Sparse matrix wave-front estimators for adaptive-optics systems for large ground-based telescopes

Details Sparse matrix wave-front estimators for adaptive-optics systems for large ground-based telescopes Sparse matrix wave-front estimators for adaptive-optics systems for large ground-based telescopes

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995optl...20..955w&link_type=abstract

Optics Letters, Volume 20, Issue 9, May 1, 1995, pp.955-957

Physics

Optics

14

Adaptive Optics, Telescopes, Matrices

Scientific paper

A closed-loop adaptive-optics servo system is an iterative
optical-digital processor that can be characterized by a first-order
difference equation. This identification leads to a new class of
wave-front estimators, some of which are extremely sparse and permit
real-time subaperture intensity weighting.

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