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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A1~Lernativel.y<br />
p = 30. m, where T in h. (lb 1<br />
Eqs, (la,b) can also be used as a rule of thumb if p varies with<br />
depth and an average resistivity is inserted.<br />
The natural magnetic source fields of the ionospheric and magneto-<br />
spheric currents offer periods approxiniately between 0.1 see and 20<br />
permitting crustal and upper mantle surveys down to a depth of<br />
approximately 800 - 1000 km. On the other side periods between 0.91<br />
and 0.002 sec are most commonly used for Sounding of? -?he first 300 c<br />
with artificial fields.<br />
Electromagnetic methods are applicab1.e for two objectives:<br />
1) ~nvestigation of the change of conductivity with depth, in par.ti-<br />
cular detection and delineation of horizontal interfaces marking<br />
a change of stratigraphy or temperature.<br />
2) Investigation of lateral conductivity variations, in particular<br />
search for local regions wiCh abnormal conductivities (e.g.<br />
meta1lj.c ore deposi-ts, salt domes, sedimeni-dry' basins, zones of<br />
eleva-ted temperature).<br />
.The results of the first investigation are often used. to construct<br />
a normal. conductivi-ty model from which local deviations are measure1<br />
In an interpretation of natural fields the c:-.ange of the electro-<br />
magnetic field quantities both with frequency and with position are<br />
used. Broadly speaking .the dependence on the position provides the<br />
lateral reso1.u-tion and the dependence on frequency gives the reso-<br />
lu-tion with depth.<br />
1.2. Dasic equations -<br />
Let - r be .the position vector and let H, g, 2nd + I he the vectoi-s of<br />
the magnetic field, electrical field and curl-2n.t density, ~?especti-<br />
vely. Using SI u11.i.-ts and a vacuurrl permeability throughout:, the<br />
0<br />
pertinent equations are<br />
cupl - H = - I i- L<br />
11.2)<br />
. -e<br />
CUI?].' - E = --kt H<br />
(1.3)<br />
0-<br />
. .<br />
'- 1 = 0- C<br />
(l.4)<br />
div - !i = 0<br />
(1.5)