Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes

Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2000.

Bibliographic Details
Main Author: Wu, Janet P., 1978-
Other Authors: James L. Elliot and David J. Osip.
Format: Thesis
Language:eng
Published: Massachusetts Institute of Technology 2018
Subjects:
Online Access:http://hdl.handle.net/1721.1/114098
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author Wu, Janet P., 1978-
author2 James L. Elliot and David J. Osip.
author_facet James L. Elliot and David J. Osip.
Wu, Janet P., 1978-
author_sort Wu, Janet P., 1978-
collection MIT
description Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2000.
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spelling mit-1721.1/1140982019-04-12T23:20:15Z Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes Wu, Janet P., 1978- James L. Elliot and David J. Osip. Wallace Astrophysical Observatory. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences. Wallace Astrophysical Observatory. Earth, Atmospheric, and Planetary Sciences. Wallace Astrophysical Observatory. Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2000. Cataloged from PDF version of thesis. Includes bibliographical references (page 61). The goal of this thesis is to propose a layout for the Wallace Astrophysical Observatory (WAO) 24-inch optical system that would utilize the full potential of the telescope and a new CCD imaging instrument. An optical analysis of the 6.5-meter Magellan I telescope was first performed to determine the optimal mounting location for the Raymond and Beverly Sackler Magellan Instant Camera (MAGIC). The analysis method used for the Magellan I model was then applied to the WAO 24-inch telescope. The results of the optical analysis of the WAO 24-inch model suggest that the optimal layout would follow a Cassegrain model with a focal ratio of between 15.3 and 16.6 to obtain image sizes of approximately 1.0 arcsecond or less over a field of up to 26.4 arcminutes in diameter. by Janet P. Wu. S.B. 2018-03-12T19:29:48Z 2018-03-12T19:29:48Z 2000 2000 Thesis http://hdl.handle.net/1721.1/114098 1027220787 eng MIT theses are protected by copyright. They may be viewed, downloaded, or printed from this source but further reproduction or distribution in any format is prohibited without written permission. http://dspace.mit.edu/handle/1721.1/7582 61 pages application/pdf Massachusetts Institute of Technology
spellingShingle Earth, Atmospheric, and Planetary Sciences.
Wallace Astrophysical Observatory.
Wu, Janet P., 1978-
Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title_full Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title_fullStr Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title_full_unstemmed Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title_short Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
title_sort optical analysis of the wallace astrophysical observatory 24 inch and magellan i 6 5 meter telescopes
topic Earth, Atmospheric, and Planetary Sciences.
Wallace Astrophysical Observatory.
url http://hdl.handle.net/1721.1/114098
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