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The model only requires one material parameter and two geometrical parameters to be determined from experiments.
Coarsening models allow both equilibrium phase compositions to be determined from the compositional measurements.
The composition of primary Cosmic Rays at > 100 TeV has to be determined from indirect experiments.
This allows the time-dependent acoustic source to be determined from Powell's vortex sound theory.
Only the damping coefficients for different plates need to be determined from experiments.
The extrapolation allows the full work of fracture to be determined, from which the fracture energy may be obtained.
These models are often unknown in the early design phase and need to be determined from laboratory experiments.
X-ray crystallography permits the detailed spatial location of each atom to be determined from a diffraction pattern.
This approach allows the excess energy of non-equilibrium grain boundaries to be determined from diffusion measurements.
Furthermore, the coefficients of the model need to be determined from some known data set (training set).
The results enable the real and imaginary parts of the shear parameter to be determined from experimental data.
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