Norwegian Barents Sea can be traced for hundreds of kilometres in the depositional strike direction and for tens of kilometres in the depositional‐dip direction. This study uses three‐dimensional seismic attribute mapping and two‐dimensional regional seismic profiles to visualize the seismic facies of these shoreface deposits and to map their internal stratigraphic architecture at a regional scale. The shoreface deposits are generally elongate but show variable width from north‐east to south‐west, which corresponds to a sediment source in the northern part of the basin and a southward decrease in longshore sediment transport. The Snadd Formation presents an example of how large‐scale progradational shoreface deposits develop. The linear nature of its shoreface deposits contrasts with more irregular, cuspate wave‐dominated deltaic shorelines that contain river outlets, and instead implies longshore drift as the main sediment source. In map view, discrete sets of linear features bounded by truncation surfaces scale directly to beach ridge sets in modern counterparts. The shoreface deposits studied here are characteristic in terms of scale and basin‐wide continuity, and offer insight into the contrast between shallow marine deposition under stable Triassic Greenhouse and fluctuating Holocene Icehouse climates. Findings presented herein are also important for hydrocarbon exploration in the Barents Sea, because they describe a hitherto poorly understood reservoir play in the Triassic interval, wherein the most prominent reservoir plays have so far been considered to be found in channelized deposits in net‐progradational delta‐plain strata that form the topsets to shelf‐edge clinoforms. The documented presence of widespread wave‐dominated shoreface deposits also has implications for how the relative importance of different sedimentary processes is considered within the basin during this period. 相似文献
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A. Smith R. W. Atkins S. Bradbury O. Celik Y. C. K. Chow P. Cogan C. Dowdall S. J. Fegan P. Fortin D. Gall G. H. Gillanders J. Grube K. J. Gutierrez T. A. Hall D. Hanna J. Holder D. Horan S. B. Hughes T. B. Humensky I. Jung P. Kaaret G. Kenny M. Kertzman D. B. Kieda A. Konopelko H. Krawczynski F. Krennrich M. J. Lang S. Le Bohec G. Maier J. Millis P. Moriarty R. A. Ong J. S. Perkins K. Ragan G. H. Sembroski J. A. Toner L. Valcarcel V. V. Vassiliev R. G. Wagner S. P. Wakely T. C. Weekes R. J. White D. A. Williams 《Astrophysics and Space Science》2007,309(1-4):299-303
In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the
Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source
is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained
with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006
season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are
placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set.
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3.
Alf Amsler 《International Journal of Earth Sciences》1929,20(4-5):342-342
4.
Sren Grube Pedersen Martin Schiller James N. Connelly Martin Bizzarro 《Meteoritics & planetary science》2019,54(6):1215-1227
Planetary bodies a few hundred kilometers in radii are the precursors to larger planets but it is unclear whether these bodies themselves formed very rapidly or accreted slowly over several millions of years. Ordinary H chondrite meteorites provide an opportunity to investigate the accretion time scale of a small planetary body given that variable degrees of thermal metamorphism present in H chondrites provide a proxy for their stratigraphic depth and, therefore, relative accretion times. We exploit this feature to search for nucleosynthetic isotope variability of 54Cr, which is a sensitive tracer of spatial and temporal variations in the protoplanetary disk's solids, between 17 H chondrites covering all petrologic types to obtain clues about the parent body accretionary rate. We find no systematic variability in the mass‐biased corrected abundances of 53Cr or 54Cr outside of the analytical uncertainties, suggesting very rapid accretion of the H chondrite parent body consistent with turbulent accretion. By utilizing the μ54Cr–planetary mass relationship observed between inner solar system planetary bodies, we calculate that the H chondrite accretion occurred at 1.1 ± 0.4 or 1.8 ± 0.2 Myr after the formation of calcium‐aluminum‐rich inclusions (CAIs), assuming either the initial 26Al/27Al abundance of inner solar system solids determined from angrite meteorites or CAIs from CV chondrites, respectively. Notably, these ages are in agreement with age estimates based on the parent bodies’ thermal evolution when correcting these calculations to the same initial 26Al/27Al abundance, reinforcing the idea of a secular evolution in the isotopic composition of inner disk solids. 相似文献
5.
Jingran Zhang Sumiko Tsukamoto Alf Grube Manfred Frechen 《Boreas: An International Journal of Quaternary Research》2014,43(4):856-868
The history of sea‐level change and sediment accumulation since the last deglaciation along the German North Sea coast is still controversial because of a limitation in the quantity and quality of chronological data. In the current study, the chronology of a 16‐ka coastal sedimentary record from the Garding‐2 core, retrieved from the Eiderstedt Peninsula in Schleswig‐Holstein, northern Germany, was established using OSL and AMS 14C dating techniques. The robust chronology using 14 radiocarbon and 25 OSL dates from the Garding‐2 core is the first long‐term record that covers the Holocene as well as the last deglaciation period in one succession in the German North Sea area. It provides a new insight into understanding the Holocene transgression and coastal accumulation histories. The combined evidence from the sedimentology and chronology investigations indicates that an estuarine environment dominated in Eiderstedt Peninsula from 16 to 13 ka, followed by a depositional hiatus between 13 and 8.3 ka, attributed to erosion caused by the Holocene transgression; the onset of the Holocene transgression at the core site occurred at around 8.3 ka. The sea level continued to rise with a decelerated rate until around 3 ka. Since 3 ka, the shoreline has begun to prograde. Foreshore (tidal flat) sediments have been deposited at the drilling site with a very high sedimentation rate of about 10 m ka?1. At around 2 ka, a sandy beach deposit accumulated in the sedimentary succession, indicating that the coastline shifted landward, which may represent a small‐scale transgression in the late Holocene. At around 1.5 ka, terrestrial clastic sediment started to accumulate, indicating a retreat of the relative sea level in this area, which may be related to local diking activities undertaken since the 11th century. 相似文献
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Alf Nyberg 《Meteorology and Atmospheric Physics》1954,7(1):99-113
Summary Horizontal flux of enthalpy and latent heat has been computed from synoptic maps over a large part of the northern hemisphere for several isobaric levels during 3 months. The flux of enthalpy and also the flux of latent heat is lowest in July and 3 to 4 times larger in winter. The flux is largest at 850 mb. The large scale eddy conductivity for the enthalpy increases with the horizontal meridional temperature gradient showing that the atmospheric energy exchange processes become more effective when the gradients are strong. From the convergence of the flux values the mean heating of an air column has been computed. This heating has a winter maximum of about 1° C/24 hrs at latitude 60°–70° N. The values for the polar region are considerably lower, indicating a considerable mean descending motion in the region. The correlation between flux or convergence of flux and circulation indices is found to be rather small. There is even a negative correlation between convergence of enthalpy and the zonal index.
With 6 Figures. 相似文献
Zusammenfassung Der horizontale Transport von Enthalpie und latenter Wärme wurde auf Grund von Wetterkarten für verschiedene Druckniveaus über einem großen Teil der nördlichen Hemisphäre für drei verschiedene Monate berechnet. Sowohl der Enthalpie- wie der latente Wärmestrom ist am geringsten im Juli und drei- bis viermal größer im Winter; am größten ist er bei 850 mb. Der Großaustauschkoeffizient der Enthalpie nimmt mit dem horizontalen meridionalen Temperaturgradienten zu, was sich durch die Steigerung der atmosphärischen Energieaustauschprozesse bei Verstärkung des Gradienten erklärt. Aus der Strömungskonvergenz wurde die durchschnittliche Erwärmung einer Luftsäule berechnet. Diese Erwärmung zeigt ein Maximum von zirka 1° C/24 Studen im Winter in einer Breite von 60 bis 70° N. Die Werte für das Polargebiet sind beträchtlich niedriger und lassen eine merkliche absinkende Strömung erkennen. Die Korrelation zwischen Strömung oder Strömungskonvergenz und Zirkulationsgrößen hat sich als eher niedrig erwiesen. Die Korrelation zwischen der Konvergenz der Enthalpie und dem Zonalindex ist sogar negativ.
Résumé Le flux horizontal d'enthalpie et de chaleur latente a été calculé à partir de cartes synoptiques couvrant une grande partie de l'hémisphère nord et cela pendant 3 mois pour plusieurs niveaux isobariques. Le flux d'enthalpie ainsi que celui de chaleur latente est à son minimum en juillet et est 3 à 4 fois plus grand en hiver. Le flux le plus important se trouve au niveau de 850 mb. Le coefficient de la conductivité turbulente de l'enthalpie à grande échelle croît avec le gradient horizontal méridional de température, et montre ainsi que les processus de l'échange d'énergie atmosphérique augmentent avec la force du gradient. L'auteur a calculé le réchauffement moyen d'une colonne d'air en partant de la convergence des valeurs du flux. Ce réchauffement atteint un maximum hivernal d'environ 1° C/24 h à 60°–70° de latitude N. Les valeurs des régions polaires sont notablement plus petites et laissent reconnaître un mouvement descendant considérable dans cette région. La corrélation entre le courant ou la convergence de flux et les valeurs de la circulation s'est avérée plutôt petite. Il y a même une corrélation négative entre la convergence de l'enthalpie et l'index zonal.
With 6 Figures. 相似文献
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Alf Nyberg 《Pure and Applied Geophysics》1980,119(3):510-514
10.
J?rg E. Aarnes Vegard Kippe Knut-Andreas Lie Alf Birger Rustad 《Computational Geosciences》2002,6(1):1-4