Tracking the last sea-level cycle: seafloor morphology and shallow stratigraphy of the latest Quaternary New Jersey middle continental shelf     

Catherine Schuur Duncan  John A. Goff  James A. AustinJr.  Craig S. Fulthorpe 《Marine Geology》2000,170(3-4):395-421

Seafloor geomorphology and surficial stratigraphy of the New Jersey middle continental shelf provide a detailed record of sea-level change during the last advance and retreat of the Laurentide ice sheet (120 kyr B.P. to Present). A NW–SE-oriented corridor on the middle shelf between water depths of 40 m (the mid-shelf “paleo-shore”) and 100 m (the Franklin “paleo-shore”) encompasses 500 line-km of 2D Huntec boomer profiles (500–3500 Hz), an embedded 4.6 km² 3D volume, and a 490 km² swath bathymetry map. We use these data to develop a relative stratigraphy. Core samples from published studies also provide some chronological and sedimentological constraints on the upper <5 m of the stratigraphic succession.The following stratigraphic units and surfaces occur (from bottom to top): (1) “R”, a high-amplitude reflection that separates sediment >46.5 kyr old (by AMS ¹⁴C dating) from overlying sediment wedges; (2) the outer shelf wedge, a marine unit up to 50 m thick that onlaps “R”; (3) “Channels”, a reflection sub-parallel to the seafloor that incises “R”, and appears as a dendritic system of channels in map view; (4) “Channels” fill, the upper portion of which is sampled and known to represent deepening-upward marine sediments 12.3 kyr in age; (5) the “T” horizon, a seismically discontinuous surface that caps “Channels” fill; (6) oblique ridge deposits, coarse-grained shelly units comprised of km-scale, shallow shelf bedforms; and (7) ribbon-floored swales, bathymetric depressions parallel to modern shelf currents that truncate the oblique ridges and cut into surficial deposits.We interpret this succession of features in light of a global eustatic sea-level curve and the consequent migration of the coastline across the middle shelf during the last 120 kyr. The morphology of the New Jersey middle shelf shows a discrete sequence of stratigraphic elements, and reflects the pulsed episodicity of the last sea-level cycle. “R” is a complicated marine/non-marine erosional surface formed during the last regression, while the outer shelf wedge represents a shelf wedge emplaced during a minor glacial retreat before maximum Wisconsin lowstand (i.e., marine oxygen isotope stage 3.1). “Channels” is a widespread fluvial subarial erosion surface formed at the late Wisconsin glacial maximum 22 kyr B.P. The shoreline migrated back across the mid-shelf corridor non-uniformly during the period represented by “Channels” fill. Oblique ridges are relict features on the New Jersey middle shelf, while the ribbon-floored swales represent modern shelf erosion. There is no systematic relationship between modern seafloor morphology and the very shallowly buried stratigraphic succession.  相似文献   

X-ray emission from nearby M-dwarfs: the super-saturation phenomenon     

David J. James  Moira M. Jardine  Robin D. Jeffries  Sofia Randich  rew Collier Cameron  Miguel Ferreira 《Monthly notices of the Royal Astronomical Society》2000,318(4):1217-1226

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Observations of the post-common-envelope binaries EG UMa and PG 1026+002     

James N. Bleach  Janet H. Wood  M. S. Catalán  W. F. Welsh  E. L. Robinson  W. Skidmore 《Monthly notices of the Royal Astronomical Society》2000,312(1):70-82

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Numbers,types, and compositions of an unbiased collection of cosmic spherules     

Susan TAYLOR  James H. LEVER  Ralph P. HARVEY 《Meteoritics & planetary science》2000,35(4):651-666

Abstract— Micrometeorites collected from the bottom of the South Pole water well (SPWW) may represent a complete, well‐preserved sample of the cosmic dust that accreted on Earth from 1100–1500 A.D. We classified 1588 cosmic spherules in the size range 50–800 μm. The collection has 41% barred olivine spherules, 17% glass spheres, 12% cryptocrystalline spherules, 11% porphyritic olivine spherules, 12% relicgrain‐bearing spherules, 3% scoriaceous spherules, 2% I‐type spherules, 1% Ca‐AI‐Ti‐rich (CAT) spherules, and 1% G‐type spherules. We also found bubbly glass spherules, spherules with glass caps, and ones with sulfide coatings—particles that are absent from other collections. A classification sequence of the stony spherules (scoriaceous, relic‐grain‐bearing, porphyritic, barred olivine, cryptocrystalline, glass, and CAT) is consistent with progressive heating and evaporation of Fe from chondritic materials. The modern‐day accretion rate and size distribution measured at the SPWW can account for the stony spherules present in deep‐sea collection through preferential dissolution of glass and small stony spherules. However, weathering alone cannot account for the high accretion rate of I‐type spherules determined for two deep‐sea collections. The SPWW collection provides data to constrain models of atmospheric‐entry heating and to assess the effects of terrestrial weathering.  相似文献   

High Angular Resolution Studies of Coronal Structures with SOHO     

Margarita Karovska  Brian Wood  John W. Cook  James Chen  Russ Howard 《Astrophysics and Space Science》2000,273(1-4):7-15

Since January 1996, the Solar and Heliospheric Observatory (SOHO)has been providing unprecedented views of the extended solar coronato heliocentric distances of up to 32 solar radii. During the past threeyears we carried out studies of the morphology and dynamical evolutionof various structures in the solar corona using two instruments on boardSOHO: the Large Angle Spectrometric Coronagraph (LASCO) and the ExtremeUltraviolet Imaging Telescope (EIT). We have applied advanced image resolutionenhancement techniques to explore in detail the characteristics of thesmall-scale structures and/or the low contrast structures in the solarcorona. We describe here the results from these high-angular resolutionstudies, including of the kinematics of several Coronal Mass Ejections andpolar jets.  相似文献   

A dynamical model of the inner Galaxy     

Ralf Häfner  N. Wyn Evans  Walter Dehnen  James Binney 《Monthly notices of the Royal Astronomical Society》2000,314(3):433-452

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Analysis of Thomsen parameters for finely layered VTI media   总被引：2，自引：0，他引：2  

James G. Berryman  Vladimir Y. Grechka  & Patricia A. Berge 《Geophysical Prospecting》1999,47(6):959-978

Since the work of Postma and Backus, much has been learned about elastic constants in vertical transversely isotropic (VTI) media when the anisotropy is due to fine layering of isotropic elastic materials. Nevertheless, there has continued to be some uncertainty about the possible range of Thomsen's anisotropy parameters ε and δ for such media. We use both Monte Carlo studies and detailed analysis of Backus' equations for both two- and three-component layered media to establish the results presented. We show that ε lies in the range ?3/8 ε ½[〈v²_p〉〈v^?2_p〉?1], for finely layered media; smaller positive and all negative values of ε occur for media with large fluctuations in the Lamé parameter λ in the component layers. We show that δ can also be either positive or negative, and that for constant density media, sign (δ) = sign (〈v^?2_p〉 ? 〈v^?2_s〉〈v²_s/v²_p〉). Monte Carlo simulations show that among all theoretically possible random media, positive and negative δ are equally likely in finely layered media. (Of course, the δs associated with real earth materials may span some smaller subset of those that are theoretically possible, but answering this important question is beyond our present scope.) Layered media having large fluctuations in λ are those most likely to have positive δ. This is somewhat surprising since ε is often negative or a small positive number for such media, and we have the general constraint that ε ? δ > 0 for layered VTI media. Since Gassmann's results for fluid-saturated porous media show that the mechanical effects of fluids influence only the Lamé parameter λ, not the shear modulus μ, these results suggest that small positive δ occurring together with small positive ε (but somewhat larger than δ) may be indicative of changing fluid content in a layered earth.  相似文献   

Core-Based Investigation of NMR Logging as a Tool for Characterization of Shallow Unconsolidated Aquifers     

Robert A. James  Robert Ehrlich 《Ground water》1999,37(1):48-57

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Caffeine and Pharmaceuticals as Indicators of Waste Water Contamination in Wells   总被引：6，自引：0，他引：6  

Ralph L. Seiler  Steven D. Zaugg  James M. Thomas  Darcy L. Howcroft 《Ground water》1999,37(3):405-410

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Automated GPS Data Analysis Service   总被引：5，自引：1，他引：4  

James F. Zumberge 《GPS Solutions》1999,2(3):76-78

Automatic analysis of geodetic-quality GPS data is available with the use of e-mail and ftp (file transfer program) as an interface to a computer at the Jet Propulsion Laboratory (JPL), where precise transmitter parameters – GPS ephemerides and clock errors – are computed regularly. The interface is such that e-mail from an external user causes the JPL computer to fetch the user's data. The computer than analyzes the data, and places the results in an area accessible to the user. An e-mail to the user gives information on the location of the analysis results, which the user can subsequently fetch. Operations on the JPL computer are entirely automatic, and require essentially no labor. ? 1999 John Wiley & Sons, Inc.  相似文献