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11.
Yugo Nakamura Yoshinori Katayama Kazuomi Hirakawa 《Journal of Volcanology and Geothermal Research》2002,114(3-4)
Refractive indices of incompletely hydrated tephra glasses vary widely. Thus, glass refractive index is not a practical indicator for identifying Holocene tephras. Hydration near the surface of tephra glass shards can be removed by either hydrofluoric acid treatment or annealing for 12 h at 400°C. The annealing procedure is a particularly reliable and simple way to dehydrate tephra glasses. Standard deviations (s) of refractive indices for glasses after 12 h annealing are small (s=0.0014–0.0018), in contrast with untreated glasses (s=0.0034–0.0405). The refractive indices of dehydrated tephra glasses are 0.006–0.014 lower than those of the untreated (hydrated) glasses. Using the 400°C 12-h annealing procedure, values for the refractive indices of eight Holocene tephras in Hokkaido were obtained. These refractive indices are useful indicators for identification and correlation of Holocene tephras. 相似文献
12.
Formation elements logging is a neutron gamma spectroscopy logging technique used to acquire the content of elements and minerals by recording the gamma ray produced by the reaction of neutron and elemental nucleus in the formation. It has a wide usage in discriminating complex lithology and evaluating unconventional reservoir. The Monte Carlo simulation model of formation elements logging tool is established in this paper, with which the effects of tool parameters including the material and length of the scintillation crystal and source spacing on logging responses are modeled. The results show that the energy response of LaBr_3: Ce crystal is better than others, and the detection efficiency increases with the crystal length but decrease with source spacing. The above results may be used as a reference for optimizing the tool structure design. 相似文献
13.
Having in mind the potential impact of the results presented by Veprev and Muromtsev (2012) [13] on our knowledge of the universe, we reinvestigated the liquid scintillation measurement of the count rate variations of 3H. Making use of the sophisticated Quantulus liquid scintillation spectrometer, we found that the measurement of the high-energy tail of 3H spectrum may be significantly influenced by instrumental instability. Thus, the possible explanation for the relatively high count rate variations of Veprev and Muromtsev (2012) [13] can be attributed mainly to the walk of the cut-off in the integrated spectrum, although weak variations of different origin could be masked by such cut-off drifts. In our experiment we have also registered the oscillatory behavior of measured high-energy tail of 3H spectrum, but with very small amplitude (less than 0.5%), which cannot be easily explained only by instrumental instability. When the total 3H spectrum was measured, no significant variations in the count rate were found. 相似文献
14.
The propagation features of extremely low frequency electromagnetic waves through the multicomponent ionospheric plasma are studied. It is shown that at relatively lower frequencies refractive index for right hand mode is higher than the left-hand mode, which is reversed at higher frequencies. The thermal temperature of plasma particle causes decrease in phase and group velocities of both right and left-hand modes. The crossover frequencies for different plasma models are computed and variation with ion concentration and thermal velocity is studied. Explicit expression for group velocity and travel time has been derived and studied numerically. Finally, we have presented simulation of the ion whistler spectrograms for Hydrogen, Helium and Oxygen ions present in the ionospheric plasma. The results are compared with the experimentally detected hydrogen and helium ion whistlers. The importance of the present study in the exploration of ionospheric plasma is illustrated. 相似文献
15.
R. Hanbury Brown 《Journal of Astrophysics and Astronomy》1984,5(1):19-30
The Chatterton Astronomy Department aims to apply interferometers with very high resolving power to optical astronomy. The
programme of the stellar intensity interferometer at Narrabri Observatory was completed in 1972 and since then the work has
been directed towards building a more sensitive instrument with higher resolving power. As a first step a much larger intensity
interferometer was designed but was not built because it was large, expensive and not as sensitive as desired. Efforts are
now being made to design a more sensitive and cheaper instrument. A version of Michelson’s stellar interferometer is being
built using modern techniques. It is hoped that it will reach stars of magnitude +8 and will work reliably in the presence
of atmospheric scintillation. It is expected to cost considerably less than an intensity interferometer of comparable performance.
The pilot model of this new instrument is almost complete and should be ready for test in 1984.
Text of an Academy Lecture delivered at the Raman Research Institute, Bangalore on January 27, 1984. 相似文献
16.
Didier Miallier Serge Sanzelle Thierry Pilleyre Gérard Vernet Sarah Brugière Tohru Danhara 《Comptes Rendus Geoscience》2004,336(1):1-8
A trachytic tephra, discovered in the ancient lake of Sarliève, ‘Grande Limagne’, has been dated using the thermoluminescence technique. The obtained age, 16±4 ka (), is older than that of the trachytic volcanoes of the Cha??ne des Puys, the ashes of which have already been locally recognised in the region. Its analysis confirms its originality. In the course of the comparisons made to search for its spring, it appears that the wide-dispersion tephra CF7, beforehand correlated by hypothesis to the Puy de Clierzou, probably originates from the Kilian crater or the Puy de Vasset. To cite this article: D. Miallier et al., C. R. Geoscience 336 (2004). 相似文献
17.
2013年中国发射了首颗进行全球导航卫星系统(global navigation satellite system,GNSS)掩星观测的气象卫星风云3号C星(Fengyun-3C,FY-3C),且已发布自2014年6月以来的FY-3C掩星大气产品,但目前还未见将其应用于大气边界层的相关研究.首次尝试利用FY-3C折射率... 相似文献
18.
本文用比较严格的理论讨论了由连续介质和散射薄屏组成的星际介质对河外射电源的折射闪烁.对折射闪烁引起的流量变化的结构函数D(τ)(τ为迟后时间)的计算表明,结构函数的幂律部份的指数P(D(τ)(∝τP)依赖于上述两个成份的相对散射强度,即在连续介质散射为主的情况下;而在薄屏散射为主的情况下;若两个成份的散射可相比较时,1<P<2.因此本模型可以用于解释在河外射电源和脉冲星中观测到的折射闪烁的结构函数具有不同幂指数的情形,特别是P~1.5的情形. 相似文献
19.
20.
A. Gelencsér A. Hoffer G. Kiss E. Tombácz R. Kurdi L. Bencze 《Journal of Atmospheric Chemistry》2003,45(1):25-33
Current climate models seem to underestimate the flux of solar energy absorbed by the global troposphere. All of these models are constrained with the assumption that cloud droplets consist of pure water. Here we demonstrate in a simple laboratory experiment that aromatic hydroxy-acids which are found in continental fine aerosol can react with hydroxyl radicals under typical conditions prevalent in cloud water influenced by biomass burning. The reactions yield colored organic species which do absorb solar radiation. We also suggest that the products of such reactions may be humic-like substances whose presence in continental aerosol has been confirmed but their source mechanisms are still much sought after. We also attempt to give a first order estimate of the enhancement of water absorption at a visible wavelength under atmospheric conditions. 相似文献