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For numerical solving of the equations, we assume that the plasma sheath variables vary only in the z-direction.
Solving of the equations revealed that radial, along-track and cross-track velocity changes in the order of 7.9, 0.3 and −1.4 m/s were imparted on the main body due to the fragmentation.
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However, the polynomial blocking approach apparently requires the solving of matrix equations to obtain those matrices A i, B i, i = 0, 1, …, α + 1.
The solution of the system consists of solving the equations of the heat transfer fluid (HTF), the pipe wall and the phase change material (PCM) as one domain.
Otherwise, we may need to solve some of the equations numerically.
The difficulty of solving the equations is one reason why, after being first vindicated in 1919 by observations of "bent" starlight during a solar eclipse, the theory languished for decades.
The result of solving the equations is presented in Fig. 13.
Standard integrators typically lead to numerical growth or decay of energy while solving the equations of motion.
But even if European startups are now free to grow to their full potential, that only solves half of the equation.
The problem of solving the equation (5) is reduced to the problem of solving a equation over R, X^{T},X+hequiv 0,, text{mod} N.
Periodic boundary conditions are assumed in the a, b directions of the supercell in solving the equations of motion.
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