Since the gas-kinetic scheme uses a continuous gas distribution function at a cell interface for the fluxes evaluation, the moments of a gas distribution function can be explicitly obtained for the multiple temperature model.
Temperature evolutions at the centers of different-sized icy planetesimals, with radii 10 km, 50 km, 100 km, 500 km and 1000 km, which formed 1.0 Myr after CAI formation with 70 K for the initial temperature (models 10 10B, 50-10B, 100–10B, 500 10B and 1000 10B, respectively), are shown in Fig. 6.
The results for 500-km-size icy planetesimals, which formed 1.0 Myr, 1.5 Myr, 2.0 Myr and 2.4 Myr after CAI formation with 130 K for the initial temperature (models 500 10A, 500 15A, 500 20A and 500 24A, respectively), are shown in Fig. 7.
The PV temperature model accounts for the variation in the PV module temperature due to changes in the ambient temperature and the amount of the global irradiance absorbed by the PV module.
An exact analytical solution, for the temperature-independent model without radiation effect, is also derived.
Indeed, our sensitivity analyses indicate that the observed associations may be subject to some residual confounding by both PM (in urban areas) and temperature, despite extensive adjustment for the temperature in our models.
As the initial condition for the temperature distribution in the model space, we use a layered thermal state of a cooling oceanic plate described by an error function.
The MRT-TLBE consists of two sets of distribution functions, i.e., a D2Q9 model for the mass-momentum equations and a D2Q5 model for the temperature equation.
Questions related to the accuracy of the estimates with random process models vis-a-vis random variable models for the temperature fluctuations are examined.
These measurements agree with the model for the temperature of a thermocouple's hot junction.
