Paper
30 January 2004 Application of a large space-based diffractive optical element telescope to the Terrestrial Planet-Finder mission: design and tolerance issues
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Abstract
An analytical description of the scattered light from a 10 meter diameter Diffractive Optical Element lens-based telescope operating at 1 micron wavelength has been formulated. The specifics of the grating and blaze as well as physical manufacturing constraints were made a part of the problem to be solved. A major simplifying approximation made is that a 1 dimensional lens was assumed for the calculations. This simplified model still serves to illustrate the important effects and limitations of a high performance lens used as a telescope. Focal plane light scattering has been rigorously determined for simplified cases.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel J. Hoppe, Richard L. Baron, and Thomas A. Cwik "Application of a large space-based diffractive optical element telescope to the Terrestrial Planet-Finder mission: design and tolerance issues", Proc. SPIE 5166, UV/Optical/IR Space Telescopes: Innovative Technologies and Concepts, (30 January 2004); https://doi.org/10.1117/12.506531
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Cited by 1 scholarly publication.
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KEYWORDS
Point spread functions

Light scattering

Tolerancing

Diffraction

Space telescopes

Planets

Telescopes

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