Based on the Hartmann testing principle, this paper proposes a novel image quality testing technology which applies to a large-aperture space optical system. Compared with the traditional testing method through a large-aperture collimator, the scanning Hartmann testing technology has great advantages due to its simple structure, low cost, and ability to perform wavefront measurement of an optical system. The basic testing principle of the scanning Hartmann testing technology, data processing method, and simulation process are presented in this paper. Certain simulation results are also given to verify the feasibility of this technology. Furthermore, a measuring system is developed to conduct a wavefront measurement experiment for a 200 mm aperture optical system. The small deviation (6.3%) of root mean square (RMS) between experimental results and interferometric results indicates that the testing system can measure low-order aberration correctly, which means that the scanning Hartmann testing technology has the ability to test the imaging quality of a large-aperture space optical system.
© 2017 Optical Society of AmericaFull Article | PDF Article
OSA Recommended Articles
Steven C. West, Samuel H. Bailey, James H. Burge, Brian Cuerden, Jeff Hagen, Hubert M. Martin, and Michael T. Tuell
Appl. Opt. 49(18) 3522-3537 (2010)
J. Opt. Soc. Am. A 35(10) 1717-1729 (2018)
Isaac Trumper, Pascal Hallibert, Jonathan W. Arenberg, Hideyo Kunieda, Olivier Guyon, H. Philip Stahl, and Dae Wook Kim
Adv. Opt. Photon. 10(3) 644-702 (2018)