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General Theory of Light Propagation and Imaging Through the Atmosphere

Title
General Theory of Light Propagation and Imaging Through the Atmosphere [electronic resource] / by T. Stewart McKechnie.
ISBN
9783030988289
Edition
2nd ed. 2022.
Publication
Cham : Springer International Publishing : Imprint: Springer, 2022.
Physical Description
1 online resource (XXXV, 678 p.) 213 illus., 105 illus. in color.
Local Notes
Access is available to the Yale community.
Access and use
Access restricted by licensing agreement.
Summary
This 2nd edition lays out an updated version of the general theory of light propagation and imaging through Earth's turbulent atmosphere initially developed in the late '70s and '80s, with additional applications in the areas of laser communications and high-energy laser beam propagation. New material includes a chapter providing a comprehensive mathematical tool set for precisely characterizing image formation with the anticipated Extremely Large Telescopes (ELTS), enabling a staggering range of star image shapes and sizes; existing chapters rewritten or modified so as to supplement the mathematics with clearer physical insight through written and graphical means; a history of the development of present-day understanding of light propagation and imaging through the atmosphere as represented by the general theory described. Beginning with the rudimentary, geometrical-optics based understanding of a century ago, it describes advances made in the 1960s, including the development of the 'Kolmogorov theory,' the deficiencies of which undermined its credibility, but not before it had done enormous damage, such as construction of a generation of underperforming 'light bucket' telescopes. The general theory requires no a priori turbulence assumptions. Instead, it provides means for calculating the turbulence properties directly from readily-measurable properties of star images.
Variant and related titles
Springer ENIN.
Other formats
Printed edition:
Printed edition:
Printed edition:
Format
Books / Online
Language
English
Added to Catalog
October 27, 2022
Series
Progress in Optical Science and Photonics, 20
Progress in Optical Science and Photonics, 20
Contents
Introduction
Terms, Definitions and Theoretical foundations
Diffraction
Wave propagation after scattering by a thin atmospheric layer
Wave propagation over extended atmospheric paths
Properties of point-object im ages formed by telescopes
Properties of point-object im ages formed by telescopes
Average intensity envelopes of unresolved star images
Core and halo structure in star images formed by large telescopes
Statistical properties of stellar speckle patterns
Star image appear ance for small and large average turbulence structure sizes
Approximate intensity envelopes for star images formed by telescopes with/without AO
Telescope optical tolerances and telescope resolution
Laboratory simulation of im ages formed by large telescopes
Laser beam propagation and atmospheric path characterization
Atmospheric isoplanatic angle: Image stabilization and AO image correction.
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