Electrical and thermal conductivities of Fe–Ni–Si alloy under core conditions
By F. Stacey, O. Anderson. 2001
168 citations recorded by the source corpus.
Subfields: Geophysics, Materials Chemistry, Mechanical Engineering
View Paper: https://www.semanticscholar.org/paper/d930f7a2abe101b26764561a52e3805e9ac5c38d
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Citations in the corpus
- Internal and tectonic evolution of Mercury (2003, background): “A superadiabatic temperature gradient, which corresponds to a heat flux from the core of at least 12–13 mW/m(2) (given a core thermal conductivity of f 40 W/(m K) [55] and the parameters in Table 1), or growth of an inner core with its attendant release of buoyant S, may independently be sufficient ”
- Energetics of the Core (2015, methodology): “The latter data were used by Stacey and Anderson (2001) to conclude that k at the CMB was 46 W m−1 K−1.”
- Sulfur's impact on core evolution and magnetic field generation on Ganymede (2005, methodology): “Assuming a core thermal conductivity of 40 W m K 1 [e.g., Stacey and Anderson, 2001], only models with twice chondritic heat production and 6–8.5 wt % bulk core sulfur content satisfy this dynamo requirement after 4.5 Gyr.”
- The high conductivity of iron and thermal evolution of the Earth’s core (2013, background): “2007) and SA01 (Stacey and Anderson, 2001) show the earlier estimates.”