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91.
92.
Mineral modes have been determined for specimens of eight rocktypes from CuK X-ray powder diffraction data using the Rietveldmethod. The samples include two granites, a granodiorite, adamellite,gabbro, basalt, trachyte, and two granulite-facies metamorphicrocks. Up to eight individual mineral components have been measuredin each sample (no glassy phases were observed), with a detectionlimit of {small tilde}1 wt.%, depending on the mineral assemblage.Marked variations in grain size (i.e., granite vs. trachyte)provide no difficulties for the X-ray method. The X-ray resultscompare very favourably with (1) optical modes determined forthe mediumcoarse-grained samples by point counting, (2)normative calculations obtained using locally enhanced catanormand mesonorm software, and (3) corresponding Rietveld modesdetermined, for two samples, from neutron powder data. Wheredifferences occur, these are discussed in relation to the limitationsof each of the methods. The improved accuracy of the X-ray method is due primarily tothe incorporation of the full diffraction profile in the Rietveldanalysis calculations, and the elimination of preferred orientationby collecting the data from samples packed in glass capillaries(i.e., DebyeScherrer mode). The good agreement of theX-ray and neutron modes shows that the usual problems encounteredwith microabsorption, extinction, and sampling are of littleconcern in these rocks. The results highlight one of the majoradvantages provided by Rietveld modal analysis over the moretraditional reference intensity X-ray methods,namely, that the crystal chemistry (and thus the calibrationconstants) of the individual phases can be adjusted dynamicallyduring each individual analysis. This not only provides moreaccurate phase abundances, but also gives important supplementaryinformation about the mineralogy of the major components. 相似文献
93.
A 2D finite volume model for bebris flow and its application to events occurred in the Eastern Pyrenees 总被引:1,自引:0,他引:1
V.MEDINA A.BATEMAN M.HüRLIMANN Ph.D student Sediment Transport Research Group Department of Engineering Hydraulic Marine Environmental Engineering Technical University of Catalonia 《国际泥沙研究》2008,23(4):348-360
FLATModel is a 2D finite volume code that contains several original approaches to improve debris-flow simulation. Firstly, FLATModel incorporates a "stop-and-go" technique in each cell to allow continuous collapses and remobilizations of the debris-flow mass. Secondly, flow velocity and consequently yield stress is directly associated with the type of rheology to improve boundary accuracy. Thirdly, a simple approach for entrainment is also included in the model to analyse the effect of basal erosion of debris flows. FLATMODEL was tested at several events that occurred in the Eastern Pyrenees and simulation results indicated that the model can represent rather well the different characteristics observed in the field. 相似文献
94.
E. G. Kolomyts 《Russian Meteorology and Hydrology》2008,33(7):430-440
The gradient (ordination) analysis was used to find the tendencies and the rate of changes in discrete parameters of the cycle of forest phytomasses accompanying a growing thermoarid climatic trend. The prognostic estimates of biotic regulation of the carbon cycle by forest biogeocenoses according to the HadCM3 (version A2) climatic scenarios, describing the most powerful coming global warming, are presented. 相似文献
95.
Diurnal variation of deep cloud systems over the Indian region using INSAT-1B pixel data 总被引:1,自引:0,他引:1
Summary
Among the various time scales of deep clouds, diurnal variation is found to be prominent over the tropics. The present study
examines the diurnal variation in the number and area cover associated with the cloud systems over the tropical Indian region
using INSAT-1B pixel data. Three periods, namely, April–May 1988, July–August 1988, and January–February 1989 are considered.
The dependence of diurnal characteristics on the temperature threshold, life duration and size of cloud systems, and land-sea
contrast has been explored. The diurnal characteristics of cloud systems living for more than a day have been studied for
the first time. It is shown that cloud systems exhibit strong diurnal dependence at the coldest temperature threshold used
(201 K). Also, the diurnal variation is more for larger cloud systems and for longer living systems. In general, more deep
cloud activity is found from the satellite data during the pre-dawn and early morning hours. Precipitation is enhanced during
morning to early noon hours. Further, using data from a recent field experiment, clear evidence of diurnal variation in precipitation
over the Bay of Bengal is also presented.
Received March 20, 2000/Revised October 3, 2000 相似文献
96.
It is shown that the chronology of flare star discoveries in the Pleiades cluster and the Orion association can be described satisfactorily by various distribution functions (gamma, binomial, decreasing exponential, and delta) for the mean frequencies of stellar flares. However, it has been found that this is due to the uncertainty in the observationally derived distribution function for the mean frequency of stellar flares. The most likely function is that derived by Ambartsumian, which has a physical basis.Translated fromAstrofizika, Vol. 38, No. 1, pp. 25–32, January–March, 1995. 相似文献
97.
98.
99.
R. Ostertag G. Amthauer H. Rager H.Y. McSween 《Earth and Planetary Science Letters》1984,67(2):162-166
ALHA 77005, a shocked achondrite of the shergottite group, is unique in containing cumulus olivine crystals which display a brownish color in thin section. Mössbauer, EPR, and optical spectroscopic studies show the presence of Fe3+ in the olivine. Approximately 4.5 wt.% of the total iron in the olivine (24 wt.% as FeO) is in the trivalent state. The Fe3+ ions preferentially occupy M2 lattice positions. Charge transfer between Fe3+ and Fe2+ as well as between Fe3+ and oxygen ligands causes a broad absorption band in the optical spectrum at high energies which is the reason for the olivine color. It is concluded that the color of the ALHA 77005 olivine is preterrestrial and may be the result of shock-induced oxidation of the olivine crystals on the meteorite parent body. 相似文献
100.
Ostapchuk A. A. Kocharyan G. G. Morozova K. G. Pavlov D. V. Gridin G. A. 《Izvestiya Physics of the Solid Earth》2021,57(5):659-670
Izvestiya, Physics of the Solid Earth - Abstract—Granular media determine the dynamics of many natural systems including faults in the Earth’s crust. The paper addresses the laboratory... 相似文献