Estimation of periodicities in hydrologic data     

A. R. Rao  G. D. Jeong  Fi-John Chang 《Stochastic Hydrology and Hydraulics》1992,6(4):270-288

Periodicites in hydrologic data are frequently estimated and studied. In some cases the periodic components are subtracted from the data to obtain the stochastic components. In other cases the physical reasons for the occurrence of these periodicities are investigated. Apart from the annual cycle in the hydrologic data, periods corresponding to the 11 year sunspot cycle, the Hale cycle and others have been detected.The conclusions from most of these studies depend on the reliability and robustness of the methods used to detect these periodicities. Several spectral analysis methods have been proposed to investigate periodicities in time series data. Several of these have been compared to each other. The methods by Siddiqui and Wang and by Damsleth and Spjotvoll, which are stepwise procedures of spectrum estimation, have not been evaluated.  相似文献   

Sediment shear Q from airgun OBS data   总被引：2，自引：0，他引：2  

P. D. Bromirski  L. N. Frazer  F. K. Duennebier 《Geophysical Journal International》1992,110(3):465-485

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Internal wave characteristics in the eastern Arabian Sea during summer monsoon     

P G K Murthy  G S Sharma  V V James  K V Suseela 《Journal of Earth System Science》1992,101(4):317-327

The time series BT profiles and surface winds and atmospheric pressure, collected in the deep waters off Ratnagiri and Karwar during summer monsoon were utilized to document the characteristics of internal waves (IW). Low-frequency (≤2, cycle per day (cpd)) IW off Ratnagiri are found to propagate at 83 cm/s with wavelengths of 45 km and wave heights upto 40 m. These parameters for high-frequency (>2 cpd) IW off Karwar correspond to 99 cm/s, 3 km and 23 m. The IW off Karwar appear to leave the station at 70° (±10°) (measured from the horizontal). The data sets were further analysed to address the harmonic composition of the IW and identify the possible sources for the observed IW fields. Power spectra of the IW indicated energy peaks at inertial (0·6 cpd) and tidal (1 and 2 cpd) frequencies off Ratnagiri and in the high-frequency band of 0·5–2·0 cycles per hour off Karwar. The coherence between the IW and wind/tide is found to be good at several frequencies within the IW spectrum. This feature probably suggests tides as a source for the IW of tidal frequencies and winds and tides as a joint source for the IW at the remaining frequencies.  相似文献   

Multifractal modeling and spatial point processes   总被引：8，自引：0，他引：8  

Quiming Cheng  Frederik P. Agterberg 《Mathematical Geology》1995,27(7):831-845

The multifractal model can be applied to spatial point processes. It provides new, approximately power-law type, expressions for their second-order intensity and K (r) functions. The box-counting and cluster dimensions are different but mutually interrelated according to multifractal theory. This approach is used to describe the underlying spatial structure of gold mineral occurrences in the Iskut River area, northwestern British Columbia. The box-counting and cluster dimensions for the example are estimated to be 1.335±0.077 and 1.219±0.037, respectively. The relatively strong clustering of the gold deposits is reflected by the fact that both values are considerably less than the corresponding Euclidean dimension (=2).  相似文献   

Spectral magnitude and seismic radiated energy computed from CDSN records     

Pei-Shan Chen  Seweryn J. Duda 《地震学报(英文版)》1993,6(4):803-811

We have employed 10 digital records and computed the spectral magnitude and the seismic radiated energy for 18 large earthquakes (M _s≥6) occurred in Eur-asian belt during 1986–1989. The nine digital stations (CD-SN) distribute all over China and one in Germany. The spectral magnitudes of various period have different stability among stations. The stability is better for maximum spectral magnitudemi and seismic radiated energyE, their differences among stations are smaller, especially for the stations where the ray path main penetrates the low mantle. But the stability of corner period is usually not good. The relation between seismic radiated energy and seismic moment magnitudeM _w is lg (E)=1.5Mw+c, wherec is a constant. The maximum spectral magnitudemi=M _w+0.1, it is consistant with theoretical prediction. The Chinese version of this paper appeared in the Chinese edition ofActa Seismologica Sinica,15, 418–426, 1993. This work supported by the Deutsche Forschungsgemeinschaft, Bonn, F. R. Germany. The support is grateful acknowledge.  相似文献   

金相分析中消除划痕的两种方法     

梁采 《成都信息工程学院学报》1999,(4):91

介绍了两种在金相分析中采用模式识别技术,以距离聚类和角度类消除划痕的方法,使主体更加突出,分类评级更加准确,也降低了对试样的磨制要求。  相似文献   

一次东北冷涡过程的宏微观物理特征分析     

李冬楠  刘星光  高倩楠  袁潮  李鹏  安英玉 《气象科技》2021,49(2):227-234

利用2019年5月20日机载DMT和SPEC粒子测量系统获取的飞机云微物理探测资料,结合高空、地面、卫星云图产品等常规气象数据,分析了东北冷涡在发展成熟期的云宏微观结构特征。结果表明:飞机探测区域为冷性层积混合云,云水充沛。云粒子探头(CDP)和二维云粒子图像探头(CIP)探测到的最大粒子数浓度分别为362.10cm~(-3)、191.08L~(-1),液态含水量变化范围为0～0.88g/m~3;CDP粒子谱呈指数型下降,谱宽较窄;CIP粒子谱呈双峰结构。云粒子图像探测仪CPI表明,层积云上部主要为冰雪晶粒子,以冰晶的核化和凝华增长为主;中上部粒子主要为小冰晶形态,也有冰晶聚合体和枝状冰晶;中下部是过冷水和冰晶粒子的共存区,过冷水较为丰富。  相似文献   

The gravitational perturbation spectrum in linear satellite theory     

Stefano Casotto 《Celestial Mechanics and Dynamical Astronomy》1995,62(1):1-22

A new method for calculating the perturbation spectrum in the framework of Kaula's linear satellite theory (LST) is introduced. The novelty of this approach consists in using recent results on the spectral decomposition of the perturbation frequencies in LST to provide a closed formulation for the amplitude and the phase of each line in the perturbation spectrum. The theory presented here can be applied to perturbations in the elements or in the radial and transverse directions due to the geopotential or to the tides. Separate algorithms are developed for application to orbits with circulating or frozen perigee.  相似文献   

Optical depth effects on the formation of spectral lines in rotating and expanding spherical atmospheres     

A. Peraiah  G. Raghunath  K. N. Nagendra 《Journal of Astrophysics and Astronomy》1981,2(3):277-284

We have investigated the effects of increasing optical depths on spectral lines formed in a rotating and expanding spherical shell. We have assumed a shell whose outer radius is 3 times the inner radius, with the radial optical depths equal to 10, 50, 100, 500. We have employed a constant velocity with no velocity gradients in the shell. The shell is assumed to be rotating with velocities varying as 1/_ρ, where_ρ is the perpendicular distance from the axis of rotation, implying the conservation of angular momentum. Two expansion (radial) velocities are treated: (1)V = 0 (static case) and (2)V = 10 mean thermal units. The maximum rotational velocities areV _rot = 0, 5, 10 and 20. In the shell where there are no radial motions, we obtain symmetric lines with emission in the wings forV _rot = 0 and 5 while forV _rot ≥ 10 we obtain symmetric absorption lines. In the case of an expanding shell, we obtain lines with central emission.  相似文献   

A study on the combination of satellite, airborne, and terrestrial gravity data   总被引：3，自引：2，他引：1  

M. Kern  K. K. P. P. Schwarz  N. Sneeuw 《Journal of Geodesy》2003,77(3-4):217-225

Satellite gravity missions, such as CHAMP, GRACE and GOCE, and airborne gravity campaigns in areas without ground gravity will enhance the present knowledge of the Earths gravity field. Combining the new gravity information with the existing marine and ground gravity anomalies is a major task for which the mathematical tools have to be developed. In one way or another they will be based on the spectral information available for gravity data and noise. The integration of the additional gravity information from satellite and airborne campaigns with existing data has not been studied in sufficient detail and a number of open questions remain. A strategy for the combination of satellite, airborne and ground measurements is presented. It is based on ideas independently introduced by Sjöberg and Wenzel in the early 1980s and has been modified by using a quasi-deterministic approach for the determination of the weighting functions. In addition, the original approach of Sjöberg and Wenzel is extended to more than two measurement types, combining the Meissl scheme with the least-squares spectral combination. Satellite (or geopotential) harmonics, ground gravity anomalies and airborne gravity disturbances are used as measurement types, but other combinations are possible. Different error characteristics and measurement-type combinations and their impact on the final solution are studied. Using simulated data, the results show a geoid accuracy in the centimeter range for a local test area.  相似文献