Speckle imaging of satellite at the U.S. Air Force Maui Optical Station

Physics – Optics

Scientific paper

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Binary Stars, Charge Coupled Devices, Image Reconstruction, Power Spectra, Satellite Imagery, Speckle Interferometry, Autocorrelation, Fourier Transformation, Hubble Space Telescope, Signal To Noise Ratios

Scientific paper

Results are presented from a series of experiments in which the U.S. Air Force Maui Optical Station's 1.6-m telescope and a bare CCD speckle camera system were used to image satellites at distances of up to 1000 km. A brief overview of the image reconstruction algorithms is presented. The choice of the experiment site and various imaging parameters are described. Power spectra and power spectral signal-to-noise ratio curves that result from imaging several point stars are compared with theory. Reconstructed images of several binary stars are shown as a base-line assessment of our technique. High-quality image reconstructions of an earth-satellite, the Hubble Space Telescope, are presented. The results confirm that speckle imaging techniques can be used with a bare CCD imaging system to provide a powerful and flexible method for imaging objects of moderate magnitude.

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