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Proceedings Paper

Fabrication Experiments On Supersmooth Optics For Extrasolar Planet Detection
Author(s): C. Ftaclas; M. H. Krim; R. J. Terrile
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Paper Abstract

The direct detection of extrasolar planets .by imaging will require reductions in scattered and diffracted light by factors in excess of 103 within one arcsecond of a bright source. While diffraction can be reduced by a number of approaches, small angle scatter can only be reduced by controlling mid-spatial frequency figure errors. We review the surface requirements and consider their meaning when compared to the data base of existing mirrors. We describe experiments that were successful in reducing mid-spatial frequency figure so that the scatter level was 500 times less than diffraction for a 25 cm spherical mirror.

Paper Details

Date Published: 11 October 1989
PDF: 9 pages
Proc. SPIE 1113, Reflective Optics II, (11 October 1989); doi: 10.1117/12.955572
Show Author Affiliations
C. Ftaclas, Perkin-Elmer (United States)
M. H. Krim, Perkin-Elmer (United States)
R. J. Terrile, California Institute of Technology (United States)

Published in SPIE Proceedings Vol. 1113:
Reflective Optics II
Dietrich G. Korsch, Editor(s)

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