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Optical matching for fiber optic spectroscopySingle silica fibers of the type developed for communications are useful in the design of astronomical spectrographs. They can be used to couple light from many objects over a wide field to a single spectrograph, or to eliminate wavelength errors from image motion and gravitational flexure. For many applications it will be advantageous to use small lenses to make the most efficient coupling into and out of a fiber. If the telescope pupil is imaged on the fiber core, an efficient coupling can be made that preserves image size over a certain range. This method is demonstrated by a laboratory test using sapphire spheres as coupling lenses.
Document ID
19850043222
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hill, J. M.
(Arizona Univ. Tucson, AZ, United States)
Angel, J. R. P.
(Steward Observatory Tucson, AZ, United States)
Richardson, E. H.
(Dominion Astrophysical Observatory Victoria, British Columbia, Canada)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Subject Category
Optics
Meeting Information
Meeting: Instrumentation in astronomy V
Location: London
Start Date: September 7, 1983
End Date: September 9, 1983
Sponsors: SPIE and ISOE
Accession Number
85A25373
Funding Number(s)
CONTRACT_GRANT: NAGW-121
CONTRACT_GRANT: NSF AST-81-16965
Distribution Limits
Public
Copyright
Other

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