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21.
The analysis of sand samples by X-ray fluorescent spectroscopy (XRF) gives the ratio of the geochemical elements to construct
the sand samples. The application of the ratio matching to sand samples represents the correlation number between two sand
samples with respect to geochemical elements. When the correlation number between two sand samples is low, the two samples
are not geochemically similar each other. This denotes that the exchange of sand between two sampling points is scarce or
the two samples are independent. When the correlation number between two sand samples is high, the two samples are geochemically
similar, signifying that the exchange of sand between two sampling points is frequent or there is sand movement between two
sampling points. If there exists prominent sand movement in the study area, the correlation number is almost 1 and kilo count
number per second of each geochemical element per weight decreases along the flow direction. The decrease is caused by the
reduction of sizes and the adherence of dirt on the surface of sand particles. Since the flow direction in rivers is usually
the same as the direction of sand movement, it can be verified. This study obtains satisfactory results applying the method
of prediction in sand movement to sediments in rivers.
Received: 17 May 1995 · Accepted: 14 August 1995 相似文献
22.
A ray tracing computer program for non-ducted whistler mode waves in a warm plasma in the magnetosphere is developed, where electron temperature effects are taken into account. The refractive index is calculated from the warm-plasma approximation and is used in the ray tracing after its accuracy has been checked by comparison with the hot-plasma solution without approximation. The ray paths do not depend appreciably on electron temperature. However, there are regions where the waves are heavily damped by Landau damping. By paying attention to this damping region, the electron temperature can be estimated from a satellite observation of the Doppler shift and damping of a ground-based VLF signal. 相似文献
23.
Mikio Shimizu 《Astrophysics and Space Science》1979,62(2):509-513
Carbon suboxide (C3O2) polymers formed in the primitive atmosphere would have produced an organic compound soup of high concentration on the Earth. Various vestiges of C3O2 are found in the present genetic scheme, which might suggest that the living system had formed from the polymer soup. 相似文献
24.
Masaru Nakano Hiroyuki Kumagai Bernard A. Chouet 《Journal of Volcanology and Geothermal Research》2003,122(3-4):149-164
We investigate the source mechanism of long-period (LP) events observed at Kusatsu–Shirane Volcano, Japan, based on waveform inversions of their effective excitation functions. The effective excitation function, which represents the apparent excitation observed at individual receivers, is estimated by applying an autoregressive filter to the LP waveform. Assuming a point source, we apply this method to seven LP events the waveforms of which are characterized by simple decaying and nearly monochromatic oscillations with frequency in the range 1–3 Hz. The results of the waveform inversions show dominant volumetric change components accompanied by single force components, common to all the events analyzed, and suggesting a repeated activation of a sub-horizontal crack located 300 m beneath the summit crater lakes. Based on these results, we propose a model of the source process of LP seismicity, in which a gradual buildup of steam pressure in a hydrothermal crack in response to magmatic heat causes repeated discharges of steam from the crack. The rapid discharge of fluid causes the collapse of the fluid-filled crack and excites acoustic oscillations of the crack, which produce the characteristic waveforms observed in the LP events. The presence of a single force synchronous with the collapse of the crack is interpreted as the release of gravitational energy that occurs as the slug of steam ejected from the crack ascends toward the surface and is replaced by cooler water flowing downward in a fluid-filled conduit linking the crack and the base of the crater lake. 相似文献
25.
Large-Eddy Simulation Of Radiation Fog 总被引:1,自引:0,他引:1
Mikio Nakanishi 《Boundary-Layer Meteorology》2000,94(3):461-493
In order to study the three-dimensional structure of radiation fogand to obtain a basic understanding of its generation mechanism,a numerical experiment is performed with a large-eddysimulation model and compared with the observation at Cabauw in the Netherlands. After confirming that the results are insatisfactory agreement with the observations, the structure of thefog and its generation mechanism are examined in more detail.Before the fog forms, the atmosphere is stable and an inversionlayer exists almost adjacent to the ground surface. As the fog grows, however, the stratification is destabilized and a mixed layerdevelops gradually. The longwave radiative cooling near thefog top contributes to the destabilization more than thecondensational heating does.The evolution of the fog can be classified into three stagesaccording to the behaviour of turbulent kinetic energy (TKE):formation, development, and dissipation stages.The fog layer has different flow structures at each stage.During the formation stage, longitudinal rolls similar tostreaks in channel flows appear near the ground surface.The development stage is characterized by an initiation oftransverse bands due to Kelvin–Helmholtz instability anda sudden increase of TKE. During the dissipation stage, longitudinalrolls and polygonal cells due to convective instability are organized. 相似文献
26.
多数大地震都是沿大洋板块向大陆板块俯冲的海沟发生.现在已经清楚矩震级Mw达到9级的巨大地震只发生在几个地区,包括智利、阿拉斯加、堪察加半岛和苏门答腊.日本海沟是太平洋板块向鄂霍次克海板块俯冲的地区,并没有历史记载表明这里曾发生过矩震级9级的大地震,唯一可能的例外是公元869年贞观(Jogan)大地震[1],其震级到现在... 相似文献
27.
A computational scheme for an improved Mellor–Yamada(M–Y) Level-3 model with condensation physics is proposedand its performance is examined against large-eddy-simulationdata on radiation fog. The improved M–Y model greatlycorrects several shortcomings of the original M–Y model:the underestimations of the mixed-layer depth and themagnitude of turbulent kinetic energy, and the discrepanciesin the formation and dissipation times of the fog. Inaddition the improved M–Y model can reproduce theoccurrence of Kelvin–Helmholtz instability and periodicoscillations due to its energy cycle. It is shown that theoptimization of both the closure constants and the masterlength scale is required for this improvement.The improved M–Y model has an improvement also in theLevel-2.5 version. Although the performance of theLevel-2.5 version is not so good as that of the Level-3version, the former has the advantage of relatively lowcomputational cost and is popularly used in operationalweather forecasts. Our computational scheme for theimproved M–Y model allows us to switch its hierarchylevels easily according to the purpose. 相似文献
28.
Structural changes of synthetic opal by heat treatment 总被引:1,自引:0,他引:1
Akane Arasuna Masayuki Okuno Hiroki Okudera Tomoyuki Mizukami Shoji Arai Shin’ichi Katayama Mikio Koyano Nobuaki Ito 《Physics and Chemistry of Minerals》2013,40(9):747-755
The structural changes of synthetic opal by heat treatment up to 1,400 °C were investigated using scanning electron microscopy, X-ray diffraction, and Fourier transform infrared and Raman spectroscopies. The results indicate that the dehydration and condensation of silanol in opal are very important factors in the structural evolution of heat-treated synthetic opal. Synthetic opal releases water molecules and silanols by heat treatment up to 400 °C, where the dehydration of silanol may lead to the condensation of a new Si–O–Si network comprising a four-membered ring structure of SiO4 tetrahedra, even at 400 °C. Above 600 °C, water molecules are lost and the opal surface and internal silanol molecules are completely dehydrated by heat effect, and the medium-temperature range structure of opal may begin to thermally reconstruct to six-membered rings of SiO4 tetrahedra. Above 1,000 °C, the opal structure almost approaches that of silica glass with an average structure of six-membered rings. Above 1,200 °C, the opal changes to low-cristobalite; however, minor evidence of low-tridymite stacking was evident after heat treatment at 1,400 °C. 相似文献
29.
Mikio Shimizu 《Astrophysics and Space Science》1977,51(1):241-243
The argument for the similarity of the composition of cometary volatiles to that of interstellar molecules has been strengthened by the analysis of CO+ and CO
2
+
emission of the comet West. The strong 6300 Å emission of oxygen atoms can be interpreted in terms of photodissociation of OH by the solar Lyman-alpha radiation, and not as being due to photo-dissociation of CO2 of speculatively large amount. 相似文献
30.