2026-09-20T08:20:41Zhttps://dspace.mit.edu/server/oai/requestoai:dspace.mit.edu:1721.1/1140982022-01-13T07:53:59Zcom_1721.1_7582com_1721.1_7581col_1721.1_131024
James L. Elliot and David J. Osip.
Wu, Janet P., 1978-
Wallace Astrophysical Observatory.
Wallace Astrophysical Observatory.
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
2018-03-12T19:29:48Z
2018-03-12T19:29:48Z
2000
2000
http://hdl.handle.net/1721.1/114098
1027220787
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.
61 pages
eng
Massachusetts Institute of Technology
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
Earth, Atmospheric, and Planetary Sciences.
Wallace Astrophysical Observatory.
Optical analysis of the Wallace Astrophysical Observatory 24-inch and Magellan I 6.5-meter telescopes
Thesis
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<Abstract>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.</Abstract>
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