We present a full-scale numerical study of thermally induced optical aberrations on the primary mirror of a beam director telescope. In particular, we investigate high-power laser-induced deformations, resulting monochromatic aberrations, and their effects on imaging and laser focusing performance of primary telescope mirrors in shared aperture beam director systems. As a practical example, we consider a system based on 6 × 4 kW single-mode high-power laser sources and a primary mirror having a 500 mm circular clear aperture. A detailed comparison of the monochromatic aberrations and their implications on the optical performance is provided for borosilicate and Zerodur® substrates having identical reflective coatings for potential laser beam director applications. Our analyses show that high-power lasers can be efficiently directed with negligible imaging degradation using athermal substrates (i.e., Zerodur®) with high reflective coatings (>99.9 % ) for primary mirrors. On the other hand, substrates with a relatively higher coefficient of thermal expansion (i.e., borosilicate) can only be used effectively under a strictly controlled ambient temperature.
We provide a unified framework for the evaluation of number of dazzled pixels of camera sensors for free space laser dazzling applications considering laser, beam director, sensor, camera optics and atmosphere parameters. In addition, we present a comparison of our analytical approach to experimental results, where a 1070 nm fiber laser and a CCD based sensor are utilized, for dazzling analysis based on system parameters. This framework can be applied to a variety of free space optical system configurations operating in various optical bands (e.g. UV, SWIR and MWIR) for dazzling performance analysis.
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