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P. Schmoldt, PhD - MTNet - DIAS

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5. Earth’s properties observable with magnetotellurics<br />

1000/T (K -1 )<br />

1.6<br />

1.4<br />

1.2<br />

1<br />

0.8<br />

0.6<br />

Ionic conduction<br />

Proton conduction<br />

Small polaron conduction<br />

0.4<br />

0 1 2 3 4 5 6 7<br />

Log (ρ) (Ωm)<br />

10<br />

Fig. 5.12.: Conductivity of hydrogen-iron bearing mantle silicate minerals; redrawn from Yoshino [2010]<br />

Mineral σ0H (S/m) HH (eV) σ0P (S/m) H0 P<br />

(eV) α<br />

Wadsleyite 399(311) 1.49(10) 7.74(4.08) 0.68(3) 0.02(2)<br />

Ringwoodite 838(442) 1.36(5) 27.7(9.6) 1.12(3) 0.67(3)<br />

Tab. 5.5.: Parameter values for wadsleyite and ringwoodite derived in lab studies by Yoshino et al. [2008]. Numbers in parentheses<br />

denote the errors determined through nonlinear least squares fitting (1 σ standard deviation).<br />

(Fig. 5.12). One of the most recent formulation for the relationship between mantle mineral<br />

semiconduction and its controlling parameters was given by Yoshino et al. [2008].<br />

The authors extended earlier formulations by taking into account the influence of both the<br />

intrinsic and the extrinsic conductivity, as well as the effect of water onto the extrinsic<br />

term:<br />

<br />

σ = σ0H exp − ∆HH<br />

<br />

kBT<br />

+ σ0PCw exp<br />

⎛<br />

⎜⎝ −∆H0<br />

P<br />

− αC1/3<br />

W<br />

kBT<br />

⎞<br />

⎟⎠<br />

(5.11)<br />

with CW: water content in wt%, α: fitting factor, and subscripts H and P denoting small<br />

polaron (hopping) conduction and proton conduction, respectively. Parameter values for<br />

the olivine high-pressure polymorphs wadsleyite and ringwoodite, derived by the authors<br />

by fitting measured laboratory data to Equation 5.11, are given in Table 5.5. Conductivity<br />

of the individual mantle materials, their specific parameters, and relation to pressure,<br />

temperature, and fluid content are examined in more detail in Section 5.3.<br />

5.2.3. The Earth’s core<br />

The Earth’s core is situated beneath the CMB at around 2890 km depth, down to the centre<br />

of the Earth, approximately 6378 km from the Earth’s surface. The core is subdivided<br />

into a liquid outer core and a solid inner core. The existence of a solid inner core was<br />

first proposed by Inge Lehmann in 1936, using the observations of seismic waves caused<br />

98

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