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Off-axis Two-mirror System with Wide Field of View Based on Diffractive Mirror
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 Title & Authors
Off-axis Two-mirror System with Wide Field of View Based on Diffractive Mirror
Meng, Qingyu; Dong, Jihong; Wang, Dong; Liang, Wenjing;
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An unobstructed off-axis two-mirror system is presented in this paper. First a suitable initial configuration is established based on third-order aberration theory. In order to achieve a wide field of view (FOV) with high image quality , the diffractive mirror is adopted in the two-mirror system to increase the optimization freedom and the aberration relationship between diffractive phase coefficients and Zernike coefficients is derived. Furthermore, a complete comparison design example with a focal length of 1200 mm, F-number of 12, and FOV of 40° × 2° is given to verify the aberration correction ability of the diffractive mirror. The system average wavefront error is 0.007 λ (λ
Optical systems;Optical design;Aberrations;Diffractive optics;Remote sensing;
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T. V. Viard, “COROT TELESCOPE(COROTEL),” in Proc. 6th Internet Conference on Space Optics (Noordwijk, The Netherlands, June 2006), 42.1-42.6.

J. M. Sasian, “Design of a Schwarzschild flat-field, anastigmatic, unobstructed, wide-field telescope,” Opt. Eng. 29, 1-5 (1990). crossref(new window)

J. Liu, F. Long, W. Zhang, and Z. Wang, “Optical design of a flat field unobstructed two-mirror system with wide field of view,” Acta Photonica Sinica 34, 1351-1354 (2005).

Q. Meng, W. Wang, H. Ma, and J. Dong, “Easy-aligned off-axis three-mirror system with wide field of view using freeform surface based on integration of primary and tertiary mirror,” Appl. Opt. 53, 3028-3034 (2014). crossref(new window)

J. X. Sun, Q. Sun, D. X. Li, and Z. W. Lu, “Conformal dome aberration correction with diffractive elements,” Acta Phys. Sin. 56, 3900-3905 (2007).

T. Schmid, K. P. Thompson, and J. P. Rolland, “Misalignment-induced nodal aberration fields in two-mirror astronomical telescopes,” Appl. Opt. 49, D131-D144 (2010). crossref(new window)

M. L. Lampton, M. J. Sholl, and M. E. Levi, “Off-axis telescopes for dark energy investigations,” Proc. SPIE 7731, 77311G-1~77311G-11 (2010).

V. N. Mahajan, Optical Imaging and Aberrations: Part 1. Ray Geometrical Optics (SPIE, Washington, USA, 1998), Chapter 4.

J. Pan, The Design, Manufacture and Test of the Aspherical Optical Surfaces (SuZhou University, SuZhou, China, 2004), Chapter 3.

D. A. Buralli and G. M. Morris, “Design of a wide field diffractive landscape lens,” Appl. Opt. 28, 3950-3959 (1989). crossref(new window)

D. Malacara, Optical Shop Testing, 3rd ed. (China Machine Press, Beijing, China, 2012), Chapter 9.

A. D. Kathman and S. K. Pitalo, “Binary optics in lens design,” in Proc. International Lens Design Conference (Monterey, USA, Jan. 1990), pp. 297-309.

CODE V Reference Manual, ORA (Optical Research Associates).

S. I. Barnes, P. L. Cottrell, M. D. Albrow, N. Frost, G. Graham, G. Kershaw, R. Ritchie, D. Jones, R. Sharples, D. Bramall, J. Schmoll, P. Luke, P. Clark, L. Tyas, D. A. H. Buckley, and J. Brink, “The optical design of the Southern African Large Telescope High Resolution Spectrograph: SALT HRS,” Proc. SPIE 7014, 70140K-1~70140K-12 (2008).

M. R. Haas, “Optical design and diffraction analysis for AIRES: an airborne infrared Echelle spectometer,” Proc. SPIE 4857, 85-96 (2003).

J. Qiao, A. Kalb, and M. J. Guardalben, “Large-aperture grating tiling by interferometry for petawatt chirped-pulse-amplification systems,” Opt. Express 15, 9562-9574 (2007). crossref(new window)

L. Shi, “Fabrication of large-size diffraction gratings: Latent-image-based optical mosaic technique,” Doctoral Dissertation, Tsinghua University (2011).

H. P. Herzig, Micro-Optics Elements, System and Applications (Taylor & Francis Ltd., London, UK, 1997), Chapter 2.

S. Kristof, K. Jens, S. Danilo, and L. Hubert, “Distortion correction of all-reflective unobscured optical-power zoom objective,” Appl. Opt. 49, 2712-2719 (2010). crossref(new window)

T. H. Ebben, J. Bergstrom, P. Spuhler, A. Delamere, and D. Gallagher, “Mission to Mars: the HiRISE camera on-board MRO,” Proc. SPIE 6690, 66900B-1~66900B-22 C.

A. S. McEwen, E. M. Eliason, J. W. Bergstrom, N. T. Bridges, C. J. Hansen, W. A. Delamere, J. A. Grant, V. C. Gulick, K. E. Herkenhoff, L. Keszthelyi, R. L. Kirk, M. T. Mellon, S. W. Squyres, N. Thomas, and C. M. Weitz, “Mars reconnaissance orbiter’s High Resolution Imaging Science Experiment (HiRISE),” Journal of Geophysical Research 112, E05S02 (2007).