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1.
Alan M Bond Julie R Bradbury Henry A Hudson John S Garnham Peter J Hanna Stanley Strother 《Marine Chemistry》1985,16(1):1-9
Evidence was found that uptake of lead from seawater in both model and natural systems by the leaves of the seagrass Zostera muelleri does occur for live, dead and scraped leaves at all the lead concentrations tested. Positive uptake of lead was measured using the three analytical techniques of radio-tracer, differential pulse anodic stripping voltammetry and atomic absorption spectrometry; similar uptake profiles were obtained for each technique. Profiles always showed an initial rapid uptake phase followed by a gradual transition to a plateau phase at which an approximate equilibrium between lead attached to seagrass and free ionic lead in seawater was reached. The presence of active lead uptake processes was indicated in experiments which attempted to remove lead from leaves by a chelating agent. 相似文献
2.
The interior motions in steady, layered, geostrophic models of large scale wind-driven phenomena are severely constrained if there is no stress transfer across the interfaces. In particular, there will be no motion in the subsurface layers except in regions where the layers rise to the surface and are exposed to the wind-stress or unless the layers are in contact with lateral boundary layers with which they exchange fluid. These results follow directly from quite general considerations that are outlined in this paper. 相似文献
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Dwarf elliptical (dE) galaxies, with blue absolute magnitudes typically fainter than MB =?16, are the most numerous type of galaxy in the nearby universe. Tremendous advances have been made over the past several years in delineating the properties of both Local Group satellite dE's and the large dE populations of nearby clusters. We review some of these advances, with particular attention to how well currently available data can constrain
- models for the formation of dE's
- the physical and evolutionary connections between different types of galaxies (nucleated and nonnucleated dE's, compact E's, irregulars, and blue compact dwarfs) that overlap in the same portion of the mass-spectrum of galaxies
- the contribution of dE's to the galaxy luminosity functions in clusters and the field
- the star-forming histories of dE's and their possible contribution to faint galaxy counts, and
- the clustering properties of dE's.
5.
Anton P le Roex Henry J B Dick Ronald T Watkins 《Contributions to Mineralogy and Petrology》1992,110(2-3):253-268
Glassy pillow basalts with unusual geochemical characteristics for mid-ocean ridge basalt (MORB) have been dredge sampled from the Southwest Indian Ridge between 12 and 15°E during Leg ANT IV/4 of the F.S. POLARSTERN. Lavas from 4 of 6 dredges are moderately nepheline normative, highly K-enriched (0.5–1.77 wt% K2O) alkali basalts and hawaiites. Mg-numbers indicate that many of the lavas are fairly primitive (Mg No.=63–67), yet show extreme enrichment in incompatible elements; e.g. Nb (24–60 ppm), Ba (170–470 ppm) and Sr (258–460 ppm). Incompatible-element ratios such as Zr/Nb (3–5) and Y/Nb (0.46–1.1) are extremely low even for E-type (enriched) MORB, whereas (La/Yb)n ratios are particularly high (3.4–7.8). 87Sr/86Sr (0.70290–0.70368), 143Nd/144Nd (0.51302–0.51284) and 206Pb/204Pb (18.708–19.564) isotopic ratios further indicate the geochemically enriched nature of these lavas, which range from the compositional field for depleted N-type (normal) MORB towards the composition of Bouvet Island lavas. Mutually correlated incompatible-element and Sr-, Nd- and Pb-isotopic ratios allow a fairly well constrained model to be developed for the petrogenesis of these unusually alkalic mid-ocean ridge lavas. The alkalic nature and degree of enrichment in incompatible elements is ascribed to particularly low degrees of partial melting (3–5 wt%), at greater than usual depth, of a source region that has experienced prior geochemical enrichment (by veining) related to the upwelling Bouvet mantle plume. To account for the observed compositional variations, a model is proposed whereby mixing between partial melts derived from these geochemically enriched silicate veins, and an incipient to low percentage (±2%) melt from the surrounding geochemically depleted suboceanic asthenosphere occurs as a consequence of increasing degree of melting with adiabatic upwelling. Eruption of these alkalic lavas in this spreading ridge environment is attributed to a temporary hiatus in tholeiitic volcanism and associated spreading along this section of the Southwest Indian Ridge, related to readjustment of spreading direction to a more stable plate geometry. 相似文献
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7.
Boualem Bayou Mohamed El-Messaoud Derder Bernard Henry Hamou Djellit Mohamed Amenna 《Comptes Rendus Geoscience》2002,334(2):81-87
Palaeomagnetic study, carried out in the Moscovian (~305 Ma) formation in the Edjeleh anticline, shows the existence of three magnetisation components. Two of them are probably Cenozoic and Permian remagnetisations. The third component determined by both well defined ChRMs and remagnetisation circles analysis passes the fold test. Because the folding started before or during the Stephano-Autunian, this third component is the primary magnetisation. Its palaeomagnetic pole (28.3°S, 58.9°E), close to other poles from the Saharan platform obtained from neighbouring periods but without palaeomagnetic tests, confirms the age of these last data. To cite this article: B. Bayou et al., C. R. Geoscience 334 (2002) 81–87. 相似文献
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10.
Bernard Henry Grobéty 《Contributions to Mineralogy and Petrology》1997,127(3):237-247
Anthophyllite crystals found in ultramafic lenses of the Lepontine Alps (Switzerland) contain coherent, submicroscopic intergrowths
of ordered and disordered biopyribole polysomes. The chain width distributions of disordered polysomes were analyzed using
high resolution transmission electron microscopy (HRTEM). Chains wider than triple were interpreted as intermediate products
in the transformation of anthophyllite to the triple chain silicate jimthompsonite. The concentration of individual chain
types is strongly correlated with the reaction progress. Based on observed zipper terminations and the transformation rules
given by Veblen and Buseck (1980) a scheme of possible reaction paths leading from anthophyllite to jimthomp sonite is proposed.
The reaction scheme and a simple kinetic model for elementary reactions allow modeling of the observed chain width distributions.
The model suggests that the complex reaction paths involving steps with increasing and decreasing chain width are more important
in the formation of jimthompsonite than the direct transformation from anthophyllite. The wide chains (>triple) occurring
as intermediate products of the multi-step paths are structurally closer to talc than jimthompsonite. The back-transformation
of these wide chains to triple chains is, therefore, a strong argument that jimthompsonite is a stable phase and not only
a metastable intermediate product in the transformation of anthophyllite to talc.
Received: 8 July 1996 / Accepted: 13 December 1996 相似文献