A step-by-step model for active telescope systems

Details A step-by-step model for active telescope systems A step-by-step model for active telescope systems

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1114...84z&link_type=abstract

IN: Active telescope systems; Proceedings of the Meeting, Orlando, FL, Mar. 28-31, 1989 (A90-30852 12-74). Bellingham, WA, Socie

Physics

Optics

Atmospheric Correction, Optical Transfer Function, Telescopes, Wave Front Deformation, Atmospheric Optics, Digital Computers, Error Correcting Codes, Error Detection Codes

Scientific paper

The 'step-by-step' model presently developed for the study of adaptive telescopic optics system performance capitalizes on the finite time required for a wavefront-compensation system to successively complete wavefront detection, correction-command generation, and corrector-response procedures. The statistical optical transfer function of a wavefront-compensation system is evaluated on the basis of the step-by-step model. This function is associated with the structural function of the compensated wavefront; this in turn is related to detection error, corrector-setting errors, and the atmosphere's spatial response function.

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