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The early evolution of the solid Earth and its atmosphere and oceans is covered in geologic history of Earth.
The evolution of the solid volume fraction fS=1−fL is analyzed in terms of the Johnson Mehl Avrami model.
Impact processes influence the surface evolution of the solid bodies in the Solar System, as asteroids or comets.
Numerical analysis of 2D and 3D images of the microstructure measured by X-ray radiography and microtomography reveals the evolution of the solid particles during annealing.
To optimize and control such processes, it is essential to understand the sequence of events that occur in the evolution of the solid phase, rather than simply characterizing the final product recovered at the end of the process.
Unraveling important processes such as the evolution of the solid earth, global cycling of energy, oxygen, water, etc., the responses of the biosphere to disturbances, and others mandates the best possible exploitation of the data.
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During the crystallization process, the changes in the amount and the identity of the solid phase are established from the time evolution of the solid-state NMR spectrum.
The influence of nanoparticle volume fraction and metal foam porosity on the evolution of the solid-liquid interfaces, distribution of isotherms, and liquid-fraction profile over the whole solidification process was studied.
As already mentioned, several experiments were carried out to observe the evolution of the solids at different conversion values.
The model describes the GCT unit with all critical design parameters, and predicts the composition of the overflow, underflow and discharge streams and the spatio-temporal evolution of the solids species concentrations inside the unit.
The evolution of the solid-state C NMR spectrum is shown in Figure 3.
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