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461.
C. M. Pieters A. Nathues G. Thangjam M. Hoffmann T. Platz M. C. de Sanctis E. Ammannito F. Tosi F. Zambon J. H. Pasckert H. Hiesinger S. E. Schröder R. Jaumann K.‐D. Matz J. C. Castillo‐Rogez O. Ruesch L. A. McFadden D. P. O'Brien M. Sykes C. A. Raymond C. T. Russell 《Meteoritics & planetary science》2018,53(9):1983-1998
The geologic context of red organic‐rich materials (ROR) found across an elongated 200 km region on Ceres is evaluated with spectral information from the multispectral framing camera (FC) and the visible and near‐infrared mapping spectrometer (VIR) of Dawn. Discrete areas of ROR materials are found to be associated with small fresh craters less than a few hundred meters in diameter. Regions with the highest concentration of discrete ROR areas exhibit a weaker diffuse background of ROR materials. The observed pattern could be consistent with a field of secondary impacts, but no appropriate primary crater has been found. Both endogenic and exogenic sources are being considered for these distinctive organic materials. 相似文献
462.
Simultaneous observations obtained with the HAO/SPO coronal emission-line polarimeter and the new SPO emission-line coronagraph are compared. The polarimeter data are measured in the Fexiii (10747 Å) line and the coronagraph observations are recorded in the Fexiv (5303 Å) line. The polarimeter field-of-view is relatively coarse compared with the resolution limit of the coronagraph. Therefore, the observed coronal polarization cannot be related directly to the detailed loop structures that characterize the localized coronal distribution, but it is found that large-scale emission features have corresponding polarization signatures. Since the measured linear polarization vectors describe the projected magnetic field direction, as shown theoretically, it follows that the form of the large-scale coronal distribution describes corresponding magnetic field structures. Measured polarization values are consistent with those predicted theoretically. Interpretation of these data to obtain corresponding magnetic field directions suggests that the value usually accepted for iron abundance in the corona might be too large.The National Center for Atmospheric Research is sponsored by the National Science Foundation.Operated by the Association of Universities for Research in Astronomy, Inc. under contract AST 78-17292 with the National Science Foundation. 相似文献
463.
Michel Dagbert Raymond Pertsowsky Michel David Guy Perrault 《Geochimica et cosmochimica acta》1975,39(11):1499-1504
An attempt is made to describe global variations in the geochemistry of major and minor elements within a population of nepheline syenite samples defined by mineralogical criteria.Using correspondence analysis, a new pattern recognition procedure, it is possible to define a few trends of common behaviour which reflect most of the initial dispersion.As Al and Na participate in the scattering along the two main trends, agpaicity is recorded by them. However, the traditional form of the coefficient which measures it is proved to be unsatisfactory as variations of K are not significant. 相似文献
464.
The purpose of this study is to investigate the effects of salt marsh geomorphology on the distribution of surface metal content. Surface sediment samples (46) were taken along two transects across an intertidal salt marsh island. Abundance of Ca, Al, Fe, Ni, Cr, Cu, Zn, Rb, Sr, As, and Zr vary up to 300?% with statistically significant differences along transects and between transects. Along transect, metal abundances are strongly influenced by elevation and distance from the subtidal channel. Between transects, salt marsh morphodynamics, relative marsh age, and water sources seem to affect metal distribution. These observations lead us to hypothesize that at least three scales of variability can be expected for assessing salt marsh sediment metal distributions. Larger-scale variations associated with salt marsh sediment sources and age, and another related to local salt marsh geomorphic structure. Therefore, studies that characterize salt marsh metal loading should explicitly consider the variability imposed over a range of spatial scales. 相似文献
465.
An Attempt to Close the Daytime Surface Energy Balance Using Spatially-Averaged Flux Measurements 总被引:1,自引:0,他引:1
Matthias Mauder Raymond L. Desjardins Elizabeth Pattey Devon Worth 《Boundary-Layer Meteorology》2010,136(2):175-191
Single-tower eddy-covariance measurements represent the complete surface flux of a scalar only under idealized conditions.
Therefore, we often find an underestimation of energy fluxes expressed as a lack of energy balance closure at many sites.
In this study, a multi-tower approach to measure atmospheric energy fluxes based on spatial averaging is evaluated and possible
mechanisms causing a lack of energy balance closure are analysed, focussing on daytime data only. It is shown that the multi-tower
technique is also unable to measure the entire flux for our site, likely because the assumption of horizontal homogeneity
is violated. Heterogeneity-induced and buoyancy-driven quasi-stationary circulations are probably the dominant processes causing
the underestimation of energy fluxes. A dependence of the energy balance residual on stability is found, with residuals close
to zero for stable stratification, a maximum under unstable to near-neutral conditions and still relatively large residuals
for stronger instability. Assuming the processes transporting energy and CO2 are similar, the implications on long-term CO2 flux measurements are analysed. Accordingly, the resulting selective systematic error of cumulative net ecosystem exchange
estimates for agricultural regions such as ours can be of the order of more than 100%, since mainly the fluxes during periods
of net CO2 uptake are underestimated while periods of net CO2 release are much less affected by this bias. Further investigations about this issue are highly warranted. 相似文献
466.
Raymond Hide 《Pure and Applied Geophysics》1983,121(3):365-374
An outline is given of some recent and current research in the Geophysical Fluid Dynamics Laboratory of the UK Meteorological Office, on the dynamics of rotating fluids and planetary atmospheres. Many of these investigations bear on the problem of creating a theoretical framework for atmospheric predictability studies. 相似文献
467.
468.
469.
Fayalite, hypersthene, basalt, and obsidian were dissolved in buffered solutions (25°C; pH 4.5 and 5.5) under air, N2 or O2 atmospheres, in order to follow the kinetics of dissolution. Each dissolved more rapidly at lower pH values, dissolving most rapidly in the initial few days, followed by slower dissolution for periods up to six months. Dissolution was more rapid when air was excluded. In oxygen atmospheres an Fe(OH)3 precipitate armors mineral surfaces, thus inhibiting further dissolution, and further affects the solution by scavenging dissolved silica and cations. Dissolution reactions include initial exchange between cations and H+, incongruent dissolution of silicate structures, oxidation of Fe2+ in solution, precipitation of Fe(OH)3, and scavenging of dissolved silica and cations by Fe(OH)3. Dissolution kinetics may explain weathering of mafic rocks and minerals at the Earth's surface, the formation of Fe-oxide coatings on mineral grains, weathering of submarine mafic rocks and intrastratal solution of mafic minerals in buried sandstones. Early Precambrian weathering would have been more rapid before the appearance of large amounts of oxygen in the atmosphere, and continental denudation rates may have been higher than at present because of this effect and the predominance of mafic igneous rocks at an early stage of continent formation and growth. 相似文献