1 August 2002 Large sparse aperture space optical systems
Aden B. Meinel, Marjorie P. Meinel
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The issue of how best to distribute a large optical collecting area is revisited, including the added integration time required for a scene imaged by sparse-aperture configurations to be processed to equal that of a filled aperture, and also its influence on system architecture. The optical performance of three sparse-aperture configurations arising from a 1998 study is presented as a function of field angle and optimization criteria. Optimization of these three specific configurations shows ray FWHM and residual rms values small enough to assure excellent diffraction-limited imagery. Practical issues concerning fabrication, assembly, testing, and on-orbit phasing are identified.
©(2002) Society of Photo-Optical Instrumentation Engineers (SPIE)
Aden B. Meinel and Marjorie P. Meinel "Large sparse aperture space optical systems," Optical Engineering 41(8), (1 August 2002). https://doi.org/10.1117/1.1490557
Published: 1 August 2002
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Cited by 26 scholarly publications.
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KEYWORDS
Space telescopes

Telescopes

Mirrors

Diffraction

Monochromatic aberrations

Collimation

Astronomical imaging

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