Velocity interferometer system for any reflector

Velocity interferometer system for any reflector (VISAR) is a time-resolved velocity measurement system that uses laser interferometry to measure the surface velocity of solids moving at high speeds. For solids experiencing high velocity impact or explosive conditions, VISAR plots the free-surface velocity against time to show the shock wave profile of a material (See Figure). VISAR is a useful tool in determining the pressure-density relationship of a material known as the Rankine-Hugoniot conditions or simply the 'Hugoniot'. Velocity interferometer system for any reflector (VISAR) is a time-resolved velocity measurement system that uses laser interferometry to measure the surface velocity of solids moving at high speeds. For solids experiencing high velocity impact or explosive conditions, VISAR plots the free-surface velocity against time to show the shock wave profile of a material (See Figure). VISAR is a useful tool in determining the pressure-density relationship of a material known as the Rankine-Hugoniot conditions or simply the 'Hugoniot'. In recent years another time-resolved velocity measurement tool called laser Doppler velocimetry has achieved popularity in the shock physics community as an adjunct or replacement for VISAR. This device is essentially a Displacement interferometer of the normal Michelson variety. As such it requires extremely fast data acquisition devices (digital oscilloscopes with bandwidths of 10GHz or higher) and is limited in the range of velocities it can cover. As the surface moves, the reflected light interferes with itself and sinusoidal 'fringes' in light intensity are produced and recorded. A cycle of light intensity or fringe count indicates a displacement of the surface corresponding to one wavelength of the light. The rate at which these fringes occur is thus proportional to the velocity of the surface. To derive a velocity history the fringe (displacement) data must be differentiated with respect to time, usually by Fourier Analysis. This differentiation or FA step inevitably reduces the time resolution and accuracy of the velocity history. The VISAR on the other hand is configured to 'optically differentiate' so that the light intensity variation due to interference varies sinusoidally with the velocity of the surface not the displacement. Also called a 'Delay-Leg Interferometer,' it is an extremely clever device and remains the best and most accurate method for recording the velocity history of fast moving surfaces.

[ "Astronomical interferometer" ]
Parent Topic
Child Topic
    No Parent Topic