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61.
Emergent Pleistocene sea level indicators in the northern Bahamas include: a bioerosional notch at +5.3 to 5.9 m; sea caves, notches, and marine terraces at about +4.3 m; and lithified coral rubble and reef deposits between 0 and 3 m. Thorium 230 dates of the fossil corals, which were deposited as these features were being produced, span the age range from 100 to 145 thousand years BP with a majority falling between 115 and 130 thousand years BP. The notch at about +5.6 m is interpreted to be the product of a sea level stand 125 thousand years BP, while the features at +4.3 m are believed to be formed sometime later as sea level fell from the higher position. Part of the age span is inherent in the dating technique and possible sample alteration. Another cause of the spread may be mixing of corals of different ages into a single deposit. 相似文献
62.
Heinrich Neumann 《Ocean Dynamics》1966,19(6):253-266
Zusammenfassung Es wurden mehrere Tausend Trifkarten ausgeworfen. Ihr Weg vom Auswurfort zum Fundort wurde mit Hilfe einer elektronischen Rechenanlage durch Modellrechnungen verfolgt, bei denen das Windfeld über der Nordsee vorgegeben war. Die Rechnung wurde so variiert, daß tatsächliche und rechnerische Fundorte der Karten möglichst gut übereinstimmten. (Abb. 3.). Hiernach treiben die Triftkarten in Windrichtung mit 4,2 v. H. der Windgeschwindigkeit. Das nur aus dem Wind gewonnene Bild des Triftweges läßt sich verbessern, wenn zusätzlich Oberflächenströmungen angenommen werden. Durch rechnerische Experimente wurde ein zu diesem Windfaktor passendes Stromfeld für die Nordsee ermittelt (Abb. 15).
Relation between wind and surface current derived from drift card investigations
Summary Several thousands of drift cards were released. Their route from the place of release to the place of retrieval was traced on an electronic computer by means of model computations where the wind field over the North Sea was preset. The computation was varied so to achieve the best possible agreement of actual and computational places of retrieval (Fig. 3). According to this, the cards are drifting in wind direction at 4.2 per cent of the wind velocity. The drift route exclusively derived from the wind can be improved by assuming, in addition, surface currents. Computational experiments delivered a current distribution in the North Sea corresponding to this wind factor (Fig. 15).
Les relations entre vent et courant superficiel déduites des études par cartes-flotteurs
Résumé Plusieurs milliers de cartes-flotteurs ayant été lancées, leur trajet du point de lancement au point de recupération a été établi à l'aide d'une calculatrice électronique avec un programme de calcul dans lequel était introduit le champ des vents en mer du Nord. Le calcul était si détaillé que le meilleur accord possible a été trouvé entre les lieux réels et calculés de découverte des cartes (fig. 3). On constate que les cartes sont poussées dans la direction du vent avec une vitesse égale à 4,2% de celle du vent. La représentation obtenue pour les trajets de dérive à partir du vent seul peut être amélioré si on considère en plus les courants superficiels. La représentation calculée montre pour la mer du Nord un champ de courant en accord avec ce facteur de vent (fig. 15).相似文献
63.
The influence of soil moisture on evaporation from a 6-m grass-covered lysimeter and from Class A pans was assessed for one summer using the -parameter of the Priestley-Taylor evaporation model appropriate for the individual surfaces computed on a daily basis. Net radiation over the pan was estimated from above-grass measurements using a correlation established between the two, using measurements made in the previous two summers. Changes in heat storage of the water were considered in the derivation of for the pan. A unique relationship for the particular conditions of the site was determined between the for the lysimeter and soil moisture, approaching 1.29 at soil moisture near field capacity, but decreasing to as low as 0.5 for dry soil. The corresponding relationship for the pan showed more scatter, but this was improved by using 5-day running means of evaporation and stratifying the data in terms of wind speed to yield a family of curves. Values for at wet soil conditions varied from 1.07 for 100 km day–1 wind run to 1.17 for 250 km day–1 wind run. For each curve, values of increased by about 20%; as the soil dried. The relationships may be used to reduce observed Class A pan evaporation to equivalent values for wet-soil conditions and to estimate near-surface soil moisture and actual evapotranspiration for this particular site. Extension of the technique to other areas requires derivation of similar relationships appropriate for those other locations 相似文献
64.
Tveitite is a new mineral with formula of the type is approximately 0.3. It is found in a cleavelandite pegmatite at Høydalen in Tørdal, Telemark, S. Norway. The sub-cell is thought to be monoclinic, . The structure is very similar to that of fluorite and can be described in terms of a pseudo-cubic cell which contains approximately 1[YCa3F9]. The mineral shows twinning in at lest three different directions giving a grating structure probably due to high-low inversion. DTA studies show an inversion point at about 670°C. Material heated above this temperature gives X-ray diffraction patterns corresponding to yttrofluorite (a0 5.528). The effect of trivalent ions on the stability of fluorite is discussed. 相似文献
65.
Rebecca G. Martin J. E. Pringle Christopher A. Tout 《Monthly notices of the Royal Astronomical Society》2007,381(4):1617-1624
We consider the shape of an accretion disc whose outer regions are misaligned with the spin axis of a central black hole and calculate the steady state form of the warped disc in the case where the viscosity and surface densities are power laws in the distance from the central black hole. We discuss the shape of the resulting disc in both the frame of the black hole and that of the outer disc. We note that some parts of the disc and also any companion star maybe shadowed from the central regions by the warp. We compute the torque on the black hole caused by the Lense–Thirring precession, and hence compute the alignment and precession time-scales. We generalize the case with viscosity and hence surface density independent of radius to more realistic density distributions for which the surface density is a decreasing function of radius. We find that the alignment time-scale does not change greatly but the precession time-scale is more sensitive. We also determine the effect on this time-scale if we truncate the disc. For a given truncation radius, the time-scales are less affected for more sharply falling density distributions. 相似文献
66.
Benjamin Poulter Rebecca L. Feldman Mark M. Brinson Benjamin P. Horton Michael K. Orbach Samuel H. Pearsall Enrique Reyes Stanley R. Riggs John C. Whitehead 《Ocean & Coastal Management》2009,52(3-4):147-153
Coastal areas are among the world's most vulnerable landscapes to impacts related to climate change, including inundation from sea-level rise (SLR), increased exposure to shoreline erosion, and greater frequency and intensity of storms. The status of research on the physical, ecological, and socio-economic effects of vulnerability to SLR and progress toward planning for its consequences varies from region to region worldwide. Here, we synthesize the results of three decades of SLR research and the development of coastal management policies in North Carolina, USA. We identify the major factors responsible for opening new policy ‘windows’ that address SLR, including how stakeholders have developed an increased understanding of the risks, the extent of public dialogue about potential response strategies, and advances in political receptivity to policy change. Research and policy progress in North Carolina continue to provide a model for other regions to help guide and evaluate the development of coastal policies. 相似文献
67.
Hyperspectral mapping of alteration assemblages within a hydrothermal vug at the Haughton impact structure,Canada
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Rebecca N. Greenberger John F. Mustard Gordon R. Osinski Livio L. Tornabene Alexandra J. Pontefract Cassandra L. Marion Roberta L. Flemming Janette H. Wilson Edward A. Cloutis 《Meteoritics & planetary science》2016,51(12):2274-2292
Meteorite impacts on Earth and Mars can generate hydrothermal systems that alter the primary mineralogies of rocks and provide suitable environments for microbial colonization. We investigate a calcite–marcasite‐bearing vug at the ~23 km diameter Haughton impact structure, Devon Island, Nunavut, Canada, using imaging spectroscopy of the outcrop in the field (0.65–1.1 μm) and samples in the laboratory (0.4–2.5 μm), point spectroscopy (0.35–2.5 μm), major element chemistry, and X‐ray diffraction analyses. The mineral assemblages mapped at the outcrop include marcasite; marcasite with minor gypsum and jarosite; fibroferrite and copiapite with minor gypsum and melanterite; gypsum, Fe3+ oxides, and jarosite; and calcite, gypsum, clay, microcline, and quartz. Hyperspectral mapping of alteration phases shows spatial patterns that illuminate changes in alteration conditions and formation of specific mineral phases. Marcasite formed from the postimpact hydrothermal system under reducing conditions, while subsequent weathering oxidized the marcasite at low temperatures and water/rock ratios. The acidic fluids resulting from the oxidation collected on flat‐lying portions of the outcrop, precipitating fibroferrite + copiapite. That assemblage then likely dissolved, and the changing chemistry and pH resulting from interaction with the calcite‐rich host rock formed gypsum‐bearing red coatings. These results have implications for understanding water–rock interactions and habitabilities at this site and on Mars. 相似文献
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70.
Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements: 2009 总被引:5,自引:0,他引:5
B. A. Archinal M. F. A��Hearn E. Bowell A. Conrad G. J. Consolmagno R. Courtin T. Fukushima D. Hestroffer J. L. Hilton G. A. Krasinsky G. Neumann J. Oberst P. K. Seidelmann P. Stooke D. J. Tholen P. C. Thomas I. P. Williams 《Celestial Mechanics and Dynamical Astronomy》2011,109(2):101-135
Every three years the IAU Working Group on Cartographic Coordinates and Rotational Elements revises tables giving the directions of the poles of rotation and the prime meridians of the planets, satellites, minor planets, and comets. This report takes into account the IAU Working Group for Planetary System Nomenclature (WGPSN) and the IAU Committee on Small Body Nomenclature (CSBN) definition of dwarf planets, introduces improved values for the pole and rotation rate of Mercury, returns the rotation rate of Jupiter to a previous value, introduces improved values for the rotation of five satellites of Saturn, and adds the equatorial radius of the Sun for comparison. It also adds or updates size and shape information for the Earth, Mars?? satellites Deimos and Phobos, the four Galilean satellites of Jupiter, and 22 satellites of Saturn. Pole, rotation, and size information has been added for the asteroids (21) Lutetia, (511) Davida, and (2867) ?teins. Pole and rotation information has been added for (2) Pallas and (21) Lutetia. Pole and rotation and mean radius information has been added for (1) Ceres. Pole information has been updated for (4) Vesta. The high precision realization for the pole and rotation rate of the Moon is updated. Alternative orientation models for Mars, Jupiter, and Saturn are noted. The Working Group also reaffirms that once an observable feature at a defined longitude is chosen, a longitude definition origin should not change except under unusual circumstances. It is also noted that alternative coordinate systems may exist for various (e.g. dynamical) purposes, but specific cartographic coordinate system information continues to be recommended for each body. The Working Group elaborates on its purpose, and also announces its plans to occasionally provide limited updates to its recommendations via its website, in order to address community needs for some updates more often than every 3 years. Brief recommendations are also made to the general planetary community regarding the need for controlled products, and improved or consensus rotation models for Mars, Jupiter, and Saturn. 相似文献