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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 38, Iss. 7 — Mar. 1, 1999
  • pp: 1096–1102

Theory and computation of three Cosmic Origin Spectrograph aspheric gratings recorded with a multimode deformable mirror

Michel Duban  »View Author Affiliations


Applied Optics, Vol. 38, Issue 7, pp. 1096-1102 (1999)
http://dx.doi.org/10.1364/AO.38.001096


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Abstract

The theory of three Cosmic Origin Spectrograph holographic gratings recorded with a deformable plane mirror is presented. Their working conditions are severe, since they have to correct the strong spherical aberration and the field astigmatism of the Hubble Space Telescope. Recorded on aspherized substrates, the gratings produce images that are diffraction limited with regard to spectral resolution.

© 1999 Optical Society of America

OCIS Codes
(050.7330) Diffraction and gratings : Volume gratings
(230.4040) Optical devices : Mirrors

History
Original Manuscript: July 9, 1998
Revised Manuscript: October 27, 1998
Published: March 1, 1999

Citation
Michel Duban, "Theory and computation of three Cosmic Origin Spectrograph aspheric gratings recorded with a multimode deformable mirror," Appl. Opt. 38, 1096-1102 (1999)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-38-7-1096


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References

  1. J. C. Green, “HST Cosmic Origins Spectrograph: replacement instrument for the 2002 reservicing mission,” in Space Telescope and Instruments V, P. Y. Bely, B. Breckinridge, eds., Proc. SPIE3356, 265–270 (1998). [CrossRef]
  2. J. A. Morse, J. C. Green, “Performance and science goals of the Cosmic Origins Spectrograph for HST,” in Space Telescope and Instruments V, P. Y. Bely, B. Breckinridge, eds., Proc. SPIE3356, 361–368 (1998). [CrossRef]
  3. J. C. Green, “The Cosmic Origin Spectrograph,” (Colorado University, Boulder, Colo., 1997), pp. 97–752.
  4. M. Duban, K. Dohlen, G. R. Lemaı̂tre, “Illustration of the use of multimode deformable plane mirrors to record high-resolution concave gratings: results for the Cosmic Origins Spectrograph gratings of the Hubble Space Telescope,” Appl. Opt. 37, 7214–7217.
  5. G. R. Lemaı̂tre, M. Wang, “Active mirrors warpedusing Clebsch–Zernike polynomials for correcting off-axisaberrations,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).
  6. M. Duban, G. R. Lemaı̂tre, R. F. Malina, “Recording method for obtaining high-resolution holographic gratings through use of multimode deformable plane mirrors,” Appl. Opt. 37, 3438–3439 (1998). [CrossRef]
  7. M. Duban, “Holographic aspheric gratings printed with aberrant waves,” Appl. Opt. 26, 4263–4273 (1987). [CrossRef] [PubMed]
  8. M. Duban, “Third-generation Rowland holographic mounting,” Appl. Opt. 30, 4019–4025 (1991). [CrossRef] [PubMed]
  9. M. Duban, “Theory of spherical holographic gratings recorded by use of a multimode deformable mirror,” Appl. Opt. 37, 7209–7213.

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