Stratigraphic evidence for an Early Aptian sea-level fluctuation: the Graua Limestone of south-eastern Ethiopia     

Alfonso Bosellini  Antonio Russo  Rolf Schroeder 《Cretaceous Research》1999,20(6):783

The occurrence of a thin band of marine limestone (Graua Limestone) within a thick succession of fluviatile sandstones in south-eastern Ethiopia is direct evidence of flooding of part of the East African craton (Horn of Africa). According to the presence of abundant orbitolinid foraminifers (Palorbitolina lenticularis Blumenbach andPraeorbitolina cormyi Schroeder), the age of the Graua Limestone can be referred to the Early Aptian. Stratigraphy and palaeogeographic reconstructions for the Early Cretaceous in the surrounding regions (Kenya, Somalia, Yemen, Socotra, Oman, Syria, Lebanon, Israel, Egypt and Libya) show that the Early Aptian transgression was of regional extent. Our data seem to confirm that this transgression was of relatively short duration. This pulse cannot be related to tectono-eustatic mechanisms, which are too slow. A short-lived event should be invoked: either a regional tectonic pulse or the desiccation of the proto-South Atlantic.  相似文献   

High-frequency near-bottom acoustic reflection signatures of hydrocarbon seeps on the Northern Gulf of Mexico continental slope   总被引：2，自引：2，他引：0  

W. W. Sager  Chang S. Lee  I. R. MacDonald  W. W. Schroeder 《Geo-Marine Letters》1999,18(4):267-276

 Acoustic reflection signatures of four hydro-carbon seeps were classified using near-bottom 25-kHz echosounder profiles. Echo patterns were compared with ground-truth data obtained by submersible observations and shallow coring. Six echo types were distinguished: strong reflections from (1) exposed or (2) buried hard substrates, such as authigenic carbonate or gas hydrate; acoustic scattering in (3) unlayered or (4) layered sediments owing to gas, shells, or disseminated carbonates; (5) attenuation caused by gas; and (6) undisturbed sediments. Echo type distributions suggest that high spatial variability indicates a younger, vigorous seep, whereas extensive hard substrate implies an older, encrusted seep. Received: 29 May 1998 / Revision received: 7 October 1998  相似文献   

A Snapshot of the Sun Near Solar Minimum: The Whole Heliosphere Interval     

Barbara J. Thompson  Sarah E. Gibson  Peter C. Schroeder  David F. Webb  Charles N. Arge  Mario M. Bisi  Giuliana de Toma  Barbara A. Emery  Antoinette B. Galvin  Deborah A. Haber  Bernard V. Jackson  Elizabeth A. Jensen  Robert J. Leamon  Jiuhou Lei  Periasamy K. Manoharan  M. Leila Mays  Patrick S. McIntosh  Gordon J. D. Petrie  Simon P. Plunkett  Liying Qian  Peter Riley  Steven T. Suess  Munetoshi Tokumaru  Brian T. Welsch  Thomas N. Woods 《Solar physics》2011,274(1-2):29-56

We present an overview of the data and models collected for the Whole Heliosphere Interval, an international campaign to study the three-dimensional solar?Cheliospheric?Cplanetary connected system near solar minimum. The data and models correspond to solar Carrington Rotation 2068 (20 March??C?16 April 2008) extending from below the solar photosphere, through interplanetary space, and down to Earth??s mesosphere. Nearly 200 people participated in aspects of WHI studies, analyzing and interpreting data from nearly 100 instruments and models in order to elucidate the physics of fundamental heliophysical processes. The solar and inner heliospheric data showed structure consistent with the declining phase of the solar cycle. A closely spaced cluster of low-latitude active regions was responsible for an increased level of magnetic activity, while a highly warped current sheet dominated heliospheric structure. The geospace data revealed an unusually high level of activity, driven primarily by the periodic impingement of high-speed streams. The WHI studies traced the solar activity and structure into the heliosphere and geospace, and provided new insight into the nature of the interconnected heliophysical system near solar minimum.  相似文献   

A high-resolution real-time forecasting system for predicting the fate of oil spills in the Strait of Bonifacio (western Mediterranean Sea)   总被引：1，自引：0，他引：1  

Cucco A  Sinerchia M  Ribotti A  Olita A  Fazioli L  Perilli A  Sorgente B  Borghini M  Schroeder K  Sorgente R 《Marine pollution bulletin》2012,64(6):1186-1200

The Strait of Bonifacio is a long and narrow area between Corsica and Sardinia. To manage environmental emergencies related to the spill of oil from vessels, an innovative forecasting system was developed. This tool is capable of operationally predicting the dispersion of hydrocarbon spills in the coastal area of the Bonifacio Strait, either from an instantaneous or continuous spill and either in forward or backward mode. Experimental datasets, including ADCP water current measurements and the trajectories of drifter buoys released in the area, were used to evaluate the accuracy of this system. A comparison between the simulation results and experimental data revealed that both the water circulation and the surface transport processes are accurately reproduced by the model. The overall accuracy of the system in reproducing the transport of an oil spill at sea was estimated for both forward and backward prediction mode and in relation to different forecasting time lags.  相似文献   

FerryBox - Application of continuous water quality observations along transects in the North Sea   总被引：3，自引：2，他引：1  

Wilhelm Petersen  Friedhelm Schroeder  Frank-Detlef Bockelmann 《Ocean Dynamics》2011,61(10):1541-1554

In 2002, the Helmholtz-Zentrum Geesthacht, Germany, started to use FerryBox-automated monitoring systems on Ships of Opportunity to continuously record standard oceanographic, biological and chemical in situ data in the North Sea. The present study summarises the operational experience gathered since the beginning of this deployment and reflects on the potential and limits of FerryBox systems as a monitoring tool. One part relates to the instrumental performance, constancy of shipping services, and the availability and quality of the recorded in situ data. The other considers integration of the FerryBox observations in scientific applications and routine monitoring campaigns. Examples are presented that highlight the added value of the recorded data for the study of both long- and short-term variability in water mass stability, plankton communities and surface water productivity in the North Sea. Through the assessment of technical and scientific performance, it is evident that FerryBoxes have become a valuable tool in marine research that helps to fill gaps in coastal and open ocean operational observation networks.  相似文献   

Potential Atmospheric Transport Pathways for Mercury Measured in the Canadian High Arctic     

Meng-Dawn Cheng  William H. Schroeder 《Journal of Atmospheric Chemistry》2000,35(1):101-107

Large-scale transport pathways for atmospheric gaseous mercury emitted from surrounding source regions to reach the Alert sampling site located at the Northwest Territories of Canada between August 1992 and August 1993 were investigated. The 12-month atmospheric mercury data set comprises blank-corrected total gaseous mercury (TGM) concentrations collected on gold-coated sand traps during one-week long sampling intervals. For TGM concentrations above the 12-month mean TGM level, the analysis reveals regions in Eastern Europe (close to East Germany and Poland), areas on Northeastern America in Canada (Northwest Territories), and central Siberia of the former U.S.S.R. Identification of the physical locations of the emission sources was limited by the temporal resolution of weekly averaged data; however, major atmospheric pathways of mercury transport to the Arctic were successfully resolved. The objective of this note is to demonstrate that the potential source contribution function could be applied to resolve the sources and recover transport pathways of atmospheric mercury over a large scale.  相似文献   

Temporal variability of remotely sensed suspended sediment and sea surface temperature patterns in Mobile Bay,Alabama     

James B. Rucker  Richard P. Stumpf  William W. Schroeder 《Estuaries and Coasts》1990,13(2):155-160

Distribution patterns of suspended sediments and sea surface temperatures in, Mobile Bay were derived from algorithms using digital data from the visible, near infrared, and infrared channels of the Advanced Very High Resolution Radiometer (AVHRR) on the NOAA-TIROS-N satellite. Closely spaced AVHRR scenes for January 20, 24, and 29, 1982, were compared with available environmental information taken during the same period. A complex interaction between river discharge, winds, and astronomical tides controlled the distribution patterns of suspended sediments. These same variables, coupled with air temperatures, also governed the distribution patterns of sea surface temperatures.  相似文献   

2. Kristallographische und röntgenographische Bestimmungen am „Wittichenit von Sadisdorf”     

Werner Borchert  Robert Schroeder 《Contributions to Mineralogy and Petrology》1947,1(1):112-117

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Eolian dust in the coastal desert of the sudan: Aggregates cemented by evaporites     

Johannes H. Schroeder  Klaus-Dieter Kachholz  Michael Heuer 《Geo-Marine Letters》1984,4(3-4):139-144

Eolian dusts collected after dust storms contain aggregates that are cemented by evaporitic salts, mainly halite. They vary in shape, fabrics, and surface roughness. Aggregation changes grainshape, density and size distribution of dust particles (i.e., characteristics determining erosion and transport); on deposition in the sea, cements dissolve and aggregates disintegrate, leaving the resultant eolo-marine sediment component with a misleading paleo-climatic record. The eolian transport of salts with dust from the arid coastal plain to the sea constitutes a portion of anticyclic salt movement and probably plays a role in the geochemical balance of the oceans.  相似文献   

Observation of a Complex Solar Wind Reconnection Exhaust from Spacecraft Separated by over 1800 R E     

Lavraud  B.  Gosling  J. T.  Rouillard  A. P.  Fedorov  A.  Opitz  A.  Sauvaud  J.-A.  Foullon  C.  Dandouras  I.  Génot  V.  Jacquey  C.  Louarn  P.  Mazelle  C.  Penou  E.  Phan  T. D.  Larson  D. E.  Luhmann  J. G.  Schroeder  P.  Skoug  R. M.  Steinberg  J. T.  Russell  C. T. 《Solar physics》2009,256(1-2):379-392

We analyze Wind, ACE, and STEREO (ST-A and ST-B) plasma and magnetic field data in the vicinity of the heliospheric current sheet (HCS) crossed by all spacecraft between 22:15 UT on 31 March and 01:25 UT on 1 April 2007 corresponding to its observation at ST-A and ST-B, which were separated by over 1800 R _E (or over 1200 R _E across the Sun?–?Earth line). Although only Wind and ACE provided good ion flow data in accord with a solar wind magnetic reconnection exhaust at the HCS, the magnetic field bifurcation typical of such exhausts was clearly observed at all spacecraft. They also all observed unambiguous strahl mixing within the exhaust, consistent with the sunward flow deflection observed at Wind and ACE and thus with the formation of closed magnetic field lines within the exhaust with both ends attached to the Sun. The strong dawnward flow deflection in the exhaust is consistent with the exhaust and X-line orientations obtained from minimum variance analysis at each spacecraft so that the X-line is almost along the GSE Z-axis and duskward of all the spacecraft. The observation of strahl mixing in extended and intermittent layers outside the exhaust by ST-A and ST-B is consistent with the formation of electron separatrix layers surrounding the exhaust. This event also provides further evidence that balanced parallel and antiparallel suprathermal electron fluxes are not a necessary condition for identification of closed field lines in the solar wind. In the present case the origin of the imbalance simply is the mixing of strahls of substantially different strengths from a different solar source each side of the HCS. The inferred exhaust orientations and distances of each spacecraft relative to the X-line show that the exhaust was likely nonplanar, following the Parker spiral orientation. Finally, the separatrix layers and exhausts properties at each spacecraft suggest that the magnetic reconnection X-line location and/or reconnection rate were variable in both space and time at such large scales.

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