Presentation + Paper
3 October 2022 Tailoring the stiffness of large mirrors to reduce specific optical aberrations
Christopher L. Hopkins
Author Affiliations +
Abstract
Presented is a method that tailors the geometry of a mirror’s core structure as well as the mounting interface such that a desired set of aberrations is reduced. It will be shown that targeting specific aberrations as opposed to reducing overall surface figure error (SFE) is a valid method to reduce weight or improve performance. Analyzed first is the self-weight deflection of a thin circular plate of uniform thickness continuously supported along its outer edge. The Kirchhoff-Love plate bending equations are related to the radially symmetric Zernike polynomials of piston, defocus, and primary spherical aberration. Next, the mirror’s radial thickness is optimized to eliminate primary and secondary spherical aberrations when the outer edge is simply supported. As an example, the method is demonstrated using a 2-meter diameter aluminum mirror where surface deflections can have an appreciable effect at mid-to-near infrared wavelengths.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christopher L. Hopkins "Tailoring the stiffness of large mirrors to reduce specific optical aberrations", Proc. SPIE 12215, Optical Modeling and Performance Predictions XII, 1221509 (3 October 2022); https://doi.org/10.1117/12.2636038
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Monochromatic aberrations

Finite element methods

Optical aberrations

Aluminum

Telescopes

MATLAB

Back to Top