Abstract
This paper describes new optical correctors which are phase conjugated to a mirror and allow, in most cases, a residual distorsion of the outgoing wave front as low as λ/40 (16 nm) peak to peak. Such a high resolution system is possible with Deep U.V. photoresist correctors registered at 257 nm in a diverging Michelson-Twyman interferometer directly by the mirror to be corrected itself, without any intermediary steps. Some results obtained with this technique are given. They show the potential interest of this method for optical imaging system in space involving large mirror and/or Ultraviolet imaging.
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BAHCALL, J.N. and SPITZER Jr., L.: 1982, The Space Telescope, Sci. Am. 247, 38
DAME, L., BONNET, R.M. and ARTZNER, G.E.: On the possible use of Deep U.V. Photoresists correctors to obtain the ultimate U.V. Resolution of Space Borne Telescopes, Proc. SPIE 446, to be published
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DAME, L. and VAKILI, F.: 1984, The Ultra Violet Resolution of Large Mirrors via Hartmann Tests and Two Dimensionnal Fast Fourrier Transform analysis, Opt. Eng., to be published (Nov/Dec 1984 issue)
ROBINSON, L.J.: An eye for tomorrow, Sky and Telescope 63, 1982
WETHERELL, W.B.: 1982, The effects of mirror surface ripple on image quality, Proc. SPIE 332
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© 1985 Springer-Verlag
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Dame, L., Decaudin, M. (1985). Hundredths of arcsec resolutions with new optical correctors on deep u.v. photoresist. In: Muller, R. (eds) High Resolution in Solar Physics. Lecture Notes in Physics, vol 233. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0022405
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DOI: https://doi.org/10.1007/BFb0022405
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