Abstract
Single-iteration multigrid (SIMG) wavefront reconstruction schemes were implemented and validated on the adaptive optics system at the Hale 5.1 m telescope at the Palomar Observatory. Results indicate that even the simplest such method produces a performance indistinguishable from that of the standard least-squares reconstructor for both bright and dim guide stars. SIMG provides a dramatic reduction in computational cost when compared to vector-matrix multiplication and can be implemented in parallel, making it the obvious choice for reconstruction in future large-scale adaptive optics systems.
Original language | English (US) |
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Pages (from-to) | 2047-2049 |
Number of pages | 3 |
Journal | Optics Letters |
Volume | 33 |
Issue number | 18 |
DOIs | |
State | Published - Sep 15 2008 |
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics