Friday, October 28, 2011
Hall 1-2 (San Jose Convention Center)
Due to the spatial resolution limits of current satellite-tracking systems, successful imaging of satellites within a geostationary earth orbit (GEO) has never knowingly been performed. The scenario of a malfunctioning GEO satellite, prompting a long costly damage assessment, could be mitigated by a visual assessment of the satellite. Shadow imaging proposes an inexpensive solution to this problem by capturing the diffraction pattern created from a satellite occultation. When a satellite passes between the Earth and a specific star, a shadow of the satellite can be observed from Earth in the form of a diffraction pattern. By utilizing an array of inexpensive mobile telescopes(14”) equipped with rapid readout photon counting detectors, the diffraction pattern created by a satellites occultation can be captured. The diffracted silhouette of the satellite can then be processed in an algorithm which corrects for diffraction to produce a high resolution silhouette of the satellite.