Titlebook: General Theory of Light Propagation and Imaging Through the Atmosphere; T. Stewart McKechnie Book 20161st edition Springer International P

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https://doi.org/10.1007/978-3-642-22432-4h properties identical to those of actual images obtained by large telescopes in the field. The imaging optic used in the simulator—typically 5 mm in diameter—is designed to provide a suitably scaled replica of the telescope point-spread function. Scaling procedures are also described for designing

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Introduction,h include dimensional inconsistences and image predictions at odds with observed characteristics. Around 1990, it became clear to astronomers that much better resolution was possible from ground-based telescopes and the lax optical tolerances prescribed by this theory were promptly abandoned. Yet, i

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Wave Propagation After Scattering by a Thin Atmospheric Layer,al) thin inhomogeneous atmospheric layer. The propagation behavior is examined in the near-field Fresnel space beyond the layer which, at this preliminary stage, we consider homogeneous free space. The behavior of the crucially important, two-point two-wavelength correlation function of the complex

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