Multi-aperture imaging system

Abstract

A multi-aperture imaging system for continuous dwell imaging of complex extended scenes which are not required to contain localized point sources. The multi-aperture imaging system includes a plurality of subaperture telescopes, each of which collect image data of an instantaneous field of view of an extended object scene within a field of regard of the imaging system. The image data collected by each subaperture telescope is transferred by respective optical delay paths to a beam combiner which combines all the image data in coherent fashion to form a single high resolution image of said object scene at a focal plane of the beam combiner. The subaperture telescopes are optically phased using phase diversity techniques which include using a phase diversity sensor located at the focal plane of the beam combiner to detect wavefront errors in the collected images. A phase controller is used to make phase and tilt adjustments to moveable mirror in the optical delay paths of the respective subaperture telescopes to ensure that the path length travelled by the collected image data from each subaperture telescope is maintained equal. The subaperture telescopes are supported on a deployable Y-shaped framework which folds up for compact stowage within a satellite launch canister. The subaperture telescopes are spaced in a redundant array sufficient to provide a desired uniform coverage of the spatial frequencies of a modulation transfer function (MTF) of the imaging system.