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231.
232.
An integrated model of clastic injectites and basin floor lobe complexes: implications for stratigraphic trap plays
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Sarah Louise Cobain David Mark Hodgson Jeff Peakall Michelle Nicole Shiers 《Basin Research》2017,29(6):816-835
Injectites sourced from base‐of‐slope and basin‐floor parent sandbodies are rarely reported in comparison to submarine slope channel systems. This study utilizes the well‐constrained palaeogeographic and stratigraphic context of three outcrop examples exposed in the Karoo Basin, South Africa, to examine the relationship between abrupt stratigraphic pinchouts in basin‐floor lobe complexes, and the presence, controls, and character of injectite architecture. Injectites in this palaeogeographic setting occur where there is: (i) sealing mudstone both above and below the parent sand to create initial overpressure; (ii) an abrupt pinchout of a basin‐floor lobe complex through steep confinement to promote compaction drive; (iii) clean, proximal sand beds aiding fluidization; and (iv) a sharp contact between parent sand and host lithology generating a source point for hydraulic fracture and resultant injection of sand. In all outcrop cases, dykes are orientated perpendicular to palaeoslope, and the injected sand propagated laterally beneath the parent sand, paralleling the base to extend beyond its pinchout. Understanding the mechanisms that determine and drive injection is important in improving the prediction of the location and character of clastic injectites in the subsurface. Here, we highlight the close association of basin‐floor stratigraphic traps and sub‐seismic clastic injectites, and present a model to explain the presence and morphology of injectites in these locations. 相似文献
233.
Nicole St-Louis 《Astrophysics and Space Science》1998,260(1-2):161-171
In this paper, I present a brief overview of the observational evidence for the interaction between the winds of hot stars
and their surrounding interstellar medium (ISM). As the star evolves, it will impinge on the gas in different ways depending
on the nature of its wind and on the physical state of the interstellar gas. The three main evolutionary phases of massive
stars, the main sequence O phase, the intermediate red supergiant or luminous blue variable phase and finally the Wolf-Rayet
phase are discussed. The study of the ISM in the vicinity of hot stars is shown to be a powerful tool to study the history
of the gas and gain more insight into the evolution of the star.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
234.
235.
Leontine E. Becking Daniel F. R. Cleary Nicole J. de Voogd Willem Renema Manon de Beer Rob W. M. van Soest & Bert W. Hoeksema 《Marine Ecology》2006,27(1):76-88
In order to preserve diversity it is essential to understand how assemblages change across space. Despite this fact, we still know very little about how marine diversity is spatially distributed, especially among lesser‐studied invertebrate taxa. In the present study beta‐diversity patterns of sea urchins, sponges, mushroom corals and larger foraminifera were assessed in the Spermonde Archipelago (Indonesia). Using ordinations we showed that the inshore zone (<5 km offshore), midshore zone (5 < x < 30 km offshore) and distance offshore zone (>30 km offshore) all contained distinct assemblages of sponges and corals, while only foraminifera assemblages from the inshore (<5 km offshore) zone were distinct. There was a significant spatial pattern of community similarity for all taxa surveyed, but this pattern proved to be wholly related to environmental variables for sponges and foraminifera, and primarily for mushroom corals and sea urchins. The lack of a pure spatial component suggests that these taxa may not be dispersal limited within the spatial scales of this study (c. 1600 km2). The analyses of the corals and foraminifera were additionally tested at two spatial scales of sampling. Both taxa were primarily associated with local‐scale environmental variables at the local scale and larger‐scale variables at the larger scale. Mean inter‐plot similarity was also higher and variation lower at the larger scale. The results suggest that substantial variation in similarity can be predicted using simple locally assessed environmental variables combined with remotely sensed parameters. 相似文献
236.
William Gladstone Nicole Hacking Vanessa Owen 《Estuarine, Coastal and Shelf Science》2006,67(4):708-720
Intermittently opening estuaries are artificially opened to manage flood risk, water quality, recreational amenity, and fisheries; however, the ecological impacts of this management technique are incompletely understood. During 2001 and 2004, this study assessed the impacts of artificial openings on the macroinvertebrates of entrance barriers of intermittently opening estuaries in New South Wales (Australia). In 2001 macroinvertebrates were sampled once before artificial opening and 9 and 25 d after re-formation of the entrance barrier. A multiple before–after-control-impact analysis found that, although entrance barriers were destroyed by the artificial openings and then re-formed naturally by wave action, significant interactions for taxonomic richness, density of the amphipod Paracalliope australis (Gammaridae) and density of the gastropod mollusc Aschoris victoriae (Hydrobiidae) meant that the effects of this disturbance could not be distinguished from the natural variations that occurred in unopened estuaries. Multivariate analyses found that assemblages at both opened and unopened estuaries changed from before to after the openings, and the magnitude of the dissimilarity between times varied between estuaries. In 2004, macroinvertebrates were sampled on three randomly selected days within each of three periods (before, 3 d and 42 d after) at one opened and three unopened estuaries. Asymmetrical analysis of this modified before–after-control-impact study found that the change in taxonomic richness at the opened estuary from before to after opening did not differ from temporal changes that occurred in unopened estuaries. Short-term variation (i.e. between days) in total density of macroinvertebrates and density of P. australis in the re-formed entrance barrier of the opened estuary also did not differ from the variation in the control estuaries. Additionally, assemblage structure was not significantly changed by the opening and assemblages at two control estuaries were also unchanged over the same time. Individual taxa and assemblages of macroinvertebrates in entrance barriers of these intermittently open estuarine systems appear to be resilient to the habitat disturbance caused by artificial openings. 相似文献
237.
Boris Radosavljevic Hugues Lantuit Wayne Pollard Paul Overduin Nicole Couture Torsten Sachs Veit Helm Michael Fritz 《Estuaries and Coasts》2016,39(4):900-915
Arctic coastal infrastructure and cultural and archeological sites are increasingly vulnerable to erosion and flooding due to amplified warming of the Arctic, sea level rise, lengthening of open water periods, and a predicted increase in frequency of major storms. Mitigating these hazards necessitates decision-making tools at an appropriate scale. The objectives of this paper are to provide such a tool by assessing potential erosion and flood hazards at Herschel Island, a UNESCO World Heritage candidate site. This study focused on Simpson Point and the adjacent coastal sections because of their archeological, historical, and cultural significance. Shoreline movement was analyzed using the Digital Shoreline Analysis System (DSAS) after digitizing shorelines from 1952, 1970, 2000, and 2011. For purposes of this analysis, the coast was divided in seven coastal reaches (CRs) reflecting different morphologies and/or exposures. Using linear regression rates obtained from these data, projections of shoreline position were made for 20 and 50 years into the future. Flood hazard was assessed using a least cost path analysis based on a high-resolution light detection and ranging (LiDAR) dataset and current Intergovernmental Panel on Climate Change sea level estimates. Widespread erosion characterizes the study area. The rate of shoreline movement in different periods of the study ranges from ?5.5 to 2.7 m·a?1 (mean ?0.6 m·a?1). Mean coastal retreat decreased from ?0.6 m·a?1 to ?0.5 m·a?1, for 1952–1970 and 1970–2000, respectively, and increased to ?1.3 m·a?1 in the period 2000–2011. Ice-rich coastal sections most exposed to wave attack exhibited the highest rates of coastal retreat. The geohazard map combines shoreline projections and flood hazard analyses to show that most of the spit area has extreme or very high flood hazard potential, and some buildings are vulnerable to coastal erosion. This study demonstrates that transgressive forcing may provide ample sediment for the expansion of depositional landforms, while growing more susceptible to overwash and flooding. 相似文献
238.
Chlorine and fluorine were measured from whole-rock samples from tholeiites (150,000 years old) to present-day hawaiites. The overall range of F content is from 240 to 985 ppm, with a slight decrease of F/Th and F/Cl ratios, from tholeiites to hawaiites. Chlorine is positively correlated with Th (Cl/Th=100) as well as K2O and P2O5, as the differentiation progresses, and, increases from 220 ppm in tholeiites to 2410 ppm in mugearites. Data obtained from present-day hawaiites indicate that Cl lost by degassing during eruption is limited. However, Cl contents of some whole-rock samples are inconsistent with previous results published for melt inclusions of phenocrysts from the same historic hawaiite samples and suggesting outgassing of Cl prior to the eruption. This implies that apparent correlation between Cl and Th can be considered as the result of superimposition of several petrogenetic processes. Results point out the richness of Etnean tholeiites in chlorine compared to M.A.R. basalts. Such a character could have been inherited from the mantle source or during the mantle source melting. 相似文献
239.
Nicole Le Breton 《Contributions to Mineralogy and Petrology》1989,103(3):387-396
CO2 molecules were introduced experimentally into the structural channels of synthetic well ordered Mgcordierite (Mg2
[VI][(Al4Si5)[IV]O18]) at temperatures of 600 and 800° C, and pressures of 7, 8, 10, 12, and 25 kbar. Powder infrared spectra of the run products show five absorption bands in the region of the asymmetric stretching mode of CO2. Two of them, strong and sharp, occurring at 2353 cm–1 {2} and 2348 cm–1 {3}, are related to two different types of CO2 molecules. The relative intensity of the band {2} (type I) increases with the cell parameter co whereas the relative intensity of the band {3} (type II) increases with the parameter a0 of the crystal. It is concluded that CO2 molecules of type I may be oriented with their elongation parallel to the c-axis of the crystal, while CO2 molecules of type II lie with their O-C-O vector parallel to the a-axis. Analytical data indicate that the intensity ratio Z of these two bands ({2}/{3}) is a linear function of the CO2 content of cordierite. This ratio depends also on the temperature and, to a less extent, on the pressure under which cordierite entrapped CO2 molecules. It is proposed to combine this infrared parameter Z together with an estimate of the P-T conditions of the incorporation of CO2 into the channels, in order to determine the CO2 content of natural cordierites. The samples do not need to be of high purity and only small amounts (<5 mg) are necessary. This semi-empirical analytical method, which does not require complicated data treatments, is suitable for CO2-rich cordierites of granulite facies rocks. 相似文献
240.
Nicole Girardin 《Physics of the Earth and Planetary Interiors》1980,23(3):199-206
PP waves have been used to transform PP residuals with respect to Jeffreys-Bullen time into P-wave travel-time delays close to the reflection point. It is found that P-wave travel-time delays decrease with the age of the plate for oceanic structures. Average oceanic lithosphere (100 My) has a residual similar to that of a typical continental platform (Siberia). The absence of a P-wave low velocity zone under platform regions is sufficient to explain the small difference in residuals between old oceanic regions and the Siberian platform. Thus, from these observations, there is no evidence that would favour a substantial structural difference between continents and oceans at depths greater than 250 km. 相似文献