Thermal and magnetic evolution of the Earth’s core
By Stéphane Labrosse. 2003
216 citations recorded by the source corpus.
Subfields: Geophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/20f3b0ac074a726e4c0144947c093c1d332e4297
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In Geophysics
- F. Nimmo
- Julien Aubert
- U. Christensen
- Charles Poitou
- Stéphane Labrosse
- Claude Jaupart
- P. Olson
- A. Dombard
In Molecular Biology
Citations in the corpus
- Thermal versus elastic heterogeneity in high‐resolution mantle circulation models with pyrolite composition: High plume excess temperatures in the lowermost mantle (2009, background): “…our current limited understanding provides estimates ranging from 0.1 to 3.5 TW [Roberts and Glatzmaier, 2000; Buffett, 2002; Roberts et al., 2003; Labrosse, 2003; Gubbins et al., 2003; Christensen and Tilgner, 2004], The total core heat loss may thus approach 9–12 TW. Specifically, this implies…”
- The intensity of the geomagnetic field in the late-Archaean: new measurements and an analysis of the updated IAGA palaeointensity database (2009, background): “P b SH R IM P zi rc on (B la ke et al ., 20 04 ). convection (Buffett, 2003; Labrosse, 2003).”
- The paleomagnetism of single silicate crystals: Recording geomagnetic field strength during mixed polarity intervals, superchrons, and inner core growth (2006, background): “Most generally predict that the solid inner core started to grow no earlier than approx- imately 2.5–2.7 billion years ago [e.g., Labrosse et al., 2001; Labrosse, 2003; Labrosse and Macouin, 2003; Buffett, 2003], but some prefer a greater age [e.g., Gubbins et al., 2004].”
- Energetics of the Core (2015, methodology): “…will be useful to expand Is as follows: Is = 4 3 πTcenρcenr 3 ce −r2c/A2 ( 1 + 2 5 r2c A2 + · · · ) (56) The temperature profile will depart from the adiabat in the inner core, but Labrosse (2003) argues that the integral may be taken over the entire core without introducing significant errors.”
- Dipole moment scaling for convection-driven planetary dynamos (2005, background): “Thermal historymodels indicate that the buoyancy flux F has changed with time, due to secular cooling and inner core growth [34,35].”
- Dynamo Scaling Laws and Applications to the Planets (2010, background): “The amount of ohmic dissipation in the Earth’s core has been a contentious issue, with estimates ranging between 0.1 and 3.5 TW (Buffett 2002; Roberts et al. 2003; Labrosse 2003; Gubbins et al. 2003; Christensen and Tilgner 2004).”
- Modelling the palaeo-evolution of the geodynamo (2009, background): “Thus, in order to achieve scaling predictions relevant to the Precambrian Earth dynamo, one needs a time-series of the dynamo power, which can be evaluated from core thermodynamics and Earth cooling histories (e.g. Labrosse 2003; Lister 2003).”
- Temperatures, Heat, and Energy in the Mantle of the Earth (2007, background): “Such a slow variation is compatible with thermal evolution models of the Earth’s core, provided that ohmic dissipation increased by a factor of four when the inner core started crystallizing (Labrosse, 2003).”
- Sulfur's impact on core evolution and magnetic field generation on Ganymede (2005, background): “accurate to second-order [Labrosse, 2003].”
- Thermal evolution of the core with a high thermal conductivity (2014, unknown): “This behavior was already discussed (Labrosse, 2003; Labrosse and Macouin, 2003; Aubert et al., 2009) and shows that addressing the question of the minimum value of the dissipation at the present time is not sufficient: because the inner core is so young, the present CMB heat flow is in fact…”