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7 September 2013The optical performance test of lightweight primary mirror of space Cassegrain telescope
The Remote sensing instrument ( RSI ) under developing is a Cassegrain telescope with clear aperture of 450 mm. In
order to meet specifications for thermal distortion, self-weight deformation of the mirror and weight budget of the system,
the primary mirror has been lightweighted at the ratio about 50 % with hexagon cell structures from a Zerodur blank. For
this mid-large lightweight mirror, the optical performance test is challenging during both the manufacture and assembly
phases. While in the optical measurement, there are some unexpected errors caused erroneous judgments for the mirror
induced by the external force or environmental deviation. For example, it’s difficult to specify the measured astigmatism
caused from the form error after polishing or surface deformation by the external force from the supporter or mechanical
mount. In this paper, the optical performance test called bench test to get the absolute measurement result for the
lightweight mirror is presented. After measurement, a novel algorithm is adopted to analyze the astigmatism caused from
the gravity effect and form error from manufacture and the deformation from the mounting or supporter. Also, the
measurements with different supporter compared with vertical and horizontal setup are compared in the end of this
article.
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Wei-Cheng Lin, Shenq-Tsong Chang, Ting-Ming Huang, Ming-Ying Hsu, Yu-Chuan Lin, "The optical performance test of lightweight primary mirror of space Cassegrain telescope," Proc. SPIE 8838, Optical Manufacturing and Testing X, 883812 (7 September 2013); https://doi.org/10.1117/12.2024246