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901.
Eighty ferromanganese nodules from a wide variety of marine and fresh-water environments have been analyzed by electron spin resonance spectroscopy. The purpose has been to gain information on the forms in which the major constituents of manganese nodules are present. Contributions to ESR spectra of the nodules come mainly from Mn2+ and Fe3+. Deep-sea samples generally showed only broad resonance lines, and those with larger peaks close to g = 2.0 are believed to contain more Mn2+ than others. Some Antarctic and fresh-water nodules lack a strong Mn2+ resonance and have a peak around g = 4.0 which is most likely tetrahedral Fe3+. A number of smaller peaks in several samples could not be readily interpreted in terms of contributions from individual ionic species because of fundamental problems in preparing standards having the ion of interest in the same micro-environment as it experiences in the nodules. 相似文献
902.
One very specific operational requirement of the Tropical Cyclone (TC) Programme of the Regional Specialized Meteorological
Centre, New Delhi is to provide 12-hourly forecasts valid up to 48 h (preferably 72 h) on the intensity of cyclones over the
southern Indian Seas. In this paper, a simple empirical model for predicting the intensity of TCs occurring in the Bay of
Bengal is proposed. The model parameter has been determined from a database assembled on 30 recent cyclones, and the model
itself is based on the assumption that a TC intensifies exponentially. A method for correcting the forecast during subsequent
observation hours (6- or 12-h intervals) is also presented. The results show that the forecast skill for forecasts of up to
48 h is reasonably good. The absolute mean errors are less than 12 knots for 48-h forecasts, with the forecast skill decreasing
with time. With the incorporation of a correction procedure based on the latest observations, some improvement in the forecast
skill can be obtained. The model is expected to be useful to operational forecasters. 相似文献
903.
Morphology and environment of cold-water coral carbonate mounds on the NW European margin 总被引:6,自引:0,他引:6
A. J. Wheeler A. Beyer A. Freiwald H. de Haas V. A. I. Huvenne M. Kozachenko K. Olu-Le Roy J. Opderbecke 《International Journal of Earth Sciences》2007,96(1):37-56
Cold-water coral carbonate mounds, owing their presence mainly to the framework building coral Lophelia pertusa and the activity of associated organisms, are common along the European margin with their spatial distribution allowing them
to be divided into a number of mound provinces. Variation in mound attributes are explored via a series of case studies on
mound provinces that have been the most intensely investigated: Belgica, Hovland, Pelagia, Logachev and Norwegian Mounds.
Morphological variation between mound provinces is discussed under the premise that mound morphology is an expression of the
environmental conditions under which mounds are initiated and grow. Cold-water coral carbonate mounds can be divided into
those exhibiting “inherited” morphologies (where mound morphology reflects the morphology of the colonised features) and “developed”
morphology (where the mounds assume their own gross morphology mainly reflecting dominant hydrodynamic controls). Finer-scale,
surface morphological features mainly reflecting biological growth forms are also discussed. 相似文献
904.
Salah S. Abdalmogith Roy M. Harrison Zahari Zlatev 《Journal of Atmospheric Chemistry》2006,54(1):43-66
Nitrate and sulphate concentrations were measured over the period January 2002–December 2003 on daily basis at two stations in the UK: a rural site (Harwell) and an urban site (Belfast). The measurements were compared with model results obtained by using the Unified Danish Eulerian Model (UNI-DEM), which was run using both a coarse resolution grid (50 km × 50 km surface cells) and a fine resolution grid (10 km × 10 km surface cells). The results from the comparison show reasonably good agreement between concentrations measured at the two stations and calculated by the model. This is achieved despite the absence of aqueous phase sulphur oxidation chemistry in the model. The model results were also used to predict the spatial distributions of nitrate and sulphate concentrations in the UK which agree well with observations. The contribution of mainland European emission sources and that of UK sources to pollution levels in the UK was estimated. The relative proportions differ substantially across the UK with the imported contribution to UK sulphate and nitrate typically in the range 20–45% and 35–65% respectively. 相似文献
905.
Mark A. Pegg Clay L. Pierce Anindya Roy 《Aquatic Sciences - Research Across Boundaries》2003,65(1):63-72
Human alteration of large rivers is commonplace, often resulting in significant changes in flow characteristics. We used a time series approach to examine daily mean flow data from locations throughout the mainstem Missouri River. Data from a pre-alteration period (1925-1948) were compared with a post-alteration period (1967-1996), with separate analyses conducted using either data from the entire year or restricted to the spring fish spawning period (1 April-30 June). Daily mean flows were significantly higher during the post-alteration period at all locations. Flow variability was markedly reduced during the post-alteration period as a probable result of flow regulation and climatological shifts. Daily mean flow during the spring fish spawning period was significantly lower during the post-alteration period at the most highly altered locations in the middle portion of the river, but unchanged at the least altered locations in the upper and lower port ions of the river. Our data also corroborate other analyses, using alternate statistical approaches, that suggest similar changes to the Missouri River system. Our results suggest human alterations on the Missouri River, particularly in the middle portion most strongly affected by impoundments and channelization, have resulted in changes to the natural flow regime. 相似文献
906.
Roger F. Reinking A. Shelby Frisch Brad W. Orr David L. Korn Luc R. Bissonnette Gilles Roy 《Boundary-Layer Meteorology》2003,109(3):255-284
Trapped Kelvin–Helmholtz (K–H) waves and vortices were monitored as they were generated immediately upwind of a mountain and driven into the barrier by a low-level jet. A stratus cloud visually revealed the embedded, propagating, gravity-shear waves. Interactions of the waves with the mountain were deciphered using remote sensing measurements of the structure, motions, and microphysics within the cloud and conceptual models based on existing theories. The observations show that the mountain acted as a dam to the flow that was primed for, but did not spontaneously induce, the waves. In response to the blocking, the waves spatially developed a pattern of formation, amplification, and breakdown between the upstream flow and the barrier, and altered the associated clouds in the process. Notably, radar signatures of velocity variance depicted organized, intertwined ribbons of relatively large vorticity within the wave layer. These provided measured evidence of the vortex sheet and streamwise vortex tubes predicted by advanced K–Hinstability theory, the three-dimensional version of Scorer's `stripe', the layer of rotational fluid between opposed flows that led to the wave generation. A theory of resonant interaction of wave trains, but with blocking imposed, appears to explain the internal structure of the pile-up of the flow and wave amplification approaching the barrier. Evolution of the supporting atmospheric thermal structure and introduction of a boundary-layer flow reversal follow a current model of blocking, although some features may have developed more directly from wave-driven mixing. The remote sensors also measured the influence of the waves on the cloud liquid water, including a cumulative enlargement of droplets as they were carried through a series of waves. 相似文献
907.
S. K. Roy Bhowmik 《Journal of Earth System Science》2003,112(4):499-519
At the India Meteorological Department (IMD), New Delhi, a 12-level limited area model with 100 km horizontal resolution has
been in use for weather forecasting. The present study uses this model together with a higher horizontal resolution (50 km)
and vertical resolution (16-levels) model to examine the impact of increased resolution to simulate mesoscale features of
rainfall during monsoon disturbances. The model was run for 22 days in the month of August 1997 and one week in September
1997 during three monsoon depressions and one cyclonic storm in the Bay of Bengal. The model results are compared with observations.
The study shows that the model can capture mesoscale convective organization associated with monsoon depression. 相似文献
908.
Motion of the Scotia Sea plates 总被引:2,自引:0,他引:2
909.
A. L. Roy R. P. Norris M. J. Kesteven E. R. Troup & J. E. Reynolds 《Monthly notices of the Royal Astronomical Society》1998,301(4):1019-1030
We have observed a sample of 149 Seyfert galaxies and radio-quiet quasars at 13 cm with both a 275-km radio interferometer and the 6-km compact array of the Australia Telescope. The high-resolution observations searched for the presence of compact, high-brightness-temperature radio emission from the active nucleus. The low-resolution observations measured the total radio emission from the galaxy disc and Seyfert core and lobes. From these we draw the following conclusions. (i) Seyfert galaxies that lack compact radio cores display a correlation between radio and far-infrared (FIR) emission similar to the correlation displayed by normal spirals, albeit with greater scatter. The correlation is found to be intrinsic and is not an artefact of the richness effect. (ii) A very different radio–FIR correlation is displayed by those Seyferts that harbour compact radio cores. These tend to be more radio-loud than either normal spirals or the Seyferts that lack compact cores. The compact core emission thus seems to be responsible for the generally poor radio–FIR correlation displayed by Seyfert galaxies. (iii) The radio–FIR correlation is not significantly improved by subtracting off the 0.1-arcsec (20- to 200-pc) compact radio emission from the total radio emission. This suggests that the emission from the active galactic nucleus has significant structure on scales larger than 0.1 arcsec. Perhaps these structures are the 'linear' radio features that have been seen previously in Seyfert nuclei. 相似文献
910.
Pijush Pal Roy 《Geotechnical and Geological Engineering》1998,16(2):151-166
The author considers the structural response of various types of surface structures along with their resonance characteristics as well as magnification and attenuation problems. Experimental data from 20 different mines in India, are compiled and analysed to develop simple general equations for use in field conditions. Interpretation of low frequency waves and their active role in enhancing damage probability of structures is also discussed. Particular situations are examined where low and high dominant band frequencies could obtain. It is suggested that a response analysis be undertaken before establishing damage threshold values of any type of structure. © Rapid Science Ltd. 1998 相似文献