Factors disturbing a preshaped membrane mirror

Details Factors disturbing a preshaped membrane mirror Factors disturbing a preshaped membrane mirror

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4091..144k&link_type=abstract

Proc. SPIE Vol. 4091, p. 144-151, Imaging Technology and Telescopes, James W. Bilbro; James B. Breckinridge; Richard A. Carreras

Physics

Optics

2

Scientific paper

Today the peak of the conventional method of telescope design is the space telescope named after Hubble (2,4 m-diameter of the primary mirror). Further increase of the input-aperture diameter of telescopes requires the application of new architectures of their design based on the recent progress in optics and the development of super-light mirrors. The paper is devoted to development of the concept of a new-generation membrane primary mirror for extra-atmospheric imaging telescopes basing on the recent progress in non-linear technique of correction for dynamic distortions.

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