IntroductionUse of the laser-heated diamond cell with modern synchrotron beam lines makes it possible to study mineral and rock samples in situ at the pressures and temperatures of the Earth's deep mantle and core. These are steady state experiments, with continuous wave (CW) laser heating allowing the conditions of high temperatures and pressures to be sustained for time periods from minutes to hours. Such experiments yield measurements that are essential for interpreting geophysical observations, from s½ismology and geod½sy, in terms of the composition, state, and key processes of the planetary interior.To obtain quantitative measurements from the experiments, however, it is critical to document the temperature and pressure variations across the sample. This is accomplished partially through the use of spectroradiometry and internal calibrants, but it remains necessary to understand and fully model the heat transfer within the sample in order to ensure reliable results. In particular, the effects of axial temperature gradients that are not measured explicitly through spectroradiometry must be considered. An added benefit is that such modeling also yields information about the thermal conductivity of the sample as a function of pressure and temperature.The largest temperature increases with depth in the planet take place across thermal boundary layers, where conduction