一种利用广义点和物方补偿纠正建筑影像的算法

针对双灭点条件下纠正大倾角近景影像算法的不足,提出了基于灭点理论、空间直线几何补偿联合广义点(直线)摄影测量光束法平差的建筑物影像自动纠正算法。实验结果表明,改进算法具有一定效果。     

采用灰度分割的自适应矩匹配条带噪声去除方法

针对国产卫星全色影像中的随机条带噪声现象,提出了一种采用灰度分割的自适应矩匹配条带噪声去除方法。该方法首先将不同反射特性的地物按照灰度差异进行分割处理,然后对每一个分割区域分别采用标准矩匹配进行处理,从而抑制标准矩匹配处理过程中造成的灰度畸变。选取资源1号02C-HR光学影像进行实验,结果表明,与现有的去噪方法相比,所得图像质量有较大提升。     

海洋沉积物粒度参数3种计算方法的对比研究

海洋沉积物粒度参数是反映沉积物物质来源及水动力条件的敏感性指标。目前国内对海洋沉积物粒度参数计算方法并不完全统一,制约了粒度数据的整合和使用。利用长江口外近海348个表层沉积物粒度数据,分别使用Folk和Ward的图解法公式、Collias等的矩法公式和McManus的矩法公式进行了粒度参数的计算。运用相关分析和基本统计分析等方法,讨论了不同方法计算结果间的差异和影响因素。结果显示:图解法与矩法计算的平均粒径和分选系数分别呈显著线性相关,且不受沉积物物质来源的影响。对于偏态和峰态,3种不同方法计算结果的相关性较低,甚至表现为不相关。不同方法计算的沉积物粒度参数的差异性均与沉积物类型和频率曲线分布形态有关。当物质组成均匀、频率曲线近正态分布时,不同方法计算的粒度参数的相关性显著提高。当沉积物较粗或较细时,粒度分布偏离正态且具有明显尾部特征,用不同方法计算结果的差异会随之增大。对3种不同公式综合对比认为Collias等的矩法公式反映沉积物粒度分布特征更加灵敏、可靠,建议在进行资料整合时采用。     

Dipolar magnetic moment of the bodies of the solar system and the Hot Jupiters

Context

The planets magnetic field has been explained based on the dynamo theory, which presents as many difficulties in mathematical terms as well as in predictions. It proves to be extremely difficult to calculate the dipolar magnetic moment of the extrasolar planets using the dynamo theory.

Objective

The aim is to find an empirical relationship (justifying using first principles) between the planetary magnetic moment, the mass of the planet, its rotation period and the electrical conductivity of its most conductive layer. Then this is applied to Hot Jupiters.

Method

Using all the magnetic planetary bodies of the solar system and tracing a graph of the dipolar magnetic moment versus body mass parameter, the rotation period and electrical conductivity of the internal conductive layer is obtained. An empirical, functional relation was constructed, which was adjusted to a power law curve in order to fit the data. Once this empirical relation has been defined, it is theoretically justified and applied to the calculation of the dipolar magnetic moment of the extra solar planets known as Hot Jupiters.

Results

Almost all data calculated is interpolated, bestowing confidence in terms of their validity. The value for the dipolar magnetic moment, obtained for the exoplanet Osiris (HD209458b), helps understand the way in which the atmosphere of a planet with an intense magnetic field can be eroded by stellar wind. The relationship observed also helps understand why Venus and Mars do not present any magnetic field.     

Analysing seismic-source mechanisms by linear-programming methods

Summary. Linear-programming methods are powerful and efficient tools for objectively analysing seismic focal mechanisms and are applicable to a wide range of problems, including tsunami warning and nuclear explosion identification. The source mechanism is represented as a point in the six-dimensional space of moment-tensor components. Each observed polarity provides an inequality constraint, linear with respect to the moment tensor components, that restricts the solution to a half-space bounded by a hyperplane passing through the origin. The intersection of these half-spaces is the convex set of all acceptable solutions. Using linear programming, a solution consistent with the polarity constraints can be obtained that maximizes or minimizes any desired linear function of the moment tensor components; the dilatation, the thrust-like nature, and the strike-slip-like nature of an event are examples of such functions. The present method can easily be extended to fit observed seismic-wave amplitudes (either signed or absolute) subject to polarity constraints, and to assess the range of mechanisms consistent with a set of measured amplitudes.     

Fault plane solutions of microearthquakes and small events in the Hellenic arc

The Hellenic arc is the most active seismic region of the transition zone between the African and Eurasian plates. In this rapidly deforming region, the physical state of the crust and upper mantle may vary laterally and vertically. However, a detailed 3D model of the region is lacking. The reliable determination of fault plane solutions is crucial if such a model is to be produced. On this basis, fault plane solutions have been determined from recent microearthquakes and small events to assess their reliability for use in tectonic interpretation. A search algorithm on first motion data and amplitude ratios and also a waveform-matching scheme were employed on data from our temporal network, operated on the western part of the island of Crete. There, a network of 47 three-component digital stations with an aperture of 60 km and an average station spacing of 5 km was operated in 1997. The majority of the shallow microearthquakes under Crete for which fault plane solutions were determined have a near horizontal T-axis oriented essentially E–W. Differences between well determined fault plane solutions from the search algorithm and the waveform-matching technique were significant (strike up to 45°, dip up to 10°, and slip up to 50°). Second, data of small events within the Hellenic subduction zone were obtained from recently installed broadband stations at local and regional distances and inverted for a deviatoric seismic moment tensor. Available solutions from other sources such as the Harvard group, EMSC, or SED show drastic differences in part. Owing to still limited azimuthal station coverage, the resulting fault plane solutions of small events have generally not been well constrained. The observed large variation of fault plane solutions for micoearthquakes and small events poses a caveat to tectonic interpretation in case of using data from a few stations only.     

The effect of focal depth error on moment tensor inversion

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2000年上半年全球地震活动

2000年上半年全球共发生MW≥6．5地震14次。其中MW≥7．0地震7次；浅源地震10次；中源地震3次；深源地震1次。浅源大地震发生的区域集中于印度尼西亚和南印度洋地区。6月份发生的地震所释放的地震矩占上半年全球所有地震释放的地震矩的一大半。