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In addition, numerical acceleration excitation thresholds and basins of attraction are provided to investigate the potential for energy harvesting performance enhancement using the suitable equilibrium positions, appropriate initial conditions or external disturbances, due to high-energy interwell oscillations in the multi-solution ranges.
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The first four numerical responses for acceleration, velocity and displacement are presented.
In addition, the effects of the string's initial velocity are examined, a stability analysis is carried out, and a series of numerical simulations of acceleration waves on a finite string are presented.
The static displacements are calculated by double numerical integration after removing acceleration steps from the acceleration signals.
The velocity distribution is then obtained through a numerical integration of the acceleration over time.
By regarding SFT as an elastic-plastic vibrating system and inputting seismic acceleration records, numerical simulation results are obtained.
The parameters a and tO are determined from a linearly-increasing velocity signal calculated by numerical integration of the acceleration signal.
The ability to prescribe de- sired initial conditions for computational -and, in this case, also possibly for laboratory- experiments provides an interesting link between traditional, matrix-free numerical analysis and the acceleration of dynamic studies.
We review here recent numerical results concerning the acceleration and collimation of relativistic outflows from neutron stars, and we discuss their implications for models of magnetars in their hypothesized initial high rotation states.
We used the photogrammetric method described above to measure the position of blowflies, and then followed the usual approach of determining velocity and acceleration by numerical differencing.
An error function is defined as the time integral of the least-squared errors between measured accelerations and calculated accelerations by a numerical model of a structure.
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