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Title: Large aperture Fresnel telescopes/011

Abstract

At Livermore we`ve spent the last two years examining an alternative approach towards very large aperture (VLA) telescopes, one based upon transmissive Fresnel lenses rather than on mirrors. Fresnel lenses are attractive for VLA telescopes because they are launchable (lightweight, packagable, and deployable) and because they virtually eliminate the traditional, very tight, surface shape requirements faced by reflecting telescopes. Their (potentially severe) optical drawback, a very narrow spectral bandwidth, can be eliminated by use of a second (much smaller) chromatically-correcting Fresnel element. This enables Fresnel VLA telescopes to provide either single band ({Delta}{lambda}/{lambda} {approximately} 0.1), multiple band, or continuous spectral coverage. Building and fielding such large Fresnel lenses will present a significant challenge, but one which appears, with effort, to be solvable.

Authors:
Publication Date:
Research Org.:
Lawrence Livermore National Lab., CA (United States)
Sponsoring Org.:
USDOE, Washington, DC (United States)
OSTI Identifier:
304513
Report Number(s):
UCRL-ID-131320
R&D Project: 97-ERD-060; ON: DE98058780; BR: YN0100000
DOE Contract Number:
W-7405-ENG-48
Resource Type:
Technical Report
Resource Relation:
Other Information: PBD: 16 Jul 1998
Country of Publication:
United States
Language:
English
Subject:
44 INSTRUMENTATION, INCLUDING NUCLEAR AND PARTICLE DETECTORS; TELESCOPES; FRESNEL LENS

Citation Formats

Hyde, R.A., LLNL. Large aperture Fresnel telescopes/011. United States: N. p., 1998. Web. doi:10.2172/304513.
Hyde, R.A., LLNL. Large aperture Fresnel telescopes/011. United States. doi:10.2172/304513.
Hyde, R.A., LLNL. Thu . "Large aperture Fresnel telescopes/011". United States. doi:10.2172/304513. https://www.osti.gov/servlets/purl/304513.
@article{osti_304513,
title = {Large aperture Fresnel telescopes/011},
author = {Hyde, R.A., LLNL},
abstractNote = {At Livermore we`ve spent the last two years examining an alternative approach towards very large aperture (VLA) telescopes, one based upon transmissive Fresnel lenses rather than on mirrors. Fresnel lenses are attractive for VLA telescopes because they are launchable (lightweight, packagable, and deployable) and because they virtually eliminate the traditional, very tight, surface shape requirements faced by reflecting telescopes. Their (potentially severe) optical drawback, a very narrow spectral bandwidth, can be eliminated by use of a second (much smaller) chromatically-correcting Fresnel element. This enables Fresnel VLA telescopes to provide either single band ({Delta}{lambda}/{lambda} {approximately} 0.1), multiple band, or continuous spectral coverage. Building and fielding such large Fresnel lenses will present a significant challenge, but one which appears, with effort, to be solvable.},
doi = {10.2172/304513},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Thu Jul 16 00:00:00 EDT 1998},
month = {Thu Jul 16 00:00:00 EDT 1998}
}

Technical Report:

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