Abstract
We formulated a gravity unloading strategy for a monolithic silicon carbide (SiC) mirror with a $\Phi {3}\,\rm m$ aperture in space. Employing the finite element analysis (FEA) technique, a rapid solution analytical approach for determining optimal support forces during gravity unloading is introduced. This method demonstrates enhanced efficiency and accuracy compared to conventional approaches. A quantitative evaluation methodology for the gravity release error, grounded in the minimum-energy mode, is delineated. The adverse impacts could be expeditiously computed by assessing the maximum deflection of minimum-energy modes generated by various errors. The analytical findings revealed that compliance with the stipulated gravity release error criterion of less than 6 nm (root-mean-square) necessitated the gravity unloading force error to fall within the range of $\pm {0.1}\;{\rm N}$. Additionally, the gravity unloading support position error was required to be within $\Phi {0.5}\;{\rm mm}$, and the measurement error pertaining to the rib thickness of the actual mirror blank had to be within $\pm {0.02}\;{\rm mm}$.
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