Fine-resolution astronomical imaging with phase-diverse speckle

Richard G. Paxman; John H. Seldin

doi:10.1117/12.162007

9 November 1993 Fine-resolution astronomical imaging with phase-diverse speckle

Richard G. Paxman, John H. Seldin

Proceedings Volume 2029, Digital Image Recovery and Synthesis II; (1993) https://doi.org/10.1117/12.162007
Event: SPIE's 1993 International Symposium on Optics, Imaging, and Instrumentation, 1993, San Diego, CA, United States

Abstract

Phase-diverse speckle imaging is a novel post-detection correction technique for use in imaging through atmospheric turbulence. When the wavelength dependence is introduced, the data-collection model and problem statement are seen to accommodate a variety of existing and proposed data-collection schemes, including speckle imaging, multi-frame blind deconvolution, deconvolution with wavefront sensing, and hybrid adaptive optics.

Citation Download Citation

Richard G. Paxman and John H. Seldin "Fine-resolution astronomical imaging with phase-diverse speckle", Proc. SPIE 2029, Digital Image Recovery and Synthesis II, (9 November 1993); https://doi.org/10.1117/12.162007

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