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复杂构造地震成像主要取决于叠前地震数据品质、偏移速度可靠性和偏移算子成像精度. 库车坳陷异常复杂的近地表条件导致极低信噪比的地震采集数据. 该区逆冲推覆高陡构造刺穿盐体大面积分布, 盐层厚度变化大、顶底面形态复杂, 盐下断裂带破碎、小断块发育, 形成异常复杂的地震成像问题. 本文重点研究三个关键环节:(1)精细的叠前地震预处理研究: 根据该区地震地质复杂性和地震资料特征, 采用一些新的方法技术和技术组合从振幅与时移的大、中、小尺度变化三个层次来解决资料信噪比问题, 重建深部反射信号; (2)三级偏移速度分析研究:利用库车坳陷盐刺穿逆冲推覆构造建模理论及变速成图配套技术解决叠前时间偏移速度场时深转换问题,利用井约束低频速度地震迭代反演技术解决连井层速度场与偏移速度场的融合问题,实现从DMO速度分析、叠前时间偏移速度分析到叠前深度偏移速度分析的有机衔接,建立拓扑结构相对保持的叠前深度偏移速度模型;(3)基于退化Fourier偏移算子的半解析波动方程叠前时间和深度偏移研究, 极大地改善了地震偏移过程中高波数波的成像问题. 通过对库车坳陷大北、博孜、却勒、西秋4和西秋10等复杂高陡构造的叠前时间和深度偏移地震成像处理,取得了较好的应用效果. 相似文献
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1 INTRODUCTIONThe broad emission lines, the most important characteristics of active galactic nuclei (AGN),are generally believed to be emitted by photoionized gas in the clouds that are illuminated bythe UV to X-ray continuum radiation of the celltral source (Netzer 1990). The photoionizationmodel is quite successful in explaining the average emission line properties of AGNs using anaverage ionizing continuum. To date, there are two sets of statistical relationships between thecolltin… 相似文献
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系统介绍多通道海洋激光雷达溢油监测系统的硬件结构和高台实验,探讨多通道激光雷达探测溢油的可行性;此系统采用355 nm波长的3倍频Nd:YAG激光作为激发源,利用125 m高的实验平台,在白天和夜晚2种环境下进行实验,获得多种目标的雷达信号,并提取不同目标的特征荧光光谱,分析结果与实际情况相符。实验证明多通道海洋激光雷达溢油监测系统性能可靠,可以有效地进行溢油探测。 相似文献
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Xue-Guang Zhang Ting-Gui Wang You-Jun LuCenter for Astrophysics and Department of Astronomy Applied Physics University of Science Technology of China Hefei zxg@mail.ustc.edu.cn 《中国天文和天体物理学报》2003,3(3):212-224
The question whether the radio properties of quasars are related to the mass of the central black hole or the accretion rate is important for our understanding of the formation of relativistic jets, but no consensus has been reached from statistical analyses. Using two large quasar samples, one radio-selected, one optical-selected, we re-exarnined these relations and find that previous differences between radio- and optical- selected samples can be ascribed, at least partly, to the effect of the narrow line component. All previous claimed correlations are much weaker, if exist at all. 相似文献
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A number of observations suggest that He II in the intergalactic medium(IGM) was fully ionized at z ～ 3, probably by quasi-stellar objects(QSOs). Here we construct a simple model of a QSO to study the reionization of He II and the corresponding thermal evolution of the IGM. We assume that QSOs are triggered by major mergers of dark matter halos, and the luminosity evolution of individual QSOs is described by an initial accretion stage with a constant Eddington ratio and then a powerlaw decay driven by long term disk evolution or fueling. Once a QSO is triggered, it immediately ionizes its surrounding area as an ionized bubble. The resulting changes in size and volume of the bubble are determined by the luminosity evolution of the central QSO. With the emergence of more and more bubbles, they eventually overlap each other and finally permeate the whole universe. During the He II reionization,the IGM temperature increases due to the photoheating by the ionization processes.Applying the bubble model and considering various heating and cooling mechanisms,we trace the thermal evolution of the IGM and obtain the average IGM temperature as a function of redshift, which is very consistent with observations. The increase in IGM temperature due to the reionization of He II may be determined more accurately in the future, which may put robust constraints on the QSO model and the physics of He II reionization. 相似文献
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大菱鲆幼鱼蛋白质消化特征及其对水环境的影响 总被引：2，自引：0，他引：2
采用单因素随机区组设计,选择平均初重34.5±5.5g的大菱鲆幼鱼225尾,平均分为5组(A~E),每组3重复。分别饲喂蛋白质水平45%,48%,50%,52%和54%的5种膨化颗粒饲料,研究大菱鲆幼鱼的蛋白质消化特征及其对水环境的影响。结果表明:随着饲料蛋白质水平的提高,幼鱼的生长性能提高,饲料系数相应降低;蛋白质消化率先升后降,在50%蛋白组取得最大;蛋白质摄入量、消化量以及粪氮排出量明显增加;养殖水环境中氨氮和亚硝氮的浓度也不断提高。特别是在50%蛋白质水平以上时,幼鱼生长性能提高幅度缓慢,而粪氮排出量和水环境中氨氮含量显著提高(p<0.05)。试验表明,大菱鲆幼鱼环保饲料中蛋白质的适宜水平为50%。 相似文献
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