Wavefront correction in very large monolithic segmented mirror telescopes.

Details Wavefront correction in very large monolithic segmented mirror telescopes. Wavefront correction in very large monolithic segmented mirror telescopes.

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988vlti....1..479m&link_type=abstract

ESO Conference on Very Large Telescopes and their Instrumentation, Vol. 1, p. 479 - 486

Physics

Optics

Reflectors: Astronomical Optics

Scientific paper

Upgrading optical performance of a very large telescope is potentially an important factor in minimizing time and cost for completion of optical subsystems. Careful protection of the local environment at a telescope will give 0.25 asec FWHM image to the focal plane. In order to match this seeing the specification that must be placed on the optics approaches that for the Hubble Space Telescope.

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