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Periodical
Atmospheric and oceanic optics.
Authors: --- ---
ISSN: 20700393 10248560 Year: 1992 Publisher: Tomsk : Institute of Atmospheric Optics

Physics of the aurora and airglow
Author:
ISBN: 1118668049 1283525569 0080954405 0875908578 9780080954400 9781118668047 9780875908571 Year: 1995 Publisher: Washington, D.C. American Geophysical Union

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Abstract

For advanced undergraduate and beginning graduate students in atmospheric, oceanic, and climate science, Atmosphere, Ocean and Climate Dynamics is an introductory textbook on the circulations of the atmosphere and ocean and their interaction, with an emphasis on global scales. It will give students a good grasp of what the atmosphere and oceans look like on the large-scale and why they look that way. The role of the oceans in climate and paleoclimate is also discussed.


Book
The Monte Carlo methods in atmospheric optics
Author:
ISBN: 0387094024 3540094024 9780387094021 9783540094029 3662135035 3540352376 Year: 1980 Volume: 12 Publisher: Berlin : Springer-Verlag,


Book
General Theory of Light Propagation and Imaging Through the Atmosphere
Author:
ISBN: 3319182080 3319182099 Year: 2016 Publisher: Cham : Springer International Publishing : Imprint: Springer,

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Abstract

This book lays out a new, general theory of light propagation and imaging through Earth’s turbulent atmosphere. Current theory is based on the – now widely doubted – assumption of Kolmogorov turbulence. The new theory is based on a generalized atmosphere, the turbulence characteristics of which can be established, as needed, from readily measurable properties of point-object, or star, images. The pessimistic resolution predictions of Kolmogorov theory led to lax optical tolerance prescriptions for large ground-based astronomical telescopes which were widely adhered to in the 1970s and 1980s. Around 1990, however, it became clear that much better resolution was actually possible, and Kolmogorov tolerance prescriptions were promptly abandoned. Most large telescopes built before 1990 have had their optics upgraded (e.g., the UKIRT instrument) and now achieve, without adaptive optics (AO), almost an order of magnitude better resolution than before. As well as providing a more comprehensive and precise understanding of imaging through the atmosphere with large telescopes (both with and without AO), the new general theory also finds applications in the areas of laser communications and high-energy laser beam propagation.

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