Rapid sedimentation causes low surface heat flow values, apparently due to a delay in recovery from the disturbed thermal equilibrium.
The apparent effect of thermal insulation caused by the Sydney Basin coal measures results in an overall rise in the temperature field underneath those coal measures, despite exhibiting relatively low surface heat flux (Rawling et al. 2014).
Merit indices of material properties are deduced, and optimal materials are selected on the basis of these criteria, for the case of a high Biot number (high surface heat transfer) and a low Biot number (low surface heat transfer).
These conditions are characterized by the lowest surface temperature and heat transfer coefficient at which spallation can be successfully initiated.
Rolandone et al. (2013) determined a uniformly low (45 mW m−2) surface heat flow in the entire region of the eastern Arabian Platform, which is in accordance with the results determined from the newly measured temperature profiles of this study.
This low near-surface heat flux could characterize a convergent margin (Hopkins et al. 2010), rigid plate tectonics (Korenaga 2011), stagnant-lid model (Condie and O'Neill 2010), or heat-pipe model (Moore and Webb 2013).
Furthermore, due to its high surface heat flux and low velocities under natural circulation in any post-LOCA scenario, three effects impair the capability of turbulent gas flow to remove heat from the GFR core, namely: (1) acceleration effect, (2) buoyancy effect and (3) property variation.
In the HZ, this steady state can produce a super-cooling of the core when tidal heating is strong enough to heat the mantle and decrease its viscosity and low enough not to dominate the surface heat flow.
The low surface coverage isosteirc heat of CO2 adsorption (Qst) is calculated by the Clausius Clapeyron equation using the data obtained at 273 and 298 K, and the calculated value of Qst is 58.4 kJ mol−1.
