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Proceedings Paper

Four-dimensional computer dynamic model of an atmospheric optical system
Author(s): Vladimir P. Lukin; Boris V. Fortes; Feodor Yu. Kanev; Peter A. Konyaev
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Paper Abstract

A computer code for simulation of high-power beams thermal blooming in the turbulent atmosphere and imaging in a ground- based telescope is described. This code also allows one to simulate the components of adaptive systems, such as the Hartmann-Shack wavefront sensor and various flexible and segmented mirrors. Our software can be used for estimation of beams and images parameters in the atmosphere and for the investigations of adaptive optical system efficiency.

Paper Details

Date Published: 29 June 1994
PDF: 5 pages
Proc. SPIE 2222, Atmospheric Propagation and Remote Sensing III, (29 June 1994); doi: 10.1117/12.178020
Show Author Affiliations
Vladimir P. Lukin, Institute of Atmospheric Optics (Russia)
Boris V. Fortes, Institute of Atmospheric Optics (Russia)
Feodor Yu. Kanev, Institute of Atmospheric Optics (Russia)
Peter A. Konyaev, Institute of Atmospheric Optics (Russia)


Published in SPIE Proceedings Vol. 2222:
Atmospheric Propagation and Remote Sensing III
Walter A. Flood; Walter B. Miller, Editor(s)

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