Sentence examples for At cmb from inspiring English sources

At CMB temperatures less than ∼1420 K, solid Fe 3−x S 2 will simultaneously crystallize at the bottom of the core.

Therefore, crystallization of the core of the planets must have started at CMB.

This corresponds to the idea that the representation errors at CMB are simply proportional to the SV Gauss coefficients.

We conclude that the V p at CMB is constrained well by the τ−p inversion to 8.03 ± 0.01 km/s, irrespective of the starting model.

Therefore, the core mantle boundary (CMB) temperature can be calculated as follows: {T}_{mathrm{CMB}}={T}_{mathrm{ICB}}{left(frac{rho_{mathrm{CMB}}}{rho_{mathrm{ICB}}}right)}^{gamma mathrm{th}} where T CMB and T ICB are temperatures at the CMB and the ICB conditions, respectively, and ρ CMB and ρ ICB are densities of the molten core at CMB and ICB, respectively.

The adiabatic temperature of the core of Mercury estimated by this work, 27 K/GPa, is given as a red curve, S, under the assumption that the temperature at CMB of Mercury is 1800 K (e.g., Dumberry and Rivoldini 2015; Malavergne et al. 2010).

Dietrich et al. (2015) discuss effects of thermal anomalies at the CMB (CMB hotspots) on planetary dynamos and imply that a possible Martian hemispherical dynamo cannot explain the dichotomy observed in the crustal magnetization on Mars.

The points A (at the CMB) and B (at the 200 km depth) are located at 33°S and 76°S, respectively.

We therefore cannot compare meaningfully maps of the SV at the CMB with those obtained at earlier epochs.

They imply that iron snow can be a dynamo mechanism for the Moon, Mercury, and Ganymede and likely for Mars and that FeS crystallization can occur not only at the ICB but also at the CMB, in the core.

The latitude of central points is, for example, about 33°S for paths bottoming at the CMB and about 76°S for paths bottoming at a 200 km depth.