16 September 2004 Low-cost active optics for 2.1 m at San Pedro Martir: computer simulations
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The support system of the primary mirror of 2.1m telescope at SPM allows correction of some optical aberrations. A low cost Active Optics System (AOS) can be developed based on this property of the support system. Within the preliminary development of this system, computer simulations were being performed. The general propose of simulations was to find the optimal scheme for the wavefront control of the primary mirror. This paper presents results for the wavefront sensor of the AOS proposed for the 2.1m telescope at San Pedro Martir.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Valeri Orlov, Valeri Orlov, Esteban Luna, Esteban Luna, Evguenia Orlova, Evguenia Orlova, } "Low-cost active optics for 2.1 m at San Pedro Martir: computer simulations", Proc. SPIE 5497, Modeling and Systems Engineering for Astronomy, (16 September 2004); doi: 10.1117/12.550615; https://doi.org/10.1117/12.550615


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