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A Systems Approach to Mechanisms for A White Light Coronagraph X-Ray XUV TelescopeA combined instrument package containing nine mechanisms was designed and developed for the international solar polar mission (ISPM). This complement of instruments, commonly called the CXX, is the only imaging system on either the NASA or ESA spacecraft and consists of a white light coronagraph mounted parallel to a combined X-ray and extreme ultra-violet (XUV) telescope. Requirements for and implementation of mechanisms in the CXX instrument are discussed.
Document ID
19810013863
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
External Source(s)
https://ntrs.nasa.gov/citations/19810013857
Authors
R Mastronardi (American Science and Engineering (United States) Billerica, Massachusetts, United States)
R E Cabral (American Science and Engineering (United States) Billerica, Massachusetts, United States)
Date Acquired
August 11, 2013
Publication Date
May 1, 1981
Publication Information
Publication: 15th Aerospace Mechanisms Symposium
Publisher: National Aeronautics and Space Administration
Subject Category
Optics
Report/Patent Number
NASA-CP-2181
Meeting Information
Meeting: 15th Aerospace Mechanisms Symposium
Location: Huntsville, AL
Country: US
Start Date: May 14, 1981
End Date: May 15, 1981
Sponsors: California Institute of Technology, Lockheed Martin (United States), National Aeronautics and Space Administration
Accession Number
81N22394
Funding Number(s)
CONTRACT_GRANT: NSF ATM-77-23757
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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