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71.
Göran Björk Leif G. Anderson Martin Jakobsson Dennis Antony Björn Eriksson Patrick B. Eriksson Benjamin Hell Sofia Hjalmarsson Timothy Janzen Sara Jutterström Johanna Linders Ludvig Löwemark Christian Marcussen K. Anders Olsson Bert Rudels Emma Sellén Morten Sølvsten 《Deep Sea Research Part I: Oceanographic Research Papers》2010,57(4):577-586
The LOMROG 2007 expedition targeted the previously unexplored southern part of the Lomonosov Ridge north of Greenland together with a section from the Morris Jesup Rise to Gakkel Ridge. The oceanographic data show that Canadian Basin Deep Water (CBDW) passes the Lomonosov Ridge in the area of the Intra Basin close to the North Pole and then continues along the ridge towards Greenland and further along its northernmost continental slope. The CBDW is clearly evident as a salinity maximum and oxygen minimum at a depth of about 2000 m. The cross-slope sections at the Amundsen Basin side of the Lomonosov Ridge and further south at the Morris Jesup Rise show a sharp frontal structure higher up in the water column between Makarov Basin water and Amundsen Basin water. The frontal structure continues upward into the Atlantic Water up to a depth of about 300 m. The observed water mass division at levels well above the ridge crest indicates a strong topographic steering of the flow and that different water masses tend to pass the ridge guided by ridge-crossing isobaths at local topographic heights and depressions. A rough scaling analysis shows that the extremely steep and sharply turning bathymetry of the Morris Jesup Rise may force the boundary current to separate and generate deep eddies. 相似文献
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74.
A. C. Layden P. A. Fox J. M. Howard A. Sarajedini K. H. Schatten S. Sofia 《Solar physics》1991,132(1):1-40
In this paper we present a general framework for forecasting the smoothed maximum level of solar activity in a given cycle, based on a simple understanding of the solar dynamo. This type of forecasting requires knowledge of the Sun's polar magnetic field strength at the preceeding activity minimum. Because direct measurements of this quantity are difficult to obtain, we evaluate the quality of a number of proxy indicators already used by other authors which are physically related to the Sun's polar field. We subject these indicators to a rigorous statistical analysis, and specify in detail the analysis technique for each indicator in order to simplify and systematize reanalysis for future use. We find that several of these proxies are in fact poorly correlated or uncorrelated with solar activity, and thus are of little value for predicting activity maxima.We also present a scheme in which the predictions of the individual proxies are combined via an appropriately weighted mean to produce a compound prediction. We then apply the scheme to the current cycle 22, and estimate a maximum smoothed International sunspot number of 171 ± 26, which can be expressed alternatively as a smoothed 2800 MHz radio flux (F
10.7) of 211 ± 23 × (10–22 Wm–2Hz–1), or as a smoothed sunspot area of 2660 ± 430 millionths of a solar disk. Once the actual maximum for cycle 22 has been established, we will have both additional statistics for all the proxy indicators, and a clearer indication of how accurately the present scheme can predict solar activity levels. 相似文献
75.
Sofia?De GregorioEmail author Silvio?G.?Rotolo Igor?M.?Villa 《International Journal of Earth Sciences》2003,92(6):852-872
The Peloritani Mountains are a fragment of an orogen variably attributed to the Alpine or Hercynian orogeny. On the basis of 39Ar-40Ar, U-Pb and Rb-Sr dating, the main metamorphism of the two medium–high grade metamorphic units, the Mela and Aspromonte Units, and most of the thrusting responsible for stacking the orogenic edifice are seen to be Hercynian. The main thrusting of the Aspromonte Unit over the lower grade units took place at 301±2 Ma. Brittle deformation during Tertiary reactivation of Hercynian thrust planes did not generate any rejuvenation of white micas in the studied sector. Our dataset shows a great complexity and we propose to unravel it by considering different levels of information. To first order, the Mela and Aspromonte Units differ in their metamorphic paths and their geochronological evolution. The Mela Unit shows generally younger ages (Carboniferous) than the Aspromonte Unit and, unlike the latter, was extensively retrogressed in greenschist facies. The Aspromonte Unit is itself geochronologically heterogeneous. Proterozoic ages are preserved both in titanite and in amphibole relics of one tectonic subunit; Devonian to Carboniferous amphibole ages are found in different other subunits; tertiary overprint is minor and spatially limited. We propose to consider the chronologically heterogeneous subunits as accreted pre-Hercynian terranes amalgamated late during the Hercynian orogeny. Micas in both units give scattered Mesozoic 39Ar-40Ar and Rb-Sr ages, with evidence for heterochemical mica generations. We interpret them as a result of widespread hydrothermal circulation event(s). Tertiary overprint is generally absent, with the exception of a small area near Messina where biotite and muscovite underwent a complex recrystallisation history in the interval between 48 and 61 Ma.An erratum to this article can be found at 相似文献
76.
The basic design and the scientific aims of the EUDOSSO project are described. EUDOSSO is a space instrument conceived for achieving very high accuracy and long term stability in measuring solar diameter time variations. Therefore it is suitable for measuring long periodg-modes, oblateness and long-term diameter variations possibly relevant to climatic changes. 相似文献
77.
An analysis of axially and torsionally loaded piles is presented in which the pile is treated as an elastic bar supported on two series of interacting non-linear axial and torsional springs. The characteristics of these springs depend on the soil properties and the diameter of the pile as well as on the interaction between the axial and torsional response. Predicted pile responses are compared to the results of model tests conducted on piles installed in a soft clay bed and loaded with combined axial and torsional loads. Both experimental results and theoretical predictions show that a torque applied to the pile head affects significantly the settlement and the axial bearing capacity of the pile. 相似文献
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The study of numerous archaeological excavations permits us to concludethat shortly after AD 355–361, the wealthy Roman town of Kisamos inwestern Crete was affected by a devastating earthquake (minimum intensityXI), which left many of the town's inhabitants buried under the ruins. Thisearthquake can be related to the July 21, 365 earthquake (M > 8),which was associated with a great tsunami, and was probably responsible forup to 9 m uplift of Western Crete; it probably resulted from thereactivation of a major thrust fault along the Hellenic Arc. Thearchaeological stratigraphy of Kisamos between circa AD 50 and AD650 testifies to two other, small-scale stratigraphic discontinuities that maybe related to two other smaller earthquakes, which produced 10–20 cmof coastal subsidence in AD 46–66 and in circa AD 270. There isevidence for a tsunami associated with the AD 46–66 earthquake, whichagrees with sedimentological data from the nearby ancient harbour ofPhalasarna, which was uplifted about 6.5 m in AD 365.The following evidence indicates that Western Crete is not seismicallyquiescent, as previously believed on the basis of historical data, but that ithas been affected by very strong, AD 365-type earthquakes followed byrelatively quiescence periods, that were at least several thousand years long:(1) Major earthquakes of Western Crete produced coastal uplift orsubsidence, while coastal stability indicates the absence of strongearthquakes; such stability characterizes this part of the island after AD365; (2) No evidence of earthquakes exist in the archaeological record ofKisamos between AD 365 and circa AD 650 and of Chania since AD1400/1500. 相似文献
80.
The feeding habits of several fish species in a water reservoir of the Ria Formosa, Portugal, that has similar ecological characteristics to the outside tidal channels, were studied and compared with food availability. The gilthead seabream (Sparus aurata), the most abundant fish species, mainly selected gastropods and bivalves, although occasionally fish and small crustaceans such as tanaids, ostracods, and cumaceans were also selected. Polychaetes, although abundant in the environment, were not particularly selected by any of the fish species studied. The diets of all the species studied were characterized by a large variety of prey, allowing them to survive in environments of low diversity and poor stability, such as coastal lagoons. These fish are largely benthic feeders, essentially eating the epimacroinvertebrates and endomacroinvertebrates and, occasionally, fish.Diplodus vulgaris andDiplodus annularis preferentially selected gastropods and small crustaceans.Spondyliosoma cantharus generally preyed on crustaceans, including the highly mobile epifauma, the mysids, and decapods.Halobatrachus didactylus andAnguilla anguilla, had very diversified diets that included fish.Mullus barbatus were found to have selected all groups of crustaceans and also bivalves. Wrasses, gobies, andDiplodus sargus, all small-sized fish, singled out small crustaceans, gastropods, and bivalves. The Sparids were the least specialized predators, with broader niches than the other species. They preferentially selected molluscs, which were abundant in the environment. A large overlap of diets was observed and competition may be important when fish biomass is high. 相似文献