Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4994
Title: Speckle Imaging: a boon for astronomical observations
Authors: Saha, S. K
Keywords: Speckle Imaging
Photographic Technique
Isoplanatic Patch
Telescope Aberrations
Atmospheric Turbulence
Effect on Flat Wavefront
Stellar Source
Earth’s Atmosphere
Speckle Interferometric Technique
Conventional Imaging
Basic Fourier Optics
Issue Date: 2003
Publisher: Centre for Space Physics
Citation: S K Chakrabarti, S B Das, B Basu. and M. Khan., eds., Recent Trends in Astro and Plasma Physics in India., pp. 223 - 238
Abstract: The speckle imaging is a photographic technique that resolves objects viewed through severely distorted media. The results are insensitive to the errors caused by apparent size of the isoplanatic patch and the telescope aberrations. In this article, a short descriptions of the atmospheric turbulence and its effect on the flat wavefront from a stellar source is presented; the shortcomings of the conventional long-exposure images in the presence of Earth’s atmosphere are discussed. The advantages of the speckle interferometric technique over conventional imaging are enumerated. The technical details of the method, basic Fourier optics, data analysis procedures are also described.
URI: http://hdl.handle.net/2248/4994
Appears in Collections:IIAP Publications

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