Adiabatic temperature profile in the mantle

By T. Katsura, A. Yoneda, D. Yamazaki, T. Yoshino, E. Ito. 2010

437 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/654252deca374dc918551fb6450c4de5371c93b7

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In Geophysics

Citations in the corpus

Mantle dynamics in super-Earths: Post-perovskite rheology and self-regulation of viscosity (2012, background): “9x10 K at Earth’s CMB pressure, consistent with mineral physics 299 constraints (Chopelas and Boehler, 1992; Katsura et al., 2010; Komabayashi et al., 2008; 300 Mosenfelder et al., 2009), and to about 1.”
Dynamics and evolution of the deep mantle resulting from thermal, chemical, phase and melting effects (2012, background): “Almost all mineral physics papers that calculate the expansivity at CMB pressures find values of 1.0–1.2×10−5/K (e.g., Anderson et al., 1992; Chopelas and Boehler, 1992; Katsura et al., 2010; Kombayashi et al., 2008; Mosenfelder et al., 2009; Tsuchiya et al., 2005).”
Primary magmas and mantle temperatures through time (2017, background): “An adiabatic temperature increase of 0.4–0.5 and 0.38C/km has been proposed through the upper and lower mantle, respectively [Schubert et al., 2001; Katsura et al., 2010].”
SUPER-EARTH ATMOSPHERES: SELF-CONSISTENT GAS ACCRETION AND RETENTION (2015, methodology): “This simplification is in accordance with realistic adiabatic profiles, in which the temperature changes only by a factor of order unity, while the pressure varies by orders of magnitude (e.g., Katsura et al. 2010).”
The composition of Mars (2019, background): “Temperature profile in the Martian mantle (areotherm) is estimated assuming an Earthlike profile (Katsura et al., 2010), mantle potential temperature of ∼1,500 K (Baratoux et al.”