System wavefront correction using a complex aspheric mirror

Details System wavefront correction using a complex aspheric mirror System wavefront correction using a complex aspheric mirror

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004spie.5533..108k&link_type=abstract

Advances in Mirror Technology for X-Ray, EUV Lithography, Laser, and Other Applications II. Edited by Khounsary, Ali M.; Dinger,

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A hardware demonstration has been performed in which a nominally flat, complex aspheric mirror is used to correct the high-order aberrated wavefront error of an off-axis parabolic mirror to 0.5 nm rms. The purpose of the project is to demonstrate the viability of using a static, aspheric optic to correct a telescope wavefront to the degree needed for detection of extra-solar Jovian planets. The demonstration procedure and test results are presented.

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