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171.
172.
Soil moisture dynamics under different land uses on karst hillslope in northwest Guangxi,China 总被引:5,自引:1,他引:5
Temporal and spatial dynamics of soil moisture are little known on karst hillslope with shallow soil in subtropical region.
The objectives of this paper were (1) to investigate the temporal dynamics of soil moisture at depth of 0–10 cm under different
land uses; and (2) to understand the relationship between mean and coefficient of variation (CV) of moisture contents on karst
hillslope in northwest Guangxi, China. Soil moisture contents had a moderate variation (CV 17.5–30.3%) over an 8-month period
and they had a significant difference among different land uses at the 0.01 level with a decreasing order: native scrubland > abandoned
cropland and sloping cropland > economic forestland. There were higher mean and lower CV of moisture contents in rainy season
than those in drought season. Mean and CV of moisture contents had a significant negative linear relationship except in abandoned
cropland with higher soil and vegetation heterogeneity. This suggested that spatial variability of soil moisture within sampling
sites would decrease when soils were wet and increase when soils were arid. Compared with rainy season, more soil samples
may be needed and the interval for sampling should be shortened in drought season. Such information provided some insights
to better understand the dynamics and variability of soil moisture at a larger scale in karst region of southwest China. 相似文献
173.
Alaska is considered to be tectonically comprised of five elongate blocks separated by transcurrent faults formed prior to rotation which enter the state from the southeast and continue westward to the edge of the Bering Sea continental shelf. We propose an additional, inactive fault, indicated by gravity and magnetic data and other observations, to extend between the Bering Strait and the Arctic Ocean continental shelf east of the Northwind escarpment, separating northern Alaska from northeast Siberia. Near the center of the state the faults are bent, concave to the south, about the north-south axis of the so-called Alaska orocline. In our reconstruction the blocks have rotated from a position whereby the north slope was adjacent to Banks Island of the Canadian basin. During the rotation the northernmost, or Brooks block, was squeezed, up to 15% in the western end, to its present width. After rotation, when the three southern blocks were in their present position, the Brooks block and the next block to the south were pushed eastward by North America moving against Siberia, forming the bend in the British-Richardson-Ogilvie Mountains we call the Ogilvie orocline. 相似文献
174.
W.J. Trahar 《International Journal of Mineral Processing》1981,8(4):289-327
From the examination of data from detailed plant surveys and associated laboratory batch testing, the principal effects of particle size in flotation have been identified. The current state of knowledge concerning the role of this variable is discussed in terms of the evidence presented. It is concluded that the minimum degree of hydrophobicity necessary for the flotation of a particle depends upon its size and as a result, recovery-size curves are a valuable diagnostic aid to the assessment of flotation performance. Entrainment is shown to be an important contributory mechanism to the recovery of fine particles which, when coupled with a low rate of genuine flotation, can account for much of the observed behaviour of such fines. The significance of particle size and its consequences in flotation research, in plant operations and in control schemes has been under-rated. The separate conditioning or flotation or both of separate size fractions seems inevitable as ores become increasingly difficult to concentrate. 相似文献
175.
In coastal areas, abnormally high pressure may be caused by the tide-induced water table variation under extensive pavements,
particularly during rainfall. To simulate the rainfall infiltration effects on the air permeability of asphalt pavements in
coastal area, column-shaped asphalt sample was fixed in the upper part of a steel cylinder with its upper surface saturated
with ponding water (depth < 5 mm) and open to the atmosphere. The cylinder’s lower part formed an air chamber. The chamber
was pressurized and then the air therein was released naturally through the sample. The pressure variation with time in the
chamber was recorded for analysis. Based on the Green–Ampt piston model for the surface water infiltration, an approximate
analytical solution was derived to describe the pressure–time relationship in the chamber. A new parameter called the escape
pressure was introduced to describe the air pressure needed for the chamber air to break through the capillary pressure induced
by the ponding water. The analytical solution gave good estimations of both the escape pressures and the harmonic averages
of the permeabilities of the wet and dry parts of 14 samples in the sense that excellent fittings were obtained between the
observed and predicted air pressures in the air chamber. The estimated escape pressure ranges from 0.0 to 1.74 kPa. The harmonic
average of the permeabilities of the wet and dry parts is 5–94% of the dry sample’s permeability. 相似文献
176.
Aleido J. van Bennekom Sjierk J. van der Gaast 《Geochimica et cosmochimica acta》1976,40(10):1149-1152
Comparison of X-ray diffraction spectra of marine diatom frustules and suspended clay minerals suggests the presence of a distinctive smectite in diatoms. The frustules contained 1.5% Al2O3 and were partly covered with particles of 0.02 μm in diameter. The source of Al and the fate of diatoms in the sediment are briefly discussed. 相似文献
177.
An experimental study was undertaken to determine how the spectral and photometric properties of representative Martian areas are affected by fallout of atmospheric dust suspended during dust forms. A laboratory apparatus was used to simulate the uniform fallout and deposition of particles 1 to 5 μm in diameter. Spectral measurements from 0.4- to 1.2-μm wavelengths and photometric measurements at several wavelengths were made for a number of Mars-analog materials before and after deposition of 6 × 10?5 to 1.5 × 10?3 g/cm2 of simulated fallout. These results indicate that the spectral and photometric properties of Martian regions can be affected significantly even by minute amounts of fallout. For instance, the reflectance at 0.56 μm of an average dark area will increase by 35% after deposition of only 9 × 10?5 g/cm2, and by 70% after deposition of 1.5 × 10?4 g/cm2. Thus the fallout from even one dust storm season (~2 × 10?3 g/cm2) is sufficient to change significantly the spectral and photometric characteristics of the substrate material, if the fallout were ubiquitous over the surface and if no competing processes of dust removal from surface grains occured. 相似文献
178.
An important challenge in theoretical ecology is to find good coarse-grained representations of complex food webs. Here, we
use the approach of generalized modeling to show that it may be possible to formulate a coarse-graining algorithm that conserves
the local dynamics of the model exactly. We show examples of food webs with a different number of species that have exactly
identical local bifurcation diagrams. Based on these observations, we formulate a conjecture governing which populations of
complex food webs can be grouped together into a single variable without changing the local dynamics. As an illustration,
we use this conjecture to show that chaotic regions generically exist in the parameter space of a class of food webs with
more than three trophic levels. While our conjecture is at present only applicable to relatively special cases, we believe
that its applicability could be greatly extended if a more sophisticated mapping of parameters were used in the model reduction. 相似文献
179.
Yang Liu Alfred T. Anderson Colin J. N. Wilson Andrew M. Davis Ian M. Steele 《Contributions to Mineralogy and Petrology》2006,151(1):71-87
Large pyroclastic rhyolites are snapshots of evolving magma bodies, and preserved in their eruptive pyroclasts is a record
of evolution up to the time of eruption. Here we focus on the conditions and processes in the Oruanui magma that erupted at
26.5 ka from Taupo Volcano, New Zealand. The 530 km3 (void-free) of material erupted in the Oruanui event is comparable in size to the Bishop Tuff in California, but differs
in that rhyolitic pumice and glass compositions, although variable, did not change systematically with eruption order. We
measured the concentrations of H2O, CO2 and major and trace elements in zoned phenocrysts and melt inclusions from individual pumice clasts covering the range from
early to late erupted units. We also used cathodoluminescence imaging to infer growth histories of quartz phenocrysts. For
quartz-hosted inclusions, we studied both fully enclosed melt inclusions and reentrants (connecting to host melt through a
small opening). The textures and compositions of inclusions and phenocrysts reflect complex pre-eruptive processes of incomplete
assimilation/partial melting, crystallization differentiation, magma mixing and gas saturation. ‘Restitic’ quartz occurs in
seven of eight pumice clasts studied. Variations in dissolved H2O and CO2 in quartz-hosted melt inclusions reflect gas saturation in the Oruanui magma and crystallization depths of ∼3.5–7 km. Based
on variations of dissolved H2O and CO2 in reentrants, the amount of exsolved gas at the beginning of eruption increased with depth, corresponding to decreasing
density with depth. Pre-eruptive mixing of magma with varying gas content implies variations in magma bulk density that would
have driven convective mixing.
Electronic Supplementary Material Supplementary material is available for this article at and is accessible for authorized users. 相似文献
180.
The genesis of Lower Eocene calcite-cemented columns, “pisoid”-covered structures and horizontal interbeds, clustered in dispersed outcrops in the Pobiti Kamani area (Varna, Bulgaria) is related to fossil processes of hydrocarbon migration. Field observations, petrography and stable isotope geochemistry of the cemented structures and associated early-diagenetic veins, revealed that varying seepage rates of a single, warm hydrocarbon-bearing fluid, probably ascending along active faults, controlled the type of structure formed and its geochemical signature. Slow seepage allowed methane to oxidize within the sediment under ambient seafloor conditions (δ18O = − 1 ± 0.5‰ V-PDB), explaining columns' depleted δ13C ratios of − 43‰. Increasing seepage rates caused methane to emanate into the water column (δ13C = − 8‰) and raised precipitation temperatures (δ18O = − 8‰). Calcite-cemented conduits formed and upward migrating fluids also affected interbed cementation. Even higher-energy fluid flow and temperatures likely controlled the formation of “pisoids”, whereby sediment was whirled up and cemented. 相似文献