基于反馈迭代和独立分量分析的多次波压制技术研究     

常青  徐秀刚  孙道朋 《中国海洋大学学报(自然科学版)》2018,(10)

随着海洋油气勘探的不断深入和勘探目标的日趋复杂化,如何有效的解决多次波的压制问题是目前海洋地震资料处理中的重点和难点。常规的多次波压制技术是基于输出信号能量最小准则进行匹配压制的,这一准则是基于二阶统计量实现的,不能很好的处理有效波和多次波非正交情况下的多次波压制。针对上述问题,本文将基于波动方程的反馈迭代方法与基于高阶统计量的独立分量分析法(ICA)结合起来实现自由表面多次波的压制。首先基于反馈迭代技术实现自由表面多次波的预测,然后基于高阶统计量的快速固定点寻优独立分量分析算法实现多次波和有效波的有效匹配,最终实现多次波的有效压制。资料试算结果表明,本文方法在处理非正交情况下多次波压制时,既能有效的保持有效波的能量,还能实现对于多次波,特别是中、深层多次波的良好压制。  相似文献   

Impact-generated atmospheres over Titan, Ganymede, and Callisto     

Zahnle K  Pollack JB  Grinspoon D  Dones L 《Icarus》1992,95(1):1-23

The competition between impact erosion and impact supply of volatiles to planetary atmospheres can determine whether a planet or satellite accumulates an atmosphere. In the absence of other processes (e.g., outgassing), we find either that a planetary atmosphere should be thick, or that there should be no atmosphere at all. The boundary between the two extreme cases is set by the mass and velocity distributions and intrinsic volatile content of the impactors. We apply our model specifically to Titan, Callisto, and Ganymede. The impacting population is identified with comets, either in the form of stray Uranus-Neptune planetesimals or as dislodged Kuiper belt comets. Systematically lower impact velocities on Titan allow it to retain a thick atmosphere, while Callisto and Ganymede get nothing. Titan's atmosphere may therefore be an expression of a late-accreting, volatile-rich veneer. An impact origin for Titan's atmosphere naturally accounts for the high D/H ratio it shares with Earth, the carbonaceous meteorites, and Halley. It also accounts for the general similarity of Titan's atmosphere to those of Triton and Pluto, which is otherwise puzzling in view of the radically different histories and bulk compositions of these objects.  相似文献   

Will the Russians return from the near abroad?     

Dunlop JB 《Post-Soviet geography》1994,35(4):204-215

The author "examines a range of issues surrounding the involuntary migration of Russian populations from the non-Russian republics of the former USSR. Among the questions addressed are possible magnitudes of in-migration into Russia (with special attention paid to conditions in one of the major source regions, Central Asia), attitudes in Russia regarding appropriate policy with respect to treatment of co-nationals in the near abroad and whether their return to Russia would have a positive or negative impact, and conditions in areas of Russia that presently are absorbing the greatest numbers of migrants. The assertion that Russian policy should seek aggressively to prevent the out-migration of Russian populations [from] the near abroad is assessed critically."  相似文献   

Coupled atmosphere-ocean models of Titan's past     

McKay CP  Pollack JB  Lunine JI  Courtin R 《Icarus》1993,102(1):88-98

We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time. The partial pressures of N2 and CH4 in the atmosphere are dependent on the ocean temperature and composition. We find that the resulting system is stable against a runaway greenhouse. Accounting for the decreased solar luminosity, we find that Titan's surface temperature was about 20 K colder 4 Gyr ago. Without an ocean, but only small CH4 lakes, the temperature change is 12 K. In both cases we find that the surface of Titan may have been ice covered about 3 Gyr ago. In the lakes case condensation of N2 provides the ice, whereas in the ocean case the ocean freezes. The dominant factor influencing the evolution of Titan's surface temperature is the change in the solar constant--amplified, if an ocean is present, by the temperature dependence of the solubility of N2. Accretional heating can dramatically alter the surface temperature; a surface thermal flux of 500 erg cm-2 sec-1, representative of small levels of accretional heating, results in a approximately 20 K change in surface temperatures.  相似文献   

第四系沉积地层内剪切波分裂：新马德里地震带中部的新构造含意     

Harr.  JB 徐明才 《物探化探译丛》1997,(2):26-35

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一种用于探测和修补砾石充填缺陷的独特的机械和测井系统     

Toney  JB 潘葆芝 《物探化探译丛》1991,(6):69-70

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墨西哥ZacatecasFresnillo地区SantoNino脉的银硫盐     

Gemm.  JB 陈殿芬 《国外矿床地质》1995,(1):36-53

黑西哥ＦｒｅｓｎｉｌｌｏＡｇ－Ｐｂ－Ｚｎ地区的ＳａｎｔｏＮｉｎｏ脉中，银含在螺状硫银矿及三个含银矿盐固溶体系列的矿物中，这些硫盐矿物是：浓红银矿、淡红银矿、硫锑铜银矿、硒硫铜银矿、黝铜矿及脆银矿。  相似文献   

Preliminary evidence for human fecal contamination in corals of the Florida Keys,USA   总被引：6，自引：0，他引：6  

Lipp EK  Jarrell JL  Griffin DW  Lukasik J  Jacukiewicz J  Rose JB 《Marine pollution bulletin》2002,44(7):666-670

Corals and reef environments are under increased stress from anthropogenic activities, particularly those in the vicinity of heavily populated areas such as the Florida Keys. The potential adverse impacts of wastewater can affect both the environment and human health; however, because of the high decay rate of bacterial indicators in coral reef waters it has been difficult to document the presence of microbial contaminants and to assign risks in these environments. Here we show initial evidence that microorganisms associated with human feces are concentrated along the surface of coral heads relative to the overlying water column in the Florida Keys. Bacterial indicators (fecal coliform bacteria, enterococci or Clostridium perfringens) were detected in 66.7% of the coral surface microlayer (CSM) samples at levels between five and 1000 CFU/100 ml, but were found infrequently and at low numbers in the overlying water column ( < or = 2.5 CFU/100 ml). Similarly, enterovirus nucleic acid sequences, an indicator of human-specific waste, were detected in 93.3% of the CSM samples and only once in the water column by cell culture. Results show that coral mucus may accumulate enteric microorganisms in reef environments, and may indicate a risk to public and environmental health despite low indicator levels in the surrounding water.  相似文献   

First Results from Viper: Detection of Small-scale Anisotropy at 40 GHz     

Peterson JB  Griffin GS  Newcomb MG  Alvarez DL  Cantalupo CM  Morgan D  Miller KW  Ganga K  Pernic D  Thoma M 《The Astrophysical journal》2000,535(2):L83-L86

Using all available major samples of Seyfert galaxies and their corresponding closely matched control samples of nonactive galaxies, we find that the bar ellipticities (or axial ratios) in Seyfert galaxies are systematically different from those in nonactive galaxies. Overall, there is a deficiency of bars with large ellipticities (i.e., "thin" or "strong" bars) in Seyfert galaxies compared to nonactive galaxies. Accompanied with a large dispersion due to small number statistics, this effect is strictly speaking at the 2 sigma level. To obtain this result, the active galaxy samples of near-infrared surface photometry were matched to those of normal galaxies in type, host galaxy ellipticity, absolute magnitude, and, to some extent, redshift. We discuss possible theoretical explanations of this phenomenon within the framework of galactic evolution, and, in particular, of radial gas redistribution in barred galaxies. Our conclusions provide further evidence that Seyfert hosts differ systematically from their nonactive counterparts on scales of a few kiloparsecs.  相似文献   

国产高分三号卫星干涉测量试验     

黄震  赵双明  常青 《测绘地理信息》2021,46(4):7-11

主要利用国产高分三号(GF-3)卫星数据通过合成孔径雷达干涉测量(interferometric synthetic aperture radar,InSAR)技术提取试验区域数字高程模型(digital elevation model,DEM).首先介绍了GF-3卫星及其主要成像模式;然后介绍了InSAR数据处理过程及其关键技术,包括基线估计、影像配准、相位解缠等,并介绍其典型算法;最后利用GF-3试验数据提取DEM并对其进行精度评价.试验验证了目前国产SAR(synthetic aperture radar)卫星在干涉成像、干涉测量方面的能力.  相似文献