Schmucker-Weidelt Lecture Notes, Aarhus, 1975 - MTNet

Schmucker-Weidelt Lecture Notes, Aarhus, 1975 - MTNet Schmucker-Weidelt Lecture Notes, Aarhus, 1975 - MTNet

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. A as transfer function between A and B in the wave number domain, which contains the information about the internal resistivity distribution. A vertical sounding of this distribution is made by considering h R as a function of frequency, k being fixed, or vice versz. If the array covers the whole globe, the sphericity of the Earth re- quires the replacement of the krigonometric functions by spherical harmonics in spherical coordinates Cr,B,A): a: Garth' s radius ; p:(cos@ : Associated' spherical function. The trans-. fer functions have then the form The first and still basic investigations of the Earth's deep conduc- tivity structure have been carried out by this approach (SCHUSTER, CHAPMAN and PRICE). If the array of stations covers only a region of Limited extent, it may be !impracticable to de'compose the observed field into wave- spec-tral components or it may be even impossible because only a small. section of the source field structure has been observed. In that case vertical array soundings are carried out preferably with response functi.ons in the frequency-distance domain. Suppose the source field is quasi-uniform ,i.n one horizon.ta1 direc-- j tion, say, U = UCw,y) and V : V(w,y). Ls't * . % be the inverse Fourier transform of R. Then, if V is given by the ,. A roduct of R with U in the (u,k) domain, V will be given by a corlvolution 05 R with IJ in the (w,y) domain: +w with .R U = 1 RCw,y-n) UCq)dq. -m

If, for instance E = V and H = U, the magnetotelluric relation A ,. X Y EX = WM, C II of the k-w domain will transform& into Y with N(w,y) as Fourier - transform of C(o,k). Observe that reversely 4 -iky CCw,k) = I N(w,y)e. dy and therefore -03 f- CCw,O) = J N(w,y)dy. -m Hence, if H is quasi-uniform within the range of the kernel M, Y which is the CAGNIARD-TIKHONOV relaticn con~monly used for single 1 site sounding-s. In a similar way the magnetic ratio, of vertical to horizontal' va- riations can be generalized to with MCw,y) as Fourier transform of ik C(w ,k ) . Y Y The response functions N and M have their highes-t valuei. close to y - O and approach zero for distances y which are large i.n compari- son to the modulus of C(w,k=O): d.;:.rn,-Lc. do-,,o. :., ----. - ---. . A.

. A<br />

as transfer function between A and B in the wave number domain, which<br />

contains the information about the internal resistivity distribution.<br />

A vertical sounding of this distribution is made by considering<br />

h<br />

R as a function of frequency, k being fixed, or vice versz.<br />

If the array covers the whole globe, the sphericity of the Earth re-<br />

quires the replacement of the krigonometric functions by spherical<br />

harmonics in spherical coordinates Cr,B,A):<br />

a: Garth' s radius ; p:(cos@ : Associated' spherical function. The trans-.<br />

fer functions have then the form<br />

The first and still basic investigations of the Earth's deep conduc-<br />

tivity structure have been carried out by this approach (SCHUSTER,<br />

CHAPMAN and PRICE).<br />

If the array of stations covers only a region of Limited extent, it<br />

may be !impracticable to de'compose the observed field into wave-<br />

spec-tral components or it may be even impossible because only a small.<br />

section of the source field structure has been observed. In that<br />

case vertical array soundings are carried out preferably with response<br />

functi.ons in the frequency-distance domain.<br />

Suppose the source field is quasi-uniform ,i.n one horizon.ta1 direc-- j<br />

tion, say,<br />

U = UCw,y) and V : V(w,y). Ls't<br />

* . %<br />

be the inverse Fourier transform of R. Then, if V is given by the<br />

,. A<br />

roduct of R with U in the (u,k) domain, V will be given by a<br />

corlvolution 05 R with IJ in the (w,y) domain:<br />

+w<br />

with .R U = 1 RCw,y-n) UCq)dq.<br />

-m

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