On unified dual fields and Einstein deconvolution

Citation
D. Loewenthal et Ea. Robinson, On unified dual fields and Einstein deconvolution, GEOPHYSICS, 65(1), 2000, pp. 293-303
Citations number
22
Categorie Soggetti
Earth Sciences
Journal title
GEOPHYSICS
ISSN journal
00168033 → ACNP
Volume
65
Issue
1
Year of publication
2000
Pages
293 - 303
Database
ISI
SICI code
0016-8033(200001/02)65:1<293:OUDFAE>2.0.ZU;2-5
Abstract
In many physical phenomena, the laws governing motion can be looked at as t he relationship between unified dual fields which are continuous in time an d space. Both fields are activated by a single source. The most notable exa mple of such phenomena is electromagnetism, in which the dual fields are th e electric field and the magnetic field. Another example is acoustics, in w hich the dual fields are the particle-velocity field and the pressure field . The two fields are activated by the same source and satisfy two first-ord er partial differential equations, such as those obtained by Newton's laws or Maxwell's equations. These equations are symmetrical in time and space, i.e., they obey the same wave equation, which differs only in the interface condition changing sign. The generalization of the Einstein velocity addit ion equation to a layered system explains how multiple reflections are gene rated. This result shows how dual sensors at a receiver point at depth prov ide the information required for a new deconvolution method. This method is called Einstein deconvolution in honor of Albert Einstein. Einstein deconv olution requires measurements of the pressure signal, the particle velocity signal, and the rock impedance, all at the receiver point. From these meas urements, the downgoing and upgoing waves at the receiver are computed. Ein stein deconvolution is the process of deconvolving the upgoing wave by the downgoing wave. Knowledge of the source signature is not required. Einstein deconvolution removes the unknown source signature and strips off the effe cts of all the layers above the receiver point. Specifically, the output of Einstein deconvolution is the unit-impulse reflection response of the laye rs below the receiver point. Compared with the field data, the unit-impulse reflection response gives a much clearer picture of the deep horizons, a d esirable result in all remote detection problems. In addition, the unit-imp ulse reflection response is precisely the input required to perform dynamic deconvolution. Dynamic deconvolution yields the reflectivity (i.e., reflec tion-coefficient series) of the interfaces below the receiver point. Altern atively, predictive deconvolution can be used instead of dynamic deconvolut ion.