Seeing timescales for large-aperture optical/infrared interferometers from simulations

Computer Science

Scientific paper

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Scientific paper

Numerical simulations of interferometers with spatial filters and large apertures are presented. These simulations are particularly aimed at measuring the fringe (or OPD) motion caused by atmospherically induced wavefront corrugations (high order Zernike modes) across the telescope apertures. This component of the fringe motion results from the coupling in a spatial filter of high-order Zernike modes to the fringe motion. The Piston Mode component is found to be an inadequate approximation to the OPD in an interferometer with large apertures, spatial filters and tip-tilt correction. The fringe motion at

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