Paper
12 October 2004 Wavelength-agile telescope system with diffractive wavefront control and acousto-optic spectral filter
Mark T. Gruneisen, Raymond C. Dymale, James R. Rotge, Donald L. Lubin, David G. Voelz, Melinda Deramo
Author Affiliations +
Abstract
Programmable diffractive optics (PDO) based on liquid-crystal (LC) technology has been demonstrated as a wavelength-agile means of compensating large aberrations over limited instantaneous spectral bandwidths. Acousto-optic tunable filters (AOTF) based on acousto-optic Bragg diffraction have been demonstrated as wavelength-agile means for selecting narrow spectral bands from white light with high rejection ratios. These technologies are integrated into a telescope system that includes a conventional primary mirror utilized off axis with more than 40 waves of aberration to view a white-light illuminated object bar chart. A high-resolution LC PDO, situated in a pupil plane, compensates for the large primary mirror aberration. The AOTF, operating in an image plane, rejects light outside a 2 nm spectral band centered about the wavelength at which the modulo-lambda phase profile of the PDO is defined. Wavelength-agile operation is achieved by synchronously tuning the PDO and AOTF over a 100nm spectral range. Near-diffraction-limited image quality is demonstrated.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark T. Gruneisen, Raymond C. Dymale, James R. Rotge, Donald L. Lubin, David G. Voelz, and Melinda Deramo "Wavelength-agile telescope system with diffractive wavefront control and acousto-optic spectral filter", Proc. SPIE 5553, Advanced Wavefront Control: Methods, Devices, and Applications II, (12 October 2004); https://doi.org/10.1117/12.561732
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Cited by 3 scholarly publications.
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KEYWORDS
Telescopes

Optical filters

Acousto-optics

Mirrors

Modulation transfer functions

Tunable filters

Wavefronts

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