NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The Extreme Ultraviolet ExplorerThe Extreme Ultraviolet Explorer Mission is described. The purpose of this mission is to search the celestial sphere for astronomical sources of extreme ultraviolet (EUV) radiation (100 to 1000 A). The search will be accomplished with the use of three EUV telescopes, each sensitive to different bands within the EUV band. A fourth telescope will perform a higher sensitivity search of a limited sample of the sky in a single EUV band. In six months, the entire sky will be scanned at a sensitivity level comparable to existing surveys in other more traditional astronomical bandpasses.
Document ID
19820055202
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Malina, R. F.
(California Univ. Berkeley, CA, United States)
Bowyer, S.
(California Univ. Berkeley, CA, United States)
Lampton, M.
(California Univ. Berkeley, CA, United States)
Finley, D.
(California Univ. Berkeley, CA, United States)
Paresce, F.
(California Univ. Berkeley, CA, United States)
Penegor, G.
(California Univ. Berkeley, CA, United States)
Heetderks, H.
(California, University Berkeley, CA, United States)
Date Acquired
August 10, 2013
Publication Date
August 1, 1982
Publication Information
Publication: Optical Engineering
Volume: 21
Subject Category
Launch Vehicles And Space Vehicles
Accession Number
82A38737
Funding Number(s)
CONTRACT_GRANT: NAS5-24445
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available