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排序方式: 共有411条查询结果,搜索用时 218 毫秒
1.
Steven J. Ostro Lance A. M. Benner Christopher Magri Jon D. Giorgini Randy Rose Raymond F. Jurgens Donald K. Yeomans Alice A. Hine Michael C. Nolan Daniel J. Scheeres Stephen B. Broschart Mikko Kaasalainen Jean‐Luc Margot 《Meteoritics & planetary science》2005,40(11):1563-1574
Abstract— We present June 2004 radar images of asteroid 25143 Itokawa (1998 SF36) that improve upon the longitude‐latitude coverage of images obtained in 2001 by Ostro et al. (2004) and use the 2001–2004 data to refine that paper's constraints on Itokawa's shape. The 2004 images, the first of the asteroid's southern side, look distinctly different from the 2001 images, revealing leading edges that are much more curved and rugged than the nearly convex leading edges seen at northern latitudes in 2001. Itokawa is shaped like a slightly asymmetrical, bent, lumpy ellipsoid with dimensions along the principal axes within 10% of 594 times 320 times 288 m. To illustrate the uncertainty space associated with shape reconstruction from images with suboptimal orientational coverage, we present two alternative three‐dimensional models of the object. 相似文献
2.
David M. Sherman Caroline L. Peacock Christopher G. Hubbard 《Geochimica et cosmochimica acta》2008,72(2):298-310
Sorption of U(VI) to goethite is a fundamental control on the mobility of uranium in soil and groundwater. Here, we investigated the sorption of U on goethite using EXAFS spectroscopy, batch sorption experiments and DFT calculations of the energetics and structures of possible surface complexes. Based on EXAFS spectra, it has previously been proposed that U(VI), as the uranyl cation , sorbs to Fe oxide hydroxide phases by forming a bidentate edge-sharing (E2) surface complex, >Fe(OH)2UO2(H2O)n. Here, we argue that this complex alone cannot account for the sorption capacity of goethite (α-FeOOH). Moreover, we show that all of the EXAFS signal attributed to the E2 complex can be accounted for by multiple scattering. We propose that the dominant surface complex in CO2-free systems is a bidentate corner-sharing (C2) complex, (>FeOH)2UO2(H2O)3 which can form on the dominant {101} surface. However, in the presence of CO2, we find an enhancement of UO2 sorption at low pH and attribute this to a (>FeO)CO2UO2 ternary complex. With increasing pH, U(VI) desorbs by the formation of aqueous carbonate and hydroxyl complexes. However, this desorption is preceded by the formation of a second ternary surface complex (>FeOH)2UO2CO3. The three proposed surface complexes, (>FeOH)2UO2(H2O)3, >FeOCO2UO2, and (>FeOH)2UO2CO3 are consistent with EXAFS spectra. Using these complexes, we developed a surface complexation model for U on goethite with a 1-pK model for surface protonation, an extended Stern model for surface electrostatics and inclusion of all known UO2-OH-CO3 aqueous complexes in the current thermodynamic database. The model gives an excellent fit to our sorption experiments done in both ambient and reduced CO2 environments at surface loadings of 0.02-2.0 wt% U. 相似文献
3.
Martin R. Lee Mark E. Hodson Maureen MacKenzie Caroline L. Smith 《Geochimica et cosmochimica acta》2008,72(20):4962-4975
Our ability to identify thin non-stoichiometric and amorphous layers beneath mineral surfaces has been tested by undertaking X-ray photoelectron spectroscopy (XPS) and transmission electron microscopy (TEM) work on alkali feldspars from pH 1 dissolution experiments. The outcomes of this work were used to help interpret XPS and TEM results from alkali feldspars weathered for <10,000 years in soils overlying the Shap Granite (north-west England). The chemistry of effluent solutions indicates that silica-rich layers a few nanometers in thickness formed during the pH 1 experiments. These layers can be successfully identified by XPS and have lower Al/Si, Na/Si, K/Si and Ca/Si values than the outermost ∼9 nm of unweathered controls. Development of Al-Si non-stoichiometry is coupled with loss of crystal structure to produce amorphous layers that are identifiable by TEM where >∼2.5 nm thick, whereas the crystallinity of albite is retained despite leaching of Na to depths of tens to hundreds on nanometers. Integration of XPS data over the outermost 6-9 nm of naturally weathered Shap feldspars shows that they have stoichiometric Al/Si and K/Si ratios, which is consistent with findings of previous TEM work on the same material that they lack amorphous layers. There is some XPS evidence for loss of K from the outermost couple of nanometers of Shap orthoclase, and the possibility of leaching of Na from albite to greater depths cannot be excluded using the XPS or TEM results. This study demonstrates that the leached layer model, as formulated from laboratory experiments, is inapplicable to the weathering of alkali feldspars within acidic soils, which is an essentially stoichiometric reaction. 相似文献
4.
Geologic relations indicate that silica phases transformed in the Monterey Formation in two zones that persist over a narrow
depth/temperature range and do not stratigraphically overlap. The wide and overlapping range of reported temperatures of these
transformations is mainly a result of the many uncertainties inherent in the different methods used to estimate temperature
and does not indicate that phases transform throughout these ranges. Our approach to a reliable temperature scale for silica
diagenesis combines as empirical zonation of silica phases with temperature calibration from a sequence at maximum temperature
and depth of burial. 相似文献
5.
Carbon balance in a salt marsh: Interactions of diffusive export, tidal deposition and rainfall-caused erosion 总被引:1,自引:0,他引:1
Alice G. Chalmers Richard G. Wiegert Paul L. Wolf 《Estuarine, Coastal and Shelf Science》1985,21(6):757-771
Studies of the concentrations of particulate and dissolved organic carbon in the Duplin River, of the tidal exchange of POC and DOC in the marsh, of the standing stock and movement of Spartina alterniflora wrack in the Duplin, and of the removal of carbon from the surface of the marsh by rain were conducted at Sapelo Island, Georgia in order to test three hypotheses about export of carbon from the Duplin River watershed. We found that the gradients in POC and DOC concentrations are such that carbon is being transported down the Duplin River throughout the year, although in smaller quantities than previously believed. In contrast, almost all tidal exchanges within the marsh result in deposition of carbon. Most of this deposited carbon is subsequently eroded as a result of rain falling on the exposed marsh surface, and is washed back into the tidal creeks. This cycle of deposition and erosion is a possible mechanism keeping POC in the thin aerobic surface layer of the marsh, thus increasing its availability to detritivores and aerobic microbes. The standing stock of wrack is only a fraction of the S. alterniflora produced each year, and its export is a negligible term in the carbon balance equation. 相似文献
6.
The Global Programme of Action for the Protection of the Marine Environment from Land-based Activities (GPA) represents an ambitious attempt to make the leap between the rhetoric of protecting and preserving the marine environment and action. With degradation of the marine environment from land based activities posing one of the most serious threats to the quality and productivity of the coastal and marine environment, the GPA can only be viewed as a milestone rather than a destination, as so much work remains to be done in this field.States supporting the GPA are entering the most challenging phase of the program, that of implementation. But the international community in taking on this challenge is not without a few signposts. The failure of the Montreal Guidelines to be implemented, provides States with many important lessons. This paper suggests that if the GPA is to have an impact on the complex problem of land-based activities then several tasks need to be grappled with. Substantial financial support needs to be generated, a proactive and cooperative secretariat established and the nexus between the GPA and United Nations Environment Programme Regional Seas Programme examined. The importance of people and training to the capacity building process needs to be recognised and a wider variety of stakeholders engaged in the follow up phase. Pivotal to the aforementioned is the need to generate political will to address the problem, without which the GPA will become yet another dusty volume on the bookshelf. 相似文献
7.
Caroline M. Isaacs 《Geo-Marine Letters》1985,5(1):25-30
Although best known as a deposit rich in silica and organic matter, the Miocene Monterey Formation actually had long-term
rates of silica and organic Matter accumulation equal to or lower than values in the underlying and overlying detritus-rich
formations in the Santa Barbara coastal area. The factor Mainly influencing the composition of the Monterey Formation in this
area was the slow accumulation of terrigenous debris. In contrast, with greater than average silica abundance within the Monterey
Formation probably resulted from rapid short-term silica accumulation (of hundreds to tens of thousands years duration) rather
than from especially slow accumulation of diluting debris. 相似文献
8.
Fragmentation, or the "coming apart" of magma during a plinian eruption, remains one of the least understood processes in
volcanology, although assumptions about the timing and mechanisms of fragmentation are key parameters in all existing eruption
models. Despite evidence to the contrary, most models assume that fragmentation occurs at a critical vesicularity (volume
percent vesicles) of 75–83%. We propose instead that the degree to which magma is fragmented is determined by factors controlling
bubble coalescence: magma viscosity, temperature, bubble size distribution, bubble shapes, and time. Bubble coalescence in
vesiculating magmas creates permeability which serves to connect the dispersed gas phase. When sufficiently developed, permeability
allows subsequent exsolved and expanded gas to escape, thus preserving a sufficiently interconnected region of vesicular magma
as a pumice clast, rather than fully fragmenting it to ash. For this reason pumice is likely to preserve information about
(a) how permeability develops and (b) the critical permeability needed to insure clast preservation. We present measurements
and calculations that constrain the conditions (vesicularity, bubble size distribution, time, pressure difference, viscosity)
necessary for adequate permeability to develop. We suggest that magma fragments explosively to ash when and where, in a heterogeneously
vesiculating magma, these conditions are not met. Both the development of permeability by bubble wall thinning and rupture
and the loss of gas through a permeable network of bubbles require time, consistent with the observation that degree of fragmentation
(i.e., amount of ash) increases with increasing eruption rate.
Received: 5 July 1995 / Accepted: 27 December 1995 相似文献
9.
In order to better understand condensation processes that took place in the solar nebula and to evaluate the effect of kinetics on the condensed matter, we have built an experimental apparatus for studying condensation of multi-elemental refractory gases at high-temperature and low-pressure. The condensation of a Mg-Si-rich gas, with solar interelement ratios of Ca, Al, Mg and Si, and of a Ca-Al-rich gas under a total pressure of ∼4 × 10−3 bar at temperatures from 1045 to 1285 °C and for run times of 4-60 min results in direct formation of crystalline oxides or silicates such as corundum, spinel, anorthite, melilite, Al-diopside, forsterite and enstatite. The mineralogy of the condensates, close to that predicted at equilibrium, varies with the duration of an experiment and the temperature of condensation. The chemical reactions between gas and condensates are rapid enough to attain a steady state in less than one hour. The condensation results in chemical fractionation of the gas, i.e. a depletion of the gas in refractory elements at high temperature. Finally, besides revealing the textures of refractory crystals, which condense from a gas of complex chemical composition, this study shows that certain phases, such as spinel, have favored kinetics of condensation. Our experimental results confirm that refractory inclusions in primitive meteorites could have formed by condensation from a hot nebular gas. Similarly, we confirm that crystalline grains can condense at high temperature in the outflows of evolved stars. In both cases, our results indicate that kinetic processes certainly influence grain mineralogy. Kinetic processes must thus be taken into account in modeling the pressure-temperature conditions of circumstellar environments. 相似文献
10.
Estimating concentrations or flow rates along a stream network requires specific models. Two classes of models, recently proposed in the literature, are generalized, to the intrinsic case in particular. We present a global construction by ‘streams’, i.e. on the whole set of paths between sources and outlet. Combining stationary or intrinsic one-dimensional random functions leads to stationary or intrinsic models on segments, with discontinuities at the forks. A construction from outlet to sources, leads to stationary or intrinsic models on each stream, without any discontinuity at the forks. The linear variogram is found as a particular case. The extension to the linear model of coregionalization is immediate, allowing a multivariate modelling of concentrations. To cite this article: C. de Fouquet, C. Bernard-Michel, C. R. Geoscience 338 (2006). 相似文献