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41.
基于炮集数据的常规叠前深度偏移波场外推的计算量非常大,控制照明叠前深度偏移是基于快速的组合炮技术,通过在目的层上控制震源波场,高效实现对地质目标的高质量成像. 组合炮所需的合成算子,由在目的层定义的震源波场反向外推到地表建立. 本文提出一种更快速的地表旋转控制照明方法,直接在地表对震源波场进行面向目标的照明控制,实现目标区域高质量成像. 该方法只需对某一核合成算子进行简单的几何旋转建立合成算子函数,避免了复杂的波场外推. 这种新的控制照明方法与快速的一般组合炮偏移效率相同,但对复杂目标区域的成像能力显著增强. 应用本文方法对Marmousi模型进行计算,得到深层复杂构造非常理想的成像结果. 相似文献
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石英胶结物是砂岩中重要的胶结物类型。用纳米离子探针(CAMECA Nano SIMS 50L)对石英胶结物中Al、Ca和Mg等重要微量元素进行原位分析,可为成岩作用研究提供重要基础依据。然而,由于缺乏相应的标准物质,一直不能对石英胶结物中Al、Ca和Mg进行研究。针对不均一的石英颗粒样品,文中采用细磨、混合、高温熔融(2000℃,6个小时)与快速冷却等措施,制作均一化的石英玻璃。经纳米离子探针验证,该石英玻璃中Al、Ca和Mg在亚微米尺度上是均一的,已能满足成岩作用研究的需要。随后,用电感耦合等离子体发射光谱和激光剥蚀电感耦合等离子体质谱测定了石英玻璃中Al、Ca和Mg的含量。相对灵敏度因子分析显示,这些测试结果是协调、合理的。该均一化的石英玻璃可作为亚微米尺度Al、Ca和Mg原位分析的标准物质。 相似文献
43.
A. L.?Huber M.?Heuer K. T.?FehrEmail author K.?Bente E.?Schmidbauer G. D.?Bromiley 《Physics and Chemistry of Minerals》2004,31(2):67-79
Clinopyroxenes along the solid solution series hedenbergite (CaFeSi2O6)–petedunnite (CaZnSi2O6) were synthesized under hydrothermal conditions and different oxygen fugacities at temperatures of 700 to 1200 °C and pressures of 0.2 to 2.5 GPa. Properties were determined by means of X-ray diffraction, electron microprobe analysis and 57Fe Mössbauer spectroscopy at 298 K. Unit-cell parameters display a linear dependency with changing composition. Parameters a0 and b0 exhibit a linear decrease with increasing Zn content while the monoclinic angle increases linearly. Parameter c0 is not affected by composition and remains constant at a value of 5.248 Å. The molar volume can be described according to the equation Vmol (ccm mol–1)=33.963(16)–0.544(31)*Zn pfu. The isomer shifts of ferrous iron on the octahedral M1 site in hedenbergite are not affected by composition along the hedenbergite–petedunnite solid solution series and remain constant at an average value of 1.18 mm s–1. Quadrupole splittings of Fe2+ on the M1 are, however, strongly affected by composition, and they decrease linearly with increasing petedunnite component in hedenbergite, ranging from 2.25 mm s–1 for pure hedenbergite end member to 1.99 mm s–1 for a solid solution containing 84 mole% petedunnite. The half-widths of intermediate solid solutions vary between 0.26 and 0.33 mm s–1, indicating, in accordance with the microprobe analyses and X-ray diffraction, that samples are homogeneous and well-crystallized. The data from this study demonstrate that the crystallinity of hedenbergitic clinopyroxenes can be improved by using oxide mixtures as starting materials. Crystal sizes for intermediate compositions range up to 70 m, suitable for standard single-crystal X-ray analysis.This paper is dedicated to Prof. Dr. Georg Amthauer, Salzburg, on occasion of his 60th birthday 相似文献
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17—115℃沥青铀矿的合成及其形成速度的实验研究 总被引:1,自引:0,他引:1
本文介绍了17—115℃沥青铀矿合成的方法及对产品的鉴定结果。实验是在只有六价铀与硫代乙酰胺存在的非常简单的体系中进行的。合成的最低温度为17℃。沥青铀矿的结晶速度在不同的温度和pH条件下是不同的。温度越高,结晶速度越快。在酸性溶液中沥青铀矿结晶速度快,中性中较慢,碱性中最慢。但随着温度的提高,酸、中、碱性溶液结晶速度的差值迅速缩小。82℃时,无论酸、中、碱性溶液中的沥青铀矿均能在半小时内结晶出来。 相似文献
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《Chemie der Erde / Geochemistry》2016,76(3):449-460
Four iron-containing natural oxalates, usually classified as organic minerals, are known (humboldtine, minguzzite, stepanovite and zhemchuzhnikovite). Their occurrences and general properties are presented and briefly discussed. The subsequent part of the review is devoted to the discussion of synthetic oxalato-complexes, analogous to these natural species, including usual synthetic procedures and a thorough analysis of their crystallographic and structural peculiarities. The thermal, spectroscopic and magnetic properties of these complexes are also analyzed in detail and comparisons with other closely related complexes are also included in the discussions. 相似文献
50.
K. Golap N. Udaya Shankar S. Sachdev R. Dodson Ch. V. Sastry 《Journal of Astrophysics and Astronomy》1998,19(1-2):35-53
A new, meter-wave radio telescope has been built in the north-east of Mauritius, an island in the Indian Ocean, at a latitude
of -20.14‡. The Mauritius Radio Telescope (MRT) is a Fourier Synthesis T-shaped array, consisting of a 2048 m long East-West
arm and an 880 m long South arm. In the East-West arm 1024 fixed helices are arranged in 32 groups and in the South arm 16
trolleys, with four helices on each, which move on a rail are used. A 512-channel digital complex correlation receiver is
used to measure the visibility function. At least 60 days of observing are required for obtaining the visibilities up to 880
m spacing. The Fourier transform of the calibrated visibilities produces a map of the area of the sky under observation with
a synthesized beam width 4′ × 4.6′ sec(δ + 20.14‡) at 151.5 MHz.
The primary objective of the telescope is to produce a sky survey in the declination range –70‡ to –10‡ with a point source
sensitivity of about 200 mJy (3a level). This will be the southern sky equivalent of the Cambridge 6C survey. In this paper
we describe the telescope, discuss the array design and the calibration techniques used, and present a map made using the
telescope. 相似文献