Multiple suppression by 2D filtering in the parabolic τ–p domain: a wave-equation-based method1     

Binzhong Zhou  Stewart Greenhalgh 《Geophysical Prospecting》1996,44(3):375-401

The filter for wave-equation-based water-layer multiple suppression, developed by the authors in the x-t, the linear τ-p, and the f-k domains, is extended to the parabolic τ-2 domain. The multiple reject areas are determined automatically by comparing the energy on traces of the multiple model (which are generated by a wave-extrapolation method from the original data) and the original input data (multiples + primaries) in τ-p space. The advantage of applying the data-adaptive 2D demultiple filter in the parabolic τ-p domain is that the waves are well separated in this domain. The numerical examples demonstrate the effectiveness of such a dereverberation procedure. Filtering of multiples in the parabolic τ-p domain works on both the far-offset and the near-offset traces, while the filtering of multiples in the f-k domain is effective only for the far-offset traces. Tests on a synthetic common-shot-point (CSP) gather show that the demultiple filter is relatively immune to slight errors in the water velocity and water depth which cause arrival time errors of the multiples in the multiple model traces of less than the time dimension (about one quarter of the wavelet length) of the energy summation window of the filter. The multiples in the predicted multiple model traces do not have to be exact replicas of the multiples in the input data, in both a wavelet-shape and traveltime sense. The demultiple filter also works reasonably well for input data contaminated by up to 25% of random noise. A shallow water CSP seismic gather, acquired on the North West Shelf of Australia, demonstrates the effectiveness of the technique on real data.  相似文献   

A radiative-conductive model for the prediction of radiation fog   总被引：2，自引：0，他引：2  

Wilford G. Zdunkowski  Allen E. Barr 《Boundary-Layer Meteorology》1972,3(2):152-177

A conductive-radiative model is used to predict the formation and growth of radiation fog. This is accomplished by solving numerically the heat and mass transport equations in conjunction with an approximate form of the radiative transfer equation. The equations of motion in simplified form are included in the physical system to make use of Blackadar's (1962) formulation of the exchange coefficient of the boundary layer.It is found for a number of hypothetical test cases that the model gives results which appear to represent real physical conditions. One actual situation is tested. Results show that the model reproduces better than qualitatively those parameters which are obtained from routine observations.  相似文献   

Comparison of acoustic instruments in an atmospheric turbulent flow over water     

M. Miyake  R. W. Stewart  R. W. Burling  L. R. Tsvang  B. M. Koprov  O. A. Kuznetzov 《Boundary-Layer Meteorology》1971,2(2):228-245

In the fall of 1968 an International Intercomparison Experiment was conducted to compare, among other things, acoustic anemometers designed for measurements of atmospheric turbulence. Excellent agreement was obtained in measurements of the vertical component, but an important discrepancy was revealed in measurements of the downwind velocity. The discrepancy proved far more significant in the cospectra than in the spectra themselves. It is evident that great care must be taken in the design of such instruments. An acoustic instrument was shown to have insufficient signal-to-noise ratio to serve as a thermometer under the near-neutral conditions often encountered over water.Comparison of the data-handling and data-analysis techniques showed that although the methods differed widely, the results were essentially identical.  相似文献   

UNDERGROUND WATERS NOW UNDEVELOPED     

Stewart L. Udall 《Ground water》1967,5(4):2-5

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Relativistically induced instellar density fluctuations     

P. Stewart 《Astrophysics and Space Science》1973,24(1):269-277

The spectrum of cold electron density fluctuations induced by a relativistic electron gas is investigated and the results discussed in relation to the interstellar medium.  相似文献   

Aleutian Strain Events: Observations and Interpretation     

J. H. Pfluke  R. M. Stewart 《Geophysical Journal International》1973,35(1-3):229-241

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Evolution of Planetesimal Velocities Based on Three-Body Orbital Integrations and Growth of Protoplanets     

Keiji OhtsukiGlen R. Stewart  Shigeru Ida 《Icarus》2002,155(2):436-453

We obtain the viscous stirring and dynamical friction rates of planetesimals with a Rayleigh distribution of eccentricities and inclinations, using three-body orbital integration and the procedure described by Ohtsuki (1999, Icarus137, 152), who evaluated these rates for ring particles. We find that these rates based on orbital integrations agree quite well with the analytic results of Stewart and Ida (2000, Icarus 143, 28) in high-velocity cases. In low-velocity cases where Kepler shear dominates the relative velocity, however, the three-body calculations show significant deviation from the formulas of Stewart and Ida, who did not investigate the rates for low velocities in detail but just presented a simple interpolation formula between their high-velocity formula and the numerical results for circular orbits. We calculate evolution of root mean square eccentricities and inclinations using the above stirring rates based on orbital integrations, and find excellent agreement with N-body simulations for both one- and two-component systems, even in the low-velocity cases. We derive semi-analytic formulas for the stirring and dynamical friction rates based on our numerical results, and confirm that they reproduce the results of N-body simulations with sufficient accuracy. Using these formulas, we calculate equilibrium velocities of planetesimals with given size distributions. At a stage before the onset of runaway growth of large bodies, the velocity distribution calculated by our new formulas are found to agree quite well with those obtained by using the formulas of Stewart and Ida or Wetherill and Stewart (1993, Icarus106, 190). However, at later stages, we find that the inclinations of small collisional fragments calculated by our new formulas can be much smaller than those calculated by the previously obtained formulas, so that they are more easily accreted by larger bodies in our case. The results essentially support the previous results such as runaway growth of protoplanets, but they could enhance their growth rate by 10-30% after early runaway growth, where those fragments with low random velocities can significantly contribute to rapid growth of runaway bodies.  相似文献   

Editorial     

John Wilson  Stewart Fotheringham  Gary Hunter  Jochen Albrecht 《Transactions in GIS》2006,10(2):153-153

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Ten Years On . . .     

John Wilson  Stewart Fotheringham  Gary Hunter  Jochen Albrecht 《Transactions in GIS》2006,10(3):333-333

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Automated correction of surface obstruction errors in digital surface models using off-the-shelf image processing   总被引：1，自引：0，他引：1  

Timothy D.  James  Stuart L.  Barr  Stuart N.  Lane 《The Photogrammetric Record》2006,21(116):373-397

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