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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The field within the conducting sphere, r - < a, is derived from - P as described in Sec. 7.3. Observing that the radial component of rot rot - P reduces by the use of spherical harmonics to the field components of the spherical harmonic of degree n and order m are: and The impedance of the field at spherical sur'aces, expressed in terms of c:, is then as in the case of plane donductors given by For the field outside of the conducting sphere, r - > a, the solution of the radial function is (in quasi-stationary approximation) Hence, the surface value of the charlac-terisll-ic scale length for r = a is found to be The ratio of internal. -to external. parts of the magnetj.~ surfacc fleld is by definition

yielding The ratio of internal to external parts is therefore derived from cm according to n which demonstrates the r$le of n/a, respec-tive1.y (n+l)/a, as equi- c valent wavenumber of the source fielh in spherical coordinates (cf. Sec. 9.1). The spherical version of the input function for the inverse problem, based on a linearisation according to the $-algorithm, is con- veniently defined as with K~ = itopO/pO. It w ill be shown that the spherical ccrrection 0 is of the order (n[~[/a)', if the conductivity is more or less uniform. If degree and order of the spherical. harmonic representation of the source field are independent of frequency (this is true for;D st but -- not for S ), the inverse problem can be solved by deriving 9 from spherical response functions a prel-iminary plane-earth model h This model. is subsequently transformed into a spherical. Earth model p(r) with WEIDELT's transformation formula: with

yielding<br />

The ratio of internal to external parts is therefore derived from<br />

cm according to<br />

n<br />

which demonstrates the r$le of n/a, respec-tive1.y (n+l)/a, as equi- c<br />

valent wavenumber of the source fielh in spherical coordinates<br />

(cf. Sec. 9.1).<br />

The spherical version of the input function for the inverse problem,<br />

based on a linearisation according to the $-algorithm, is con-<br />

veniently defined as<br />

with K~ = itopO/pO. It w ill be shown that the spherical ccrrection<br />

0<br />

is of the order (n[~[/a)', if the conductivity is more or less<br />

uniform.<br />

If degree and order of the spherical. harmonic representation of<br />

the source field are independent of frequency (this is true for;D st<br />

but -- not for S ), the inverse problem can be solved by deriving<br />

9<br />

from spherical response functions a prel-iminary plane-earth model<br />

h<br />

This model. is subsequently transformed into a spherical. Earth<br />

model p(r) with WEIDELT's transformation formula:<br />

with

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