By Robert Tyson

ISBN-10: 0824782755

ISBN-13: 9780824782757

This instruction manual offers analytical instruments for the layout and improvement of adaptive optics platforms to reinforce their skill to regulate for atmospheric turbulence, optical fabrication mistakes, thermally brought on distortions, and laser gadget aberrations. It presents suggestions for choosing, checking out and fitting a wavefront reimbursement system.

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R. P. Angel, D. G. Sandler, T. K. Barrett, P. C. McGuire, T. A. Rhoadarmer, D. G. Bruns. S. M. Miller, D. W. McGarthy, M. Cheselka, Proc. SPIE 3353, 82 (1998). T. R. Rimmele, R. R. , Proc. SPIE 3353, 72 (1998). D. S. Acton, P. L. Wizinowich, P. J. Stomski, J. C. Shelton, 0. Lai, J . M. Brase, Proc. SPlE 3353, 125 (1998). E. J. Kibblewhite, M. R. Chun, J. E. Larkin, V. Scor, F. Shi, M. F. Smutko, W. J. Wild, Proc. SPIE 3353, 60 (1998). L. K. Saddlemyer, G. -P. Veran, J. M. Fletcher. Proc. SPIE 3353, 150 ( 1998).

And Proc. 48, European Southern Observatory, Garching bei Munchen, Germany ( 1994), p. 535. J. W. Hardy, Sci. , June (1994), p. 60 D. L. Fried, J. Opt. Soc. Am. 56, 1380 (1966). D. P. Greenwood, J. Opt. Soc. Am. 67, 390 (1977). G. A. Tyler, J. Opt. Soc. Am. A, 1, 251 (1984). V. P. Lukin, Atmospheric Adaptive Optics, SPIE Opt. Engr. Press, Bellingham, WA, 1995. R. Foy, A. Labeyrie, Astron. Astrophys. 152, L29 ( I 985). R. A. , San Jose, CA, Paper FH2, 1991. R. Q. Fugate, D. L. Fried, G. A. Ameer, B.

San Diego, CA). 6 electrons read noise operating at 390 kHz. The wavefront control computer uses Texas Instruments TMS320C40 DSPs for slope processors and matrix multipliers. 73-11s pulse length. The laser will be upgraded to a doubled Raman-shifted fiber laser to operate CW at 10 W. J. National Solar Observatory The National Solar Observatory, Sacrament0 Peak, NM, experimented with adaptive optics on the 76-cm vacuum tower telescope (VTT) in I99 1. The early system used a Lockheed segmented deformable mirror and a Shack-Hartmann WFS based on an array of quad-cell detectors.

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