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Thus, the elastic constants could be determined by dispersion (velocity) and the viscous constants by an attenuation curve.
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We introduce a new dispersion-velocity particle method for approximating solutions of linear and nonlinear dispersive equations.
The main analytical result we provide is the short time existence and uniqueness of a solution to the resulting dispersion-velocity transport equation.
In addition, the calculation of the solar motion provides dispersion in velocity.
Fibers: single- and multi-mode, attenuation, modal dispersion, group-velocity dispersion, polarization-mode dispersion.
In a fatigued muscle, when membrane propagation is slowing, the SD-PV will broaden as a result of the temporal dispersion of velocities.
Linear pore velocities, dispersion coefficients, and dispersivity values were spatially determined at the downstream end of the core samples.
Recent determinations of solar motion from high-dispersion radial velocities have suggested that most previous K-terms (which averaged a few kilometres per second) were the result of systematic errors in stellar spectra caused by blends of spectral lines.
We determined experimentally the attenuation and velocity dispersion induced by scattering from the synthetic seismograms, using a waveform averaging technique.
We experimentally determine the attenuation and velocity dispersion induced by scattering from the synthetic seismograms, using a waveform averaging technique.
Velocity dispersion is a statistical measure of the range of velocities of all stars in a galaxy, easily obtainable with a spectrograph.
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